000316770 001__ 316770
000316770 005__ 20211110140507.0
000316770 020__ $$a978-3-935702-43-0
000316770 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2015-02/villar_patricia
000316770 0247_ $$2ISSN$$a1435-8077
000316770 037__ $$aPUBDB-2017-00168
000316770 041__ $$aEnglish
000316770 1001_ $$0P:(DE-HGF)0$$aAmare, J.$$b0
000316770 1112_ $$0C15-06-22.2$$2inspire$$a11th Patras Workshop on Axions, WIMPs and WISPs$$cZaragoza$$d2015-06-22 - 2015-06-26$$gAXION-WIMP 2015$$wSpain
000316770 245__ $$aBackground Model of NaI(Tl) Detectors for the ANAIS Dark Matter Project
000316770 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2015
000316770 29510 $$aAmare, J. "Background Model of NaI(Tl) Detectors for the ANAIS Dark Matter Project" in Proceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015) / Irastorza, Igor G., Redondo, Javier, Carmona, José Manuel, Cebrian, Susana, Dafni, Theopisti, Iguaz, Francisco J., Luzon, Gloria (eds.), Verlag Deutsches Elektronen-Synchrotron : 2015 ; AXION-WIMP 2015 : 11th Patras Workshop on Axions, WIMPs and WISPs, 2015-06-22 - 2015-06-26, Zaragoza
000316770 300__ $$a232-235
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000316770 520__ $$aA thorough understanding of the background sources is mandatory in any experiment searching for rare events. The ANAIS (Annual Modulation with NaI(Tl) Scintillators) experiment aims at the confirmation of the DAMA/LIBRA signal at the Canfranc Underground Laboratory (LSC). Two NaI(Tl) crystals of 12.5 kg each produced by Alpha Spectra have been taking data since December 2012. The complete background model of these detectors and more precisely in the region of interest will be described. Preliminary background analysis of a new 12.5 kg crystal received at Canfranc in March 2015 will be presented too. Finally, the power of anticoincidence rejection in the region of interest has been analyzed in a 4x5 12.5 kg detector matrix.
000316770 7001_ $$0P:(DE-HGF)0$$aCebrian, S.$$b1
000316770 7001_ $$0P:(DE-HGF)0$$aCuesta, C.$$b2
000316770 7001_ $$0P:(DE-HGF)0$$aGarcia, E.$$b3
000316770 7001_ $$0P:(DE-HGF)0$$aMartinez, M.$$b4
000316770 7001_ $$0P:(DE-HGF)0$$aOlivan, M. A.$$b5
000316770 7001_ $$0P:(DE-HGF)0$$aOrtigoza, Y.$$b6
000316770 7001_ $$0P:(DE-HGF)0$$aOrtiz de Solorzano, A.$$b7
000316770 7001_ $$0P:(DE-HGF)0$$aPobes, C.$$b8
000316770 7001_ $$0P:(DE-HGF)0$$aPuimedon, J.$$b9
000316770 7001_ $$0P:(DE-HGF)0$$aSarsa, M. L.$$b10
000316770 7001_ $$0P:(DE-HGF)0$$aVillar, J. A.$$b11
000316770 7001_ $$0P:(DE-HGF)0$$aVillar, P.$$b12
000316770 7870_ $$0PUBDB-2017-00118$$aIrastorza, Igor G. et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2015-02$$tProceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015)
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