Fig. 10

Left columns present, for three different bins in the error of parallaxes and for all our program red clump stars, a comparison between the distance modulus obtained with the photometric parallaxes from Keenan & Barnbaum (2000) calibrations and distance modulus obtained with the revised Hipparcos parallaxes of van Leeuwen (2008). The lines represent the 1:1 correspondence. Each different spectral type is represented with a different symbol. The right columns give the corresponding distribution in VT magnitudes.
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