  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.

Astrophysics