The influence of the cosmic web on the properties of dwarf galaxies in the Fornax-Eridanus supercluster

Open Access

Fig. B.1.

Fraction of group dwarfs as a function of projected distance from the Fornax Wall spine for M_*, Sérsic n, ${\bar{μ}}_{e, r}$ $Mathematical equation: $ \bar{\mu}_{e,r} $$ , ellipticity, R_e, r, and g − r colour bins (left). Table with the labels in Column 1 and the corresponding bins in Column 2 (right).

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