Fig. 10.
Number counts of background galaxies per K magnitude interval of the width 0.5 mag. Filled squares with vertical error bars: spectroscopically established background galaxies, the horizontal bars indicate the bin widths. Open squares: Total number of expected background galaxies. Diagonal lines: galaxy number counts N(K) from 2MASS (Frith et al. 2003, solid) and GAMA (Whitbourn & Shanks 2014, dashed).
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