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dc.creatorGarcía, Beatríz
dc.date.accessioned2024-05-02T14:39:51Z
dc.date.available2024-05-02T14:39:51Z
dc.date.issued2022-01-01
dc.identifier.citationJournal of Low Temperature Physicses_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12272/10705
dc.description.abstractThe Q & U Bolometric Interferometer for Cosmology (QUBIC) is a cosmology experiment that aims to measure the B-mode polarization of the cosmic microwave background (CMB). Measurements of the primordial B-mode pattern of the CMB polarization are in fact among the most exciting goals in cosmology as it would allow testing of the infationary paradigm. Many experiments are attempting to measure the B-modes, from the ground and the stratosphere, using imaging Stokes polarimeters. The QUBIC collaboration developed an innovative concept to measure CMB polarization using bolometric interferometry. This approach mixes the high sensitivity of bolometric detectors with the accurate control of systematics due to the interferometric layout of the instrument. We present the calibration results for the Technological Demonstrator, before its commissioning in the Argentinian observing site and preparation for frst light.es_ES
dc.formatpdfes_ES
dc.language.isoenges_ES
dc.rightsopenAccesses_ES
dc.rights.urihttp://creativecommons.org/publicdomain/zero/1.0/*
dc.rights.uriCC0 1.0 Universal*
dc.subjectCMB, CMB bolometric detectors, QUBIC experimentes_ES
dc.titleQUBIC Experiment toward the first lightes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.holderUniversidad Tecnológica Nacional. Facultad Regional Mendozaes_ES
dc.description.affiliationUniversidad Tecnológica Nacional. Facultad Regional Mendoza, Argentinaes_ES
dc.description.peerreviewedPeer Reviewedes_ES
dc.type.versionacceptedVersiones_ES
dc.rights.useCompartir iguales_ES
dc.identifier.doihttps://doi.org/10.1007/s10909-022-02775-z


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