Cosmic rays in the TeV region with the ARGO-YBJ detector
- 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
Publication date
January 2012
DOIAbstract
""\\"Very High Energy (VHE) γ-astronomy and cosmic ray physics are. the main goals of the ARGO-YBJ experiment. The detector is located in Tibet. (People’s Republic of China) and is a full-coverage Extensive Air Shower array consisting. of a carpet of Resistive Plate Chambers (RPCs). Altitude and full coverage. ensure an unprecedented reconstruction of showers close to their maximum size.. The performances of the detector and the present results concerning TeV cosmic. ray physics will be presented.\\""
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