Free Access
Volume 575, March 2015
Article Number A116
Number of page(s) 24
Section Cosmology (including clusters of galaxies)
Published online 06 March 2015

Online material

Appendix A: Individual cluster GLFs

thumbnail Fig. A.1

GLFs in the B,V,R and I rest-frame bands (from left to right) for individual clusters ordered by right ascension. Red and blue points correspond to red-sequence and blue GLFs normalized to 1 deg2. The red vertical lines indicate the 90% completeness limit. The red and blue curves show the best Schechter fits to red sequence and blue galaxies, and the faint-end slope parameter (α) is displayed in the corresponding colour. Only galaxies brighter than the 90% completeness limit are taken into account in the fits. Also, we only show GLFs richer than 20 galaxies after the colour separation and after subtracting the field.

Open with DEXTER

Table A.1

Parameters of the best Schechter function fit for every cluster normalized to 1 deg2.

© ESO, 2015

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