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Conference Paper: Swift observations of GRB050712

TitleSwift observations of GRB050712
Authors
Poole, T. S.De Pasquale, M.Grupe, D.Breeveld, A. A.Zane, S.Rosen, S. R.Page, M. J.Mason, K. O.Burrows, D. N.Krimm, H. A.Gehrels, N.Nousek, J. A.Roming, P. W.A.Kobayashi, S.Zhang, B.
Issue Date2006
Citation
Nuovo Cimento Della Societa Italiana Di Fisica B, 2006, v. 121, n. 12, p. 1567-1568 How to Cite?
DOI: http://dx.doi.org/10.1393/ncb/i2007-10321-y
AbstractSwift observations of GRB050712 show that the X-ray light curve of this burst exhibits flaring activity in the first 500 s. We find that the initial flares can be due to "inner engine" activity, where the later flare may be explained in terms of the interaction of the ejecta with the surrounding medium. An optical counterpart was detected in the U and V band of UVOT up to 15000 s after the trigger. © Société Italiana di Fisica.
Persistent Identifierhttp://hdl.handle.net/10722/361099
ISSN
1594-9982

 

DC FieldValueLanguage
dc.contributor.authorPoole, T. S.-
dc.contributor.authorDe Pasquale, M.-
dc.contributor.authorGrupe, D.-
dc.contributor.authorBreeveld, A. A.-
dc.contributor.authorZane, S.-
dc.contributor.authorRosen, S. R.-
dc.contributor.authorPage, M. J.-
dc.contributor.authorMason, K. O.-
dc.contributor.authorBurrows, D. N.-
dc.contributor.authorKrimm, H. A.-
dc.contributor.authorGehrels, N.-
dc.contributor.authorNousek, J. A.-
dc.contributor.authorRoming, P. W.A.-
dc.contributor.authorKobayashi, S.-
dc.contributor.authorZhang, B.-
dc.date.accessioned2025-09-16T04:14:43Z-
dc.date.available2025-09-16T04:14:43Z-
dc.date.issued2006-
dc.identifier.citationNuovo Cimento Della Societa Italiana Di Fisica B, 2006, v. 121, n. 12, p. 1567-1568-
dc.identifier.issn1594-9982-
dc.identifier.urihttp://hdl.handle.net/10722/361099-
dc.description.abstractSwift observations of GRB050712 show that the X-ray light curve of this burst exhibits flaring activity in the first 500 s. We find that the initial flares can be due to "inner engine" activity, where the later flare may be explained in terms of the interaction of the ejecta with the surrounding medium. An optical counterpart was detected in the U and V band of UVOT up to 15000 s after the trigger. © Société Italiana di Fisica.-
dc.languageeng-
dc.relation.ispartofNuovo Cimento Della Societa Italiana Di Fisica B-
dc.titleSwift observations of GRB050712-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1393/ncb/i2007-10321-y-
dc.identifier.scopuseid_2-s2.0-35349021027-
dc.identifier.volume121-
dc.identifier.issue12-
dc.identifier.spage1567-
dc.identifier.epage1568-

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