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Fig. 6

image

Comparison of our distances and host cluster distances dcluster for a subsample of clusters with SEGUE observations. For each cluster the median distance and 68% quantiles (as error bars) are shown assuming the following different scenarios: open diamonds uncalibrated SSPP DR9 parameters with field priors; black pentagons: a log g shift of 0.25 dex and field priors; and red circles: a shifted log g and a simple cluster age prior. For visibility the different symbols are slightly offset with respect to dcluster. The lower panel shows the distance residuals, similar to the right column of panels in Fig. 5.

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