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Fig. 13


Major merger rate RMM as a function of redshift for MB ≤ − 20 − 1.1z galaxies. The stars are from the ALHAMBRA photometric survey, the circles from the VVDS-Deep spectroscopic survey, and the inverted triangle from the MGC spectroscopic survey. The dashed line is the best fit of a power-law to the data. The power-law index of the best fit is labelled in the panel. The grey area marks the 68% confidence interval of the fit.

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