Self-calibration of LHAASO-KM2A electromagnetic particle detectors using single particles within extensive air showers
dc.contributor.author | Aharonian F. | |
dc.contributor.author | An Q. | |
dc.contributor.author | Axikegu | |
dc.contributor.author | Bai L.X. | |
dc.contributor.author | Bai Y.X. | |
dc.contributor.author | Bao Y.W. | |
dc.contributor.author | Bastieri D. | |
dc.contributor.author | Bi X.J. | |
dc.contributor.author | Bi Y.J. | |
dc.contributor.author | Cai J.T. | |
dc.contributor.author | Cao Z. | |
dc.contributor.author | Cao Z. | |
dc.contributor.author | Chang J. | |
dc.contributor.author | Chang J.F. | |
dc.contributor.author | Chen E.S. | |
dc.contributor.author | Chen L. | |
dc.contributor.author | Chen L. | |
dc.contributor.author | Chen L. | |
dc.contributor.author | Chen M.J. | |
dc.contributor.author | Chen M.L. | |
dc.contributor.author | Chen Q.H. | |
dc.contributor.author | Chen S.H. | |
dc.contributor.author | Chen S.Z. | |
dc.contributor.author | Chen T.L. | |
dc.contributor.author | Chen Y. | |
dc.contributor.author | Cheng H.L. | |
dc.contributor.author | Cheng N. | |
dc.contributor.author | Cheng Y.D. | |
dc.contributor.author | Cui S.W. | |
dc.contributor.author | Cui X.H. | |
dc.contributor.author | Cui Y.D. | |
dc.contributor.author | D'Ettorre Piazzoli B. | |
dc.contributor.author | Dai B.Z. | |
dc.contributor.author | Dai H.L. | |
dc.contributor.author | Dai Z.G. | |
dc.contributor.author | Danzengluobu | |
dc.contributor.author | Della Volpe D. | |
dc.contributor.author | Duan K.K. | |
dc.contributor.author | Fan J.H. | |
dc.contributor.author | Fan Y.Z. | |
dc.contributor.author | Fan Z.X. | |
dc.contributor.author | Fang J. | |
dc.contributor.author | Fang K. | |
dc.contributor.author | Feng C.F. | |
dc.contributor.author | Feng L. | |
dc.contributor.author | Feng S.H. | |
dc.contributor.author | Feng X.T. | |
dc.contributor.author | Feng Y.L. | |
dc.contributor.author | Gao B. | |
dc.contributor.author | Gao C.D. | |
dc.contributor.author | Gao L.Q. | |
dc.contributor.author | Gao Q. | |
dc.contributor.author | Gao W. | |
dc.contributor.author | Gao W.K. | |
dc.contributor.author | Ge M.M. | |
dc.contributor.author | Geng L.S. | |
dc.contributor.author | Gong G.H. | |
dc.contributor.author | Gou Q.B. | |
dc.contributor.author | Gu M.H. | |
dc.contributor.author | Guo F.L. | |
dc.contributor.author | Guo J.G. | |
dc.contributor.author | Guo X.L. | |
dc.contributor.author | Guo Y.Q. | |
dc.contributor.author | Guo Y.Y. | |
dc.contributor.author | Han Y.A. | |
dc.contributor.author | He H.H. | |
dc.contributor.author | He H.N. | |
dc.contributor.author | He S.L. | |
dc.contributor.author | He X.B. | |
dc.contributor.author | He Y. | |
dc.contributor.author | Heller M. | |
dc.contributor.author | Hor Y.K. | |
dc.contributor.author | Hou C. | |
dc.contributor.author | Hou X. | |
dc.contributor.author | Hu H.B. | |
dc.contributor.author | Hu Q. | |
dc.contributor.author | Hu S. | |
dc.contributor.author | Hu S.C. | |
dc.contributor.author | Hu X.J. | |
dc.contributor.author | Huang D.H. | |
dc.contributor.author | Huang W.H. | |
dc.contributor.author | Huang X.T. | |
dc.contributor.author | Huang X.Y. | |
dc.contributor.author | Huang Y. | |
dc.contributor.author | Huang Z.C. | |
dc.contributor.author | Ji X.L. | |
dc.contributor.author | Jia H.Y. | |
dc.contributor.author | Jia K. | |
dc.contributor.author | Jiang K. | |
dc.contributor.author | Jiang Z.J. | |
dc.contributor.author | Jin M. | |
dc.contributor.author | Kang M.M. | |
dc.contributor.author | Ke T. | |
dc.contributor.author | Kuleshov D. | |
dc.contributor.author | Levochkin K. | |
dc.contributor.author | Li B.B. | |
dc.contributor.author | Li C. | |
dc.contributor.author | Li C. | |
dc.contributor.author | Li F. | |
dc.contributor.author | Li H.B. | |
dc.contributor.other | Mahidol University | |
dc.date.accessioned | 2023-06-18T18:15:55Z | |
dc.date.available | 2023-06-18T18:15:55Z | |
dc.date.issued | 2022-12-15 | |
dc.description.abstract | In the Large High Altitude Air Shower Observatory (LHAASO), the square kilometer array, with 5249 electromagnetic particle detectors (EDs) and 1188 muon detectors, is deployed to explore the gamma-ray sources above 30 TeV with unprecedented sensitivity and to measure primary cosmic rays in the energy range from 10 TeV to 100 PeV. The energetic particles produced by extensive air showers can serve as a continuously available source for calibration of the numerous EDs over a large area. In this study, the detector untriggered probability is first proposed to estimate the particle density at different distances from the shower core and distinguish the characteristic single-particle signal detected by each ED. This method uses science data directly, and does not require prior knowledge of the cosmic-ray elemental composition or hadronic interaction model. Experimental results show that this self-calibration can be used to determine the number of particles detected by each ED with an accuracy better than 2% within a time scale of hours, which is adequate to meet the physics requirements of the LHAASO experiment. With this high efficiency and accuracy, this calibration also provides an ideal method to monitor the detector performance throughout an expected lifetime of >10 years. | |
dc.identifier.citation | Physical Review D Vol.106 No.12 (2022) | |
dc.identifier.doi | 10.1103/PhysRevD.106.122004 | |
dc.identifier.eissn | 24700029 | |
dc.identifier.issn | 24700010 | |
dc.identifier.scopus | 2-s2.0-85144764013 | |
dc.identifier.uri | https://repository.li.mahidol.ac.th/handle/20.500.14594/86903 | |
dc.rights.holder | SCOPUS | |
dc.subject | Physics and Astronomy | |
dc.title | Self-calibration of LHAASO-KM2A electromagnetic particle detectors using single particles within extensive air showers | |
dc.type | Article | |
mu.datasource.scopus | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85144764013&origin=inward | |
oaire.citation.issue | 12 | |
oaire.citation.title | Physical Review D | |
oaire.citation.volume | 106 | |
oairecerif.author.affiliation | State Key Laboratory of Particle Detection & Electronics | |
oairecerif.author.affiliation | Yunnan Observatories | |
oairecerif.author.affiliation | Nanjing University | |
oairecerif.author.affiliation | Shanghai Astronomical Observatory Chinese Academy of Sciences | |
oairecerif.author.affiliation | Institute for Nuclear Research of the Russian Academy of Sciences | |
oairecerif.author.affiliation | Shandong University | |
oairecerif.author.affiliation | Yunnan University | |
oairecerif.author.affiliation | Institute of High Energy Physics Chinese Academy of Science | |
oairecerif.author.affiliation | University of Chinese Academy of Sciences | |
oairecerif.author.affiliation | Guangzhou University | |
oairecerif.author.affiliation | Tsinghua University | |
oairecerif.author.affiliation | Sun Yat-Sen University | |
oairecerif.author.affiliation | University of Science and Technology of China | |
oairecerif.author.affiliation | Zhengzhou University | |
oairecerif.author.affiliation | Institiúid Ard-Lénn Bhaile Átha Cliath | |
oairecerif.author.affiliation | Università degli Studi di Napoli Federico II | |
oairecerif.author.affiliation | Sichuan University | |
oairecerif.author.affiliation | National Astronomical Observatories Chinese Academy of Sciences | |
oairecerif.author.affiliation | Max-Planck-Institut für Kernphysik | |
oairecerif.author.affiliation | Southwest Jiaotong University | |
oairecerif.author.affiliation | Purple Mountain Observatory Chinese Academy of Sciences | |
oairecerif.author.affiliation | Université de Genève | |
oairecerif.author.affiliation | Hebei Normal University | |
oairecerif.author.affiliation | Tibet University | |
oairecerif.author.affiliation | TIANFU Cosmic Ray Research Center |