| Issue |
A&A
Volume 575, March 2015
|
|
|---|---|---|
| Article Number | A116 | |
| Number of page(s) | 24 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361/201423796 | |
| Published online | 06 March 2015 | |
Online material
Appendix A: Individual cluster GLFs
 |
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 | |
 |
Fig. A.1
continued. |
| Open with DEXTER | |
 |
Fig. A.1
continued. |
| Open with DEXTER | |
Parameters of the best Schechter function fit for every cluster normalized to 1 deg2.
© ESO, 2015
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