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Early ROTSE-III observations of GRB afterglows

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dc.contributor.authorPandey, S. B.
dc.contributor.authorAkerlof, C. W.
dc.contributor.authorZheng, W.
dc.contributor.authorYuan, Fang
dc.contributor.authorRykoff, E. S.
dc.contributor.authorMcKay, T. A.
dc.coverage.spatialAnnapolis USA
dc.date.accessioned2015-12-13T23:01:46Z
dc.date.createdNovember 1-4 2010
dc.date.issued2011
dc.date.updated2016-02-24T08:42:59Z
dc.description.abstractEarly observations of 15 GRB afterglows taken (2008-09) by ROTSE-III along with the published data of 26 others have been used to study the rising temporal nature seen at optical frequencies. A good fraction of early time temporal rising indices found to
dc.identifier.isbn9780735409163
dc.identifier.urihttp://hdl.handle.net/1885/84575
dc.publisherAmerican Institute of Physics (AIP)
dc.relation.ispartofseriesGamma Ray Bursts 2010
dc.sourceGamma Ray Bursts 2010
dc.source.urihttp://scitation.aip.org/content/aip/proceeding/aipcp/1358
dc.subjectKeywords: Afterglows; Gamma-ray bursts; Optical
dc.titleEarly ROTSE-III observations of GRB afterglows
dc.typeConference paper
local.bibliographicCitation.lastpage161
local.bibliographicCitation.startpage158
local.contributor.affiliationPandey, S B, University of Michigan
local.contributor.affiliationAkerlof, C W, University of Michigan
local.contributor.affiliationZheng, W., University of Michigan
local.contributor.affiliationYuan, Fang, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationRykoff, E S, University of California
local.contributor.affiliationMcKay, T A, University of California
local.contributor.authoruidYuan, Fang, u4981546
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020106 - High Energy Astrophysics; Cosmic Rays
local.identifier.ariespublicationf5625xPUB12859
local.identifier.doi10.1063/1.3621761
local.identifier.scopusID2-s2.0-80052428450
local.type.statusPublished Version

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