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Fig. 2.
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AGN fraction as a function of stellar mass for galaxies in each defined environment. Galaxies in under-dense environments are more likely to host an AGN than those in denser environments, particularly for M∗ ∼ 1010.5 M⊙, at z = 0. Errors show the 16th and 84th percentiles from the bootstrap distribution of 1000 samples.
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