The Application of 20 inch MCP-PMT In LHAASO-WCDA

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dc.contributor.authorYou X.
dc.contributor.otherMahidol University
dc.date.accessioned2023-06-18T18:06:22Z
dc.date.available2023-06-18T18:06:22Z
dc.date.issued2022-03-18
dc.description.abstractIn the Large High Altitude Air Shower Observatory (LHAASO), the main physics objective of the Water Cherenkov Detector Array (WCDA) is to survey the gamma-ray sky continuously in the energy range from 100 GeV to PeV. The Water Cherenkov detector array, covering an area of about 78,000 m2 area, is constituted by 3120 detector units divided into 3 separate arrays. In the second and third array are installed 2220 20" PMTs instead of the 8 PMT used in the first 150 × 150m2 array. This type of PMT has large sensitive area, high quantum efficiency (QE), and large peak-to-valley (P/V) ratio for single photoelectron detection. In this work, we will report on the application of 20 inch MCP-PMT at LHAASO-WCDA.
dc.identifier.citationProceedings of Science Vol.395 (2022)
dc.identifier.eissn18248039
dc.identifier.scopus2-s2.0-85145017975
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/20.500.14594/86557
dc.rights.holderSCOPUS
dc.subjectMultidisciplinary
dc.titleThe Application of 20 inch MCP-PMT In LHAASO-WCDA
dc.typeConference Paper
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85145017975&origin=inward
oaire.citation.titleProceedings of Science
oaire.citation.volume395
oairecerif.author.affiliationState Key Laboratory of Particle Detection & Electronics
oairecerif.author.affiliationNanjing University
oairecerif.author.affiliationShanghai Astronomical Observatory Chinese Academy of Sciences
oairecerif.author.affiliationInstitute for Nuclear Research of the Russian Academy of Sciences
oairecerif.author.affiliationShandong University
oairecerif.author.affiliationWuhan University
oairecerif.author.affiliationYunnan University
oairecerif.author.affiliationInstitute of High Energy Physics Chinese Academy of Science
oairecerif.author.affiliationUniversity of Chinese Academy of Sciences
oairecerif.author.affiliationGuangzhou University
oairecerif.author.affiliationTsinghua University
oairecerif.author.affiliationSun Yat-Sen University
oairecerif.author.affiliationUniversity of Science and Technology of China
oairecerif.author.affiliationZhengzhou University
oairecerif.author.affiliationInstitiúid Ard-Lénn Bhaile Átha Cliath
oairecerif.author.affiliationUniversità degli Studi di Napoli Federico II
oairecerif.author.affiliationSichuan University
oairecerif.author.affiliationNational Astronomical Observatories Chinese Academy of Sciences
oairecerif.author.affiliationMax-Planck-Institut für Kernphysik
oairecerif.author.affiliationSouthwest Jiaotong University
oairecerif.author.affiliationPurple Mountain Observatory Chinese Academy of Sciences
oairecerif.author.affiliationUniversité de Genève
oairecerif.author.affiliationHebei Normal University
oairecerif.author.affiliationTibet University
oairecerif.author.affiliationTIANFU Cosmic Ray Research Center

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