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Fig. 5


SSFRs of interacting galaxies normalized by SSFRs of non-interacting galaxies (i.e. Rn > rvir,nei in Fig. 3) as a function of redshift for a) early-type and b) late-type neighbor case. Filled and open circles are median values for strongly (i.e. Rn ≤ 0.1rvir,nei), and weakly interacting (i.e. Rn ≤ 0.5rvir,nei) galaxies, respectively, at each redshift bin (0.005 ≤ z ≤ 0.0656, 0.4 ≤ z ≤ 0.8, and 0.8 ≤ z ≤ 1.2).

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