Journal Article

The extreme, red afterglow of GRB 060923A: distance or dust?

N. R. Tanvir, A. J. Levan, E. Rol, R. L. C. Starling, J. Gorosabel, R. S. Priddey, D. Malesani, P. Jakobsson, P. T. O'Brien, A. O. Jaunsen, J. Hjorth, J. P. U. Fynbo, A. Melandri, A. Gomboc, B. Milvang-Jensen, A. S. Fruchter, M. Jarvis, C. A. C. Fernandes and T. Wold

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 388, issue 4, pages 1743-1750
Published in print August 2008 | ISSN: 0035-8711
Published online August 2008 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2008.13496.x
The extreme, red afterglow of GRB 060923A: distance or dust?

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Gamma-ray bursts (GRBs) are powerful probes of the early Universe, but locating and identifying very distant GRBs remain challenging. We report here the discovery of the K-band afterglow of Swift GRB 060923A, imaged within the first hour post-burst, and the faintest so far found. It was not detected in any bluer bands to deep limits, making it a candidate very high-z burst (z≳ 11). However, our later-time optical imaging and spectroscopy reveal a faint galaxy coincident with the GRB position which, if it is the host, implies a more moderate redshift (most likely z≲ 2.8) and therefore that dust is the likely cause of the very red-afterglow colour. This being the case, it is one of the few instances so far found of a GRB afterglow with high-dust extinction.

Keywords: galaxies: high-redshift; gamma-rays: bursts

Journal Article.  5922 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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