We present the results of MeerKAT radio observations of eleven nearby novalike cataclysmic variables .
We have detected radio emission from IM Eri , RW Sex , V3885 Sgr and V603 Aql .
While RW Sex , V3885 Sgr and V603 Aql had been previously detected , this is the first reported radio detection of IM Eri .
Our observations have doubled the sample of non-magnetic CVs with sensitive radio data .
We observe that at our radio detection limits , a specific optical luminosity \gtrsim 2.2 \times 10 ^ { 18 } erg s ^ { -1 } Hz ^ { -1 } ( corresponding to M _ { V } \lesssim 6.0 ) is required to produce a radio detection .
We also observe that the X-ray and radio luminosities of our detected NLs are on an extension of the L _ { X } \propto L _ { R } ^ { \sim 0.7 } power law originally proposed for non-pulsating neutron star low-mass X-ray binaries .
We find no other correlations between the radio emission and emission in other wavebands or any other system parameters for the existing sample of radio-detected non-magnetic CVs .
We measure in-band ( 0.9–1.7 GHz ) radio spectral indices that are consistent with reports from earlier work .
Finally , we constructed broad spectral energy distributions for our sample from published multi-wavelength data , and use them to place constraints on the mass transfer rates of these systems .