A MeerKAT survey of nearby dwarf novae: I. New detections
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2025) staf556
The jet paths of radio active galactic nuclei and their cluster weather
Astronomy & Astrophysics EDP Sciences 695 (2025) a178
Supernova remnants on the outskirts of the Large Magellanic Cloud
Astronomy & Astrophysics EDP Sciences 693 (2025) l15
MIGHTEE: the continuum survey Data Release 1
Monthly Notices of the Royal Astronomical Society Oxford University Press 536:3 (2024) 2187-2211
Abstract:
The MeerKAT International GHz Tiered Extragalactic Exploration Survey (MIGHTEE) is one of the large survey projects using the MeerKAT telescope, covering four fields that have a wealth of ancillary data available. We present Data Release 1 of the MIGHTEE continuum survey, releasing total intensity images and catalogues over ∼20 deg2, across three fields at ∼1.2-1.3 GHz. This includes 4.2 deg2 over the Cosmic Evolution Survey (COSMOS) field, 14.4 deg2 over the XMM Large-Scale Structure (XMM-LSS) field and deeper imaging over 1.5 deg2 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 deg2) and, using the areal coverage of MIGHTEE we measure the sample variance for differing areas of sky. We find a typical sample variance of 10-20percnt for 0.3 and 0.5 sq. deg. sub-regions at S1.4 ≤ 200 μJy, which increases at brighter flux densities, given the lower source density and expected higher galaxy bias for these sources.MeerKAT observations of Herschel protocluster candidates
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 535:1 (2024) 370-391