Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted)
- Autores
- Regnier, M.; Laclavere, T.; Hamilton, Jean-christophe; Bunn, E.; Chabirand, V.; Chanial, P.; Goetz, L.; Kardum, L.; Masson, P.; Mirón Granese, Nahuel Omar; Scoccola, Claudia Graciela; Torchinsky, S.; Battistelli, E.; Bersanelli, M.; Columbro, F.; Coppolecchia, A.; Costanza, María Belén; De Bernardis, P.; De Gasperis, G.; Ferrazolli, S.; Flood, A. B.; Ganga, K. M.; Gervasi, M.; Grandsire, L.; Manzan, E.; Masi, S.; Mennella, A.; Mousset, L.; O'Sullivan, C.; Paiella, A.; Piacentini, F.; Piat, M.; Piccirillo, L.; Rasztocky, Emiliano; Stolpovskiy, M.; Zannoni, M.
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The detection of B-modes in the CMB polarization pattern is a major issue in modern cosmology and must therefore be handled with analytical methods that produce reliable results. We describe a method that uses the frequency dependency of the QUBIC synthesized beam to perform component separation at the map-making stage, to obtain more precise results. We aim to demonstrate the feasibility of component separation during the map-making stage in time domain space. This new technique leads to a more accurate description of the data and reduces the biases in cosmological analysis. The method uses a library for highly parallel computation which facilitates the programming and permits the description of experiments as easily manipulated operators. These operators can be combined to obtain a joint analysis using several experiments leading to maximized precision. The results show that the method works well and permits end-to-end analysis for the CMB experiments, and in particular, for QUBIC. The method includes astrophysical foregrounds, and also systematic effects like gain variation in the detectors. We developed a software pipeline that produces uncertainties on tensor-to-scalar ratio at the level of using only QUBIC simulated data.
Fil: Regnier, M.. Universite de Paris; Francia
Fil: Laclavere, T.. Universite de Paris; Francia
Fil: Hamilton, Jean-christophe. Universite de Paris; Francia
Fil: Bunn, E.. University of Richmond; Estados Unidos
Fil: Chabirand, V.. Universite de Paris; Francia. École Polytechnique; Francia
Fil: Chanial, P.. Universite de Paris; Francia
Fil: Goetz, L.. Universite de Paris; Francia
Fil: Kardum, L.. Universite de Paris; Francia
Fil: Masson, P.. Universite de Paris; Francia
Fil: Mirón Granese, Nahuel Omar. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Scoccola, Claudia Graciela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Universidad de Chile. Facultad de Ciencias Físicas y Matemáticas; Chile
Fil: Torchinsky, S.. Université Paris Cité; Francia
Fil: Battistelli, E.. Università degli studi di Roma "La Sapienza"; Italia
Fil: Bersanelli, M.. Università degli Studi di Milano; Italia
Fil: Columbro, F.. Università degli studi di Roma "La Sapienza"; Italia
Fil: Coppolecchia, A.. Università degli studi di Roma "La Sapienza"; Italia
Fil: Costanza, María Belén. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: De Bernardis, P.. Università degli studi di Roma "La Sapienza"; Italia
Fil: De Gasperis, G.. Università degli studi di Roma "La Sapienza"; Italia
Fil: Ferrazolli, S.. Università degli studi di Roma "La Sapienza"; Italia
Fil: Flood, A. B.. National University of Ireland Galway; Irlanda
Fil: Ganga, K. M.. Université Paris Cité; Francia
Fil: Gervasi, M.. Università degli Studi di Milano; Italia
Fil: Grandsire, L.. Université Paris Cité; Francia
Fil: Manzan, E.. Università degli Studi di Milano; Italia
Fil: Masi, S.. Università degli studi di Roma "La Sapienza"; Italia
Fil: Mennella, A.. Università degli Studi di Milano; Italia
Fil: Mousset, L.. Sorbonne University; Francia
Fil: O'Sullivan, C.. National University of Ireland Galway; Irlanda
Fil: Paiella, A.. Università degli studi di Roma "La Sapienza"; Italia
Fil: Piacentini, F.. Università degli studi di Roma "La Sapienza"; Italia
Fil: Piat, M.. Université Paris Cité; Francia
Fil: Piccirillo, L.. University of Manchester; Reino Unido
Fil: Rasztocky, Emiliano. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Stolpovskiy, M.. University of Bern; Suiza
Fil: Zannoni, M.. Università degli Studi di Milano; Italia - Materia
-
COSMIC MICROWAVE BACKGROUND
DATA ANALYSIS
INFLATION - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/283698
Ver los metadatos del registro completo
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Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted)Regnier, M.Laclavere, T.Hamilton, Jean-christopheBunn, E.Chabirand, V.Chanial, P.Goetz, L.Kardum, L.Masson, P.Mirón Granese, Nahuel OmarScoccola, Claudia GracielaTorchinsky, S.Battistelli, E.Bersanelli, M.Columbro, F.Coppolecchia, A.Costanza, María BelénDe Bernardis, P.De Gasperis, G.Ferrazolli, S.Flood, A. B.Ganga, K. M.Gervasi, M.Grandsire, L.Manzan, E.Masi, S.Mennella, A.Mousset, L.O'Sullivan, C.Paiella, A.Piacentini, F.Piat, M.Piccirillo, L.Rasztocky, EmilianoStolpovskiy, M.Zannoni, M.COSMIC MICROWAVE BACKGROUNDDATA ANALYSISINFLATIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The detection of B-modes in the CMB polarization pattern is a major issue in modern cosmology and must therefore be handled with analytical methods that produce reliable results. We describe a method that uses the frequency dependency of the QUBIC synthesized beam to perform component separation at the map-making stage, to obtain more precise results. We aim to demonstrate the feasibility of component separation during the map-making stage in time domain space. This new technique leads to a more accurate description of the data and reduces the biases in cosmological analysis. The method uses a library for highly parallel computation which facilitates the programming and permits the description of experiments as easily manipulated operators. These operators can be combined to obtain a joint analysis using several experiments leading to maximized precision. The results show that the method works well and permits end-to-end analysis for the CMB experiments, and in particular, for QUBIC. The method includes astrophysical foregrounds, and also systematic effects like gain variation in the detectors. We developed a software pipeline that produces uncertainties on tensor-to-scalar ratio at the level of using only QUBIC simulated data.Fil: Regnier, M.. Universite de Paris; FranciaFil: Laclavere, T.. Universite de Paris; FranciaFil: Hamilton, Jean-christophe. Universite de Paris; FranciaFil: Bunn, E.. University of Richmond; Estados UnidosFil: Chabirand, V.. Universite de Paris; Francia. École Polytechnique; FranciaFil: Chanial, P.. Universite de Paris; FranciaFil: Goetz, L.. Universite de Paris; FranciaFil: Kardum, L.. Universite de Paris; FranciaFil: Masson, P.. Universite de Paris; FranciaFil: Mirón Granese, Nahuel Omar. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Scoccola, Claudia Graciela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Universidad de Chile. Facultad de Ciencias Físicas y Matemáticas; ChileFil: Torchinsky, S.. Université Paris Cité; FranciaFil: Battistelli, E.. Università degli studi di Roma "La Sapienza"; ItaliaFil: Bersanelli, M.. Università degli Studi di Milano; ItaliaFil: Columbro, F.. Università degli studi di Roma "La Sapienza"; ItaliaFil: Coppolecchia, A.. Università degli studi di Roma "La Sapienza"; ItaliaFil: Costanza, María Belén. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: De Bernardis, P.. Università degli studi di Roma "La Sapienza"; ItaliaFil: De Gasperis, G.. Università degli studi di Roma "La Sapienza"; ItaliaFil: Ferrazolli, S.. Università degli studi di Roma "La Sapienza"; ItaliaFil: Flood, A. B.. National University of Ireland Galway; IrlandaFil: Ganga, K. M.. Université Paris Cité; FranciaFil: Gervasi, M.. Università degli Studi di Milano; ItaliaFil: Grandsire, L.. Université Paris Cité; FranciaFil: Manzan, E.. Università degli Studi di Milano; ItaliaFil: Masi, S.. Università degli studi di Roma "La Sapienza"; ItaliaFil: Mennella, A.. Università degli Studi di Milano; ItaliaFil: Mousset, L.. Sorbonne University; FranciaFil: O'Sullivan, C.. National University of Ireland Galway; IrlandaFil: Paiella, A.. Università degli studi di Roma "La Sapienza"; ItaliaFil: Piacentini, F.. Università degli studi di Roma "La Sapienza"; ItaliaFil: Piat, M.. Université Paris Cité; FranciaFil: Piccirillo, L.. University of Manchester; Reino UnidoFil: Rasztocky, Emiliano. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Stolpovskiy, M.. University of Bern; SuizaFil: Zannoni, M.. Università degli Studi di Milano; ItaliaCornell University2024-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/283698Regnier, M.; Laclavere, T.; Hamilton, Jean-christophe; Bunn, E.; Chabirand, V.; et al.; Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted); Cornell University; arXiv.org; 9-2024; 1-152331-8422CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2409.18714info:eu-repo/semantics/altIdentifier/doi/10.48550/arXiv.2409.18714info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-08-25T14:38:25Zoai:ri.conicet.gov.ar:11336/283698instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982026-08-25 14:38:25.872CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted) |
| title |
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted) |
| spellingShingle |
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted) Regnier, M. COSMIC MICROWAVE BACKGROUND DATA ANALYSIS INFLATION |
| title_short |
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted) |
| title_full |
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted) |
| title_fullStr |
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted) |
| title_full_unstemmed |
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted) |
| title_sort |
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted) |
| dc.creator.none.fl_str_mv |
Regnier, M. Laclavere, T. Hamilton, Jean-christophe Bunn, E. Chabirand, V. Chanial, P. Goetz, L. Kardum, L. Masson, P. Mirón Granese, Nahuel Omar Scoccola, Claudia Graciela Torchinsky, S. Battistelli, E. Bersanelli, M. Columbro, F. Coppolecchia, A. Costanza, María Belén De Bernardis, P. De Gasperis, G. Ferrazolli, S. Flood, A. B. Ganga, K. M. Gervasi, M. Grandsire, L. Manzan, E. Masi, S. Mennella, A. Mousset, L. O'Sullivan, C. Paiella, A. Piacentini, F. Piat, M. Piccirillo, L. Rasztocky, Emiliano Stolpovskiy, M. Zannoni, M. |
| author |
Regnier, M. |
| author_facet |
Regnier, M. Laclavere, T. Hamilton, Jean-christophe Bunn, E. Chabirand, V. Chanial, P. Goetz, L. Kardum, L. Masson, P. Mirón Granese, Nahuel Omar Scoccola, Claudia Graciela Torchinsky, S. Battistelli, E. Bersanelli, M. Columbro, F. Coppolecchia, A. Costanza, María Belén De Bernardis, P. De Gasperis, G. Ferrazolli, S. Flood, A. B. Ganga, K. M. Gervasi, M. Grandsire, L. Manzan, E. Masi, S. Mennella, A. Mousset, L. O'Sullivan, C. Paiella, A. Piacentini, F. Piat, M. Piccirillo, L. Rasztocky, Emiliano Stolpovskiy, M. Zannoni, M. |
| author_role |
author |
| author2 |
Laclavere, T. Hamilton, Jean-christophe Bunn, E. Chabirand, V. Chanial, P. Goetz, L. Kardum, L. Masson, P. Mirón Granese, Nahuel Omar Scoccola, Claudia Graciela Torchinsky, S. Battistelli, E. Bersanelli, M. Columbro, F. Coppolecchia, A. Costanza, María Belén De Bernardis, P. De Gasperis, G. Ferrazolli, S. Flood, A. B. Ganga, K. M. Gervasi, M. Grandsire, L. Manzan, E. Masi, S. Mennella, A. Mousset, L. O'Sullivan, C. Paiella, A. Piacentini, F. Piat, M. Piccirillo, L. Rasztocky, Emiliano Stolpovskiy, M. Zannoni, M. |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
COSMIC MICROWAVE BACKGROUND DATA ANALYSIS INFLATION |
| topic |
COSMIC MICROWAVE BACKGROUND DATA ANALYSIS INFLATION |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
The detection of B-modes in the CMB polarization pattern is a major issue in modern cosmology and must therefore be handled with analytical methods that produce reliable results. We describe a method that uses the frequency dependency of the QUBIC synthesized beam to perform component separation at the map-making stage, to obtain more precise results. We aim to demonstrate the feasibility of component separation during the map-making stage in time domain space. This new technique leads to a more accurate description of the data and reduces the biases in cosmological analysis. The method uses a library for highly parallel computation which facilitates the programming and permits the description of experiments as easily manipulated operators. These operators can be combined to obtain a joint analysis using several experiments leading to maximized precision. The results show that the method works well and permits end-to-end analysis for the CMB experiments, and in particular, for QUBIC. The method includes astrophysical foregrounds, and also systematic effects like gain variation in the detectors. We developed a software pipeline that produces uncertainties on tensor-to-scalar ratio at the level of using only QUBIC simulated data. Fil: Regnier, M.. Universite de Paris; Francia Fil: Laclavere, T.. Universite de Paris; Francia Fil: Hamilton, Jean-christophe. Universite de Paris; Francia Fil: Bunn, E.. University of Richmond; Estados Unidos Fil: Chabirand, V.. Universite de Paris; Francia. École Polytechnique; Francia Fil: Chanial, P.. Universite de Paris; Francia Fil: Goetz, L.. Universite de Paris; Francia Fil: Kardum, L.. Universite de Paris; Francia Fil: Masson, P.. Universite de Paris; Francia Fil: Mirón Granese, Nahuel Omar. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Scoccola, Claudia Graciela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Universidad de Chile. Facultad de Ciencias Físicas y Matemáticas; Chile Fil: Torchinsky, S.. Université Paris Cité; Francia Fil: Battistelli, E.. Università degli studi di Roma "La Sapienza"; Italia Fil: Bersanelli, M.. Università degli Studi di Milano; Italia Fil: Columbro, F.. Università degli studi di Roma "La Sapienza"; Italia Fil: Coppolecchia, A.. Università degli studi di Roma "La Sapienza"; Italia Fil: Costanza, María Belén. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: De Bernardis, P.. Università degli studi di Roma "La Sapienza"; Italia Fil: De Gasperis, G.. Università degli studi di Roma "La Sapienza"; Italia Fil: Ferrazolli, S.. Università degli studi di Roma "La Sapienza"; Italia Fil: Flood, A. B.. National University of Ireland Galway; Irlanda Fil: Ganga, K. M.. Université Paris Cité; Francia Fil: Gervasi, M.. Università degli Studi di Milano; Italia Fil: Grandsire, L.. Université Paris Cité; Francia Fil: Manzan, E.. Università degli Studi di Milano; Italia Fil: Masi, S.. Università degli studi di Roma "La Sapienza"; Italia Fil: Mennella, A.. Università degli Studi di Milano; Italia Fil: Mousset, L.. Sorbonne University; Francia Fil: O'Sullivan, C.. National University of Ireland Galway; Irlanda Fil: Paiella, A.. Università degli studi di Roma "La Sapienza"; Italia Fil: Piacentini, F.. Università degli studi di Roma "La Sapienza"; Italia Fil: Piat, M.. Université Paris Cité; Francia Fil: Piccirillo, L.. University of Manchester; Reino Unido Fil: Rasztocky, Emiliano. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Stolpovskiy, M.. University of Bern; Suiza Fil: Zannoni, M.. Università degli Studi di Milano; Italia |
| description |
The detection of B-modes in the CMB polarization pattern is a major issue in modern cosmology and must therefore be handled with analytical methods that produce reliable results. We describe a method that uses the frequency dependency of the QUBIC synthesized beam to perform component separation at the map-making stage, to obtain more precise results. We aim to demonstrate the feasibility of component separation during the map-making stage in time domain space. This new technique leads to a more accurate description of the data and reduces the biases in cosmological analysis. The method uses a library for highly parallel computation which facilitates the programming and permits the description of experiments as easily manipulated operators. These operators can be combined to obtain a joint analysis using several experiments leading to maximized precision. The results show that the method works well and permits end-to-end analysis for the CMB experiments, and in particular, for QUBIC. The method includes astrophysical foregrounds, and also systematic effects like gain variation in the detectors. We developed a software pipeline that produces uncertainties on tensor-to-scalar ratio at the level of using only QUBIC simulated data. |
| publishDate |
2024 |
| dc.date.none.fl_str_mv |
2024-09 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/283698 Regnier, M.; Laclavere, T.; Hamilton, Jean-christophe; Bunn, E.; Chabirand, V.; et al.; Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted); Cornell University; arXiv.org; 9-2024; 1-15 2331-8422 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/283698 |
| identifier_str_mv |
Regnier, M.; Laclavere, T.; Hamilton, Jean-christophe; Bunn, E.; Chabirand, V.; et al.; Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry (submitted); Cornell University; arXiv.org; 9-2024; 1-15 2331-8422 CONICET Digital CONICET |
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eng |
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eng |
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info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2409.18714 info:eu-repo/semantics/altIdentifier/doi/10.48550/arXiv.2409.18714 |
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openAccess |
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Cornell University |
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Cornell University |
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