Fig. 25.
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Expected counts of GC galaxies (with reliable spectroscopic redshifts) in deg−2 (see text) in ecliptic coordinates. Here the number counts decrease faster with latitude than for the WL counts (cf. Fig. 24) since the impact of stars (spectra) from our Galaxy on the GC one-dimensional spectra is more severe than the impact of stars (point-like) on the two-dimensional WL data.
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