We report new radio observations of a sample of thirty-six neutron star (NS) X-ray binaries, more than doubling the sample in the literature observed at current-day sensitivities. These sources include thirteen weakly-magnetised (B<10^{10} G) and twenty-three strongly-magnetised (B\geq10^{10} G) NSs. Sixteen of the latter category reside in high-mass X-ray binaries,... Show more