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Conference Paper: Panchromatic study of GRB 060124: From precursor to afterglow

TitlePanchromatic study of GRB 060124: From precursor to afterglow
Authors
Romano, P.Campana, S.Chincarini, G.Cummings, J.Cusumano, G.Holland, S. T.Mangano, V.Mineo, T.Page, K. L.Pal'shin, V.Rol, E.Sakamoto, T.Zhang, B.Aptekar, R.Barbier, S.Barthelmy, S.Beardmore, A. P.Boyd, P.Burrows, D. N.Capalbi, M.Fenimore, E. E.Frederiks, D.Gehrels, N.Giommi, P.Goad, M. R.Godet, O.Golenetskii, S.Guetta, D.Kennea, J. A.La Parola, V.Malesani, D.Marshall, F.Moretti, A.Nousek, J. A.O'Brien, P. T.Osborne, J. P.Perri, M.Tagliaferri, G.
Issue Date2006
Citation
Nuovo Cimento Della Societa Italiana Di Fisica B, 2006, v. 121, n. 10-11, p. 1067-1071 How to Cite?
DOI: http://dx.doi.org/10.1393/ncb/i2007-10062-y
AbstractWe present observations of GRB 060124, the first event for which both the prompt and the afterglow emission could be observed simultaneously and in their entirety by the three Swift instruments and by Konus-Wind. Thanks to these exceptional circumstances, the temporal and spectral properties of the prompt emission could be studied in the optical, X-ray and gamma-ray ranges (up to 2 MeV). While the X-ray emission (0.2-10 keV) clearly tracks the gamma-ray burst, the optical component follows a different pattern, likely indicating a different origin, possibly the onset of external shocks. © Società Italiana di Fisica.
Persistent Identifierhttp://hdl.handle.net/10722/361088
ISSN
1594-9982

 

DC FieldValueLanguage
dc.contributor.authorRomano, P.-
dc.contributor.authorCampana, S.-
dc.contributor.authorChincarini, G.-
dc.contributor.authorCummings, J.-
dc.contributor.authorCusumano, G.-
dc.contributor.authorHolland, S. T.-
dc.contributor.authorMangano, V.-
dc.contributor.authorMineo, T.-
dc.contributor.authorPage, K. L.-
dc.contributor.authorPal'shin, V.-
dc.contributor.authorRol, E.-
dc.contributor.authorSakamoto, T.-
dc.contributor.authorZhang, B.-
dc.contributor.authorAptekar, R.-
dc.contributor.authorBarbier, S.-
dc.contributor.authorBarthelmy, S.-
dc.contributor.authorBeardmore, A. P.-
dc.contributor.authorBoyd, P.-
dc.contributor.authorBurrows, D. N.-
dc.contributor.authorCapalbi, M.-
dc.contributor.authorFenimore, E. E.-
dc.contributor.authorFrederiks, D.-
dc.contributor.authorGehrels, N.-
dc.contributor.authorGiommi, P.-
dc.contributor.authorGoad, M. R.-
dc.contributor.authorGodet, O.-
dc.contributor.authorGolenetskii, S.-
dc.contributor.authorGuetta, D.-
dc.contributor.authorKennea, J. A.-
dc.contributor.authorLa Parola, V.-
dc.contributor.authorMalesani, D.-
dc.contributor.authorMarshall, F.-
dc.contributor.authorMoretti, A.-
dc.contributor.authorNousek, J. A.-
dc.contributor.authorO'Brien, P. T.-
dc.contributor.authorOsborne, J. P.-
dc.contributor.authorPerri, M.-
dc.contributor.authorTagliaferri, G.-
dc.date.accessioned2025-09-16T04:14:40Z-
dc.date.available2025-09-16T04:14:40Z-
dc.date.issued2006-
dc.identifier.citationNuovo Cimento Della Societa Italiana Di Fisica B, 2006, v. 121, n. 10-11, p. 1067-1071-
dc.identifier.issn1594-9982-
dc.identifier.urihttp://hdl.handle.net/10722/361088-
dc.description.abstractWe present observations of GRB 060124, the first event for which both the prompt and the afterglow emission could be observed simultaneously and in their entirety by the three Swift instruments and by Konus-Wind. Thanks to these exceptional circumstances, the temporal and spectral properties of the prompt emission could be studied in the optical, X-ray and gamma-ray ranges (up to 2 MeV). While the X-ray emission (0.2-10 keV) clearly tracks the gamma-ray burst, the optical component follows a different pattern, likely indicating a different origin, possibly the onset of external shocks. © Società Italiana di Fisica.-
dc.languageeng-
dc.relation.ispartofNuovo Cimento Della Societa Italiana Di Fisica B-
dc.titlePanchromatic study of GRB 060124: From precursor to afterglow-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1393/ncb/i2007-10062-y-
dc.identifier.scopuseid_2-s2.0-34548216350-
dc.identifier.volume121-
dc.identifier.issue10-11-
dc.identifier.spage1067-
dc.identifier.epage1071-

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