THE ARGO-YBJ EXPERIMENT: A FULL COVERAGE ARRAY FOR γ-RAY ASTRONOMY
- Aielli G
- Bacci C
- Bartoli B
- Bernardini P
- Bi XJ
- Bleve C
- Branchini P
- Budano A
- Bussino S
- 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 SM
- 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
""The ARGO-YBJ experiment is an Extensive Air Shower (EAS) array which combines. high altitude location and full coverage active area in order to reach low energy threshold. at a level of few hundred of GeV. The large field of view (≈ 2 sr) and the high duty cycle. (≥ 90%) allow the continuous monitoring of the sky searching for unknown sources and. unpredictable events, such as flares in blazar emissions and high energy Gamma-Ray. Bursts (GRBs). In this paper I will briefly report on the detector performance and on. some preliminary results achieved in γ-ray astronomy."
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