Fig. 25
Comparison of the distances obtained using asteroseismology and the direct method adopted in (Miglio et al. 2013), with the distances provided in RAVE (DR4, DR5 and DR5-SC) and the distances determined using PARAM (blue points). Typical errors of each method are shown in the top-left of the figure (both DR5 and DR5-SC have the same typical error).
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