Show simple item record

dc.contributor.authorHeywood, I.
dc.contributor.authorJarvis, M.J.
dc.contributor.authorHale, C.L.
dc.date.accessioned2022-03-02T13:14:55Z
dc.date.available2022-03-02T13:14:55Z
dc.date.issued2022
dc.identifier.citationHeywood, I., Jarvis, M.J., Hale, C.L., Whittam, I.H., Bester, H.L., Hugo, B., Kenyon, J.S., Prescott, M., Smirnov, O.M., Tasse, C. and Afonso, J.M., 2022. MIGHTEE: total intensity radio continuum imaging and the COSMOS/XMM-LSS Early Science fields. Monthly Notices of the Royal Astronomical Society, 509(2), pp.2150-2168.en_US
dc.identifier.issn00358711
dc.identifier.urihttp://doi.org/10.1093/mnras/stab3021
dc.identifier.urihttp://hdl.handle.net/10566/7301
dc.description.abstractMIGHTEE is a galaxy evolution survey using simultaneous radio continuum, spectropolarimetry, and spectral line observations from the South African MeerKAT telescope. When complete, the survey will image ∼20 deg2 over the COSMOS, E-CDFS, ELAIS-S1, and XMM-Newton Large Scale Structure field (XMM-LSS) extragalactic deep fields with a central frequency of 1284 MHz. These were selected based on the extensive multiwavelength data sets from numerous existing and forthcoming observational campaigns. Here, we describe and validate the data processing strategy for the total intensity continuum aspect of MIGHTEE, using a single deep pointing in COSMOS (1.6 deg2) and a three-pointing mosaic in XMM-LSS (3.5 deg2). The processing includes the correction of direction-dependent effects, and results in thermal noise levels below 2 μJy beam−1 in both fields, limited in the central regions by classical confusion at ∼8 arcsec angular resolution, and meeting the survey specifications. We also produce images at ∼5 arcsec resolution that are ∼3 times shallower. The resulting image products form the basis of the Early Science continuum data release for MIGHTEE. From these images we extract catalogues containing 9896 and 20 274 radio components in COSMOS and XMM-LSS, respectively. We also process a close-packed mosaic of 14 additional pointings in COSMOS and use these in conjunction with the Early Science pointing to investigate methods for primary beam correction of broad-band radio images, an analysis that is of relevance to all full-band MeerKAT continuum observations, and wide-field interferometric imaging in general. A public release of the MIGHTEE Early Science continuum data products accompanies this article.en_US
dc.language.isoenen_US
dc.publisherUniversity of the Western Capeen_US
dc.subjecttechniquesen_US
dc.subjectgalaxy evolutionen_US
dc.subjectgalaxyen_US
dc.subjectcosmologyen_US
dc.subjectradio continuumen_US
dc.subjectEarly Science continuumen_US
dc.subjectinterferometric imagingen_US
dc.titleMIGHTEE: Total intensity radio continuum imaging and the COSMOS/XMM-LSS Early Science fieldsen_US
dc.typeArticleen_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record