Fig. 4.
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Star formation main sequence (SFMS) in the JWST ALT survey (Naidu et al. 2024; Di Cesare et al. 2026) with SFRs calculated using the T19 calibration (gray) and the new SFR(Hα) calibrations given in Eq. (2) (cyan) and Eq. (3) (magenta). The diamonds show the running median, with the error bars indicating the standard error on the median. The shaded regions indicate the 68% (1σ) confidence interval. The dashed lines show the linear regression fits to the SFMS individually for each calibration.
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