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Fig. B.1.


Fraction of optical nuclear activity with respect to the QLSS environmental parameter according to their sSFR status. Low-mass galaxies (10.0  ≤  log(M)  <   10.5 M) are represented by cyan circles, and high-mass galaxies (10.5  ≤  log(M)  ≤  11.4 M) are represented by orange squares. The fraction of SFN, optical AGN, and passive star forming SIG galaxies (NT = 577, 541, and 91, respectively) is represented from top to bottom in the left panels, and for quenched SIG galaxies (NT = 8, 611, and 468, 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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