Please use this identifier to cite or link to this item: http://hdl.handle.net/2307/368
Title: ARGO-YBJ constraints on very high energy emission from GRBs
Authors: Aielli, G.
Bacci, Cesare
Bartoli, B.
Bernardini, P.
Bi, X. J.
Bleve, C.
Branchini, Paolo
Budano, Antonio
Bussino, Severino
Calabrese Melcarne, A. K.
Camarri, P.
Zhang, JianLi
Zhang, L.
Zhang, P.
Zhang, X. Y.
Zhang, Y.
Zhaxisangzhu
Zhou, X. X.
Zhu, F. R.
Zhu, Q. Q.
Zizzi, G.
Cao, Z.
Cappa, A.
Cardarelli, R.
Catalanotti, S.
Cattaneo, C.
Celio, Paola
Chen, S. Z.
Chen, Y.
Cheng, N.
Creti, P.
Cui, S. W.
Dai, B. Z.
D'Ali Staiti, G.
Danzengluobu
Dattoli, M.
De Mitri, I.
D'Ettorre Piazzoli, B.
De Vincenzi, Mario
Di Girolamo, T.
Ding, X. H.
Di Sciascio, G.
Feng, C. F.
Feng, Zhaoyang
Feng, Zhenyong
Galeazzi, Fulvio
Galeotti, P.
Gargana, Riccardo
Gou, Q. B.
Guo, Y. Q.
He, H. H.
Hu, Haibing
Hu, Hongbo
Huang, Q.
Iacovacci, M.
Iuppa, R.
James, Irina
Jia, H. Y.
Labaciren
Li, H. J.
Li, J. Y.
Li, X. X.
Liberti, B.
Liguori, G.
Liu, C.
Liu, C. Q.
Liu, M. Y.
Liu, J.
Lu, H.
Ma, X. H.
Mancarella, G.
Mari, Stefano Maria
Marsella, G.
Martello, D.
Mastroianni, S.
Meng, X. R.
Montini, Paolo
Ning, C. C.
Pagliaro, A.
Panareo, M.
Perrone, L.
Pistilli, Pio
Qu, X. B.
Rossi, E.
Ruggieri, Federico
Saggese, L.
Salvini, P.
Santonico, R.
Shen, P. R.
Sheng, X. D.
Shi, F.
Stanescu, Cristian
Surdo, A.
Tan, Y. H.
Vallania, P.
Vernetto, S.
Vigorito, C.
Wang, B.
Wang, H.
Wu, C. Y.
Wu, H. R.
Xu, B.
Xue, L.
Yan, Y. X.
Yang, Q. Y.
Yang, X. C.
Yuan, A. F.
Zha, M.
Zhang, H. M.
Zhang, JiLong
Keywords: GAMMA-RAY BURSTS
COSMIC RAYS
AIR SHOWER EXPERIMENTS
GAMMA RAY
ASTROPARTICLE PHYSICS
Issue Date: Aug-2009
Publisher: Elsevier
Abstract: The 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.
URI: http://hdl.handle.net/2307/368
ISSN: 0927-6505
DOI: 10.1016/j.astropartphys.2009.05.005
metadata.dc.identifier.url: http://arxiv.org/abs/0903.0119
Appears in Collections:A - Articolo su rivista
X_Dipartimento di Fisica 'Edoardo Amaldi'

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