SFR versus stellar mass for AURORA sources, shown in squares color-coded by redshift. Overlaid are the L. Clarke et al. (2024) and J. S. Speagle et al. (2014) star-forming main-sequence relations based on SFR(hα), where the latter is lowered by 0.32 dex to be consistent with our adopted calibration. Note that the J. S. Speagle et al. (2014) measurement is limited to ﹩{\mathrm{log}}_{10}M/{M}_{\odot }=[9.7,11.1]﹩; however, we extrapolate it to visualize the relative offset from our AURORA sample. Offsets from the L. Clarke et al. (2024) relations are shown in the bottom panel. AURORA sources lie on and above the main sequence, reaching as high as 31 times the typical SFR at fixed mass.