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020 _ _ |a 978-3-945931-17-2
024 7 _ |a 10.3204/DESY-PROC-2017-02/kim_kyungwon
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037 _ _ |a PUBDB-2018-01756
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088 _ _ |a DESY-PROC-2017-02
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100 1 _ |a Kim, Kyungwon
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111 2 _ |a 13th Patras Workshop on Axions, WIMPs and WISPs
|c Thessaloniki
|d 2017-05-15 - 2017-05-19
|g AXION-WIMP 2017
|0 C17-05-15.4
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245 _ _ |a Status of the COSINE-100 Experiment
260 _ _ |a Hamburg
|c 2018
|b Verlag Deutsches Elektronen-Synchrotron
295 1 0 |a Kim, 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
300 _ _ |a 126-129
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520 _ _ |a Presently 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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700 1 _ |a COSINE Collaboration
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787 0 _ |a Maroudas, Marios
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|t Proceedings of the 13th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2017
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