Peta–electron volt gamma-ray emission from the Crab Nebula-Reference-Cited by-同舟云学术

Peta–electron volt gamma-ray emission from the Crab Nebula

Published:2021-07-23 Issue:6553 Volume:373 Page:425-430
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

,Cao Zhen^ORCID,Aharonian F.^ORCID,An Q.,Axikegu ,Bai L. X.,Bai Y. X.,Bao Y. W.^ORCID,Bastieri D.^ORCID,Bi X. J.^ORCID,Bi Y. J.,Cai H.,Cai J. T.,Cao Zhe,Chang J.^ORCID,Chang J. F.,Chen B. M.,Chen E. S.,Chen J.,Chen Liang^ORCID,Chen Liang,Chen Long,Chen M. J.,Chen M. L.,Chen Q. H.^ORCID,Chen S. H.,Chen S. Z.^ORCID,Chen T. L.^ORCID,Chen X. L.,Chen Y.,Cheng N.,Cheng Y. D.^ORCID,Cui S. W.^ORCID,Cui X. H.^ORCID,Cui Y. D.,D’Ettorre Piazzoli B.,Dai B. Z.^ORCID,Dai H. L.,Dai Z. G.,Danzengluobu ,della Volpe D.^ORCID,Dong X. J.,Duan K. K.,Fan J. H.^ORCID,Fan Y. Z.^ORCID,Fan Z. X.,Fang J.,Fang K.^ORCID,Feng C. F.^ORCID,Feng L.,Feng S. H.,Feng Y. L.,Gao B.,Gao C. D.,Gao L. Q.,Gao Q.,Gao W.^ORCID,Ge M. M.,Geng L. S.,Gong G. H.^ORCID,Gou Q. B.,Gu M. H.,Guo F. L.,Guo J. G.^ORCID,Guo X. L.,Guo Y. Q.,Guo Y. Y.,Han Y. A.^ORCID,He H. H.^ORCID,He H. N.^ORCID,He J. C.,He S. L.,He X. B.,He Y.,Heller M.^ORCID,Hor Y. K.,Hou C.,Hou X.,Hu H. B.,Hu S.,Hu S. C.,Hu X. J.,Huang D. H.,Huang Q. L.,Huang W. H.,Huang X. T.^ORCID,Huang X. Y.,Huang Z. C.,Ji F.,Ji X. L.,Jia H. Y.,Jiang K.,Jiang Z. J.,Jin C.,Ke T.,Kuleshov D.^ORCID,Levochkin K.,Li B. B.,Li Cheng,Li Cong^ORCID,Li F.,Li H. B.,Li H. C.,Li H. Y.,Li Jian,Li Jie,Li K.,Li W. L.,Li X. R.,Li Xin,Li Xin,Li Y.,Li Y. Z.,Li Zhe,Li Zhuo,Liang E. W.^ORCID,Liang Y. F.,Lin S. J.^ORCID,Liu B.^ORCID,Liu C.,Liu D.,Liu H.,Liu H. D.^ORCID,Liu J.,Liu J. L.,Liu J. S.,Liu J. Y.,Liu M. Y.,Liu R. Y.^ORCID,Liu S. M.^ORCID,Liu W.,Liu Y.,Liu Y. N.,Liu Z. X.,Long W. J.^ORCID,Lu R.,Lv H. K.,Ma B. Q.^ORCID,Ma L. L.,Ma X. H.^ORCID,Mao J. R.^ORCID,Masood A.,Min Z.,Mitthumsiri W.^ORCID,Montaruli T.,Nan Y. C.,Pang B. Y.,Pattarakijwanich P.,Pei Z. Y.^ORCID,Qi M. Y.,Qi Y. Q.,Qiao B. Q.,Qin J. J.,Ruffolo D.^ORCID,Rulev V.,Saiz A.^ORCID,Shao L.^ORCID,Shchegolev O.,Sheng X. D.,Shi J. Y.,Song H. C.,Stenkin Yu. V.^ORCID,Stepanov V.,Su Y.,Sun Q. N.,Sun X. N.^ORCID,Sun Z. B.,Tam P. H. T.^ORCID,Tang Z. B.^ORCID,Tian W. W.,Wang B. D.,Wang C.,Wang H.,Wang H. G.,Wang J. C.,Wang J. S.^ORCID,Wang L. P.,Wang L. Y.^ORCID,Wang R. N.,Wang Wei^ORCID,Wang Wei,Wang X. G.^ORCID,Wang X. J.^ORCID,Wang X. Y.,Wang Y.,Wang Y. D.,Wang Y. J.,Wang Y. P.,Wang Z. H.,Wang Z. X.,Wang Zhen,Wang Zheng,Wei D. M.^ORCID,Wei J. J.,Wei Y. J.,Wen T.,Wu C. Y.,Wu H. R.,Wu S.,Wu W. X.,Wu X. F.^ORCID,Xi S. Q.,Xia J.,Xia J. J.,Xiang G. M.,Xiao D. X.,Xiao G.,Xiao H. B.,Xin G. G.,Xin Y. L.^ORCID,Xing Y.,Xu D. L.,Xu R. X.,Xue L.,Yan D. H.,Yan J. Z.,Yang C. W.,Yang F. F.^ORCID,Yang J. Y.,Yang L. L.,Yang M. J.,Yang R. Z.^ORCID,Yang S. B.,Yao Y. H.,Yao Z. G.^ORCID,Ye Y. M.,Yin L. Q.^ORCID,Yin N.,You X. H.,You Z. Y.,Yu Y. H.,Yuan Q.^ORCID,Zeng H. D.^ORCID,Zeng T. X.,Zeng W.,Zeng Z. K.,Zha M.^ORCID,Zhai X. X.,Zhang B. B.^ORCID,Zhang H. M.,Zhang H. Y.,Zhang J. L.,Zhang J. W.,Zhang L. X.,Zhang Li,Zhang Lu,Zhang P. F.,Zhang P. P.,Zhang R.,Zhang S. R.,Zhang S. S.^ORCID,Zhang X.,Zhang X. P.,Zhang Y. F.,Zhang Y. L.,Zhang Yi^ORCID,Zhang Yong,Zhao B.,Zhao J.,Zhao L.,Zhao L. Z.,Zhao S. P.,Zheng F.,Zheng Y.,Zhou B.,Zhou H.,Zhou J. N.,Zhou P.,Zhou R.,Zhou X. X.,Zhu C. G.,Zhu F. R.,Zhu H.,Zhu K. J.,Zuo X.

Abstract

High-energy photons from the Crab Nebula The Crab Nebula contains a pulsar that excites the surrounding gas to emit high-energy radiation. The combination of the pulsar's youth and nearby location makes the nebula the brightest gamma-ray source in the sky. The LHAASO Collaboration report observations of this source at energies of tera– to peta–electron volts, extending the spectrum of this prototypical object. They combine these data with observations at lower energies to model the physics of the emission process. The multiwave-length data can be explained by a combination of synchrotron radiation and inverse Compton scattering. Science , abg5137, this issue p. 425

Funder

National Natural Science Foundation of China

National Key Research and Development Program of China Stem Cell and Translational Research

Thailand Science Research and Innovation

China by National Key R&D

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference63 articles.

1. Suspected New Stars Recorded in Old Chronicles and Among Recent Meridian Observations

2. Ground- and Space-Based Gamma-Ray Astronomy

3. Detection of Small Flares from the Crab Nebula with Fermi-LAT

4. Measurement of the Crab Nebula spectrum over three decades in energy with the MAGIC telescopes

5. The Crab Nebula and Pulsar between 500 GeV and 80 TeV: Observations with the HEGRA Stereoscopic Air Cerenkov Telescopes

Cited by 94 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Method to measure muon content of extensive air showers with LHAASO KM2A-WCDA synergy;Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment;2024-02

2. The expected potential of hadronic PeVatron searches with spectral γ-ray data from the Southern Wide-field Gamma-ray Observatory;Astroparticle Physics;2024-02

3. Determining the Origin of Very-high-energy Gamma Rays from Galactic Sources by Future Neutrino Observations;The Astrophysical Journal;2024-01-31

4. On the Source Contribution to the Galactic Diffuse Gamma Rays above 398 TeV Detected by the Tibet ASγ Experiment;The Astrophysical Journal Letters;2024-01-01

5. Silicon Photomultiplier selection for Large Array of Imaging Atmospheric Cherenkov Telescopes;Journal of Instrumentation;2024-01-01