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GRB 081008: From burst to afterglow and the transition phase in between

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dc.contributor.authorYuan, Fang
dc.contributor.authorSchady, P.
dc.contributor.authorRacusin, J. L.
dc.contributor.authorWillingale, R.
dc.contributor.authorKruhler, T.
dc.contributor.authorO'Brien, P. T.
dc.contributor.authorGreiner, J.
dc.contributor.authorOates, S. R.
dc.contributor.authorRykoff, E. S.
dc.contributor.authorAharonian, F.
dc.contributor.authorAkerlof, C. W.
dc.date.accessioned2015-12-10T22:58:06Z
dc.date.issued2010
dc.date.updated2016-02-24T10:07:44Z
dc.description.abstractWe present a multi-wavelength study of GRB 081008, at redshift 1.967, by Swift, ROTSE-III, and Gamma-Ray Burst Optical/NearInfrared Detector. Compared to other Swift GRBs, GRB 081008 has a typical gamma-ray isotropic equivalent energy output (∼1053 erg)
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/60695
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Gamma; Ray burst: individual (GRB 081008)
dc.titleGRB 081008: From burst to afterglow and the transition phase in between
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage880
local.bibliographicCitation.startpage870
local.contributor.affiliationYuan, Fang, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSchady, P, UCL Mullard Space Science Laboratory
local.contributor.affiliationRacusin, J L, Pennsylvania State University
local.contributor.affiliationWillingale, R., University of Leicester
local.contributor.affiliationKruhler, T, Max Planck Institut for Extraterrestrial Physics
local.contributor.affiliationO'Brien, P T, University of Leicester
local.contributor.affiliationGreiner, J, Max Planck Institut for Extraterrestrial Physics
local.contributor.affiliationOates, S R, UCL Mullard Space Science Laboratory
local.contributor.affiliationRykoff, E S, University of California
local.contributor.affiliationAharonian, F, Max-Planck-Institut fur Kernphysik
local.contributor.affiliationAkerlof, C W, University of Michigan
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.ariespublicationU3488905xPUB557
local.identifier.citationvolume711
local.identifier.doi10.1088/0004-637X/711/2/870
local.identifier.scopusID2-s2.0-77649212718
local.type.statusPublished Version

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