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Fig. 1.

image

Upper panel: redshift distribution of the total sample of galaxy pairs. Lower panel: median projected distances, Me(rp), and median radial velocity difference, MeV), for the different galaxy pair classes. Error bars corresponds to the standard deviations of rp and ΔV distributions obtained for each class. Noninteracting pairs tend to have larger rp distances than interacting pairs. On the other hand, rp distributions for red and blue pairs, as well as higher- and lower-luminosity pairs, are all in agreement with the total sample rp distribution.

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