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Fig. 5

image

a) Central galaxy stellar mass as a function of group mass in different large-scale environments defined by the luminosity density field. The error limits are estimated using the bootstrap re-sampling technique. b) Central galaxy stellar mass as a function of group mass for groups in and outside of filaments having luminosity densities, Den8 < 1.5. c) Central galaxy stellar mass as a function of group mass for groups in and outside of filaments having luminosity densities, 1.5 < Den8 < 5. d) Central galaxy stellar mass as a function of group mass for groups in and outside of filaments having luminosity densities, Den8 > 5.

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