468 citations · 4.4k across the 117 of their papers we have counts for
117 papers
An e-MERLIN & EVN radio counterpart to the ultraluminous X-ray source M82 X-1
D. Williams-Baldwin, T. W. B. Muxlow, G. Lucatelli +1
Ultra-luminous X-ray sources (ULXs) are X-ray bright (L310erg s) extra-galactic objects that are powered by either neutron stars, or stellar o…
New insights on supernova remnants and HII regions in M82
D. Williams-Baldwin, G. Lucatelli, T. W. B. Muxlow +7
The nearby (d=3.6 Mpc) starburst galaxy M82 has been studied for several decades by very long baseline interferometry (VLBI) networks such as e-MERLIN and the European VLBI Network…
The radio properties of the JWST-discovered AGN
G. Mazzolari, R. Gilli, R. Maiolino +23
We explore the radio emission of JWST-selected Broad Line AGN (BLAGN, or type 1) in the GOODS-N field. We use deep radio data at different frequencies (144\,MHz, 1.5\,GHz, 3\,GHz,…
The VLBA CANDELS GOODS-North Survey. II -- Wide-field source catalogue comparison between the VLBA, EVN, e-MERLIN and VLA
Ann Njeri, Roger. P. Deane, J. F. Radcliffe +5
Deep radio surveys of extragalactic legacy fields trace a large range of spatial and brightness temperature sensitivity scales, and therefore have differing biases to radio-emittin…
Radio jets in NGC 1068 with e-MERLIN and VLA: structure and morphology
Isaac M. Mutie, David Williams-Baldwin, Robert J. Beswick +7
We present new high-sensitivity e-MERLIN and VLA radio images of the prototypical Seyfert 2 galaxy NGC 1068 at 5, 10 and 21 GHz. We image the radio jet, from the compact components…
Revisiting a flux recovery systematic error arising from common deconvolution methods used in aperture-synthesis imaging
Jack F. Radcliffe, R. J. Beswick, A. P. Thomson +2
The point-spread function (PSF) is a fundamental property of any astronomical instrument. In interferometers, differing array configurations combined with their coverage, and…