Table 1.
Summary of passbands considered in this work.
| Band | 5σ depth [AB] | λmean [Å] | FWHM [Å] |
|---|---|---|---|
| IE | 28.2 | 7140 | 3627 |
| YE | 26.3 | 10 829 | 2667 |
| JE | 26.5 | 13 696 | 4053 |
| HE | 26.4 | 17 762 | 5032 |
| Rubin/u | 26.1 (26.8) (a) | 3685 | 516 |
| Rubin/g | 27.4 (28.4) | 4802 | 1461 |
| Rubin/r | 27.5 (28.5) | 6231 | 1356 |
| Rubin/i | 26.8 (28.3) | 7542 | 1248 |
| Rubin/z | 26.1 (28.0) | 8690 | 1028 |
| Rubin/y | 24.9 (26.2) | 9736 | 9699 |
| CFHT/u | 26.2 | 3832 | 3899 |
| HSC/g | 27.5 | 4816 | 4724 |
| HSC/r | 27.5 | 6234 | 6136 |
| HSC/i | 27.0 | 7741 | 7654 |
| HSC/z | 26.5 | 8911 | 8902 |
| IRAC/3.6 μm | 24.8 | 35 634 | 7444 |
| IRAC/4.5 μm | 24.7 | 45 110 | 10 119 |
Notes. Expected 5σ depth (for point-like objects) in the Euclid Deep Fields, mean wavelength, and full width half maximum (FWHM) of the four Euclid filters, the Rubin ugrizy filters, the CFHT u and Subaru/HSC griz filters (McPartland et al., in prep.), and the Spitzer IRAC 3.6 and 4.5 μm filters (Euclid Collaboration 2022c).
Rubin depth after 10 years of observing; in parentheses we show the depths expected for the Rubin DDF (Foley et al. 2018).
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