Filters covered in the surveys used and the reported observational depth of individual filters. Solid lines (“—”) indicate JWST NIRCam filters, dashed lines (“- -”) indicate filters from the HST, and dotted lines (“…”) indicate filters from the JWST MIRI instrument. Apertures were set variably according to the Rayleigh criterion formula and thus range from 0.035^′′ to 0.81^′′. The depth data presented was derived from reported values by survey authors (Weaver et al. 2023; D’Eugenio et al. 2025; Rieke et al. 2023; Hainline et al. 2024; Guo et al. 2013; Bagley et al. 2023; Yang et al. 2023). Some surveys employ in-house processes to the Hubble data and thus report adjusted depths.