GRB071028B, a burst behind large amounts of dust in an unabsorbed galaxy

Abstract

Aims. We report on the discovery and properties of the fading afterglow and underlying host galaxy of GRB071028B, thereby facilitating a detailed comparison between these two. Methods. Observations were performed with the Gamma-ray Burst Optical and Near-infrared Detector at the 2.2 m telescope on the La Silla Paranal Observatory in Chile. We conducted five observations from 1.9 d to 227.2 d after the trigger and obtained deep images in the g′r′i′z′ and JHKs bands. Results. Based on accurate seven-channel photometry covering the optical to near-infrared wavelength range, we derive a photometric redshift of z = 0.94 +0.05-0.10 for the unabsorbed host galaxy of GRB071028B. In contrast, we show that the afterglow with an intrinsic extinction of A SBV = (0.70±0.11) mag is moderately absorbed and requires a relatively flat extinction curve. According to the reported Swift/BAT observations, the energetics yield an isotropic energy release of E resty,iso = 1.4+2.4-0.7)× 1051 erg. © 2011 ESO.