Fig. 6.
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Number of lopsided and symmetric galaxies with one or more massive neighbors (stellar mass-ratio >1:10) within 0.5×R200 during the last 3 Gyr of the galaxy history, normalized by the total number of lopsided and symmetric galaxies, respectively, at the five different specific redshift z = 2, 1.5, 1, 0.5, 0. Here, we only focus on the central galaxies in our sample.
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