Underground water Cherenkov muon detector array with the Tibet air shower array for gamma-ray astronomy in the 100 TeV region
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Amenomori, M
a
Ayabe, S
b
Bi, X J
c
Chen, D
d
Cui, S W
e
Danzengluobu,
f
Ding, L K
c
Ding, X H
f
Feng, C F
g
Feng, Zhaoyang
c
Feng, Z Y
h
Gao, X Y
i
Geng, Q X
i
Guo, H W
f
He, H H
c
He, M
g
Hibino, K
j
Hotta, N
k
Hu, Haibing
f
Hu, H B
c
Huang, J
l
Huang, Q
h
Jia, H Y
h
Kajino, F
m
Kasahara, K
n
Katayose, Y
d
Kato, C
o
Kawata, K
l
Labaciren,
f
Le, G M
p
Li, A F
g
Li, J Y
g
Lu, H
c
Lu, S L
c
Meng, X R
f
Mizutani, K
b,q
Mu, J
i
Munakata, K
o
Nagai, A
k
Nanjo, H
a
Nishizawa, M
r
Ohnishi, M
l
Ohta, I
s
Onuma, H
b
Ouchi, T
j
Ozawa, S
l
Ren, J R
c
Saito, T
t
Saito, T Y
l
Sakata, M
m
Sako, T K
l
Sasaki, T
j
Shibata, M
d
Shiomi, A
l
Shirai, T
j
Sugimoto, H
u
Takita, M
l
Tan, Y H
c
Tateyama, N
j
Torii, S
q
Tsuchiya, H
v
Udo, S
l
Wang, B
i
Wang, H
c
Wang, X
l
Wang, Y G
g
Wu, H R
c
Xue, L
g
Yamamoto, Y
m
Yan, C T
l
Yang, X C
i
Yasue, S
o
Ye, Z H
p
Yu, G C
h
Yuan, A F
f
Yuda, T
j
Zhang, H M
c
Zhang, J L
c
Zhang, N J
g
Zhang, X Y
g
Zhang, Y
c
Zhang, Yi
c
Zhaxisangzhu,
f
Zhou, X X
h
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