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Fig. A.4.

Fig. A.4. Refer to the following caption and surrounding text.

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No PD: Comparison of luminosities estimated from 1) our photometric method (presented on X-axis) and 2) CIGALE estimates without and with contaminations for 4 redshift bins. The dashed lines is the 1:1 relation, while the solid black line is the best-fit regression. In the fourth row the outliers were also accounted for, defined as objects below 1σ error (green lines), marked with stars. Then the outliers were extracted and another regression was fit (dashed gray line).

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