000316758 001__ 316758
000316758 005__ 20211110140506.0
000316758 020__ $$a978-3-935702-43-0
000316758 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2015-02/woollet_nathan
000316758 0247_ $$2ISSN$$a1435-8077
000316758 037__ $$aPUBDB-2017-00156
000316758 041__ $$aEnglish
000316758 1001_ $$0P:(DE-HGF)0$$aWoollett, N.$$b0
000316758 1112_ $$0C15-06-22.2$$2inspire$$a11th Patras Workshop on Axions, WIMPs and WISPs$$cZaragoza$$d2015-06-22 - 2015-06-26$$gAXION-WIMP 2015$$wSpain
000316758 245__ $$aPreliminary Results of the CASCADE Hidden Sector Photon Search
000316758 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2015
000316758 29510 $$aWoollett, N. "Preliminary Results of the CASCADE Hidden Sector Photon Search" 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
000316758 300__ $$a179-182
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000316758 3367_ $$0PUB:(DE-HGF)7$$2PUB:(DE-HGF)$$aContribution to a book$$mcontb
000316758 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000316758 520__ $$aLight shining through a wall experiments can be used to make measurements of photon-WISP couplings. The first stage of the CASCADE experiment at the Cockcroft Institute of Accelerator Science and Technology is intended to be a proof-of-principle experiment utilising standard microwave technologies to make a modular, cryogenic HSP detector to take advantage of future high-power superconducting cavity tests. In these proceedings we will be presenting the preliminary results of the CASCADE LSW experiment showing a peak expected exclusion of $1.10\times10^{-8}$ in the mass range from 1.96\,$\mu$eV to 5.38\,$\mu$eV, exceeding current limits.
000316758 7001_ $$0P:(DE-HGF)0$$aBailey, I.$$b1
000316758 7001_ $$0P:(DE-HGF)0$$aBurt, G.$$b2
000316758 7001_ $$0P:(DE-HGF)0$$aChattopadhyay, S.$$b3
000316758 7001_ $$0P:(DE-HGF)0$$aDainton, J.$$b4
000316758 7001_ $$0P:(DE-HGF)0$$aDexter, A.$$b5
000316758 7001_ $$0P:(DE-HGF)0$$aGoudket, P.$$b6
000316758 7001_ $$0P:(DE-HGF)0$$aJenkins, M.$$b7
000316758 7001_ $$0P:(DE-HGF)0$$aKalliokoski, M.$$b8
000316758 7001_ $$0P:(DE-HGF)0$$aMoss, A.$$b9
000316758 7001_ $$0P:(DE-HGF)0$$aPattalwar, S.$$b10
000316758 7001_ $$0P:(DE-HGF)0$$aThakker, T.$$b11
000316758 7001_ $$0P:(DE-HGF)0$$aWilliams, P.$$b12
000316758 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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000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a Lancaster U.$$b0
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b0
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a Lancaster U.$$b1
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b1
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a Lancaster U.$$b2
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b2
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Northern Illinois U.$$b3
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Fermilab$$b3
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1004243$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b4
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Liverpool U. $$b4
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a Lancaster U.$$b5
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b5
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b6
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a Lancaster U.$$b7
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b7
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 CERN$$b8
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b9
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b10
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b11
000316758 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Cockcroft Inst. Accel. Sci. Tech.$$b12
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