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A statistical comparison of the optical/UV and X-ray afterglows of gamma-ray bursts using the Swift Ultraviolet Optical and X-ray Telescopes

dc.contributor.authorChester, M. M.
dc.contributor.authorOates, S. R.
dc.contributor.authorPage, M. J.
dc.contributor.authorSchady, P.
dc.contributor.authorDE PASQUALE, Massımılıano
dc.contributor.authorEvans, P. A.
dc.contributor.authorPage, K. L.
dc.contributor.authorSiegel, M. H.
dc.contributor.authorZane, S.
dc.contributor.authorNousek, J. A.
dc.contributor.authorRoming, P. W. A.
dc.contributor.authorKuin, N. P. M.
dc.contributor.authorKoch, T. S.
dc.contributor.authorCurran, P. A.
dc.date.accessioned2022-02-18T09:33:52Z
dc.date.available2022-02-18T09:33:52Z
dc.date.issued2011
dc.identifier.citationOates S. R. , Page M. J. , Schady P., DE PASQUALE M., Evans P. A. , Page K. L. , Chester M. M. , Curran P. A. , Koch T. S. , Kuin N. P. M. , et al., "A statistical comparison of the optical/UV and X-ray afterglows of gamma-ray bursts using the Swift Ultraviolet Optical and X-ray Telescopes", MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.412, sa.1, ss.561-579, 2011
dc.identifier.issn0035-8711
dc.identifier.othervv_1032021
dc.identifier.otherav_467b7e70-5ca2-4417-83c0-180062687985
dc.identifier.urihttp://hdl.handle.net/20.500.12627/177451
dc.identifier.urihttps://doi.org/10.1111/j.1365-2966.2010.17928.x
dc.description.abstractWe present the systematic analysis of the Ultraviolet/Optical Telescope (UVOT) and X-ray Telescope (XRT) light curves for a sample of 26 Swift gamma-ray bursts (GRBs). By comparing the optical/UV and X-ray light curves, we found that they are remarkably different during the first 500 s after the Burst Alert Telescope trigger, while they become more similar during the middle phase of the afterglow, i.e. between 2000 and 20 000 s.
dc.language.isoeng
dc.subjectPhysics and Astronomy (miscellaneous)
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectGeneral Physics and Astronomy
dc.subjectSpace and Planetary Science
dc.subjectAstronomy and Astrophysics
dc.subjectPhysical Sciences
dc.titleA statistical comparison of the optical/UV and X-ray afterglows of gamma-ray bursts using the Swift Ultraviolet Optical and X-ray Telescopes
dc.typeMakale
dc.relation.journalMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
dc.contributor.departmentUniversity Of London , ,
dc.identifier.volume412
dc.identifier.issue1
dc.identifier.startpage561
dc.identifier.endpage579
dc.contributor.firstauthorID3378737


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