Star formation rate as a function of stellar mass for our samples of HAEs from BOSS1244 and BOSS1542 overplotted on the coeval sample of field galaxies with SFRs and stellar masses from Osborne & Salim (2024) in the CANDELS fields. The color of the coeval field sample galaxy represents the likelihood that a given galaxy is at z = 2.246 ± 0.02 based on the photometric redshifts from Kodra et al. (2023). We overplotted an estimate of the star formation main sequence at z = 2.23 based on the analysis in Popesso et al. (2023) in green. Because the star formation main sequence is calibrated using a Kroupa IMF, we converted the star formation rates and stellar masses to reflect the Chabrier IMF used in Osborne & Salim (2024). Although we measured the likelihood that all galaxies, regardless of the median redshift estimate are at z = 2.246, in the above plot, we only included those galaxies with a median photometric redshift (or spectroscopic redshift) of 2 < z < 3. The vertical line represents the 90% stellar mass completeness limit for BOSS1244 and BOSS1542 (10^10.3 M_⊙) based on the analysis in Liu et al. (2023). The horizontal line shows our estimate of the SFR completeness limit (20 M_⊙/yr).