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Fig. 9.

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Impact of photometric redshifts of source galaxies on scaling relation parameter estimation. Left: The filled contours show the constraints when using true redshifts of source galaxies. Dashed contours are obtained when considering the BPZ photometric redshifts. Empty contours are obtained using BPZ photometric redshifts, after marginalizing over the (1 + b) correcting factor, considered as a free parameter, used to correct from photometric redshift calibration issues. Right: same as left panel, but for FlexZBoost.

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