QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43

This work focuses on the study of the anomalous microwave emission (AME), an important emission mechanism between 10 and 60 GHz whose polarisation properties are not yet fully understood and is therefore a potential contaminant for future cosmic microwave background (CMB) polarisation observations....

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Authors: González-González, R., Génova-Santos, R., Rubiño-Martín, J. A., Peel, Michael W., Guidi, Federica, López-Caraballo, Carlos H., Férnandez-Torreiro, M., Rebolo López, Rafael, Hernández-Monteagudo, Carlos, Adak, Debabrata, Artal, Eduardo, Ashdown, Mark, Barreiro, R. Belén, Casas-Reinares, F. J., Cepeda-Arroita, Roke, Hoz, Elena de la, Fasano, Alessandro, Herranz, Diego, Hoyland, Roger J., Martínez-González, Enrique, Pascual Cisneros, Guillermo, Piccirillo, Lucio, Poidevin, Frédérick, Ruiz-Granados, Beatriz, Tramonte, Denis, Vansyngel, F., Vielva, Patricio, Watson, R. A.
Format: article
Status:Published version
Publication Date:2025
Country:España
Institution:Consejo Superior de Investigaciones Científicas (CSIC)
Repository:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/391955
Online Access:http://hdl.handle.net/10261/391955
Access Level:Open access
Keyword:ISM: general
HII regions
Cosmic background radiation
Cosmology: observations
Diffuse radiation
Inflation
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dc.title.none.fl_str_mv QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43
title QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43
spellingShingle QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43
González-González, R.
ISM: general
HII regions
Cosmic background radiation
Cosmology: observations
Diffuse radiation
Inflation
title_short QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43
title_full QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43
title_fullStr QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43
title_full_unstemmed QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43
title_sort QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43
dc.creator.none.fl_str_mv González-González, R.
Génova-Santos, R.
Rubiño-Martín, J. A.
Peel, Michael W.
Guidi, Federica
López-Caraballo, Carlos H.
Férnandez-Torreiro, M.
Rebolo López, Rafael
Hernández-Monteagudo, Carlos
Adak, Debabrata
Artal, Eduardo
Ashdown, Mark
Barreiro, R. Belén
Casas-Reinares, F. J.
Cepeda-Arroita, Roke
Hoz, Elena de la
Fasano, Alessandro
Herranz, Diego
Hoyland, Roger J.
Martínez-González, Enrique
Pascual Cisneros, Guillermo
Piccirillo, Lucio
Poidevin, Frédérick
Ruiz-Granados, Beatriz
Tramonte, Denis
Vansyngel, F.
Vielva, Patricio
Watson, R. A.
author González-González, R.
author_facet González-González, R.
Génova-Santos, R.
Rubiño-Martín, J. A.
Peel, Michael W.
Guidi, Federica
López-Caraballo, Carlos H.
Férnandez-Torreiro, M.
Rebolo López, Rafael
Hernández-Monteagudo, Carlos
Adak, Debabrata
Artal, Eduardo
Ashdown, Mark
Barreiro, R. Belén
Casas-Reinares, F. J.
Cepeda-Arroita, Roke
Hoz, Elena de la
Fasano, Alessandro
Herranz, Diego
Hoyland, Roger J.
Martínez-González, Enrique
Pascual Cisneros, Guillermo
Piccirillo, Lucio
Poidevin, Frédérick
Ruiz-Granados, Beatriz
Tramonte, Denis
Vansyngel, F.
Vielva, Patricio
Watson, R. A.
author_role author
author2 Génova-Santos, R.
Rubiño-Martín, J. A.
Peel, Michael W.
Guidi, Federica
López-Caraballo, Carlos H.
Férnandez-Torreiro, M.
Rebolo López, Rafael
Hernández-Monteagudo, Carlos
Adak, Debabrata
Artal, Eduardo
Ashdown, Mark
Barreiro, R. Belén
Casas-Reinares, F. J.
Cepeda-Arroita, Roke
Hoz, Elena de la
Fasano, Alessandro
Herranz, Diego
Hoyland, Roger J.
Martínez-González, Enrique
Pascual Cisneros, Guillermo
Piccirillo, Lucio
Poidevin, Frédérick
Ruiz-Granados, Beatriz
Tramonte, Denis
Vansyngel, F.
Vielva, Patricio
Watson, R. A.
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
dc.contributor.none.fl_str_mv Agencia Estatal de Investigación (España)
Ministerio de Ciencia e Innovación (España)
Ministerio de Economía y Competitividad (España)
Ministerio de Ciencia, Innovación y Universidades (España)
Instituto de Salud Carlos III
Gobierno de Canarias
European Research Council
European Commission
Department of Energy (US)
Ministero dell'Istruzione, dell'Università e della Ricerca
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv ISM: general
HII regions
Cosmic background radiation
Cosmology: observations
Diffuse radiation
Inflation
topic ISM: general
HII regions
Cosmic background radiation
Cosmology: observations
Diffuse radiation
Inflation
description This work focuses on the study of the anomalous microwave emission (AME), an important emission mechanism between 10 and 60 GHz whose polarisation properties are not yet fully understood and is therefore a potential contaminant for future cosmic microwave background (CMB) polarisation observations. We used new QUIJOTE-MFI maps at 11, 13, 17, and 19 GHz obtained from the combination of the public wide survey data and additional 1800 h of dedicated raster scan observations together with other public ancillary data, including WMAP and Planck, to study the polarisation properties of the AME in three Galactic regions: ρ Ophiuchi, Perseus, and W43. We obtained the spectral energy distributions (SEDs) of the three regions over the frequency range 0.4–3000 GHz in intensity and polarisation. The intensity SEDs are well described by a combination of free-free emission, thermal dust, AME, and CMB anisotropies. In polarisation, we extracted the flux densities using all available data between 11 and 353 GHz. We implemented an improved intensity-to-polarisation leakage correction that allowed reliable polarisation constraints well below the 1% level from Planck-LFI data to be derived for the first time. A frequency stacking of maps in the range 10–60 GHz allowed us to reduce the statistical noise and to push the upper limits on the AME polarisation level. We obtained upper limits on the AME polarisation fraction of the order ≲1% (95% confidence level) for the three regions. In particular, we obtained ΠAME < 1.0% (at 28.4 GHz), ΠAME < 0.9% (at 28.4 GHz), and ΠAME < 0.28% (at 33 GHz) in ρ Ophiuchi, Perseus, and W43, respectively. At the QUIJOTE 17 GHz frequency band, we found ΠAME < 5.0% for ρ Ophiuchi, ΠAME < 3.4% for Perseus, and ΠAME < 0.85% for W43. We note that for the ρ Ophiuchi molecular cloud, the new QUIJOTE-MFI data allowed us to set the first constraints on the AME polarisation in the range 10–20 GHz. Our final upper limits derived using the stacking procedure are ΠAME < 0.58% for ρ Ophiuchi, ΠAME < 0.67% for Perseus, and ΠAME < 0.31% for W43. Altogether, these are the most stringent constraints to date on the AME polarisation fraction of these three star-forming regions.
publishDate 2025
dc.date.none.fl_str_mv 2025
2025
2025
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url http://hdl.handle.net/10261/391955
dc.language.none.fl_str_mv Inglés
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spelling QUIJOTE scientific results: XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43González-González, R.Génova-Santos, R.Rubiño-Martín, J. A.Peel, Michael W.Guidi, FedericaLópez-Caraballo, Carlos H.Férnandez-Torreiro, M.Rebolo López, RafaelHernández-Monteagudo, CarlosAdak, DebabrataArtal, EduardoAshdown, MarkBarreiro, R. BelénCasas-Reinares, F. J.Cepeda-Arroita, RokeHoz, Elena de laFasano, AlessandroHerranz, DiegoHoyland, Roger J.Martínez-González, EnriquePascual Cisneros, GuillermoPiccirillo, LucioPoidevin, FrédérickRuiz-Granados, BeatrizTramonte, DenisVansyngel, F.Vielva, PatricioWatson, R. A.ISM: generalHII regionsCosmic background radiationCosmology: observationsDiffuse radiationInflationThis work focuses on the study of the anomalous microwave emission (AME), an important emission mechanism between 10 and 60 GHz whose polarisation properties are not yet fully understood and is therefore a potential contaminant for future cosmic microwave background (CMB) polarisation observations. We used new QUIJOTE-MFI maps at 11, 13, 17, and 19 GHz obtained from the combination of the public wide survey data and additional 1800 h of dedicated raster scan observations together with other public ancillary data, including WMAP and Planck, to study the polarisation properties of the AME in three Galactic regions: ρ Ophiuchi, Perseus, and W43. We obtained the spectral energy distributions (SEDs) of the three regions over the frequency range 0.4–3000 GHz in intensity and polarisation. The intensity SEDs are well described by a combination of free-free emission, thermal dust, AME, and CMB anisotropies. In polarisation, we extracted the flux densities using all available data between 11 and 353 GHz. We implemented an improved intensity-to-polarisation leakage correction that allowed reliable polarisation constraints well below the 1% level from Planck-LFI data to be derived for the first time. A frequency stacking of maps in the range 10–60 GHz allowed us to reduce the statistical noise and to push the upper limits on the AME polarisation level. We obtained upper limits on the AME polarisation fraction of the order ≲1% (95% confidence level) for the three regions. In particular, we obtained ΠAME < 1.0% (at 28.4 GHz), ΠAME < 0.9% (at 28.4 GHz), and ΠAME < 0.28% (at 33 GHz) in ρ Ophiuchi, Perseus, and W43, respectively. At the QUIJOTE 17 GHz frequency band, we found ΠAME < 5.0% for ρ Ophiuchi, ΠAME < 3.4% for Perseus, and ΠAME < 0.85% for W43. We note that for the ρ Ophiuchi molecular cloud, the new QUIJOTE-MFI data allowed us to set the first constraints on the AME polarisation in the range 10–20 GHz. Our final upper limits derived using the stacking procedure are ΠAME < 0.58% for ρ Ophiuchi, ΠAME < 0.67% for Perseus, and ΠAME < 0.31% for W43. Altogether, these are the most stringent constraints to date on the AME polarisation fraction of these three star-forming regions.The QUIJOTE experiment is being developed by the Instituto de Astrofisica de Canarias (IAC), the Instituto de Fisica de Cantabria (IFCA), and the Universities of Cantabria, Manchester and Cambridge. Partial financial support was provided by the Spanish Ministry of Science and Innovation under the projects AYA2007-68058-C03-01, AYA2007-68058-C03-02, AYA2010-21766-C03-01, AYA2010-21766-C03-02, AYA2014-60438-P, ESP2015-70646-C2-1-R, AYA2017-84185-P, ESP2017-83921-C2-1-R, PGC2018-101814-B-I00, PID2019-110610RB-C21, PID2020-120514GB-I00, IACA13-3E-2336, IACA15-BE-3707, EQC2018-004918-P, PID2023-150398NB-I00 and PID2023-151567NB-I00, the Severo Ochoa Programs SEV-2015-0548 and CEX2019-000920-S, the Maria de Maeztu Program MDM-2017-0765, and by the Consolider-Ingenio project CSD2010-00064 (EPI: Exploring the Physics of Inflation). We acknowledge support from the ACIISI, Consejeria de Economia, Conocimiento y Empleo del Gobierno de Canarias and the European Regional Development Fund (ERDF) under grant with reference ProID2020010108, and Red de Investigación RED2022-134715-T funded by MCIN/AEI/10.13039/501100011033. This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement number 687312 (RADIOFOREGROUNDS), and the Horizon Europe research and innovation program under GA 101135036 (RadioForegroundsPlus). This research made use of computing time available on the high-performance computing systems at the IAC. We thankfully acknowledge the technical expertise and assistance provided by the Spanish Supercomputing Network (Red Española de Supercomputación), as well as the computer resources used: the Deimos/Diva Supercomputer, located at the IAC. This research used resources of the National Energy Research Scientific Computing Center, that is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. RGG acknowledges support from Italian Ministry of education, university and research. MFT acknowledges support from from the Agencia Estatal de Investigación (AEI) of the Ministerio de Ciencia, Innovación y Universidades (MCIU), from the European Social Fund (ESF) under grant with reference PRE-C-2018-0067 and from the French Programme d’investissements d’avenir through the Enigmass Labex. FP acknowledges support from the Spanish Ministerio de Ciencia, Innovación y Universidades (MICINN) under grant numbers PID2022-141915NB-C21. DT acknowledges financial support from the XJTLU Research Development Fund (RDF) grant with number RDF-22-02-068. CHM acknowledges financial support from the Spanish Ministry of Science and Innovation under project PID2021-126616NB-I00.With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2019-000920-S).Peer reviewedEDP SciencesAgencia Estatal de Investigación (España)Ministerio de Ciencia e Innovación (España)Ministerio de Economía y Competitividad (España)Ministerio de Ciencia, Innovación y Universidades (España)Instituto de Salud Carlos IIIGobierno de CanariasEuropean Research CouncilEuropean CommissionDepartment of Energy (US)Ministero dell'Istruzione, dell'Università e della RicercaConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202520252025info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/391955reponame:DIGITAL.CSIC. 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