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Fig. 8

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Total (major + minor, μ ≥ 1/10) merger fraction as a function of redshift. Dots are from the present work in the COSMOS field for M   ≥ 1011  M galaxies, diamonds are from Mármol-Queraltó et al. (2012) for massive galaxies, squares are from Newman et al. (2012) for M   ≥ 5 × 1010  M galaxies, crosses are from Jogee et al. (2009) for M   ≥ 2.5 × 1010  M galaxies by morphological criteria, and inverted triangles are from Lotz et al. (2011) for M   ≥ 1010  M galaxies by morphological criteria. The dashed line is the least-squares best fit of a power-law function, fm ∝ (1 + z)0.6, to the total merger fraction data in the present work.

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