QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer

Autores
Gamboa Lerena, Martín Miguel; Mundo, Luis Mariano; Ringegni, Pablo Lorenzo; Scóccola, Claudia Graciela
Año de publicación
2019
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this paper, we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the-art bolometric detectors with the systematic effects control typical of interferometers. QUBIC’s unique features are the so-called “self-calibration”, a technique that allows us to clean the measured data from instrumental effects, and its spectral imaging power, i.e., the ability to separate the signal into various sub-bands within each frequency band. QUBIC will observe the sky in two main frequency bands: 150 GHz and 220 GHz. A technological demonstrator is currently under testing and will be deployed in Argentina during 2019, while the final instrument is expected to be installed during 2020.
La lista completa de autores que integran el documento puede consultarse en el archivo.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Astronomía
B-modes
bolometers
Cosmic Microwave Background
inflation
polarimetry
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/124814
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/124814
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling QUBIC: Exploring the Primordial Universe with the Q&U Bolometric InterferometerGamboa Lerena, Martín MiguelMundo, Luis MarianoRingegni, Pablo LorenzoScóccola, Claudia GracielaAstronomíaB-modesbolometersCosmic Microwave BackgroundinflationpolarimetryIn this paper, we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the-art bolometric detectors with the systematic effects control typical of interferometers. QUBIC’s unique features are the so-called “self-calibration”, a technique that allows us to clean the measured data from instrumental effects, and its spectral imaging power, i.e., the ability to separate the signal into various sub-bands within each frequency band. QUBIC will observe the sky in two main frequency bands: 150 GHz and 220 GHz. A technological demonstrator is currently under testing and will be deployed in Argentina during 2019, while the final instrument is expected to be installed during 2020.La lista completa de autores que integran el documento puede consultarse en el archivo.Facultad de Ciencias Astronómicas y Geofísicas2019-01-23info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/124814enginfo:eu-repo/semantics/altIdentifier/issn/2218-1997info:eu-repo/semantics/altIdentifier/doi/10.3390/universe5020042info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:10:44Zoai:sedici.unlp.edu.ar:10915/124814Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:10:44.27SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
spellingShingle QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
Gamboa Lerena, Martín Miguel
Astronomía
B-modes
bolometers
Cosmic Microwave Background
inflation
polarimetry
title_short QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title_full QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title_fullStr QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title_full_unstemmed QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title_sort QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
dc.creator.none.fl_str_mv Gamboa Lerena, Martín Miguel
Mundo, Luis Mariano
Ringegni, Pablo Lorenzo
Scóccola, Claudia Graciela
author Gamboa Lerena, Martín Miguel
author_facet Gamboa Lerena, Martín Miguel
Mundo, Luis Mariano
Ringegni, Pablo Lorenzo
Scóccola, Claudia Graciela
author_role author
author2 Mundo, Luis Mariano
Ringegni, Pablo Lorenzo
Scóccola, Claudia Graciela
author2_role author
author
author
dc.subject.none.fl_str_mv Astronomía
B-modes
bolometers
Cosmic Microwave Background
inflation
polarimetry
topic Astronomía
B-modes
bolometers
Cosmic Microwave Background
inflation
polarimetry
dc.description.none.fl_txt_mv In this paper, we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the-art bolometric detectors with the systematic effects control typical of interferometers. QUBIC’s unique features are the so-called “self-calibration”, a technique that allows us to clean the measured data from instrumental effects, and its spectral imaging power, i.e., the ability to separate the signal into various sub-bands within each frequency band. QUBIC will observe the sky in two main frequency bands: 150 GHz and 220 GHz. A technological demonstrator is currently under testing and will be deployed in Argentina during 2019, while the final instrument is expected to be installed during 2020.
La lista completa de autores que integran el documento puede consultarse en el archivo.
Facultad de Ciencias Astronómicas y Geofísicas
description In this paper, we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the-art bolometric detectors with the systematic effects control typical of interferometers. QUBIC’s unique features are the so-called “self-calibration”, a technique that allows us to clean the measured data from instrumental effects, and its spectral imaging power, i.e., the ability to separate the signal into various sub-bands within each frequency band. QUBIC will observe the sky in two main frequency bands: 150 GHz and 220 GHz. A technological demonstrator is currently under testing and will be deployed in Argentina during 2019, while the final instrument is expected to be installed during 2020.
publishDate 2019
dc.date.none.fl_str_mv 2019-01-23
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/124814
url http://sedici.unlp.edu.ar/handle/10915/124814
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/2218-1997
info:eu-repo/semantics/altIdentifier/doi/10.3390/universe5020042
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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