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Fig. 4

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Distances to open clusters (dCLUSTER) from Dias et al. (2002, 2007) compared to spectroscopic distances d of cluster members observed by RAVE from B10 a), and to values derived here using the YY b), Dartmouth c), and Padova d) isochrones. Circles denote dwarfs (log gRAVE > 3.8) and triangles likely giants (log gRAVE ≤ 3.8). Open symbols mark the likely members of M 67. The line marks the 1:1 relation. The pairs of distances in the shaded area are equal to within 20%.

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