QUBIC Experiment toward the first light
- Autores
- García, Beatríz
- Año de publicación
- 2022
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión aceptada
- Descripción
- The 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.
Fil: Universidad Tecnológica Nacional. Facultad Regional Mendoza, Argentina
Peer Reviewed - Materia
- CMB, CMB bolometric detectors, QUBIC experiment
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- 2024-05-02T14:39:51Z
- Repositorio
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- Institución
- Universidad Tecnológica Nacional
- OAI Identificador
- oai:ria.utn.edu.ar:20.500.12272/10705
Ver los metadatos del registro completo
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QUBIC Experiment toward the first lightGarcía, BeatrízCMB, CMB bolometric detectors, QUBIC experimentThe 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.Fil: Universidad Tecnológica Nacional. Facultad Regional Mendoza, ArgentinaPeer Reviewed2024-05-02T14:39:51Z2024-05-02T14:39:51Z2022-01-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articulopdfapplication/pdfJournal of Low Temperature Physicshttp://hdl.handle.net/20.500.12272/10705https://doi.org/10.1007/s10909-022-02775-zenginfo:eu-repo/semantics/openAccess2024-05-02T14:39:51Zhttp://creativecommons.org/publicdomain/zero/1.0/CC0 1.0 UniversalUniversidad Tecnológica Nacional. Facultad Regional MendozaCompartir igualreponame:Repositorio Institucional Abierto (UTN)instname:Universidad Tecnológica Nacional2026-09-24T12:45:07Zoai:ria.utn.edu.ar:20.500.12272/10705instacron:UTNInstitucionalhttp://ria.utn.edu.ar/Universidad públicaNo correspondehttp://ria.utn.edu.ar/oaigestionria@rec.utn.edu.ar; fsuarez@rec.utn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:a2026-09-24 12:45:08.233Repositorio Institucional Abierto (UTN) - Universidad Tecnológica Nacionalfalse |
| dc.title.none.fl_str_mv |
QUBIC Experiment toward the first light |
| title |
QUBIC Experiment toward the first light |
| spellingShingle |
QUBIC Experiment toward the first light García, Beatríz CMB, CMB bolometric detectors, QUBIC experiment |
| title_short |
QUBIC Experiment toward the first light |
| title_full |
QUBIC Experiment toward the first light |
| title_fullStr |
QUBIC Experiment toward the first light |
| title_full_unstemmed |
QUBIC Experiment toward the first light |
| title_sort |
QUBIC Experiment toward the first light |
| dc.creator.none.fl_str_mv |
García, Beatríz |
| author |
García, Beatríz |
| author_facet |
García, Beatríz |
| author_role |
author |
| dc.subject.none.fl_str_mv |
CMB, CMB bolometric detectors, QUBIC experiment |
| topic |
CMB, CMB bolometric detectors, QUBIC experiment |
| dc.description.none.fl_txt_mv |
The 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. Fil: Universidad Tecnológica Nacional. Facultad Regional Mendoza, Argentina Peer Reviewed |
| description |
The 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. |
| publishDate |
2022 |
| dc.date.none.fl_str_mv |
2022-01-01 2024-05-02T14:39:51Z 2024-05-02T14:39:51Z |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/acceptedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
| format |
article |
| status_str |
acceptedVersion |
| dc.identifier.none.fl_str_mv |
Journal of Low Temperature Physics http://hdl.handle.net/20.500.12272/10705 https://doi.org/10.1007/s10909-022-02775-z |
| identifier_str_mv |
Journal of Low Temperature Physics |
| url |
http://hdl.handle.net/20.500.12272/10705 https://doi.org/10.1007/s10909-022-02775-z |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess 2024-05-02T14:39:51Z http://creativecommons.org/publicdomain/zero/1.0/ CC0 1.0 Universal Universidad Tecnológica Nacional. Facultad Regional Mendoza Compartir igual |
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openAccess |
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2024-05-02T14:39:51Z http://creativecommons.org/publicdomain/zero/1.0/ CC0 1.0 Universal Universidad Tecnológica Nacional. Facultad Regional Mendoza Compartir igual |
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pdf application/pdf |
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