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Title: BAT2 GRB Catalog - Prompt Emission Properties of Swift GRBs

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3509266· OSTI ID:21439587
 [1]; ; ; ;  [2]; ;  [1]; ;  [3];  [1];  [1];  [4];  [5];  [6]
  1. CRESST and NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
  2. NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
  3. Los Alamos National Laboratory, P.O. Box 1663, Los Alamos, NM, 87545 (United States)
  4. Department of Astronomy, University of Maryland, College Park, MD 20742 (United States)
  5. Center for Cosmology and Astro-Particle Physics, Department of Physics, Ohio State University, 191 West Woodruff Avenue, Columbus, OH 43210 (United States)
  6. Center for Nuclear Studies, Department of Physics, George Washington University, Washington, D.C. 20052 (United States)

We present the second Swift Burst Alert Telescope (BAT) catalog of gamma-ray bursts (GRBs), which contains 476 bursts detected by the BAT between 2004 December 19 and 2009 December 21. This catalog presents burst trigger time, location, 90% error radius, duration, fluence, peak flux, time-averaged spectral parameters and time-resolved spectral parameters measured by the BAT. The BAT T{sub 90} duration peaks at 70 s. We confirm that the spectra of the BAT short-duration GRBs are generally harder than those of the long-duration GRBs. The observed durations of the BAT high redshift GRBs are not systematically longer than those of the moderate redshift GRBs. Furthermore, the observed spectra of the BAT high redshift GRBs are similar to or harder than the moderate redshift GRBs.

OSTI ID:
21439587
Journal Information:
AIP Conference Proceedings, Vol. 1279, Issue 1; Conference: Conference on deciphering the ancient universe with gamma-ray bursts, Kyoto (Japan), 19-23 Apr 2010; Other Information: DOI: 10.1063/1.3509266; (c) 2010 American Institute of Physics; ISSN 0094-243X
Country of Publication:
United States
Language:
English