Outshining the quasars at reionisation: The X-ray spectrum and lightcurve of the redshift 6.29 Gamma-Ray Burst GRB050904

Details Outshining the quasars at reionisation: The X-ray spectrum and lightcurve of the redshift 6.29 Gamma-Ray Burst GRB050904 Outshining the quasars at reionisation: The X-ray spectrum and lightcurve of the redshift 6.29 Gamma-Ray Burst GRB050904

2005-09-21

arxiv.org/abs/astro-ph/0509640v3

Astrophys.J. 637 (2006) L69-L72

Astronomy and Astrophysics

Astrophysics

Accepted for publication in ApJL. 5 pages with emulateapj, 3 figures

Scientific paper

10.1086/501004

Gamma-ray burst (GRB) 050904 is the most distant X-ray source known, at z=6.295, comparable to the farthest AGN and galaxies. Its X-ray flux decays, but not as a power-law; it is dominated by large variability from a few minutes to at least half a day. The spectra soften from a power-law with photon index Gamma=1.2 to 1.9, and are well-fit by an absorbed power-law with possible evidence of large intrinsic absorption. There is no evidence for discrete features, in spite of the high signal-to-noise ratio. In the days after the burst, GRB 050904 was by far the brightest known X-ray source at z>4. In the first minutes after the burst, the flux was >10^{-9} erg cm^-2 s^-1 in the 0.2-10keV band, corresponding to an apparent luminosity >10^5 times larger than the brightest AGN at these distances. More photons were acquired in a few minutes with Swift-XRT than XMM-Newton and Chandra obtained in ~300 ks of pointed observations of z>5 AGN. This observation is a clear demonstration of concept for efficient X-ray studies of the high-z IGM with large area, high-resolution X-ray detectors, and shows that early-phase GRBs are the only backlighting bright enough for X-ray absorption studies of the IGM at high redshift.

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