Fig. 12.
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Merger fractions as a function of environment. Top left: Our entire sample. Top right: Merger fractions in two redshift bins: 1.3 < z < 1.6 (dark blue circles) and 1.6 < z < 2.8 (light blue circles). Bottom: Merger fractions as a function of galaxy stellar mass. The grey region shows the ±1 σ range of the CANDELS merger fraction. The merger fraction in our cluster sample is significantly higher than in CANDELS and shows a moderate correlation with environment and mass.
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