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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-ray bursts
Issue Date2007
Citation
Aip Conference Proceedings, 2007, v. 924, p. 453-456 How to Cite?
DOI: http://dx.doi.org/10.1063/1.2774895
AbstractGRBs 050223 and 050911 are examples of Swift bursts with two of the faintest X-ray afterglows at (relatively) early times. While a faint, fading X-ray afterglow was located for GRB 050223, GRB 050911 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. © 2007 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/361097
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.accessioned2025-09-16T04:14:42Z-
dc.date.available2025-09-16T04:14:42Z-
dc.date.issued2007-
dc.identifier.citationAip Conference Proceedings, 2007, v. 924, p. 453-456-
dc.identifier.issn0094-243X-
dc.identifier.urihttp://hdl.handle.net/10722/361097-
dc.description.abstractGRBs 050223 and 050911 are examples of Swift bursts with two of the faintest X-ray afterglows at (relatively) early times. While a faint, fading X-ray afterglow was located for GRB 050223, GRB 050911 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. © 2007 American Institute of Physics.-
dc.languageeng-
dc.relation.ispartofAip Conference Proceedings-
dc.subjectGamma-ray bursts-
dc.titleA tale of two faint bursts: GRB 050223 and GRB 050911-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1063/1.2774895-
dc.identifier.scopuseid_2-s2.0-35348953334-
dc.identifier.volume924-
dc.identifier.spage453-
dc.identifier.epage456-
dc.identifier.eissn1551-7616-

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