Fig. 5.
Distribution of Heliocentric distances. Results from Bailer-Jones et al. (2018) for sources in Muraveva et al. (2014), (top panel), and Pawlak et al. (2013), (bottom panel); the respective bin widths of the histograms are 0.38 kpc and 0.23 kpc (see the text for details). The vertical black bars signal the true values from Pietrzyński et al. (2013), (top panel), and Hilditch et al. (2005), (bottom panel). The cumulative relative frequency is plotted as a discontinuous curve.
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