tipa -- 7/4/2013

The Locations of Short Gamma-ray Bursts as Evidence for Compact Object Binary Progenitors

• Wen-fai Fong, Edo Berger (Harvard)

Improving Dark Energy Constraints with High Redshift Type Ia Supernovae from CANDELS and CLASH

• Vincenzo Salzano, Steven A. Rodney, Irene Sendra, Ruth Lazkoz, Adam G. Riess, Marc Postman, Tom Broadhurst, Dan Coe

Constraints on dark energy with the LOSS SN Ia sample

• Mohan Ganeshalingam, Weidong Li, Alexei V. Filippenko

Galactic Constraints on Supernova Progenitor Models

• I.Acharova, B.Gibson, Yu.Mishurov, V.Kovtyukh

A method for quantifying the Gamma Ray Burst "bias". Application in the redshift range 0-1.1

• S. Boissier, R. Salvaterra, E. Le Floc'h, S. Basa, V. Buat, N. Prantzos, S.D. Vergani, S. Savaglio

Massive double compact object mergers: gravitational wave sources and r-process-element production sites

• N. Mennekens, D. Vanbeveren

A new mechanism for saturating unstable r-modes in neutron stars

• Brynmor Haskell, Kostas Glampedakis, Nils Andersson

X-ray Observations of the Supernova Remnant CTB 87 (G74.9+1.2): An Evolved Pulsar Wind Nebula

• H. Matheson, S. Safi-Harb, R. Kothes

Is the CMB telling us that dark matter is weaker than weakly interacting?

• Dan Hooper

The Daya Bay Antineutrino Detector Filling System and Liquid Mass Measurement

• H.R. Band, J.J. Cherwinka, E. Draeger, K.M. Heeger, P. Hinrichs, C.A. Lewis, H. Mattison, M.C. McFarlane, D.M. Webber, D. Wenman, W. Wang, T. Wise, Q. Xiao