Rest-frame B-band luminosity function VIPERS from z = 0.5 to z = 1.3. The LF is shown for the total sample (black circles), for red galaxies defined using the colour-bimodality (red triangles, solid line), and for red galaxies selected using the SED criterion (red squares, dashed line). Lines indicate the fits to the luminosity function using a Schechter function. For reference, the black dotted line shows the Schechter function of a local sample by (Ilbert et al. 2005).