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000408356 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/choi_junghoon
000408356 0247_ $$2ISSN$$a1435-8077
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000408356 041__ $$aEnglish
000408356 0881_ $$aDESY-PROC-2013-04
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000408356 1001_ $$0P:(DE-HGF)0$$aChoi, J. H.$$b0$$eCorresponding author
000408356 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408356 245__ $$aAnnual modulation study of dark matter using CsI$(Tl)$ crystals in KIMS experiment
000408356 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408356 29510 $$aChoi, J.H. "Annual modulation study of dark matter using CsI(Tl) crystals in KIMS experiment" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
000408356 300__ $$a185-188
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000408356 520__ $$aThe orbital motion of the Earth can result in annual modulation signatures of dark matter. The DAMA group reported a positive signal for an annual modulation with NaI(Tl) crystal detectors. The KIMS experiment uses a CsI(Tl) crystal detector array to search for dark matter and, if the DAMA result is in fact due to WIMP interactions, can be expected to see a similar annual modulation signal. This paper presents results of a search for a dark-matter-induced annual modulation of signals in CsI(Tl) detectors over a 2.5 year period.
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000408356 7001_ $$0P:(DE-HGF)0$$aKim, B. H.$$b1
000408356 7001_ $$0P:(DE-HGF)0$$aKim, G. B.$$b2
000408356 7001_ $$0P:(DE-HGF)0$$aBhang, H. C.$$b3
000408356 7001_ $$0P:(DE-HGF)0$$aKim, H. J.$$b4
000408356 7001_ $$0P:(DE-HGF)0$$aLee, H. S.$$b5
000408356 7001_ $$0P:(DE-HGF)0$$aHahn, I. S.$$b6
000408356 7001_ $$0P:(DE-HGF)0$$aLee, J. H.$$b7
000408356 7001_ $$0P:(DE-HGF)0$$aSo, J. H.$$b8
000408356 7001_ $$0P:(DE-HGF)0$$aLee, J. K.$$b9
000408356 7001_ $$0P:(DE-HGF)0$$aLi, J.$$b10
000408356 7001_ $$0P:(DE-HGF)0$$aLi, J.$$b11
000408356 7001_ $$0P:(DE-HGF)0$$aKim, K. W.$$b12
000408356 7001_ $$0P:(DE-HGF)0$$aYue, Q.$$b13
000408356 7001_ $$0P:(DE-HGF)0$$aKim, S. C.$$b14
000408356 7001_ $$0P:(DE-HGF)0$$aChoi, S. H.$$b15
000408356 7001_ $$0P:(DE-HGF)0$$aKim, S. K.$$b16
000408356 7001_ $$0P:(DE-HGF)0$$aOlsen, S. L.$$b17
000408356 7001_ $$0P:(DE-HGF)0$$aMyung, S. S.$$b18
000408356 7001_ $$0P:(DE-HGF)0$$aKang, W. G.$$b19
000408356 7001_ $$0P:(DE-HGF)0$$aLi, X. R.$$b20
000408356 7001_ $$0P:(DE-HGF)0$$aKim, Y. D.$$b21
000408356 7001_ $$0P:(DE-HGF)0$$aLie, Y. J.$$b22
000408356 7870_ $$0PUBDB-2015-05816$$aOberlack, Uwe et. al.$$iisPartOf$$rDESY-PROC-2013-04$$tProceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
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