| タイトル | The Second SWIFT Burst Alert Telescope (BAT) Gamma-Ray Burst Catalog |
| 本文（外部サイト） | http://hdl.handle.net/2060/20120017376 |
| 著者（英） | Parsons, A. M.; Zhang, B.; Sato, G.; Gehrels, N.; Markwardt, C. B.; Stamatikos, M.; Barthelmy, S. D.; Tueller, J.; Ukwatta, T. N.; Sakamoto, T.; Palmer, D. M.; Krimm, H. A.; Fenimore, E. E.; Baumgartner, W. H.; Cummings, J. R. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2012-01-01 |
| 言語 | eng |
| 内容記述 | 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 (hereafter the BAT2 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. In the correlation study of various observed parameters extracted from the BAT prompt emission data, we distinguish among long-duration GRBs (L-GRBs), short-duration GRBs (S-GRBs), and short-duration GRBs with extended emission (S-GRBs with E.E.) to investigate differences in the prompt emission properties. The fraction of L-GRBs, S-GRBs and S-GRBs with E.E. in the catalog are 89%, 8% and 2% respectively. We compare the BAT prompt emission properties with the BATSE, BeppoSAX and HETE-2 GRB samples.. We also correlate the observed prompt emission properties with the redshifts for the GRBs with known redshift. The BAT T(sub 90) and T(sub 50) durations peak at 70 s and 30 s, respectively. We confirm that the spectra of the BAT S-GRBs are generally harder than those of the L-GRBs. |
| NASA分類 | Astrophysics |
| レポートNO | GSFC.JA.6653.2012 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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