Fig. 22.
Observational HRDs of Gaia DR2 sources that have relative parallax uncertainties better than 10%. Top panel: density map of LAV candidates from Dataset C, while bottom panel: random selection of variable+constant sources with good BP and RP flux excess. The black contour lines in both panels correspond to the density lines of the sample shown in the bottom panel. No correction for interstellar reddening and extinction is applied.
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