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Fig. 18


Comparison of the DL07-based Mgas estimate obtained, including artificial ALMA band 6 photometry to expectations, based on the Scoville et al. (2015) recipe, and applied to the same artificial ALMA band 6 data. Color coding is based on the number of available photometric bands (see Fig. 17). Left: direct comparison: error bars only include statistic noise. Right: ratio of the two estimates as a function of redshift and DL07-based gas mass.

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