tipa -- 1/9/2007

Discovery of a Probable Physical Triple Quasar

• Authors: S.G. Djorgovski, F. Courbin, G. Meylan, D. Sluse, D.J. Thompson, A. Mahabal, E. Glikman

XMM-Newton observations reveal the X-ray counterpart of the very-high-energy gamma-ray source HESSJ1640-465

• Authors: S.Funk, J.A.Hinton, G.Puehlhofer, F.A.Aharonian, W.Hofmann, O.Reimer, S.Wagner

Ultrahigh energy cosmic rays as heavy nuclei from cluster accretion shocks

• Authors: Susumu Inoue (NAOJ), Guenter Sigl (APC/IAP), Francesco Miniati (ETHZ), Eric Armengaud (DSM/DAPNIA)

Do long-duration GRBs follow star formation?

• Authors: Dafne Guetta, Tsvi Piran

Ruling out a massive-asymptotic giant-branch star as the progenitor of supernova 2005cs

• Authors: J.J. Eldridge, S. Mattila, S.J. Smartt

Neutrino astronomy and gamma-ray bursts

• Authors: E. Waxman (Weizmann Inst.)

Can the early X-ray afterglow of GRBs be explained by a contribution from the reverse shock?

• Authors: Franck Genet (1), Frederic Daigne (1), Robert Mochkovitch (1) ((1) Institut d'Astrophysique de Paris, UMR7095 CNRS-Universite Pierre et Marie Curie-Paris 6)

Large-Mass Ultra-Low Noise Germanium Detectors: Performance and Applications in Neutrino and Astroparticle Physics

• Authors: P.S. Barbeau, J.I. Collar, O. Tench