Notes. Summary of the verifications made of the whole optimistic sample to determine whether a target is a reliable anti-solar DR candidate. The halo flag indicates whether the target is in the light halo of a brighter star from the visual inspection of 2MASS images (1) or not (0). The neighboring flag indicates whether a neighbor is at least visible in the Kepler acquisition FoV (1, 2, and 3) or not (0). If this is the case, we determined whether the main target light curve might be (2) or is clearly (3) polluting the target star, or if we acknowledge no pollution of the rotational signal (1). The shape flag indicates whether the shape of the target in the FoV is deformed or elongated, suggesting multiple stars (1) (possibly a close companion in the FOV), or not (0). The log₁₀g flag indicates whether an uncertainty in the log₁₀g value is suspiciously large and might cause us to consider a subgiant target. When we concluded during the inspection that the P_rot value extracted by S19-21 clearly derived from the rotational signal of the target (0) or not (1). If the light curve showed a rotational signal and we were able to improve the measurement and provide a new reliable P_rot, we provide flags 2 and 3. In this case, we indicate whether the new corresponding Ro_f/Ro_f, ⊙ value is high enough to keep the target above the selection threshold and in the optimistic sample (3) (i.e., if the new lower limit of this value is higher than 1.3/0.9 = 1.44) or not (2). We finally indicate with the candidate flag whether we consider the target as an anti-solar DR candidate (1) or not (0). The full table is available at the CDS.