The Metallicity and Dust Content of a Redshift 5 Gamma-Ray Burst Host Galaxy

Observations of the afterglows of long gamma-ray bursts (GRBs) allow the study of star-forming galaxies across most of cosmic history. Here we present observations of GRB 111008A, from which we can measure metallicity, chemical abundance patterns, dust-to-metals ratio (DTM), and extinction of the GRB host galaxy at z = 5.0. The host absorption system is a damped Lyalpha absorber with a very large neutral hydrogen column density of log N({H,{scriptsize {I}}})/cm^{-2}=22.30+/- 0.06 and a metallicity of [S/H] = -1.70 0.10. It is the highest-redshift GRB with such a precise metallicity measurement. The presence of fine-structure lines confirms the z = 5.0 system as the GRB host galaxy and makes this the highest redshift where Fe II fine-structure lines have been detected. The afterglow is mildly reddened with A<SUB>V</SUB> = 0.11 0.04 mag, and the host galaxy has a DTM that is consistent with being equal to or lower than typical values in the Local Group. Based on observations carried out under ESO program ID 088.A-0051(B) and 091.A-0703(A).