Fig. 1
Both plots: Relative frequencies of galaxies in the (Mr, mst)-plane are shown.The brighter the colour, the higher the frequency within a given pixel. The left plot is shown with all galaxies, whereas the right plot only shows galaxies with a neighbouring galaxy at a distance of r ∈ [1, 3] Mpc. The normalisation of the logarithmic quantities Mr and mst is given in Appendix A.1.
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