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J/ApJS/199/18 The Fermi GBM catalog (Paciesas+, 2012)
The following files can be converted to FITS (extension .fit or fit.gz)
table1.dat table2.dat table3.dat table[45].dat
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-r--r--r-- 1 cats archive 2574 Mar 23 2012 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
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-r--r--r-- 1 cats archive 37144 Mar 23 2012 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html]
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Beginning of ReadMe :J/ApJS/199/18 The Fermi GBM catalog (Paciesas+, 2012)
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The Fermi GBM Gamma-Ray Burst catalog: the first two years.
Paciesas W.S., Meegan C.A., von Kienlin A., Bhat P.N., Bissaldi E.,
Briggs M.S., Burgess J.M., Chaplin V., Connaughton V., Diehl R.,
Fishman G.J., Fitzpatrick G., Foley S., Gibby M., Giles M., Goldstein A.,
Greiner J., Gruber D., Guiriec S., van der Horst A.J., Kippen R.M.,
Kouveliotou C., Lichti G., Lin L., McBreen S., Preece R.D., Rau A.,
Tierney D., Wilson-Hodge C.
<Astrophys. J. Suppl. Ser., 199, 18 (2012)>
=2012ApJS..199...18P
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ADC_Keywords: Gamma rays ; Surveys
Mission_Name: Fermi
Keywords: catalogs - gamma-ray burst: general
Abstract:
The Fermi Gamma-ray Burst Monitor (GBM) is designed to enhance the
scientific return from Fermi in studying gamma-ray bursts (GRBs). In
its first two years of operation GBM triggered on 491 GRBs. We
summarize the criteria used for triggering and quantify the general
characteristics of the triggered GRBs, including their locations,
durations, peak flux, and fluence. This 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.
Description:
The Fermi Gamma-ray Space Telescope was launched on 2008 June 11 on a
mission to study the universe at high energies. The onboard Gamma-ray
Burst Monitor (GBM) trigger system for detecting GRBs was first
enabled on 2008 July 12. In this paper, we provide a catalog of GRBs
that triggered the GBM during its first two years of operation. During
this time the instrument burst detection algorithms were triggered 908
times: 492 of these are classified as GRBs, 79 as terrestrial
gamma-ray flashes (TGFs), 170 as soft gamma-ray repeaters (SGRs), 31
as solar flares, 61 as charged particles, and 75 as others (galactic
sources, accidental statistical fluctuations, or too weak to
classify). Of the 491 GRBs (in one case the same GRB triggered GBM
twice), 18 were detected by the LAT with high confidence above 100MeV
(A. Abdo et al. 2012ApJ...744..146A).