A Micromegas-based low-background x-ray detector coupled to a slumped-glass telescope for axion research
Aznar Tabuenca, Francisco ; Castel Pablo, Juan Francisco ; Christensen, F.E. ; Dafni , Theopisti (Universidad de Zaragoza) ; Decker, T.A. ; Ferrer-Ribas, E. ; García Pascual, Juan Antonio (Universidad de Zaragoza) ; Giomataris, I. ; Gracia Garza, Javier (Universidad de Zaragoza) ; Hailey, C.J. ; Hill, R.M. ; Iguaz Gutiérrez, Francisco José (Universidad de Zaragoza) ; García Irastorza, Igor (Universidad de Zaragoza) ; Jakobsen, A.C. ; Luzón Marco, Gloria (Universidad de Zaragoza) ; Mirallas Sánchez, Héctor ; Papaevangelou, T. ; Pivovaroff, M.J. ; Ruz Armendariz, Jaime ; Vafeiadis, T. ; Vogel, J.K.
Resumen: We report on the design, construction and operation of a low background x-ray detection line composed of a shielded Micromegas detector of the microbulk technology. The detector is made from radiopure materials and is placed at the focal point of a similar to 5 cm diameter, 1.5 m focal-length, cone-approximation Wolter I x-ray telescope (XRT) assembled from thermally-formed (or "slumped") glass substrates deposited with multilayer coatings. The system has been conceived as a technological pathfinder for the future International Axion Observatory (IAXO), as it combines two of the techniques (optic and detector) proposed in the conceptual design of the project. It is innovative for two reasons: it is the first time an x-ray optic has been designed and fabricated specifically for axion research, and the first time a Micromegas detector has been operated with an x-ray optic. The line has been installed at one end of the CERN Axion Solar Telescope (CAST) magnet and is currently looking for solar axions. The combination of the XRT and Micromegas detector provides the best signal-to-noise ratio obtained so far by any detection system of the CAST experiment with a background rate of 5.4 x 10(-3) counts per hour in the energy region-of-interest and signal spot area.
Idioma: Inglés
DOI: 10.1088/1475-7516/2015/12/008
Año: 2015
Publicado en: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS 2015, 12 (2015), 008
ISSN: 1475-7516
Factor impacto JCR: 5.634 (2015)
Categ. JCR: ASTRONOMY & ASTROPHYSICS rank: 9 / 61 = 0.148 (2015) - Q1 - T1
Categ. JCR: PHYSICS, PARTICLES & FIELDS rank: 5 / 28 = 0.179 (2015) - Q1 - T1
Financiación: info:eu-repo/grantAgreement/EUR/FP7/ERC2009-StG-240054
Financiación: info:eu-repo/grantAgreement/ES/MICINN/CPAN-CSD2007-00042
Financiación: info:eu-repo/grantAgreement/ES/MINECO-FEDER/FPA2008-03456
Financiación: info:eu-repo/grantAgreement/ES/MINECO-FEDER/FPA2011-24058
Tipo y forma: Article (PostPrint)
Área (Departamento): Física Atómica, Molecular y Nuclear (Departamento de Física Teórica)
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Exportado de SIDERAL (2016-11-30-09:16:19)
Idioma: Inglés
DOI: 10.1088/1475-7516/2015/12/008
Año: 2015
Publicado en: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS 2015, 12 (2015), 008
ISSN: 1475-7516
Factor impacto JCR: 5.634 (2015)
Categ. JCR: ASTRONOMY & ASTROPHYSICS rank: 9 / 61 = 0.148 (2015) - Q1 - T1
Categ. JCR: PHYSICS, PARTICLES & FIELDS rank: 5 / 28 = 0.179 (2015) - Q1 - T1
Financiación: info:eu-repo/grantAgreement/EUR/FP7/ERC2009-StG-240054
Financiación: info:eu-repo/grantAgreement/ES/MICINN/CPAN-CSD2007-00042
Financiación: info:eu-repo/grantAgreement/ES/MINECO-FEDER/FPA2008-03456
Financiación: info:eu-repo/grantAgreement/ES/MINECO-FEDER/FPA2011-24058
Tipo y forma: Article (PostPrint)
Área (Departamento): Física Atómica, Molecular y Nuclear (Departamento de Física Teórica)
0
Exportado de SIDERAL (2016-11-30-09:16:19)
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articulos > articulos-por-area > fisica_atomica,_molecular_y_nuclear
Notice créée le 2016-11-30, modifiée le 2016-11-30
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