dc.contributor.author | Herranz Muñoz, Diego | |
dc.contributor.author | López-Caniego, Marcos | |
dc.contributor.author | López-Caraballo, Carlos H. | |
dc.contributor.author | Génova-Santos, Ricardo Tanausu | |
dc.contributor.author | Perrott, Yvette C. | |
dc.contributor.author | Rubiño-Martín, Alberto Alberto | |
dc.contributor.author | Rebolo, R. L. | |
dc.contributor.author | Artal Latorre, Eduardo | |
dc.contributor.author | Ashdown, Mark A.J. | |
dc.contributor.author | Barreiro Vilas, Rita Belén | |
dc.contributor.author | Casas Reinares, Francisco Javier | |
dc.contributor.author | Hoz López-Collado, Elena de la | |
dc.contributor.author | Fernandez-Torreiro, Mateo | |
dc.contributor.author | Guidi, Frederica | |
dc.contributor.author | Hoyland, Roger J. | |
dc.contributor.author | Lasenby, Anthony N. | |
dc.contributor.author | Martínez González, Enrique | |
dc.contributor.author | Peel, Mike W. | |
dc.contributor.author | Piccirillo, L. | |
dc.contributor.author | Vielva Martínez, Patricio | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2024-02-16T08:48:47Z | |
dc.date.available | 2024-02-16T08:48:47Z | |
dc.date.issued | 2023-03-01 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.issn | 1365-2966 | |
dc.identifier.other | AYA2007-68058-C03-01 | es_ES |
dc.identifier.other | AYA2007-68058-C03-02 | es_ES |
dc.identifier.other | AYA2010-21766-C03-01 | es_ES |
dc.identifier.other | AYA2010-21766-C03-02 | es_ES |
dc.identifier.other | AYA2014-60438-P | es_ES |
dc.identifier.other | ESP2015-70646-C2-1-R | es_ES |
dc.identifier.other | AYA2017-84185-P | es_ES |
dc.identifier.other | ESP2017-83921-C2-1-R | es_ES |
dc.identifier.other | AYA2017-90675-REDC | es_ES |
dc.identifier.other | PID2019-105552RB-C43 | es_ES |
dc.identifier.uri | https://hdl.handle.net/10902/31793 | |
dc.description.abstract | We present the catalogue of Q-U-I JOint TEnerife (QUIJOTE) Wide Survey radio sources extracted from the maps of the Multi-Frequency Instrument compiled between 2012 and 2018. The catalogue contains 786 sources observed in intensity and polarization, and is divided into two separate sub-catalogues: one containing 47 bright sources previously studied by the Planck collaboration and an extended catalogue of 739 sources either selected from the Planck Second Catalogue of Compact Sources or found through a blind search carried out with a Mexican Hat 2 wavelet. A significant fraction of the sources in our catalogue (38.7 per cent) are within the |b| ≤ 20◦ region of the Galactic plane. We determine statistical properties for those sources that are likely to be extragalactic. We find that these statistical properties are compatible with currently available models, with a ∼1.8 Jy completeness limit at 11 GHz. We provide the polarimetric properties of (38, 33, 31, 23) sources with P detected above the 99.99 per cent significance level at (11, 13, 17, 19) GHz respectively. Median polarization fractions are in the 2.8–4.7 per cent range in the 11–19 GHz frequency interval. We do not distinguish between Galactic and extragalactic sources here. The results presented here are consistent with those reported in the literature for flat- and steep-spectrum radio sources. | es_ES |
dc.description.sponsorship | We thank the staff of the Teide Observatory for invaluable assistance in the commissioning and operation of QUIJOTE. The QUIJOTE experiment is being developed by the Instituto de Astrofísica de Canarias (IAC), the Instituto de Física 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, AYA2017-90675-REDC (co-funded with EU FEDER funds), PGC2018-101814-B-I00, PID2019-110610RBC21, PID2020-120514GB-I00, IACA13-3E-2336, IACA15-BE3707, EQC2018-004918-P, the Severo Ochoa Programs SEV-2015- 0548 and CEX2019-000920-S, the María de Maeztu Program MDM-2017-0765, and by the Consolider-Ingenio project CSD2010- 00064 (EPI: Exploring the Physics of Inflation). DT acknowledges the support from the Chinese Academy of Sciences (CAS) President’s International Fellowship Initiative (PIFI) with Grant N. 2020PM0042. FP acknowledges support from the Spanish State Research Agency (AEI) under grant number PID2019-105552RBC43. We acknowledge support from the ACIISI, Consejería de Economía, 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). This research has made use of data from the OVRO 40-m monitoring program (Richards et al. 2011), supported by private funding from the California Insitute of Technology and the Max Planck Institute forRadio Astronomy, and by NASA grants NNX08AW31G, NNX11A043G, and NNX14AQ89G and NSF grants AST-0808050 and AST-1109911. Some of the results in this paper have been derived using the HEALPY and HEALPIX packages (Gorski et al. 2005; Zonca et al. 2019). The packages ASTROPY (Astropy Collaboration 2013, 2018), SCIPY (Virtanen et al. 2020), MATPLOTLIB (Hunter 2007), NUMPY (Harris et al. 2020), and EMCEE (Foreman-Mackey et al. 2013) have been extensively used for data analysis and plotting. | es_ES |
dc.format.extent | 20 p. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | Oxford University Press | es_ES |
dc.rights | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2023 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | es_ES |
dc.source | Monthly Notices of the Royal Astronomical Society, 2023, 519(3), 3526-3545 | es_ES |
dc.subject.other | Cosmic background radiation | es_ES |
dc.subject.other | Radio continuum: galaxies | es_ES |
dc.title | QUIJOTE scientific results - IX. Radio sources in the QUIJOTE-MFI wide survey maps | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | https://doi.org/10.1093/mnras/stac3657 | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/EC/H2020/687312/EU/Ultimate modelling of Radio foregrounds: a key/RADIOFOREGROUNDS/ | es_ES |
dc.identifier.DOI | 10.1093/mnras/stac3657 | |
dc.type.version | publishedVersion | es_ES |