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Fig. 7


Luminosity functions for the whole galaxy population of D3-6 (top) and D3-43-S3 (bottom) per bin of 0.5 mag normalised to 1 deg2. The vertical lines show the limits in absolute magnitude computed from the i′ = 2490% completeness limit, applying the distance modulus and the mean K-correction in the D3-6 and D3-43-S3 fields.

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