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Fig. 3


Left: joint probability density for the Gaia sources, derived using the LF evolution model described in the text. Right: DNCF as a function of the G-band magnitude. We use a combined observational sample of the SDSS-DR3 and 2QZ/6QZ for magnitudes brighter (fainter) than i ~ 19, converted to G-band magnitudes and thus assuming the DNCF shape in G-band to be similar. We also show the fit used to estimate the DNCF.

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