Pith. sign in

REVIEW

Gamma-ray Observation of the Cygnus Region in the 100 TeV Energy Region

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2107.01064 v1 pith:IZFJUCRG submitted 2021-07-02 astro-ph.HE

Gamma-ray Observation of the Cygnus Region in the 100 TeV Energy Region

M. Amenomori , Y. W. Bao , X. J. Bi , D. Chen , T. L. Chen , W. Y. Chen , Xu Chen , Y. Chen
show 105 more authors
Cirennima S. W. Cui Danzengluobu L. K. Ding J. H. Fang K. Fang C. F. Feng Zhaoyang Feng Z. Y. Feng Qi Gao A. Gomi Q. B. Gou Y. Q. Guo Y. Y. Guo H. H. He Z. T. He K. Hibino N. Hotta Haibing Hu H. B. Hu J. Huang H. Y. Jia L. Jiang P. Jiang H. B. Jin K. Kasahara Y. Katayose C. Kato S. Kato K. Kawata M. Kozai D. Kurashige Labaciren G. M. Le A. F. Li H. J. Li W. J. Li Y. Li Y. H. Lin B. Liu C. Liu J. S. Liu L. Y. Liu M. Y. Liu W. Liu X. L. Liu Y.-Q. Lou H. Lu X. R. Meng K. Munakata H. Nakada Y. Nakamura Y. Nakazawa H. Nanjo C. C. Ning M. Nishizawa M. Ohnishi T. Ohura S. Okukawa S. Ozawa L. Qian X. Qian X. L. Qian X. B. Qu T. Saito M. Sakata T. Sako T. K. Sako J. Shao M. Shibata A. Shiomi H. Sugimoto W. Takano M. Takita Y. H. Tan N. Tateyama S. Torii H. Tsuchiya S. Udo H. Wang Y. P. Wang Wangdui H. R. Wu Q. Wu J. L. Xu L. Xue Y. Yamamoto Z. Yang Y. Q. Yao J. Yin Y. Yokoe N. P. Yu A. F. Yuan L. M. Zhai C. P. Zhang H. M. Zhang J. L. Zhang X. Zhang X. Y. Zhang Y. Zhang Yi Zhang Ying Zhang S. P. Zhao Zhaxisangzhu X. X. Zhou (The Tibet AS$\gamma$ Collaboration)
This is my paper
classification astro-ph.HE
keywords gamma-rayregioncygnuspulsarenergysourcesaccelerationaround
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

We report observations of gamma-ray emissions with energies in the 100 TeV energy region from the Cygnus region in our Galaxy. Two sources are significantly detected in the directions of the Cygnus OB1 and OB2 associations. Based on their positional coincidences, we associate one with a pulsar PSR J2032+4127 and the other mainly with a pulsar wind nebula PWN G75.2+0.1 with the pulsar moving away from its original birthplace situated around the centroid of the observed gamma-ray emission. This work would stimulate further studies of particle acceleration mechanisms at these gamma-ray sources.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.