2011AIP conference proceedingsRequires access

Rest-frame statistics of 32 GBM-GRBs

D. Gruber, F. Olivares, A. Rau, A. von Kienlin, J. Greiner, J. E. McEnery, J. L. Racusin, N. Gehrels

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Abstract

For many years the peak energy and duration distributions of gamma‐ray bursts (GRBs) have been studied in the observer frame, which does not provide information about the intrinsic spectral properties of the event. In this paper, we study the sample of 32 GRBs that have measured redshift and were observed with the Fermi Gamma‐ray Burst Monitor (GBM) up to October 16th, 2010. We reconstruct their intrinsic spectral (Ep,rest) and temporal (T90,rest) properties.

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What this paper is about

For many years the peak energy and duration distributions of gamma‐ray bursts (GRBs) have been studied in the observer frame, which does not provide information about the intrinsic spectral properties of the event. In this paper, we study the sample of 32 GRBs that have measured redshift and were observed with the Fermi Gamma‐ray Burst Monitor (GBM) up to October 16th, 2010. We reconstruct their intrinsic spectral (Ep,rest) and temporal (T90,rest) properties.

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Available abstract

For many years the peak energy and duration distributions of gamma‐ray bursts (GRBs) have been studied in the observer frame, which does not provide information about the intrinsic spectral properties of the event. In this paper, we study the sample of 32 GRBs that have measured redshift and were observed with the Fermi Gamma‐ray Burst Monitor (GBM) up to October 16th, 2010. We reconstruct their intrinsic spectral (Ep,rest) and temporal (T90,rest) properties.

Key concepts: Rest frame, Rest (music), Gamma-ray burst, Redshift, Physics, Fermi Gamma-ray Space Telescope, Frame (networking), Astrophysics

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