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dc.contributor.authorHoyland, Roger J.
dc.contributor.authorAguiar González, Marta
dc.contributor.authorGénova Santos, Ricardo Tanausú
dc.contributor.authorGómez Reñasco, María Francisca
dc.contributor.authorLópez-Caraballo, Carlos
dc.contributor.authorRebolo López, Rafael
dc.contributor.authorRubiño Martín, José Alberto
dc.contributor.authorSánchez de la Rosa, Vicente
dc.contributor.authorVega Moreno, Afrodisio
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.authorOrtiz García, David
dc.contributor.authorTerán Collantes, José Vicente 
dc.contributor.authorVilla Benito, Enrique 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2017-01-13T13:33:43Z
dc.date.available2017-01-13T13:33:43Z
dc.date.issued2014
dc.identifier.issn0277-786X
dc.identifier.issn1996-756X
dc.identifier.urihttp://hdl.handle.net/10902/9998
dc.description.abstractThe QUIJOTE TGI instrument is currently being assembled and tested at the IAC in Spain. The TGI is a 31 pixel 26-36 GHz polarimeter array designed to be mounted at the focus of the second QUIJOTE telescope. This follows a first telescope and multi-frequency instrument that have now been observing almost 2 years. The polarimeter design is based on the QUIET polarimeter scheme but with the addition of an extra 90º phase switch which allows for quasiinstantaneous complete QUI measurements through each detector. The advantage of this is a reduction in the systematics associated with differencing two independent radiometer channels. The polarimeters are split into a cold front end and a warm back end. The back end is a highly integrated design by engineers at DICOM. It is also sufficiently modular for testing purposes. In this presentation the high quality wide band components used in the optical design (also designed in DICOM) are presented as well as the novel cryogenic modular design. Each polarimeter chain is accessible individually and can be removed from the cryostat and replaced without having to move the remaining pixels. The optical components work over the complete Ka band showing excellent performance. Results from the sub unit measurements are presented and also a description of the novel calibration technique that allows for bandpass measurement and polar alignment. Terrestrial Calibration for this instrument is very important and will be carried out at three points in the commissioning phase: in the laboratory, at the telescope site and finally a reduce set of calibrations will be carried out on the telescope before measurements of extraterrestrial sources begin. The telescope pointing model is known to be more precise than the expected calibration precision so no further significant error will be added through the telescope optics. The integrated back-end components are presented showing the overall arrangement for mounting on the cryostat. Many of the microwave circuits are in-house designs with performances that go beyond commercially available products. Individual component performance is be presented showing for each of the sub modules.es_ES
dc.format.extent17 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, 9153, 915332es_ES
dc.sourceMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, Montreal, 2014es_ES
dc.subject.otherPolarizationes_ES
dc.subject.otherCMBres_ES
dc.subject.otherInstrumentationes_ES
dc.subject.otherSpectrometeres_ES
dc.subject.otherForegroundses_ES
dc.subject.otherB-modeses_ES
dc.subject.otherMappinges_ES
dc.titleThe QUIJOTE TGIes_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.relation.publisherVersionhttp://dx.doi.org/10.1117/12.2055414es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1117/12.2055414
dc.type.versionacceptedVersiones_ES


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