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dc.contributor.authorPérez de Taoro, María del Rosario Ángeles
dc.contributor.authorAguiar González, Marta
dc.contributor.authorGénova Santos, Ricardo Tanausú
dc.contributor.authorGómez Reñasco, María Francisca
dc.contributor.authorHoyland, Roger J.
dc.contributor.authorLópez Caraballo, Carlos
dc.contributor.authorPeláez Santos, Alba Eva
dc.contributor.authorPoidevin, Frédérick
dc.contributor.authorTramonte, Denis
dc.contributor.authorRebolo López, Rafael
dc.contributor.authorMartínez González, Enrique
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.authorCagigas Ibañez, Jaime 
dc.contributor.authorCano de Diego, Juan Luis 
dc.contributor.authorCuerno García, Eva María 
dc.contributor.authorFuente Rodríguez, Luisa María de la 
dc.contributor.authorPérez Quintanilla, Ana Rosa 
dc.contributor.authorTerán Collantes, José Vicente 
dc.contributor.authorVilla Benito, Enrique 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2017-01-13T13:30:10Z
dc.date.available2017-01-13T13:30:10Z
dc.date.issued2014
dc.identifier.issn0277-786X
dc.identifier.issn1996-756X
dc.identifier.urihttp://hdl.handle.net/10902/9997
dc.description.abstractThe QUIJOTE-CMB experiment (Q-U-I JOint TEnerife CMB experiment) is an ambitious project to obtain polarization measurements of the sky microwave emission in the 10 to 47 GHz range. With this aim, a pair of 2,5m telescopes and three instruments are being sited at the Teide Observatory, in Tenerife (Canary Islands, Spain). The first telescope and the first instrument (the MFI: Multi Frequency Instrument) are both already operating in the band from 10 to 20 GHz, since November 2012. The second telescope and the second instrument (TGI: Thirty GHz instrument) is planned to be in commissioning by the end of summer 2014, covering the range of 26 to 36 GHz. After that, a third instrument named FGI (Forty GHz instrument) will be designed and manufactured to complete the sky survey in the frequency range from 37 to 47 GHz. In this paper we present an overview of the whole project current status, from the technical point of view.es_ES
dc.format.extent8 p.es_ES
dc.language.isoenges_ES
dc.publisherSPIE Society of Photo-Optical Instrumentation Engineerses_ES
dc.rights© 2014 Society of Photo-Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic electronic or print reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.es_ES
dc.sourceProceedings of SPIE, 2014, 9145, 91454Tes_ES
dc.sourceGround-based and Airborne Telescopes V, Montreal, 2014es_ES
dc.subject.otherMicrowaveses_ES
dc.subject.otherPolarizationes_ES
dc.subject.otherCMBes_ES
dc.subject.otherB-modeses_ES
dc.subject.otherTelescopeses_ES
dc.subject.otherInstrumentationes_ES
dc.titleQUIJOTE-CMB experiment: a technical overviewes_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.relation.publisherVersionhttp://dx.doi.org/10.1117/12.2055821es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1117/12.2055821
dc.type.versionacceptedVersiones_ES


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