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The QUIJOTE-CMB experiment: studying the polarisation of the galactic and cosmological microwave emissions

dc.contributor.authorRubiño Martín, José Alberto
dc.contributor.authorRebolo López, Rafael
dc.contributor.authorAguiar González, Marta
dc.contributor.authorMartínez González, Enrique
dc.contributor.authorBarreiro Vilas, Rita Belén 
dc.contributor.authorCasas Reinares, Francisco Javier 
dc.contributor.authorDiego Rodríguez, José María 
dc.contributor.authorFernández Cobos, Raúl 
dc.contributor.authorHerranz Muñoz, Diego 
dc.contributor.authorLópez-Caniego Alcarria, Marcos
dc.contributor.authorOrtiz García, David
dc.contributor.authorVielva Martínez, Patricio 
dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorCagigas Ibañez, Jaime 
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.accessioned2020-10-06T15:29:13Z
dc.date.available2020-10-06T15:29:13Z
dc.date.issued2012-09
dc.identifier.issn0277-786X
dc.identifier.issn1996-756X
dc.identifier.otherAYA2010-21766-C03es_ES
dc.identifier.otherCSD2010-00064es_ES
dc.identifier.urihttp://hdl.handle.net/10902/19299
dc.description.abstractThe QUIJOTE (Q-U-I JOint Tenerife) CMB Experiment will operate at the Teide Observatory with the aim of characterizing the polarisation of the CMB and other processes of Galactic and extragalactic emission in the frequency range of 10-40GHz and at large and medium angular scales. The first of the two QUIJOTE telescopes and the first multi-frequency (10-30GHz) instrument are already built and have been tested in the laboratory. QUIJOTE-CMB will be a valuable complement at low frequencies for the Planck mission, and will have the required sensitivity to detect a primordial gravitational-wave component if the tensor-to-scalar ratio is larger than r = 0.05.es_ES
dc.description.sponsorshipThe QUIJOTE-CMB experiment is being developed by the Instituto de Astrofisica de Canarias (IAC), the Instituto de Fisica de Cantabria (IFCA), and the Universities of Cantabria, Manchester and Cambridge. Partial financial support is provided by the Spanish Ministry of Economy and Competitiveness (MINECO) under the projects AYA2010-21766-C03 (01, 02 and 03), and also by the Consolider-Ingenio project CSD2010-00064 (EPI: Exploring the Physics of Inflation49).es_ES
dc.format.extent11 p.es_ES
dc.language.isoenges_ES
dc.publisherSPIE Society of Photo-Optical Instrumentation Engineerses_ES
dc.rights© 2012 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, 2012, 8444, 84442Yes_ES
dc.sourceGround-based and Airborne Telescopes IV, Amsterdam, 2012es_ES
dc.subject.otherCosmic microwave backgroundes_ES
dc.subject.otherPolarisationes_ES
dc.subject.otherCosmological parameterses_ES
dc.subject.otherEarly Universees_ES
dc.subject.otherTelescopees_ES
dc.subject.otherInstrumentationes_ES
dc.titleThe QUIJOTE-CMB experiment: studying the polarisation of the galactic and cosmological microwave emissionses_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.relation.publisherVersionhttps://doi.org/10.1117/12.926581es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1117/12.926581
dc.type.versionpublishedVersiones_ES


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