Fig. 2.
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Stellar mass, SFR, and Re of our galaxies (in red) and all low-redshift MUSE-Wide emission line galaxies (in gray). All values are matched from the 3D-HST GOODS-S photometric catalogs. The dashed black line represents the highest redshift at which the Hα and [N II] emission line can be observed (z ∼ 0.42). This is limited by the wavelength range of MUSE.
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