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Anatomy of a dark burst - The afterglow of GRB 060108

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posted on 2012-10-24, 09:06 authored by S. R. Oates, De Pasquale M., S. Zane, A. J. Blustin, M. J. Page, C. G. Mundell, A. Monfardini, A. Melandri, C. Guidorzi, A. Gomboc, D. Carter, S. Kobayashi, R. J. Smith, IA. Steele, S. Piranomonte, KL. Page, N. Bannister, PT. O'Brien, D. Malesani, M. Capalbi, P. D'Avanzo, HA. Krimm, N. Tanvir
We present a multiwavelength study of GRB 060108 – the 100th gamma-ray burst discovered by Swift. The X-ray flux and light curve (three segments plus a flare) detected with the X-ray Telescope are typical of Swift long bursts. We report the discovery of a faint optical afterglow detected in deep BVRi′-band imaging obtained with the Faulkes Telescope North beginning 2.75 min after the burst. The afterglow is below the detection limit of the Ultraviolet/Optical Telescope within 100 s of the burst, while is evident in K-band images taken with the United Kingdom Infrared Telescope 45 min after the burst. The optical light curve is sparsely sampled. Observations taken in the R and i′ bands can be fitted either with a single power-law decay in flux, F(t) ∝t−α where α= 0.43 ± 0.08, or with a two-segment light curve with an initial steep decay α1 < 0.88 ± 0.2, flattening to a slope α2∼ 0.31 ± 0.12. A marginal evidence for rebrightening is seen in the i′ band. Deep R-band imaging obtained ∼12 d post-burst with the Very Large Telescope reveals a faint, extended object (R∼ 23.5 mag) at the location of the afterglow. Although the brightness is compatible with the extrapolation of the slow decay with index α2, significant flux is likely due to a host galaxy. This implies that the optical light curve had a break before 12 d, akin to what observed in the X-rays. We derive the maximum photometric redshift z < 3.2 for GRB 060108. We find that the spectral energy distribution at 1000 s after the burst, from the optical to the X-ray range, is best fitted by a simple power law, Fν∝ν−β, with βOX= 0.54 and a small amount of extinction. The optical to X-ray spectral index (βOX) confirms GRB 060108 to be one of the optically darkest bursts detected. Our observations rule out a high redshift as the reason for the optical faintness of GRB 060108. We conclude that a more likely explanation is a combination of an intrinsic optical faintness of the burst, a hard optical to X-ray spectrum and a moderate amount of extinction in the host galaxy.

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Citation

Monthly Notices of the Royal Astronomical Society, 2006, 372 (1), pp. 327-337

Version

  • VoR (Version of Record)

Published in

Monthly Notices of the Royal Astronomical Society

Publisher

Royal Astronomical Society (RAS)

issn

0035-8711

eissn

1365-2966

Copyright date

2006

Available date

2012-10-24

Publisher version

http://mnras.oxfordjournals.org/content/372/1/327

Language

en

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