dc.contributor.author | Hale, C. L. | |
dc.contributor.author | Heywood, I. | |
dc.contributor.author | Jarvis, M. J. | |
dc.contributor.author | Whittam, I. H. | |
dc.contributor.author | Best, P. N. | |
dc.contributor.author | An, Fangxia | |
dc.contributor.author | Bowler, R. A. A. | |
dc.contributor.author | Harrison, I. | |
dc.contributor.author | Matthews, A. | |
dc.contributor.author | Smith, D. J. B. | |
dc.contributor.author | Taylor, A. R. | |
dc.contributor.author | Vaccari, M. | |
dc.date.accessioned | 2025-01-28T09:30:01Z | |
dc.date.available | 2025-01-28T09:30:01Z | |
dc.date.issued | 2025-01-01 | |
dc.identifier.citation | Hale , 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.issn | 0035-8711 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/2411.04958v1 | |
dc.identifier.uri | http://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.abstract | The 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.extent | 25 | |
dc.format.extent | 8897615 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.subject | astro-ph.GA | |
dc.subject | radio continuum: general | |
dc.subject | surveys | |
dc.subject | catalogues | |
dc.subject | radio continuum: galaxies | |
dc.subject | Astronomy and Astrophysics | |
dc.subject | Space and Planetary Science | |
dc.title | Mightee: The Continuum Survey Data Release 1 | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
dc.identifier.url | http://www.scopus.com/inward/record.url?scp=85215687743&partnerID=8YFLogxK | |
rioxxterms.versionofrecord | 10.1093/mnras/stae2528 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |