Fig. C.1.
PCA components derived from VIPERS spectra by Marchetti et al. (2013) for the 11 FEM classes. VIPERS PDR1 galaxies are marked with grey dots. The distribution of 2688, 1428, 2185, 2674, 2201, 598, 3300, 1096, 3630, 7885, 1395 eigen coefficients for the 11 FEM classes are colour-coded according to their redshift values. The location of the Kinney–Calzetti spectra (Calzetti et al. 1994; Kinney et al. 1996) for different galaxy families are marked with white stars following Marchetti et al. (2013).
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