Spectral energy distribution fits (top) and postage stamp cutouts (bottom) of the 30 most luminous galaxies in the U+E sample. (See Fig. 3 for a description of the SED plots.) The title of the SED indicates the object ID, absolute magnitude M_UV, and the literature ID if it has been previously identified. The postage stamps, from left to right, are from I_E, Y_E, J_E, H_E, and a VISTA YJHK_s stack. The stamps are 6″ × 6″ and are scaled to saturate at 5 σ above and 2 σ below the noise level. Objects with names beginning with UVISTA were identified in Bowler et al. (2014). Objects with names labelled as [ESC2021] and [ESC2021a] were first identified in Endsley et al. (2021b) and Endsley et al. (2021a), respectively. [DMD23] 892014 is from Donnan et al. (2023). COSMOS2015 and COSMOS2020 objects were identified in Laigle et al. (2016) and Weaver et al. (2022), respectively. S-CANDELS objects are galaxies identified in HST imaging (Ashby et al. 2015), and LAE-17 was identified in Hu et al. (2017). The SSTSL source is also identified as REBELS-21 (Bouwens et al. 2022).