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

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

9 pages, 3 figures. Accepted in ApJL

Scientific paper

10.1086/501048

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.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Detection of a very bright optical flare from a gamma-ray burst at redshift 6.29 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Detection of a very bright optical flare from a gamma-ray burst at redshift 6.29, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of a very bright optical flare from a gamma-ray burst at redshift 6.29 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-469576

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.