Gaia Data Release 2
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Fig. 48

image

Percentage of Gaia DR2 LPV candidates for which a crossmatch is found with OGLE-III LPVs (solid line) in the reference sky regions towards the SMC (top panel), LMC (middle panel), and Galactic bulge (bottom panel) as a function of crossmatch radius. The percentages of Gaia (OGLE-III) LPV candidates for which a crossmatch is found with AllWISE sources are shown as dashed (dotted) lines in each panel. The reference sky regions are shown in Figs. 45and 46.

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