Fig. 1.
Comparison between A(V)β and A(V)SED. Galaxies from MUSE UDF with CONFID = 3 and z = 2.2 − 4.7 with continuum S/N ≳ 3 are shown here and are colour-coded by their mass. The one-to-one line is shown as a black dashed line. The solid black line shows the linear regression model fit to the data along with its 1σ uncertainty (computed using 1000 bootstrap resamples) shaded in grey.
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