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Title: Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array
Authors: F. Aharonian
V. Alekseenko
Q. An
L. X. Bai
Y. W. Bao
D. Bastieri
X. J. Bi
H. Cai
Zhe Cao
Zhen Cao
J. Chang
J. F. Chang
X. C. Chang
S. P. Chao
B. M. Chen
J. Chen
L. Chen
L. Chen
M. L. Chen
M. J. Chen
Q. H. Chen
S. H. Chen
S. Z. Chen
T. L. Chen
X. L. Chen
Y. Chen
N. Cheng
Y. D. Cheng
S. W. Cui
X. H. Cui
Y. D. Cui
B. Z. Dai
H. L. Dai
Z. G. Dai
B. D'Ettorre Piazzoli
J. Fang
J. H. Fan
Y. Z. Fan
C. F. Feng
L. Feng
S. H. Feng
Y. L. Feng
B. Gao
Q. Gao
W. Gao
M. M. Ge
L. S. Geng
G. H. Gong
Q. B. Gou
M. H. Gu
Y. Q. Guo
Y. Y. Guo
Y. A. Han
H. H. He
J. C. He
M. Heller
S. L. He
Y. He
C. Hou
D. H. Huang
Q. L. Huang
W. H. Huang
X. T. Huang
H. B. Hu
S. Hu
H. Y. Jia
K. Jiang
F. Ji
C. Jin
X. L. Ji
K. Levochkin
E. W. Liang
Y. F. Liang
Cheng Li
Cong Li
F. Li
H. Li
H. B. Li
H. C. Li
H. M. Li
J. Li
K. Li
W. L. Li
X. Li
X. R. Li
Y. Li
Z. Li
Z. Li
B. Liu
C. Liu
D. Liu
H. D. Liu
H. Liu
J. Liu
J. Y. Liu
M. Y. Liu
R. Y. Liu
S. M. Liu
Nanjing University
Shanghai Astronomical Observatory Chinese Academy of Sciences
Institute for Nuclear Research of the Russian Academy of Sciences
Shandong University
Guangxi University
Wuhan University
Yunnan University
Institute of High Energy Physics Chinese Academy of Science
University of Chinese Academy of Sciences
Guangzhou University
Tsinghua University
Sun Yat-Sen University
University of Science and Technology of China
Zhengzhou University
Dublin Institute for Advanced Studies
Università degli Studi di Napoli Federico II
Sichuan University
Peking University
National Astronomical Observatories Chinese Academy of Sciences
Southwest Jiaotong University
Purple Mountain Observatory Chinese Academy of Sciences
Université de Genève
Hebei Normal University
Tibet University
TIANFU Cosmic Ray Research Center
Max-Planck-Institut für Physiologie
Keywords: Physics and Astronomy
Issue Date: 1-Jun-2020
Citation: Chinese Physics C. Vol.44, No.6 (2020)
Abstract: © 2020 Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd. The Water Cherenkov Detector Array (WCDA) is a major component of the Large High Altitude Air Shower Array Observatory (LHAASO), a new generation cosmic-ray experiment with unprecedented sensitivity, currently under construction. WCDA is aimed at the study of TeV γ-rays. In order to evaluate the prospects of searching for TeV γ-ray sources with WCDA, we present a projection of the one-year sensitivity of WCDA to TeV γ-ray sources from TeVCat using an all-sky approach. Out of 128 TeVCat sources observable by WCDA up to a zenith angle of*circ;, we estimate that 42 would be detectable in one year of observations at a median energy of 1 TeV. Most of them are Galactic sources, and the extragalactic sources are Active Galactic Nuclei (AGN).
ISSN: 16741137
Appears in Collections:Scopus 2020

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