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Fig. 3.


Specific star formation rate (sSFR) as a function of the stellar mass for isolated E galaxies. The black line shows Eq. (16) to separate SF and quenched galaxies. The open black stars and open black triangles show the blue SF isolated ellipticals from the SIG and L16 samples, respectively. The color bars correspond to the QLSS parameter (top panel), ηk,LSS parameter (middle panel), and the distance to the fifth nearest neighbor galaxy out to 5 Mpc (bottom panel). The total number of galaxies is indicated in each panel.

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