Fig. 11.

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Fraction of stripped mass (left), SFR ratio (centre), and minimum pericentric distance normalised to the virial radius (right) for the green BS galaxy sub-types (upper panels) are shown for the period from their entry into the R200 region until they exit. Similarly, for the green RINs sub-types (lower panels), the analysis covers the period from their entry into the R200 region until z = 0. Circles represent the median values, while bars indicate the standard deviation, calculated using the bootstrap method for each sub-type. The dashed grey horizontal lines denote the median values of the green galaxies of the corresponding properties.
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