Table 3
Summary of the instrumental PSF and depths adopted for the image simulations in this work from Merlin et al. (2021).
| Instrument | Filter | PSF(arcsec) | 5σ depth AB |
|---|---|---|---|
| HST ACS | F435W | 0.08 | 28.83(a) |
| F606W | 0.08 | 29.24(a) | |
| F814W | 0.09 | 29.35(a) | |
| F850LP | 0.09 | 28.54(a) | |
| HST WFC3 | F105W | 0.15 | 28.70(a) |
| F125W | 0.16 | 28.85(a) | |
| F140W | 0.17 | 27.64(a) | |
| F160W | 0.17 | 28.72(a) | |
| VLT HAWK-I | Ks | 0.43 | 26.26(b) |
| Spitzer IRAC | CH1 | 1.66 | 25.63(b) |
| CH2 | 1.72 | 25.51(b) | |
| CH3 | 1.88 | 23.28(b) | |
| CH4 | 1.98 | 23.16(b) |
Notes. (a)Median aperture magnitudes within a fixed radius of 0.17”; the given values are averages of the varying depths in the CANDELS GOODS-South field (including CANDELS-deep field and the HUDF depths). (b)Median total magnitude at 5σ; the given values are averages of the varying depths in the CANDELS GOODS-South field.
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