Fig. 7.
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KS diagram as a function of galaxy merger stage based on clump identification. From left to right and top to bottom, the merger stages are isolated galaxies (blue), galaxy pairs (red), early-stage mergers (orange), mid-stage mergers (magenta), and late-stage mergers (black). The black solid line represents the best fit for each dataset. The Spearman’s rank correlation coefficients (ρs) and the power-law indices (N) of the derived best-fit KS relations is at the top left of each panel. The grey dashed lines mark constant star formation efficiencies (SFE = ΣSFR/ΣH2).
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