Fig. A.2.
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Same as Figure 7, but with SFR inferred from the (attenuation corrected) Hα flux (or Hβ, at z ≳ 7). The calibration for low metallicity galaxies described in Reddy et al. 2022; Shapley et al. 2023b is adopted for the entire JWST sample in the left-hand panel, while in the right-hand panel the SFR is derived following the calibration from Kennicutt & Evans 2012 for solar metallicity.
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