Fig. 8
Comparison of our distance estimates against the RAVE DR4 distances from Binney et al. (2014a) for the high-S/N sample of Boeche et al. (2013a). In each panel the vertical axis shows the absolute distance residuals normalised to the combined uncertainty from both methods, 
, as a function of the main spectroscopic parameters Teff, [Z/H] and log g as well as the RAVE distance, dRAVE.
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