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000408359 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/kozlov_valentin
000408359 0247_ $$2ISSN$$a1435-8077
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000408359 0881_ $$aDESY-PROC-2013-04
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000408359 1001_ $$0P:(DE-HGF)0$$aKozlov, V.$$b0$$eCorresponding author
000408359 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408359 245__ $$aThe EDELWEISS Dark Matter search program
000408359 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408359 29510 $$aKozlov, V. "The EDELWEISS Dark Matter search program" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
000408359 300__ $$a195-200
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000408359 520__ $$aThe Edelweiss experiment is a direct Dark Matter search experiment with a primary goal to detect Weakly Interacting Massive Particles (WIMPs). The setup is installed in the Modane underground laboratory (LSM, France) in French- Italian Alps. The second phase of the experiment was completed in 2011 and results are published setting new limits on the spin-independent WIMP-nucleon scattering cross-section and excluding most of the parameter space favored in some recent experimental hints. Currently the upgrades of the setup towards better sensitivity are being finalized and new detectors are being installed. The scientific goals of Edelweiss-III program will be presented, including improvements of the background, data-acquisition and measurements with a subset of the forty 800-g detectors. Ongoing installation works of the Edelweiss-III setup and further plans for a next generation experiment, EURECA, are discussed.
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000408359 7001_ $$0P:(DE-HGF)0$$aEDELWEISS Collaboration$$b1$$eCollaboration author
000408359 7870_ $$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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