Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/18792
Title: Anatomy of a dark burst - The afterglow of GRB 060108
Authors: Oates, S. R.
De Pasquale M.
Zane, S.
Blustin, A. J.
Page, M. J.
Mundell, C. G.
Monfardini, A.
Melandri, A.
Guidorzi, C.
Gomboc, A.
Carter, D.
Kobayashi, S.
Smith, R. J.
Steele, IA.
Piranomonte, S.
Page, KL.
Bannister, N.
O'Brien, PT.
Monfardini, A.
Malesani, D.
Gomboc, A.
Capalbi, M.
D'Avanzo, P.
Krimm, HA.
Tanvir, N.
First Published: 11-Oct-2006
Publisher: Royal Astronomical Society (RAS)
Citation: Monthly Notices of the Royal Astronomical Society, 2006, 372 (1), pp. 327-337
Abstract: 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.
DOI Link: 10.1111/j.1365-2966.2006.10866.x
ISSN: 0035-8711
eISSN: 1365-2966
Links: http://hdl.handle.net/2381/18792
http://mnras.oxfordjournals.org/content/372/1/327
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2006 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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