Fig. A.1.
Same as Fig. 1 but showing the n(z) in the first four tomographic bins for KV450 (this study, red), KiDS-450 (H17, blue), and KiDS-450 calibrated with 9-band photometry (green). This illustrates the better high-z behaviour of the optical and infrared photo-z. We note that the galaxies in the bins are different in the two studies.
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