  Radio continuum observations offer a new window on compact objects in
globular clusters compared to typical X-ray or optical studies. As part of the
MAVERIC survey, we have used the Australia Telescope Compact Array to carry out
a deep (median central noise level of approximately 4 microJy per beam) radio
continuum survey of 26 southern globular clusters at central frequencies of 5.5
and 9.0 GHz. This paper presents a catalogue of 1285 radio continuum sources in
the fields of these 26 clusters. Considering the surface density of background
sources, we find significant evidence for a population of radio sources in
seven of the 26 clusters, and also identify at least 11 previously known
compact objects (6 pulsars and 5 X-ray binaries). While the overall density of
radio continuum sources with 7.25-GHz flux densities greater than about 20
microJy in typical globular clusters is relatively low, the survey has already
led to the discovery of several exciting compact binaries, including a
candidate ultracompact black hole X-ray binary in 47 Tuc. Many of the
unclassified radio sources near the centres of the clusters are likely to be
true cluster sources, and multi-wavelength follow-up will be necessary to
classify these objects and better understand the demographics of accreting
compact binaries in globular clusters.
