EDP Sciences
Free Access
Issue
A&A
Volume 581, September 2015
Article Number A11
Number of page(s) 49
Section Cosmology (including clusters of galaxies)
DOI https://doi.org/10.1051/0004-6361/201526080
Published online 25 August 2015

Online material

Table 1

Schechter function parameters.

thumbnail Fig. A.1

LF for the cluster A85: the black continuous line is the original LF, the dashed line is the same LF corrected for completeness. The vertical line shows the magnitude limit (different for each cluster) at which the completeness is 90%. In red and green we show the LF of the two subsamples of galaxies and galaxies and unknown object, respectively. These two last distributions have been corrected for field contamination (whose number counts are shown in the inset). Superimposed on the red LF is the best fit that we obtained using a single Schechter function (left panel) and a double Schechter function (right panel). In the bottom right insets we give the relative parameters.

Open with DEXTER


© ESO, 2015

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