Please use this identifier to cite or link to this item: http://hdl.handle.net/2307/368
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dc.contributor.authorAielli, G.-
dc.contributor.authorBacci, Cesare-
dc.contributor.authorBartoli, B.-
dc.contributor.authorBernardini, P.-
dc.contributor.authorBi, X. J.-
dc.contributor.authorBleve, C.-
dc.contributor.authorBranchini, Paolo-
dc.contributor.authorBudano, Antonio-
dc.contributor.authorBussino, Severino-
dc.contributor.authorCalabrese Melcarne, A. K.-
dc.contributor.authorCamarri, P.-
dc.contributor.authorZhang, JianLi-
dc.contributor.authorZhang, L.-
dc.contributor.authorZhang, P.-
dc.contributor.authorZhang, X. Y.-
dc.contributor.authorZhang, Y.-
dc.contributor.authorZhaxisangzhu-
dc.contributor.authorZhou, X. X.-
dc.contributor.authorZhu, F. R.-
dc.contributor.authorZhu, Q. Q.-
dc.contributor.authorZizzi, G.-
dc.contributor.authorCao, Z.-
dc.contributor.authorCappa, A.-
dc.contributor.authorCardarelli, R.-
dc.contributor.authorCatalanotti, S.-
dc.contributor.authorCattaneo, C.-
dc.contributor.authorCelio, Paola-
dc.contributor.authorChen, S. Z.-
dc.contributor.authorChen, Y.-
dc.contributor.authorCheng, N.-
dc.contributor.authorCreti, P.-
dc.contributor.authorCui, S. W.-
dc.contributor.authorDai, B. Z.-
dc.contributor.authorD'Ali Staiti, G.-
dc.contributor.authorDanzengluobu-
dc.contributor.authorDattoli, M.-
dc.contributor.authorDe Mitri, I.-
dc.contributor.authorD'Ettorre Piazzoli, B.-
dc.contributor.authorDe Vincenzi, Mario-
dc.contributor.authorDi Girolamo, T.-
dc.contributor.authorDing, X. H.-
dc.contributor.authorDi Sciascio, G.-
dc.contributor.authorFeng, C. F.-
dc.contributor.authorFeng, Zhaoyang-
dc.contributor.authorFeng, Zhenyong-
dc.contributor.authorGaleazzi, Fulvio-
dc.contributor.authorGaleotti, P.-
dc.contributor.authorGargana, Riccardo-
dc.contributor.authorGou, Q. B.-
dc.contributor.authorGuo, Y. Q.-
dc.contributor.authorHe, H. H.-
dc.contributor.authorHu, Haibing-
dc.contributor.authorHu, Hongbo-
dc.contributor.authorHuang, Q.-
dc.contributor.authorIacovacci, M.-
dc.contributor.authorIuppa, R.-
dc.contributor.authorJames, Irina-
dc.contributor.authorJia, H. Y.-
dc.contributor.authorLabaciren-
dc.contributor.authorLi, H. J.-
dc.contributor.authorLi, J. Y.-
dc.contributor.authorLi, X. X.-
dc.contributor.authorLiberti, B.-
dc.contributor.authorLiguori, G.-
dc.contributor.authorLiu, C.-
dc.contributor.authorLiu, C. Q.-
dc.contributor.authorLiu, M. Y.-
dc.contributor.authorLiu, J.-
dc.contributor.authorLu, H.-
dc.contributor.authorMa, X. H.-
dc.contributor.authorMancarella, G.-
dc.contributor.authorMari, Stefano Maria-
dc.contributor.authorMarsella, G.-
dc.contributor.authorMartello, D.-
dc.contributor.authorMastroianni, S.-
dc.contributor.authorMeng, X. R.-
dc.contributor.authorMontini, Paolo-
dc.contributor.authorNing, C. C.-
dc.contributor.authorPagliaro, A.-
dc.contributor.authorPanareo, M.-
dc.contributor.authorPerrone, L.-
dc.contributor.authorPistilli, Pio-
dc.contributor.authorQu, X. B.-
dc.contributor.authorRossi, E.-
dc.contributor.authorRuggieri, Federico-
dc.contributor.authorSaggese, L.-
dc.contributor.authorSalvini, P.-
dc.contributor.authorSantonico, R.-
dc.contributor.authorShen, P. R.-
dc.contributor.authorSheng, X. D.-
dc.contributor.authorShi, F.-
dc.contributor.authorStanescu, Cristian-
dc.contributor.authorSurdo, A.-
dc.contributor.authorTan, Y. H.-
dc.contributor.authorVallania, P.-
dc.contributor.authorVernetto, S.-
dc.contributor.authorVigorito, C.-
dc.contributor.authorWang, B.-
dc.contributor.authorWang, H.-
dc.contributor.authorWu, C. Y.-
dc.contributor.authorWu, H. R.-
dc.contributor.authorXu, B.-
dc.contributor.authorXue, L.-
dc.contributor.authorYan, Y. X.-
dc.contributor.authorYang, Q. Y.-
dc.contributor.authorYang, X. C.-
dc.contributor.authorYuan, A. F.-
dc.contributor.authorZha, M.-
dc.contributor.authorZhang, H. M.-
dc.contributor.authorZhang, JiLong-
dc.date.accessioned2010-07-28T14:10:39Z-
dc.date.available2010-07-28T14:10:39Z-
dc.date.issued2009-08-
dc.identifier.issn0927-6505-
dc.identifier.urihttp://hdl.handle.net/2307/368-
dc.description.abstractThe ARGO-YBJ (Astrophysical Radiation Ground-based Observatory at YangBajing) experiment is designed for very high energy gamma-astronomy and cosmic ray researches. Due to the full coverage of a large area(5600 m(2)) with resistive plate chambers at a very high altitude (4300m a.s.l.), the ARGO-YBJ detector is used to search for transient phenomena, such as Gamma-ray bursts (GRBs). Because the ARGO-YBJ detector has a large field of view (similar to 2 sr) and is operated with a high duty cycle (>90%), it is well suited for GRB surveying and can be operated in searches for high energy GRBs following alarms set by satellite-borne observations at lower energies. In this paper, the sensitivity of the ARGO-YBJ detector for GRB detection is estimated. Upper limits to fluence with 99% confidence level for 26 GRBs inside the field of view from June 2006 to January 2009 are set in the two energy ranges 10-100 GeV and 10 GeV-1 TeV.en
dc.language.isoenen
dc.publisherElsevieren
dc.relation.ispartofAstroparticle Physicsen
dc.rightsElsevier B.V.en
dc.subjectGAMMA-RAY BURSTSen
dc.subjectCOSMIC RAYSen
dc.subjectAIR SHOWER EXPERIMENTSen
dc.subjectGAMMA RAYen
dc.subjectASTROPARTICLE PHYSICSen
dc.titleARGO-YBJ constraints on very high energy emission from GRBsen
dc.typeArticleen
dc.subject.miurSettori Disciplinari MIUR::Scienze fisiche::FISICA SPERIMENTALEen
dc.subject.miurScienze fisiche-
dc.subject.isicruiCategorie ISI-CRUI::Scienze fisiche::Physicsen
dc.subject.isicruiScienze fisiche-
dc.subject.anagraferoma3Scienze fisicheen
dc.relation.volumenumber32en
dc.relation.pagenumber47-52en
dc.identifier.urlhttp://arxiv.org/abs/0903.0119-
dc.identifier.doi10.1016/j.astropartphys.2009.05.005-
dc.relation.issuenumber1en
dc.description.romatrecurrentDipartimento di Fisica 'Edoardo Amaldi'*
item.fulltextWith Fulltext-
item.grantfulltextrestricted-
item.languageiso639-1other-
Appears in Collections:A - Articolo su rivista
X_Dipartimento di Fisica 'Edoardo Amaldi'
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