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dc.contributor.authorPérez de Taoro, María del Rosario Ángeles
dc.contributor.authorAguiar González, Marta
dc.contributor.authorCózar Castellano, Juan
dc.contributor.authorGénova Santos, Ricardo Tanausú
dc.contributor.authorGómez Reñasco, María Francisca
dc.contributor.authorHoyland, Roger J.
dc.contributor.authorPeláez Santos, Alba Eva
dc.contributor.authorPoidevin, Frédérick
dc.contributor.authorTramonte, Denis
dc.contributor.authorRebolo López, Rafael
dc.contributor.authorCasas Reinares, Francisco Javier 
dc.contributor.authorMartínez González, Enrique
dc.contributor.authorOrtiz García, David
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.authorCano de Diego, Juan Luis 
dc.contributor.authorFuente Rodríguez, Luisa María de la 
dc.contributor.authorMediavilla Sánchez, Ángel 
dc.contributor.authorTerán Collantes, José Vicente 
dc.contributor.authorVilla Benito, Enrique 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2017-05-31T13:17:57Z
dc.date.available2017-05-31T13:17:57Z
dc.date.issued2016
dc.identifier.issn0277-786X
dc.identifier.issn1996-756X
dc.identifier.urihttp://hdl.handle.net/10902/11122
dc.description.abstractThe QUIJOTE Experiment (Q-U-I JOint TEnerife) is a combined operation of two telescopes and three instruments working in the microwave band to measure the polarization of the Cosmic Microwave Background (CMB) from the northern hemisphere, at medium and large angular scales. The experiment is located at the Teide Observatory in Tenerife, one of the seven Canary Islands (Spain). The project is a consortium maintained by several institutions: the Instituto de Astrofísica de Canarias (IAC), the Instituto de Física de Cantabria (IFCA), the Communications Engineering Department (DICOM) at Universidad de Cantabria, and the Universities of Manchester and Cambridge. The consortium is led by the IAC.es_ES
dc.format.extent8 p.es_ES
dc.language.isoenges_ES
dc.publisherSPIE Society of Photo-Optical Instrumentation Engineerses_ES
dc.rightsCopyright 2016 Society of Photo Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic 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, 2016, 9906, 99061Kes_ES
dc.sourceGround-based and Airborne Telescopes VI, Edinburgh, United Kingdom, 2016es_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.subject.otherCryogenicses_ES
dc.subject.otherTemperature controles_ES
dc.titleQUIJOTE Experiment: status of telescopes and instrumentationes_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.relation.publisherVersionhttps://doi.org/10.1117/12.2233225es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1117/12.2233225
dc.type.versionpublishedVersiones_ES


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