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Fig. 6.

image

Merger history in different accretion classes. Left: median accretion history parameters as a function of the stellar mass. Right: median mass fractions from different mass ratio mergers and from stripped galaxies as a function of the stellar mass. Shaded regions or error bars show the 25th to 75th percentiles of the distributions. In the bottom left panel (number of major mergers since z = 1) we show mean profiles and standard deviations around the mean. Galaxies are divided into the accretion classes as shown in the legend. The accretion classes defined in Sect. 4.1 are the results of different merger histories.

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