Hubble Space Telescope and Spitzer Observations of the Afterglow and Host Galaxy of GRB 050904 at z = 6.295
Gladders, M. D.; Cenko, S. B.; Peterson, B. A.; Price, P. A.; Berger, E.; Djorgovski, S. G.; Kulkarni, S. R.; Schmidt, B. P.; Chary, R.; Barger, A. J.; Cowie, L. L.; Fox, D. B.; McCarthy, P. J.; Soderberg, A. M.
United States, Australia
Abstract
We present deep Hubble Space Telescope (HST) and Spitzer Space Telescope observations of GRB 050904 at z=6.295. We detect the afterglow in the H band more than 3 weeks after the burst and confirm the presence of a jet break at t~2.1 days. This leads to an estimated opening angle of about 4° and a beaming-corrected energy of about 1051 ergs, similar to those of lower redshift gamma-ray bursts (GRBs). We do not detect an underlying host galaxy with either HST or Spitzer. From the upper limits we infer an extinction-corrected absolute magnitude MUV>~-20.3 mag, or L<~L*, a star formation rate of <~5.7 Msolar yr-1, and a stellar mass of <~few×109 Msolar. A comparison to spectroscopically confirmed galaxies at z>5.5 reveals that the host of GRB 050904 is fainter and has a lower star formation rate than at least 80% of these objects. Finally, using our luminosity limits, and the metallicity of about 0.05 Zsolar inferred from the afterglow absorption spectrum, we place the first limit on the luminosity-metallicity relation at z>6. Future afterglow and host galaxy observations of z>~4 GRBs should elucidate whether the mass- and luminosity-metallicity relations continue to evolve beyond the present limits of z<~2.