Fermi/GBM and BATSE Gamma-Ray Bursts: comparison of the spectral properties
Lara Nava, Giancarlo Ghirlanda, Gabriele Ghisellini, Annalisa, Celotti

TL;DR
This study compares the spectral properties of gamma-ray bursts detected by Fermi/GBM and BATSE, revealing similarities and differences in their spectral distributions and confirming certain correlations are not due to instrumental biases.
Contribution
It provides a comprehensive comparison of GBM and BATSE GRB spectral properties, extending known correlations and analyzing the presence of outliers with improved energy range coverage.
Findings
GBM and BATSE long bursts have similar fluence, Epeak, and peak flux distributions.
GBM bursts have a slightly harder low-energy spectral index than BATSE bursts.
GBM confirms that Epeak-Fluence and Epeak-P correlations are not due to selection effects.
Abstract
The Gamma-ray Burst Monitor (GBM) on board Fermi allows to study the spectra of Gamma Ray Bursts (GRBs) over an unprecedented wide energy range (8 keV - 35 MeV). We compare the spectral properties of short and long GRBs detected by the GBM (up to March 2010) with those of GRBs detected by the BATSE instrument on board the CGRO. GBM and BATSE long bursts have similar distributions of fluence (F), Epeak and peak flux (P) but GBM bursts have a slightly harder low-energy spectral index \alpha with respect to BATSE GRBs. GBM and BATSE short bursts have similar distributions of fluence, \alpha and peak flux, with GBM bursts having slightly larger Epeak. We discuss these properties in light of the found correlations between Epeak and the fluence and the peak flux. GBM bursts confirm that these correlations are not determined by instrumental selection effects. Indeed, GBM bursts extend the…
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