Publication:
A dynamic range extension system for LHAASO WCDA-1

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dc.contributor.authorF. Aharonianen_US
dc.contributor.authorQ. Anen_US
dc.contributor.authorAxikeguen_US
dc.contributor.authorL. X. Baien_US
dc.contributor.authorY. X. Baien_US
dc.contributor.authorY. W. Baoen_US
dc.contributor.authorD. Bastierien_US
dc.contributor.authorX. J. Bien_US
dc.contributor.authorY. J. Bien_US
dc.contributor.authorH. Caien_US
dc.contributor.authorJ. T. Caien_US
dc.contributor.authorZ. Caoen_US
dc.contributor.authorZ. Caoen_US
dc.contributor.authorJ. Changen_US
dc.contributor.authorJ. F. Changen_US
dc.contributor.authorX. C. Changen_US
dc.contributor.authorB. M. Chenen_US
dc.contributor.authorJ. Chenen_US
dc.contributor.authorL. Chenen_US
dc.contributor.authorL. Chenen_US
dc.contributor.authorL. Chenen_US
dc.contributor.authorM. J. Chenen_US
dc.contributor.authorM. L. Chenen_US
dc.contributor.authorQ. H. Chenen_US
dc.contributor.authorS. H. Chenen_US
dc.contributor.authorS. Z. Chenen_US
dc.contributor.authorT. L. Chenen_US
dc.contributor.authorX. L. Chenen_US
dc.contributor.authorY. Chenen_US
dc.contributor.authorN. Chengen_US
dc.contributor.authorY. D. Chengen_US
dc.contributor.authorS. W. Cuien_US
dc.contributor.authorX. H. Cuien_US
dc.contributor.authorY. D. Cuien_US
dc.contributor.authorB. Z. Daien_US
dc.contributor.authorH. L. Daien_US
dc.contributor.authorZ. G. Daien_US
dc.contributor.authorDanzengluobuen_US
dc.contributor.authorD. della Volpeen_US
dc.contributor.authorB. D’Ettorre Piazzolien_US
dc.contributor.authorX. J. Dongen_US
dc.contributor.authorJ. H. Fanen_US
dc.contributor.authorY. Z. Fanen_US
dc.contributor.authorZ. X. Fanen_US
dc.contributor.authorJ. Fangen_US
dc.contributor.authorK. Fangen_US
dc.contributor.authorC. F. Fengen_US
dc.contributor.authorL. Fengen_US
dc.contributor.authorS. H. Fengen_US
dc.contributor.authorY. L. Fengen_US
dc.contributor.authorB. Gaoen_US
dc.contributor.authorC. D. Gaoen_US
dc.contributor.authorQ. Gaoen_US
dc.contributor.authorW. Gaoen_US
dc.contributor.authorM. M. Geen_US
dc.contributor.authorL. S. Gengen_US
dc.contributor.authorG. H. Gongen_US
dc.contributor.authorQ. B. Gouen_US
dc.contributor.authorM. H. Guen_US
dc.contributor.authorJ. G. Guoen_US
dc.contributor.authorX. L. Guoen_US
dc.contributor.authorY. Q. Guoen_US
dc.contributor.authorY. Y. Guoen_US
dc.contributor.authorY. A. Hanen_US
dc.contributor.authorH. H. Heen_US
dc.contributor.authorH. N. Heen_US
dc.contributor.authorJ. C. Heen_US
dc.contributor.authorS. L. Heen_US
dc.contributor.authorX. B. Heen_US
dc.contributor.authorY. Heen_US
dc.contributor.authorM. Helleren_US
dc.contributor.authorY. K. Horen_US
dc.contributor.authorC. Houen_US
dc.contributor.authorX. Houen_US
dc.contributor.authorH. B. Huen_US
dc.contributor.authorS. Huen_US
dc.contributor.authorS. C. Huen_US
dc.contributor.authorX. J. Huen_US
dc.contributor.authorD. H. Huangen_US
dc.contributor.authorQ. L. Huangen_US
dc.contributor.authorW. H. Huangen_US
dc.contributor.authorX. T. Huangen_US
dc.contributor.authorY. Huangen_US
dc.contributor.authorZ. C. Huangen_US
dc.contributor.authorF. Jien_US
dc.contributor.authorX. L. Jien_US
dc.contributor.authorH. Y. Jiaen_US
dc.contributor.authorK. Jiangen_US
dc.contributor.authorZ. J. Jiangen_US
dc.contributor.authorC. Jinen_US
dc.contributor.authorD. Kuleshoven_US
dc.contributor.authorK. Levochkinen_US
dc.contributor.authorB. B. Lien_US
dc.contributor.authorC. Lien_US
dc.contributor.authorC. Lien_US
dc.contributor.authorF. Lien_US
dc.contributor.authorH. B. Lien_US
dc.contributor.authorH. C. Lien_US
dc.contributor.authorH. Y. Lien_US
dc.contributor.authorJ. Lien_US
dc.contributor.otherState Key Laboratory of Particle Detection & Electronicsen_US
dc.contributor.otherNanjing Universityen_US
dc.contributor.otherShanghai Astronomical Observatory Chinese Academy of Sciencesen_US
dc.contributor.otherInstitute for Nuclear Research of the Russian Academy of Sciencesen_US
dc.contributor.otherShandong Universityen_US
dc.contributor.otherWuhan Universityen_US
dc.contributor.otherYunnan Universityen_US
dc.contributor.otherInstitute of High Energy Physics Chinese Academy of Scienceen_US
dc.contributor.otherUniversity of Chinese Academy of Sciencesen_US
dc.contributor.otherGuangzhou Universityen_US
dc.contributor.otherTsinghua Universityen_US
dc.contributor.otherSun Yat-Sen Universityen_US
dc.contributor.otherUniversity of Science and Technology of Chinaen_US
dc.contributor.otherZhengzhou Universityen_US
dc.contributor.otherDublin Institute for Advanced Studiesen_US
dc.contributor.otherUniversità degli Studi di Napoli Federico IIen_US
dc.contributor.otherSichuan Universityen_US
dc.contributor.otherNational Astronomical Observatories Chinese Academy of Sciencesen_US
dc.contributor.otherMax-Planck-Institut für Kernphysiken_US
dc.contributor.otherSouthwest Jiaotong Universityen_US
dc.contributor.otherPurple Mountain Observatory Chinese Academy of Sciencesen_US
dc.contributor.otherUniversité de Genèveen_US
dc.contributor.otherHebei Normal Universityen_US
dc.contributor.otherTibet Universityen_US
dc.contributor.otherTIANFU Cosmic Ray Research Centeren_US
dc.date.accessioned2022-08-04T08:33:31Z
dc.date.available2022-08-04T08:33:31Z
dc.date.issued2021-12-01en_US
dc.description.abstractPurpose: The main scientific goal of LHAASO-WCDA is to survey gamma-ray sources with energy from 100 GeV to 30 TeV. To observe high-energy shower events, especially to measure the energy spectrum of cosmic rays from 100 TeV to 10 PeV, a dynamic range extension system (WCDA++) is designed to use a 1.5-inch PMT with a dynamic range of four orders of magnitude for each cell in WCDA-1. Method: The dynamic range is extended by using these PMTs to measure the effective charge density in the core region of air shower events, which is an important parameter for identifying the composition of primary particles. Result and Conclusion: The system has been running for more than one year. In this paper, the details of the design and performance of WCDA++ are presented.en_US
dc.identifier.citationRadiation Detection Technology and Methods. Vol.5, No.4 (2021), 520-530en_US
dc.identifier.doi10.1007/s41605-021-00275-4en_US
dc.identifier.issn25099949en_US
dc.identifier.issn25099930en_US
dc.identifier.other2-s2.0-85114164158en_US
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/20.500.14594/76890
dc.rightsMahidol Universityen_US
dc.rights.holderSCOPUSen_US
dc.source.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85114164158&origin=inwarden_US
dc.subjectEnergyen_US
dc.subjectPhysics and Astronomyen_US
dc.titleA dynamic range extension system for LHAASO WCDA-1en_US
dc.typeArticleen_US
dspace.entity.typePublication
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85114164158&origin=inwarden_US

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