File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Conference Paper: The short GRB 051210 observed by Swift

TitleThe short GRB 051210 observed by Swift
Authors
La Parola, V.Mangano, V.Zhang, B.Cusumano, G.Mineo, T.Troja, E.Burrows, D. N.Campana, S.Capalbi, M.Chincarini, G.Giommi, P.Moretti, A.Perri, M.Romano, P.Tagliaferri, G.
Issue Date2006
Citation
Nuovo Cimento Della Societa Italiana Di Fisica B, 2006, v. 121, n. 12, p. 1505-1506 How to Cite?
DOI: http://dx.doi.org/10.1393/ncb/i2007-10299-4
AbstractWe report on the short GRB 051210 detected by the Swift-BAT. The light curve, on which we focus mainly, shows a hint of extended emission in the BAT energy range, a steep decay of the X-ray emission, without any flattening or break, and two small flares in the first 300 s. The emission fades out after ∼ 1000 s. © Societá Italiana di Fisica.
Persistent Identifierhttp://hdl.handle.net/10722/361095
ISSN
1594-9982

 

DC FieldValueLanguage
dc.contributor.authorLa Parola, V.-
dc.contributor.authorMangano, V.-
dc.contributor.authorZhang, B.-
dc.contributor.authorCusumano, G.-
dc.contributor.authorMineo, T.-
dc.contributor.authorTroja, E.-
dc.contributor.authorBurrows, D. N.-
dc.contributor.authorCampana, S.-
dc.contributor.authorCapalbi, M.-
dc.contributor.authorChincarini, G.-
dc.contributor.authorGiommi, P.-
dc.contributor.authorMoretti, A.-
dc.contributor.authorPerri, M.-
dc.contributor.authorRomano, P.-
dc.contributor.authorTagliaferri, G.-
dc.date.accessioned2025-09-16T04:14:42Z-
dc.date.available2025-09-16T04:14:42Z-
dc.date.issued2006-
dc.identifier.citationNuovo Cimento Della Societa Italiana Di Fisica B, 2006, v. 121, n. 12, p. 1505-1506-
dc.identifier.issn1594-9982-
dc.identifier.urihttp://hdl.handle.net/10722/361095-
dc.description.abstractWe report on the short GRB 051210 detected by the Swift-BAT. The light curve, on which we focus mainly, shows a hint of extended emission in the BAT energy range, a steep decay of the X-ray emission, without any flattening or break, and two small flares in the first 300 s. The emission fades out after ∼ 1000 s. © Societá Italiana di Fisica.-
dc.languageeng-
dc.relation.ispartofNuovo Cimento Della Societa Italiana Di Fisica B-
dc.titleThe short GRB 051210 observed by Swift-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1393/ncb/i2007-10299-4-
dc.identifier.scopuseid_2-s2.0-35348929429-
dc.identifier.volume121-
dc.identifier.issue12-
dc.identifier.spage1505-
dc.identifier.epage1506-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats