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Fig. 15


Correlations between the broadband magnitudes and the [Oii] flux. The contours represent the density of galaxies predicted by the weighted data (from dark blue to brown 10, 50, 100, 200, 500 galaxy deg-2). The g band correlates best in the redshift range 0.7 <z< 1.1. The r magnitude correlates best in the range 1.3 <z< 1.6. The fluxes corresponding to a luminosity of 1041 and 1042 erg s-1 and the mean redshift (0.9 and 1.3) are represented by dashed blue lines.

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