Near-IR period-luminosity relations for pulsating stars in ω Centauri (NGC?5139) (Corrigendum)

摘要

An incorrect zero point for the empirical period-luminosity-metallicity (PL-Z) relations for RR Lyrae (RRL) stars in ω Cen-tauri (NGC5139) was inadvertently reported in Table 2 andEqs. (4) and (5) of our original paper. The corrected table andequations are given below. The actual analysis that is describedinthepaperwasbasedonthecorrectzeropoints,andsoalloftheresults reported in our original publication remain unchanged.