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 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.
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15 October 2010
DECIPHERING THE ANCIENT UNIVERSE WITH GAMMA‐RAY BURSTS
19–23 April 2010
Terrsa, Kyoto, (Japan)
Research Article|
October 15 2010
BAT2 GRB Catalog—Prompt Emission Properties of Swift GRBs—
T. Sakamoto;
T. Sakamoto
aCRESST and NASA Goddard Space Flight Center, Greenbelt, MD 20771
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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S. Barthelmy;
S. Barthelmy
cNASA Goddard Space Flight Center, Greenbelt, MD 20771
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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W. Baumgartner;
W. Baumgartner
aCRESST and NASA Goddard Space Flight Center, Greenbelt, MD 20771
bCenter for Space Science and Technology, University of Maryand, Baltimore County, Baltimore, MD 21250
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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J. Cummings;
J. Cummings
aCRESST and NASA Goddard Space Flight Center, Greenbelt, MD 20771
bCenter for Space Science and Technology, University of Maryand, Baltimore County, Baltimore, MD 21250
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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E. Fenimore;
E. Fenimore
dLos Alamos National Laboratory, P.O. Box 1663, Los Alamos, NM, 87545
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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N. Gehrels;
N. Gehrels
cNASA Goddard Space Flight Center, Greenbelt, MD 20771
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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H. Krimm;
H. Krimm
aCRESST and NASA Goddard Space Flight Center, Greenbelt, MD 20771
eUniversities Space Research Association, 10211 Wincopin Circle, Suite 500, Columbia, MD 21044‐3432
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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C. Markwardt;
C. Markwardt
aCRESST and NASA Goddard Space Flight Center, Greenbelt, MD 20771
fDepartment of Astronomy, University of Maryland, College Park, MD 20742
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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D. Palmer;
D. Palmer
dLos Alamos National Laboratory, P.O. Box 1663, Los Alamos, NM, 87545
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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A. Parsons;
A. Parsons
cNASA Goddard Space Flight Center, Greenbelt, MD 20771
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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G. Sato;
G. Sato
fDepartment of Astronomy, University of Maryland, College Park, MD 20742
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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M. Stamatikos;
M. Stamatikos
hCenter for Cosmology and Astro‐Particle Physics, Department of Physics, The Ohio State University, 191 West Woodruff Avenue, Columbus, OH 43210
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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J. Tueller;
J. Tueller
cNASA Goddard Space Flight Center, Greenbelt, MD 20771
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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T. Ukwatta
T. Ukwatta
iCenter for Nuclear Studies, Department of Physics, The George Washington University, Washington, D.C. 20052
gInstitute of Space and Astronautical Science, JAXA, Kanagawa 229‐8510, Japan
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AIP Conf. Proc. 1279, 20–23 (2010)
Citation
T. Sakamoto, S. Barthelmy, W. Baumgartner, J. Cummings, E. Fenimore, N. Gehrels, H. Krimm, C. Markwardt, D. Palmer, A. Parsons, G. Sato, M. Stamatikos, J. Tueller, T. Ukwatta; BAT2 GRB Catalog—Prompt Emission Properties of Swift GRBs—. AIP Conf. Proc. 15 October 2010; 1279 (1): 20–23. https://doi.org/10.1063/1.3509266
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