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dc.contributor.authorHale, C. L.
dc.contributor.authorHeywood, I.
dc.contributor.authorJarvis, M. J.
dc.contributor.authorWhittam, I. H.
dc.contributor.authorBest, P. N.
dc.contributor.authorAn, Fangxia
dc.contributor.authorBowler, R. A. A.
dc.contributor.authorHarrison, I.
dc.contributor.authorMatthews, A.
dc.contributor.authorSmith, D. J. B.
dc.contributor.authorTaylor, A. R.
dc.contributor.authorVaccari, M.
dc.date.accessioned2025-01-28T09:30:01Z
dc.date.available2025-01-28T09:30:01Z
dc.date.issued2025-01-01
dc.identifier.citationHale , C L , Heywood , I , Jarvis , M J , Whittam , I H , Best , P N , An , F , Bowler , R A A , Harrison , I , Matthews , A , Smith , D J B , Taylor , A R & Vaccari , M 2025 , ' Mightee: The Continuum Survey Data Release 1 ' , Monthly Notices of the Royal Astronomical Society , vol. 536 , no. 3 , stae2528 , pp. 2187-2211 . https://doi.org/10.1093/mnras/stae2528
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/2411.04958v1
dc.identifier.urihttp://hdl.handle.net/2299/28741
dc.description© 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an open access article distributed under the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/
dc.description.abstractThe MeerKAT International GHz Tiered Extragalactic Exploration Surv e y (MIGHTEE) is one of the large surv e y projects using the MeerKAT telescope, co v ering four fields that have a wealth of ancillary data available. We present Data Release 1 of the MIGHTEE continuum surv e y, releasing total intensity images and catalogues o v er ∼20 de g 2 , across three fields at ∼1.2-1.3 GHz. This includes 4.2 de g 2 o v er the Cosmic Evolution Surv e y (COSMOS) field, 14.4 de g 2 o v er the XMM Large-Scale Structure (XMM-LSS) field and deeper imaging o v er 1.5 de g 2 of the Extended Chandra Deep Field South (CDFS). We release images at both a lower resolution (7-9 arcsec) and higher resolution ( ∼5 arcsec). These images have central rms sensitivities of ∼1 . 3 -2.7 μJy beam -1 ( ∼1 . 2 -3.6 μJy beam -1 ) in the lower (higher) resolution images, respectively. We also release catalogues comprised of ∼144 000 ( ∼114 000) sources using the lower (higher) resolution images. We compare the astrometry and flux-density calibration with the Early Science data in the COSMOS and XMM-LSS fields and previous radio observations in the CDFS field, finding broad agreement. Furthermore, we extend the source counts at the ∼10 μJy level to these larger areas ( ∼20 deg 2 ) and, using the areal co v erage of MIGHTEE we measure the sample variance for differing areas of sky. We find a typical sample variance of 10 -20 per cent for 0.3 and 0.5 de g 2 subre gions at S 1 . 4 ≤200 μJy, which increases at brighter flux densities, given the lower source density and expected higher galaxy bias for these sources.en
dc.format.extent25
dc.format.extent8897615
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.GA
dc.subjectradio continuum: general
dc.subjectsurveys
dc.subjectcatalogues
dc.subjectradio continuum: galaxies
dc.subjectAstronomy and Astrophysics
dc.subjectSpace and Planetary Science
dc.titleMightee: The Continuum Survey Data Release 1en
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85215687743&partnerID=8YFLogxK
rioxxterms.versionofrecord10.1093/mnras/stae2528
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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