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000395471 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2009-03/Cantatore_Giovanni
000395471 0247_ $$2ISSN$$a1435-8077
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000395471 0881_ $$aDESY-PROC-2016-03
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000395471 1001_ $$0P:(DE-HGF)0$$aCantatore, G.$$b0
000395471 1112_ $$0C16-06-20.4$$2inspire$$a12th Patras Workshop on Axions, WIMPs and WISPs$$cJeju Island$$d2016-06-20 - 2016-06-24$$gAXION-WIMP 2016$$wSouth Korea
000395471 245__ $$aLatest Results with the KWISP force Sensor at CAST
000395471 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2017
000395471 29510 $$aCantatore, G. "Latest Results with the KWISP force Sensor at CAST" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20 - 2016-06-24, Jeju Island
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000395471 520__ $$aThe KWISP opto-mechanical force sensor has started searching for solar chameleons through their direct coupling to matter. Its sensing element, a 100 nm thick Si$_3$N$_4$ membrane, was mounted in the focal plane of the CAST X-ray telescope and several solar trackings were completed using the unique capabilities of the CAST magnet. KWISP is designed to detect, with interferometric techniques, extremely tiny membrane displacements due to the force exerted by chameleons reflecting off it, while a specially devised chameleon beam chopper provides the reference frequency necessary for detection. We will present the initial KWISP setup, discussing its status and results.
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000395471 7001_ $$0P:(DE-HGF)0$$aCAST Collaboration$$b1$$eCollaboration author
000395471 7870_ $$0PUBDB-2017-11637$$aKim, Younglm et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2016-03$$t12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016
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000395471 9101_ $$aUniversity and INFN Trieste - Italy$$b0
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