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000408354 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/tanner_david
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000408354 1001_ $$0P:(DE-HGF)0$$aTanner, D. B.$$b0$$eCorresponding author
000408354 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408354 245__ $$aSearch for Axionic Dark Matter
000408354 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408354 29510 $$aTanner, D.B. "Search for Axionic Dark Matter" 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
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000408354 520__ $$aThe Axion Dark Matter eXperiment (ADMX) searches for axions as part of the halo of our galaxy. These axions have a mass in the range 1–10 µeV and convert to photons in a microwave cavity permeated by a strong magnetic field. ADMX recently incorporated low-noise SQUID amplifiers into the experiment and at present is being upgraded with a dilution refrigerator, permitting operation with noise temperatures of 100–200 mK. 
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