P_rot distributions for metal poor (left), solar metallicity (middle), and metal rich (right) stars within 100 K to the T_eff of the Sun (top) and Doris (bottom). Dark red shows the distribution for all stars, while light red corresponds to those with spectroscopic parameters. We only consider main-sequence stars. The shaded regions in blue and turquoise mark the P_rot interval used to select Sun-like and Doris-like stars. The white circles indicate the median values, while the black bars indicate the 1st and 3rd quartiles of the distributions.