THE THIRD SWIFT BURST ALERT TELESCOPE GAMMA-RAY BURST CATALOG

被引:216
作者
Lien, Amy [1 ,2 ,3 ]
Sakamoto, Takanori [4 ]
Barthelmy, Scott D. [5 ]
Baumgartner, Wayne H. [1 ,2 ,3 ]
Cannizzo, John K. [1 ,2 ,3 ]
Chen, Kevin [6 ]
Collins, Nicholas R. [1 ,2 ,3 ]
Cummings, Jay R. [5 ]
Gehrels, Neil [5 ]
Krimm, Hans A. [1 ,2 ,7 ]
Markwardt, Craig. B. [5 ]
Palmer, David M. [8 ]
Stamatikos, Michael [9 ,10 ]
Troja, Eleonora [1 ,2 ,11 ,12 ]
Ukwatta, T. N. [8 ]
机构
[1] CRESST, Greenbelt, MD 20771 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Univ Maryland Baltimore Cty, Dept Phys, 1000 Hilltop Circle, Baltimore, MD 21250 USA
[4] Aoyama Gakuin Univ, Coll Sci & Engn, Dept Math & Phys, Chuo Ku, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 2525258, Japan
[5] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[6] Univ Calif Berkeley, Dept Phys, 366 LeConte Hall MC 7300, Berkeley, CA USA
[7] Univ Space Res Assoc, 10211 Wincopin Circle,Suite 500, Columbia, MD 21044 USA
[8] Loa Alamos Natl Lab, Space & Remote Sensing ISR 2, Los Alamos, NM 87544 USA
[9] Ohio State Univ, Dept Astron, Dept Phys, Columbus, OH 43210 USA
[10] Ohio State Univ, Ctr Cosmol & AstroParticle Phys, Columbus, OH 43210 USA
[11] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[12] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
关键词
gamma-ray burst: general; HARD X-RAY; COMPREHENSIVE ANALYSIS; LUMINOSITY FUNCTION; EXTENDED EMISSION; COMPLETE SAMPLE; TIME DILATION; GRB; 130925A; BAT; SPECTRA; PROMPT;
D O I
10.3847/0004-637X/829/1/7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
To date, the Burst Alert Telescope (BAT) onboard Swift has detected similar to 1000 gamma-ray bursts (GRBs), of which similar to 360 GRBs have redshift measurements, ranging from z = 0.03 to z = 9.38. We present the analyses of the BAT-detected GRBs for the past similar to 11 years up through GRB 151027B. We report summaries of both the temporal and spectral analyses of the GRB characteristics using event data (i.e., data for each photon within approximately 250 s before and 950 s after the BAT trigger time), and discuss the instrumental sensitivity and selection effects of GRB detections. We also explore the GRB properties with redshift when possible. The result summaries and data products are available at http://swift.gsfc.nasa.gov/results/batgrbcat/index.html. In addition, we perform searches for GRB emissions before or after the event data using the BAT survey data. We estimate the false detection rate to be only one false detection in this sample. There are 15 ultra-long GRBs (similar to 2% of the BAT GRBs) in this search with confirmed emission beyond similar to 1000 s of event data, and only two GRBs (GRB 100316D and GRB 101024A) with detections in the survey data prior to the starting of event data.
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页数:47
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