Notes. Columns include: central wavelength, sky brightness (in AB magnitudes/arcsec²), zero-points (for AB magnitudes and fluxes in e⁻/s), and AB magnitude limits for point sources detected at S/N = 10 in 600 s using PSF photometry, accounting for dark current, read-out noise and pixel sampling. Note that the sensitivities provided in Laureijs (2009) differ substantially because they apply to objects measured using aperture photometry, with a higher sky background because the EUCLID wide survey cannot be confined to high ecliptic latitudes.