ARGO-YBJ constraints on very high energy emission from GRBs
- Aielli G
- Bacci C
- Bartoli B
- Bernardini P
- Bi XJ
- Bleve C
- Branchini P
- Budano A
- BUSSINO, Severino Angelo Maria
- Melcarne AKC
- Camarri P
- Cao Z
- Cappa A
- Cardarelli R
- Catalanotti S
- Cattaneo C
- Celio P
- Chen SZ
- Chen Y
- Cheng N
- Creti P
- Cui SW
- Dai BZ
- Staiti GD
- Danzengluobu
- Dattoli M
- De Mitri I
- Piazzoli BD
- DE VINCENZI, Mario
- Di Girolamo T
- Ding XH
- Di Sciascio G
- Feng CF
- Feng ZY
- Feng ZY
- Galeazzi F
- Galeotti P
- Gargana R
- Gou QB
- Guo YQ
- He HH
- Hu HB
- Hu HB
- Huang Q
- Iacovacci M
- Iuppa R
- James I
- Jia HY
- Labaciren
- Li HJ
- Li JY
- Li XX
- Liberti B
- Liguori G
- Liu C
- Liu CQ
- Liu MY
- Liu J
- Lu H
- Ma XH
- Mancarella G
- MARI, Stefano Maria
- Marsella G
- Martello D
- Mastroianni S
- Meng XR
- Montini P
- Ning CC
- Pagliaro A
- Panareo M
- Perrone L
- Pistilli P
- Qu XB
- Rossi E
- Ruggieri F
- Saggese L
- Salvini P
- Santonico R
- Shen PR
- Sheng XD
- Shi F
- Stanescu C
- Surdo A
- Tan YH
- Vallania P
- Vernetto S
- Vigorito C
- Wang B
- Wang H
- Wu CY
- Wu HR
- Xu B
- Xue L
- Yan YX
- Yang QY
- Yang XC
- Yuan AF
- Zha M
- Zhang HM
- Zhang JL
- Zhang JL
- Zhang L
- Zhang P
- Zhang XY
- Zhang Y
- Zhaxisangzhu
- Zhou XX
- Zhu FR
- Zhu QQ
- Zizzi G.
DOIAbstract
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 (4300 m 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 esti...
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