EDP Sciences
Free Access
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.

thumbnail 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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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.

thumbnail 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).

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© ESO, 2015

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