Fig. 4
Major merger fraction, fMM, versus 
. Dots are for z = 0.8 galaxies, and squares for z = 0.5 galaxies. The lines are the least-squares best fit of a power-law function, 
, to the data. In both cases the power-law index is q = 0.95. The points are shifted to avoid overlap. (A colour version of this plot is available in electronic form.)
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