Gaia DR2 colour-magnitude diagram for all stars for which we constructed light curves. The best-defined members (satisfying all four criteria) are marked in orange, members according to three criteria are marked in green, and those fulfilling only two in blue. Non-members are marked in black. We note that photometric binaries are retained. The arrow indicates the colour of the Sun (Casagrande & VandenBerg 2018) for context. The spectral classifications at the top are according to Pecaut & Mamajek (2013). In the upper right we display representative uncertainties for stars on the cluster sequence. Uncertainties for (G_BP − G_RP)₀ <  2.3 and for G are within the symbol size and are not shown here.