von Kienlin, Andreas 2014 Fermi GBM四年的catalog

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Title:		The 2nd Fermi GBM Gamma-Ray Burst Catalog: The First Four Years
Authors:		von Kienlin, Andreas; Meegan, Charles A.; Paciesas, William S.; Bhat, P. N.; Bissaldi, Elisabetta; Briggs, Michael S.; Burgess, J. Michael; Byrne, David; Chaplin, Vandiver; Cleveland, William; Connaughton, Valerie; Collazzi, Andrew C.; Fitzpatrick, Gerard; Foley, Suzanne; Gibby, Melissa; Giles, Misty; Goldstein, Adam; Greiner, Jochen; Gruber, David; Guiriec, Sylvain; van der Horst, Alexander J.; Kouveliotou, Chryssa; Layden, Emily; McBreen, Sheila; McGlynn, Sinead; Pelassa, Veronique; Preece, Robert D.; Rau, Arne; Tierney, Dave; Wilson-Hodge, Colleen A.; Xiong, Shaolin; Younes, George; Yu, Hoi-Fung
Publication:		eprint arXiv:1401.5080
Publication Date:		01/2014
Origin:		ARXIV
Keywords:		Astrophysics - High Energy Astrophysical Phenomena
Comment:		151 pages, 10 figures, 9 tables; to be published in ApJS
Bibliographic Code:		2014arXiv1401.5080V

Abstract

This is the second of a series of catalogs of gamma-ray bursts (GRBs) observed with the Fermi Gamma-ray Burst Monitor (GBM). It extends the first two-year catalog by two more years, resulting in an overall list of 953 GBM triggered GRBs. The intention of the GBM GRB catalog is to provide information to the community on the most important observables of the GBM detected GRBs. For each GRB the location and main characteristics of the prompt emission, the duration, peak flux and fluence are derived. The latter two quantities are calculated for the 50 - 300 keV energy band, where the maximum energy release of GRBs in the instrument reference system is observed and also for a broader energy band from 10 - 1000 keV, exploiting the full energy range of GBMs low-energy detectors. Furthermore, information is given on the settings and modifications of the triggering criteria and exceptional operational conditions during years three and four in the mission. This second catalog is an official product of the Fermi GBM science team, and the data files containing the complete results are available from the High-Energy Astrophysics Science Archive Research Center (HEASARC).

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