GRB110721A: An extreme peak energy and signatures of the photosphere
dc.contributor.author | AXELSSON, Magnus | |
dc.contributor.author | BALDINI, Luca | |
dc.contributor.author | BARBIELLINI, Guido | |
dc.contributor.author | G. BARING, M. | |
dc.contributor.author | BELLAZZINI, R. | |
dc.contributor.author | BREGEON, J. | |
dc.contributor.author | BRIGIDA, M. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | BRUEL, Pascal | |
dc.contributor.author | BUEHLER, R. | |
dc.contributor.author | A. CALIANDRO, G. | |
dc.contributor.author | A. CAMERON, R. | |
dc.contributor.author | CARAVEO, P. A. | |
dc.contributor.author | CECCHI, C. | |
hal.structure.identifier | Max-Planck-Institut für Kernphysik [MPIK] | |
dc.contributor.author | CHAVES, R.C.G. | |
dc.contributor.author | CHEKHTMAN, A. | |
dc.contributor.author | CHIANG, J. | |
dc.contributor.author | CLAUS, R. | |
dc.contributor.author | CONRAD, J. | |
dc.contributor.author | CUTINI, S. | |
dc.contributor.author | D'AMMANDO, F. | |
dc.contributor.author | DE PALMA, F. | |
dc.contributor.author | D. DERMER, C. | |
dc.contributor.author | DO COUTO E SILVA, E. | |
dc.contributor.author | S. DRELL, P. | |
dc.contributor.author | FAVUZZI, C. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | J. FEGAN, S. | |
dc.contributor.author | C. FERRARA, E. | |
dc.contributor.author | B. FOCKE, W. | |
dc.contributor.author | FUKAZAWA, Y. | |
dc.contributor.author | FUSCO, P. | |
dc.contributor.author | GARGANO, F. | |
dc.contributor.author | GASPARRINI, D. | |
dc.contributor.author | GEHRELS, N. | |
dc.contributor.author | GERMANI, S. | |
dc.contributor.author | GIGLIETTO, N. | |
dc.contributor.author | GIROLETTI, M. | |
dc.contributor.author | GODFREY, G. | |
dc.contributor.author | GUIRIEC, S. | |
dc.contributor.author | HADASCH, D. | |
dc.contributor.author | HANABATA, Y. | |
dc.contributor.author | HAYASHIDA, M. | |
hal.structure.identifier | GLAST | |
dc.contributor.author | HOU, X. | |
dc.contributor.author | IYYANI, S. | |
dc.contributor.author | S. JACKSON, M. | |
dc.contributor.author | KOCEVSKI, D. | |
dc.contributor.author | KUSS, M. | |
dc.contributor.author | LARSSON, J. | |
dc.contributor.author | LARSSON, S. | |
dc.contributor.author | LONGO, F. | |
dc.contributor.author | LOPARCO, F. | |
dc.contributor.author | LUNDMAN, C. | |
dc.contributor.author | N. MAZZIOTTA, M. | |
dc.contributor.author | E. MCENERY, J. | |
dc.contributor.author | MIZUNO, T. | |
dc.contributor.author | E. MONZANI, M. | |
dc.contributor.author | MORETTI, E. | |
dc.contributor.author | MORSELLI, A. | |
dc.contributor.author | MURGIA, S. | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | NUSS, E. | |
dc.contributor.author | NYMARK, T. | |
dc.contributor.author | OHNO, M. | |
dc.contributor.author | OMODEI, N. | |
dc.contributor.author | PESCE-ROLLINS, M. | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | PIRON, F. | |
dc.contributor.author | PIVATO, G. | |
dc.contributor.author | L. RACUSIN, J. | |
dc.contributor.author | RAIN'O, S. | |
dc.contributor.author | RAZZANO, M. | |
dc.contributor.author | RAZZAQUE, S. | |
dc.contributor.author | REIMER, A. | |
dc.contributor.author | ROTH, M. | |
dc.contributor.author | RYDE, F. | |
dc.contributor.author | SANCHEZ, D.A. | |
dc.contributor.author | SGR'O, C. | |
dc.contributor.author | J. SISKIND, E. | |
dc.contributor.author | SPANDRE, G. | |
dc.contributor.author | SPINELLI, P. | |
dc.contributor.author | STAMATIKOS, M. | |
dc.contributor.author | TIBALDO, L. | |
dc.contributor.author | TINIVELLA, M. | |
dc.contributor.author | L. USHER, T. | |
dc.contributor.author | VANDENBROUCKE, J. | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | VASILEIOU, V. | |
dc.contributor.author | VIANELLO, G. | |
dc.contributor.author | VITALE, V. | |
dc.contributor.author | P. WAITE, A. | |
dc.contributor.author | L. WINER, B. | |
dc.contributor.author | S. WOOD, K. | |
dc.contributor.author | M. BURGESS, J. | |
dc.contributor.author | N. BHAT, P. | |
dc.contributor.author | BISSALDI, E. | |
dc.contributor.author | S. BRIGGS, M. | |
dc.contributor.author | CONNAUGHTON, V. | |
dc.contributor.author | FISHMAN, G. | |
dc.contributor.author | FITZPATRICK, G. | |
dc.contributor.author | FOLEY, S. | |
dc.contributor.author | GRUBER, D. | |
dc.contributor.author | M. KIPPEN, R. | |
dc.contributor.author | KOUVELIOTOU, C. | |
dc.contributor.author | JENKE, P. | |
dc.contributor.author | MCBREEN, S. | |
dc.contributor.author | MCGLYNN, S. | |
dc.contributor.author | MEEGAN, C. | |
dc.contributor.author | S. PACISAS, W. | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | PELASSA, V. | |
dc.contributor.author | PREECE, R. | |
dc.contributor.author | TIERNEY, D. | |
dc.contributor.author | VON KIENLIN, A. | |
dc.contributor.author | WILSON-HODGE, C. | |
dc.contributor.author | XIONG, S. | |
dc.contributor.author | PE'ER, A. | |
dc.date.issued | 2012 | |
dc.identifier.issn | 2041-8205 | |
dc.description.abstractEn | GRB110721A was observed by the Fermi Gamma-ray Space Telescope using its two instruments the Large Area Telescope (LAT) and the Gamma-ray Burst Monitor (GBM). The burst consisted of one major emission episode which lasted for ~24.5 seconds (in the GBM) and had a peak flux of 5.7\pm0.2 x 10^{-5} erg/s/cm^2. The time-resolved emission spectrum is best modeled with a combination of a Band function and a blackbody spectrum. The peak energy of the Band component was initially 15\pm2 MeV, which is the highest value ever detected in a GRB. This measurement was made possible by combining GBM/BGO data with LAT Low Energy Events to achieve continuous 10--100 MeV coverage. The peak energy later decreased as a power law in time with an index of -1.89\pm0.10. The temperature of the blackbody component also decreased, starting from ~80 keV, and the decay showed a significant break after ~2 seconds. The spectrum provides strong constraints on the standard synchrotron model, indicating that alternative mechanisms may give rise to the emission at these energies. | |
dc.language.iso | en | |
dc.publisher | Bristol : IOP Publishing | |
dc.title.en | GRB110721A: An extreme peak energy and signatures of the photosphere | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1088/2041-8205/757/2/L31 | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.identifier.arxiv | 1207.6109 | |
bordeaux.journal | The Astrophysical journal letters | |
bordeaux.page | L31 | |
bordeaux.volume | 757 | |
bordeaux.peerReviewed | oui | |
hal.identifier | in2p3-00743070 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//in2p3-00743070v1 | |
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