| Issue |
A&A
Volume 578, June 2015
|
|
|---|---|---|
| Article Number | A79 | |
| Number of page(s) | 14 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361/201425293 | |
| Published online | 10 June 2015 | |
Online material
Appendix A: Magnitude histograms
The magnitude histograms in the five bands of the 4 999 968 galaxies of the initial magnitude catalogue used to compute absolute magnitudes are shown in Fig. A.1.
 |
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: |
| Open with DEXTER | |
Appendix B: Completeness simulations
We show in Fig. B.1 the percentages of redetected galaxies as a function of absolute magnitude in the i′ band derived from our simulations in five magnitude bins: z = 0.2 in black, z = 0.3 in blue, z = 0.4 in green, z = 0.5 in red, and z = 0.6 in magenta (see Sect. 5.2.1). Simulations in the other bands give comparable curves and are not shown here to save space.
 |
Fig. B.1
Percentage of redetected galaxies as a function of absolute magnitude in the i′ band derived from our simulations in five magnitude bins: z = 0.2 in black, z = 0.3 in blue, z = 0.4 in green, z = 0.5 in red, and z = 0.6 in magenta (see Sect. 5.2.1). |
| Open with DEXTER | |
© ESO, 2015
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