Spectral evolution of GRBs observed with BeppoSAX WFCs and GRBM
arXiv:0909.3451
Abstract
We present some preliminary results obtained from a systematic analysis of almost all GRBs simultaneously observed with the Gamma Ray Burst Monitor and the Wide Field Cameras aboard the BeppoSAX satellite.
10 pages, 7 figures, paper presented at the Conference "Neutron Stars and gamma-ray Bursts", 30 March - 4 April, Cairo & Alexandria; to be published in AIP procs (on-line only) and in ASR
References in corpus (10)
- Intrinsic spectra and energetics of BeppoSAX Gamma-Ray Bursts with known redshifts
- GRB Formation Rates inferred from the Spectral Peak Energy - Luminosity Relation
- Measuring the cosmological parameters with the Ep,i-Eiso correlation of Gamma-Ray Bursts
- A Complete Catalog of Swift GRB Spectra and Durations: Demise of a Physical Origin for Pre-Swift High-Energy Correlations
- Quasi-blackbody component and radiative efficiency of the prompt emission of gamma-ray bursts
- Testing the Gamma-Ray Burst Energy Relationships
- Peak energy of the prompt emission of long Gamma Ray Bursts vs their fluence and peak flux
- Generalized Tests for Selection Effects in GRB High-Energy Correlations
- Probing the existence of the E_peak-E_iso correlation in long Gamma Ray Bursts
- Selection effects on GRB spectral-energy correlations