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000408357 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/marrodan_undagoitia_teresa
000408357 0247_ $$2ISSN$$a1435-8077
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000408357 1001_ $$0P:(DE-HGF)0$$aMarrodán Undagoitia, T.$$b0$$eCorresponding author
000408357 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408357 245__ $$aDirect Dark Matter Search with XENON
000408357 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408357 29510 $$aUndagoitia, T.Marrodán "Direct Dark Matter Search with XENON" 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
000408357 300__ $$a189-194
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000408357 500__ $$aLiteraturangaben; English
000408357 520__ $$aDirect dark matter searches using liquid xenon have shown a great potential to detect WIMPs (Weakly Interacting Massive Particles) via elastic scattering off the target nuclei. XENON100 operates with an active volume of 62 kg liquid xenon and it is located at the Gran Sasso underground laboratory in Italy. So far the data released provides no evidence for dark matter. The resulting exclusion limits on the WIMP-nucleon cross section for spin-dependent and-independent interactions probe already significant regions of the cross section and WIMP mass parameter space. The XENON1T experiment currently under construction will improve the current sensitivity by two orders of magnitude. 
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000408357 7001_ $$0P:(DE-HGF)0$$aXENON Collaboration$$b1$$eCollaboration author
000408357 7870_ $$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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