<?xml version='1.0' encoding='UTF-8'?><?xml-stylesheet href="http://www.blogger.com/styles/atom.css" type="text/css"?><feed xmlns='http://www.w3.org/2005/Atom' xmlns:openSearch='http://a9.com/-/spec/opensearchrss/1.0/' xmlns:georss='http://www.georss.org/georss' xmlns:gd='http://schemas.google.com/g/2005' xmlns:thr='http://purl.org/syndication/thread/1.0'><id>tag:blogger.com,1999:blog-110791865256541639</id><updated>2012-01-26T22:41:27.586-05:00</updated><title type='text'>today in particle astrophysics</title><subtitle type='html'>a daily record of papers of interest in particle astrophysics, neutrinos, cosmology, and physics in general</subtitle><link rel='http://schemas.google.com/g/2005#feed' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/posts/default'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default?max-results=100'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/'/><link rel='hub' href='http://pubsubhubbub.appspot.com/'/><link rel='next' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default?start-index=101&amp;max-results=100'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><generator version='7.00' uri='http://www.blogger.com'>Blogger</generator><openSearch:totalResults>1581</openSearch:totalResults><openSearch:startIndex>1</openSearch:startIndex><openSearch:itemsPerPage>100</openSearch:itemsPerPage><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-3162048739869194118</id><published>2012-01-26T22:41:00.001-05:00</published><updated>2012-01-26T22:41:27.595-05:00</updated><title type='text'>tipa -- 1/27/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5376"&gt;The Chemical Signature of a Relic Star Cluster in the Sextans Dwarf Spheroidal Galaxy - Implications for Near-Field Cosmology&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Karlsson_T/0/1/0/all/0/1"&gt;Torgny Karlsson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bland_Hawthorn_J/0/1/0/all/0/1"&gt;Joss Bland-Hawthorn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Freeman_K/0/1/0/all/0/1"&gt;Ken Freeman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Silk_J/0/1/0/all/0/1"&gt;Joe Silk&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5390"&gt;Signatures of photon-axion conversion in the thermal spectra and polarization of neutron stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perna_R/0/1/0/all/0/1"&gt;Rosalba Perna&lt;/a&gt; (JILA/Colorado), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ho_W/0/1/0/all/0/1"&gt;Wynn Ho&lt;/a&gt; (U. of Southampton), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Verde_L/0/1/0/all/0/1"&gt;Licia Verde&lt;/a&gt; (ICREA, Barcelona), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Adelsberg_M/0/1/0/all/0/1"&gt;Matthew van Adelsberg&lt;/a&gt; (Georgia Tech), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jimenez_R/0/1/0/all/0/1"&gt;Raul Jimenez&lt;/a&gt; (ICREA, Barcelona)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5393"&gt;SN 2006oz: rise of a super-luminous supernova observed by the SDSS-II SN Survey&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Leloudas_G/0/1/0/all/0/1"&gt;G. Leloudas&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chatzopoulos_E/0/1/0/all/0/1"&gt;E. Chatzopoulos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dilday_B/0/1/0/all/0/1"&gt;B. Dilday&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gorosabel_J/0/1/0/all/0/1"&gt;J. Gorosabel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vinko_J/0/1/0/all/0/1"&gt;J. Vinko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gallazzi_A/0/1/0/all/0/1"&gt;A. Gallazzi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wheeler_J/0/1/0/all/0/1"&gt;J. C. Wheeler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bassett_B/0/1/0/all/0/1"&gt;B. Bassett&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fischer_J/0/1/0/all/0/1"&gt;J. Fischer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Frieman_J/0/1/0/all/0/1"&gt;J. A. Frieman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fynbo_J/0/1/0/all/0/1"&gt;J. P. U. Fynbo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Goobar_A/0/1/0/all/0/1"&gt;A. Goobar&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jelinek_M/0/1/0/all/0/1"&gt;M. Jelinek&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Malesani_D/0/1/0/all/0/1"&gt;D. Malesani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nichol_R/0/1/0/all/0/1"&gt;R. C. Nichol&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nordin_J/0/1/0/all/0/1"&gt;J. Nordin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ostman_L/0/1/0/all/0/1"&gt;L. Ostman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sako_M/0/1/0/all/0/1"&gt;M. Sako&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schneider_D/0/1/0/all/0/1"&gt;D. P. Schneider&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Smith_M/0/1/0/all/0/1"&gt;M. Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sollerman_J/0/1/0/all/0/1"&gt;J. Sollerman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stritzinger_M/0/1/0/all/0/1"&gt;M. D. Stritzinger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Thoene_C/0/1/0/all/0/1"&gt;C. C. Thoene&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Postigo_A/0/1/0/all/0/1"&gt;A. de Ugarte Postigo&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5398"&gt;Radioactively-Powered Rising Lightcurves of Type Ia Supernovae&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Piro_A/0/1/0/all/0/1"&gt;Anthony L. Piro&lt;/a&gt; (Caltech)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5581"&gt;X-Rays from Supernova Shocks in Dense Mass Loss&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chevalier_R/0/1/0/all/0/1"&gt;Roger A. Chevalier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Irwin_C/0/1/0/all/0/1"&gt;Christopher M. Irwin&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5595"&gt;Search for decays of stopped, long-lived particles from 7 TeV pp collisions with the ATLAS detector&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Collaboration_ATLAS/0/1/0/all/0/1"&gt;ATLAS Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-3162048739869194118?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/3162048739869194118/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=3162048739869194118' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3162048739869194118'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3162048739869194118'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1272012.html' title='tipa -- 1/27/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-8398549265648358216</id><published>2012-01-25T22:15:00.001-05:00</published><updated>2012-01-25T22:15:40.349-05:00</updated><title type='text'>tipa -- 1/26/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5120"&gt;Radio Observations Reveal Unusual Circumstellar Environments for Some Type Ibc Supernova Progenitors&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wellons_S/0/1/0/all/0/1"&gt;Sarah Wellons&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Soderberg_A/0/1/0/all/0/1"&gt;Alicia M. Soderberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chevalier_R/0/1/0/all/0/1"&gt;Roger A. Chevalier&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5123"&gt;Normal Type Ia supernovae from violent mergers of white dwarf binaries&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pakmor_R/0/1/0/all/0/1"&gt;R. Pakmor&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kromer_M/0/1/0/all/0/1"&gt;M. Kromer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taubenberger_S/0/1/0/all/0/1"&gt;S. Taubenberger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sim_S/0/1/0/all/0/1"&gt;S. A. Sim&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Roepke_F/0/1/0/all/0/1"&gt;F. K. Roepke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hillebrandt_W/0/1/0/all/0/1"&gt;W. Hillebrandt&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5124"&gt;On particle acceleration rate in GRB afterglows&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sagi_E/0/1/0/all/0/1"&gt;Eran Sagi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nakar_E/0/1/0/all/0/1"&gt;Ehud Nakar&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5160"&gt;Five New Millisecond Pulsars From a Radio Survey of 14 Unidentified Fermi-LAT Gamma-ray Sources&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kerr_M/0/1/0/all/0/1"&gt;M. Kerr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Camilo_F/0/1/0/all/0/1"&gt;F. Camilo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Johnson_T/0/1/0/all/0/1"&gt;T. J. Johnson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ferrara_E/0/1/0/all/0/1"&gt;E. C. Ferrara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guillemot_L/0/1/0/all/0/1"&gt;L. Guillemot&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harding_A/0/1/0/all/0/1"&gt;A. K. Harding&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hessels_J/0/1/0/all/0/1"&gt;J. Hessels&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Johnston_S/0/1/0/all/0/1"&gt;S. Johnston&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Keith_M/0/1/0/all/0/1"&gt;M. Keith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kramer_M/0/1/0/all/0/1"&gt;M. Kramer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ransom_S/0/1/0/all/0/1"&gt;S. M. Ransom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ray_P/0/1/0/all/0/1"&gt;P. S. Ray&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reynolds_J/0/1/0/all/0/1"&gt;J. E. Reynolds&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sarkissian_J/0/1/0/all/0/1"&gt;J. Sarkissian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wood_K/0/1/0/all/0/1"&gt;K. S. Wood&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5197"&gt;Newly-born pulsars as sources of ultrahigh energy cosmic rays&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fang_K/0/1/0/all/0/1"&gt;Ke Fang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kotera_K/0/1/0/all/0/1"&gt;Kumiko Kotera&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Olinto_A/0/1/0/all/0/1"&gt;Angela V. Olinto&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5194"&gt;New limits on radiative sterile neutrino decays from a search for single photons in neutrino interactions&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Gninenko_S/0/1/0/all/0/1"&gt;S. N. Gninenko&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-8398549265648358216?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/8398549265648358216/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=8398549265648358216' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8398549265648358216'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8398549265648358216'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1262012.html' title='tipa -- 1/26/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-4902094376794686984</id><published>2012-01-24T22:58:00.000-05:00</published><updated>2012-01-24T22:59:14.894-05:00</updated><title type='text'>tipa -- 1/25/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4859"&gt;The Star Formation History of Leo T from Hubble Space Telescope Imaging&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Weisz_D/0/1/0/all/0/1"&gt;Daniel R. Weisz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zucker_D/0/1/0/all/0/1"&gt;Daniel B. Zucker&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dolphin_A/0/1/0/all/0/1"&gt;Andrew E. Dolphin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Martin_N/0/1/0/all/0/1"&gt;Nicolas F. Martin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jong_J/0/1/0/all/0/1"&gt;Jelte T. A. de Jong&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holtzman_J/0/1/0/all/0/1"&gt;Jon A. Holtzman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dalcanton_J/0/1/0/all/0/1"&gt;Julianne J. Dalcanton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gilbert_K/0/1/0/all/0/1"&gt;Karoline M. Gilbert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Williams_B/0/1/0/all/0/1"&gt;Benjamin F. Williams&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bell_E/0/1/0/all/0/1"&gt;Eric F. Bell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Belokurov_V/0/1/0/all/0/1"&gt;Vasily Belokurov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Evans_N/0/1/0/all/0/1"&gt;N. Wyn Evans&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4947"&gt;Constraints on Obscured Star Formation in Host Galaxies of Gamma-ray Bursts&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hatsukade_B/0/1/0/all/0/1"&gt;Bunyo Hatsukade&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hashimoto_T/0/1/0/all/0/1"&gt;Tetsuya Hashimoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ohta_K/0/1/0/all/0/1"&gt;Kouji Ohta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nakanishi_K/0/1/0/all/0/1"&gt;Kouichiro Nakanishi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tamura_Y/0/1/0/all/0/1"&gt;Yoichi Tamura&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kohno_K/0/1/0/all/0/1"&gt;Kotaro Kohno&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.5013"&gt;On the Eddington limit and WR Stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Maeder_A/0/1/0/all/0/1"&gt;André Maeder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Georgy_C/0/1/0/all/0/1"&gt;Cyril Georgy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meynet_G/0/1/0/all/0/1"&gt;Georges Meynet&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ekstrom_S/0/1/0/all/0/1"&gt;Sylvia Ekström&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-4902094376794686984?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/4902094376794686984/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=4902094376794686984' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4902094376794686984'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4902094376794686984'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1252012.html' title='tipa -- 1/25/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-1938579792220366487</id><published>2012-01-23T21:07:00.001-05:00</published><updated>2012-01-23T21:07:43.756-05:00</updated><title type='text'>tipa -- 1/24/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4387"&gt;The Stellar IMF, Core Mass Function, &amp;amp; The Last-Crossing Distribution&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hopkins_P/0/1/0/all/0/1"&gt;Philip F. Hopkins&lt;/a&gt; (Berkeley)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4389"&gt;Tidal Disruptions of White Dwarfs from Ultra-Close Encounters with Intermediate Mass Spinning Black Holes&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Haas_R/0/1/0/all/0/1"&gt;Roland Haas&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shcherbakov_R/0/1/0/all/0/1"&gt;Roman V. Shcherbakov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bode_T/0/1/0/all/0/1"&gt;Tanja Bode&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Laguna_P/0/1/0/all/0/1"&gt;Pablo Laguna&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4405"&gt;Probing the Intergalactic Magnetic Field with the Anisotropy of the Extragalactic Gamma-ray Background&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Venters_T/0/1/0/all/0/1"&gt;Tonia M. Venters&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pavlidou_V/0/1/0/all/0/1"&gt;Vasiliki Pavlidou&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4413"&gt;Implications For The Origin Of GRB 051103 From LIGO Observations&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_LIGO_Scientific/0/1/0/all/0/1"&gt;LIGO Scientific Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4491"&gt;Magnetic substructure in the northern Fermi Bubble revealed by polarized WMAP emission&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jones_D/0/1/0/all/0/1"&gt;David I. Jones&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Crocker_R/0/1/0/all/0/1"&gt;Roland M. Crocker&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reich_W/0/1/0/all/0/1"&gt;Wolfgang Reich&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ott_J/0/1/0/all/0/1"&gt;Jürgen Ott&lt;/a&gt; (3), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Aharonian_F/0/1/0/all/0/1"&gt;Felix A. Aharonian&lt;/a&gt; (4,1) ((1) MPIK, (2) MPIfR, (3) NRAO, (4) DIAS)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4613"&gt;Gravitational-wave emission from compact Galactic binaries&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nissanke_S/0/1/0/all/0/1"&gt;Samaya Nissanke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vallisneri_M/0/1/0/all/0/1"&gt;Michele Vallisneri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nelemans_G/0/1/0/all/0/1"&gt;Gijs Nelemans&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Prince_T/0/1/0/all/0/1"&gt;Thomas A. Prince&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4674"&gt;Cosmic-ray-induced ionization in molecular clouds adjacent to supernova remnants - Tracing hadonic origin of GeV gamma radiation&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schuppan_F/0/1/0/all/0/1"&gt;F. Schuppan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Becker_J/0/1/0/all/0/1"&gt;J. K. Becker&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Black_J/0/1/0/all/0/1"&gt;J. H. Black&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Casanova_S/0/1/0/all/0/1"&gt;S. Casanova&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4684"&gt;The proper motion of PSR J1550-5418 measured with VLBI: a second magnetar velocity measurement&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Deller_A/0/1/0/all/0/1"&gt;A. T. Deller&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Camilo_F/0/1/0/all/0/1"&gt;F. Camilo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reynolds_J/0/1/0/all/0/1"&gt;J. E. Reynolds&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Halpern_J/0/1/0/all/0/1"&gt;J. P. Halpern&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4711"&gt;Indications for a pair-production anomaly from the propagation of VHE gamma-rays&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Horns_D/0/1/0/all/0/1"&gt;Dieter Horns&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meyer_M/0/1/0/all/0/1"&gt;Manuel Meyer&lt;/a&gt; (Institute for Experimental Physics, University of Hamburg)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4664"&gt;Measurement of the Double-Beta Decay Half-life of ^{136}Xe in KamLAND-Zen&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; The &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Collaboration_KamLAND_Zen/0/1/0/all/0/1"&gt;KamLAND-Zen Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-1938579792220366487?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/1938579792220366487/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=1938579792220366487' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/1938579792220366487'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/1938579792220366487'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1242012.html' title='tipa -- 1/24/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-233989625230152031</id><published>2012-01-22T23:25:00.001-05:00</published><updated>2012-01-22T23:25:57.816-05:00</updated><title type='text'>tipa -- 1/23/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4181"&gt;Broadband study of GRB 091127: a sub-energetic burst at higher redshift?&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Troja_E/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;E. Troja&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sakamoto_T/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;T. Sakamoto&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guidorzi_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. Guidorzi&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Norris_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;J. P. Norris&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Panaitescu_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A. Panaitescu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kobayashi_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. Kobayashi&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Omodei_N/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;N. Omodei&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brown_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;J. C. Brown&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Burrows_D/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;D. N. Burrows&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Evans_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. A. Evans&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gehrels_N/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;N. Gehrels&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marshall_F/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;F. E. Marshall&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mawson_N/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;N. Mawson&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Melandri_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A. Melandri&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mundell_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. G. Mundell&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Oates_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. R. Oates&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Palshin_V/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;V. Pal'shin&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Preece_R/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;R. D. Preece&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Racusin_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;J. L. Racusin&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Steele_I/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;I. A. Steele&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tanvir_N/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;N. R. Tanvir&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vasileiou_V/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;V. Vasileiou&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wilson_Hodge_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. Wilson-Hodge&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yamaoka_K/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;K. Yamaoka&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1201.4186"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;What Sets the Initial Rotation Rates of Massive Stars?&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rosen_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Anna L. Rosen&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Krumholz_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Mark R. Krumholz&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ramirez_Ruiz_E/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Enrico Ramirez-Ruiz&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1201.4191"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Hadronic-Origin TeV gamma-Rays and Ultra-High Energy Cosmic Rays from Centaurus A&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sahu_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Sarira Sahu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_B/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Bing Zhang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fraija_N/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Nissim Fraija&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1201.4272"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Constraining viewing geometries of pulsars with single-peaked gamma-ray profiles using a multiwavelength approach&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Seyffert_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A.S. Seyffert&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; (1), &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Venter_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C Venter&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; (1), &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Johnson_T/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;T. J. Johnson&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; (2 and 3), &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harding_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A. K. Harding&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; (2) ((1) Centre for Space Research, North-West University, Potchefstroom Campus, South Africa, (2) Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, USA, (3) Department of Physics, University of Maryland, USA)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1201.4371"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Picogauss magnetic fields in voids from ultra-high energy cosmic rays&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pshirkov_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M. S. Pshirkov&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tinyakov_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. G. Tinyakov&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-233989625230152031?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/233989625230152031/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=233989625230152031' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/233989625230152031'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/233989625230152031'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1232012.html' title='tipa -- 1/23/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-6962470758483145072</id><published>2012-01-19T22:27:00.000-05:00</published><updated>2012-01-19T22:28:22.629-05:00</updated><title type='text'>tipa -- 1/20/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3948"&gt;Constraining the High-Energy Emission from Gamma-ray Bursts with Fermi&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Fermi_LAT/0/1/0/all/0/1"&gt;Fermi-LAT Collaboration&lt;/a&gt;, The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Fermi_GBM/0/1/0/all/0/1"&gt;Fermi-GBM Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3989"&gt;The Hubble Space Telescope Cluster Supernova Survey: III. Correlated Properties of Type Ia Supernovae and Their Hosts at 0.9 &amp;lt; z &amp;lt; 1.46&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meyers_J/0/1/0/all/0/1"&gt;J. Meyers&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Aldering_G/0/1/0/all/0/1"&gt;G. Aldering&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Barbary_K/0/1/0/all/0/1"&gt;K. Barbary&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Barrientos_L/0/1/0/all/0/1"&gt;L. F. Barrientos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brodwin_M/0/1/0/all/0/1"&gt;M. Brodwin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dawson_K/0/1/0/all/0/1"&gt;K. S. Dawson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Deustua_S/0/1/0/all/0/1"&gt;S. Deustua&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Doi_M/0/1/0/all/0/1"&gt;M. Doi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eisenhardt_P/0/1/0/all/0/1"&gt;P. Eisenhardt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Faccioli_L/0/1/0/all/0/1"&gt;L. Faccioli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fakhouri_H/0/1/0/all/0/1"&gt;H. K. Fakhouri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fruchter_A/0/1/0/all/0/1"&gt;A. S. Fruchter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gilbank_D/0/1/0/all/0/1"&gt;D. G. Gilbank&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gladders_M/0/1/0/all/0/1"&gt;M. D. Gladders&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Goldhaber_G/0/1/0/all/0/1"&gt;G. Goldhaber&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gonzalez_A/0/1/0/all/0/1"&gt;A. H. Gonzalez&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hattori_T/0/1/0/all/0/1"&gt;T. Hattori&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hsiao_E/0/1/0/all/0/1"&gt;E. Hsiao&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ihara_Y/0/1/0/all/0/1"&gt;Y. Ihara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kashikawa_N/0/1/0/all/0/1"&gt;N. Kashikawa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Koester_B/0/1/0/all/0/1"&gt;B. Koester&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Konishi_K/0/1/0/all/0/1"&gt;K. Konishi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lidman_C/0/1/0/all/0/1"&gt;C. Lidman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lubin_L/0/1/0/all/0/1"&gt;L. Lubin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Morokuma_T/0/1/0/all/0/1"&gt;T. Morokuma&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Oda_T/0/1/0/all/0/1"&gt;T. Oda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perlmutter_S/0/1/0/all/0/1"&gt;S. Perlmutter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Postman_M/0/1/0/all/0/1"&gt;M. Postman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ripoche_P/0/1/0/all/0/1"&gt;P. Ripoche&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rosati_P/0/1/0/all/0/1"&gt;P. Rosati&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rubin_D/0/1/0/all/0/1"&gt;D. Rubin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rykoff_E/0/1/0/all/0/1"&gt;E. Rykoff&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Spadafora_A/0/1/0/all/0/1"&gt;A. Spadafora&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stanford_S/0/1/0/all/0/1"&gt;S. A. Stanford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Suzuki_N/0/1/0/all/0/1"&gt;N. Suzuki&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Takanashi_N/0/1/0/all/0/1"&gt;N. Takanashi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tokita_K/0/1/0/all/0/1"&gt;K. Tokita&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yasuda_N/0/1/0/all/0/1"&gt;N. Yasuda&lt;/a&gt;, for the &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Project_S/0/1/0/all/0/1"&gt;Supernova Cosmology Project&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4074"&gt;Morphological and spectral properties of the W51 region measured with the MAGIC telescopes&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_MAGIC/0/1/0/all/0/1"&gt;MAGIC Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4135"&gt;A multiwavelength view of the flaring state of PKS 2155-304 in 2006&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_HESS/0/1/0/all/0/1"&gt;HESS Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4163"&gt;General Relativistic Magnetohydrodynamic Simulations of Magnetically Choked Accretion Flows around Black Holes&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McKinney_J/0/1/0/all/0/1"&gt;Jonathan C. McKinney&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tchekhovskoy_A/0/1/0/all/0/1"&gt;Alexander Tchekhovskoy&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Blandford_R/0/1/0/all/0/1"&gt;Roger D. Blandford&lt;/a&gt; (1) ((1) Stanford, (2) Princeton)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.4128"&gt;Neutrino production coherence and oscillation experiments&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Akhmedov_E/0/1/0/all/0/1"&gt;Evgeny Akhmedov&lt;/a&gt; (MPIK Heidelberg), &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Hernandez_D/0/1/0/all/0/1"&gt;Daniel Hernandez&lt;/a&gt; (ICTP Trieste), &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Smirnov_A/0/1/0/all/0/1"&gt;Alexei Smirnov&lt;/a&gt; (ICTP Trieste)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-6962470758483145072?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/6962470758483145072/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=6962470758483145072' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6962470758483145072'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6962470758483145072'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1202012.html' title='tipa -- 1/20/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-5335643379275482047</id><published>2012-01-18T21:40:00.001-05:00</published><updated>2012-01-18T21:40:52.843-05:00</updated><title type='text'>tipa -- 1/19/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3625"&gt;Variable gamma-ray sky at 1 GeV&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pshirkov_M/0/1/0/all/0/1"&gt;M. S. Pshirkov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rubtsov_G/0/1/0/all/0/1"&gt;G. I. Rubtsov&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3629"&gt;Discovery of an unidentified Fermi object as a black widow-like millisecond pulsar&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kong_A/0/1/0/all/0/1"&gt;A. K. H. Kong&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Huang_R/0/1/0/all/0/1"&gt;R. H. H. Huang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cheng_K/0/1/0/all/0/1"&gt;K. S. Cheng&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Takata_J/0/1/0/all/0/1"&gt;J. Takata&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yatsu_Y/0/1/0/all/0/1"&gt;Y. Yatsu&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cheung_C/0/1/0/all/0/1"&gt;C. C. Cheung&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Donato_D/0/1/0/all/0/1"&gt;D. Donato&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lin_L/0/1/0/all/0/1"&gt;L. C. C. Lin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kataoka_J/0/1/0/all/0/1"&gt;J. Kataoka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Takahashi_Y/0/1/0/all/0/1"&gt;Y. Takahashi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Maeda_K/0/1/0/all/0/1"&gt;K. Maeda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hui_C/0/1/0/all/0/1"&gt;C. Y. Hui&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tam_P/0/1/0/all/0/1"&gt;P. H. T. Tam&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3635"&gt;Twisting, reconnecting magnetospheres and magnetar spindown&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parfrey_K/0/1/0/all/0/1"&gt;Kyle Parfrey&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Beloborodov_A/0/1/0/all/0/1"&gt;Andrei M. Beloborodov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hui_L/0/1/0/all/0/1"&gt;Lam Hui&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3643"&gt;Gravitational detection of a low-mass dark satellite at cosmological distance&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vegetti_S/0/1/0/all/0/1"&gt;S. Vegetti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lagattuta_D/0/1/0/all/0/1"&gt;D. J. Lagattuta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McKean_J/0/1/0/all/0/1"&gt;J. P. McKean&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Auger_M/0/1/0/all/0/1"&gt;M. W. Auger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fassnacht_C/0/1/0/all/0/1"&gt;C. D. Fassnacht&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Koopmans_L/0/1/0/all/0/1"&gt;L. V. E. Koopmans&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3647"&gt;On plasma rotation and drifting subpulses in pulsars; using aligned pulsar B0826-34 as a voltmeter&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Leeuwen_J/0/1/0/all/0/1"&gt;J. van Leeuwen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Timokhin_A/0/1/0/all/0/1"&gt;A. N. Timokhin&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3848"&gt;Measurement of the cosmic ray antiproton/proton flux ratio at TeV energies with the ARGO-YBJ detector&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_ARGO_YBJ/0/1/0/all/0/1"&gt;ARGO-YBJ Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3631"&gt;Fundamental statistical limitations of future dark matter direct detection experiments&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Strege_C/0/1/0/all/0/1"&gt;Charlotte Strege&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Trotta_R/0/1/0/all/0/1"&gt;Roberto Trotta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Bertone_G/0/1/0/all/0/1"&gt;Gianfranco Bertone&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Peter_A/0/1/0/all/0/1"&gt;Annika H. G. Peter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Scott_P/0/1/0/all/0/1"&gt;Pat Scott&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3805"&gt;Measuring Active-to-Sterile Neutrino Oscillations with Neutral Current Coherent Neutrino-Nucleus Scattering&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Anderson_A/0/1/0/all/0/1"&gt;A. J. Anderson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Conrad_J/0/1/0/all/0/1"&gt;J. M. Conrad&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Figueroa_Feliciano_E/0/1/0/all/0/1"&gt;E. Figueroa-Feliciano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Ignarra_C/0/1/0/all/0/1"&gt;C. Ignarra&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Karagiorgi_G/0/1/0/all/0/1"&gt;G. Karagiorgi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Scholberg_K/0/1/0/all/0/1"&gt;K. Scholberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Shaevitz_M/0/1/0/all/0/1"&gt;M. H. Shaevitz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Spitz_J/0/1/0/all/0/1"&gt;J. Spitz&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-5335643379275482047?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/5335643379275482047/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=5335643379275482047' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5335643379275482047'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5335643379275482047'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1192012.html' title='tipa -- 1/19/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-7926509833721753894</id><published>2012-01-18T19:31:00.000-05:00</published><updated>2012-01-18T19:32:01.321-05:00</updated><title type='text'>tipa -- 1/18/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3585"&gt;Three years of Fermi GBM Earth Occultation Monitoring: Observations of Hard X-ray/Soft Gamma-Ray Sources&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wilson_Hodge_C/0/1/0/all/0/1"&gt;Colleen A. Wilson-Hodge&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Case_G/0/1/0/all/0/1"&gt;Gary L. Case&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cherry_M/0/1/0/all/0/1"&gt;Michael L. Cherry&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rodi_J/0/1/0/all/0/1"&gt;James Rodi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Camero_Arranz_A/0/1/0/all/0/1"&gt;Ascension Camero-Arranz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jenke_P/0/1/0/all/0/1"&gt;Peter Jenke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chaplin_V/0/1/0/all/0/1"&gt;Vandiver Chaplin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Beklen_E/0/1/0/all/0/1"&gt;Elif Beklen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Finger_M/0/1/0/all/0/1"&gt;Mark Finger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bhat_N/0/1/0/all/0/1"&gt;Narayan Bhat&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Briggs_M/0/1/0/all/0/1"&gt;Michael S. Briggs&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Connaughton_V/0/1/0/all/0/1"&gt;Valerie Connaughton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Greiner_J/0/1/0/all/0/1"&gt;Jochen Greiner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kippen_R/0/1/0/all/0/1"&gt;R. Marc Kippen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meegan_C/0/1/0/all/0/1"&gt;Charles A. Meegan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Paciesas_W/0/1/0/all/0/1"&gt;William S. Paciesas&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Preece_R/0/1/0/all/0/1"&gt;Robert Preece&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kienlin_A/0/1/0/all/0/1"&gt;Andreas von Kienlin&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3533"&gt;Constraints on the non-thermal emission from Eta Carinae's blast wave of 1843&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Skilton_J/0/1/0/all/0/1"&gt;J. L. Skilton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Domainko_W/0/1/0/all/0/1"&gt;W. Domainko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hinton_J/0/1/0/all/0/1"&gt;J. A. Hinton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jones_D/0/1/0/all/0/1"&gt;D. I. Jones&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ohm_S/0/1/0/all/0/1"&gt;S. Ohm&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Urquhart_J/0/1/0/all/0/1"&gt;J. S. Urquhart&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3455"&gt;Neutrino Emission from Magnetized Proto-Neutron Stars in Relativistic Mean Field Theory&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Maruyama_T/0/1/0/all/0/1"&gt;Tomoyuki Maruyama&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yasutake_N/0/1/0/all/0/1"&gt;Nobutoshi Yasutake&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cheoun_M/0/1/0/all/0/1"&gt;Myung-Ki Cheoun&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hidaka_J/0/1/0/all/0/1"&gt;Jun Hidaka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mathews_T/0/1/0/all/0/1"&gt;Toshitaka Kajino. Grant. J. Mathews&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ryu_C/0/1/0/all/0/1"&gt;Chung-Yeol Ryu&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3447"&gt;The Diffuse Gamma-ray Background from Type Ia Supernovae&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lien_A/0/1/0/all/0/1"&gt;Amy Lien&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fields_B/0/1/0/all/0/1"&gt;Brian D. Fields&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3369"&gt;Triggered star-formation in the inner filament of Centaurus A&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Crockett_R/0/1/0/all/0/1"&gt;R. Mark Crockett&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shabala_S/0/1/0/all/0/1"&gt;Stanislav S. Shabala&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kaviraj_S/0/1/0/all/0/1"&gt;Sugata Kaviraj&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Antonuccio_Delogu_V/0/1/0/all/0/1"&gt;Vincenzo Antonuccio-Delogu&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Silk_J/0/1/0/all/0/1"&gt;Joseph Silk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mutchler_M/0/1/0/all/0/1"&gt;Max Mutchler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+OConnell_R/0/1/0/all/0/1"&gt;Robert W. O'Connell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rejkuba_M/0/1/0/all/0/1"&gt;Marina Rejkuba&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Whitmore_B/0/1/0/all/0/1"&gt;Bradley C. Whitmore&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Windhorst_R/0/1/0/all/0/1"&gt;Rogier A. Windhorst&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-7926509833721753894?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/7926509833721753894/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=7926509833721753894' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7926509833721753894'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7926509833721753894'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1182012.html' title='tipa -- 1/18/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-4038158526673564668</id><published>2012-01-17T19:55:00.000-05:00</published><updated>2012-01-17T19:56:22.875-05:00</updated><title type='text'>tipa -- 1/17/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2967"&gt;Search for Antihelium with the BESS-Polar Spectrometer&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Abe_K/0/1/0/all/0/1"&gt;K. Abe&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fuke_H/0/1/0/all/0/1"&gt;H. Fuke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Haino_S/0/1/0/all/0/1"&gt;S. Haino&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hams_T/0/1/0/all/0/1"&gt;T. Hams&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hasegawa_M/0/1/0/all/0/1"&gt;M. Hasegawa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Horikoshi_A/0/1/0/all/0/1"&gt;A. Horikoshi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Itazaki_A/0/1/0/all/0/1"&gt;A. Itazaki&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kim_K/0/1/0/all/0/1"&gt;K.C. Kim&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kumazawa_T/0/1/0/all/0/1"&gt;T. Kumazawa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kusumoto_A/0/1/0/all/0/1"&gt;A. Kusumoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lee_M/0/1/0/all/0/1"&gt;M.H. Lee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Makida_Y/0/1/0/all/0/1"&gt;Y. Makida&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Matsuda_S/0/1/0/all/0/1"&gt;S. Matsuda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Matsukawa_Y/0/1/0/all/0/1"&gt;Y. Matsukawa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Matsumoto_K/0/1/0/all/0/1"&gt;K. Matsumoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mitchell_J/0/1/0/all/0/1"&gt;J.W. Mitchell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Myers_Z/0/1/0/all/0/1"&gt;Z. Myers&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nishimura_J/0/1/0/all/0/1"&gt;J. Nishimura&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nozaki_M/0/1/0/all/0/1"&gt;M. Nozaki&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Orito_R/0/1/0/all/0/1"&gt;R. Orito&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ormes_J/0/1/0/all/0/1"&gt;J.F. Ormes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sakai_K/0/1/0/all/0/1"&gt;K. Sakai&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sasaki_M/0/1/0/all/0/1"&gt;M. Sasaki&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Seo_E/0/1/0/all/0/1"&gt;E.S. Seo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shikaze_Y/0/1/0/all/0/1"&gt;Y. Shikaze&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shinoda_R/0/1/0/all/0/1"&gt;R. Shinoda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Streitmatter_R/0/1/0/all/0/1"&gt;R.E. Streitmatter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Suzuki_J/0/1/0/all/0/1"&gt;J. Suzuki&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Takasugi_Y/0/1/0/all/0/1"&gt;Y. Takasugi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Takeuchi_K/0/1/0/all/0/1"&gt;K. Takeuchi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tanaka_K/0/1/0/all/0/1"&gt;K. Tanaka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Thakur_N/0/1/0/all/0/1"&gt;N. Thakur&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yamagami_T/0/1/0/all/0/1"&gt;T. Yamagami&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yamamoto_A/0/1/0/all/0/1"&gt;A. Yamamoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yoshida_T/0/1/0/all/0/1"&gt;T. Yoshida&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yoshimura_K/0/1/0/all/0/1"&gt;K. Yoshimura&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2981"&gt;The Fermi GBM Gamma-Ray Burst Spectral Catalog: The First Two Years&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Goldstein_A/0/1/0/all/0/1"&gt;Adam Goldstein&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Burgess_J/0/1/0/all/0/1"&gt;J. Michael Burgess&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Preece_R/0/1/0/all/0/1"&gt;Robert D. Preece&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Briggs_M/0/1/0/all/0/1"&gt;Michael S. Briggs&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guiriec_S/0/1/0/all/0/1"&gt;Sylvain Guiriec&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Horst_A/0/1/0/all/0/1"&gt;Alexander J. van der Horst&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Connaughton_V/0/1/0/all/0/1"&gt;Valerie Connaughton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wilson_Hodge_C/0/1/0/all/0/1"&gt;Colleen A. Wilson-Hodge&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Paciesas_W/0/1/0/all/0/1"&gt;William S. Paciesas&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meegan_C/0/1/0/all/0/1"&gt;Charles A. Meegan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kienlin_A/0/1/0/all/0/1"&gt;Andreas von Kienlin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bhat_P/0/1/0/all/0/1"&gt;P. Narayana Bhat&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bissaldi_E/0/1/0/all/0/1"&gt;Elisabetta Bissaldi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chaplin_V/0/1/0/all/0/1"&gt;Vandiver Chaplin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Diehl_R/0/1/0/all/0/1"&gt;Roland Diehl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fishman_G/0/1/0/all/0/1"&gt;Gerald J. Fishman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fitzpatrick_G/0/1/0/all/0/1"&gt;Gerard Fitzpatrick&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Foley_S/0/1/0/all/0/1"&gt;Suzanne Foley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gibby_M/0/1/0/all/0/1"&gt;Melissa Gibby&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Giles_M/0/1/0/all/0/1"&gt;Misty Giles&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Greiner_J/0/1/0/all/0/1"&gt;Jochen Greiner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gruber_D/0/1/0/all/0/1"&gt;David Gruber&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kippen_R/0/1/0/all/0/1"&gt;R. Marc Kippen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kouveliotou_C/0/1/0/all/0/1"&gt;Chryssa Kouveliotou&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McBreen_S/0/1/0/all/0/1"&gt;Sheila McBreen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McGlynn_S/0/1/0/all/0/1"&gt;Sinead McGlynn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rau_A/0/1/0/all/0/1"&gt;Arne Rau&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tierney_D/0/1/0/all/0/1"&gt;Dave Tierney&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3220"&gt;The nuclear starburst in Arp 299-A: From the 5.0 GHz VLBI radio light-curves to its core-collapse supernova rate&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bondi_M/0/1/0/all/0/1"&gt;M. Bondi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perez_Torres_M/0/1/0/all/0/1"&gt;M. A. Perez-Torres&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Herrero_Illana_R/0/1/0/all/0/1"&gt;R. Herrero-Illana&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Alberdi_A/0/1/0/all/0/1"&gt;A. Alberdi&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3284"&gt;Cosmological bounds on tachyonic neutrinos&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Davies_P/0/1/0/all/0/1"&gt;P. C. W. Davies&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Moss_I/0/1/0/all/0/1"&gt;Ian G. Moss&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.3356"&gt;A giant radio flare from Cygnus X-3 with associated Gamma-ray emission&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Corbel_S/0/1/0/all/0/1"&gt;S. Corbel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dubus_G/0/1/0/all/0/1"&gt;G. Dubus&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tomsick_J/0/1/0/all/0/1"&gt;J. A. Tomsick&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Szostek_A/0/1/0/all/0/1"&gt;A. Szostek&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Corbet_R/0/1/0/all/0/1"&gt;R. H. D. Corbet&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Miller_Jones_J/0/1/0/all/0/1"&gt;J. C. A. Miller-Jones&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Richards_J/0/1/0/all/0/1"&gt;J. L. Richards&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pooley_G/0/1/0/all/0/1"&gt;G. Pooley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Trushkin_S/0/1/0/all/0/1"&gt;S. Trushkin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dubois_R/0/1/0/all/0/1"&gt;R. Dubois&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hill_A/0/1/0/all/0/1"&gt;A. B. Hill&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kerr_M/0/1/0/all/0/1"&gt;M. Kerr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Max_Moerbeck_W/0/1/0/all/0/1"&gt;W. Max-Moerbeck&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Readhead_A/0/1/0/all/0/1"&gt;A. C. S. Readhead&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bodaghee_A/0/1/0/all/0/1"&gt;A. Bodaghee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tudose_V/0/1/0/all/0/1"&gt;V. Tudose&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parent_D/0/1/0/all/0/1"&gt;D. Parent&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wilms_J/0/1/0/all/0/1"&gt;J. Wilms&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pottschmidt_K/0/1/0/all/0/1"&gt;K. Pottschmidt&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-4038158526673564668?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/4038158526673564668/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=4038158526673564668' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4038158526673564668'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4038158526673564668'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1172012.html' title='tipa -- 1/17/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-6933547283811730729</id><published>2012-01-17T19:46:00.001-05:00</published><updated>2012-01-17T19:46:46.140-05:00</updated><title type='text'>tipa -- 1/16/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2683"&gt;Constraints on Light Hidden Sector Gauge Bosons from Supernova Cooling&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dent_J/0/1/0/all/0/1"&gt;James B. Dent&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ferrer_F/0/1/0/all/0/1"&gt;Francesc Ferrer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Krauss_L/0/1/0/all/0/1"&gt;Lawrence M. Krauss&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2691"&gt;Search for Dark Matter Satellites using the FERMI-LAT&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Fermi_LAT/0/1/0/all/0/1"&gt;Fermi LAT Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2751"&gt;Feedback Effects on Low-Mass Star Formation&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hansen_C/0/1/0/all/0/1"&gt;Charles E. Hansen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Klein_R/0/1/0/all/0/1"&gt;Richard I. Klein&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McKee_C/0/1/0/all/0/1"&gt;Christopher F. McKee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fisher_R/0/1/0/all/0/1"&gt;Robert T. Fisher&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-6933547283811730729?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/6933547283811730729/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=6933547283811730729' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6933547283811730729'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6933547283811730729'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1162012.html' title='tipa -- 1/16/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-4285108663910955351</id><published>2012-01-13T21:36:00.000-05:00</published><updated>2012-01-13T21:37:12.873-05:00</updated><title type='text'>tipa -- 1/13/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2406"&gt;How the merger of two white dwarfs depends on their mass ratio: orbital stability and detonations at contact&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dan_M/0/1/0/all/0/1"&gt;Marius Dan&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rosswog_S/0/1/0/all/0/1"&gt;Stephan Rosswog&lt;/a&gt; (1 and 2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guillochon_J/0/1/0/all/0/1"&gt;James Guillochon&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ramirez_Ruiz_E/0/1/0/all/0/1"&gt;Enrico Ramirez-Ruiz&lt;/a&gt; (2) ((1) Jacobs University Bremen, (2) UC Santa Cruz)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2426"&gt;Effects of Unstable Dark Matter on Large-Scale Structure and Constraints from Future Surveys&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wang_M/0/1/0/all/0/1"&gt;Mei-Yu Wang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zentner_A/0/1/0/all/0/1"&gt;Andrew R. Zentner&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2460"&gt;Limits on Large Extra Dimensions Based on Observations of Neutron Stars with the Fermi-LAT&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Berenji_B/0/1/0/all/0/1"&gt;Bijan Berenji&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bloom_E/0/1/0/all/0/1"&gt;Elliott Bloom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cohen_Tanugi_J/0/1/0/all/0/1"&gt;Johann Cohen-Tanugi&lt;/a&gt;, for the &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Fermi_LAT/0/1/0/all/0/1"&gt;Fermi-LAT Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2470"&gt;A Type Ia Supernova at Redshift 1.55 in Hubble Space Telescope Infrared Observations from CANDELS&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rodney_S/0/1/0/all/0/1"&gt;Steven A. Rodney&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Riess_A/0/1/0/all/0/1"&gt;Adam G. Riess&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dahlen_T/0/1/0/all/0/1"&gt;Tomas Dahlen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Strolger_L/0/1/0/all/0/1"&gt;Louis-Gregory Strolger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ferguson_H/0/1/0/all/0/1"&gt;Henry C. Ferguson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hjorth_J/0/1/0/all/0/1"&gt;Jens Hjorth&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Frederiksen_T/0/1/0/all/0/1"&gt;Teddy F. Frederiksen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Weiner_B/0/1/0/all/0/1"&gt;Benjamin J. Weiner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mobasher_B/0/1/0/all/0/1"&gt;Bahram Mobasher&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Casertano_S/0/1/0/all/0/1"&gt;Stefano Casertano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jones_D/0/1/0/all/0/1"&gt;David O. Jones&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Challis_P/0/1/0/all/0/1"&gt;Peter Challis&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Faber_S/0/1/0/all/0/1"&gt;S. M. Faber&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Filippenko_A/0/1/0/all/0/1"&gt;Alexei V. Filippenko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Garnavich_P/0/1/0/all/0/1"&gt;Peter Garnavich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Graur_O/0/1/0/all/0/1"&gt;Or Graur&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Grogin_N/0/1/0/all/0/1"&gt;Norman A. Grogin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hayden_B/0/1/0/all/0/1"&gt;Brian Hayden&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jha_S/0/1/0/all/0/1"&gt;Saurabh W. Jha&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kirshner_R/0/1/0/all/0/1"&gt;Robert P. Kirshner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kocevski_D/0/1/0/all/0/1"&gt;Dale Kocevski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Koekemoer_A/0/1/0/all/0/1"&gt;Anton Koekemoer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McCully_C/0/1/0/all/0/1"&gt;Curtis McCully&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Patel_B/0/1/0/all/0/1"&gt;Brandon Patel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rajan_A/0/1/0/all/0/1"&gt;Abhijith Rajan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Scarlata_C/0/1/0/all/0/1"&gt;Claudia Scarlata&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2618"&gt;Spatially resolved X-ray spectroscopy and modeling of the nonthermal emission of the PWN in G0.9+0.1&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holler_M/0/1/0/all/0/1"&gt;M. Holler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schock_F/0/1/0/all/0/1"&gt;F. M. Schöck&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eger_P/0/1/0/all/0/1"&gt;P. Eger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kiessling_D/0/1/0/all/0/1"&gt;D. Kießling&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Valerius_K/0/1/0/all/0/1"&gt;K. Valerius&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stegmann_C/0/1/0/all/0/1"&gt;C. Stegmann&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2634"&gt;Discovery of VHE gamma-ray emission from the BL Lac object B3 2247+381 with the MAGIC telescopes&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_MAGIC/0/1/0/all/0/1"&gt;MAGIC Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2637"&gt;The Double Pulsar Eclipses I: Phenomenology and Multi-frequency Analysis&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Breton_R/0/1/0/all/0/1"&gt;R. P. Breton&lt;/a&gt; (1,2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kaspi_V/0/1/0/all/0/1"&gt;V. M. Kaspi&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McLaughlin_M/0/1/0/all/0/1"&gt;M. A. McLaughlin&lt;/a&gt; (3,4), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lyutikov_M/0/1/0/all/0/1"&gt;M. Lyutikov&lt;/a&gt; (5), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kramer_M/0/1/0/all/0/1"&gt;M. Kramer&lt;/a&gt; (6), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stairs_I/0/1/0/all/0/1"&gt;I. H. Stairs&lt;/a&gt; (7), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ransom_S/0/1/0/all/0/1"&gt;S. M. Ransom&lt;/a&gt; (8), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ferdman_R/0/1/0/all/0/1"&gt;R. D. Ferdman&lt;/a&gt; (9), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Camilo_F/0/1/0/all/0/1"&gt;F. Camilo&lt;/a&gt; (10), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Possenti_A/0/1/0/all/0/1"&gt;A. Possenti&lt;/a&gt; (11) ((1) University of Toronto, (2) McGill University, (3) West Virginia University, (4) NRAO Green Bank, (5) Purdue University, (6) MPIfR, (7) University of British Columbia, (8) NRAO Charlottesville, (9) University of Manchester, (10) Columbia University, (11) INAF Osservatorio Astronomico di Cagliari)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2568"&gt;Measurement of the Neutron Radius of 208Pb Through Parity-Violation in Electron Scattering&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Abrahamyan_S/0/1/0/all/0/1"&gt;S. Abrahamyan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Ahmed_Z/0/1/0/all/0/1"&gt;Z. Ahmed&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Albataineh_H/0/1/0/all/0/1"&gt;H. Albataineh&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Aniol_K/0/1/0/all/0/1"&gt;K. Aniol&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Armstrong_D/0/1/0/all/0/1"&gt;D. S. Armstrong&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Armstrong_W/0/1/0/all/0/1"&gt;W. Armstrong&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Averett_T/0/1/0/all/0/1"&gt;T. Averett&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Babineau_B/0/1/0/all/0/1"&gt;B. Babineau&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Barbieri_A/0/1/0/all/0/1"&gt;A. Barbieri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Bellini_V/0/1/0/all/0/1"&gt;V. Bellini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Beminiwattha_R/0/1/0/all/0/1"&gt;R. Beminiwattha&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Benesch_J/0/1/0/all/0/1"&gt;J. Benesch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Benmokhtar_F/0/1/0/all/0/1"&gt;F. Benmokhtar&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Bielarski_T/0/1/0/all/0/1"&gt;T. Bielarski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Boeglin_W/0/1/0/all/0/1"&gt;W. Boeglin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Camsonne_A/0/1/0/all/0/1"&gt;A. Camsonne&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Canan_M/0/1/0/all/0/1"&gt;M. Canan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Carter_P/0/1/0/all/0/1"&gt;P. Carter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Cates_G/0/1/0/all/0/1"&gt;G. D. Cates&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Chen_C/0/1/0/all/0/1"&gt;C. Chen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Chen_J/0/1/0/all/0/1"&gt;J.-P. Chen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Hen_O/0/1/0/all/0/1"&gt;O. Hen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Cusanno_F/0/1/0/all/0/1"&gt;F. Cusanno&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Dalton_M/0/1/0/all/0/1"&gt;M. M. Dalton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Leo_R/0/1/0/all/0/1"&gt;R. De Leo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Jager_K/0/1/0/all/0/1"&gt;K. de Jager&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Deconinck_W/0/1/0/all/0/1"&gt;W. Deconinck&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Decowski_P/0/1/0/all/0/1"&gt;P. Decowski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Deng_X/0/1/0/all/0/1"&gt;X. Deng&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Deur_A/0/1/0/all/0/1"&gt;A. Deur&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Dutta_D/0/1/0/all/0/1"&gt;D. Dutta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Etile_A/0/1/0/all/0/1"&gt;A. Etile&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Flay_D/0/1/0/all/0/1"&gt;D. Flay&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Franklin_G/0/1/0/all/0/1"&gt;G. B. Franklin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Friend_M/0/1/0/all/0/1"&gt;M. Friend&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Frullani_S/0/1/0/all/0/1"&gt;S. Frullani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Fuchey_E/0/1/0/all/0/1"&gt;E. Fuchey&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Garibaldi_F/0/1/0/all/0/1"&gt;F. Garibaldi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Gasser_E/0/1/0/all/0/1"&gt;E. Gasser&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Gilman_R/0/1/0/all/0/1"&gt;R. Gilman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Giusa_A/0/1/0/all/0/1"&gt;A. Giusa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Glamazdin_A/0/1/0/all/0/1"&gt;A. Glamazdin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Gomez_J/0/1/0/all/0/1"&gt;J. Gomez&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Grames_J/0/1/0/all/0/1"&gt;J. Grames&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Gu_C/0/1/0/all/0/1"&gt;C. Gu&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Hansen_O/0/1/0/all/0/1"&gt;O. Hansen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Hansknecht_J/0/1/0/all/0/1"&gt;J. Hansknecht&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Higinbotham_D/0/1/0/all/0/1"&gt;D. W. Higinbotham&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Holmes_R/0/1/0/all/0/1"&gt;R. S. Holmes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Holmstrom_T/0/1/0/all/0/1"&gt;T. Holmstrom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Horowitz_C/0/1/0/all/0/1"&gt;C. J. Horowitz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Hoskins_J/0/1/0/all/0/1"&gt;J. Hoskins&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Huang_J/0/1/0/all/0/1"&gt;J. Huang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Hyde_C/0/1/0/all/0/1"&gt;C. E. Hyde&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Itard_F/0/1/0/all/0/1"&gt;F. Itard&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Jen_C/0/1/0/all/0/1"&gt;C.-M. Jen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Jensen_E/0/1/0/all/0/1"&gt;E. Jensen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Jin_G/0/1/0/all/0/1"&gt;G. Jin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Johnston_S/0/1/0/all/0/1"&gt;S. Johnston&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Kelleher_A/0/1/0/all/0/1"&gt;A. Kelleher&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Kliakhandler_K/0/1/0/all/0/1"&gt;K. Kliakhandler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+King_P/0/1/0/all/0/1"&gt;P.M. King&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Kowalski_S/0/1/0/all/0/1"&gt;S. Kowalski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Kumar_K/0/1/0/all/0/1"&gt;K. S. Kumar&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Leacock_J/0/1/0/all/0/1"&gt;J. Leacock&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Leckey_J/0/1/0/all/0/1"&gt;J. Leckey IV&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Lee_J/0/1/0/all/0/1"&gt;J. H. Lee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+LeRose_J/0/1/0/all/0/1"&gt;J. J. LeRose&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Lindgren_R/0/1/0/all/0/1"&gt;R. Lindgren&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Liyanage_N/0/1/0/all/0/1"&gt;N. Liyanage&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Lubinsky_N/0/1/0/all/0/1"&gt;N. Lubinsky&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Mammei_J/0/1/0/all/0/1"&gt;J. Mammei&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Mammoliti_F/0/1/0/all/0/1"&gt;F. Mammoliti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Margaziotis_D/0/1/0/all/0/1"&gt;D.J. Margaziotis&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Markowitz_P/0/1/0/all/0/1"&gt;P. Markowitz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+McCreary_A/0/1/0/all/0/1"&gt;A. McCreary&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+McNulty_D/0/1/0/all/0/1"&gt;D. McNulty&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Mercado_L/0/1/0/all/0/1"&gt;L. Mercado&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Meziani_Z/0/1/0/all/0/1"&gt;Z.-E. Meziani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Michaels_R/0/1/0/all/0/1"&gt;R. W. Michaels&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Mihovilovic_M/0/1/0/all/0/1"&gt;M. Mihovilovic&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Muangma_N/0/1/0/all/0/1"&gt;N. Muangma&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Munoz_Camacho_C/0/1/0/all/0/1"&gt;C. Muñoz-Camacho&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Nanda_S/0/1/0/all/0/1"&gt;S. Nanda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Nelyubin_V/0/1/0/all/0/1"&gt;V. Nelyubin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Nuruzzaman_N/0/1/0/all/0/1"&gt;N. Nuruzzaman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Oh_Y/0/1/0/all/0/1"&gt;Y. Oh&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Palmer_A/0/1/0/all/0/1"&gt;A. Palmer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Parno_D/0/1/0/all/0/1"&gt;D. Parno&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Paschke_K/0/1/0/all/0/1"&gt;K. D. Paschke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Phillips_S/0/1/0/all/0/1"&gt;S. K. Phillips&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Poelker_B/0/1/0/all/0/1"&gt;B. Poelker&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Pomatsalyuk_R/0/1/0/all/0/1"&gt;R. Pomatsalyuk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Posik_M/0/1/0/all/0/1"&gt;M. Posik&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Puckett_A/0/1/0/all/0/1"&gt;A.J.R. Puckett&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Quinn_B/0/1/0/all/0/1"&gt;B. Quinn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Rakhman_A/0/1/0/all/0/1"&gt;A. Rakhman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Reimer_P/0/1/0/all/0/1"&gt;P. E. Reimer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Riordan_S/0/1/0/all/0/1"&gt;S. Riordan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Rogan_P/0/1/0/all/0/1"&gt;P. Rogan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Ron_G/0/1/0/all/0/1"&gt;G. Ron&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Russo_G/0/1/0/all/0/1"&gt;G. Russo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Saenboonruang_K/0/1/0/all/0/1"&gt;K. Saenboonruang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Saha_A/0/1/0/all/0/1"&gt;A. Saha&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Sawatzky_B/0/1/0/all/0/1"&gt;B. Sawatzky&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Shahinyan_A/0/1/0/all/0/1"&gt;A. Shahinyan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Silwal_R/0/1/0/all/0/1"&gt;R. Silwal&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Sirca_S/0/1/0/all/0/1"&gt;S. Sirca&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Slifer_K/0/1/0/all/0/1"&gt;K. Slifer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Solvignon_P/0/1/0/all/0/1"&gt;P. Solvignon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Souder_P/0/1/0/all/0/1"&gt;P. A. Souder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Sperduto_M/0/1/0/all/0/1"&gt;M. L. Sperduto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Subedi_R/0/1/0/all/0/1"&gt;R. Subedi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Suleiman_R/0/1/0/all/0/1"&gt;R. Suleiman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Sulkosky_V/0/1/0/all/0/1"&gt;V. Sulkosky&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Sutera_C/0/1/0/all/0/1"&gt;C. M. Sutera&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Tobias_W/0/1/0/all/0/1"&gt;W. A. Tobias&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Troth_W/0/1/0/all/0/1"&gt;W. Troth&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Urciuoli_G/0/1/0/all/0/1"&gt;G. M. Urciuoli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Waidyawansa_B/0/1/0/all/0/1"&gt;B. Waidyawansa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Wang_D/0/1/0/all/0/1"&gt;D. Wang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Wexler_J/0/1/0/all/0/1"&gt;J. Wexler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Wilson_R/0/1/0/all/0/1"&gt;R. Wilson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Wojtsekhowski_B/0/1/0/all/0/1"&gt;B. Wojtsekhowski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Yan_X/0/1/0/all/0/1"&gt;X. Yan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Yao_H/0/1/0/all/0/1"&gt;H. Yao&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Ye_Y/0/1/0/all/0/1"&gt;Y. Ye&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Ye_Z/0/1/0/all/0/1"&gt;Z. Ye&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Yim_V/0/1/0/all/0/1"&gt;V. Yim&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Zana_L/0/1/0/all/0/1"&gt;L. Zana&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Zhan_X/0/1/0/all/0/1"&gt;X. Zhan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Zhang_J/0/1/0/all/0/1"&gt;J. Zhang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Zhang_Y/0/1/0/all/0/1"&gt;Y. Zhang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Zheng_X/0/1/0/all/0/1"&gt;X. Zheng&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Zhu_P/0/1/0/all/0/1"&gt;P. Zhu&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-4285108663910955351?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/4285108663910955351/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=4285108663910955351' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4285108663910955351'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4285108663910955351'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1132012.html' title='tipa -- 1/13/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-2631232470666877558</id><published>2012-01-13T21:11:00.000-05:00</published><updated>2012-01-13T21:12:08.111-05:00</updated><title type='text'>tipa -- 1/12/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2182"&gt;On the Spin-Down of Intermittent Pulsars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_J/0/1/0/all/0/1"&gt;Jason Li&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Spitkovsky_A/0/1/0/all/0/1"&gt;Anatoly Spitkovsky&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tchekhovskoy_A/0/1/0/all/0/1"&gt;Alexander Tchekhovskoy&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2195"&gt;The center of the Type Ia supernova remnant SNR 0509-67.5 is empty of any ex-companion star to M_V=+8.4&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schaefer_B/0/1/0/all/0/1"&gt;Bradley E. Schaefer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pagnotta_A/0/1/0/all/0/1"&gt;Ashley Pagnotta&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2244"&gt;Neutrino Transfer in Three Dimensions for Core-Collapse Supernovae. I. Static Configurations&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sumiyoshi_K/0/1/0/all/0/1"&gt;Kohsuke Sumiyoshi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yamada_S/0/1/0/all/0/1"&gt;Shoichi Yamada&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2364"&gt;Evolution of massive population III stars with rotation and magnetic fields&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yoon_S/0/1/0/all/0/1"&gt;S.-C. Yoon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dierks_A/0/1/0/all/0/1"&gt;A. Dierks&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Langer_N/0/1/0/all/0/1"&gt;N. Langer&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.2400"&gt;On the capture of dark matter by neutron stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Guver_T/0/1/0/all/0/1"&gt;Tolga Guver&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Erkoca_A/0/1/0/all/0/1"&gt;Arif Emre Erkoca&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Reno_M/0/1/0/all/0/1"&gt;Mary Hall Reno&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Sarcevic_I/0/1/0/all/0/1"&gt;Ina Sarcevic&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-2631232470666877558?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/2631232470666877558/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=2631232470666877558' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/2631232470666877558'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/2631232470666877558'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1122012.html' title='tipa -- 1/12/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-5037111773717178721</id><published>2012-01-13T21:10:00.000-05:00</published><updated>2012-01-13T21:11:23.429-05:00</updated><title type='text'>tipa -- 1/11/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1909"&gt;New Neutrino Mass Bounds from Sloan Digital Sky Survey III Data Release 8 Photometric Luminous Galaxies&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Putter_R/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Roland de Putter&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mena_O/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Olga Mena&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Giusarma_E/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Elena Giusarma&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ho_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Shirley Ho&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cuesta_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Antonio Cuesta&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Seo_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Hee-Jong Seo&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ross_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Ashley Ross&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+White_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Martin White&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bizyaev_D/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Dmitry Bizyaev&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brewington_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Howard Brewington&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kirkby_D/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;David Kirkby&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Malanushenko_E/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Elena Malanushenko&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Malanushenko_V/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Viktor Malanushenko&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Oravetz_D/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Daniel Oravetz&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pan_K/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Kaike Pan&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Percival_W/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Will J. Percival&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ross_N/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Nicholas P. Ross&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schneider_D/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Donald P. Schneider&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shelden_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Alaina Shelden&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Simmons_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Audrey Simmons&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Snedden_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Stephanie Snedden&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1201.1973"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Observation of TeV gamma rays from the Cygnus region with the ARGO-YBJ experiment&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bartoli_B/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;B. Bartoli&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bernardini_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. Bernardini&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bi_X/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;X. J. Bi&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bleve_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. Bleve&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bolognino_I/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;I. Bolognino&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Branchini_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. Branchini&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Budano_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A. Budano&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Melcarne_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A. K. Calabrese Melcarne&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Camarri_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. Camarri&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cao_Z/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Z. Cao&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cardarelli_R/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;R. Cardarelli&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Catalanotti_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. Catalanotti&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cattaneo_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. Cattaneo&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chen_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. Z. Chen&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chen_T/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;T. L. Chen&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chen_Y/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Y. Chen&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Creti_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. Creti&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cui_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. W. Cui&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dai_B/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;B. Z. Dai&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Staiti_G/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;G. D'Alí Staiti&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Danzengluobu/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Danzengluobu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dattoli_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M. Dattoli&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mitri_I/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;I. De Mitri&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Piazzoli_B/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;B. D'Ettorre Piazzoli&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Girolamo_T/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;T. Di Girolamo&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ding_X/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;X. H. Ding&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sciascio_G/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;G. Di Sciascio&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Feng_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. F. Feng&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Feng_Z/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Zhaoyang Feng&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Feng_Z/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Zhenyong Feng&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Galeazzi_F/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;F. Galeazzi&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Giroletti_E/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;E. Giroletti&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gou_Q/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Q. B. Gou&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guo_Y/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Y. Q. Guo&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+He_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;H. H. He&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hu_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Haibing Hu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hu_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Hongbo Hu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Huang_Q/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Q. Huang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Iacovacci_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M. Iacovacci&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Iuppa_R/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;R. Iuppa&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+James_I/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;I. James&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jia_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;H. Y. Jia&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Labaciren/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Labaciren&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;H. J. Li&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;J. Y. Li&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_X/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;X. X. Li&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liguori_G/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;G. Liguori&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liu_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. Liu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liu_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. Q. Liu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liu_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;J. Liu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liu_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M. Y. Liu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lu_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;H. Lu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ma_L/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;L. L. Ma&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ma_X/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;X. H. Ma&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mancarella_G/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;G. Mancarella&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mari_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. M. Mari&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marsella_G/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;G. Marsella&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Martello_D/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;D. Martello&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mastroianni_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. Mastroianni&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Montini_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. Montini&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ning_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. C. Ning&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pagliaro_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A. Pagliaro&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Panareo_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M. Panareo&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Panico_B/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;B. Panico&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perrone_L/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;L. Perrone&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pistilli_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. Pistilli&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ruggieri_F/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;F. Ruggieri&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Salvini_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. Salvini&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Santonico_R/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;R. Santonico&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shen_P/0/1/0/all/0/1"&gt;P. R. Shen&lt;/a&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sheng_X/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;X. D. Sheng&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shi_F/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;F. Shi&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stanescu_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. Stanescu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Surdo_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A. Surdo&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tan_Y/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Y. H. Tan&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vallania_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. Vallania&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vernetto_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. Vernetto&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vigorito_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. Vigorito&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wang_B/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;B. Wang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wang_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;H. Wang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wu_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;C. Y. Wu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wu_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;H. R. Wu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Xu_B/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;B. Xu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Xue_L/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;L. Xue&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yang_Q/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Q. Y. Yang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yang_X/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;X. C. Yang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yao_Z/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Z.G. Yao&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yuan_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A. F. Yuan&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zha_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M. Zha&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_H/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;H. M. Zhang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Jilong Zhang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Jianli Zhang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_L/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;L. Zhang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P. Zhang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_X/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;X. Y. Zhang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_Y/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Y. Zhang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhao_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;J. Zhao&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhaxiciren/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Zhaxiciren&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhaxisangzhu/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Zhaxisangzhu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhou_X/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;X. X. Zhou&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_F/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;F. R. Zhu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_Q/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Q. Q. Zhu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zizzi_G/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;G. Zizzi&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1201.2044"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Discovery of hard-spectrum γ-ray emission from the BL Lac object 1ES 0414+009&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_HESS/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;HESS Collaboration&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1201.2091"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Temporal signatures of leptohadronic feedback mechanisms in compact sources&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Petropoulou_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Maria Petropoulou&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mastichiadis_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Apostolos Mastichiadis&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1201.2101"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Constraining the physics of the r-mode instability in neutron stars with X-ray and UV observations&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Haskell_B/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Brynmor Haskell&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Degenaar_N/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Nathalie Degenaar&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ho_W/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Wynn C.G. Ho&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-5037111773717178721?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/5037111773717178721/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=5037111773717178721' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5037111773717178721'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5037111773717178721'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1112012.html' title='tipa -- 1/11/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-6281580494413391288</id><published>2012-01-13T21:02:00.000-05:00</published><updated>2012-01-13T21:03:02.254-05:00</updated><title type='text'>tipa -- 1/10/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1895"&gt;WIMP diffusion in the solar system including solar WIMP-nucleon scattering&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sivertsson_S/0/1/0/all/0/1"&gt;Sofia Sivertsson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Edsjo_J/0/1/0/all/0/1"&gt;Joakim Edsjo&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1894"&gt;X-ray Observations of a New Unusual Magnetar Swift J1834.9-0846&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kargaltsev_O/0/1/0/all/0/1"&gt;Oleg Kargaltsev&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kouveliotou_C/0/1/0/all/0/1"&gt;Chryssa Kouveliotou&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pavlov_G/0/1/0/all/0/1"&gt;George G. Pavlov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gogus_E/0/1/0/all/0/1"&gt;Ersin Gogus&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lin_L/0/1/0/all/0/1"&gt;Lin Lin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wachter_S/0/1/0/all/0/1"&gt;Stefanie Wachter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Griffith_R/0/1/0/all/0/1"&gt;Roger L. Griffith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kaneko_Y/0/1/0/all/0/1"&gt;Yuki Kaneko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Younes_G/0/1/0/all/0/1"&gt;George Younes&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1660"&gt;Origin of TeV Galactic Cosmic Rays&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Neronov_A/0/1/0/all/0/1"&gt;A. Neronov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Semikoz_D/0/1/0/all/0/1"&gt;D. V. Semikoz&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-6281580494413391288?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/6281580494413391288/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=6281580494413391288' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6281580494413391288'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6281580494413391288'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-1102012.html' title='tipa -- 1/10/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-686648908954331521</id><published>2012-01-13T20:58:00.001-05:00</published><updated>2012-01-13T20:58:51.482-05:00</updated><title type='text'>tipa -- 1/9/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1386"&gt;First Muon-Neutrino Disappearance Study with an Off-Axis Beam&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Collaboration_T2K/0/1/0/all/0/1"&gt;T2K Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1328"&gt;Effects of Rotation on the Minimum Mass of Primordial Progenitors of Pair Instability Supernovae&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chatzopoulos_E/0/1/0/all/0/1"&gt;Emmanouil Chatzopoulos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wheeler_J/0/1/0/all/0/1"&gt;J. Craig Wheeler&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1414"&gt;Physics of the Galactic Center Cloud G2, on its Way towards the Super-Massive Black Hole&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Burkert_A/0/1/0/all/0/1"&gt;Andreas Burkert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schartmann_M/0/1/0/all/0/1"&gt;Mark Schartmann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Alig_C/0/1/0/all/0/1"&gt;Christian Alig&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gillessen_S/0/1/0/all/0/1"&gt;Stefan Gillessen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Genzel_R/0/1/0/all/0/1"&gt;Reinhard Genzel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fritz_T/0/1/0/all/0/1"&gt;Tobias Fritz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eisenhauer_F/0/1/0/all/0/1"&gt;Frank Eisenhauer&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-686648908954331521?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/686648908954331521/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=686648908954331521' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/686648908954331521'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/686648908954331521'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-192012.html' title='tipa -- 1/9/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-8919057771412747539</id><published>2012-01-08T02:26:00.001-05:00</published><updated>2012-01-08T02:26:52.469-05:00</updated><title type='text'>tipa -- 1/6/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0994"&gt;EVLA Observations Constrain the Environment and Progenitor System of Type Ia Supernova 2011fe&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chomiuk_L/0/1/0/all/0/1"&gt;Laura Chomiuk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Soderberg_A/0/1/0/all/0/1"&gt;Alicia M. Soderberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Moe_M/0/1/0/all/0/1"&gt;Maxwell Moe&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chevalier_R/0/1/0/all/0/1"&gt;Roger A. Chevalier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rupen_M/0/1/0/all/0/1"&gt;Michael P. Rupen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Badenes_C/0/1/0/all/0/1"&gt;Carles Badenes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Margutti_R/0/1/0/all/0/1"&gt;Raffaella Margutti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fransson_C/0/1/0/all/0/1"&gt;Claes Fransson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fong_W/0/1/0/all/0/1"&gt;Wen-fai Fong&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dittmann_J/0/1/0/all/0/1"&gt;Jason A. Dittmann&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1003"&gt;Evidence for extended gamma-ray emission from galaxy clusters&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Han_J/0/1/0/all/0/1"&gt;Jiaxin Han&lt;/a&gt; (1,2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Frenk_C/0/1/0/all/0/1"&gt;Carlos S. Frenk&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eke_V/0/1/0/all/0/1"&gt;Vincent R. Eke&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gao_L/0/1/0/all/0/1"&gt;Liang Gao&lt;/a&gt; (3,2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+White_S/0/1/0/all/0/1"&gt;Simon D. M. White&lt;/a&gt; (4) ((1) Shanghai A.O., (2) ICC Durham, (3) NAOC, (4) MPA)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1005"&gt;The Grand Cosmic Web of the First Stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Visbal_E/0/1/0/all/0/1"&gt;Eli Visbal&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Barkana_R/0/1/0/all/0/1"&gt;Rennan Barkana&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fialkov_A/0/1/0/all/0/1"&gt;Anastasia Fialkov&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tseliakhovich_D/0/1/0/all/0/1"&gt;Dmitriy Tseliakhovich&lt;/a&gt; (3), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hirata_C/0/1/0/all/0/1"&gt;Christopher Hirata&lt;/a&gt; (3) ((1) Harvard University, (2) Tel Aviv University, (3) Caltech)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1006"&gt;On the Mass Distribution and Birth Masses of Neutron Stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ozel_F/0/1/0/all/0/1"&gt;Feryal Ozel&lt;/a&gt; (Arizona), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Psaltis_D/0/1/0/all/0/1"&gt;Dimitrios Psaltis&lt;/a&gt; (Arizona), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Narayan_R/0/1/0/all/0/1"&gt;Ramesh Narayan&lt;/a&gt; (Harvard), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Villarreal_A/0/1/0/all/0/1"&gt;Antonio Santos Villarreal&lt;/a&gt; (Arizona)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.1217"&gt;Deep Observation of the Giant Radio Lobes of Centaurus A with the Fermi Large Area Telescope&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yang_R/0/1/0/all/0/1"&gt;Rui-zhi Yang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sahakyan_N/0/1/0/all/0/1"&gt;Narek Sahakyan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wilhelmi_E/0/1/0/all/0/1"&gt;Emma de Ona Wilhelmi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Aharonian_F/0/1/0/all/0/1"&gt;Felix Aharonian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rieger_F/0/1/0/all/0/1"&gt;Frank Rieger&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0997"&gt;Interacting dark matter contribution to the Galactic 511 keV gamma ray emission: constraining the morphology with INTEGRAL/SPI observations&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Vincent_A/0/1/0/all/0/1"&gt;Aaron C. Vincent&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Martin_P/0/1/0/all/0/1"&gt;Pierrick Martin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Cline_J/0/1/0/all/0/1"&gt;James M. Cline&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-8919057771412747539?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/8919057771412747539/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=8919057771412747539' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8919057771412747539'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8919057771412747539'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-162012.html' title='tipa -- 1/6/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-9038163446724421816</id><published>2012-01-08T02:16:00.000-05:00</published><updated>2012-01-08T02:17:02.282-05:00</updated><title type='text'>tipa -- 1/5/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0753"&gt;Fermi-LAT constraints on dark matter annihilation cross section with the Fornax cluster&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ando_S/0/1/0/all/0/1"&gt;Shin'ichiro Ando&lt;/a&gt; (Amsterdam), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nagai_D/0/1/0/all/0/1"&gt;Daisuke Nagai&lt;/a&gt; (Yale)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0757"&gt;Concordance models of reionization: implications for faint galaxies and escape fraction evolution&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kuhlen_M/0/1/0/all/0/1"&gt;M. Kuhlen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Faucher_Giguere_C/0/1/0/all/0/1"&gt;C.-A. Faucher-Giguere&lt;/a&gt; (UC Berkeley)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0770"&gt;EVLA Observations of the Radio Evolution of SN 2011dh&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Krauss_M/0/1/0/all/0/1"&gt;M. I. Krauss&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Soderberg_A/0/1/0/all/0/1"&gt;A. M. Soderberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chomiuk_L/0/1/0/all/0/1"&gt;L. Chomiuk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zauderer_B/0/1/0/all/0/1"&gt;B. A. Zauderer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brunthaler_A/0/1/0/all/0/1"&gt;A. Brunthaler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bietenholz_M/0/1/0/all/0/1"&gt;M. F. Bietenholz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chevalier_R/0/1/0/all/0/1"&gt;R. A. Chevalier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fransson_C/0/1/0/all/0/1"&gt;C. Fransson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rupen_M/0/1/0/all/0/1"&gt;M. Rupen&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0771"&gt;VLBI Observations of the Nearby Type IIb Supernova 2011dh&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bietenholz_M/0/1/0/all/0/1"&gt;M. F. Bietenholz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brunthaler_A/0/1/0/all/0/1"&gt;A. Brunthaler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Soderberg_A/0/1/0/all/0/1"&gt;A. M. Soderberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Krauss_M/0/1/0/all/0/1"&gt;M. Krauss&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bartel_N/0/1/0/all/0/1"&gt;N. Bartel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chomiuk_L/0/1/0/all/0/1"&gt;L. Chomiuk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rupen_M/0/1/0/all/0/1"&gt;M. P. Rupen&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0837"&gt;Stochastic Particle Acceleration in Multiple Magnetic Islands during Reconnection&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hoshino_M/0/1/0/all/0/1"&gt;Masahiro Hoshino&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0960"&gt;"Soft" Hadronic Cross Sections Challenge Hidden Dimensions&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Block_M/0/1/0/all/0/1"&gt;Martin M. Block&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Halzen_F/0/1/0/all/0/1"&gt;Francis Halzen&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-9038163446724421816?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/9038163446724421816/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=9038163446724421816' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/9038163446724421816'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/9038163446724421816'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-152012.html' title='tipa -- 1/5/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-4310238424124298479</id><published>2012-01-08T02:11:00.000-05:00</published><updated>2012-01-08T02:12:29.155-05:00</updated><title type='text'>tipa -- 1/4/2012</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0664"&gt;On the mechanism of hard X-ray emission from magnetars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Beloborodov_A/0/1/0/all/0/1"&gt;Andrei M. Beloborodov&lt;/a&gt; (Columbia University)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0568"&gt;Spectral index properties of milliJansky radio sources&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Randall_K/0/1/0/all/0/1"&gt;Kate Randall&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hopkins_A/0/1/0/all/0/1"&gt;Andrew Hopkins&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Norris_R/0/1/0/all/0/1"&gt;Ray Norris&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zinn_P/0/1/0/all/0/1"&gt;Peter-Christian Zinn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Middelberg_E/0/1/0/all/0/1"&gt;Enno Middelberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mao_M/0/1/0/all/0/1"&gt;Minnie Mao&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sharp_R/0/1/0/all/0/1"&gt;Rob Sharp&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0369"&gt;Measures of cosmic-ray energy densities in galaxies&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Persic_M/0/1/0/all/0/1"&gt;Massimo Persic&lt;/a&gt; (INAF+INFN Trieste), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rephaeli_Y/0/1/0/all/0/1"&gt;Yoel Rephaeli&lt;/a&gt; (Tel Aviv U, UC San Diego)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1201.0018"&gt;Measurements of the Cosmic Ray Composition with Air Shower Experiments&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kampert_K/0/1/0/all/0/1"&gt;Karl-Heinz Kampert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Unger_M/0/1/0/all/0/1"&gt;Michael Unger&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-4310238424124298479?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/4310238424124298479/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=4310238424124298479' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4310238424124298479'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4310238424124298479'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2012/01/tipa-142012.html' title='tipa -- 1/4/2012'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-6261906407254300526</id><published>2011-12-29T21:44:00.001-05:00</published><updated>2011-12-29T21:44:54.752-05:00</updated><title type='text'>tipa -- 12/30/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.6353"&gt;Indication for the disappearance of reactor electron antineutrinos in the Double Chooz experiment&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 8pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Abe_Y/0/1/0/all/0/1"&gt;Y. Abe&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Aberle_C/0/1/0/all/0/1"&gt;C. Aberle&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Akiri_T/0/1/0/all/0/1"&gt;T. Akiri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Anjos_J/0/1/0/all/0/1"&gt;J.C. dos Anjos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Ardellier_F/0/1/0/all/0/1"&gt;F. Ardellier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Barbosa_A/0/1/0/all/0/1"&gt;A.F. Barbosa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Baxter_A/0/1/0/all/0/1"&gt;A. Baxter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Bernstein_A/0/1/0/all/0/1"&gt;A. Bernstein&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Bezerra_T/0/1/0/all/0/1"&gt;T.J.C. Bezerra&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Bezrukhov_L/0/1/0/all/0/1"&gt;L. Bezrukhov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Blucher_E/0/1/0/all/0/1"&gt;E. Blucher&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Bongrand_M/0/1/0/all/0/1"&gt;M. Bongrand&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Bowden_N/0/1/0/all/0/1"&gt;N.S. Bowden&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Buck_C/0/1/0/all/0/1"&gt;C. Buck&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Busenitz_J/0/1/0/all/0/1"&gt;J. Busenitz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Cabrera_A/0/1/0/all/0/1"&gt;A. Cabrera&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Caden_E/0/1/0/all/0/1"&gt;E. Caden&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Camilleri_L/0/1/0/all/0/1"&gt;L. Camilleri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Carr_R/0/1/0/all/0/1"&gt;R. Carr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Cerrada_M/0/1/0/all/0/1"&gt;M. Cerrada&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Chang_P/0/1/0/all/0/1"&gt;P.-J. Chang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Chimenti_P/0/1/0/all/0/1"&gt;P. Chimenti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Classen_T/0/1/0/all/0/1"&gt;T. Classen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Collin_A/0/1/0/all/0/1"&gt;A. Collin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Conover_E/0/1/0/all/0/1"&gt;E. Conover&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Conrad_J/0/1/0/all/0/1"&gt;J.M. Conrad&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Cormon_S/0/1/0/all/0/1"&gt;S. Cormon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Crespo_Anadon_J/0/1/0/all/0/1"&gt;J.I. Crespo-Anadón&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Cribier_M/0/1/0/all/0/1"&gt;M. Cribier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Crum_K/0/1/0/all/0/1"&gt;K. Crum&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Cucoanes_A/0/1/0/all/0/1"&gt;A. Cucoanes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+DAgostino_M/0/1/0/all/0/1"&gt;M.V. D'Agostino&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Damon_E/0/1/0/all/0/1"&gt;E. Damon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Dawson_J/0/1/0/all/0/1"&gt;J.V. Dawson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Dazeley_S/0/1/0/all/0/1"&gt;S. Dazeley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Dierckxsens_M/0/1/0/all/0/1"&gt;M. Dierckxsens&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Dietrich_D/0/1/0/all/0/1"&gt;D. Dietrich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Djurcic_Z/0/1/0/all/0/1"&gt;Z. Djurcic&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Dracos_M/0/1/0/all/0/1"&gt;M. Dracos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Durand_V/0/1/0/all/0/1"&gt;V. Durand&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Efremenko_Y/0/1/0/all/0/1"&gt;Y. Efremenko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Endo_Y/0/1/0/all/0/1"&gt;Y. Endo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Etenko_A/0/1/0/all/0/1"&gt;A. Etenko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Falk_E/0/1/0/all/0/1"&gt;E. Falk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Fallot_M/0/1/0/all/0/1"&gt;M. Fallot&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Fechner_M/0/1/0/all/0/1"&gt;M. Fechner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Feilitzsch_F/0/1/0/all/0/1"&gt;F. von Feilitzsch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Felde_J/0/1/0/all/0/1"&gt;J. Felde&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Fernandes_S/0/1/0/all/0/1"&gt;S.M. Fernandes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Franco_D/0/1/0/all/0/1"&gt;D. Franco&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Franke_A/0/1/0/all/0/1"&gt;A. Franke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Franke_M/0/1/0/all/0/1"&gt;M. Franke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Furuta_H/0/1/0/all/0/1"&gt;H. Furuta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Gama_R/0/1/0/all/0/1"&gt;R. Gama&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Gil_Botella_I/0/1/0/all/0/1"&gt;I. Gil-Botella&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Giot_L/0/1/0/all/0/1"&gt;L. Giot&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Goger_Neff_M/0/1/0/all/0/1"&gt;M. Göger-Neff&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Gonzalez_L/0/1/0/all/0/1"&gt;L.F.G. Gonzalez&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Goodman_M/0/1/0/all/0/1"&gt;M.C. Goodman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Goon_J/0/1/0/all/0/1"&gt;J.TM. Goon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Greiner_D/0/1/0/all/0/1"&gt;D. Greiner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Guillon_B/0/1/0/all/0/1"&gt;B. Guillon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Haag_N/0/1/0/all/0/1"&gt;N. Haag&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Hagner_C/0/1/0/all/0/1"&gt;C. Hagner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Hara_T/0/1/0/all/0/1"&gt;T. Hara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Hartmann_F/0/1/0/all/0/1"&gt;F.X. Hartmann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Hartnell_J/0/1/0/all/0/1"&gt;J. Hartnell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Haruna_T/0/1/0/all/0/1"&gt;T. Haruna&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Haser_J/0/1/0/all/0/1"&gt;J. Haser&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Hatzikoutelis_A/0/1/0/all/0/1"&gt;A. Hatzikoutelis&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Hayakawa_T/0/1/0/all/0/1"&gt;T. Hayakawa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Hofmann_M/0/1/0/all/0/1"&gt;M. Hofmann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Horton_Smith_G/0/1/0/all/0/1"&gt;G. Horton-Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Ishitsuka_M/0/1/0/all/0/1"&gt;M. Ishitsuka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Jochum_J/0/1/0/all/0/1"&gt;J. Jochum&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Jollet_C/0/1/0/all/0/1"&gt;C. Jollet&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Jones_C/0/1/0/all/0/1"&gt;C.L. Jones&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kaether_F/0/1/0/all/0/1"&gt;F. Kaether&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kalousis_L/0/1/0/all/0/1"&gt;L. Kalousis&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kamyshkov_Y/0/1/0/all/0/1"&gt;Y. Kamyshkov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kaplan_D/0/1/0/all/0/1"&gt;D. Kaplan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kawasaki_T/0/1/0/all/0/1"&gt;T. Kawasaki&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Keefer_G/0/1/0/all/0/1"&gt;G. Keefer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kemp_E/0/1/0/all/0/1"&gt;E. Kemp&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kerret_H/0/1/0/all/0/1"&gt;H. de Kerret&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kibe_Y/0/1/0/all/0/1"&gt;Y. Kibe&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Konno_T/0/1/0/all/0/1"&gt;T. Konno&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kryn_D/0/1/0/all/0/1"&gt;D. Kryn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kuze_M/0/1/0/all/0/1"&gt;M. Kuze&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Lachenmaier_T/0/1/0/all/0/1"&gt;T. Lachenmaier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Lane_C/0/1/0/all/0/1"&gt;C.E. Lane&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Langbrandtner_C/0/1/0/all/0/1"&gt;C. Langbrandtner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Lasserre_T/0/1/0/all/0/1"&gt;T. Lasserre&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Letourneau_A/0/1/0/all/0/1"&gt;A. Letourneau&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Lhuillier_D/0/1/0/all/0/1"&gt;D. Lhuillier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Lima_H/0/1/0/all/0/1"&gt;H.P. Lima Jr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Lindner_M/0/1/0/all/0/1"&gt;M. Lindner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Liu_Y/0/1/0/all/0/1"&gt;Y. Liu&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Lopez_Castano_J/0/1/0/all/0/1"&gt;J.M. López-Castanõ&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+LoSecco_J/0/1/0/all/0/1"&gt;J.M. LoSecco&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Lubsandorzhiev_B/0/1/0/all/0/1"&gt;B.K. Lubsandorzhiev&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Lucht_S/0/1/0/all/0/1"&gt;S. Lucht&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+McKee_D/0/1/0/all/0/1"&gt;D. McKee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Maeda_J/0/1/0/all/0/1"&gt;J. Maeda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Maesano_C/0/1/0/all/0/1"&gt;C.N. Maesano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Mariani_C/0/1/0/all/0/1"&gt;C. Mariani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Maricic_J/0/1/0/all/0/1"&gt;J. Maricic&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Martino_J/0/1/0/all/0/1"&gt;J. Martino&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Matsubara_T/0/1/0/all/0/1"&gt;T. Matsubara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Mention_G/0/1/0/all/0/1"&gt;G. Mention&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Meregaglia_A/0/1/0/all/0/1"&gt;A. Meregaglia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Miletic_T/0/1/0/all/0/1"&gt;T. Miletic&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Milincic_R/0/1/0/all/0/1"&gt;R. Milincic&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Milzstajn_A/0/1/0/all/0/1"&gt;A. Milzstajn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Miyata_H/0/1/0/all/0/1"&gt;H. Miyata&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Motta_D/0/1/0/all/0/1"&gt;D. Motta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Mueller_T/0/1/0/all/0/1"&gt;Th.A. Mueller&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Nagasaka_Y/0/1/0/all/0/1"&gt;Y. Nagasaka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Nakajima_K/0/1/0/all/0/1"&gt;K. Nakajima&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Novella_P/0/1/0/all/0/1"&gt;P. Novella&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Obolensky_M/0/1/0/all/0/1"&gt;M. Obolensky&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Oberauer_L/0/1/0/all/0/1"&gt;L. Oberauer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Onillon_A/0/1/0/all/0/1"&gt;A. Onillon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Osborn_A/0/1/0/all/0/1"&gt;A. Osborn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Ostrovskiy_I/0/1/0/all/0/1"&gt;I. Ostrovskiy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Palomares_C/0/1/0/all/0/1"&gt;C. Palomares&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Peeters_S/0/1/0/all/0/1"&gt;S.J.M. Peeters&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Pepe_I/0/1/0/all/0/1"&gt;I.M. Pepe&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Perrin_P/0/1/0/all/0/1"&gt;P. Perrin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Pfahler_P/0/1/0/all/0/1"&gt;P. Pfahler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Porta_A/0/1/0/all/0/1"&gt;A. Porta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Potzel_W/0/1/0/all/0/1"&gt;W. Potzel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Queval_R/0/1/0/all/0/1"&gt;R. Queval&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Reichenbacher_J/0/1/0/all/0/1"&gt;J. Reichenbacher&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Reinhold_B/0/1/0/all/0/1"&gt;B. Reinhold&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Remoto_A/0/1/0/all/0/1"&gt;A. Remoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Reyna_D/0/1/0/all/0/1"&gt;D. Reyna&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Rohling_M/0/1/0/all/0/1"&gt;M. Röhling&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Roth_S/0/1/0/all/0/1"&gt;S. Roth&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Rubin_H/0/1/0/all/0/1"&gt;H.A. Rubin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Sakamoto_Y/0/1/0/all/0/1"&gt;Y. Sakamoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Santorelli_R/0/1/0/all/0/1"&gt;R. Santorelli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Sato_F/0/1/0/all/0/1"&gt;F. Sato&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Schonert_S/0/1/0/all/0/1"&gt;S. Schönert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Schoppmann_S/0/1/0/all/0/1"&gt;S. Schoppmann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Schwan_U/0/1/0/all/0/1"&gt;U. Schwan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Schwetz_T/0/1/0/all/0/1"&gt;T. Schwetz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Shaevitz_M/0/1/0/all/0/1"&gt;M. Shaevitz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Shrestha_D/0/1/0/all/0/1"&gt;D. Shrestha&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Sida_J/0/1/0/all/0/1"&gt;J-L. Sida&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Sinev_V/0/1/0/all/0/1"&gt;V. Sinev&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Skorokhvatov_M/0/1/0/all/0/1"&gt;M. Skorokhvatov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Smith_E/0/1/0/all/0/1"&gt;E. Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Stahl_A/0/1/0/all/0/1"&gt;A. Stahl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Stancu_I/0/1/0/all/0/1"&gt;I. Stancu&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Strait_M/0/1/0/all/0/1"&gt;M. Strait&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Stuken_A/0/1/0/all/0/1"&gt;A. Stüken&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Suekane_F/0/1/0/all/0/1"&gt;F. Suekane&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Sukhotin_S/0/1/0/all/0/1"&gt;S. Sukhotin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Sumiyoshi_T/0/1/0/all/0/1"&gt;T. Sumiyoshi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Sun_Y/0/1/0/all/0/1"&gt;Y. Sun&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Sun_Z/0/1/0/all/0/1"&gt;Z. Sun&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Svoboda_R/0/1/0/all/0/1"&gt;R. Svoboda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Tabata_H/0/1/0/all/0/1"&gt;H. Tabata&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Tamura_N/0/1/0/all/0/1"&gt;N. Tamura&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Terao_K/0/1/0/all/0/1"&gt;K. Terao&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Tonazzo_A/0/1/0/all/0/1"&gt;A. Tonazzo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Toups_M/0/1/0/all/0/1"&gt;M. Toups&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Thi_H/0/1/0/all/0/1"&gt;H.H. Trinh Thi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Veyssiere_C/0/1/0/all/0/1"&gt;C. Veyssiere&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Vignaud_D/0/1/0/all/0/1"&gt;D. Vignaud&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Wagner_S/0/1/0/all/0/1"&gt;S. Wagner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Watanabe_H/0/1/0/all/0/1"&gt;H. Watanabe&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+White_B/0/1/0/all/0/1"&gt;B. White&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Wiebusch_C/0/1/0/all/0/1"&gt;C. Wiebusch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Winslow_L/0/1/0/all/0/1"&gt;L. Winslow&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Worcester_M/0/1/0/all/0/1"&gt;M. Worcester&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Wurm_M/0/1/0/all/0/1"&gt;M. Wurm&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Yanovitch_E/0/1/0/all/0/1"&gt;E. Yanovitch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Yermia_F/0/1/0/all/0/1"&gt;F. Yermia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Zbiri_K/0/1/0/all/0/1"&gt;K. Zbiri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Zimmer_V/0/1/0/all/0/1"&gt;V. Zimmer&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5664"&gt;Multi-GeV Neutrino Emission from Magnetized Gamma Ray Bursts&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gao_S/0/1/0/all/0/1"&gt;Shan Gao&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meszaros_P/0/1/0/all/0/1"&gt;Peter Meszaros&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5684"&gt;Nucleosynthesis in core-collapse supernova explosions triggered by a quark-hadron phase transition&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nishimura_N/0/1/0/all/0/1"&gt;Nobuya Nishimura&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fischer_T/0/1/0/all/0/1"&gt;Tobias Fischer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Thielemann_F/0/1/0/all/0/1"&gt;Friedrich-Karl Thielemann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Frohlich_C/0/1/0/all/0/1"&gt;Carla Fröhlich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hempel_M/0/1/0/all/0/1"&gt;Matthias Hempel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kappeli_R/0/1/0/all/0/1"&gt;Roger Käppeli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Martinez_Pinedo_G/0/1/0/all/0/1"&gt;Gabriel Martínez-Pinedo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rauscher_T/0/1/0/all/0/1"&gt;Thomas Rauscher&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sagert_I/0/1/0/all/0/1"&gt;Irina Sagert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Winteler_C/0/1/0/all/0/1"&gt;Christian Winteler&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5821"&gt;Detection of X-Ray Emission from the Unidentified TeV Gamma-Ray Source TeV J2032+4130&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Murakami_H/0/1/0/all/0/1"&gt;Hiroshi Murakami&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kitamoto_S/0/1/0/all/0/1"&gt;Shunji Kitamoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kawachi_A/0/1/0/all/0/1"&gt;Akiko Kawachi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nakamori_T/0/1/0/all/0/1"&gt;Takeshi Nakamori&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.6005"&gt;First Low-Latency LIGO+Virgo Search for Binary Inspirals and their Electromagnetic Counterparts&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_LIGO_Scientific/0/1/0/all/0/1"&gt;LIGO Scientific Collaboration&lt;/a&gt;, The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Virgo/0/1/0/all/0/1"&gt;Virgo Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.6373"&gt;On the Amplification of Magnetic Field by a Supernova Blast Shock Wave in a Turbulent Medium&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guo_F/0/1/0/all/0/1"&gt;Fan Guo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_S/0/1/0/all/0/1"&gt;Shengtai Li&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_H/0/1/0/all/0/1"&gt;Hui Li&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Giacalone_J/0/1/0/all/0/1"&gt;Joe Giacalone&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jokipii_J/0/1/0/all/0/1"&gt;J. R. Jokipii&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_D/0/1/0/all/0/1"&gt;David Li&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5992"&gt;Neutrino Masses from the Top Down&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Langacker_P/0/1/0/all/0/1"&gt;Paul Langacker&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-6261906407254300526?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/6261906407254300526/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=6261906407254300526' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6261906407254300526'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6261906407254300526'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12302011.html' title='tipa -- 12/30/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-7990768188297818189</id><published>2011-12-29T21:08:00.000-05:00</published><updated>2011-12-29T21:09:14.039-05:00</updated><title type='text'>tipa -- 12/26/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5599"&gt;Cosmic Ray Anisotropy as Signature for the Transition from Galactic to Extragalactic Cosmic Rays&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Giacinti_G/0/1/0/all/0/1"&gt;G. Giacinti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kachelriess_M/0/1/0/all/0/1"&gt;M. Kachelriess&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Semikoz_D/0/1/0/all/0/1"&gt;D. V. Semikoz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sigl_G/0/1/0/all/0/1"&gt;G. Sigl&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5541"&gt;Low-energy break in the spectrum of Galactic cosmic rays&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Neronov_A/0/1/0/all/0/1"&gt;A.Neronov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Semikoz_D/0/1/0/all/0/1"&gt;D.V.Semikoz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taylor_A/0/1/0/all/0/1"&gt;A.M.Taylor&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5523"&gt;Spectra and Mass Composition of Ultrahigh-Energy Cosmic Rays from Point Sources&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kalmykov_N/0/1/0/all/0/1"&gt;N. N. Kalmykov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shustova_O/0/1/0/all/0/1"&gt;O. P. Shustova&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Uryson_A/0/1/0/all/0/1"&gt;A. V. Uryson&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-7990768188297818189?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/7990768188297818189/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=7990768188297818189' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7990768188297818189'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7990768188297818189'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12262011.html' title='tipa -- 12/26/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-5988917482096213301</id><published>2011-12-22T22:16:00.001-05:00</published><updated>2011-12-22T22:16:39.817-05:00</updated><title type='text'>tipa -- 12/23/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5185"&gt;Neutrino processes in partially degenerate neutron matter&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bacca_S/0/1/0/all/0/1"&gt;S. Bacca&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hally_K/0/1/0/all/0/1"&gt;K. Hally&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liebendorfer_M/0/1/0/all/0/1"&gt;M. Liebendörfer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perego_A/0/1/0/all/0/1"&gt;A. Perego&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pethick_C/0/1/0/all/0/1"&gt;C. J. Pethick&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schwenk_A/0/1/0/all/0/1"&gt;A. Schwenk&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5207"&gt;The Source Density and Observability of Pair-Instability Supernovae from the First Stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hummel_J/0/1/0/all/0/1"&gt;Jacob Hummel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pawlik_A/0/1/0/all/0/1"&gt;Andreas Pawlik&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Milosavljevic_M/0/1/0/all/0/1"&gt;Milos Milosavljevic&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bromm_V/0/1/0/all/0/1"&gt;Volker Bromm&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5435"&gt;Cosmological Constraints from Sunyaev-Zel'dovich-Selected Clusters with X-ray Observations in the First 178 Square Degrees of the South Pole Telescope Survey&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Benson_B/0/1/0/all/0/1"&gt;B. A. Benson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Haan_T/0/1/0/all/0/1"&gt;T. de Haan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dudley_J/0/1/0/all/0/1"&gt;J. P. Dudley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reichardt_C/0/1/0/all/0/1"&gt;C. L. Reichardt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Aird_K/0/1/0/all/0/1"&gt;K. A. Aird&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Andersson_K/0/1/0/all/0/1"&gt;K. Andersson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Armstrong_R/0/1/0/all/0/1"&gt;R. Armstrong&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bautz_M/0/1/0/all/0/1"&gt;M. Bautz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bayliss_M/0/1/0/all/0/1"&gt;M. Bayliss&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bazin_G/0/1/0/all/0/1"&gt;G. Bazin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bleem_L/0/1/0/all/0/1"&gt;L. E. Bleem&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brodwin_M/0/1/0/all/0/1"&gt;M. Brodwin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Carlstrom_J/0/1/0/all/0/1"&gt;J. E. Carlstrom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chang_C/0/1/0/all/0/1"&gt;C. L. Chang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cho_H/0/1/0/all/0/1"&gt;H. M. Cho&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Clocchiatti_A/0/1/0/all/0/1"&gt;A. Clocchiatti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Crawford_T/0/1/0/all/0/1"&gt;T. M. Crawford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Crites_A/0/1/0/all/0/1"&gt;A. T. Crites&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Desai_S/0/1/0/all/0/1"&gt;S. Desai&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dobbs_M/0/1/0/all/0/1"&gt;M. A. Dobbs&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Foley_R/0/1/0/all/0/1"&gt;R. J. Foley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Forman_W/0/1/0/all/0/1"&gt;W. R. Forman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+George_E/0/1/0/all/0/1"&gt;E. M. George&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gladders_M/0/1/0/all/0/1"&gt;M. D. Gladders&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Halverson_N/0/1/0/all/0/1"&gt;N. W. Halverson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+High_F/0/1/0/all/0/1"&gt;F. W. High&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holder_G/0/1/0/all/0/1"&gt;G. P. Holder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holzapfel_W/0/1/0/all/0/1"&gt;W. L. Holzapfel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hoover_S/0/1/0/all/0/1"&gt;S. Hoover&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hrubes_J/0/1/0/all/0/1"&gt;J. D. Hrubes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jones_C/0/1/0/all/0/1"&gt;C. Jones&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Joy_M/0/1/0/all/0/1"&gt;M. Joy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Keisler_R/0/1/0/all/0/1"&gt;R. Keisler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Knox_L/0/1/0/all/0/1"&gt;L. Knox&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lee_A/0/1/0/all/0/1"&gt;A. T. Lee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Leitch_E/0/1/0/all/0/1"&gt;E. M. Leitch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liu_J/0/1/0/all/0/1"&gt;J. Liu&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lueker_M/0/1/0/all/0/1"&gt;M. Lueker&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Luong_Van_D/0/1/0/all/0/1"&gt;D. Luong-Van&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mantz_A/0/1/0/all/0/1"&gt;A. Mantz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marrone_D/0/1/0/all/0/1"&gt;D. P. Marrone&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McDonald_M/0/1/0/all/0/1"&gt;M. McDonald&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McMahon_J/0/1/0/all/0/1"&gt;J. J. McMahon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mehl_J/0/1/0/all/0/1"&gt;J. Mehl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meyer_S/0/1/0/all/0/1"&gt;S. S. Meyer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mocanu_L/0/1/0/all/0/1"&gt;L. Mocanu&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mohr_J/0/1/0/all/0/1"&gt;J. J. Mohr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Montroy_T/0/1/0/all/0/1"&gt;T. E. Montroy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Murray_S/0/1/0/all/0/1"&gt;S. S. Murray&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Natoli_T/0/1/0/all/0/1"&gt;T. Natoli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Padin_S/0/1/0/all/0/1"&gt;S. Padin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Plagge_T/0/1/0/all/0/1"&gt;T. Plagge&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pryke_C/0/1/0/all/0/1"&gt;C. Pryke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rest_A/0/1/0/all/0/1"&gt;A. Rest&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ruel_J/0/1/0/all/0/1"&gt;J. Ruel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ruhl_J/0/1/0/all/0/1"&gt;J. E. Ruhl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Saliwanchik_B/0/1/0/all/0/1"&gt;B. R. Saliwanchik&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Saro_A/0/1/0/all/0/1"&gt;A. Saro&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schaffer_K/0/1/0/all/0/1"&gt;K. K. Schaffer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shaw_L/0/1/0/all/0/1"&gt;L. Shaw&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shirokoff_E/0/1/0/all/0/1"&gt;E. Shirokoff&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Song_J/0/1/0/all/0/1"&gt;J. Song&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Spieler_H/0/1/0/all/0/1"&gt;H. G. Spieler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stalder_B/0/1/0/all/0/1"&gt;B. Stalder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Staniszewski_Z/0/1/0/all/0/1"&gt;Z. Staniszewski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stark_A/0/1/0/all/0/1"&gt;A. A. Stark&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Story_K/0/1/0/all/0/1"&gt;K. Story&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stubbs_C/0/1/0/all/0/1"&gt;C. W. Stubbs&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Suhada_R/0/1/0/all/0/1"&gt;R. Suhada&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Engelen_A/0/1/0/all/0/1"&gt;A. van Engelen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vanderlinde_K/0/1/0/all/0/1"&gt;K. Vanderlinde&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vieira_J/0/1/0/all/0/1"&gt;J. D. Vieira&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vikhlinin_A/0/1/0/all/0/1"&gt;A. Vikhlinin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Williamson_R/0/1/0/all/0/1"&gt;R. Williamson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zahn_O/0/1/0/all/0/1"&gt;O. Zahn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zenteno_A/0/1/0/all/0/1"&gt;A. Zenteno&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-5988917482096213301?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/5988917482096213301/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=5988917482096213301' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5988917482096213301'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5988917482096213301'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12232011.html' title='tipa -- 12/23/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-8569112348217663753</id><published>2011-12-22T21:52:00.000-05:00</published><updated>2011-12-22T21:53:33.865-05:00</updated><title type='text'>tipa -- 12/22/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4843"&gt;Recollimation Boundary Layers in Relativistic Jets&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kohler_S/0/1/0/all/0/1"&gt;Susanna Kohler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Begelman_M/0/1/0/all/0/1"&gt;Mitchell C. Begelman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Beckwith_K/0/1/0/all/0/1"&gt;Kris Beckwith&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4849"&gt;New Constraints on Isospin-Violating Dark Matter&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kumar_J/0/1/0/all/0/1"&gt;Jason Kumar&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sanford_D/0/1/0/all/0/1"&gt;David Sanford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Strigari_L/0/1/0/all/0/1"&gt;Louis E. Strigari&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4940"&gt;The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Riemer__Sorensen_S/0/1/0/all/0/1"&gt;Signe Riemer--Sørensen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Blake_C/0/1/0/all/0/1"&gt;Chris Blake&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parkinson_D/0/1/0/all/0/1"&gt;David Parkinson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Davis_T/0/1/0/all/0/1"&gt;Tamara M. Davis&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brough_S/0/1/0/all/0/1"&gt;Sarah Brough&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Colless_M/0/1/0/all/0/1"&gt;Matthew Colless&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Contreras_C/0/1/0/all/0/1"&gt;Carlos Contreras&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Couch_W/0/1/0/all/0/1"&gt;Warrick Couch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Croom_S/0/1/0/all/0/1"&gt;Scott Croom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Croton_D/0/1/0/all/0/1"&gt;Darren Croton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Drinkwater_M/0/1/0/all/0/1"&gt;Michael J. Drinkwater&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Forster_K/0/1/0/all/0/1"&gt;Karl Forster&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gilbank_D/0/1/0/all/0/1"&gt;David Gilbank&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gladders_M/0/1/0/all/0/1"&gt;Mike Gladders&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Glazebrook_K/0/1/0/all/0/1"&gt;Karl Glazebrook&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jelliffe_B/0/1/0/all/0/1"&gt;Ben Jelliffe&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jurek_R/0/1/0/all/0/1"&gt;Russell J. Jurek&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_I/0/1/0/all/0/1"&gt;I-hui Li&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Madore_B/0/1/0/all/0/1"&gt;Barry Madore&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Martin_D/0/1/0/all/0/1"&gt;D. Christopher Martin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pimbblet_K/0/1/0/all/0/1"&gt;Kevin Pimbblet&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Poole_G/0/1/0/all/0/1"&gt;Gregory B. Poole&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pracy_M/0/1/0/all/0/1"&gt;Michael Pracy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sharp_R/0/1/0/all/0/1"&gt;Rob Sharp&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wisnioski_E/0/1/0/all/0/1"&gt;Emily Wisnioski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Woods_D/0/1/0/all/0/1"&gt;David Woods&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wyder_T/0/1/0/all/0/1"&gt;Ted K. Wyder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yee_H/0/1/0/all/0/1"&gt;H.K.C. Yee&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.5055"&gt;Beta-decay of nuclei around Se-90. Search for signatures of a N=56 sub-shell closure relevant the r-process&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Quinn_M/0/1/0/all/0/1"&gt;M. Quinn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Aprahamian_A/0/1/0/all/0/1"&gt;A. Aprahamian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Pereira_J/0/1/0/all/0/1"&gt;J. Pereira&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Surman_R/0/1/0/all/0/1"&gt;R. Surman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Arndt_O/0/1/0/all/0/1"&gt;O. Arndt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Baumann_T/0/1/0/all/0/1"&gt;T. Baumann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Becerril_A/0/1/0/all/0/1"&gt;A. Becerril&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Elliot_T/0/1/0/all/0/1"&gt;T. Elliot&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Estrade_A/0/1/0/all/0/1"&gt;A. Estrade&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Galaviz_D/0/1/0/all/0/1"&gt;D. Galaviz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Ginter_T/0/1/0/all/0/1"&gt;T. Ginter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Hausmann_M/0/1/0/all/0/1"&gt;M. Hausmann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Hennrich_S/0/1/0/all/0/1"&gt;S. Hennrich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Kessler_R/0/1/0/all/0/1"&gt;R. Kessler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Kratz_K/0/1/0/all/0/1"&gt;K.-L. Kratz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Lorusso_G/0/1/0/all/0/1"&gt;G. Lorusso&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Mantica_P/0/1/0/all/0/1"&gt;P. F. Mantica&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Matos_M/0/1/0/all/0/1"&gt;M. Matos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Moller_P/0/1/0/all/0/1"&gt;P. Moller&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Montes_F/0/1/0/all/0/1"&gt;F. Montes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Pfeiffer_B/0/1/0/all/0/1"&gt;B. Pfeiffer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Portillo_M/0/1/0/all/0/1"&gt;M. Portillo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Hennrich_S/0/1/0/all/0/1"&gt;S. Hennrich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Schatz_H/0/1/0/all/0/1"&gt;H. Schatz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Schertz_F/0/1/0/all/0/1"&gt;F. Schertz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Schnorrenberger_L/0/1/0/all/0/1"&gt;L. Schnorrenberger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Smith_E/0/1/0/all/0/1"&gt;E. Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Stolz_A/0/1/0/all/0/1"&gt;A. Stolz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Walters_W/0/1/0/all/0/1"&gt;W. B. Walters&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Wohr_A/0/1/0/all/0/1"&gt;A. Wohr&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-8569112348217663753?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/8569112348217663753/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=8569112348217663753' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8569112348217663753'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8569112348217663753'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12222011.html' title='tipa -- 12/22/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-4126323800501758089</id><published>2011-12-20T21:28:00.000-05:00</published><updated>2011-12-20T21:29:25.925-05:00</updated><title type='text'>tipa -- 12/21/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4479"&gt;Magnetic Fields in Population III Star Formation&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Turk_M/0/1/0/all/0/1"&gt;Matthew J. Turk&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Oishi_J/0/1/0/all/0/1"&gt;Jeffrey S. Oishi&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Abel_T/0/1/0/all/0/1"&gt;Tom Abel&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bryan_G/0/1/0/all/0/1"&gt;Greg Bryan&lt;/a&gt; (1) ((1) Columbia University, (2) Stanford University)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4518"&gt;VERITAS Observations of day-scale flaring of M87 in 2010 April&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_VERITAS/0/1/0/all/0/1"&gt;VERITAS Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4598"&gt;The Formation of Supermassive Black Holes from Low-Mass Pop III Seeds&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Whalen_D/0/1/0/all/0/1"&gt;Daniel J. Whalen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fryer_C/0/1/0/all/0/1"&gt;Chris L. Fryer&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4651"&gt;Impact of supernova dynamics on the νp-process&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Arcones_A/0/1/0/all/0/1"&gt;A. Arcones&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Frohlich_C/0/1/0/all/0/1"&gt;C. Fröhlich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Martinez_Pinedo_G/0/1/0/all/0/1"&gt;G. Martínez-Pinedo&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4799"&gt;High Energy Neutrinos from the Fermi Bubbles&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lunardini_C/0/1/0/all/0/1"&gt;Cecilia Lunardini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Razzaque_S/0/1/0/all/0/1"&gt;Soebur Razzaque&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4821"&gt;Self-consistent orbital evolution of a particle around a Schwarzschild black hole&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Diener_P/0/1/0/all/0/1"&gt;Peter Diener&lt;/a&gt;, &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Vega_I/0/1/0/all/0/1"&gt;Ian Vega&lt;/a&gt;, &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Wardell_B/0/1/0/all/0/1"&gt;Barry Wardell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Detweiler_S/0/1/0/all/0/1"&gt;Steven Detweiler&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4809"&gt;Neutral Pion Lifetime Measurements and the QCD Chiral Anomaly&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Bernstein_A/0/1/0/all/0/1"&gt;A. M. Bernstein&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Holstein_B/0/1/0/all/0/1"&gt;Barry R. Holstein&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4529"&gt;Evidence for 6ΛH&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Agnello_M/0/1/0/all/0/1"&gt;M. Agnello&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Benussi_L/0/1/0/all/0/1"&gt;L. Benussi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Bertani_M/0/1/0/all/0/1"&gt;M. Bertani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Bhang_H/0/1/0/all/0/1"&gt;H.C. Bhang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Bonomi_G/0/1/0/all/0/1"&gt;G. Bonomi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Botta_E/0/1/0/all/0/1"&gt;E. Botta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Bregant_M/0/1/0/all/0/1"&gt;M. Bregant&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Bressani_T/0/1/0/all/0/1"&gt;T. Bressani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Bufalino_S/0/1/0/all/0/1"&gt;S. Bufalino&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Busso_L/0/1/0/all/0/1"&gt;L. Busso&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Calvo_D/0/1/0/all/0/1"&gt;D. Calvo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Camerini_P/0/1/0/all/0/1"&gt;P. Camerini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Dalena_B/0/1/0/all/0/1"&gt;B. Dalena&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Mori_F/0/1/0/all/0/1"&gt;F. De Mori&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+DErasmo_G/0/1/0/all/0/1"&gt;G. D'Erasmo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Fabbri_F/0/1/0/all/0/1"&gt;F. L. Fabbri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Feliciello_A/0/1/0/all/0/1"&gt;A. Feliciello&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Filippi_A/0/1/0/all/0/1"&gt;A. Filippi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Fiore_E/0/1/0/all/0/1"&gt;E. M. Fiore&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Fontana_A/0/1/0/all/0/1"&gt;A. Fontana&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Fujioka_H/0/1/0/all/0/1"&gt;H. Fujioka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Genova_P/0/1/0/all/0/1"&gt;P. Genova&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Gianotti_P/0/1/0/all/0/1"&gt;P. Gianotti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Grion_N/0/1/0/all/0/1"&gt;N. Grion&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Lucherini_V/0/1/0/all/0/1"&gt;V. Lucherini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Marcello_S/0/1/0/all/0/1"&gt;S. Marcello&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Mirfakhrai_N/0/1/0/all/0/1"&gt;N. Mirfakhrai&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Moia_F/0/1/0/all/0/1"&gt;F. Moia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Morra_O/0/1/0/all/0/1"&gt;O. Morra&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Nagae_T/0/1/0/all/0/1"&gt;T. Nagae&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Outa_H/0/1/0/all/0/1"&gt;H. Outa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Pantaleo_A/0/1/0/all/0/1"&gt;A. Pantaleo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Paticchio_V/0/1/0/all/0/1"&gt;V. Paticchio&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Piano_S/0/1/0/all/0/1"&gt;S. Piano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Rui_R/0/1/0/all/0/1"&gt;R. Rui&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Simonetti_G/0/1/0/all/0/1"&gt;G. Simonetti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Wheadon_R/0/1/0/all/0/1"&gt;R. Wheadon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Zenoni_A/0/1/0/all/0/1"&gt;A. Zenoni&lt;/a&gt; (The FINUDA Collaboration), &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Gal_A/0/1/0/all/0/1"&gt;A. Gal&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4515"&gt;Unsolved problems in particle physics&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Troitsky_S/0/1/0/all/0/1"&gt;Sergey Troitsky&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-4126323800501758089?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/4126323800501758089/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=4126323800501758089' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4126323800501758089'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4126323800501758089'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12212011.html' title='tipa -- 12/21/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-3385184832757534721</id><published>2011-12-20T02:58:00.001-05:00</published><updated>2011-12-20T02:58:56.544-05:00</updated><title type='text'>tipa -- 12/20/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3959"&gt;The ongoing assembly of a central cluster galaxy: Phase-space substructures in the halo of M87&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Romanowsky_A/0/1/0/all/0/1"&gt;Aaron J. Romanowsky&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Strader_J/0/1/0/all/0/1"&gt;Jay Strader&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brodie_J/0/1/0/all/0/1"&gt;Jean P. Brodie&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mihos_J/0/1/0/all/0/1"&gt;J. Christopher Mihos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Spitler_L/0/1/0/all/0/1"&gt;Lee R. Spitler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Forbes_D/0/1/0/all/0/1"&gt;Duncan A. Forbes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Foster_C/0/1/0/all/0/1"&gt;Caroline Foster&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Arnold_J/0/1/0/all/0/1"&gt;Jacob A. Arnold&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3963"&gt;The Luminous Infrared Host Galaxy of Short-Duration GRB 100206A&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perley_D/0/1/0/all/0/1"&gt;Daniel A. Perley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Modjaz_M/0/1/0/all/0/1"&gt;M. Modjaz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Morgan_A/0/1/0/all/0/1"&gt;A. N. Morgan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cenko_S/0/1/0/all/0/1"&gt;S. B. Cenko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bloom_J/0/1/0/all/0/1"&gt;J. S. Bloom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Butler_N/0/1/0/all/0/1"&gt;N. R. Butler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Filippenko_A/0/1/0/all/0/1"&gt;A. V. Filippenko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Miller_A/0/1/0/all/0/1"&gt;A. A. Miller&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.4343"&gt;On the origin and composition of Galactic cosmic rays&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Prantzos_N/0/1/0/all/0/1"&gt;N. Prantzos&lt;/a&gt; (Institut d'Astrophysique de Paris, UMR7095 CNRS, and Université P. et M. Curie)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-3385184832757534721?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/3385184832757534721/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=3385184832757534721' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3385184832757534721'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3385184832757534721'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12202011.html' title='tipa -- 12/20/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-5376348394568603930</id><published>2011-12-20T02:57:00.000-05:00</published><updated>2011-12-20T02:58:06.076-05:00</updated><title type='text'>tipa -- 12/19/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3917"&gt;Detection of very high energy gamma-ray emission from NGC 1275 by the MAGIC telescopes&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_MAGIC/0/1/0/all/0/1"&gt;MAGIC Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3897"&gt;Inflationary magnetic fields spoil the homogeneity and isotropy of the Universe&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bonvin_C/0/1/0/all/0/1"&gt;Camille Bonvin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Caprini_C/0/1/0/all/0/1"&gt;Chiara Caprini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Durrer_R/0/1/0/all/0/1"&gt;Ruth Durrer&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-5376348394568603930?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/5376348394568603930/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=5376348394568603930' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5376348394568603930'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5376348394568603930'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12192011.html' title='tipa -- 12/19/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-2063598928409485219</id><published>2011-12-17T02:30:00.000-05:00</published><updated>2011-12-17T02:31:24.174-05:00</updated><title type='text'>tipa -- 12/16/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3342"&gt;The Hydrodynamic Origin of Neutron Star Kicks&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nordhaus_J/0/1/0/all/0/1"&gt;J. Nordhaus&lt;/a&gt; (RIT), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brandt_T/0/1/0/all/0/1"&gt;T. Brandt&lt;/a&gt; (Princeton), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Burrows_A/0/1/0/all/0/1"&gt;A. Burrows&lt;/a&gt; (Princeton), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Almgren_A/0/1/0/all/0/1"&gt;A. Almgren&lt;/a&gt; (LBNL)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3348"&gt;The Herschel Exploitation of Local Galaxy Andromeda (HELGA). I: Global far-infrared and sub-mm morphology&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fritz_J/0/1/0/all/0/1"&gt;J. Fritz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gentile_G/0/1/0/all/0/1"&gt;G. Gentile&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Smith_M/0/1/0/all/0/1"&gt;M. W. L. Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gear_W/0/1/0/all/0/1"&gt;W. K. Gear&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Duval_J/0/1/0/all/0/1"&gt;J. Roman Duval&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Baes_M/0/1/0/all/0/1"&gt;M. Baes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eales_S/0/1/0/all/0/1"&gt;S. A. Eales&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Verstappen_J/0/1/0/all/0/1"&gt;J. Verstappen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bendo_G/0/1/0/all/0/1"&gt;G. J. Bendo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Boquien_M/0/1/0/all/0/1"&gt;M. Boquien&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Boselli_A/0/1/0/all/0/1"&gt;A. Boselli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Braun_R/0/1/0/all/0/1"&gt;R. Braun&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Clements_D/0/1/0/all/0/1"&gt;D. Clements&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cooray_A/0/1/0/all/0/1"&gt;A. R. Cooray&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cortese_L/0/1/0/all/0/1"&gt;L. Cortese&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Looze_I/0/1/0/all/0/1"&gt;I. De Looze&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ford_G/0/1/0/all/0/1"&gt;G. Ford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Galliano_F/0/1/0/all/0/1"&gt;F. Galliano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gomez_H/0/1/0/all/0/1"&gt;H. L. Gomez&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gordon_K/0/1/0/all/0/1"&gt;K. D. Gordon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+OHalloran_B/0/1/0/all/0/1"&gt;B. O'Halloran&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kirk_J/0/1/0/all/0/1"&gt;J. Kirk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Madden_S/0/1/0/all/0/1"&gt;S. C. Madden&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Page_M/0/1/0/all/0/1"&gt;M. J. Page&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Remy_A/0/1/0/all/0/1"&gt;A. Remy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Roussel_H/0/1/0/all/0/1"&gt;H. Roussel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Spinoglio_L/0/1/0/all/0/1"&gt;L. Spinoglio&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Thilker_D/0/1/0/all/0/1"&gt;D. Thilker&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wilson_C/0/1/0/all/0/1"&gt;C. D. Wilson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vaccari_M/0/1/0/all/0/1"&gt;M. Vaccari&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Blommaert_J/0/1/0/all/0/1"&gt;J. A. D. L. Blommaert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Waelkens_C/0/1/0/all/0/1"&gt;C. Waelkens&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3595"&gt;On the Requirements for Realistic Modeling of Neutrino Transport in Simulations of Core-Collapse Supernovae&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lentz_E/0/1/0/all/0/1"&gt;Eric J. Lentz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mezzacappa_A/0/1/0/all/0/1"&gt;Anthony Mezzacappa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Messer_O/0/1/0/all/0/1"&gt;O. E. Bronson Messer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liebendorfer_M/0/1/0/all/0/1"&gt;Matthias Liebendörfer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hix_W/0/1/0/all/0/1"&gt;W. Raphael Hix&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bruenn_S/0/1/0/all/0/1"&gt;Stephen W. Bruenn&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3606"&gt;Precision muon decay measurements and improved constraints on the weak interaction&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Collaboration_TWIST/0/1/0/all/0/1"&gt;TWIST Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-2063598928409485219?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/2063598928409485219/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=2063598928409485219' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/2063598928409485219'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/2063598928409485219'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12162011.html' title='tipa -- 12/16/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-4216518773765246389</id><published>2011-12-15T01:58:00.001-05:00</published><updated>2011-12-15T01:58:53.740-05:00</updated><title type='text'>tipa -- 12/15/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3042"&gt;Polarimetry of the transient relativistic jet of GRB 110328 / Swift J164449.3+573451&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wiersema_K/0/1/0/all/0/1"&gt;K. Wiersema&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Horst_A/0/1/0/all/0/1"&gt;A. J. van der Horst&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Levan_A/0/1/0/all/0/1"&gt;A. J. Levan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tanvir_N/0/1/0/all/0/1"&gt;N. R. Tanvir&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Karjalainen_R/0/1/0/all/0/1"&gt;R. Karjalainen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kamble_A/0/1/0/all/0/1"&gt;A. Kamble&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kouveliotou_C/0/1/0/all/0/1"&gt;C. Kouveliotou&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Metzger_B/0/1/0/all/0/1"&gt;B. D. Metzger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Russell_D/0/1/0/all/0/1"&gt;D. M. Russell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Skillen_I/0/1/0/all/0/1"&gt;I. Skillen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Starling_R/0/1/0/all/0/1"&gt;R. L. C. Starling&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wijers_R/0/1/0/all/0/1"&gt;R. A. M. J. Wijers&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3114"&gt;Twinkling pulsar wind nebulae in the synchrotron cut-off regime and the gamma-ray flares in the Crab Nebula&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bykov_A/0/1/0/all/0/1"&gt;A. M. Bykov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pavlov_G/0/1/0/all/0/1"&gt;G. G. Pavlov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Artemyev_A/0/1/0/all/0/1"&gt;A. V. Artemyev&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Uvarov_Y/0/1/0/all/0/1"&gt;Yu. A. Uvarov&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3194"&gt;Time-Dependent Escape of Cosmic Rays from Supernova Remnants, and their Interaction with Dense Media&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Telezhinsky_I/0/1/0/all/0/1"&gt;I. Telezhinsky&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dwarkadas_V/0/1/0/all/0/1"&gt;V. V. Dwarkadas&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pohl_M/0/1/0/all/0/1"&gt;M. Pohl&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3264"&gt;A gas cloud on its way towards the super-massive black hole in the Galactic Centre&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gillessen_S/0/1/0/all/0/1"&gt;S. Gillessen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Genzel_R/0/1/0/all/0/1"&gt;R. Genzel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fritz_T/0/1/0/all/0/1"&gt;T. K. Fritz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Quataert_E/0/1/0/all/0/1"&gt;E. Quataert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Alig_C/0/1/0/all/0/1"&gt;C. Alig&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Burkert_A/0/1/0/all/0/1"&gt;A. Burkert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cuadra_J/0/1/0/all/0/1"&gt;J. Cuadra&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eisenhauer_F/0/1/0/all/0/1"&gt;F. Eisenhauer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pfuhl_O/0/1/0/all/0/1"&gt;O. Pfuhl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dodds_Eden_K/0/1/0/all/0/1"&gt;K. Dodds-Eden&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gammie_C/0/1/0/all/0/1"&gt;C. F. Gammie&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ott_T/0/1/0/all/0/1"&gt;T. Ott&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.3313"&gt;The 25Mg(p,g)Al reaction at low astrophysical energies&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Collaboration_LUNA/0/1/0/all/0/1"&gt;LUNA Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-4216518773765246389?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/4216518773765246389/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=4216518773765246389' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4216518773765246389'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4216518773765246389'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12152011.html' title='tipa -- 12/15/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-125610642321152553</id><published>2011-12-13T22:51:00.001-05:00</published><updated>2011-12-13T22:51:43.041-05:00</updated><title type='text'>tipa -- 12/14/2011</title><content type='html'>&lt;p class="MsoNormal"&gt;&lt;span class="faq-title"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://www.atlas.ch/news/2011/status-report-dec-2011.html"&gt;ATLAS experiment presents latest Higgs search status&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;p class="MsoNormal"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://cms.web.cern.ch/news/cms-search-standard-model-higgs-boson-lhc-data-2010-and-2011"&gt;CMS search for the Standard Model Higgs Boson in LHC data from 2010 and 2011&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2710"&gt;Pair-Instability Supernovae at the Epoch of Reionization&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pan_T/0/1/0/all/0/1"&gt;Tony Pan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kasen_D/0/1/0/all/0/1"&gt;Daniel Kasen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Loeb_A/0/1/0/all/0/1"&gt;Abraham Loeb&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2726"&gt;The Growth of the Stellar Seeds of Supermassive Black Holes&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Johnson_J/0/1/0/all/0/1"&gt;Jarrett L. Johnson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Whalen_D/0/1/0/all/0/1"&gt;Daniel J. Whalen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fryer_C/0/1/0/all/0/1"&gt;Christopher L. Fryer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_H/0/1/0/all/0/1"&gt;Hui Li&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2782"&gt;The Stochastic Gravitational Wave Background from the Single-Degenerate Channel of Type Ia Supernovae&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Falta_D/0/1/0/all/0/1"&gt;David Falta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fisher_R/0/1/0/all/0/1"&gt;Robert Fisher&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2770"&gt;The Impact of Recent Advances in Laboratory Astrophysics on our Understanding of the Cosmos&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Savin_D/0/1/0/all/0/1"&gt;D. W. Savin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brickhouse_N/0/1/0/all/0/1"&gt;N. S. Brickhouse&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cowan_J/0/1/0/all/0/1"&gt;J. J. Cowan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Drake_R/0/1/0/all/0/1"&gt;R. P. Drake&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Federman_S/0/1/0/all/0/1"&gt;S. R. Federman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ferland_G/0/1/0/all/0/1"&gt;G. J. Ferland&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Frank_A/0/1/0/all/0/1"&gt;A. Frank&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gudipati_M/0/1/0/all/0/1"&gt;M. S. Gudipati&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Haxton_W/0/1/0/all/0/1"&gt;W. C. Haxton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Herbst_E/0/1/0/all/0/1"&gt;E. Herbst&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Profumo_S/0/1/0/all/0/1"&gt;S. Profumo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Salama_F/0/1/0/all/0/1"&gt;F. Salama&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ziurys_L/0/1/0/all/0/1"&gt;L. M. Ziurys&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zweibe_E/0/1/0/all/0/1"&gt;E. G. Zweibe&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-125610642321152553?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/125610642321152553/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=125610642321152553' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/125610642321152553'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/125610642321152553'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12142011.html' title='tipa -- 12/14/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-7189565476673445012</id><published>2011-12-13T00:59:00.001-05:00</published><updated>2011-12-13T00:59:51.254-05:00</updated><title type='text'>tipa -- 12/13/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2210"&gt;Light echoes reveal an unexpectedly cool Eta Carinae during its 19th-century Great Eruption&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rest_A/0/1/0/all/0/1"&gt;A. Rest&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Prieto_J/0/1/0/all/0/1"&gt;J. L. Prieto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Walborn_N/0/1/0/all/0/1"&gt;N. R. Walborn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Smith_N/0/1/0/all/0/1"&gt;N. Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bianco_F/0/1/0/all/0/1"&gt;F. B. Bianco&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chornock_R/0/1/0/all/0/1"&gt;R. Chornock&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Welch_D/0/1/0/all/0/1"&gt;D. L. Welch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Howell_D/0/1/0/all/0/1"&gt;D. A. Howell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Huber_M/0/1/0/all/0/1"&gt;M. E. Huber&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Foley_R/0/1/0/all/0/1"&gt;R. J. Foley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fong_W/0/1/0/all/0/1"&gt;W. Fong&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sinnott_B/0/1/0/all/0/1"&gt;B. Sinnott&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bond_H/0/1/0/all/0/1"&gt;H. E. Bond&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Smith_R/0/1/0/all/0/1"&gt;R. C. Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Toledo_I/0/1/0/all/0/1"&gt;I. Toledo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Minniti_D/0/1/0/all/0/1"&gt;D. Minniti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mandel_K/0/1/0/all/0/1"&gt;K. Mandel&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2213"&gt;Evidence for inhomogeneous reionization in the local Universe from metal-poor globular cluster systems&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Spitler_L/0/1/0/all/0/1"&gt;Lee R. Spitler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Romanowsky_A/0/1/0/all/0/1"&gt;Aaron J. Romanowsky&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Diemand_J/0/1/0/all/0/1"&gt;Jürg Diemand&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Strader_J/0/1/0/all/0/1"&gt;Jay Strader&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Forbes_D/0/1/0/all/0/1"&gt;Duncan A. Forbes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Moore_B/0/1/0/all/0/1"&gt;Ben Moore&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brodie_J/0/1/0/all/0/1"&gt;Jean P. Brodie&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2534"&gt;Fermi/LAT observations of 1ES 0229+200: implications for extragalactic magnetic fields and background light&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vovk_I/0/1/0/all/0/1"&gt;Ievgen Vovk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taylor_A/0/1/0/all/0/1"&gt;Andrew M. Taylor&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Semikoz_D/0/1/0/all/0/1"&gt;Dmitri Semikoz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Neronov_A/0/1/0/all/0/1"&gt;Andrii Neronov&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2612"&gt;The Timing of Nine Globular Cluster Pulsars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lynch_R/0/1/0/all/0/1"&gt;Ryan S. Lynch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Freire_P/0/1/0/all/0/1"&gt;Paulo C. C. Freire&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ransom_S/0/1/0/all/0/1"&gt;Scott M. Ransom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jacoby_B/0/1/0/all/0/1"&gt;Bryan A. Jacoby&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2622"&gt;Intense Electromagnetic Outbursts from Collapsing Hypermassive Neutron Stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lehner_L/0/1/0/all/0/1"&gt;Luis Lehner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Palenzuela_C/0/1/0/all/0/1"&gt;Carlos Palenzuela&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liebling_S/0/1/0/all/0/1"&gt;Steven L. Liebling&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Thompson_C/0/1/0/all/0/1"&gt;Christopher Thompson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hanna_C/0/1/0/all/0/1"&gt;Chad Hanna&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2673"&gt;Nucleosynthesis of Nickel-56 from Gamma-Ray Burst Accretion Disks&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Surman_R/0/1/0/all/0/1"&gt;R. Surman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McLaughlin_G/0/1/0/all/0/1"&gt;G. C. McLaughlin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sabbatino_N/0/1/0/all/0/1"&gt;N. Sabbatino&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2683"&gt;An analysis of constraints on relativistic species from primordial nucleosynthesis and the cosmic microwave background&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nollett_K/0/1/0/all/0/1"&gt;Kenneth M. Nollett&lt;/a&gt; (Argonne), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holder_G/0/1/0/all/0/1"&gt;Gilbert P. Holder&lt;/a&gt; (McGill)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2577"&gt;Search for the Higgs boson in the H-&amp;gt;WW(*)-&amp;gt;lvlv decay channel in pp collisions at sqrt{s} = 7 TeV with the ATLAS detector&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Collaboration_ATLAS/0/1/0/all/0/1"&gt;ATLAS Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-7189565476673445012?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/7189565476673445012/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=7189565476673445012' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7189565476673445012'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7189565476673445012'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12132011.html' title='tipa -- 12/13/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-8086399546934498151</id><published>2011-12-11T22:31:00.000-05:00</published><updated>2011-12-11T22:32:00.453-05:00</updated><title type='text'>tipa -- 12/12/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1979"&gt;Gamma-ray Activity in the Crab Nebula: The Exceptional Flare of April 2011&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Buehler_R/0/1/0/all/0/1"&gt;R. Buehler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Scargle_J/0/1/0/all/0/1"&gt;J. D. Scargle&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Blandford_R/0/1/0/all/0/1"&gt;R. D. Blandford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Baldini_L/0/1/0/all/0/1"&gt;L. Baldini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Baring_M/0/1/0/all/0/1"&gt;M. G. Baring&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Belfiore_A/0/1/0/all/0/1"&gt;A. Belfiore&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Charles_E/0/1/0/all/0/1"&gt;E. Charles&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chiang_J/0/1/0/all/0/1"&gt;J. Chiang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+DAmmando_F/0/1/0/all/0/1"&gt;F. D'Ammando&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dermer_C/0/1/0/all/0/1"&gt;C. D. Dermer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Funk_S/0/1/0/all/0/1"&gt;S. Funk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Grove_J/0/1/0/all/0/1"&gt;J. E. Grove&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harding_A/0/1/0/all/0/1"&gt;A. K. Harding&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hays_E/0/1/0/all/0/1"&gt;E. Hays&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kerr_M/0/1/0/all/0/1"&gt;M. Kerr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Massaro_F/0/1/0/all/0/1"&gt;F. Massaro&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mazziotta_M/0/1/0/all/0/1"&gt;M. N. Mazziotta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Romani_R/0/1/0/all/0/1"&gt;R. W. Romani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parkinson_P/0/1/0/all/0/1"&gt;P. M. Saz Parkinson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tennant_A/0/1/0/all/0/1"&gt;A. F. Tennant&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Weisskopf_M/0/1/0/all/0/1"&gt;M. C. Weisskopf&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.2181"&gt;Corrections to the HARP-CDP Analysis of the LSND Neutrino Oscillation Backgrounds&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Garvey_G/0/1/0/all/0/1"&gt;G. T. Garvey&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Louis_W/0/1/0/all/0/1"&gt;W. C. Louis&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Mills_G/0/1/0/all/0/1"&gt;G. B. Mills&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+White_D/0/1/0/all/0/1"&gt;D. H. White&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-8086399546934498151?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/8086399546934498151/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=8086399546934498151' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8086399546934498151'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8086399546934498151'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-12122011.html' title='tipa -- 12/12/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-3318172005228736951</id><published>2011-12-09T22:23:00.001-05:00</published><updated>2011-12-09T22:23:51.265-05:00</updated><title type='text'>tipa -- 12/9/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1697"&gt;Radio Monitoring of the Tidal Disruption Event Swift J164449.3+573451. I. Jet Energetics and the Pristine Parsec-Scale Environment of a Supermassive Black Hole&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Berger_E/0/1/0/all/0/1"&gt;E. Berger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zauderer_A/0/1/0/all/0/1"&gt;A. Zauderer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pooley_G/0/1/0/all/0/1"&gt;G. G. Pooley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Soderberg_A/0/1/0/all/0/1"&gt;A. M. Soderberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sari_R/0/1/0/all/0/1"&gt;R. Sari&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brunthaler_A/0/1/0/all/0/1"&gt;A. Brunthaler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bietenholz_M/0/1/0/all/0/1"&gt;M. F. Bietenholz&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1840"&gt;Multi-year search for dark matter annihilations in the Sun with the AMANDA-II and IceCube detectors&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_IceCube/0/1/0/all/0/1"&gt;IceCube Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-3318172005228736951?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/3318172005228736951/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=3318172005228736951' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3318172005228736951'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3318172005228736951'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-1292011.html' title='tipa -- 12/9/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-5121456468966300090</id><published>2011-12-08T01:52:00.001-05:00</published><updated>2011-12-08T01:52:33.300-05:00</updated><title type='text'>tipa -- 12/8/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1419"&gt;The Cluster of Blue Stars Surrounding the M31 Nuclear Black Hole&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lauer_T/0/1/0/all/0/1"&gt;Tod R. Lauer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bender_R/0/1/0/all/0/1"&gt;Ralf Bender&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kormendy_J/0/1/0/all/0/1"&gt;John Kormendy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rosenfield_P/0/1/0/all/0/1"&gt;Philip Rosenfield&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Green_R/0/1/0/all/0/1"&gt;Richard F. Green&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1420"&gt;Remnants of Binary White Dwarf Mergers&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Raskin_C/0/1/0/all/0/1"&gt;Cody Raskin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Scannapieco_E/0/1/0/all/0/1"&gt;Evan Scannapieco&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fryer_C/0/1/0/all/0/1"&gt;Chris Fryer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rockefeller_G/0/1/0/all/0/1"&gt;Gabriel Rockefeller&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Timmes_F/0/1/0/all/0/1"&gt;F. X. Timmes&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1600"&gt;Search for the rare decays Bs -&amp;gt; mu+ mu- and B0 -&amp;gt; mu+ mu-&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Collaboration_LHCb/0/1/0/all/0/1"&gt;LHCb Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-5121456468966300090?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/5121456468966300090/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=5121456468966300090' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5121456468966300090'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5121456468966300090'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-1282011.html' title='tipa -- 12/8/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-3848688361138776450</id><published>2011-12-06T21:42:00.001-05:00</published><updated>2011-12-06T21:42:59.409-05:00</updated><title type='text'>tipa -- 12/7/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1067"&gt;The SPLASH Survey: Spectroscopy of 15 M31 Dwarf Spheroidal Satellite Galaxies&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tollerud_E/0/1/0/all/0/1"&gt;Erik J. Tollerud&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Beaton_R/0/1/0/all/0/1"&gt;Rachael L. Beaton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Geha_M/0/1/0/all/0/1"&gt;Marla C. Geha&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bullock_J/0/1/0/all/0/1"&gt;James S. Bullock&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guhathakurta_P/0/1/0/all/0/1"&gt;Puragra Guhathakurta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kalirai_J/0/1/0/all/0/1"&gt;Jason S. Kalirai&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Majewski_S/0/1/0/all/0/1"&gt;Steve R. Majewski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kirby_E/0/1/0/all/0/1"&gt;Evan N. Kirby&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gilbert_K/0/1/0/all/0/1"&gt;Karoline M. Gilbert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yniguez_B/0/1/0/all/0/1"&gt;Basilio Yniguez&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Patterson_R/0/1/0/all/0/1"&gt;Richard J. Patterson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ostheimer_J/0/1/0/all/0/1"&gt;James C. Ostheimer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Choudhury_A/0/1/0/all/0/1"&gt;Abrar Choudhury&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1078"&gt;Two ten-billion-solar-mass black holes at the centres of giant elliptical galaxies&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McConnell_N/0/1/0/all/0/1"&gt;Nicholas J. McConnell&lt;/a&gt; (UC Berkeley), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ma_C/0/1/0/all/0/1"&gt;Chung-Pei Ma&lt;/a&gt; (UC Berkeley), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gebhardt_K/0/1/0/all/0/1"&gt;Karl Gebhardt&lt;/a&gt; (UT Austin), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wright_S/0/1/0/all/0/1"&gt;Shelley A. Wright&lt;/a&gt; (UC Berkeley), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Murphy_J/0/1/0/all/0/1"&gt;Jeremy D. Murphy&lt;/a&gt; (UT Austin), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lauer_T/0/1/0/all/0/1"&gt;Tod R. Lauer&lt;/a&gt;, (NOAO), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Graham_J/0/1/0/all/0/1"&gt;James R. Graham&lt;/a&gt; (UC Berkeley and Dunlap Institute for Astronomy and Astrophysics), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Richstone_D/0/1/0/all/0/1"&gt;Douglas O. Richstone&lt;/a&gt; (UM Ann Arbor)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1140"&gt;Multimessenger Science Reach and Analysis Method for Common Sources of Gravitational Waves and High-energy Neutrinos&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Baret_B/0/1/0/all/0/1"&gt;Bruny Baret&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bartos_I/0/1/0/all/0/1"&gt;Imre Bartos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bouhou_B/0/1/0/all/0/1"&gt;Boutayeb Bouhou&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chassande_Mottin_E/0/1/0/all/0/1"&gt;Eric Chassande-Mottin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Corsi_A/0/1/0/all/0/1"&gt;Alessandra Corsi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Palma_I/0/1/0/all/0/1"&gt;Irene Di Palma&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Donzaud_C/0/1/0/all/0/1"&gt;Corinne Donzaud&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Drago_M/0/1/0/all/0/1"&gt;Marco Drago&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Finley_C/0/1/0/all/0/1"&gt;Chad Finley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jones_G/0/1/0/all/0/1"&gt;Gareth Jones&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Klimenko_S/0/1/0/all/0/1"&gt;Sergey Klimenko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kouchner_A/0/1/0/all/0/1"&gt;Antoine Kouchner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marka_S/0/1/0/all/0/1"&gt;Szabolcs Márka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marka_Z/0/1/0/all/0/1"&gt;Zsuzsa Márka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Moscoso_L/0/1/0/all/0/1"&gt;Luciano Moscoso&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Papa_M/0/1/0/all/0/1"&gt;Maria Alessandra Papa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pradier_T/0/1/0/all/0/1"&gt;Thierry Pradier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Prodi_G/0/1/0/all/0/1"&gt;Giovanni Prodi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Raffai_P/0/1/0/all/0/1"&gt;Peter Raffai&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Re_V/0/1/0/all/0/1"&gt;Virginia Re&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rollins_J/0/1/0/all/0/1"&gt;Jameson Rollins&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Salemi_F/0/1/0/all/0/1"&gt;Francesco Salemi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sutton_P/0/1/0/all/0/1"&gt;Patrick Sutton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tse_M/0/1/0/all/0/1"&gt;Maggie Tse&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Elewyck_V/0/1/0/all/0/1"&gt;Véronique Van Elewyck&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vedovato_G/0/1/0/all/0/1"&gt;Gabriele Vedovato&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-3848688361138776450?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/3848688361138776450/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=3848688361138776450' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3848688361138776450'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3848688361138776450'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-1272011.html' title='tipa -- 12/7/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-426825906311513792</id><published>2011-12-05T21:25:00.001-05:00</published><updated>2011-12-05T21:25:48.014-05:00</updated><title type='text'>tipa -- 12/6/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0938"&gt;Evidence for CP violation in time-integrated D0 -&amp;gt; h-h+ decay rates&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Collaboration_LHCb/0/1/0/all/0/1"&gt;LHCb Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0566"&gt;Surviving the hole I: Spatially resolved chemistry around Sgr A*&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Martin_S/0/1/0/all/0/1"&gt;S. Martín&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Martin_Pintado_J/0/1/0/all/0/1"&gt;J. Martín-Pintado&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Montero_Castano_M/0/1/0/all/0/1"&gt;M. Montero-Castaño&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ho_P/0/1/0/all/0/1"&gt;P. T. P. Ho&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Blundell_R/0/1/0/all/0/1"&gt;R. Blundell&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0567"&gt;Lensing of 21-cm Fluctuations by Primordial Gravitational Waves&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Book_L/0/1/0/all/0/1"&gt;Laura Book&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kamionkowski_M/0/1/0/all/0/1"&gt;Marc Kamionkowski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schmidt_F/0/1/0/all/0/1"&gt;Fabian Schmidt&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0568"&gt;General relativistic simulations of black hole-neutron star mergers: Effects of magnetic fields&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Etienne_Z/0/1/0/all/0/1"&gt;Zachariah B. Etienne&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Liu_Y/0/1/0/all/0/1"&gt;Yuk Tung Liu&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Paschalidis_V/0/1/0/all/0/1"&gt;Vasileios Paschalidis&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shapiro_S/0/1/0/all/0/1"&gt;Stuart L. Shapiro&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0569"&gt;Observational Evidence for a Correlation Between Jet Power and Black Hole Spin&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Narayan_R/0/1/0/all/0/1"&gt;Ramesh Narayan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McClintock_J/0/1/0/all/0/1"&gt;Jeffrey E. McClintock&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0593"&gt;The SN 393 -- SNR RX J1713.7-3946 (G347.3-0.5) Connection&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fesen_R/0/1/0/all/0/1"&gt;R. Fesen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kremer_R/0/1/0/all/0/1"&gt;R. Kremer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Patnaude_D/0/1/0/all/0/1"&gt;D. Patnaude&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Milisavljevic_D/0/1/0/all/0/1"&gt;D. Milisavljevic&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0777"&gt;Discovery of Two Supernovae in the Nuclear Regions of the Luminous Infrared Galaxy IC 883&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kankare_E/0/1/0/all/0/1"&gt;E. Kankare&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mattila_S/0/1/0/all/0/1"&gt;S. Mattila&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ryder_S/0/1/0/all/0/1"&gt;S. Ryder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vaisanen_P/0/1/0/all/0/1"&gt;P. Vaisanen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Alberdi_A/0/1/0/all/0/1"&gt;A. Alberdi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Alonso_Herrero_A/0/1/0/all/0/1"&gt;A. Alonso-Herrero&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Colina_L/0/1/0/all/0/1"&gt;L. Colina&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Efstathiou_A/0/1/0/all/0/1"&gt;A. Efstathiou&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kotilainen_J/0/1/0/all/0/1"&gt;J. Kotilainen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Melinder_J/0/1/0/all/0/1"&gt;J. Melinder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perez_Torres_M/0/1/0/all/0/1"&gt;M.-A. Perez-Torres&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Romero_Canizales_C/0/1/0/all/0/1"&gt;C. Romero-Canizales&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Takalo_A/0/1/0/all/0/1"&gt;A. Takalo&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0944"&gt;Predictions for mass-loss rates and terminal wind velocities of massive O-type stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Muijres_L/0/1/0/all/0/1"&gt;L. E. Muijres&lt;/a&gt; (Amsterdam), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vink_J/0/1/0/all/0/1"&gt;Jorick S. Vink&lt;/a&gt; (Armagh), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Koter_A/0/1/0/all/0/1"&gt;A. de Koter&lt;/a&gt; (Amsterdam), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mueller_P/0/1/0/all/0/1"&gt;P.E. Mueller&lt;/a&gt; (Keele), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Langer_N/0/1/0/all/0/1"&gt;N. Langer&lt;/a&gt; (Bonn)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.1026"&gt;Fission properties for r-process nuclei&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Erler_J/0/1/0/all/0/1"&gt;J. Erler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Langanke_K/0/1/0/all/0/1"&gt;K. Langanke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Loens_H/0/1/0/all/0/1"&gt;H.P. Loens&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Martinez_Pinedo_G/0/1/0/all/0/1"&gt;G. Martínez-Pinedo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Reinhard_P/0/1/0/all/0/1"&gt;P.-G. Reinhard&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-426825906311513792?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/426825906311513792/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=426825906311513792' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/426825906311513792'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/426825906311513792'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-1262011.html' title='tipa -- 12/6/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-1663317726137059523</id><published>2011-12-05T21:12:00.000-05:00</published><updated>2011-12-05T21:13:21.788-05:00</updated><title type='text'>tipa -- 12/5/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0335"&gt;Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Roberts_L/0/1/0/all/0/1"&gt;Luke F. Roberts&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shen_G/0/1/0/all/0/1"&gt;Gang Shen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cirigliano_V/0/1/0/all/0/1"&gt;Vincenzo Cirigliano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pons_J/0/1/0/all/0/1"&gt;Jose A. Pons&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reddy_S/0/1/0/all/0/1"&gt;Sanjay Reddy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Woosley_S/0/1/0/all/0/1"&gt;Stan E. Woosley&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0330"&gt;Nonlinear Evolution of Cosmological Structures in Warm Dark Matter Models&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schneider_A/0/1/0/all/0/1"&gt;Aurel Schneider&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Smith_R/0/1/0/all/0/1"&gt;Robert E. Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Maccio_A/0/1/0/all/0/1"&gt;Andrea V. Maccio&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Moore_B/0/1/0/all/0/1"&gt;Ben Moore&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0317"&gt;Identification of a Fundamental Transition in a Turbulently-Supported Interstellar Medium&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Scannapieco_E/0/1/0/all/0/1"&gt;Evan Scannapieco&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gray_W/0/1/0/all/0/1"&gt;William J. Gray&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pan_L/0/1/0/all/0/1"&gt;Liubin Pan&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-1663317726137059523?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/1663317726137059523/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=1663317726137059523' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/1663317726137059523'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/1663317726137059523'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-1252011.html' title='tipa -- 12/5/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-6763762673269391557</id><published>2011-12-01T22:23:00.000-05:00</published><updated>2011-12-01T22:24:08.150-05:00</updated><title type='text'>tipa -- 12/2/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0016"&gt;The Very Massive and Hot LMC Star VFTS 682: Progenitor of a Future Dark Gamma-Ray Burst?&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_D/0/1/0/all/0/1"&gt;Dong Zhang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stanek_K/0/1/0/all/0/1"&gt;K. Z. Stanek&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0018"&gt;A minor body falling onto a neutron star as an explanation for the unusual gamma-ray burst GRB 101225A&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Campana_S/0/1/0/all/0/1"&gt;S. Campana&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lodato_G/0/1/0/all/0/1"&gt;G. Lodato&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+DAvanzo_P/0/1/0/all/0/1"&gt;P. D'Avanzo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Panagia_N/0/1/0/all/0/1"&gt;N. Panagia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rossi_E/0/1/0/all/0/1"&gt;E. M. Rossi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Valle_M/0/1/0/all/0/1"&gt;M. Della Valle&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tagliaferri_G/0/1/0/all/0/1"&gt;G. Tagliaferri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Antonelli_L/0/1/0/all/0/1"&gt;L. A. Antonelli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Covino_S/0/1/0/all/0/1"&gt;S. Covino&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ghirlanda_G/0/1/0/all/0/1"&gt;G. Ghirlanda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ghisellini_G/0/1/0/all/0/1"&gt;G. Ghisellini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Melandri_A/0/1/0/all/0/1"&gt;A. Melandri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pian_E/0/1/0/all/0/1"&gt;E. Pian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Salvaterra_R/0/1/0/all/0/1"&gt;R. Salvaterra&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cusumano_G/0/1/0/all/0/1"&gt;G. Cusumano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+DElia_V/0/1/0/all/0/1"&gt;V. D'Elia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fugazza_D/0/1/0/all/0/1"&gt;D. Fugazza&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Palazzi_E/0/1/0/all/0/1"&gt;E. Palazzi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sbarufatti_B/0/1/0/all/0/1"&gt;B. Sbarufatti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vergani_S/0/1/0/all/0/1"&gt;S. D. Vergani&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0022"&gt;Relation of Astrophysical Turbulence and Magnetic Reconnection&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lazarian_A/0/1/0/all/0/1"&gt;A. Lazarian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eyink_G/0/1/0/all/0/1"&gt;G. Eyink&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vishniac_E/0/1/0/all/0/1"&gt;E. Vishniac&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0247"&gt;Multi-epoch high-resolution spectroscopy of SN2011fe - Linking the progenitor to its environment&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Patat_F/0/1/0/all/0/1"&gt;F. Patat&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cordiner_M/0/1/0/all/0/1"&gt;M. A. Cordiner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cox_N/0/1/0/all/0/1"&gt;N. L. J. Cox&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Anderson_R/0/1/0/all/0/1"&gt;R. I. Anderson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harutyunyan_A/0/1/0/all/0/1"&gt;A. Harutyunyan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kotak_R/0/1/0/all/0/1"&gt;R. Kotak&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Palaversa_L/0/1/0/all/0/1"&gt;L. Palaversa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stanishev_V/0/1/0/all/0/1"&gt;V. Stanishev&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tomasella_L/0/1/0/all/0/1"&gt;L. Tomasella&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Benetti_S/0/1/0/all/0/1"&gt;S. Benetti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Goobar_A/0/1/0/all/0/1"&gt;A. Goobar&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pastorello_A/0/1/0/all/0/1"&gt;A. Pastorello&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sollerman_J/0/1/0/all/0/1"&gt;J. Sollerman&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0299"&gt;It's Alive! The Supernova Impostor 1961V&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dyk_S/0/1/0/all/0/1"&gt;Schuyler D. Van Dyk&lt;/a&gt; (Spitzer Science Center/Caltech), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Matheson_T/0/1/0/all/0/1"&gt;Thomas Matheson&lt;/a&gt; (NOAO)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1112.0170"&gt;Allan Sandage and the Cosmic Expansion&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tammann_G/0/1/0/all/0/1"&gt;G. A. Tammann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reindl_B/0/1/0/all/0/1"&gt;B. Reindl&lt;/a&gt; (Department of Physics and Astronomy, Univ. of Basel)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-6763762673269391557?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/6763762673269391557/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=6763762673269391557' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6763762673269391557'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/6763762673269391557'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-1222011.html' title='tipa -- 12/2/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-9012280924566060278</id><published>2011-12-01T02:49:00.000-05:00</published><updated>2011-12-01T02:50:23.124-05:00</updated><title type='text'>tipa -- 12/1/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.7003"&gt;Yellow supergiants as supernova progenitors: an indication of strong mass loss for red supergiants?&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Georgy_C/0/1/0/all/0/1"&gt;Cyril Georgy&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.7026"&gt;Fermi Detection of γ-ray emission from the M2 Soft X-ray Flare on 2010 June 12&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Fermi_GBM/0/1/0/all/0/1"&gt;Fermi GBM Collaboration&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Fermi_LAT/0/1/0/all/0/1"&gt;Fermi LAT Collaboration&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dennis_B/0/1/0/all/0/1"&gt;B. R. Dennis&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schwartz_R/0/1/0/all/0/1"&gt;R. A. Schwartz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tolbert_A/0/1/0/all/0/1"&gt;A. K. Tolbert&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.7030"&gt;Searching for soft relativistic jets in Core-collapse Supernovae with the IceCube Optical Follow-up Program&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_IceCube/0/1/0/all/0/1"&gt;IceCube Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.7122"&gt;The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger Observatory&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Pierre_Auger/0/1/0/all/0/1"&gt;Pierre Auger Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.7316"&gt;A Chandra X-ray Survey of Ejecta in the Cassiopeia A Supernova Remnant&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hwang_U/0/1/0/all/0/1"&gt;Una Hwang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Laming_J/0/1/0/all/0/1"&gt;J. Martin Laming&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.7314"&gt;Search for Gravitational Waves from Low Mass Compact Binary Coalescence in LIGO's Sixth Science Run and Virgo's Science Runs 2 and 3&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Colaboration_L/0/1/0/all/0/1"&gt;LIGO Scientific Colaboration&lt;/a&gt;, &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Collaboration_Virgo/0/1/0/all/0/1"&gt;Virgo Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-9012280924566060278?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/9012280924566060278/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=9012280924566060278' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/9012280924566060278'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/9012280924566060278'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/12/tipa-1212011.html' title='tipa -- 12/1/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-8635680731201693060</id><published>2011-11-29T22:34:00.001-05:00</published><updated>2011-11-29T22:34:57.745-05:00</updated><title type='text'>tipa -- 11/30/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6593"&gt;Type Ia supernovae in globular clusters: observational upper limits&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Voss_R/0/1/0/all/0/1"&gt;R. Voss&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nelemans_G/0/1/0/all/0/1"&gt;G. Nelemans&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6626"&gt;Multi-epoch Spectropolarimetry of SN 2011fe&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Smith_P/0/1/0/all/0/1"&gt;Paul S. Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Williams_G/0/1/0/all/0/1"&gt;G. Grant Williams&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Smith_N/0/1/0/all/0/1"&gt;Nathan Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Milne_P/0/1/0/all/0/1"&gt;Peter A. Milne&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jannuzi_B/0/1/0/all/0/1"&gt;Buell T. Jannuzi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Green_E/0/1/0/all/0/1"&gt;E. M. Green&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6667"&gt;Simulations of GRB Jets in a Stratified External Medium: Dynamics, Afterglow Lightcurves, Jet Breaks and Radio Calorimetry&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Colle_F/0/1/0/all/0/1"&gt;Fabio De Colle&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ramirez_Ruiz_E/0/1/0/all/0/1"&gt;Enrico Ramirez-Ruiz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Granot_J/0/1/0/all/0/1"&gt;Jonathan Granot&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lopez_Camara_D/0/1/0/all/0/1"&gt;Diego Lopez-Camara&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6675"&gt;Spectrum of cosmic-ray nucleons and the atmospheric muon charge ratio&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gaisser_T/0/1/0/all/0/1"&gt;Thomas K. Gaisser&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6867"&gt;Acoustic Signatures of the Helium Core Flash&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bildsten_L/0/1/0/all/0/1"&gt;Lars Bildsten&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Paxton_B/0/1/0/all/0/1"&gt;Bill Paxton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Moore_K/0/1/0/all/0/1"&gt;Kevin Moore&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Macias_P/0/1/0/all/0/1"&gt;Phillip J. Macias&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6936"&gt;Investigating the Cosmic-Ray Ionization Rate in the Galactic Diffuse Interstellar Medium through Observations of H3+&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Indriolo_N/0/1/0/all/0/1"&gt;Nick Indriolo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McCall_B/0/1/0/all/0/1"&gt;Benjamin J. McCall&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-8635680731201693060?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/8635680731201693060/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=8635680731201693060' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8635680731201693060'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/8635680731201693060'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11302011.html' title='tipa -- 11/30/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-3742143734451649196</id><published>2011-11-28T21:22:00.001-05:00</published><updated>2011-11-28T21:22:34.363-05:00</updated><title type='text'>tipa -- 11/29/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6109"&gt;Calcium-rich gap transients in the remote outskirts of galaxies&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kasliwal_M/0/1/0/all/0/1"&gt;Mansi M. Kasliwal&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kulkarni_S/0/1/0/all/0/1"&gt;S. R. Kulkarni&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gal_Yam_A/0/1/0/all/0/1"&gt;Avishay Gal-Yam&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nugent_P/0/1/0/all/0/1"&gt;Peter E. Nugent&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sullivan_M/0/1/0/all/0/1"&gt;Mark Sullivan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bildsten_L/0/1/0/all/0/1"&gt;Lars Bildsten&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yaron_O/0/1/0/all/0/1"&gt;Ofer Yaron&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perets_H/0/1/0/all/0/1"&gt;Hagai B. Perets&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Arcavi_I/0/1/0/all/0/1"&gt;Iair Arcavi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ben_Ami_S/0/1/0/all/0/1"&gt;Sagi Ben-Ami&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bhalerao_V/0/1/0/all/0/1"&gt;Varun B. Bhalerao&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bloom_J/0/1/0/all/0/1"&gt;Joshua S. Bloom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cenko_S/0/1/0/all/0/1"&gt;S. Bradley Cenko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Filippenko_A/0/1/0/all/0/1"&gt;Alexei V. Filippenko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Frail_D/0/1/0/all/0/1"&gt;Dale A. Frail&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ganeshalingam_M/0/1/0/all/0/1"&gt;Mohan Ganeshalingam&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Horesh_A/0/1/0/all/0/1"&gt;Assaf Horesh&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Howell_D/0/1/0/all/0/1"&gt;D. Andrew Howell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Law_N/0/1/0/all/0/1"&gt;Nicholas M. Law&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Leonard_D/0/1/0/all/0/1"&gt;Douglas C. Leonard&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_W/0/1/0/all/0/1"&gt;Weidong Li&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ofek_E/0/1/0/all/0/1"&gt;Eran O. Ofek&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Polishook_D/0/1/0/all/0/1"&gt;David Polishook&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Poznanski_D/0/1/0/all/0/1"&gt;Dovi Poznanski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Quimby_R/0/1/0/all/0/1"&gt;Robert M. Quimby&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Silverman_J/0/1/0/all/0/1"&gt;Jeffrey M. Silverman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sternberg_A/0/1/0/all/0/1"&gt;Assaf Sternberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Xu_D/0/1/0/all/0/1"&gt;Dong Xu&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6186"&gt;An improved map of the Galactic Faraday sky&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Oppermann_N/0/1/0/all/0/1"&gt;N. Oppermann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Junklewitz_H/0/1/0/all/0/1"&gt;H. Junklewitz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Robbers_G/0/1/0/all/0/1"&gt;G. Robbers&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bell_M/0/1/0/all/0/1"&gt;M. R. Bell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ensslin_T/0/1/0/all/0/1"&gt;T. A. Enßlin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bonafede_A/0/1/0/all/0/1"&gt;A. Bonafede&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Braun_R/0/1/0/all/0/1"&gt;R. Braun&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brown_J/0/1/0/all/0/1"&gt;J. C. Brown&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Clarke_T/0/1/0/all/0/1"&gt;T. E. Clarke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Feain_I/0/1/0/all/0/1"&gt;I. J. Feain&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gaensler_B/0/1/0/all/0/1"&gt;B. M. Gaensler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hammond_A/0/1/0/all/0/1"&gt;A. Hammond&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harvey_Smith_L/0/1/0/all/0/1"&gt;L. Harvey-Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Heald_G/0/1/0/all/0/1"&gt;G. Heald&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Johston_Hollitt_M/0/1/0/all/0/1"&gt;M. Johston-Hollitt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Klein_U/0/1/0/all/0/1"&gt;U. Klein&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kronberg_P/0/1/0/all/0/1"&gt;P. P. Kronberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mao_S/0/1/0/all/0/1"&gt;S. A. Mao&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McClure_Griffiths_N/0/1/0/all/0/1"&gt;N. M. McClure-Griffiths&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+OSullivan_S/0/1/0/all/0/1"&gt;S. P. O'Sullivan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pratley_L/0/1/0/all/0/1"&gt;L. Pratley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Robishaw_T/0/1/0/all/0/1"&gt;T. Robishaw&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Roy_S/0/1/0/all/0/1"&gt;S. Roy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schnitzeler_D/0/1/0/all/0/1"&gt;D. H. F. M. Schnitzeler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sotomayor_Beltran_C/0/1/0/all/0/1"&gt;C. Sotomayor-Beltran&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stevens_J/0/1/0/all/0/1"&gt;J. Stevens&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stil_J/0/1/0/all/0/1"&gt;J. M. Stil&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sunstrum_C/0/1/0/all/0/1"&gt;C. Sunstrum&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tanna_A/0/1/0/all/0/1"&gt;A. Tanna&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taylor_A/0/1/0/all/0/1"&gt;A. R. Taylor&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eck_C/0/1/0/all/0/1"&gt;C. L. Van Eck&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6361"&gt;Ring-like features in directional dark matter detection&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bozorgnia_N/0/1/0/all/0/1"&gt;Nassim Bozorgnia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gelmini_G/0/1/0/all/0/1"&gt;Graciela B. Gelmini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gondolo_P/0/1/0/all/0/1"&gt;Paolo Gondolo&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6386"&gt;Cosmic microwave background constraints on the duration and timing of reionization from the South Pole Telescope&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zahn_O/0/1/0/all/0/1"&gt;O. Zahn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reichardt_C/0/1/0/all/0/1"&gt;C. L. Reichardt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shaw_L/0/1/0/all/0/1"&gt;L. Shaw&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lidz_A/0/1/0/all/0/1"&gt;A. Lidz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Aird_K/0/1/0/all/0/1"&gt;K. A. Aird&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Benson_B/0/1/0/all/0/1"&gt;B. A. Benson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bleem_L/0/1/0/all/0/1"&gt;L. E. Bleem&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Carlstrom_J/0/1/0/all/0/1"&gt;J. E. Carlstrom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chang_C/0/1/0/all/0/1"&gt;C. L. Chang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cho_H/0/1/0/all/0/1"&gt;H. M. Cho&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Crawford_T/0/1/0/all/0/1"&gt;T. M. Crawford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Crites_A/0/1/0/all/0/1"&gt;A. T. Crites&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Haan_T/0/1/0/all/0/1"&gt;T. de Haan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dobbs_M/0/1/0/all/0/1"&gt;M. A. Dobbs&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dore_O/0/1/0/all/0/1"&gt;O. Dore&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dudley_J/0/1/0/all/0/1"&gt;J. Dudley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+George_E/0/1/0/all/0/1"&gt;E. M. George&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Halverson_N/0/1/0/all/0/1"&gt;N. W. Halverson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holder_G/0/1/0/all/0/1"&gt;G. P. Holder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holzapfel_W/0/1/0/all/0/1"&gt;W. L. Holzapfel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hoover_S/0/1/0/all/0/1"&gt;S. Hoover&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hou_Z/0/1/0/all/0/1"&gt;Z. Hou&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hrubes_J/0/1/0/all/0/1"&gt;J. D. Hrubes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Joy_M/0/1/0/all/0/1"&gt;M. Joy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Keisler_R/0/1/0/all/0/1"&gt;R. Keisler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Knox_L/0/1/0/all/0/1"&gt;L. Knox&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lee_A/0/1/0/all/0/1"&gt;A. T. Lee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Leitch_E/0/1/0/all/0/1"&gt;E. M. Leitch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lueker_M/0/1/0/all/0/1"&gt;M. Lueker&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Luong_Van_D/0/1/0/all/0/1"&gt;D. Luong-Van&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McMahon_J/0/1/0/all/0/1"&gt;J. J. McMahon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mehl_J/0/1/0/all/0/1"&gt;J. Mehl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meyer_S/0/1/0/all/0/1"&gt;S. S. Meyer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Millea_M/0/1/0/all/0/1"&gt;M. Millea&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mohr_J/0/1/0/all/0/1"&gt;J. J. Mohr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Montroy_T/0/1/0/all/0/1"&gt;T. E. Montroy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Natoli_T/0/1/0/all/0/1"&gt;T. Natoli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Padin_S/0/1/0/all/0/1"&gt;S. Padin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Plagge_T/0/1/0/all/0/1"&gt;T. Plagge&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pryke_C/0/1/0/all/0/1"&gt;C. Pryke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ruhl_J/0/1/0/all/0/1"&gt;J. E. Ruhl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schaffer_K/0/1/0/all/0/1"&gt;K. K. Schaffer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shirokoff_E/0/1/0/all/0/1"&gt;E. Shirokoff&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Spieler_H/0/1/0/all/0/1"&gt;H. G. Spieler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Staniszewski_Z/0/1/0/all/0/1"&gt;Z. Staniszewski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stark_A/0/1/0/all/0/1"&gt;A. A. Stark&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Story_K/0/1/0/all/0/1"&gt;K. Story&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Engelen_A/0/1/0/all/0/1"&gt;A. van Engelen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vanderlinde_K/0/1/0/all/0/1"&gt;K. Vanderlinde&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vieira_J/0/1/0/all/0/1"&gt;J. D. Vieira&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Williamson_R/0/1/0/all/0/1"&gt;R. Williamson&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6398"&gt;Very High Angular Resolution Science with the Square Kilometre Array&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Godfrey_L/0/1/0/all/0/1"&gt;L. E. H. Godfrey&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bignall_H/0/1/0/all/0/1"&gt;H. Bignall&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tingay_S/0/1/0/all/0/1"&gt;S. Tingay&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harvey_Smith_L/0/1/0/all/0/1"&gt;L. Harvey-Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kramer_M/0/1/0/all/0/1"&gt;M. Kramer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Burke_Spolaor_S/0/1/0/all/0/1"&gt;S. Burke-Spolaor&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Miller_Jones_J/0/1/0/all/0/1"&gt;J. C. A. Miller-Jones&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Johnston_Hollitt_M/0/1/0/all/0/1"&gt;M. Johnston-Hollitt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ekers_R/0/1/0/all/0/1"&gt;R. Ekers&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gulyaev_S/0/1/0/all/0/1"&gt;S. Gulyaev&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6572"&gt;Detection of the gamma-ray binary LS I +61 303 in a low flux state at Very High Energy gamma-rays with the MAGIC Telescopes in 2009&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_MAGIC/0/1/0/all/0/1"&gt;MAGIC Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-3742143734451649196?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/3742143734451649196/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=3742143734451649196' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3742143734451649196'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3742143734451649196'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11292011.html' title='tipa -- 11/29/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-9221667444074802337</id><published>2011-11-28T20:09:00.000-05:00</published><updated>2011-11-28T20:10:07.655-05:00</updated><title type='text'>tipa -- 11/28/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5795"&gt;A New Time-Dependent Finite Difference Method for Relativistic Shock Acceleration&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Delaney_S/0/1/0/all/0/1"&gt;Sean Delaney&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dempsey_P/0/1/0/all/0/1"&gt;Paul Dempsey&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Duffy_P/0/1/0/all/0/1"&gt;Peter Duffy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Downes_T/0/1/0/all/0/1"&gt;Turlough P. Downes&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5806"&gt;In pursuit of gamma-ray burst progenitors: the identification of a sub-population of rotating Wolf-Rayet stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vink_J/0/1/0/all/0/1"&gt;Jorick S. Vink&lt;/a&gt; (Armagh Observatory), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Graefener_G/0/1/0/all/0/1"&gt;G. Graefener&lt;/a&gt; (Armagh Observatory), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harries_T/0/1/0/all/0/1"&gt;T.J. Harries&lt;/a&gt; (Exeter)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5870"&gt;PSR J1841-0500: a radio pulsar that mostly is not there&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Camilo_F/0/1/0/all/0/1"&gt;F. Camilo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ransom_S/0/1/0/all/0/1"&gt;S. M. Ransom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chatterjee_S/0/1/0/all/0/1"&gt;S. Chatterjee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Johnston_S/0/1/0/all/0/1"&gt;S. Johnston&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Demorest_P/0/1/0/all/0/1"&gt;P. Demorest&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6058"&gt;Soft nuclear equation-of-state from heavy-ion data and implications for compact stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sagert_I/0/1/0/all/0/1"&gt;Irina Sagert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tolos_L/0/1/0/all/0/1"&gt;Laura Tolos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chatterjee_D/0/1/0/all/0/1"&gt;Debarati Chatterjee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schaffner_Bielich_J/0/1/0/all/0/1"&gt;Juergen Schaffner-Bielich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sturm_C/0/1/0/all/0/1"&gt;Christian Sturm&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.6099"&gt;Geo-neutrinos as indicators of the origin and thermal history of the Earth&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/nucl-ex/1/au:+Dye_S/0/1/0/all/0/1"&gt;Steve Dye&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5646"&gt;Allan R. Sandage, 18 June 1926 - 13 November 2010&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/physics/1/au:+Lynden_Bell_D/0/1/0/all/0/1"&gt;Donald Lynden-Bell&lt;/a&gt; (IoA, Cambridge), &lt;a href="http://arxiv.org/find/physics/1/au:+Schweizer_F/0/1/0/all/0/1"&gt;Francois Schweizer&lt;/a&gt; (OCIS, Pasadena)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-9221667444074802337?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/9221667444074802337/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=9221667444074802337' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/9221667444074802337'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/9221667444074802337'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11282011.html' title='tipa -- 11/28/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-5918975367583099643</id><published>2011-11-23T22:25:00.000-05:00</published><updated>2011-11-23T22:26:02.698-05:00</updated><title type='text'>tipa -- 11/24/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5329"&gt;Basic Properties of MHD Turbulence in the Inertial Range&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Beresnyak_A/0/1/0/all/0/1"&gt;Andrey Beresnyak&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5341"&gt;The 2010 very high energy gamma-ray flare &amp;amp; 10 years of multi-wavelength observations of M 87&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_H._E._S._S./0/1/0/all/0/1"&gt;H.E.S.S. Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5343"&gt;An Experiment to Locate the Site of TeV Flaring in M87&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harris_D/0/1/0/all/0/1"&gt;D. E. Harris&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Massaro_F/0/1/0/all/0/1"&gt;F. Massaro&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cheung_C/0/1/0/all/0/1"&gt;C. C. Cheung&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Horns_D/0/1/0/all/0/1"&gt;D. Horns&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Raue_M/0/1/0/all/0/1"&gt;M. Raue&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stawarz_L/0/1/0/all/0/1"&gt;L. Stawarz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wagner_S/0/1/0/all/0/1"&gt;S. Wagner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Colin_P/0/1/0/all/0/1"&gt;P. Colin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mazin_D/0/1/0/all/0/1"&gt;D. Mazin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wagner_R/0/1/0/all/0/1"&gt;R. Wagner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Beilicke_M/0/1/0/all/0/1"&gt;M. Beilicke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+LeBohec_S/0/1/0/all/0/1"&gt;S. LeBohec&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hui_M/0/1/0/all/0/1"&gt;M. Hui&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mukherjee_R/0/1/0/all/0/1"&gt;R. Mukherjee&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5424"&gt;Photon Trapping Enables Super-Eddington Growth of Black-Hole Seeds in Galaxies at High Redshift&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wyithe_S/0/1/0/all/0/1"&gt;Stuart Wyithe&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Loeb_A/0/1/0/all/0/1"&gt;Abraham Loeb&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5544"&gt;Constraining Cosmic Rays and Magnetic Fields in the Perseus Galaxy Cluster with TeV observations by the MAGIC telescopes&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_MAGIC/0/1/0/all/0/1"&gt;MAGIC Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5331"&gt;Probing Nonstandard Standard Model Backgrounds with LHC Monojets&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Friedland_A/0/1/0/all/0/1"&gt;Alexander Friedland&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Graesser_M/0/1/0/all/0/1"&gt;Michael L. Graesser&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Shoemaker_I/0/1/0/all/0/1"&gt;Ian M. Shoemaker&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Vecchi_L/0/1/0/all/0/1"&gt;Luca Vecchi&lt;/a&gt; (Los Alamos)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5332"&gt;Leptonic CP violation&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Branco_G/0/1/0/all/0/1"&gt;G. C. Branco&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Felipe_R/0/1/0/all/0/1"&gt;R. Gonzalez Felipe&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Joaquim_F/0/1/0/all/0/1"&gt;F. R. Joaquim&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5338"&gt;The 1953 Cosmic Ray Conference at Bagneres de Bigorre&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/physics/1/au:+Cronin_J/0/1/0/all/0/1"&gt;James W. Cronin&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-5918975367583099643?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/5918975367583099643/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=5918975367583099643' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5918975367583099643'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5918975367583099643'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11242011.html' title='tipa -- 11/24/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-3400418978979272852</id><published>2011-11-22T22:05:00.001-05:00</published><updated>2011-11-22T22:05:43.351-05:00</updated><title type='text'>tipa -- 11/23/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5031"&gt;Supernova Relic Neutrino Search at Super-Kamiokande&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Collaboration_Super_Kamiokande/0/1/0/all/0/1"&gt;Super-Kamiokande Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5237"&gt;Generalized Semi-Analytical Models of Supernova Light Curves&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chatzopoulos_E/0/1/0/all/0/1"&gt;Emmanouil Chatzopoulos&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wheeler_J/0/1/0/all/0/1"&gt;J. Craig Wheeler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vinko_J/0/1/0/all/0/1"&gt;Jozsef Vinko&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5211"&gt;First Double-Chooz Results and the Reactor Antineutrino Anomaly&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Giunti_C/0/1/0/all/0/1"&gt;Carlo Giunti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Laveder_M/0/1/0/all/0/1"&gt;Marco Laveder&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.5242"&gt;An additional study of multi-muon events produced in {\boldmath $p\bar{p}$} collisions at {\boldmath $\sqrt{s}=1.96$} TeV&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Aaltonen_T/0/1/0/all/0/1"&gt;T. Aaltonen&lt;/a&gt;, et al (CDF Collaboration)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-3400418978979272852?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/3400418978979272852/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=3400418978979272852' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3400418978979272852'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3400418978979272852'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11232011.html' title='tipa -- 11/23/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-2686878746708407113</id><published>2011-11-21T22:21:00.001-05:00</published><updated>2011-11-21T22:22:35.189-05:00</updated><title type='text'>tipa -- 11/22/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4483"&gt;Probing the neutrino mass hierarchy with the rise time of a supernova burst&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chakraborty_S/0/1/0/all/0/1"&gt;Sovan Chakraborty&lt;/a&gt; (II Inst. Theor. Phys., Hamburg University), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fischer_T/0/1/0/all/0/1"&gt;Tobias Fischer&lt;/a&gt; (GSI &amp;amp; Tech. Univ. Darmstadt), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hudepohl_L/0/1/0/all/0/1"&gt;Lorenz Hudepohl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Janka_H/0/1/0/all/0/1"&gt;Hans-Thomas Janka&lt;/a&gt; (MPA, Garching), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mirizzi_A/0/1/0/all/0/1"&gt;Alessandro Mirizzi&lt;/a&gt; (II Inst. Theor. Phys., Hamburg University), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Serpico_P/0/1/0/all/0/1"&gt;Pasquale Dario Serpico&lt;/a&gt; (LAPTh, Annecy)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4505"&gt;Contemporaneous VLBA 5 GHz Observations of LAT-Detected Blazars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Linford_J/0/1/0/all/0/1"&gt;Justin D. Linford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taylor_G/0/1/0/all/0/1"&gt;Gregory B. Taylor&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Romani_R/0/1/0/all/0/1"&gt;Roger W. Romani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Helmboldt_J/0/1/0/all/0/1"&gt;Joseph F. Helmboldt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Readhead_A/0/1/0/all/0/1"&gt;Anthony C.S. Readhead&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reeves_R/0/1/0/all/0/1"&gt;Rodrigo Reeves&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Richards_J/0/1/0/all/0/1"&gt;Joseph L. Richards&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4527"&gt;The Fast and Faint SN 2010bh Associated with GRB 100316D&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bufano_F/0/1/0/all/0/1"&gt;Filomena Bufano&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pian_E/0/1/0/all/0/1"&gt;Elena Pian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sollerman_J/0/1/0/all/0/1"&gt;Jesper Sollerman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Benetti_S/0/1/0/all/0/1"&gt;Stefano Benetti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pignata_G/0/1/0/all/0/1"&gt;Giuliano Pignata&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Valenti_S/0/1/0/all/0/1"&gt;Stefano Valenti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Covino_S/0/1/0/all/0/1"&gt;Stefano Covino&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+DAvanzo_P/0/1/0/all/0/1"&gt;Paolo D'Avanzo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Malesani_D/0/1/0/all/0/1"&gt;Daniele Malesani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cappellaro_E/0/1/0/all/0/1"&gt;Enrico Cappellaro&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Valle_M/0/1/0/all/0/1"&gt;Massimo Della Valle&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fynbo_J/0/1/0/all/0/1"&gt;Johan Fynbo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hjorth_J/0/1/0/all/0/1"&gt;Jens Hjorth&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mazzali_P/0/1/0/all/0/1"&gt;Paolo A. Mazzali&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reichart_D/0/1/0/all/0/1"&gt;Daniel E. Reichart&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Starling_R/0/1/0/all/0/1"&gt;Rhaana L. C. Starling&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Turatto_M/0/1/0/all/0/1"&gt;Massimo Turatto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vergani_S/0/1/0/all/0/1"&gt;Susanna D. Vergani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wiersema_K/0/1/0/all/0/1"&gt;Klass Wiersema&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Amati_L/0/1/0/all/0/1"&gt;Lorenzo Amati&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bersier_D/0/1/0/all/0/1"&gt;David Bersier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Campana_S/0/1/0/all/0/1"&gt;Sergio Campana&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cano_Z/0/1/0/all/0/1"&gt;Zach Cano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Castro_Tirado_A/0/1/0/all/0/1"&gt;Alberto J. Castro-Tirado&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chincarini_G/0/1/0/all/0/1"&gt;Guido Chincarini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+DElia_V/0/1/0/all/0/1"&gt;Valerio D'Elia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Postigo_A/0/1/0/all/0/1"&gt;Antonio de Ugarte Postigo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Deng_J/0/1/0/all/0/1"&gt;Jinsong Deng&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ferrero_P/0/1/0/all/0/1"&gt;Patrizia Ferrero&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Filippenko_A/0/1/0/all/0/1"&gt;Alexei V. Filippenko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Goldoni_P/0/1/0/all/0/1"&gt;Paolo Goldoni&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gorosabel_J/0/1/0/all/0/1"&gt;Javier Gorosabel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Greiner_J/0/1/0/all/0/1"&gt;Jochen Greiner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hammer_F/0/1/0/all/0/1"&gt;Francois Hammer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jakobsson_P/0/1/0/all/0/1"&gt;Pall Jakobsson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kaper_L/0/1/0/all/0/1"&gt;Lex Kaper&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kawabata_K/0/1/0/all/0/1"&gt;Koji S. Kawabata&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Klose_S/0/1/0/all/0/1"&gt;Sylvio Klose&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Levan_A/0/1/0/all/0/1"&gt;Andrew J. Levan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Maeda_K/0/1/0/all/0/1"&gt;Keiichi Maeda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Masetti_N/0/1/0/all/0/1"&gt;Nicola Masetti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Milvang_Jensen_B/0/1/0/all/0/1"&gt;Bo Milvang-Jensen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mirabel_F/0/1/0/all/0/1"&gt;Felix I. Mirabel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Moller_P/0/1/0/all/0/1"&gt;Palle Moller&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nomoto_K/0/1/0/all/0/1"&gt;Kenichi Nomoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Palazzi_E/0/1/0/all/0/1"&gt;Eliana Palazzi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Piranomonte_S/0/1/0/all/0/1"&gt;Silvia Piranomonte&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Salvaterra_R/0/1/0/all/0/1"&gt;Ruben Salvaterra&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stratta_G/0/1/0/all/0/1"&gt;Giulia Stratta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tagliaferri_G/0/1/0/all/0/1"&gt;Gianpiero Tagliaferri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tanaka_M/0/1/0/all/0/1"&gt;Masaomi Tanaka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wijers_R/0/1/0/all/0/1"&gt;Ralph A.M.J. Wijers&lt;/a&gt; ((1) INAF-Osservatorio Astronomico di Catania)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4577"&gt;Voids as Alternatives to Dark Energy and the Propagation of Gamma Rays through the Universe&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lavallaz_A/0/1/0/all/0/1"&gt;Arnaud De Lavallaz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fairbairn_M/0/1/0/all/0/1"&gt;Malcolm Fairbairn&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4867"&gt;Extended clustering analyses to constrain the deflection angular scale and source density of the ultra-high-energy cosmic rays&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Decerprit_G/0/1/0/all/0/1"&gt;Guillaume Decerprit&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Busca_N/0/1/0/all/0/1"&gt;Nicolas G. Busca&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parizot_E/0/1/0/all/0/1"&gt;Etienne Parizot&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4868"&gt;Neutral pion emission from accelerated protons in the supernova remnant W44&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Giuliani_A/0/1/0/all/0/1"&gt;A. Giuliani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cardillo_M/0/1/0/all/0/1"&gt;M. Cardillo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tavani_M/0/1/0/all/0/1"&gt;M. Tavani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fukui_Y/0/1/0/all/0/1"&gt;Y. Fukui&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yoshiike_S/0/1/0/all/0/1"&gt;S. Yoshiike&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Torii_K/0/1/0/all/0/1"&gt;K. Torii&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dubner_G/0/1/0/all/0/1"&gt;G. Dubner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Castelletti_G/0/1/0/all/0/1"&gt;G. Castelletti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Barbiellini_G/0/1/0/all/0/1"&gt;G. Barbiellini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bulgarelli_A/0/1/0/all/0/1"&gt;A. Bulgarelli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Caraveo_P/0/1/0/all/0/1"&gt;P. Caraveo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Costa_E/0/1/0/all/0/1"&gt;E. Costa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cattaneo_P/0/1/0/all/0/1"&gt;P. W. Cattaneo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chen_A/0/1/0/all/0/1"&gt;A. Chen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Contessi_T/0/1/0/all/0/1"&gt;T. Contessi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Monte_E/0/1/0/all/0/1"&gt;E. Del Monte&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Donnarumma_I/0/1/0/all/0/1"&gt;I. Donnarumma&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Evangelista_Y/0/1/0/all/0/1"&gt;Y. Evangelista&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Feroci_M/0/1/0/all/0/1"&gt;M. Feroci&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gianotti_F/0/1/0/all/0/1"&gt;F. Gianotti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lazzarotto_F/0/1/0/all/0/1"&gt;F. Lazzarotto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lucarelli_F/0/1/0/all/0/1"&gt;F. Lucarelli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Longo_F/0/1/0/all/0/1"&gt;F. Longo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marisaldi_M/0/1/0/all/0/1"&gt;M. Marisaldi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mereghetti_S/0/1/0/all/0/1"&gt;S. Mereghetti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pacciani_L/0/1/0/all/0/1"&gt;L. Pacciani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pellizzoni_A/0/1/0/all/0/1"&gt;A. Pellizzoni&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Piano_G/0/1/0/all/0/1"&gt;G. Piano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Picozza_P/0/1/0/all/0/1"&gt;P. Picozza&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pittori_C/0/1/0/all/0/1"&gt;C. Pittori&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pucella_G/0/1/0/all/0/1"&gt;G. Pucella&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rapisarda_M/0/1/0/all/0/1"&gt;M. Rapisarda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rappoldi_A/0/1/0/all/0/1"&gt;A. Rappoldi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sabatini_S/0/1/0/all/0/1"&gt;S. Sabatini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Soffitta_P/0/1/0/all/0/1"&gt;P. Soffitta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Striani_E/0/1/0/all/0/1"&gt;E. Striani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Trifoglio_M/0/1/0/all/0/1"&gt;M. Trifoglio&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Trois_A/0/1/0/all/0/1"&gt;A. Trois&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vercellone_S/0/1/0/all/0/1"&gt;S. Vercellone&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Verrecchia_F/0/1/0/all/0/1"&gt;F. Verrecchia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vittorini_V/0/1/0/all/0/1"&gt;V. Vittorini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Colafrancesco_S/0/1/0/all/0/1"&gt;S. Colafrancesco&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Giommi_P/0/1/0/all/0/1"&gt;P. Giommi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bignami_G/0/1/0/all/0/1"&gt;G. Bignami&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4878"&gt;The non-thermal emission of extended radio galaxy lobes with curved electron spectra&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Duffy_P/0/1/0/all/0/1"&gt;Peter Duffy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Blundell_K/0/1/0/all/0/1"&gt;Katherine M. Blundell&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4492"&gt;Type-Ia supernova rates and the progenitor problem, a review&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Maoz_D/0/1/0/all/0/1"&gt;Dan Maoz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mannucci_F/0/1/0/all/0/1"&gt;Filippo Mannucci&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4923"&gt;Nuclear correlations and the r-process&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Arcones_A/0/1/0/all/0/1"&gt;A. Arcones&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Bertsch_G/0/1/0/all/0/1"&gt;G. F. Bertsch&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-2686878746708407113?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/2686878746708407113/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=2686878746708407113' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/2686878746708407113'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/2686878746708407113'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11222011.html' title='tipa -- 11/22/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-9008160010229352483</id><published>2011-11-21T22:16:00.001-05:00</published><updated>2011-11-21T22:16:53.615-05:00</updated><title type='text'>tipa -- 11/21/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4215"&gt;Evidence for dark matter contraction and a Salpeter IMF in a massive early-type galaxy&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sonnenfeld_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Alessandro Sonnenfeld&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Treu_T/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Tommaso Treu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gavazzi_R/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Raphael Gavazzi&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marshall_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Philip J. Marshall&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Auger_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Mattew W. Auger&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Suyu_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Sherry H. Suyu&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Koopmans_L/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Leon V. E. Koopmans&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bolton_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Adam S. Bolton&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1111.4216"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Multiwavelength Constraints on Pulsar Populations in the Galactic Center&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wharton_R/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;R. S. Wharton&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chatterjee_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. Chatterjee&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cordes_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;J. M. Cordes&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Deneva_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;J. S. Deneva&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lazio_T/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;T. J. W. Lazio&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1111.4217"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Constraining Sterile Neutrino Warm Dark Matter with Chandra Observations of the Andromeda Galaxy&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Watson_C/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Casey R. Watson&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; (Millikin U.), &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_Z/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Zhiyuan Li&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; (CfA), &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Polley_N/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Nicholas K. Polley&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; (Millikin U.)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1111.4258"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;The peak energy of dissipative GRB photospheres&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Giannios_D/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Dimitrios Giannios&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; (Princeton)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1111.4270"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;PSR J2030+3641: radio discovery and gamma-ray study of a middle-aged pulsar in the now identified Fermi-LAT source 1FGL J2030.0+3641&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Camilo_F/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;F. Camilo&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kerr_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M. Kerr&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ray_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P.S. Ray&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ransom_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S.M. Ransom&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Johnston_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;S. Johnston&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Romani_R/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;R.W. Romani&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parent_D/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;D. Parent&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+DeCesar_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M.E. DeCesar&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harding_A/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;A.K. Harding&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Donato_D/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;D. Donato&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parkinson_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P.M. Saz Parkinson&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ferrara_E/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;E.C. Ferrara&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Freire_P/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;P.C.C. Freire&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guillemot_L/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;L. Guillemot&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Keith_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M. Keith&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kramer_M/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;M. Kramer&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wood_K/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;K.S. Wood&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;a href="http://arxiv.org/abs/1111.4222"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;Statistical Tests of Noise and Harmony in Dark Matter Modulation Signals&lt;/span&gt;&lt;/b&gt;&lt;/a&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;/span&gt;&lt;a href="http://arxiv.org/find/hep-ph/1/au:+Chang_S/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Spencer Chang&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/hep-ph/1/au:+Pradler_J/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Josef Pradler&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;, &lt;/span&gt;&lt;a href="http://arxiv.org/find/hep-ph/1/au:+Yavin_I/0/1/0/all/0/1"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Itay Yavin&lt;/span&gt;&lt;/a&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-9008160010229352483?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/9008160010229352483/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=9008160010229352483' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/9008160010229352483'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/9008160010229352483'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11212011.html' title='tipa -- 11/21/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-509728241551595217</id><published>2011-11-17T23:48:00.000-05:00</published><updated>2011-11-17T23:49:01.162-05:00</updated><title type='text'>tipa -- 11/18/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3964"&gt;Constraining Sources of Ultra High Energy Cosmic Rays Using High Energy Observations with the Fermi Satellite&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Peer_A/0/1/0/all/0/1"&gt;Asaf Pe'er&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Loeb_A/0/1/0/all/0/1"&gt;Abraham Loeb&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3980"&gt;The Large, Oxygen-Rich Halos of Star-Forming Galaxies Are A Major Reservoir of Galactic Metals&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tumlinson_J/0/1/0/all/0/1"&gt;Jason Tumlinson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Thom_C/0/1/0/all/0/1"&gt;Christopher Thom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Werk_J/0/1/0/all/0/1"&gt;Jessica K. Werk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Prochaska_J/0/1/0/all/0/1"&gt;J. Xavier Prochaska&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tripp_T/0/1/0/all/0/1"&gt;Todd M. Tripp&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Weinberg_D/0/1/0/all/0/1"&gt;David H. Weinberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Peeples_M/0/1/0/all/0/1"&gt;Molly S. Peeples&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+OMeara_J/0/1/0/all/0/1"&gt;John M. O'Meara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Oppenheimer_B/0/1/0/all/0/1"&gt;Benjamin D. Oppenheimer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meiring_J/0/1/0/all/0/1"&gt;Joseph D. Meiring&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Katz_N/0/1/0/all/0/1"&gt;Neal S. Katz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dave_R/0/1/0/all/0/1"&gt;Romeel Dave&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ford_A/0/1/0/all/0/1"&gt;Amanda Brady Ford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sembach_K/0/1/0/all/0/1"&gt;Kenneth R. Sembach&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3981"&gt;A Reservoir of Ionized Gas in the Galactic Halo to Sustain Star Formation in the Milky Way&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lehner_N/0/1/0/all/0/1"&gt;Nicolas Lehner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Howk_J/0/1/0/all/0/1"&gt;J. Christopher Howk&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3982"&gt;The Hidden Mass and Large Spatial Extent of a Poststarburst Galaxy Outflow&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tripp_T/0/1/0/all/0/1"&gt;Todd M. Tripp&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meiring_J/0/1/0/all/0/1"&gt;Joseph D. Meiring&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Prochaska_J/0/1/0/all/0/1"&gt;J. Xavier Prochaska&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Willmer_C/0/1/0/all/0/1"&gt;Christopher N. A. Willmer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Howk_J/0/1/0/all/0/1"&gt;J. Christopher Howk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Werk_J/0/1/0/all/0/1"&gt;Jessica K. Werk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jenkins_E/0/1/0/all/0/1"&gt;Edward B. Jenkins&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bowen_D/0/1/0/all/0/1"&gt;David V. Bowen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lehner_N/0/1/0/all/0/1"&gt;Nicolas Lehner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sembach_K/0/1/0/all/0/1"&gt;Kenneth R. Sembach&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Thom_C/0/1/0/all/0/1"&gt;Christopher Thom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tumlinson_J/0/1/0/all/0/1"&gt;Jason Tumlinson&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3985"&gt;The r-Process in Metal Poor Stars and Black Hole Formation&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Boyd_R/0/1/0/all/0/1"&gt;Richard Boyd&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Famiano_M/0/1/0/all/0/1"&gt;Michael Famiano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meyer_B/0/1/0/all/0/1"&gt;Bradley Meyer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Motizuki_Y/0/1/0/all/0/1"&gt;Yuko Motizuki&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kajino_T/0/1/0/all/0/1"&gt;Toshitaka Kajino&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Roederer_I/0/1/0/all/0/1"&gt;Ian Roederer&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.4175"&gt;Gamma Rays from the Tycho Supernova Remnant: Leptonic or Hadronic?&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Atoyan_A/0/1/0/all/0/1"&gt;Armen Atoyan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dermer_C/0/1/0/all/0/1"&gt;Charles Dermer&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-509728241551595217?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/509728241551595217/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=509728241551595217' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/509728241551595217'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/509728241551595217'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11182011.html' title='tipa -- 11/18/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-730385993902116841</id><published>2011-11-16T20:58:00.000-05:00</published><updated>2011-11-16T20:59:24.336-05:00</updated><title type='text'>tipa -- 11/17/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3644"&gt;The Origin of OB Runaway Stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fujii_M/0/1/0/all/0/1"&gt;Michiko Fujii&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zwart_S/0/1/0/all/0/1"&gt;Simon Portegies Zwart&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3648"&gt;Pair-Instability Supernovae via Collision Runaway in Young Dense Star Clusters&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pan_T/0/1/0/all/0/1"&gt;Tony Pan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Loeb_A/0/1/0/all/0/1"&gt;Abraham Loeb&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kasen_D/0/1/0/all/0/1"&gt;Daniel Kasen&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3649"&gt;Protostellar Feedback Halts the Growth of the First Stars in the Universe&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hosokawa_T/0/1/0/all/0/1"&gt;Takashi Hosokawa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Omukai_K/0/1/0/all/0/1"&gt;Kazuyuki Omukai&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yoshida_N/0/1/0/all/0/1"&gt;Naoki Yoshida&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yorke_H/0/1/0/all/0/1"&gt;Harold W. Yorke&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3693"&gt;Was The Sun Born In A Massive Cluster?&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dukes_D/0/1/0/all/0/1"&gt;Donald Dukes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Krumholz_M/0/1/0/all/0/1"&gt;Mark R. Krumholz&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3754"&gt;Fermi Detection of a Luminous Gamma-ray Pulsar in a Globular Cluster&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Fermi_LAT/0/1/0/all/0/1"&gt;Fermi LAT Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3937"&gt;Strangelet dwarfs&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Alford_M/0/1/0/all/0/1"&gt;Mark G. Alford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Han_S/0/1/0/all/0/1"&gt;Sophia Han&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Reddy_S/0/1/0/all/0/1"&gt;Sanjay Reddy&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3713"&gt;A Search for Single Photon Events in Neutrino Interactions&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Kullenberg_C/0/1/0/all/0/1"&gt;C. T. Kullenberg&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ex/1/au:+Mishra_S/0/1/0/all/0/1"&gt;S. R. Mishra&lt;/a&gt; (NOMAD Collaboration)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-730385993902116841?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/730385993902116841/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=730385993902116841' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/730385993902116841'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/730385993902116841'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11172011.html' title='tipa -- 11/17/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-7179591210632802201</id><published>2011-11-15T23:45:00.000-05:00</published><updated>2011-11-15T23:46:19.374-05:00</updated><title type='text'>tipa -- 11/16/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3377"&gt;New Electrodynamics of Pulsars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gruzinov_A/0/1/0/all/0/1"&gt;Andrei Gruzinov&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3433"&gt;First HARPSpol discoveries of magnetic fields in massive stars&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Alecian_E/0/1/0/all/0/1"&gt;E. Alecian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kochukhov_O/0/1/0/all/0/1"&gt;O. Kochukhov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Neiner_C/0/1/0/all/0/1"&gt;C. Neiner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wade_G/0/1/0/all/0/1"&gt;G. A. Wade&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Batz_B/0/1/0/all/0/1"&gt;B. de Batz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Henrichs_H/0/1/0/all/0/1"&gt;H. Henrichs&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Grunhut_J/0/1/0/all/0/1"&gt;J. H. Grunhut&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bouret_J/0/1/0/all/0/1"&gt;J.-C. Bouret&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Briquet_M/0/1/0/all/0/1"&gt;M. Briquet&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gagne_M/0/1/0/all/0/1"&gt;M. Gagne&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Naze_Y/0/1/0/all/0/1"&gt;Y. Naze&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Oksala_M/0/1/0/all/0/1"&gt;M. E. Oksala&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rivinius_T/0/1/0/all/0/1"&gt;T. Rivinius&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Townsend_R/0/1/0/all/0/1"&gt;R .H. D. Townsend&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Walborn_N/0/1/0/all/0/1"&gt;N. R. Walborn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Weiss_W/0/1/0/all/0/1"&gt;W. Weiss&lt;/a&gt;, the &lt;a href="http://arxiv.org/find/astro-ph/1/au:+collaboration_MiMeS/0/1/0/all/0/1"&gt;MiMeS collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3544"&gt;Properties of Interstellar Turbulence from Gradients of Linear Radio Polarization Maps&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Burkhart_B/0/1/0/all/0/1"&gt;Blakesley Burkhart&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lazarian_A/0/1/0/all/0/1"&gt;A. Lazarian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gaensler_B/0/1/0/all/0/1"&gt;B. M. Gaensler&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-7179591210632802201?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/7179591210632802201/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=7179591210632802201' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7179591210632802201'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7179591210632802201'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11162011.html' title='tipa -- 11/16/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-3972886388054842556</id><published>2011-11-14T22:41:00.000-05:00</published><updated>2011-11-14T22:42:33.585-05:00</updated><title type='text'>tipa -- 11/15/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2863"&gt;An Excursion-Set Model for the Structure of GMCs and the ISM&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hopkins_P/0/1/0/all/0/1"&gt;Philip F. Hopkins&lt;/a&gt; (Berkeley)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2877"&gt;The X-ray Counterpart of the High-B Pulsar PSR J0726-2612&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Speagle_J/0/1/0/all/0/1"&gt;J. S. Speagle&lt;/a&gt; (1,2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kaplan_D/0/1/0/all/0/1"&gt;D. L. Kaplan&lt;/a&gt; (1,3), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kerkwijk_M/0/1/0/all/0/1"&gt;M. H. van Kerkwijk&lt;/a&gt; (4) ((1) University of Wisconsin-Milwaukee, (2) Harvard College, (3) corresponding author, (4) University of Toronto)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2922"&gt;Unusual Central Engine Activity in the Double Burst GRB 110709B&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_B/0/1/0/all/0/1"&gt;Bin-Bin Zhang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Burrows_D/0/1/0/all/0/1"&gt;David N. Burrows&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_B/0/1/0/all/0/1"&gt;Bing Zhang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meszaros_P/0/1/0/all/0/1"&gt;Peter Meszaros&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stratta_G/0/1/0/all/0/1"&gt;Giulia Stratta&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+DElia_V/0/1/0/all/0/1"&gt;Valerio D'Elia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Frederiks_D/0/1/0/all/0/1"&gt;Dmitry Frederiks&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Golenetskii_S/0/1/0/all/0/1"&gt;S. Golenetskii&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cummings_J/0/1/0/all/0/1"&gt;Jay R. Cummings&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wang_X/0/1/0/all/0/1"&gt;Xiang-Yu Wang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Falcone_A/0/1/0/all/0/1"&gt;Abraham D. Falcone&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Barthelmy_S/0/1/0/all/0/1"&gt;Scott D. Barthelmy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gehrels_N/0/1/0/all/0/1"&gt;Neil Gehrels&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3055"&gt;Eccentric black hole-neutron star mergers: effects of black hole spin and equation of state&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+East_W/0/1/0/all/0/1"&gt;William E. East&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pretorius_F/0/1/0/all/0/1"&gt;Frans Pretorius&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stephens_B/0/1/0/all/0/1"&gt;Branson C. Stephens&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3074"&gt;The Orbit and Companion of Probable gamma-ray Pulsar J2339-0533&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Romani_R/0/1/0/all/0/1"&gt;Roger W. Romani&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shaw_M/0/1/0/all/0/1"&gt;Michael S. Shaw&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3075"&gt;Anisotropy of TeV Cosmic Rays and the Outer Heliospheric Boundaries&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Desiati_P/0/1/0/all/0/1"&gt;P. Desiati&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lazarian_A/0/1/0/all/0/1"&gt;A. Lazarian&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3086"&gt;High-Resolution Simulations of Convection Preceding Ignition in Type Ia Supernovae Using Adaptive Mesh Refinement&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nonaka_A/0/1/0/all/0/1"&gt;A. Nonaka&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Aspden_A/0/1/0/all/0/1"&gt;A. J. Aspden&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zingale_M/0/1/0/all/0/1"&gt;M. Zingale&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Almgren_A/0/1/0/all/0/1"&gt;A. S. Almgren&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bell_J/0/1/0/all/0/1"&gt;J. B. Bell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Woosley_S/0/1/0/all/0/1"&gt;S. E. Woosley&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3331"&gt;Simultaneous multi-wavelength campaign on PKS 2005-489 in a high state&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_H._E._S._S./0/1/0/all/0/1"&gt;H.E.S.S. Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3355"&gt;Gamma-ray burst afterglow scaling relations for the full blast wave evolution&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eerten_H/0/1/0/all/0/1"&gt;H. J. van Eerten&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+MacFadyen_A/0/1/0/all/0/1"&gt;A. I. MacFadyen&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.3045"&gt;Olber's Paradox for Superluminal Neutrinos: Constraining ExtremeNeutrino Speeds at TeV-ZeV Energies with the Diffuse Neutrino Background&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Lacki_B/0/1/0/all/0/1"&gt;Brian C. Lacki&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-3972886388054842556?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/3972886388054842556/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=3972886388054842556' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3972886388054842556'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3972886388054842556'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11152011.html' title='tipa -- 11/15/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-220508400005717657</id><published>2011-11-14T22:35:00.000-05:00</published><updated>2011-11-14T22:36:10.858-05:00</updated><title type='text'>tipa -- 11/14/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2611"&gt;The Cosmic Abundance of Classical Milky Way Satellites&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Strigari_L/0/1/0/all/0/1"&gt;Louis E. Strigari&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wechsler_R/0/1/0/all/0/1"&gt;Risa H. Wechsler&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2745"&gt;The alignment of molecular cloud magnetic fields with the spiral arms in M33&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_H/0/1/0/all/0/1"&gt;Hua-bai Li&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Henning_T/0/1/0/all/0/1"&gt;Thomas Henning&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2784"&gt;A Stable, Accurate Methodology for High Mach Number, Strong Magnetic Field MHD Turbulence with Adaptive Mesh Refinement: Resolution and Refinement Studies&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Li_P/0/1/0/all/0/1"&gt;Pak Shing Li&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Martin_D/0/1/0/all/0/1"&gt;Daniel F. Martin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Klein_R/0/1/0/all/0/1"&gt;Richard I. Klein&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McKee_C/0/1/0/all/0/1"&gt;Christopher F. McKee&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2827"&gt;What Shapes the Structure of Molecular Clouds: Turbulence or Gravity?&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kritsuk_A/0/1/0/all/0/1"&gt;Alexei G. Kritsuk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Norman_M/0/1/0/all/0/1"&gt;Michael L. Norman&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2835"&gt;Lower Limits on the Strengths of Gamma Ray Lines from WIMP Dark Matter Annihilation&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Abazajian_K/0/1/0/all/0/1"&gt;Kevork N. Abazajian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Agrawal_P/0/1/0/all/0/1"&gt;Prateek Agrawal&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Chacko_Z/0/1/0/all/0/1"&gt;Zackaria Chacko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Kilic_C/0/1/0/all/0/1"&gt;Can Kilic&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-220508400005717657?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/220508400005717657/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=220508400005717657' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/220508400005717657'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/220508400005717657'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11142011.html' title='tipa -- 11/14/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-1286542041049841674</id><published>2011-11-10T22:49:00.001-05:00</published><updated>2011-11-10T22:49:56.652-05:00</updated><title type='text'>tipa -- 11/11/11</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2334"&gt;Detection of Pristine Gas Two Billion Years after the Big Bang&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fumagalli_M/0/1/0/all/0/1"&gt;Michele Fumagalli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+OMeara_J/0/1/0/all/0/1"&gt;John M. O'Meara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Prochaska_J/0/1/0/all/0/1"&gt;J. Xavier Prochaska&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2410"&gt;Cosmic Ray streaming from SNRs and gamma ray emission from nearby molecular clouds&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yan_H/0/1/0/all/0/1"&gt;Huirong Yan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lazarian_A/0/1/0/all/0/1"&gt;A. Lazarian&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schlickeiser_R/0/1/0/all/0/1"&gt;R. Schlickeiser&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2472"&gt;Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; The &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Pierre_Auger/0/1/0/all/0/1"&gt;Pierre Auger Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2497"&gt;SN 2009E: a faint clone of SN 1987A&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pastorello_A/0/1/0/all/0/1"&gt;A. Pastorello&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pumo_M/0/1/0/all/0/1"&gt;M. L. Pumo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Navasardyan_H/0/1/0/all/0/1"&gt;H. Navasardyan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zampieri_L/0/1/0/all/0/1"&gt;L. Zampieri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Turatto_M/0/1/0/all/0/1"&gt;M. Turatto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sollerman_J/0/1/0/all/0/1"&gt;J. Sollerman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taddia_F/0/1/0/all/0/1"&gt;F. Taddia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kankare_E/0/1/0/all/0/1"&gt;E. Kankare&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mattila_S/0/1/0/all/0/1"&gt;S. Mattila&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nicolas_J/0/1/0/all/0/1"&gt;J. Nicolas&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Prosperi_E/0/1/0/all/0/1"&gt;E. Prosperi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Delgado_A/0/1/0/all/0/1"&gt;A. San Segundo Delgado&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taubenberger_S/0/1/0/all/0/1"&gt;S. Taubenberger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Boles_T/0/1/0/all/0/1"&gt;T. Boles&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bachini_M/0/1/0/all/0/1"&gt;M. Bachini&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Benetti_S/0/1/0/all/0/1"&gt;S. Benetti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bufano_F/0/1/0/all/0/1"&gt;F. Bufano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cappellaro_E/0/1/0/all/0/1"&gt;E. Cappellaro&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cason_A/0/1/0/all/0/1"&gt;A. D. Cason&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cetrulo_G/0/1/0/all/0/1"&gt;G. Cetrulo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ergon_M/0/1/0/all/0/1"&gt;M. Ergon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Germany_L/0/1/0/all/0/1"&gt;L. Germany&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harutyunyan_A/0/1/0/all/0/1"&gt;A. Harutyunyan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Howerton_S/0/1/0/all/0/1"&gt;S. Howerton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hurst_G/0/1/0/all/0/1"&gt;G. M. Hurst&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Patat_F/0/1/0/all/0/1"&gt;F. Patat&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stritzinger_M/0/1/0/all/0/1"&gt;M. Stritzinger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Strolger_L/0/1/0/all/0/1"&gt;L.-G. Strolger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wells_W/0/1/0/all/0/1"&gt;W. Wells&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2509"&gt;The Type II supernovae 2006V and 2006au: two SN 1987A-like events&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taddia_F/0/1/0/all/0/1"&gt;F. Taddia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stritzinger_M/0/1/0/all/0/1"&gt;M. D. Stritzinger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sollerman_J/0/1/0/all/0/1"&gt;J. Sollerman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Phillips_M/0/1/0/all/0/1"&gt;M. M. Phillips&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Anderson_J/0/1/0/all/0/1"&gt;J. P. Anderson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ergon_M/0/1/0/all/0/1"&gt;M. Ergon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Folatelli_G/0/1/0/all/0/1"&gt;G. Folatelli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fransson_C/0/1/0/all/0/1"&gt;C. Fransson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Freedman_W/0/1/0/all/0/1"&gt;W. Freedman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hamuy_M/0/1/0/all/0/1"&gt;M. Hamuy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Morrell_N/0/1/0/all/0/1"&gt;N. Morrell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pastorello_A/0/1/0/all/0/1"&gt;A. Pastorello&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Persson_S/0/1/0/all/0/1"&gt;S. E. Persson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gonzalez_S/0/1/0/all/0/1"&gt;S. Gonzalez&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2536"&gt;Local Magnetic Turbulence and TeV-PeV Cosmic Ray Anisotropies&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Giacinti_G/0/1/0/all/0/1"&gt;G. Giacinti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sigl_G/0/1/0/all/0/1"&gt;G. Sigl&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-1286542041049841674?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/1286542041049841674/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=1286542041049841674' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/1286542041049841674'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/1286542041049841674'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-111111.html' title='tipa -- 11/11/11'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-5371468046415109011</id><published>2011-11-09T21:56:00.000-05:00</published><updated>2011-11-09T21:57:23.873-05:00</updated><title type='text'>tipa -- 11/10/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2043"&gt;Discovery of extended VHE γ-ray emission from the vicinity of the young massive stellar cluster Westerlund 1&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_HESS/0/1/0/all/0/1"&gt;HESS Collaboration&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2045"&gt;Relativistic Outflow Drives Gamma-Ray Emission in 3C345&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schinzel_F/0/1/0/all/0/1"&gt;F. K. Schinzel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lobanov_A/0/1/0/all/0/1"&gt;A. P. Lobanov&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taylor_G/0/1/0/all/0/1"&gt;G. B. Taylor&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jorstad_S/0/1/0/all/0/1"&gt;S. G. Jorstad&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marscher_A/0/1/0/all/0/1"&gt;A. P. Marscher&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zensus_J/0/1/0/all/0/1"&gt;J. A. Zensus&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2048"&gt;The Milky Way's bright satellites as an apparent failure of LCDM&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Boylan_Kolchin_M/0/1/0/all/0/1"&gt;Michael Boylan-Kolchin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bullock_J/0/1/0/all/0/1"&gt;James S. Bullock&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kaplinghat_M/0/1/0/all/0/1"&gt;Manoj Kaplinghat&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2051"&gt;Two Populations of X-ray Pulsars Produced by Two Types of Supernovae&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Knigge_C/0/1/0/all/0/1"&gt;Christian Knigge&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Coe_M/0/1/0/all/0/1"&gt;Malcolm Coe&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Podsiadlowski_P/0/1/0/all/0/1"&gt;Philipp Podsiadlowski&lt;/a&gt; (2) ((1) University of Southampton, (2) University of Oxford)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2117"&gt;2D simulations of the double-detonation model for thermonuclear transients from low-mass carbon-oxygen white dwarfs&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sim_S/0/1/0/all/0/1"&gt;S. A. Sim&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fink_M/0/1/0/all/0/1"&gt;M. Fink&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kromer_M/0/1/0/all/0/1"&gt;M. Kromer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Roepke_F/0/1/0/all/0/1"&gt;F. K. Roepke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ruiter_A/0/1/0/all/0/1"&gt;A. J. Ruiter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hillebrandt_W/0/1/0/all/0/1"&gt;W. Hillebrandt&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2163"&gt;Extended hard X-ray emission from the Vela pulsar wind nebula&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mattana_F/0/1/0/all/0/1"&gt;Fabio Mattana&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gotz_D/0/1/0/all/0/1"&gt;Diego Götz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Terrier_R/0/1/0/all/0/1"&gt;Régis Terrier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bouchet_L/0/1/0/all/0/1"&gt;Laurent Bouchet&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ponti_G/0/1/0/all/0/1"&gt;Gabriele Ponti&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Falanga_M/0/1/0/all/0/1"&gt;Maurizio Falanga&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Renaud_M/0/1/0/all/0/1"&gt;Matthieu Renaud&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Caballero_I/0/1/0/all/0/1"&gt;Isabel Caballero&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Soldi_S/0/1/0/all/0/1"&gt;Simona Soldi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Heras_J/0/1/0/all/0/1"&gt;Juan Antonio Zurita Heras&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schanne_S/0/1/0/all/0/1"&gt;Stephane Schanne&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-5371468046415109011?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/5371468046415109011/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=5371468046415109011' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5371468046415109011'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/5371468046415109011'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-11102011.html' title='tipa -- 11/10/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-7404593530947962270</id><published>2011-11-08T22:12:00.000-05:00</published><updated>2011-11-08T22:13:00.667-05:00</updated><title type='text'>tipa -- 11/9/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1735"&gt;HST-COS Observations of Hydrogen, Helium, Carbon and Nitrogen Emission from the SN 1987A Reverse Shock&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+France_K/0/1/0/all/0/1"&gt;Kevin France&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McCray_R/0/1/0/all/0/1"&gt;Richard McCray&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Penton_S/0/1/0/all/0/1"&gt;Steven V. Penton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kirshner_R/0/1/0/all/0/1"&gt;Robert P. Kirshner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Challis_P/0/1/0/all/0/1"&gt;Peter Challis&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Laming_J/0/1/0/all/0/1"&gt;J. Martin Laming&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bouchet_P/0/1/0/all/0/1"&gt;Patrice Bouchet&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chevalier_R/0/1/0/all/0/1"&gt;Roger Chevalier&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fransson_C/0/1/0/all/0/1"&gt;Claes Fransson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Garnavich_P/0/1/0/all/0/1"&gt;Peter M. Garnavich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Heng_K/0/1/0/all/0/1"&gt;Kevin Heng&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Larsson_J/0/1/0/all/0/1"&gt;Josefin Larsson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lawrence_S/0/1/0/all/0/1"&gt;Stephen Lawrence&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lundqvist_P/0/1/0/all/0/1"&gt;Peter Lundqvist&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Panagia_N/0/1/0/all/0/1"&gt;Nino Panagia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pun_C/0/1/0/all/0/1"&gt;Chun S. J. Pun&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Smith_N/0/1/0/all/0/1"&gt;Nathan Smith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sollerman_J/0/1/0/all/0/1"&gt;Jesper Sollerman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sonneborn_G/0/1/0/all/0/1"&gt;George Sonneborn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sugerman_B/0/1/0/all/0/1"&gt;Ben Sugerman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wheeler_J/0/1/0/all/0/1"&gt;J. Craig Wheeler&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1779"&gt;Detection of Gamma-Ray Polarization in Prompt Emission of GRB 100826A&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yonetoku_D/0/1/0/all/0/1"&gt;Daisuke Yonetoku&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Murakami_T/0/1/0/all/0/1"&gt;Toshio Murakami&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gunji_S/0/1/0/all/0/1"&gt;Shuichi Gunji&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mihara_T/0/1/0/all/0/1"&gt;Tatehiro Mihara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Toma_K/0/1/0/all/0/1"&gt;Kenji Toma&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sakashita_T/0/1/0/all/0/1"&gt;Tomonori Sakashita&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Morihara_Y/0/1/0/all/0/1"&gt;Yoshiyuki Morihara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Takahashi_T/0/1/0/all/0/1"&gt;Takuya Takahashi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Toukairin_N/0/1/0/all/0/1"&gt;Noriyuki Toukairin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fujimoto_H/0/1/0/all/0/1"&gt;Hirofumi Fujimoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kodama_Y/0/1/0/all/0/1"&gt;Yoshiki Kodama&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kubo_S/0/1/0/all/0/1"&gt;Shin Kubo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Team_IKAROS_Demonstration/0/1/0/all/0/1"&gt;IKAROS Demonstration Team&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1833"&gt;Supernovae without host galaxies? The low surface brightness host of SN 2009Z&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zinn_P/0/1/0/all/0/1"&gt;P.-C. Zinn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stritzinger_M/0/1/0/all/0/1"&gt;M. Stritzinger&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Braithwaite_J/0/1/0/all/0/1"&gt;J. Braithwaite&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gallazzi_A/0/1/0/all/0/1"&gt;A. Gallazzi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Grunden_P/0/1/0/all/0/1"&gt;P. Grunden&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bomans_D/0/1/0/all/0/1"&gt;D. J. Bomans&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Morrell_N/0/1/0/all/0/1"&gt;N. I. Morrell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bach_U/0/1/0/all/0/1"&gt;U. Bach&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.2036"&gt;Escape from Vela X&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hinton_J/0/1/0/all/0/1"&gt;James Hinton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Funk_S/0/1/0/all/0/1"&gt;Stefan Funk&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parsons_R/0/1/0/all/0/1"&gt;Robert Parsons&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ohm_S/0/1/0/all/0/1"&gt;Stefan Ohm&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-7404593530947962270?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/7404593530947962270/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=7404593530947962270' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7404593530947962270'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/7404593530947962270'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-1192011.html' title='tipa -- 11/9/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-1175542002775694090</id><published>2011-11-07T23:25:00.000-05:00</published><updated>2011-11-07T23:26:21.768-05:00</updated><title type='text'>tipa -- 11/8/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1234"&gt;The first Infrared study of the close environment of a long Gamma-Ray Burst&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Floch_E/0/1/0/all/0/1"&gt;E.Le Floc'h&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Charmandaris_V/0/1/0/all/0/1"&gt;V.Charmandaris&lt;/a&gt; (2,3,4), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gordon_K/0/1/0/all/0/1"&gt;K.Gordon&lt;/a&gt; (5), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Forrest_W/0/1/0/all/0/1"&gt;W.J.Forrest&lt;/a&gt; (6), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brandl_B/0/1/0/all/0/1"&gt;B.Brandl&lt;/a&gt; (7), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schaerer_D/0/1/0/all/0/1"&gt;D.Schaerer&lt;/a&gt; (8,9), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dessauges_Zavadsky_M/0/1/0/all/0/1"&gt;M.Dessauges-Zavadsky&lt;/a&gt; (8), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Armus_L/0/1/0/all/0/1"&gt;L.Armus&lt;/a&gt; (10) ((1) CEA/AIM, France, (2) Univ.of Crete, Greece, (3) Obs.de Paris, France, (4) IESL, Greece, (5) STScI, Baltimore, USA, (6) Univ.of Rochester, USA, (7) Leiden Obs., Netherlands, (8) Geneva Obs., Switzerland, (9) CNRS/IRAP, France, (10) Spitzer Science Center, Pasadena, USA)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1393"&gt;A nearby GRB host galaxy: VLT/X-shooter observations of HG 031203&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guseva_N/0/1/0/all/0/1"&gt;N. G. Guseva&lt;/a&gt; (1,2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Izotov_Y/0/1/0/all/0/1"&gt;Y. I. Izotov&lt;/a&gt; (1,2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fricke_K/0/1/0/all/0/1"&gt;K. J. Fricke&lt;/a&gt; (1,3), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Henkel_C/0/1/0/all/0/1"&gt;C. Henkel&lt;/a&gt; (1) ((1) Max-Planck-Institute for Radioastronomy, Bonn, Germany, (2) Main Astronomical Observatory, Kyiv, Ukraine, (3) Institute for Astrophysics, University of Goettingen, Goettingen, Germany)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1527"&gt;Effect of Population III Multiplicity on Dark Star Formation&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stacy_A/0/1/0/all/0/1"&gt;Athena Stacy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pawlik_A/0/1/0/all/0/1"&gt;Andreas H. Pawlik&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bromm_V/0/1/0/all/0/1"&gt;Volker Bromm&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Loeb_A/0/1/0/all/0/1"&gt;Abraham Loeb&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1607"&gt;Enhancing the Relative Fe-to-Proton Abundance in Ultra-High-Energy Cosmic Rays&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Blaksley_C/0/1/0/all/0/1"&gt;Carl Blaksley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parizot_E/0/1/0/all/0/1"&gt;Etienne Parizot&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1668"&gt;Pulsar Pair Cascades in Magnetic Fields with Offset Polar Caps&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Harding_A/0/1/0/all/0/1"&gt;Alice K. Harding&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Muslimov_A/0/1/0/all/0/1"&gt;Alex G. Muslimov&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1692"&gt;A comparison between star formation rate diagnostics and rate of core collapse supernovae within 11 Mpc&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Botticella_M/0/1/0/all/0/1"&gt;M. T. Botticella&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Smartt_S/0/1/0/all/0/1"&gt;S. J. Smartt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kennicutt_R/0/1/0/all/0/1"&gt;R. C. Kennicutt Jr.&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cappellaro_E/0/1/0/all/0/1"&gt;E. Cappellaro&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sereno_M/0/1/0/all/0/1"&gt;M. Sereno&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lee_J/0/1/0/all/0/1"&gt;J. C. Lee&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1677"&gt;Black hole-neutron star mergers for 10 solar mass black holes&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Foucart_F/0/1/0/all/0/1"&gt;Francois Foucart&lt;/a&gt;, &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Duez_M/0/1/0/all/0/1"&gt;Matthew D. Duez&lt;/a&gt;, &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Kidder_L/0/1/0/all/0/1"&gt;Lawrence E. Kidder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Scheel_M/0/1/0/all/0/1"&gt;Mark A. Scheel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Szilagyi_B/0/1/0/all/0/1"&gt;Bela Szilagyi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/gr-qc/1/au:+Teukolsky_S/0/1/0/all/0/1"&gt;Saul A. Teukolsky&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1436"&gt;Neutrino mass in cosmology: status and prospects&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wong_Y/0/1/0/all/0/1"&gt;Yvonne Y. Y. Wong&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1343"&gt;Nuclear condensate and helium white dwarfs&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Bedaque_P/0/1/0/all/0/1"&gt;Paulo F. Bedaque&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Berkowitz_E/0/1/0/all/0/1"&gt;Evan Berkowitz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/nucl-th/1/au:+Cherman_A/0/1/0/all/0/1"&gt;Aleksey Cherman&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.1691"&gt;Shining a Gluon Beam Through Quark-Gluon Plasma&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-th/1/au:+Chesler_P/0/1/0/all/0/1"&gt;Paul M. Chesler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-th/1/au:+Ho_Y/0/1/0/all/0/1"&gt;Ying-Yu Ho&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-th/1/au:+Rajagopal_K/0/1/0/all/0/1"&gt;Krishna Rajagopal&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-1175542002775694090?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/1175542002775694090/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=1175542002775694090' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/1175542002775694090'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/1175542002775694090'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-1182011.html' title='tipa -- 11/8/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-3696668760298550304</id><published>2011-11-07T23:20:00.001-05:00</published><updated>2011-11-07T23:20:54.065-05:00</updated><title type='text'>tipa -- 11/7/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0966"&gt;A Compact Degenerate Primary-Star Progenitor of SN 2011fe&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bloom_J/0/1/0/all/0/1"&gt;Joshua S. Bloom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kasen_D/0/1/0/all/0/1"&gt;Daniel Kasen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shen_K/0/1/0/all/0/1"&gt;Ken J. Shen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nugent_P/0/1/0/all/0/1"&gt;Peter E. Nugent&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Butler_N/0/1/0/all/0/1"&gt;Nathaniel R. Butler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Graham_M/0/1/0/all/0/1"&gt;Melissa L. Graham&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Howell_D/0/1/0/all/0/1"&gt;D. Andrew Howell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kolb_U/0/1/0/all/0/1"&gt;Ulrich Kolb&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holmes_S/0/1/0/all/0/1"&gt;Stefan Holmes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Haswell_C/0/1/0/all/0/1"&gt;Carole Haswell&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Burwitz_V/0/1/0/all/0/1"&gt;Vadim Burwitz&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rodriguez_J/0/1/0/all/0/1"&gt;Juan Rodriguez&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sullivan_M/0/1/0/all/0/1"&gt;Mark Sullivan&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0970"&gt;Unifying the Zoo of Jet-Driven Stellar Explosions&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lazzati_D/0/1/0/all/0/1"&gt;Davide Lazzati&lt;/a&gt; (NCSU), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Morsony_B/0/1/0/all/0/1"&gt;Brian J. Morsony&lt;/a&gt; (UWi Madison), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Blackwell_C/0/1/0/all/0/1"&gt;Christopher H. Blackwell&lt;/a&gt; (NCSU &amp;amp; UAH), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Begelman_M/0/1/0/all/0/1"&gt;Micthell C. Begelman&lt;/a&gt; (CU Boulder)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-3696668760298550304?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/3696668760298550304/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=3696668760298550304' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3696668760298550304'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/3696668760298550304'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-1172011.html' title='tipa -- 11/7/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-440822108339097535</id><published>2011-11-03T22:05:00.001-05:00</published><updated>2011-11-03T22:05:50.135-05:00</updated><title type='text'>tipa -- 11/4/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0631"&gt;Cosmic flows in the nearby universe from Type Ia Supernovae&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Turnbull_S/0/1/0/all/0/1"&gt;Stephen J. Turnbull&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hudson_M/0/1/0/all/0/1"&gt;Michael J. Hudson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Feldman_H/0/1/0/all/0/1"&gt;Hume A. Feldman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hicken_M/0/1/0/all/0/1"&gt;Malcolm Hicken&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kirshner_R/0/1/0/all/0/1"&gt;Robert P. Kirshner&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Watkin_R/0/1/0/all/0/1"&gt;Richard Watkin&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0665"&gt;Hydrodynamics of Core-Collapse Supernovae at the Transition to Explosion. I. Spherical Symmetry&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fernandez_R/0/1/0/all/0/1"&gt;Rodrigo Fernández&lt;/a&gt; (IAS)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0848"&gt;Discovery of a giant, highly-collimated jet from Sanduleak's star in the Large Magellanic Cloud&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Angeloni_R/0/1/0/all/0/1"&gt;R. Angeloni&lt;/a&gt; (1), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mille_F/0/1/0/all/0/1"&gt;F. Di Mille&lt;/a&gt; (2), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bland_Hawthorn_J/0/1/0/all/0/1"&gt;J. Bland-Hawthorn&lt;/a&gt; (3), &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Osip_D/0/1/0/all/0/1"&gt;D. Osip&lt;/a&gt; (4)- ((1) Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, (2) Australian Astronomical Observatory - Carnegie Observatories, (3) Sydney Institute for Astronomy, School of Physics, University of Sydney, (4) Las Campanas Observatory, Carnegie Observatories)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0932"&gt;A measurement of secondary cosmic microwave background anisotropies with two years of South Pole Telescope observations&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reichardt_C/0/1/0/all/0/1"&gt;C. L. Reichardt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shaw_L/0/1/0/all/0/1"&gt;L. Shaw&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zahn_O/0/1/0/all/0/1"&gt;O. Zahn&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Aird_K/0/1/0/all/0/1"&gt;K. A. Aird&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Benson_B/0/1/0/all/0/1"&gt;B. A. Benson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bleem_L/0/1/0/all/0/1"&gt;L. E. Bleem&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Carlstrom_J/0/1/0/all/0/1"&gt;J. E. Carlstrom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chang_C/0/1/0/all/0/1"&gt;C. L. Chang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cho_H/0/1/0/all/0/1"&gt;H. M. Cho&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Crawford_T/0/1/0/all/0/1"&gt;T. M. Crawford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Crites_A/0/1/0/all/0/1"&gt;A. T. Crites&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Haan_T/0/1/0/all/0/1"&gt;T. de Haan&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dobbs_M/0/1/0/all/0/1"&gt;M. A. Dobbs&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dudley_J/0/1/0/all/0/1"&gt;J. Dudley&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+George_E/0/1/0/all/0/1"&gt;E. M. George&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Halverson_N/0/1/0/all/0/1"&gt;N. W. Halverson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holder_G/0/1/0/all/0/1"&gt;G. P. Holder&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Holzapfel_W/0/1/0/all/0/1"&gt;W. L. Holzapfel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hoover_S/0/1/0/all/0/1"&gt;S. Hoover&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hou_Z/0/1/0/all/0/1"&gt;Z. Hou&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hrubes_J/0/1/0/all/0/1"&gt;J. D. Hrubes&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Joy_M/0/1/0/all/0/1"&gt;M. Joy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Keisler_R/0/1/0/all/0/1"&gt;R. Keisler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Knox_L/0/1/0/all/0/1"&gt;L. Knox&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lee_A/0/1/0/all/0/1"&gt;A. T. Lee&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Leitch_E/0/1/0/all/0/1"&gt;E. M. Leitch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lueker_M/0/1/0/all/0/1"&gt;M. Lueker&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Luong_Van_D/0/1/0/all/0/1"&gt;D. Luong-Van&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McMahon_J/0/1/0/all/0/1"&gt;J. J. McMahon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mehl_J/0/1/0/all/0/1"&gt;J. Mehl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meyer_S/0/1/0/all/0/1"&gt;S. S. Meyer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Millea_M/0/1/0/all/0/1"&gt;M. Millea&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mohr_J/0/1/0/all/0/1"&gt;J. J. Mohr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Montroy_T/0/1/0/all/0/1"&gt;T. E. Montroy&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Natoli_T/0/1/0/all/0/1"&gt;T. Natoli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Padin_S/0/1/0/all/0/1"&gt;S. Padin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Plagge_T/0/1/0/all/0/1"&gt;T. Plagge&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pryke_C/0/1/0/all/0/1"&gt;C. Pryke&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ruhl_J/0/1/0/all/0/1"&gt;J. E. Ruhl&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schaffer_K/0/1/0/all/0/1"&gt;K. K. Schaffer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Shirokoff_E/0/1/0/all/0/1"&gt;E. Shirokoff&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Spieler_H/0/1/0/all/0/1"&gt;H. G. Spieler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Staniszewski_Z/0/1/0/all/0/1"&gt;Z. Staniszewski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stark_A/0/1/0/all/0/1"&gt;A. A. Stark&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Story_K/0/1/0/all/0/1"&gt;K. Story&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Engelen_A/0/1/0/all/0/1"&gt;A. van Engelen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vanderlinde_K/0/1/0/all/0/1"&gt;K. Vanderlinde&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vieira_J/0/1/0/all/0/1"&gt;J. D. Vieira&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Williamson_R/0/1/0/all/0/1"&gt;R. Williamson&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0936"&gt;High-Energy Emission Induced by Ultra-high-Energy Photons as a Probe of Ultra-high-Energy Cosmic-Ray Accelerators Embedded in the Cosmic Web&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Murase_K/0/1/0/all/0/1"&gt;Kohta Murase&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-440822108339097535?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/440822108339097535/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=440822108339097535' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/440822108339097535'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/440822108339097535'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-1142011.html' title='tipa -- 11/4/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-4437043177885748201</id><published>2011-11-02T21:34:00.000-05:00</published><updated>2011-11-02T21:35:21.692-05:00</updated><title type='text'>tipa -- 11/3/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0523"&gt;Discovery of Nine Gamma-Ray Pulsars in Fermi-LAT Data Using a New Blind Search Method&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pletsch_H/0/1/0/all/0/1"&gt;H. J. Pletsch&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Guillemot_L/0/1/0/all/0/1"&gt;L. Guillemot&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Allen_B/0/1/0/all/0/1"&gt;B. Allen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kramer_M/0/1/0/all/0/1"&gt;M. Kramer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Aulbert_C/0/1/0/all/0/1"&gt;C. Aulbert&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fehrmann_H/0/1/0/all/0/1"&gt;H. Fehrmann&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ray_P/0/1/0/all/0/1"&gt;P. S. Ray&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Barr_E/0/1/0/all/0/1"&gt;E. D. Barr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Belfiore_A/0/1/0/all/0/1"&gt;A. Belfiore&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Camilo_F/0/1/0/all/0/1"&gt;F. Camilo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Caraveo_P/0/1/0/all/0/1"&gt;P. A. Caraveo&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Celik_O/0/1/0/all/0/1"&gt;O. Celik&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Champion_D/0/1/0/all/0/1"&gt;D. J. Champion&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dormody_M/0/1/0/all/0/1"&gt;M. Dormody&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eatough_R/0/1/0/all/0/1"&gt;R. P. Eatough&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ferrara_E/0/1/0/all/0/1"&gt;E. C. Ferrara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Freire_P/0/1/0/all/0/1"&gt;P. C. C. Freire&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hessels_J/0/1/0/all/0/1"&gt;J. W. T. Hessels&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Keith_M/0/1/0/all/0/1"&gt;M. Keith&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kerr_M/0/1/0/all/0/1"&gt;M. Kerr&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Luca_A/0/1/0/all/0/1"&gt;A. de Luca&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lyne_A/0/1/0/all/0/1"&gt;A. G. Lyne&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marelli_M/0/1/0/all/0/1"&gt;M. Marelli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+McLaughlin_M/0/1/0/all/0/1"&gt;M. A. McLaughlin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parent_D/0/1/0/all/0/1"&gt;D. Parent&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ransom_S/0/1/0/all/0/1"&gt;S. M. Ransom&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Razzano_M/0/1/0/all/0/1"&gt;M. Razzano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Reich_W/0/1/0/all/0/1"&gt;W. Reich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Parkinson_P/0/1/0/all/0/1"&gt;P. M. Saz Parkinson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stappers_B/0/1/0/all/0/1"&gt;B. W. Stappers&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wolff_M/0/1/0/all/0/1"&gt;M. T. Wolff&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0596"&gt;Improved distance determination to M51 from supernovae 2011dh and 2005cs&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vinko_J/0/1/0/all/0/1"&gt;J. Vinko&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Takats_K/0/1/0/all/0/1"&gt;K. Takats&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Szalai_T/0/1/0/all/0/1"&gt;T. Szalai&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Marion_G/0/1/0/all/0/1"&gt;G. H. Marion&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wheeler_J/0/1/0/all/0/1"&gt;J. C. Wheeler&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sarneczky_K/0/1/0/all/0/1"&gt;K. Sarneczky&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Garnavich_P/0/1/0/all/0/1"&gt;P. M. Garnavich&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kelemen_J/0/1/0/all/0/1"&gt;J. Kelemen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Klagyivik_P/0/1/0/all/0/1"&gt;P. Klagyivik&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Pal_A/0/1/0/all/0/1"&gt;A. Pal&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Szalai_N/0/1/0/all/0/1"&gt;N. Szalai&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vida_K/0/1/0/all/0/1"&gt;K. Vida&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0605"&gt;Dark Radiation from Particle Decays during Big Bang Nucleosynthesis&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Menestrina_J/0/1/0/all/0/1"&gt;Justin L. Menestrina&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Scherrer_R/0/1/0/all/0/1"&gt;Robert J. Scherrer&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-4437043177885748201?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/4437043177885748201/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=4437043177885748201' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4437043177885748201'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4437043177885748201'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-1132011.html' title='tipa -- 11/3/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-4817640611668764303</id><published>2011-11-01T21:56:00.001-05:00</published><updated>2011-11-01T21:56:23.849-05:00</updated><title type='text'>tipa -- 11/2/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0007"&gt;A Revised View of the Transient Radio Sky&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Frail_D/0/1/0/all/0/1"&gt;D. A. Frail&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kulkarni_S/0/1/0/all/0/1"&gt;S. R. Kulkarni&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ofek_E/0/1/0/all/0/1"&gt;E. O. Ofek&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bower_G/0/1/0/all/0/1"&gt;G. C. Bower&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Nakar_E/0/1/0/all/0/1"&gt;E. Nakar&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1111.0157"&gt;The VLT-FLAMES Tarantula Survey: The fastest rotating O-type star and shortest period LMC pulsar - remnants of a supernova disrupted binary?&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span class="descriptor"&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors:&lt;/span&gt;&lt;/span&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dufton_P/0/1/0/all/0/1"&gt;P. L. Dufton&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dunstall_P/0/1/0/all/0/1"&gt;P. R. Dunstall&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Evans_C/0/1/0/all/0/1"&gt;C. J. Evans&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brott_I/0/1/0/all/0/1"&gt;I. Brott&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cantiello_M/0/1/0/all/0/1"&gt;M. Cantiello&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Koter_A/0/1/0/all/0/1"&gt;A. de Koter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mink_S/0/1/0/all/0/1"&gt;S.E. de Mink&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fraser_M/0/1/0/all/0/1"&gt;M. Fraser&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Henault_Brunet_V/0/1/0/all/0/1"&gt;V. Hénault-Brunet&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Howarth_I/0/1/0/all/0/1"&gt;I. D. Howarth&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Langer_N/0/1/0/all/0/1"&gt;N. Langer&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lennon_D/0/1/0/all/0/1"&gt;D. J. Lennon&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Markova_N/0/1/0/all/0/1"&gt;N. Markova&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sana_H/0/1/0/all/0/1"&gt;H. Sana&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Taylor_W/0/1/0/all/0/1"&gt;W. D. Taylor&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;&lt;div class="blogger-post-footer"&gt;today in particle astrophysics: a daily service by someone&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/110791865256541639-4817640611668764303?l=particle-astro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://particle-astro.blogspot.com/feeds/4817640611668764303/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=110791865256541639&amp;postID=4817640611668764303' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4817640611668764303'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/110791865256541639/posts/default/4817640611668764303'/><link rel='alternate' type='text/html' href='http://particle-astro.blogspot.com/2011/11/tipa-1122011.html' title='tipa -- 11/2/2011'/><author><name>zwicky</name><uri>http://www.blogger.com/profile/04022777559763626259</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-110791865256541639.post-7845654343669592337</id><published>2011-10-31T21:16:00.000-05:00</published><updated>2011-10-31T21:17:13.600-05:00</updated><title type='text'>tipa -- 11/1/2011</title><content type='html'>&lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1110.6442"&gt;The Hubble Space Telescope Cluster Supernova Survey: VI. The Volumetric Type Ia Supernova Rate&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Barbary_K/0/1/0/all/0/1"&gt;K. Barbary&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Aldering_G/0/1/0/all/0/1"&gt;G. Aldering&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Amanullah_R/0/1/0/all/0/1"&gt;R. Amanullah&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Brodwin_M/0/1/0/all/0/1"&gt;M. Brodwin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Connolly_N/0/1/0/all/0/1"&gt;N. Connolly&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Dawson_K/0/1/0/all/0/1"&gt;K. S. Dawson&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Doi_M/0/1/0/all/0/1"&gt;M. Doi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eisenhardt_P/0/1/0/all/0/1"&gt;P. Eisenhardt&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Faccioli_L/0/1/0/all/0/1"&gt;L. Faccioli&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fadeyev_V/0/1/0/all/0/1"&gt;V. Fadeyev&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fakhouri_H/0/1/0/all/0/1"&gt;H. K. Fakhouri&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fruchter_A/0/1/0/all/0/1"&gt;A. S. Fruchter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gilbank_D/0/1/0/all/0/1"&gt;D. G. Gilbank&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gladders_M/0/1/0/all/0/1"&gt;M. D. Gladders&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Goldhaber_G/0/1/0/all/0/1"&gt;G. Goldhaber&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Goobar_A/0/1/0/all/0/1"&gt;A. Goobar&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hattori_T/0/1/0/all/0/1"&gt;T. Hattori&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hsiao_E/0/1/0/all/0/1"&gt;E. Hsiao&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Huang_X/0/1/0/all/0/1"&gt;X. Huang&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ihara_Y/0/1/0/all/0/1"&gt;Y. Ihara&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kashikawa_N/0/1/0/all/0/1"&gt;N. Kashikawa&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Koester_B/0/1/0/all/0/1"&gt;B. Koester&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Konishi_K/0/1/0/all/0/1"&gt;K. Konishi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kowalski_M/0/1/0/all/0/1"&gt;M. Kowalski&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lidman_C/0/1/0/all/0/1"&gt;C. Lidman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Lubin_L/0/1/0/all/0/1"&gt;L. Lubin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Meyers_J/0/1/0/all/0/1"&gt;J. Meyers&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Morokuma_T/0/1/0/all/0/1"&gt;T. Morokuma&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Oda_T/0/1/0/all/0/1"&gt;T. Oda&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Panagia_N/0/1/0/all/0/1"&gt;N. Panagia&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perlmutter_S/0/1/0/all/0/1"&gt;S. Perlmutter&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Postman_M/0/1/0/all/0/1"&gt;M. Postman&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ripoche_P/0/1/0/all/0/1"&gt;P. Ripoche&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rosati_P/0/1/0/all/0/1"&gt;P. Rosati&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rubin_D/0/1/0/all/0/1"&gt;D. Rubin&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schlegel_D/0/1/0/all/0/1"&gt;D. J. Schlegel&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Spadafora_A/0/1/0/all/0/1"&gt;A. L. Spadafora&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stanford_S/0/1/0/all/0/1"&gt;S. A. Stanford&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Strovink_M/0/1/0/all/0/1"&gt;M. Strovink&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Suzuki_N/0/1/0/all/0/1"&gt;N. Suzuki&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Takanashi_N/0/1/0/all/0/1"&gt;N. Takanashi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Tokita_K/0/1/0/all/0/1"&gt;K. Tokita&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Yasuda_N/0/1/0/all/0/1"&gt;N. Yasuda&lt;/a&gt;, for the &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Project_S/0/1/0/all/0/1"&gt;Supernova Cosmology Project&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1110.6479"&gt;Heavy sterile neutrinos, entropy and relativistic energy production, and the relic neutrino background&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fuller_G/0/1/0/all/0/1"&gt;George M. Fuller&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kishimoto_C/0/1/0/all/0/1"&gt;Chad T. Kishimoto&lt;/a&gt;, &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kusenko_A/0/1/0/all/0/1"&gt;Alexander Kusenko&lt;/a&gt;&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1110.6644"&gt;A new analytic solution for 2nd-order Fermi acceleration&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Mertsch_P/0/1/0/all/0/1"&gt;Philipp Mertsch&lt;/a&gt; (Oxford)&lt;/span&gt;&lt;/li&gt;&lt;/ul&gt;  &lt;p class="MsoNormal"&gt;&lt;span style="font-family: Arial;"&gt; &lt;/span&gt;&lt;/p&gt;  &lt;p class="MsoNormal" style="margin-bottom: 0.0001pt;"&gt;&lt;b style=""&gt;&lt;span style="font-family: Arial;"&gt;&lt;a href="http://arxiv.org/abs/1110.6448"&gt;Probing Novel Scalar and Tensor Interactions from (Ultra)Cold Neutrons to the LHC&lt;/a&gt;&lt;/span&gt;&lt;/b&gt;&lt;/p&gt;  &lt;ul&gt;&lt;li&gt;&lt;span style="font-size: 9pt; font-family: Arial;"&gt;Authors: &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Bhattacharya_T/0/1/0/all/0/1"&gt;Tanmoy Bhattacharya&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Cirigliano_V/0/1/0/all/0/1"&gt;Vincenzo Cirigliano&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Cohen_S/0/1/0/all/0/1"&gt;Saul D. Cohen&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Filipuzzi_A/0/1/0/all/0/1"&gt;Alberto Filipuzzi&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Gonzalez_Alonso_M/0/1/0/all/0/1"&gt;Martin Gonzalez-Alonso&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Graesser_M/0/1/0/all/0/1"&gt;Michael L. Graesser&lt;/a&gt;, &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Gupta_R/0/1/0/all/0/1"&gt;Rajan Gupta&lt;/a
