VISTA NIR light curves for all the RRLs that lacked a derived light curve or period in the literature. For each star, upper panel: J-band curve, whereas the lower one displays the K_S band instead. Our derived period for each star is provided in each panel. Note that the V180 light curve is consistent with a W UMa classification. Variables ID-91 and (especially) ID-99, from Weldrake et al. (2007), have light-curve shapes that are different from all the other RRab in ω Cen, and are suspected to be field stars.