K-band LF for the galaxies from the magnitude-limited sample MLS_W1 (stars with error bars) with the best-fit Schechter function (solid curve). The background-subtracted and incompleteness-corrected counts are shown as open squares. The LF from the galaxies with known redshift (eSCGS) is shown in red. For comparison, the LF from Kochanek et al. (2001) (dashed-dotted) and the LFs for the Coma cluster from De Propris & Pritchet (1998) and Andreon & Pelló (2000) (dashed and dotted) are overplotted, arbitrarily normalised at M_K = −24.