A northern sky survey for ultra-high-energy gamma-ray source using the Tibet air-shower array and muon-detector array.
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Pre-published on:
July 20, 2021
Published on:
March 18, 2022
Abstract
The Tibet AS๐พ 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 ๐พ-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 ๐พ-ray sources using 719 days of data from the Tibet AS experiment. The catalog represents the sensitive survey of the northern ๐พ-ray sky at energies above several tens of TeV. These ultra-high-energy ๐พ-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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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.