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Fig. 8

image

Fraction of galaxies hosting an AGN as a function of stellar mass for different galaxy populations at 0.5 < z < 1.5 (the bottom panels) and 1.5 ≤ z < 2.5 (top panels). We divide the sample into two stellar-mass bins separated at 1010.6 M. The data points for each population are plotted at the median of each mass bin.

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