Fig. 2.
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Top: Distribution of the M★ in function of redshift of the final sample from the regulator MIRI run. Bottom: Distributions of differences in the main physical properties (SFR in M⊙/yr and the M★ in M⊙, AV in mag, age in Myr) between the MIRI and no-MIRI runs. The hatched region shows the 90th percentiles of the distributions (P90) in both directions.
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