Publication:
Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array

8

item.page.dc.date.issued

2020-06-01

item.page.dc.type

Article

item.page.dc.identifier.issn

16741137

item.page.dc.identifier.doi

10.1088/1674-1137/44/6/065001

item.page.dc.identifier.other

2-s2.0-85087341360

item.page.dc.rights

Mahidol University

item.page.dc.rights.holder

SCOPUS

item.page.dc.identifier.citation

Chinese Physics C. Vol.44, No.6 (2020)

punsarn.item.page.citation

F. Aharonian, V. Alekseenko, Q. An, Axikegu, 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, Danzengluobu, 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 Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array. Chinese Physics C. Vol.44, No.6 (2020). doi:10.1088/1674-1137/44/6/065001 Retrieved from: https://repository.li.mahidol.ac.th/handle/123456789/58369

Research Projects

Organizational Units

Authors

Journal Issue

relationships.isThesisOf

item.page.dc.title

Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array

item.page.dc.contributor.author

F. Aharonian
 V. Alekseenko
 Q. An
 Axikegu
 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
 Danzengluobu
 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

item.page.dc.contributor.other

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

item.page.dc.description.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).

item.page.dc.subject

Physics and Astronomy

item.page.availability

URI

https://repository.li.mahidol.ac.th/handle/123456789/58369

Collections

Scopus 2020