Spectral properties of 438 GRBs Virtual Observatory Resource

Authors
  1. Nava L.
  2. Ghirlanda G.
  3. Ghisellini G.
  4. Celotti A.
  5. Published by
    CDS
Abstract

We present the results of the spectral analysis of the public data of 438 gamma ray bursts (GRBs) detected by the Fermi Gamma ray Burst Monitor (GBM) up to March 2010. For 432 bursts we could fit the time-integrated spectrum. In 318 cases we could reliably constrain the peak energy E^obs^_peak_ of their {nu}F{nu} spectrum by analyzing their time-integrated spectrum between 8keV and 35MeV. Eighty percent of these spectra are fitted by a power-law with an exponential cutoff, and the remaining with the Band function. Among these 318 GRBs, 274 belong to the long GRB class and 44 to the short.

Keywords
  1. gamma-ray-astronomy
  2. spectroscopy
Bibliographic source Bibcode
2011A&A...530A..21N
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/530/A21
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/530/A21
Document Object Identifer DOI
doi:10.26093/cds/vizier.35300021

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History

2012-11-08T14:54:41Z
Resource record created
2012-11-08T14:54:41Z
Created
2017-12-22T05:32:53Z
Updated

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