Astronomy & Astrophysics

Table 1: The sample. For each band the number of dE-E galaxies in the WFS (separately for the Horizontal and Vertical strips) with $m_{\rm p}\leq 19$ mag. that are members or possible members, to which we have been able to fit a Sersic profile is given. The denominator gives the number of galaxies in the VCC at the same magnitude limit.
Table 2: B-band parameters of the observed galaxies.