Image Details
 
                    Caption: Figure 6.
The Hα-based SFMS as determined from JWST observations in this study in the range 1.4 < z ≤ 2.7 (purple) and MOSDEF observations from R. L. Sanders et al. (2021) in the range 2.0 < z < 2.6 (gray). The MOSDEF data points have been shifted down by 0.32 dex to match the Hα luminosity to SFR conversion that we use in this paper.
© 2024. The Author(s). Published by the American Astronomical Society.