Search for High-Energy Emission from GRBs with the ARGO-YBJ Detector
- Aielli, G
- Bacci, C
- Bartoli, B
- Bernardini, P
- Bi, Xj
- Bleve, C
- Branchini, P
- Budano, A
- Bussino, Severino Angelo Maria
- Calabrese Melcarne, Ak
- Camarri, P
- Cao, Z
- Cappa, A
- Cardarelli, R
- Catalanotti, S
- Cattaneo, C
- Celio, P
- Chen, Sz
- Chen, Tl
- Chen, Y
- Cheng, N
- Creti, P
- Cui, Sw
- Dai, Bz
- D'Ali Staiti, G
- Danzengluobu,
- Dattoli, M
- De Mitri, I
- D'Ettorre Piazzoli, B
- De Vincenzi, M
- Di Girolamo, T
- Ding, Xh
- Di Sciascio, G
- Feng, Cf
- Feng Zhao, Yang
- Feng Zhen, Yong
- Galeazzi, F
- Galeotti, P
- Gargana, R
- Gou, Qb
- Guo, Yq
- He, Hh
- Hu, Haibing
- Hu Hong, Bo
- 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 Ji, Long
- Zhang Jian, Li
- Zhang, L
- Zhang, P
- Zhang, Xy
- Zhang, Y
- Zhaxisangzhu,
- Zhou, Xx
- Zhu, Fr
- Zhu, Qq
- Zizzi, G.
DOIAbstract
ARGO-YBJ is a "full coverage" air shower detector consisting of a 6700 m2 carpet of Resistive Plate Counters, located at Yangbajing (Tibet, P.R.China, 4300 m a.s.l). Its large field of view (~ 2 sr, limited only by the atmospheric absorption) and high duty-cycle make ARGO-YBJ particularly suitable to detect unpredictable and short duration events such as GRBs. ARGO-YBJ works using two techniques: the "Scaler Mode", which reaches the lower energy limit (~ 1 GeV) of the detector, and the "Shower Mode", with an energy threshold of a few hundreds of GeV. Here we present the results of the search for high-energy emission from GRBs in coincidence with satellite detections
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