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First Detection of Photons with Energy beyond 100 TeV from an Astrophysical Source.

Authors :
Amenomori M
Bao YW
Bi XJ
Chen D
Chen TL
Chen WY
Chen X
Chen Y
Cirennima
Cui SW
Danzengluobu
Ding LK
Fang JH
Fang K
Feng CF
Feng Z
Feng ZY
Gao Q
Gou QB
Guo YQ
He HH
He ZT
Hibino K
Hotta N
Hu H
Hu HB
Huang J
Jia HY
Jiang L
Jin HB
Kajino F
Kasahara K
Katayose Y
Kato C
Kato S
Kawata K
Kozai M
Labaciren
Le GM
Li AF
Li HJ
Li WJ
Lin YH
Liu B
Liu C
Liu JS
Liu MY
Lou YQ
Lu H
Meng XR
Mitsui H
Munakata K
Nakamura Y
Nanjo H
Nishizawa M
Ohnishi M
Ohta I
Ozawa S
Qian XL
Qu XB
Saito T
Sakata M
Sako TK
Sengoku Y
Shao J
Shibata M
Shiomi A
Sugimoto H
Takita M
Tan YH
Tateyama N
Torii S
Tsuchiya H
Udo S
Wang H
Wu HR
Xue L
Yagisawa K
Yamamoto Y
Yang Z
Yuan AF
Zhai LM
Zhang HM
Zhang JL
Zhang X
Zhang XY
Zhang Y
Zhang Y
Zhang Y
Zhaxisangzhu
Zhou XX
Source :
Physical review letters [Phys Rev Lett] 2019 Aug 02; Vol. 123 (5), pp. 051101.
Publication Year :
2019

Abstract

We report on the highest energy photons from the Crab Nebula observed by the Tibet air shower array with the underground water-Cherenkov-type muon detector array. Based on the criterion of a muon number measured in an air shower, we successfully suppress 99.92% of the cosmic-ray background events with energies E>100  TeV. As a result, we observed 24 photonlike events with E>100  TeV against 5.5 background events, which corresponds to a 5.6σ statistical significance. This is the first detection of photons with E>100  TeV from an astrophysical source.

Details

Language :
English
ISSN :
1079-7114
Volume :
123
Issue :
5
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
31491288
Full Text :
https://doi.org/10.1103/PhysRevLett.123.051101