  We aim to carry out a radio study of the SoUthern Cluster sCale Extended
Source Survey (SUCCESS) sample consisting of twenty massive (M$_{500} >
5\times10^{14}$ M$_{\odot}$), nearby (redshift $<0.3$) and southern
($-50^{\circ} < \delta < -30^\circ$) galaxy clusters detected by the Planck
satellite and the South Pole Telescope. Here we report targeted GMRT
observations (325/610 MHz) for a sub-sample of nine clusters. We also use the
first data release of MeerKAT Galaxy Cluster Legacy Survey (1283 MHz) for five
of these nine clusters. The properties of the mini-halo in RXC J0528.9-3927, a
candidate mini-halo in A3322, the radio halo and candidate double relics in
A3399, and the radio halo in RXC J0232.2-4420 are presented. We also report
detection of candidate radio relics at distances 1 and 1.9 Mpc from the center
of RXC J0232.2-4420. The southeast relic of A3399 is consistent with the radio
power - mass scaling relation for radio relics, while the candidate relics
around RXC J0232.2-4420 are outliers. This indicates an origin of the candidate
relics near RXC J0232.2-4420 to be independent of this cluster and a cluster
merger-shock origin for the relic in A3399. In this sub-sample of clusters 1/9
hosts a radio halo and double relics, 1/9 hosts a radio halo and 2/9 host
mini-halos. The dynamical states based on X-ray morphology show that A3399 is a
disturbed cluster; however, the radio halo cluster RXC J0232.2-4420 is relaxed,
and the mini-halo clusters have intermediate morphologies, adding to the cases
of the less commonly found associations.

Cosmology and Nongalactic Astrophysics;Astrophysics of Galaxies