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000402227 020__ $$a978-3-945931-17-2
000402227 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2017-02/kim_kyungwon
000402227 0247_ $$2ISSN$$a1435-8077
000402227 037__ $$aPUBDB-2018-01756
000402227 041__ $$aEnglish
000402227 0881_ $$aDESY-PROC-2017-02
000402227 088__ $$2DESY$$aDESY-PROC-2017-02
000402227 1001_ $$0P:(DE-HGF)0$$aKim, Kyungwon$$b0$$eCorresponding author
000402227 1112_ $$0C17-05-15.4$$2inspire$$a13th Patras Workshop on Axions, WIMPs and WISPs$$cThessaloniki$$d2017-05-15 - 2017-05-19$$gAXION-WIMP 2017$$wGreece
000402227 245__ $$aStatus of the COSINE-100 Experiment
000402227 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2018
000402227 29510 $$aKim, Kyungwon "Status of the COSINE-100 Experiment" in Proceedings of the 13th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2017 / Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2018 ; Patras 2017 : 13th Patras Workshop on Axions, WIMPs and WISPs, 2017-05-15 - 2017-05-19, Thessaloniki
000402227 300__ $$a126-129
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000402227 520__ $$aPresently a number of experiments are operating to search for the WIMP, a dark matter candidate. Among these experiments, DAMA/LIBRA claims to observe an annually modulated WIMP signal, while other experiments, using different technologies and target materials, exclude the DAMA/LIBRA signal region in the parameter space. The COSINE experiment aims at exploring these contradicting results by using NaI(Tl), the same target material as DAMA/LIBRA. The first phase detector with 106 kg of NaI(Tl), COSINE-100, was installed at the Yangyang underground laboratory in Korea. It consists of several shield structures, including a liquid scintillator veto system. The experiment has started physics data taking in late September 2016 and has been operating stably since then.
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000402227 7001_ $$0P:(DE-HGF)0$$aCOSINE Collaboration$$b1$$eCollaboration author
000402227 7870_ $$0PUBDB-2018-01183$$aMaroudas, Marios$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2017-02$$tProceedings of the 13th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2017
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