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000408341 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/avignone_frank
000408341 0247_ $$2ISSN$$a1435-8077
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000408341 1001_ $$0P:(DE-HGF)0$$aAvignone III, F. T.$$b0$$eCorresponding author
000408341 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408341 245__ $$aPoint-contact detectors in searches for bremsstrahlung production of axions from the Sun
000408341 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408341 29510 $$aAvignone, F.T., III "Point-contact detectors in searches for bremsstrahlung production of axions from the Sun" 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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000408341 520__ $$aThe low-energy portion of the published spectrum of the COGENT experiment has been reanalyzed to search for evidence of low-energy bremsstrahlung-generated solar axions. In the case of the DFSZ model, an upper bound of $g_{ae} ≤ 3.0 × 10^{−11}$ (90% C.L.) is placed on the direct coupling of axions to electrons. 
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000408341 7001_ $$0P:(DE-HGF)0$$aCreswick, R. J.$$b1
000408341 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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