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Fig. 3.


Fraction of optical nuclear activity with respect to the QLSS environmental parameter according to their morphology. Low-mass galaxies (10.0  ≤  log(M)  <   10.6 M) are represented by cyan circles, and high-mass galaxies (10.6  ≤  log(M)  ≤  11.4 M) are represented by orange squares. The fraction of SFN, AGN, and passive late-type SIG galaxies (NT = 462, 586, and 170, respectively) is represented from top to bottom in the left panels, and for early-type SIG galaxies (NT = 44, 362, and 306, respectively) in the right panels. The number of galaxies in each QLSS bin is shown in tables for each sample at the bottom of each panel. Error bars are given considering binomial distribution.

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