Fig. 47
Percentage of Gaia DR2 LPV candidates for which a crossmatch is found in the OGLE-III catalogue as a function of the 5–95% quantile range QR5 of G light curves towards the SMC (dotted histogram with downward-pointing triangles), the LMC (dashed histogram with upward-pointing triangles), and the Galactic bulge (solid histogram with filled circles). The percentages are computed in the sample sky areas shown in Figs. 45 and 46 using a crossmatch search radius of 1 arcsec.
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