Scheme adopted to classify the sub-types of BSs and RINs is based on the analysis of star formation status at key moments: SF or PS. For BSs, three stages are selected: the moment of entry into the R₂₀₀ region of the group, the moment of exit from that region and at z = 0. For RINs, two moments are highlighted: the entry into the R₂₀₀ region of the group and z = 0. The vertical lines delineate the transitions between these stages. The identified sub-types are: always star-forming (aS), quenched in post-splashback stage (qB, only for BSs), quenched during the diving stage (qD), and always passive (aP). Among the green BSs, 44.7% are aS, 39.9% are qB, 15.4% are qD, and none are aP. Among the green RINs, 35.6% are aS, 42.4% are qD, and 22.0% are aP.