伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章,另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.

星期三, 十一月 08, 2006

Berger2006 几个高红移短暴的观测

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文章信息:


astro-ph/0611128 [abs, ps, pdf, other] :
Title: A New Population of High Redshift Short-Duration Gamma-Ray Bursts
Authors: E. Berger, D.B. Fox, P.A. Price, E. Nakar, A. Gal-Yam, D.E. Holz, B.P. Schmidt, A. Cucchiara, S.B. Cenko, S.R. Kulkarni, A.M. Soderberg, D.A. Frail, B.E. Penprase, A. Rau, E. Ofek, S.J. Bell Burnell, P.B. Cameron, L.L. Cowie, M.A. Dopita, I. Hook, B.A. Peterson, Ph. Podsiadlowski, K.C. Roth, R.E. Rutledge, S.S. Sheppard, A. Songaila
Comments: Submitted to ApJ; 6 figures, 1 table; comments are welcome

The redshift distribution of the short-duration GRBs is a crucial, but currently fragmentary, clue to the nature of their progenitors. Here we present optical observations of seven short GRBs obtained with Gemini, Magellan, and HST. We detect the afterglows and host galaxies of two short bursts, and host galaxies for two additional bursts with known optical afterglow positions, and three with X-ray positions (<4.5" r="23-26.5" r="17-22" z="1.1304">0.7 (97% confidence level), suggesting that 1/4-2/3 of all short GRBs originate at higher redshifts than previously determined. This has two important implications: (i) We constrain the acceptable age distributions to a wide lognormal (sigma~1) with tau~4-8 Gyr, or to a power law, P(tau)~tau^n, with -1<0;>

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