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dc.contributor.authorBondi, M.
dc.contributor.authorScaramella, R.
dc.contributor.authorZamorani, G.
dc.contributor.authorCiliegi, P.
dc.contributor.authorVitello, F.
dc.contributor.authorArias, M.
dc.contributor.authorBest, P.N.
dc.contributor.authorBonato, M.
dc.contributor.authorBotteon, A.
dc.contributor.authorBrienza, M.
dc.contributor.authorBrunetti, G.
dc.contributor.authorHardcastle, M. J.
dc.contributor.authorMagliocchetti, M.
dc.contributor.authorMassaro, F.
dc.contributor.authorMorabito, L. K
dc.contributor.authorPentericci, L.
dc.contributor.authorPrandoni, I.
dc.contributor.authorRöttgering, H. J. A.
dc.contributor.authorShimwell, T. W.
dc.contributor.authorTasse, C.
dc.contributor.authorWeeren, R. J. van
dc.contributor.authorWhite, G. J.
dc.date.accessioned2024-04-12T15:30:01Z
dc.date.available2024-04-12T15:30:01Z
dc.date.issued2024-03-18
dc.identifier.citationBondi , M , Scaramella , R , Zamorani , G , Ciliegi , P , Vitello , F , Arias , M , Best , P N , Bonato , M , Botteon , A , Brienza , M , Brunetti , G , Hardcastle , M J , Magliocchetti , M , Massaro , F , Morabito , L K , Pentericci , L , Prandoni , I , Röttgering , H J A , Shimwell , T W , Tasse , C , Weeren , R J V & White , G J 2024 , ' LOFAR HBA observations of the Euclid Deep Field North (EDFN) ' , Astronomy & Astrophysics , vol. 683 , A179 , pp. 1-12 . https://doi.org/10.1051/0004-6361/202348333
dc.identifier.issn0004-6361
dc.identifier.otherRIS: urn:90F8083742BD4784D3D5359F546FB034
dc.identifier.otherRIS: 10.105100046361202348333
dc.identifier.urihttp://hdl.handle.net/2299/27747
dc.description© 2024 The Author(s). Published by EDP Sciences, This is an open access article distributed under the terms of the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/
dc.description.abstractWe present the first deep (72 h of observations) radio image of the Euclid Deep Field North (EDFN) obtained with the LOw-Frequency ARray (LOFAR) High Band Antenna (HBA) at 144 MHz. The EDFN is the latest addition to the LOFAR Two-Metre Sky Survey (LoTSS) Deep Fields, and these observations represent the first data release for this field. The observations produced a 6″ resolution image with a central rms noise of 32 μJy beam−1. A catalogue of ~23 000 radio sources above a signal-to-noise ratio threshold of five is extracted from the inner circular 10 deg2 region. We discuss the data analysis, and we provide a detailed description of how we derived the catalogue of radio sources, the issues related to direction-dependent calibration, and their effects on the final products. Finally, we derive the radio source counts at 144 MHz in the EDFN using catalogues of mock radio sources to derive the completeness correction factors. The source counts in the EDFN are consistent with those obtained from the first data release of the other LoTSS Deep Fields (ELAIS-N1, Lockman Hole and Bootes), despite the different method adopted to construct the final catalogue and to assess its completeness.en
dc.format.extent12
dc.format.extent772957
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.titleLOFAR HBA observations of the Euclid Deep Field North (EDFN)en
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSPECS Deans Group
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1051/0004-6361/202348333
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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