Detection of a very bright optical flare from a gamma-ray burst at redshift 6.29

Michel Boër (1) , J.L. Atteia (2) , Y. Damerdji (1, 3) , B. Gendre (4) , A. Klotz (1, 3) , G. Stratta (3)

1 OHP - Observatoire de Haute-Provence
2 LATT - Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées
3 CESR - Centre d'étude spatiale des rayonnements
4 IASF-Roma - Istituto di Astrofisica Spaziale e Fisica cosmica - Roma

In this letter we discuss the flux and the behavior of the bright optical flare emission detected by the 25 cm TAROT robotic telescope during the prompt high-energy emission and the early afterglow. We combine our data with simultaneous observations performed in X-rays and we analyze the broad-band spectrum. These observations lead us to emphasize the similarity of GRB 050904 with GRB 990123, a remarkable gamma-ray burst whose optical emission reached 9th magnitude. While GRB 990123 was, until now, considered as a unique event, this observation suggests the existence of a population of GRBs which have very large isotropic equivalent energies and extremely bright optical counterparts. The luminosity of these GRBs is such that they are easily detectable through the entire universe. Since we can detect them to very high redshift even with small aperture telescopes like TAROT, they will constitute powerful tools for the exploration of the high-redshift Universe and might be used to probe the first generation of stars.

Mots clés: gamma-ray bursts; cosmology

Domaines: Cosmologie et astrophysique extra-galactique [astro-ph.CO]; Astrophysique [astro-ph]

Michel Boër, J.L. Atteia, Y. Damerdji, B. Gendre, A. Klotz, et al.. Detection of a very bright optical flare from a gamma-ray burst at redshift 6.29. 2006. ⟨hal-00011202v2⟩