Fig. D.1.

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Comparison between stellar masses of the REQUIEM-ALMA sample reported in previous works (Newman et al. 2018; Man et al. 2021) and computed here from HST+Spitzer SEDs with metallicity priors. The masses from the literature were converted to a Salpeter (1955) IMF and both have been de-magnified; however, the error bars shown here do not account for magnification uncertainties. The dashed line shows the one-to-one relation.
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