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The impact of selection biases on the Epeak-LISO correlation of gamma-ray bursts
Ghirlanda G., Ghisellini G., Nava L., Salvaterra R., Tagliaferri G. et al
Monthly Notices of the Royal Astronomical Society 422 (2012) 2553-2559 - http://hal.archives-ouvertes.fr/hal-00719738
Physique/Astrophysique/Phénomènes cosmiques de haute energie
Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie
The impact of selection biases on the Epeak-LISO correlation of gamma-ray bursts
G. Ghirlanda1, G. Ghisellini1, L. Nava2, R. Salvaterra3, G. Tagliaferri1, S. Campana1, S. Covino1, P. D'Avanzo1, D. Fugazza1, A. Melandri1, S. D. Vergani1
1 :  INAF/OAB - Osservatorio Astronomico di Brera
INAF
Italie
2 :  APC - UMR 7164 - AstroParticule et Cosmologie
http://www.apc.univ-paris7.fr/
CNRS : UMR7164 – IN2P3 – Observatoire de Paris – Université Paris VII - Paris Diderot – CEA : DSM/IRFU
APC - UMR 7164, Université Paris Diderot, 10 rue Alice Domon et Léonie Duquet, case postale 7020, F-75205 Paris Cedex 13
France
3 :  INAF-IASF Milano
INAF
Italie
APC - AHE
We study the possible effects of selection biases on the Epeak-LISO 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 Epeak-Liso 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.
Anglais

Monthly Notices of the Royal Astronomical Society
Publisher Oxford University Press (OUP): Policy P - Oxford Open Option A
ISSN 0035-8711 (eISSN : 1365-8711)
internationale
Articles dans des revues avec comité de lecture
05/2012
422
2553-2559

radiation mechanisms: non-thermal – gamma-ray burst: general

Lien vers le texte intégral : 
http://fr.arXiv.org/abs/1203.0003