PoS - Proceedings of Science
Volume 395 - 37th International Cosmic Ray Conference (ICRC2021) - GAI - Gamma Ray Indirect
A northern sky survey for ultra-high-energy gamma-ray source using the Tibet air-shower array and muon-detector array.
X.ย Chen* ย on behalf of the Tibet ASgamma Collaboration
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Pre-published on: July 20, 2021
Published on: March 18, 2022
The Tibet AS๐›พ experiment located at 4300 m above sea level, Tibet, China, has a wide field of view and large effective area. It consists of the Tibet air-shower array (Tibet-AS), the air-shower core- detector array (YAC) and the underground water-Cherenkov muon-detector array (Tibet-MD). The Tibet-MD array significantly improves ๐›พ-ray sensitivity in the 10-1000 TeV energy region by an order of magnitude better than any other previously existing experiments in the world. In this work we will present the catalog of TeV ๐›พ-ray sources using 719 days of data from the Tibet AS experiment. The catalog represents the sensitive survey of the northern ๐›พ-ray sky at energies above several tens of TeV. These ultra-high-energy ๐›พ-ray sources are believed to be related to pulsars and supernova remnants.
DOI: https://doi.org/10.22323/1.395.0880
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