Galaxy Zoo 2 vote fractions for the known RPS sample and two comparison samples. (a) Debiased fraction of votes that consider a galaxy to have features or a disk. Compared to the cluster and field comparison samples, the known RPS candidates have a much higher proportion of disk galaxies, in line with expectations. (b) Debiased fraction of votes for a galaxy to be considered odd. Compared to the group comparison sample, the known RPS candidates have a much higher proportion of odd candidates. (c) Debiased fraction of votes for galaxies to have irregular, disturbed, or other features, for galaxies with p_odd > 50%. (d) Debiased fraction of votes for galaxies to have merger features, for galaxies with p_odd > 50%. Compared to either the group or field comparison samples, the ram pressure stripped galaxies are considered to be disturbed or irregular, and are not considered to be mergers. All counts are normalised such that the area under each curve is equal to one.