Fig. 10
Spectroscopic LF of WINGS cluster members. The single Schechter fit to the SLF is drawn in red, while black lines represent the fit to the photometric LF (continuous line), and the Schechter function obtained using the median values of the whole sample (dotted line). In the inset we compare our SLF with those by Rines & Geller (2008) for Virgo and A2199, and by Agulli et al. (2014) for A85.
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