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dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorFuente Rodríguez, Luisa María de la 
dc.contributor.authorPascual Gutiérrez, Juan Pablo 
dc.contributor.authorVilla Benito, Enrique
dc.contributor.authorCalero de Ory, Marina
dc.contributor.authorRodríguez Rodríguez, David
dc.contributor.authorRollano, Víctor
dc.contributor.authorMagaz, M.T.
dc.contributor.authorGómez Gutiérrez, Alicia
dc.contributor.authorGranados Ruiz, Daniel
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2025-05-20T11:23:11Z
dc.date.available2025-05-20T11:23:11Z
dc.date.issued2024-08-16
dc.identifier.issn0277-786X
dc.identifier.issn1996-756X
dc.identifier.otherPID2022-137779OB-C43es_ES
dc.identifier.otherPID2022-137779OB-C41es_ES
dc.identifier.otherPID2022-137779OB-C42es_ES
dc.identifier.otherRED2022-134839-Tes_ES
dc.identifier.urihttps://hdl.handle.net/10902/36405
dc.description.abstractThis work deals with the development of superconducting Kinetic Inductance Detectors (KIDs) for highly sensitive radio astronomy receivers within W-band (75 to 110 GHz). A bilayer based on superconducting titanium/aluminum (Ti/Al) thin films has been used for assessing its absorption performance in this frequency band at millikelvin temperature. A lumped-element inductor based on a 4th order Hilbert structure is designed to absorb the incoming radiation in two orthogonal linear polarizations. The development of a large-format camera prototype is presented. On one hand, ambient temperature quasi-optical characterization demonstrates a suitable absorption for both polarizations within the W-band. On the other hand, dark cryogenic characterization confirms the successful operation of the multiplexed KID devices providing high-quality factors and an operation yield of 97%. These results confirm these developments to be used in future polarimeter receivers.es_ES
dc.description.sponsorshipThis work is funded by the following grants: 2023/TCN/005 (Universidad de Cantabria) by Consejería de Industria, Empleo, Innovación y Comercio, Gobierno de Cantabria, Spain; PID2022-137779OB-C43 (Universidad de Cantabria), PID2022-137779OB-C41 (CAB) and PID2022-137779OB-C42 (IMDEA-Nanociencia) by MCIN/AEI/10.13039/501100011033, “ERDF A way of making Europe”, EU “NextGenerationEU”/PRTR; RED2022-134839-T (all groups) by MCIN/AEI/10.13039/501100011033. IMDEA-Nanociencia acknowledges financial support from the ‘Severo Ochoa’ Programme for Centres of Excellence in R&D (CEX2020-001039-S) and CAB from CSIC Research Platform PTI-001 and ‘Tecnologías avanzadas para la exploración del Universo y sus componentes’ (PR47/21 TAU-CM) project funded by Com. de Madrid, by the Recovery, Transformation and Resilience Plan from the Spanish State, and by NextGenerationEU from the EU Recovery and Resilience Facility.es_ES
dc.format.extent7 p.es_ES
dc.language.isoenges_ES
dc.publisherSPIE Society of Photo-Optical Instrumentation Engineerses_ES
dc.rights© 2024 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this publication for a fee or for commercial purposes, and modification of the contents of the publication are prohibited.es_ES
dc.sourceProceedings of SPIE, 2024, 13102, 131020Zes_ES
dc.source12th Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy, Yokohama, Japan, 2024es_ES
dc.subject.otherKinetic inductance detectorses_ES
dc.subject.otherMillimeter-wave radio astronomyes_ES
dc.subject.otherPolarimeteres_ES
dc.titleDual polarization kinetic inductance detectors for large imaging cameras at millimeter wave bandses_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.relation.publisherVersionhttps://doi.org/10.1117/12.3014677es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1117/12.3014677
dc.type.versionpublishedVersiones_ES


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