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The ARGO-YBJ contribution to the cosmic ray physics

Authors :
Aielli G
Bacci C
Bartoli B
Bernardini P
Bi XJ
Bleve C
Branchini P
Budano A
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, Mario
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
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.
BUSSINO, Severino Angelo Maria
MARI, Stefano Maria
G., Aielli
C., Bacci
B., Bartoli
Bernardini, Paolo
X. J., Bi
C., Bleve
P., Branchini
A., Budano
S., Bussino
A. K., CALABRESE MELCARNE
P., Camarri
Z., Cao
A., Cappa
R., Cardarelli
S., Catalanotti
C., Cattaneo
P., Celio
S. Z., Chen
Y., Chen
N., Cheng
P., Creti
S. W., Cui
B. Z., Dai
G., D’ALÍ STAITI
Danzengluobu
M., Dattoli
DE MITRI, Ivan
B., D’ETTORRE PIAZZOLI
M., DE VINCENZI
T., DI GIROLAMO
X. H., Ding
G., DI SCIASCIO
C. F., Feng
Zhaoyang, Feng
Zhenyong, Feng
F., Galeazzi
P., Galeotti
R., Gargana
Q. B., Gou
Y. Q., Guo
H. H., He
Haibing, Hu
Hongbo, Hu
Q., Huang
M., Iacovacci
R., Iuppa
I., Jame
H. Y., Jia
Labaciren
H. J., Li
J. Y., Li
X. X., Li
B., Liberti
G., Liguori
C., Liu
C. Q., Liu
M. Y., Liu
J., Liu
H., Lu
X. H., Ma
Mancarella, Giovanni
S. M., Mari
Marsella, Giovanni
Martello, Daniele
S., Mastroianni
X. R., Meng
P., Montini
C. C., Ning
A., Pagliaro
Panareo, Marco
Perrone, Lorenzo
P., Pistilli
X. B., Qu
E., Rossi
F., Ruggieri
L., Saggese
P., Salvini
R., Santonico
P. R., Shen
X. D., Sheng
F., Shi
C., Stanescu
A., Surdo
Y. H., Tan
P., Vallania
S., Vernetto
C., Vigorito
B., Wang
H., Wang
C. Y., Wu
H. R., Wu
B., Xu
L., Xue
Y. X., Yan
Q. Y., Yang
X. C., Yang
A. F., Yuan
M., Zha
H. M., Zhang
Jilong, Zhang
Jianli, Zhang
L., Zhang
P., Zhang
X. Y., Zhang
Y., Zhang
Zhaxisangzhu
X. X., Zhou
F. R., Zhu
Q. Q., Zhu
G., Zizzi
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
Dattoli, M
De Mitri, I
D'Ettorre Piazzoli, B
DE VINCENZI, Mario
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
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
Zhou, Xx
Zhu, Fr
Zhu, Qq
Zizzi, G.
Iacovacci, M.
Bartoli, B.
Catalanotti, S.
Di Girolamo, T.
D'Ettorre Piazzoli, B.
Mastroianni, S.
Source :
Nuclear Physics B - Proceedings Supplements. :59-67
Publication Year :
2011
Publisher :
Elsevier BV, 2011.

Abstract

""The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray. Laboratory (Tibet, P.R.China, 4300 m a.s.l.). It exploits a full coverage and high altitude approach to the. small air showers detection. The detector is made of a single layer of RPCs operated in streamer mode, fully. instrumenting a central carpet of about 5700 m2, then a guard ring extends the partially instrumented area to. about 11,000 m2. The large field of view (∼ 2 sr) and the high duty cycle (≥ 85%) allow a continuous monitoring. of the sky in the declination band from -10. ◦. to 70. ◦. ; the detector operates with an energy threshold of a few. hundred GeV. Recent achieved results will be reported""

Details

ISSN :
09205632
Database :
OpenAIRE
Journal :
Nuclear Physics B - Proceedings Supplements
Accession number :
edsair.doi.dedup.....be0e6ef1609731f2c3e6536e28db39d0
Full Text :
https://doi.org/10.1016/j.nuclphysbps.2011.03.008