Статья

THE <i>FERMI</i> GBM GAMMA-RAY BURST SPECTRAL CATALOG: FOUR YEARS OF DATA

David GruberMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, GermanyAdam GoldsteinUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USAVictoria Weller von AhlefeldMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, GermanyP. Narayana BhatUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USAElisabetta BissaldiDipartimento di Fisica, Universita' di Trieste, I-34127 Trieste, ItalyMichael S. BriggsUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USADave ByrneSchool of Physics, University College Dublin, Belfield, Stillorgan Road, Dublin 4, IrelandWilliam H. ClevelandUniversities Space Research Association, 320 Sparkman Drive, Huntsville, AL 35805, USAValerie ConnaughtonUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USARoland DiehlMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, GermanyGerald J. FishmanSpace Science Office, VP62, NASA/Marshall Space Flight Center, Huntsville, AL 35812, USAGerard FitzpatrickSchool of Physics, University College Dublin, Belfield, Stillorgan Road, Dublin 4, IrelandSuzanne FoleySchool of Physics, University College Dublin, Belfield, Stillorgan Road, Dublin 4, IrelandMelissa GibbyJacobs Technology, Inc., Huntsville, AL, USAMisty M. GilesJacobs Technology, Inc., Huntsville, AL, USAJochen GreinerMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, GermanySylvain GuiriecNASA Goddard Space Flight Center, Greenbelt, MD 20771, USAAlexander J. van der HorstAstronomical Institute, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The NetherlandsAndreas von KienlinMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, GermanyChryssa KouveliotouSpace Science Office, VP62, NASA/Marshall Space Flight Center, Huntsville, AL 35812, USAEmily LaydenUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USALin LinSabancıUniversity, Faculty of Engineering and Natural Sciences, Orhanlı–Tuzla, İstanbul 34956, TurkeyCharles A. MeeganUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USASinéad McGlynnSchool of Physics, University College Dublin, Belfield, Stillorgan Road, Dublin 4, IrelandWilliam S. PaciesasUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USAVèronique PelassaUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USARobert D. PreeceUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USAArne RauMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, GermanyColleen A. Wilson-HodgeSpace Science Office, VP62, NASA/Marshall Space Flight Center, Huntsville, AL 35812, USAShaolin XiongUniversity of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USAGeorge YounesUniversities Space Research Association, 320 Sparkman Drive, Huntsville, AL 35805, USAHoi-Fung YuMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, Germany

2014en

ABI

Аннотация

In this catalog we present the updated set of spectral analyses of gamma-ray bursts (GRBs) detected by the Fermi Gamma-Ray Burst Monitor during its first four years of operation. It contains two types of spectra, time-integrated spectral fits and spectral fits at the brightest time bin, from 943 triggered GRBs. Four different spectral models were fitted to the data, resulting in a compendium of more than 7500 spectra. The analysis was performed similarly but not identically to Goldstein et al. All 487 GRBs from the first two years have been re-fitted using the same methodology as that of the 456 GRBs in years three and four. We describe, in detail, our procedure and criteria for the analysis and present the results in the form of parameter distributions both for the observer-frame and rest-frame quantities. The data files containing the complete results are available from the High-Energy Astrophysics Science Archive Research Center.

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Идентификаторы

DOI: 10.1088/0067-0049/211/1/12

Цитирования и источники

Цитирований: 2Использованных источников: 0

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