Notes. Target integration times are quantified per pointing (i.e. not summed across the field) and listed in units of hours. Imaging in Subaru HSC y and the narrow bands were not targeted under the Cosmic Dawn or H20 surveys, but were included as archival data and thus have no ‘target’ integration time. For Spitzer integration times, the reader is referred to Euclid Collaboration: Moneti et al. (2022).