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Fig. 8.

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Fraction of galaxies considered to be expert classified RPS candidates in each of the three samples defined in Sect. 4.1. The fraction of expert classified RPS is shown with a circle, while the fraction of new strong candidates, with J class ¯ 3 $ \overline{J_{\mathrm{class}}} \ge 3 $, is shown with a triangle. Binomial one-sigma confidence intervals are also shown. We see that known ram pressure stripped candidates have the highest fraction. Additionally, the GZ motivated sample contains a higher fraction than the control sample.

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