Table 1.
Filters and associated observed depths.
| Band | λeff [μm] | EDF-F | EDF-N | EDF-S |
|---|---|---|---|---|
| CFHT/MegaCam u | 0.372 | 23.4 | ||
| HSC g | 0.480 | 24.9 | ||
| CFHT/MegaCam r | 0.640 | 24.0 | ||
| PAN-STARRS i | 0.755 | 23.1 | ||
| HSC z | 0.891 | 23.3 | ||
| Decam g | 0.473 | 24.6 | 24.7 | |
| Decam r | 0.642 | 24.3 | 24.4 | |
| Decam i | 0.784 | 23.8 | 23.8 | |
| Decam z | 0.926 | 23.1 | 23.1 | |
| VIS/IE | 0.715 | 24.7 | 24.7 | 24.7 |
| NISP/YE | 1.085 | 23.1 | 23.2 | 23.1 |
| NISP/JE | 1.375 | 23.2 | 23.3 | 23.3 |
| NISP/HE | 1.773 | 23.2 | 23.2 | 23.2 |
| IRAC/IRAC1 | 3.550 | 24.0 | 24.0 | 23.1 |
| IRAC/IRAC2 | 4.493 | 24.0 | 24.0 | 23.0 |
| IRAC/IRAC3 | 5.696 | 21.2 | 20.0 | |
| IRAC/IRAC4 | 7.799 | 19.9 | 21.1 |
Notes. The reported magnitudes are the 10σ observed depths. The optical and Euclid magnitudes refer to an extended source in an aperture with a diameter of 2 × FWHM and correspond to the median depths of the observing tiles (Euclid Collaboration: Romelli et al. 2026). For the IRAC1 and IRAC2 values, see Euclid Collaboration: Moneti et al. (2022) and Euclid Collaboration: McPartland et al. (2025). The depths correspond to average values in the fields that were derived considering empty apertures of 2″. For the IRAC3 and IRAC channels, we report the average depths derived from the catalogue after correction of the aperture to the total magnitudes.
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