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Fig. 13

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Comparison of the parameters obtained by fitting Schechter functions to the FUV (left) and NUV (right) luminosity functions of the Virgo cluster down to magnitude limits of M ≤  − 10 (black filled circles and solid contours) and of M ≤  − 13 (black empty circles and dotted contour or error bars) with their uncertainty, of the Coma cluster (red empty square; from Cortese et al. 2008b), of A1367 (green filled triangle; from Cortese et al. 2005), of the Shapley supercluster (yellow filled square; from Haines et al. 2010) and of the field (blue asterisk; from Wyder et al. 2005).

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