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dc.contributor.authorVilla Benito, Enrique 
dc.contributor.authorCano de Diego, Juan Luis 
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorTerán Collantes, José Vicente 
dc.contributor.authorFuente Rodríguez, Luisa María de la 
dc.contributor.authorMediavilla Sánchez, Ángel 
dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2019-01-22T15:01:27Z
dc.date.available2019-03-31T02:45:14Z
dc.date.issued2018-03
dc.identifier.issn0922-6435
dc.identifier.issn1572-9508
dc.identifier.otherCSD2010-00064es_ES
dc.identifier.otherESP2015-70646-C2-2-Res_ES
dc.identifier.urihttp://hdl.handle.net/10902/15463
dc.description.abstractThis paper describes the analysis, design and characterization of a polarimetric receiver developed for covering the 35 to 47 GHz frequency band in the new instrument aimed at completing the ground-based Q-U-I Joint Tenerife Experiment. This experiment is designed to measure polarization in the Cosmic Microwave Background. The described high frequency instrument is a HEMT-based array composed of 29 pixels. A thorough analysis of the behaviour of the proposed receiver, based on electronic phase switching, is presented for a noise-like linearly polarized input signal, obtaining simultaneously I, Q and U Stokes parameters of the input signal. Wideband subsystems are designed, assembled and characterized for the polarimeter. Their performances are described showing appropriate results within the 35-to-47 GHz frequency band. Functionality tests are performed at room and cryogenic temperatures with adequate results for both temperature conditions, which validate the receiver concept and performance.es_ES
dc.description.sponsorshipThe authors would like to thank the Spanish Ministry of Economy, Industry and Competitiveness for the financial support provided through the CONSOLIDER-INGENIO 2010 program under the grant CSD2010-00064 and under the grant ESP2015-70646-C2-2-R.es_ES
dc.format.extent19 p.es_ES
dc.language.isoenges_ES
dc.publisherSpringer Naturees_ES
dc.rights© Springer Nature. This is a post-peer-review, pre-copyedit version of an article published in Experimental Astronomy. The final authenticated version is available online at: https://doi.org/10.1007/s10686-018-9579-0es_ES
dc.sourceExperimental Astronomy, 2018, 45(1), 127-146es_ES
dc.subject.otherBroadband receiveres_ES
dc.subject.otherPolarimetryes_ES
dc.subject.otherCMBes_ES
dc.subject.otherAstronomical instrumentses_ES
dc.subject.otherStokes parameterses_ES
dc.subject.otherMicrowave radiometryes_ES
dc.titlePolarimetric receiver in the forty gigahertz band: new instrument for the Q-U-I joint Tenerife experimentes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1007/s10686-018-9579-0es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1007/s10686-018-9579-0
dc.type.versionacceptedVersiones_ES


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