Notes. The standard M_std and instrumental m_ins magnitudes listed in Cols. 5 and 6 respectively correspond to the cluster, variable star, filter and epoch of mid-exposure listed in Cols. 1–4, respectively. The uncertainty on m_ins is listed in Col. 7, which also corresponds to the uncertainty on M_std. For completeness, we also list the reference flux f_ref and the differential flux f_diff (Cols. 8 and 10 respectively), along with their uncertainties (Cols. 9 and 11), as well as the photometric scale factor p. Instrumental magnitudes are related to the other quantities via m_ins = 17.5 − 2.5·log ₁₀(f_ref + f_diff/p). This is a representative extract from the full table, which is available at the CDS.