Notes. Among the 4465 stars under study in this paper, this table excludes the 30 stars with no oscillations, and another 18 stars with inconsistent M and R. Numbers are provided for the whole sample (4417 stars) and for specific mass ranges. We included the [0.5, 1.1] M_⊙ range to compare with results from Tayar et al. (2015) and Ceillier et al. (2017). The “known status” column indicates the number and fraction of RGs whose evolutionary status could be determined. The RGB and RC columns report the number and fractions of these types of RGs for each mass range, and the “l = 1 depleted” column indicate the number and fraction of RGs with depleted dipolar modes, according to the Mosser et al. (2017) criterion. The terms “active” and “inactive” refer to RGs with or without detected rotational modulation. The label “frac” indicates the fraction of active RGBs and RCs among all RGBs and RCs of the considered mass range. These fractions take into account the fraction of known evolutionary status. Most of the content of this table (not the l = 1 depleted RGs) can be visualized in Fig. 10.