Fig. B.3
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Conversion from limiting z-band magnitude to limiting redshift zvlim for galaxies with a luminosity L = 0.2 L* (orange) and L = 0.4 L* (blue). Restricting the sample to brighter members allows for probing higher redshifts. For reference, the green histogram shows the distribution of limiting magnitudes in the z band for the combined full LS DR10 south and LS DR9 north areas.
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