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dc.contributor.authorWA105 collaboration
dc.date.accessioned2021-10-19T06:31:01Z
dc.date.available2021-10-19T06:31:01Z
dc.date.issued2021
dc.identifier.citationWA105 collaboration. (2021). Performance study of a 3×1×1 m3 dual phase liquid Argon Time Projection Chamber exposed to cosmic rays. <i>Journal of Instrumentation</i>, <i>16</i>(8), Article P08063. <a href="https://doi.org/10.1088/1748-0221/16/08/P08063" target="_blank">https://doi.org/10.1088/1748-0221/16/08/P08063</a>
dc.identifier.otherCONVID_101505046
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/78252
dc.description.abstractWe report the results of the analyses of the cosmic ray data collected with a 4 tonne (3×1×1 m3) active mass (volume) Liquid Argon Time-Projection Chamber (TPC) operated in a dual-phase mode. We present a detailed study of the TPC's response, its main detector parameters and performance. The results are important for the understanding and further developments of the dual-phase technology, thanks to the verification of key aspects, such as the extraction of electrons from liquid to gas and their amplification through the entire one square metre readout plain, gain stability, purity and charge sharing between readout views.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherIOP Publishing
dc.relation.ispartofseriesJournal of Instrumentation
dc.rightsCC BY 4.0
dc.subject.otherlarge detector systems for particle and astroparticle physics
dc.subject.otherneutrino detectors
dc.subject.otherparticle tracking detectors
dc.subject.othertime projection chambers
dc.titlePerformance study of a 3×1×1 m3 dual phase liquid Argon Time Projection Chamber exposed to cosmic rays
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202110195281
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.description.reviewstatuspeerReviewed
dc.relation.issn1748-0221
dc.relation.numberinseries8
dc.relation.volume16
dc.type.versionpublishedVersion
dc.rights.copyright© 2021 CERN. Published by IOP Publishing Ltd on behalf of Sissa Medialab
dc.rights.accesslevelopenAccessfi
dc.subject.ysokosminen säteily
dc.subject.ysoneutriinot
dc.subject.ysohiukkasfysiikka
dc.subject.ysotutkimuslaitteet
dc.subject.ysoilmaisimet
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14258
jyx.subject.urihttp://www.yso.fi/onto/yso/p5219
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p2440
jyx.subject.urihttp://www.yso.fi/onto/yso/p4220
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1088/1748-0221/16/08/P08063
jyx.fundinginformationThis work would not have been possible without the support of the Swiss National Science Foundation, Switzerland; CEA and CNRS/IN2P3, France; KEK and the JSPS program, Japan; Ministerio de Ciencia e Innovación in Spain under grants FPA2016-77347-C2, SEV-2016-0588 and MdM-2015-0509, Comunidad de Madrid, the CERCA program of the Generalitat de Catalunya and the fellowship (LCF/BQ/DI18/11660043) from “La Caixa” Foundation (ID 100010434); the Programme PNCDI III, CERN-RO, under Contract 2/2020, Romania; the U.S. Department of Energy under Grant No. DE-SC0011686. This project has received funding from the European Union’s Horizon 2020 Research and Innovation program under Grant Agreement no. 654168. The authors are also grateful to the French government operated by the National Research Agency (ANR) for the LABEX Enigmass, LABEX Lyon Institute of Origins (ANR-10-LABX-0066) of the Université de Lyon for its financial support within the program “Investissements d’Avenir” (ANR-11-IDEX-0007).


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