Table 1
Characteristics of the bands considered in this work.
band | ![]() |
sky (AB/arcsec2) | zp (e−/s) | 10σ (600 s, ps) |
|
||||
g | 4965 | 23.19 | 24.27 | 25.1 |
r | 5958 | 22.89 | 24.32 | 25.1 |
i | 7162 | 22.68 | 24.18 | 24.9 |
z | 8574 | 22.60 | 23.72 | 24.4 |
y | 10 476 | 22.47 | 24.32 | 24.4 |
J | 12 549 | 22.44 | 24.37 | 24.4 |
H | 15 148 | 22.31 | 24.41 | 24.4 |
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.
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