The host galaxies of Swift dark gamma-ray bursts: Observational constraints on highly obscured and very high redshift GRBs

D. A. Perley, S. B. Cenko, J. S. Bloom, H. W. Chen, Nathaniel Butler, D. Kocevski, J. X. Prochaska, M. Brodwin, K. Glazebrook, M. M. Kasliwal, S. R. Kulkarni, S. Lopez, E. O. Ofek, M. Pettini, A. M. Soderberg, D. Starr

Research output: Contribution to journalArticle

166 Citations (Scopus)

Abstract

In this work, we present the first results of our imaging campaign at Keck Observatory to identify the host galaxies of "dark" gamma-ray bursts (GRBs), events with no detected optical afterglow or with detected optical flux significantly fainter than expected from the observed X-ray afterglow. We find that out of a uniform sample of 29 Swiftbursts rapidly observed by the Palomar 60 inch telescope through 2008 March (14 of which we classify as dark), all events have either a detected optical afterglow, a probable optical host-galaxy detection, or both. Our results constrain the fraction of SwiftGRBs coming from very high redshift (z>7), such as the recent GRB 090423, to between 0.2% and 7% at 80% confidence. In contrast, a significant fraction of the sample requires large extinction columns (host-frame AV ≳ 1mag, with several events showing AV > 2-6mag), identifying dust extinction as the dominant cause of the dark GRB phenomenon. We infer that a significant fraction of GRBs (and, by association, of high-mass star formation) occurs in highly obscured regions. However, the host galaxies of dark GRBs seem to have normal optical colors, suggesting that the source of obscuring dust is local to the vicinity of the GRB progenitor or highly unevenly distributed within the host galaxy.

Original languageEnglish (US)
Pages (from-to)1690-1708
Number of pages19
JournalAstronomical Journal
Volume138
Issue number6
DOIs
StatePublished - 2009
Externally publishedYes

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gamma ray bursts
galaxies
afterglows
extinction
dust
observatory
star formation
confidence
observatories
telescopes
color
causes
x rays

Keywords

  • dust, extinction
  • galaxies: high-redshift
  • galaxies: photometry
  • gamma rays: bursts

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

The host galaxies of Swift dark gamma-ray bursts : Observational constraints on highly obscured and very high redshift GRBs. / Perley, D. A.; Cenko, S. B.; Bloom, J. S.; Chen, H. W.; Butler, Nathaniel; Kocevski, D.; Prochaska, J. X.; Brodwin, M.; Glazebrook, K.; Kasliwal, M. M.; Kulkarni, S. R.; Lopez, S.; Ofek, E. O.; Pettini, M.; Soderberg, A. M.; Starr, D.

In: Astronomical Journal, Vol. 138, No. 6, 2009, p. 1690-1708.

Research output: Contribution to journalArticle

Perley, DA, Cenko, SB, Bloom, JS, Chen, HW, Butler, N, Kocevski, D, Prochaska, JX, Brodwin, M, Glazebrook, K, Kasliwal, MM, Kulkarni, SR, Lopez, S, Ofek, EO, Pettini, M, Soderberg, AM & Starr, D 2009, 'The host galaxies of Swift dark gamma-ray bursts: Observational constraints on highly obscured and very high redshift GRBs', Astronomical Journal, vol. 138, no. 6, pp. 1690-1708. https://doi.org/10.1088/0004-6256/138/6/1690
Perley, D. A. ; Cenko, S. B. ; Bloom, J. S. ; Chen, H. W. ; Butler, Nathaniel ; Kocevski, D. ; Prochaska, J. X. ; Brodwin, M. ; Glazebrook, K. ; Kasliwal, M. M. ; Kulkarni, S. R. ; Lopez, S. ; Ofek, E. O. ; Pettini, M. ; Soderberg, A. M. ; Starr, D. / The host galaxies of Swift dark gamma-ray bursts : Observational constraints on highly obscured and very high redshift GRBs. In: Astronomical Journal. 2009 ; Vol. 138, No. 6. pp. 1690-1708.
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AU - Perley, D. A.

AU - Cenko, S. B.

AU - Bloom, J. S.

AU - Chen, H. W.

AU - Butler, Nathaniel

AU - Kocevski, D.

AU - Prochaska, J. X.

AU - Brodwin, M.

AU - Glazebrook, K.

AU - Kasliwal, M. M.

AU - Kulkarni, S. R.

AU - Lopez, S.

AU - Ofek, E. O.

AU - Pettini, M.

AU - Soderberg, A. M.

AU - Starr, D.

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