Fig. 12.


Colour-absolute magnitude diagram for S1+S2-selected objects (open orange circles), S1+S2+S3-selected objects (full orange circle), and the Gaia Hyades CaMD from Gaia Collaboration (2018b) as open grey circles. For the selection criteria S1, S2, and S3, see Sect. 3.1. The PARSEC isochrone is plotted as a black line. The missing binary sequence in our selected points is most likely due to the RUWE filtering, which partially filters out unresolved binary stars. Mean error bars computed in MG bins computed based on Gaia photometric fluxes (see Gaia DR2 primer, issue 1.5) are shown in red at the right.

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