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dc.contributor.authorCalero de Ory, Marina
dc.contributor.authorRodríguez Rodríguez, David
dc.contributor.authorFuente Rodríguez, Luisa María de la 
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorVilla Benito, Enrique
dc.contributor.authorBordner Cano, Daniel
dc.contributor.authorPascual Gutiérrez, Juan Pablo 
dc.contributor.authorGranados Ruiz, Daniel
dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.authorGómez Gutiérrez, Alicia
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2024-03-18T16:22:44Z
dc.date.available2024-03-18T16:22:44Z
dc.date.issued2023
dc.identifier.isbn979-8-3503-4764-7
dc.identifier.otherPID2019-105552RB-C41es_ES
dc.identifier.otherPID2019-105552RB-C44es_ES
dc.identifier.otherPID2019-110610RB-C22es_ES
dc.identifier.urihttps://hdl.handle.net/10902/32312
dc.description.abstractA polarimetric detector in the W-band based on Lumped-Element Kinetic Inductance Detectors (LEKIDs) is presented. Each single optical element consists of two Ti/Al LEKIDs placed in orthogonal configuration on both sides of a Silicon substrate. Room temperature quasi-optical characterization demonstrates the high frequency design and the absorption in the W-band. Cryogenic characterization confirms the high quality factor of the fabricated resonators and polarization sensitivity in the W-band. The design proposed in this work is suitable for the development of polarimetric cameras of large arrays of LEKIDs for future astronomical experiments.es_ES
dc.description.sponsorshipCAB and IMDEA-Nanoscience work is supported by grants PID2019-105552RB-C41 and PID2019- 105552RB-C44 and by Comunidad de Madrid under Grant P2018/NMT-4291 TEC2SPACE-CM. IMDEA Nanoscience acknowledges financial support from the “Severo Ochoa” Programme for Centers of Excellence in R&D (MINECO, Grant SEV-2016-0686). D.G. and A.G also acknowledge Grant DEFROST N62909-19-1-2053 from ONR Global. We also acknowledge financial support from CSIC Research Platform PTI-001. The work of Universidad de Cantabria is supported by the Ministry of Science and Innovation under Grant PID2019-110610RB-C22.es_ES
dc.format.extent4 p.es_ES
dc.language.isoenges_ES
dc.publisherInstitute of Electrical and Electronics Engineers, Inc.es_ES
dc.rights© 2023 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.es_ES
dc.sourceIEEE/MTT-S International Microwave Symposium (IMS), San Diego, 2023, 570-573es_ES
dc.subject.otherKinetic inductor detectores_ES
dc.subject.otherSuperconducting resonatorses_ES
dc.subject.otherMillimeter astronomyes_ES
dc.subject.otherPolarimeteres_ES
dc.titleDevelopment of W-band dual-polarization kinetic inductance detectors on silicones_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.relation.publisherVersionhttps://doi.org/10.1109/IMS37964.2023.10188209es_ES
dc.rights.accessRightsopenAccesses_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-105552RB-C41/ES/CONTRIBUCION DEL CAB A SPICA, DESARROLLO DE INSTRUMENTACION CRIOGENICA Y EXPLOTACION CIENTIFICA MULTILONGITUD DE ONDA
dc.relation.projectIDinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-105552RB-C44/ES/FABRICACION DE DETECTORES SUPERCONDUCTORES MULTI-FRECUENCIA PARA FUTURAS MISIONES ESPACIALES EN EL FIR%2FSUB-MM%2FMM
dc.relation.projectIDinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-110610RB-C22/ES/POLARIMETRO PARA EL FONDO COSMICO DE MICROONDAS CON DETECTORES DE INDUCTANCIA CINETICA/
dc.identifier.DOI10.1109/IMS37964.2023.10188209
dc.type.versionacceptedVersiones_ES


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