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Fig. 12

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Individual parallaxes of Hyades members derived in this work compared to the secular parallaxes of de Bruijne et al. (2001) derived using proper motion data from the Hipparcos (left panel) and tycho2 (right panel) catalogs. The red line represents the expected distribution for equal results. The rms with respect to the Hipparcos secular parallaxes is 1.55 mas and 1.68 mas for tycho2 secular parallaxes, and the mean difference between the parallaxes is 0.23 mas and –0.27 mas.

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