activity
20002023
most citedCalibrating Extinction-Free Star Formation Rate Diagnostics with 33GHz Free-Free Emission in NGC6946

859 citations · 6.6k across the 70 of their papers we have counts for

collaborators

70 papers

astro-ph.GA2023★ 21 cited

MeerKAT view of the Dancing Ghosts -- Peculiar Galaxy Pair PKS 2130-538 in Abell 3785

Velibor Velović, William D. Cotton, Miroslav D. Filipovi'c +3

We present MeerKAT L-band (886-1682 MHz) observations of the extended radio structure of the peculiar galaxy pair PKS 2130-538 known as the "Dancing Ghosts". The complex of bending…

astro-ph.GA2023★ 20 cited

The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field

Minhee Hyun, Myungshin Im, Ian R. Smail +14

The James Webb Space Telescope Time-Domain Field (JWST-TDF) is an 14 diameter field near the North Ecliptic Pole that will be targeted by one of the JWST Guaranteed Time O…

astro-ph.HE2022★ 3 cited

The Curious Case of the "Heartworm" Nebula

W. D. Cotton, F. Camilo, W. Becker +9

The curious Galactic features near G357.20.2 were observed with the MeerKAT radio interferometer array in the UHF and L bands (0.56--1.68 GHz). There are two possibly related fe…

astro-ph.GA2021

A MeerKAT 1.28 GHz Atlas of Southern Sources in the IRAS Revised Bright Galaxy Sample

J. J. Condon, W. D. Cotton, T. Jarrett +4

The IRAS Revised Bright Galaxy Sample (RBGS) comprises galaxies and unresolved mergers stronger than Jy at with galactic latitudes $\vert b \vert > 5…

astro-ph.GA2021★ 44 cited

Threads, Ribbons, and Rings in the Radio Galaxy IC 4296

J. J. Condon, W. D. Cotton, S. V. White +5

The nearby elliptical galaxy IC4296 has produced a large (510 kpc) low-luminosity radio source with typical FR I core/jet/lobe morphology. The unprecedented combination of brightne…

astro-ph.GA2021★ 24 cited

Outflows, Shocks and Coronal Line Emission in a Radio-Selected AGN in a Dwarf Galaxy

M. Molina, A. E. Reines, J. E. Greene +2

Massive black holes (BHs) in dwarf galaxies can provide strong constraints on BH seeds, however reliably detecting them is notoriously difficult. High resolution radio observations…