Journal Article

The impact of selection biases on the <i>E</i><sub>peak</sub> –<i>L</i><sub>iso</sub> correlation of gamma-ray bursts

G. Ghirlanda, G. Ghisellini, L. Nava, R. Salvaterra, G. Tagliaferri, S. Campana, S. Covino, P. D’Avanzo, D. Fugazza, A. Melandri and S. D. Vergani

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 422, issue 3, pages 2553-2559
Published in print May 2012 | ISSN: 0035-8711
Published online May 2012 | e-ISSN: 1365-2966 | DOI:
The impact of selection biases on the Epeak –Liso correlation of gamma-ray bursts

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We study the possible effects of selection biases on the EpeakLiso correlation caused by the unavoidable presence of flux limits in the existing samples of gamma-ray bursts (GRBs). We consider a well-defined complete sample of Swift GRBs and perform Monte Carlo simulations of the GRB population under different assumptions for their luminosity functions. If we assume that there is no correlation between the peak energy Epeak and the isotropic luminosity Liso, we are unable to reproduce it due to the flux limit threshold of the Swift complete sample. We can reject the null hypothesis that there is no intrinsic correlation between Epeak and Liso at more than 2.7σ level of confidence. This result is robust against the assumptions of our simulations and it is confirmed if we consider, instead of Swift, the trigger threshold of the BATSE instrument. Therefore, there must be a physical relation between these two quantities. Our simulations seem to exclude, at a lower confidence level of 1.6σ, the possibility that the observed EpeakLiso correlation among different bursts is caused by a boundary, i.e. such that for any given Epeak, we see only the largest Liso, which has a flux above the threshold of the current instruments.

Keywords: radiation mechanisms: non-thermal; gamma-ray burst: general

Journal Article.  5733 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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