QUIJOTE scientific results – IX. Radio sources in the QUIJOTE-MFI wide survey maps

  1. Herranz, D 3
  2. López-Caniego, M 1011
  3. López-Caraballo, C H 12
  4. Génova-Santos, R T 12
  5. Perrott, Y C 16
  6. Rubiño-Martín, J A 12
  7. Rebolo, R 1212
  8. Artal, E 9
  9. Ashdown, M 67
  10. Barreiro, R B 3
  11. Casas, F J 3
  12. de la Hoz, E 35
  13. Fernández-Torreiro, M 12
  14. Guidi, F 1213
  15. Hoyland, R J 12
  16. Lasenby, A N 67
  17. Martínez-González, E 3
  18. Peel, M W 12
  19. Piccirillo, L 8
  20. Poidevin, F 12
  21. Ruiz-Granados, B 124
  22. Tramonte, D 121415
  23. Vansyngel, F 12
  24. Vielva, P 3
  25. Watson, R A 8
  1. 1 Instituto de Astrofísica de Canarias , E-38200 La Laguna, Tenerife, Spain
  2. 2 Departamento de Astrofísica, Universidad de La Laguna , E-38206 La Laguna, Tenerife, Spain
  3. 3 Instituto de Física de Cantabria (IFCA), CSIC-Univ. de Cantabria , Avda. los Castros s/n, E-39005 Santander, Spain
  4. 4 Departamento de Física. Facultad de Ciencias. Universidad de Córdoba. Campus de Rabanales , Edif. C2. Planta Baja. E-14071 Córdoba, Spain
  5. 5 Dpto. de Física Moderna, Universidad de Cantabria , Avda. de los Castros s/n, E-39005 Santander, Spain
  6. 6 Astrophysics Group, Cavendish Laboratory, University of Cambridge , J J Thomson Avenue, Cambridge CB3 0HE, UK
  7. 7 Kavli Institute for Cosmology, University of Cambridge , Madingley Road, Cambridge CB3 0HA, UK
  8. 8 Jodrell Bank Centre for Astrophysics, Alan Turing Building, Department of Physics and Astronomy, School of Nature Sciences, University of Manchester , Oxford Road, Manchester M13 9PL, UK
  9. 9 Departamento de Ingenieria de COMunicaciones (DICOM), Edificio Ingenieria de Telecomunicacion , Plaza de la Ciencia s/n, E-39005 Santander, Spain
  10. 10 Aurora Technology for the European Space Agency (ESA), European Space Astronomy Centre (ESAC) , Camino Bajo del Castillo s/n, E-28692 Villanueva de la Cañada, Madrid, Spain
  11. 11 Universidad Europea de Madrid , E-28670 Madrid, Spain
  12. 12 Consejo Superior de Investigaciones Cientificas , E-28006 Madrid, Spain
  13. 13 Institut d’Astrophysique de Paris , UMR 7095, CNRS & Sorbonne Université, 98 bis boulevard Arago, F-75014 Paris, France
  14. 14 Purple Mountain Observatory , CAS, No.10 Yuanhua Road, Qixia District, Nanjing 210034, China
  15. 15 NAOC-UKZN Computational Astrophysics Center (NUCAC), University of Kwazulu-Natal , Durban 4000, South Africa
  16. 16 School of Chemical and Physical Sciences, Victoria University of Wellington , PO Box 600, Wellington 6140, New Zealand
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Revista:
Monthly Notices of the Royal Astronomical Society

ISSN: 0035-8711,  1365-2966

Año de publicación: 2023

Volumen: 519

Número: 3

Páginas: 3526-3545

Tipo: Artículo

DOI: 10.1093/MNRAS/STAC3657 GOOGLE SCHOLAR lock_openAcceso abierto editor

Otras publicaciones en: Monthly Notices of the Royal Astronomical Society

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Resumen

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 percent 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.

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