Fig. 9


Top: absolute i band magnitude as a function of photometric redshift. In the redshift range 0.35−0.5 a slight decrease can be seen. Bottom: comparison of the number of galaxies in each VTA overdense region with a cut in absolute i-band magnitude (Mi ≤ − 19), and a cut in observed i-band magnitude applied in this paper (mi ≤ 23.5).

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