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Conference Paper: A tale of two faint bursts: GRB 050223 and GRB 050911

TitleA tale of two faint bursts: GRB 050223 and GRB 050911
Authors
Page, K. L.Barthelmy, S. D.Beardmore, A. P.Burrows, D. N.Campana, S.Chincharini, G.Cummings, J. R.Cusumano, G.Gehrels, N.Giommi, P.Goad, M. R.Godet, O.Graham, J.Kaneko, Y.Kennea, J. A.Mangano, V.Markwardt, C. B.O'Brien, P. T.Osborne, J. P.Reichart, D. E.Rol, E.Sakamoto, T.Tagliaferri, G.Tanvir, N. R.Wells, A. A.Zhang, B.
KeywordsGamma-rays bursts
Issue Date2006
Citation
Aip Conference Proceedings, 2006, v. 836, p. 321-324 How to Cite?
DOI: http://dx.doi.org/10.1063/1.2207912
AbstractGRBs 050223 and 050911 were discovered by the Swift Burst Alert Telescope (BAT) on 23rd February and 11th September 2005 respectively. The observation of GRB 050223 showed a faint, fading X-ray source, which was identified as the afterglow; GRB 050911, however, was not detected, making any X-ray afterglow extremely faint. The faintness of the afterglow of GRB 050223 could be explained by a large opening or viewing angle, or by the burst being at high redshift. The non-detection of GRB 050911 may indicate the burst occurred in a low-density environment, or, alternatively, was due to a compact object merger, in spite of the apparent long duration of the burst. © 2006 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/361049
ISSN
0094-243X
2023 SCImago Journal Rankings: 0.152

 

DC FieldValueLanguage
dc.contributor.authorPage, K. L.-
dc.contributor.authorBarthelmy, S. D.-
dc.contributor.authorBeardmore, A. P.-
dc.contributor.authorBurrows, D. N.-
dc.contributor.authorCampana, S.-
dc.contributor.authorChincharini, G.-
dc.contributor.authorCummings, J. R.-
dc.contributor.authorCusumano, G.-
dc.contributor.authorGehrels, N.-
dc.contributor.authorGiommi, P.-
dc.contributor.authorGoad, M. R.-
dc.contributor.authorGodet, O.-
dc.contributor.authorGraham, J.-
dc.contributor.authorKaneko, Y.-
dc.contributor.authorKennea, J. A.-
dc.contributor.authorMangano, V.-
dc.contributor.authorMarkwardt, C. B.-
dc.contributor.authorO'Brien, P. T.-
dc.contributor.authorOsborne, J. P.-
dc.contributor.authorReichart, D. E.-
dc.contributor.authorRol, E.-
dc.contributor.authorSakamoto, T.-
dc.contributor.authorTagliaferri, G.-
dc.contributor.authorTanvir, N. R.-
dc.contributor.authorWells, A. A.-
dc.contributor.authorZhang, B.-
dc.date.accessioned2025-09-16T04:14:28Z-
dc.date.available2025-09-16T04:14:28Z-
dc.date.issued2006-
dc.identifier.citationAip Conference Proceedings, 2006, v. 836, p. 321-324-
dc.identifier.issn0094-243X-
dc.identifier.urihttp://hdl.handle.net/10722/361049-
dc.description.abstractGRBs 050223 and 050911 were discovered by the Swift Burst Alert Telescope (BAT) on 23rd February and 11th September 2005 respectively. The observation of GRB 050223 showed a faint, fading X-ray source, which was identified as the afterglow; GRB 050911, however, was not detected, making any X-ray afterglow extremely faint. The faintness of the afterglow of GRB 050223 could be explained by a large opening or viewing angle, or by the burst being at high redshift. The non-detection of GRB 050911 may indicate the burst occurred in a low-density environment, or, alternatively, was due to a compact object merger, in spite of the apparent long duration of the burst. © 2006 American Institute of Physics.-
dc.languageeng-
dc.relation.ispartofAip Conference Proceedings-
dc.subjectGamma-rays bursts-
dc.titleA tale of two faint bursts: GRB 050223 and GRB 050911-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1063/1.2207912-
dc.identifier.scopuseid_2-s2.0-33845571564-
dc.identifier.volume836-
dc.identifier.spage321-
dc.identifier.epage324-
dc.identifier.eissn1551-7616-

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