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Fig. A.1


Magnitude histograms in the five bands of the 4 999 968 galaxies of the initial magnitude catalogue used to compute absolute magnitudes. The full vertical lines show the 90% completeness limits beyond which the galaxy counts will not be considered as fitting the GLFs. These limits are: , , , , and . The dotted vertical lines show the 90% completeness limits derived from Fig. 8 in Annis et al. (2014) for comparison.

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