Home > Private Collections > >DESY > >FH > L > Axion Search and Research with Low Background Micromegas > print

001     316742
005     20211110140505.0
020 _ _ |a 978-3-935702-43-0
024 7 _ |a 10.3204/DESY-PROC-2015-02/garcia_juanan
|2 datacite_doi
024 7 _ |a 1435-8077
|2 ISSN
037 _ _ |a PUBDB-2017-00140
041 _ _ |a English
100 1 _ |a Garcia, J. A.
|0 P:(DE-HGF)0
|b 0
111 2 _ |a 11th Patras Workshop on Axions, WIMPs and WISPs
|c Zaragoza
|d 2015-06-22 - 2015-06-26
|g AXION-WIMP 2015
|0 C15-06-22.2
|2 inspire
|w Spain
245 _ _ |a Axion Search and Research with Low Background Micromegas
260 _ _ |a Hamburg
|c 2015
|b Verlag Deutsches Elektronen-Synchrotron
295 1 0 |a Garcia, J. A. "Axion Search and Research with Low Background Micromegas" 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
300 _ _ |a 104-108
336 7 _ |a CONFERENCE_PAPER
|2 ORCID
336 7 _ |a Conference Paper
|0 33
|2 EndNote
336 7 _ |a INPROCEEDINGS
|2 BibTeX
336 7 _ |a conferenceObject
|2 DRIVER
336 7 _ |a Output Types/Conference Paper
|2 DataCite
336 7 _ |a Contribution to a conference proceedings
|b contrib
|m contrib
|0 PUB:(DE-HGF)8
|s 1484734433_28524
|2 PUB:(DE-HGF)
336 7 _ |a Contribution to a book
|0 PUB:(DE-HGF)7
|2 PUB:(DE-HGF)
|m contb
490 0 _ |a DESY-PROC
|0 PERI:(DE-600)2450075-6
520 _ _ |a Helioscopes are one of the most promising techniques for axion discovery in which low background X-ray detectors are mandatory. We report the latest developments of the Micromegas detectors for the CERN Axion Solar Telescope (CAST). The use of low background techniques has led to background levels below $10^{-6}$~c~keV$^{-1}$~cm$^{-2}$~s$^{-1}$, more than a factor 100 lower than the first generation of Micromegas detectors at CAST. The helioscope technique can be enhanced by the use of an X-ray focusing device, increasing the signal-to-background ratio. A new dedicated X-ray optic was installed at CAST during 2014 with a low background Micromegas in its focal plane. Apart from increasing CAST’s sensitivity, the system has been conceived as a technological pathfinder for the International Axion Observatory IAXO.
700 1 _ |a Aznar, F.
|0 P:(DE-HGF)0
|b 1
700 1 _ |a Castel, J.
|0 P:(DE-HGF)0
|b 2
700 1 _ |a Christensen, F. E.
|0 P:(DE-HGF)0
|b 3
700 1 _ |a Dafni, T.
|0 P:(DE-HGF)0
|b 4
700 1 _ |a Decker, T. A.
|0 P:(DE-HGF)0
|b 5
700 1 _ |a Ferrer-Ribas, E.
|0 P:(DE-HGF)0
|b 6
700 1 _ |a Giomataris, I.
|0 P:(DE-HGF)0
|b 7
700 1 _ |a Gracia, J. G.
|0 P:(DE-HGF)0
|b 8
700 1 _ |a Hailey, C. J.
|0 P:(DE-HGF)0
|b 9
700 1 _ |a Hill, R. M.
|0 P:(DE-HGF)0
|b 10
700 1 _ |a Iguaz, F. J.
|0 P:(DE-HGF)0
|b 11
700 1 _ |a Irastorza, I. G.
|0 P:(DE-HGF)0
|b 12
700 1 _ |a Jakobsen, A. C
|0 P:(DE-HGF)0
|b 13
700 1 _ |a Luzon, G.
|0 P:(DE-HGF)0
|b 14
700 1 _ |a Mirallas, H.
|0 P:(DE-HGF)0
|b 15
700 1 _ |a Papaevangelou, T.
|0 P:(DE-HGF)0
|b 16
700 1 _ |a Pivovaroff, M. J.
|0 P:(DE-HGF)0
|b 17
700 1 _ |a Ruz, J.
|0 P:(DE-HGF)0
|b 18
700 1 _ |a Vafeiadis, T.
|0 P:(DE-HGF)0
|b 19
700 1 _ |a Vogel, J. K.
|0 P:(DE-HGF)0
|b 20
787 0 _ |a Irastorza, Igor G. et. al.
|d Verlag Deutsches Elektronen-Synchrotron
|i isPartOf
|0 PUBDB-2017-00118
|r DESY-PROC-2015-02
|t Proceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015)
856 4 _ |u https://bib-pubdb1.desy.de/record/316742/files/fulltext.pdf
|y OpenAccess
909 C O |o oai:bib-pubdb1.desy.de:316742
|p openaire
|p open_access
|p driver
|p dnbdelivery
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 0
|6 P:(DE-HGF)0
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 1
|6 P:(DE-HGF)0
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 2
|6 P:(DE-HGF)0
910 1 _ |a Denmark, Tech. U.
|0 I:(DE-HGF)0
|b 3
|6 P:(DE-HGF)0
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 4
|6 P:(DE-HGF)0
910 1 _ |a LLNL, Livermore
|0 I:(DE-HGF)0
|b 5
|6 P:(DE-HGF)0
910 1 _ |a Saclay
|0 I:(DE-HGF)0
|b 6
|6 P:(DE-HGF)0
910 1 _ |a Saclay
|0 I:(DE-HGF)0
|b 7
|6 P:(DE-HGF)0
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 8
|6 P:(DE-HGF)0
910 1 _ |a Columbia U., Astron. Astrophys.
|0 I:(DE-HGF)0
|b 9
|6 P:(DE-HGF)0
910 1 _ |a LLNL, Livermore
|0 I:(DE-HGF)0
|b 10
|6 P:(DE-HGF)0
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 11
|6 P:(DE-HGF)0
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 12
|6 P:(DE-HGF)0
910 1 _ |a Denmark, Tech. U.
|0 I:(DE-HGF)0
|b 13
|6 P:(DE-HGF)0
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 14
|6 P:(DE-HGF)0
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 15
|6 P:(DE-HGF)0
910 1 _ |a Saclay
|0 I:(DE-HGF)0
|b 16
|6 P:(DE-HGF)0
910 1 _ |a LLNL, Livermore
|0 I:(DE-HGF)0
|b 17
|6 P:(DE-HGF)0
910 1 _ |a LLNL, Livermore
|0 I:(DE-HGF)0
|b 18
|6 P:(DE-HGF)0
910 1 _ |a Aristotle U., Thessaloniki
|0 I:(DE-HGF)0
|b 19
|6 P:(DE-HGF)0
910 1 _ |a LLNL, Livermore
|0 I:(DE-HGF)0
|b 20
|6 P:(DE-HGF)0
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Hosted Content
|0 StatID:(DE-HGF)10000
|2 StatID
915 _ _ |a Creative Commons Attribution CC BY 4.0
|0 LIC:(DE-HGF)CCBY4
|2 HGFVOC
980 _ _ |a contrib
980 _ _ |a contb
980 _ _ |a I:(DE-H253)L-20120731
980 1 _ |a UNRESTRICTED
980 1 _ |a FullTexts

LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21