Fig. 6.
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Size-mass relations for our pz sample (black), based on photometric redshifts, and a sample of dwarf galaxies with spectroscopy from the DESI Y1 data release (blue). The error bars show the dispersion (σ) of the maximum likelihood fits to the size distribution at a given mass. The purple contours show the full distribution of the DESI Y1 galaxies.
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