Abstract
We report the discovery of the optical and radio afterglow of GRB 010921, the first gamma-ray burst afterglow to be found from a localization by the High Energy Transient Explorer satellite. We present optical spectroscopy of the host galaxy, which we find to be a dusty and apparently normal star-forming galaxy at z = 0.451. The unusually steep optical spectral slope of the afterglow can be explained by heavy extinction, Av > 0.5 mag, along the line of sight to the GRB. Dust with similar Av for the host galaxy as a whole appears to be required by the measurement of a Balmer decrement in the spectrum of the host galaxy.
| Original language | English |
|---|---|
| Pages (from-to) | L121-L125 |
| Journal | Astrophysical Journal |
| Volume | 571 |
| Issue number | 2 II |
| DOIs | |
| Publication status | Published - 1 Jun 2002 |
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