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http://hdl.handle.net/10261/349869
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dc.contributor.author | Poidevin, Frédérick | es_ES |
dc.contributor.author | Génova-Santos, R. | es_ES |
dc.contributor.author | Rubiño-Martín, J. A. | es_ES |
dc.contributor.author | López-Caraballo, Carlos H. | es_ES |
dc.contributor.author | Watson, R. A. | es_ES |
dc.contributor.author | Artal, Eduardo | es_ES |
dc.contributor.author | Ashdown, Mark | es_ES |
dc.contributor.author | Barreiro, R. Belén | es_ES |
dc.contributor.author | Casas-Reinares, F. J. | es_ES |
dc.contributor.author | Hoz, Elena de la | es_ES |
dc.contributor.author | Férnandez-Torreiro, M. | es_ES |
dc.contributor.author | Guidi, Federica | es_ES |
dc.contributor.author | Herranz, D. | es_ES |
dc.contributor.author | Hoyland, Roger J. | es_ES |
dc.contributor.author | Lasenby, Anthony N. | es_ES |
dc.contributor.author | Martínez-González, Enrique | es_ES |
dc.contributor.author | Peel, Michael W. | es_ES |
dc.contributor.author | Piccirillo, Lucio | es_ES |
dc.contributor.author | Rebolo López, Rafael | es_ES |
dc.contributor.author | Ruiz-Granados, Beatriz | es_ES |
dc.contributor.author | Tramonte, D. | es_ES |
dc.contributor.author | Vansyngel, F. | es_ES |
dc.contributor.author | Vielva, Patricio | es_ES |
dc.date.accessioned | 2024-03-11T08:37:14Z | - |
dc.date.available | 2024-03-11T08:37:14Z | - |
dc.date.issued | 2023 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society 519(3): 3481-3503 (2023) | es_ES |
dc.identifier.other | CEX2019-000920-S | - |
dc.identifier.uri | http://hdl.handle.net/10261/349869 | - |
dc.description.abstract | The QUIJOTE-MFI Northern Hemisphere Wide Survey has provided maps of the sky above declinations −30° at 11, 13, 17, and 19 GHz. These data are combined with ancillary data to produce Spectral Energy Distributions in intensity in the frequency range 0.4–3 000 GHz on a sample of 52 candidate compact sources harbouring anomalous microwave emission (AME). We apply a component separation analysis at 1° scale on the full sample from which we identify 44 sources with high AME significance. We explore correlations between different fitted parameters on this last sample. QUIJOTE-MFI data contribute to notably improve the characterization of the AME spectrum, and its separation from the other components. In particular, ignoring the 10–20 GHz data produces on average an underestimation of the AME amplitude, and an overestimation of the free–free component. We find an average AME peak frequency of 23.6 ± 3.6 GHz, about 4 GHz lower than the value reported in previous studies. The strongest correlation is found between the peak flux density of the thermal dust and of the AME component. A mild correlation is found between the AME emissivity (AAME/τ250) and the interstellar radiation field. On the other hand no correlation is found between the AME emissivity and the free–free radiation Emission Measure. Our statistical results suggest that the interstellar radiation field could still be the main driver of the intensity of the AME as regards spinning dust excitation mechanisms. On the other hand, it is not clear whether spinning dust would be most likely associated with cold phases of the interstellar medium rather than with hot phases dominated by free–free radiation. | es_ES |
dc.description.sponsorship | 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,AYA2017-90675-REDC (co-funded with EU FEDER - Fondo Europeo de Desarrollo Regional - funds), PGC2018-101814-B-I00, PID2019-110610RB-C21, PID2020-120514GB-I00, IACA13-3E-2336, IACA15-BE-3707, EQC2018-004918-P, 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. This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement number 687312 (RADIOFOREGROUNDS). FP acknowledges the European Commission under the Marie Sklodowska-Curie Actions within the European Union’s Horizon 2020 research and innovation programme under Grant Agreement number 658499 (PolAME). FP acknowledges support from the Spanish State Research Agency (AEI) under grant numbers PID2019-105552RB-C43. FG acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 101001897). EdlH acknowledge partial financial support from the Concepción Arenal Programme of the Universidad de Cantabria. BR-G acknowledges the Agenzia Spaziale Italiana – Istituto Nazionale di Fisica Nucleare (ASI-INFN) Agreement 2014-037-R.0. DT acknowledges the support from the Chinese Academy of Sciences President’s International Fellowship Initiative, Grant No. 2020PM0042. We acknowledge the use of data from the Planck /ESA mission, downloaded from the Planck Legacy Archive, and of the Legacy Archive for Microwave Background Data Analysis (LAMBDA). Support for LAMBDA is provided by the NASA Office of Space Science. Some of the results in this paper have been derived using the HEALPIX (Górski et al. 2005) package. | es_ES |
dc.description.sponsorship | With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2019-000920-S). | es_ES |
dc.format | application/pdf | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | Oxford University Press | es_ES |
dc.relation | info:eu-repo/grantAgreement/MINECO//AYA2014-60438-P/ES/COSMOLOGIA DE PRECISION CON PLANCK, QUIJOTE Y SDSS/ | es_ES |
dc.relation | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2017-83921-C2-1-R/ES/INSTRUMENTACION FOTONICA Y CALIBRACION DE KIDS PARA LA OBSERVACION DEL CMB. COSMOLOGIA DE FRONTERA CON DATOS DEL CMB Y LA LSS/ | es_ES |
dc.relation | info:eu-repo/grantAgreement/MINECO//ESP2015-70646-C2-1-R/ES/ESTUDIO DEL UNIVERSO PRIMIGENIO CON DATOS DE CMB Y LSS. DESARROLLO DE UN CORRELADOR ELECTRO-OPTICO Y PREPARACION PARA UNA FUTURA MISION ESPACIAL/ | es_ES |
dc.relation | info:eu-repo/grantAgreement/AEI//AYA2017-90675-REDC | es_ES |
dc.relation | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2017-84185-P/ES/COSMOLOGIA DE PRECISION CON EL FONDO COSMICO DE MICROONDAS: QUIJOTE, PLANCK Y OTROS EXPERIMENTOS DE MICROONDAS EN EL OBSERVATORIO DEL TEIDE/ | es_ES |
dc.relation | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-101814-B-I00/ES/LENTES OSCURAS. LA BUSQUEDA DE LA NATURALEZA DE LA MATERIA OSCURA/ | es_ES |
dc.relation | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-110610RB-C21/ES/SISTEMA DE CALIBRACION PARA ESPACIO Y ESTUDIO COMPARATIVO DE TECNOLOGIAS PARA INSTRUMENTACION DEL CMB. INVESTIGACION DE FRONTERA EN COSMOLOGIA CON LITEBIRD Y QUIJOTE/ | es_ES |
dc.relation | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2020-120514GB-I00/ES/COSMOLOGIA DE PRECISION CON EL FONDO COSMICO DE MICROONDAS: QUIJOTE Y OTROS EXPERIMENTOS DE MICROONDAS EN EL OBSERVATORIO DEL TEIDE, Y LA MISION ESPACIAL LITEBIRD/ | es_ES |
dc.relation | info:eu-repo/grantAgreement/MINECO//SEV-2015-0548/ES/INSTITUTO DE ASTROFISICA DE CANARIAS/ | es_ES |
dc.relation | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/CEX2019-000920-S | es_ES |
dc.relation | info:eu-repo/grantAgreement/AEI//MDM-2017-0765 | es_ES |
dc.relation | info:eu-repo/grantAgreement/EC/H2020/687312 | es_ES |
dc.relation.isversionof | Publisher's version | es_ES |
dc.relation.isbasedon | The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.1093/mnras/stac3151 | es_ES |
dc.rights | openAccess | es_ES |
dc.subject | Radiation mechanisms: general | es_ES |
dc.subject | Radiation mechanisms: non-thermal | es_ES |
dc.subject | Radiation mechanisms: thermal | es_ES |
dc.subject | ISM: clouds | es_ES |
dc.subject | Photodissociation region (PDR) | es_ES |
dc.subject | Radio continuum: ISM | es_ES |
dc.title | QUIJOTE scientific results – VII. Galactic AME sources in the QUIJOTE-MFI northern hemisphere wide survey | es_ES |
dc.type | artículo | es_ES |
dc.identifier.doi | 10.1093/mnras/stac3151 | - |
dc.description.peerreviewed | Peer reviewed | es_ES |
dc.relation.publisherversion | https://doi.org/10.1093/mnras/stac3151 | es_ES |
dc.identifier.e-issn | 1365-2966 | - |
dc.contributor.funder | Ministerio de Ciencia, Innovación y Universidades (España) | es_ES |
dc.contributor.funder | Ministerio de Ciencia e Innovación (España) | es_ES |
dc.contributor.funder | European Commission | es_ES |
dc.contributor.funder | Agencia Estatal de Investigación (España) | es_ES |
dc.contributor.funder | Gobierno de Canarias | es_ES |
dc.contributor.funder | Agenzia Spaziale Italiana | es_ES |
dc.contributor.funder | Istituto Nazionale di Fisica Nucleare | es_ES |
dc.contributor.funder | National Aeronautics and Space Administration (US) | es_ES |
dc.contributor.funder | European Commission | es_ES |
dc.relation.csic | Sí | es_ES |
oprm.item.hasRevision | no ko 0 false | * |
dc.identifier.funder | http://dx.doi.org/10.13039/501100011033 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100003981 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100000780 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100004837 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/100000104 | es_ES |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
item.openairetype | artículo | - |
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quijotesurvey.pdf | 3,55 MB | Adobe PDF | Visualizar/Abrir |
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