Gamma-ray burst afterglows : luminosity clustering at infrared wavelengths?
B. Gendre (1), S. Pelisson (1), M. Boer (2), S. Basa (1), A. Mazure, ((1) LAM/CNRS/Universite de Provence, (2) OHP/CNRS)

TL;DR
This study investigates whether gamma-ray burst afterglows exhibit luminosity clustering in near-infrared wavelengths, confirming previous optical and X-ray findings and providing constraints on the fireball's total energy.
Contribution
It demonstrates the presence of luminosity clustering in near-infrared afterglows, extending prior optical and X-ray results and refining fireball energy estimates.
Findings
Luminosity clustering confirmed in near-infrared wavelengths.
Clustering similar to optical and X-ray observations.
Constraints set on the total energy of the fireball.
Abstract
Clustering in the luminosity of the afterglows of gamma-ray burst has been reported in the optical and X-ray. We investigate the possibility that a clustering in the luminosity of the afterglows of gamma-ray burst exists in near infrared (J, H, K bands). We use observations of events occurring from 1997 to the end of 2007. We correct the gamma-ray burst afterglow light curve for distance effect and time dilation, and replace all light curves to a common distance of z=1. We used only observations of signal emitted in the near infrared (in the burst frame). We observe a clustering identical to the one observed in optical and similar to the one observed in X-ray. We thus confirm the previous works made in optical. We set a constraint on the total energy of the fireball.
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