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Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z = 3.2 gamma-ray burst

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dc.contributor.authorThone, C. C.
dc.contributor.authorKann, D. A.
dc.contributor.authorJohannesson, G.
dc.contributor.authorSelj, J. H.
dc.contributor.authorJaunsen, A. O.
dc.contributor.authorFynbo, J. P. U.
dc.contributor.authorAkerlof, C. W.
dc.contributor.authorBaliyan, K. S.
dc.contributor.authorFruchter, A. S.
dc.contributor.authorIbrahimov, Mansur
dc.contributor.authorYuan, Fang
dc.contributor.authorGraham, J. F.
dc.date.accessioned2015-12-13T22:45:02Z
dc.date.issued2010
dc.date.updated2016-02-24T09:38:42Z
dc.description.abstractAims: With this paper we want to investigate the highly variable afterglow light curve and environment of gamma-ray burst (GRB) 060526 at z = 3.221. Methods: We present one of the largest photometric datasets ever obtained for a GRB afterglow, consisting
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/79575
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Absorption lines; Analytical model; Broad bands; Broken power law; Central engines; Column density; Curve-of-growth; Data points; Data sets; Energy distributions; Energy injection; Galaxies:high-redshift; Gamma ray bursts; gamma rays bursts: individual: G galaxies: high-redshift; gamma rays bursts: individual: GRB 060526; ISM: abundances
dc.titlePhotometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z = 3.2 gamma-ray burst
dc.typeJournal article
local.bibliographicCitation.issue5
local.bibliographicCitation.startpageA70
local.contributor.affiliationThone, C C, University of Copenhagen
local.contributor.affiliationKann, D A, Thuringer Landessternwarte Tautenburg
local.contributor.affiliationJohannesson, G, University of Iceland
local.contributor.affiliationSelj, J H, University of Oslo
local.contributor.affiliationJaunsen, A O, University of Oslo
local.contributor.affiliationFynbo, J. P. U, University of Copenhagen
local.contributor.affiliationAkerlof, C W, University of Michigan
local.contributor.affiliationBaliyan, K S, Physical Research Laboratory
local.contributor.affiliationFruchter, A S, Space Telescope Science Institute
local.contributor.affiliationIbrahimov, Mansur, Ulugh Beg Astronomical Institute
local.contributor.affiliationYuan, Fang, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationGraham, J F, Space Telescope Science Institute
local.contributor.authoruidYuan, Fang, u4981546
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020106 - High Energy Astrophysics; Cosmic Rays
local.identifier.ariespublicationf5625xPUB7986
local.identifier.citationvolume523
local.identifier.doi10.1051/0004-6361/200810340
local.identifier.scopusID2-s2.0-78549243755
local.type.statusPublished Version

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