Table 2.
Expected photometric depths for each of the fields covered by the DAWN survey.
Instrument/Band | EDF-N | EDF-F | EDF-S | COSMOS | SXDS | VVDS | AEGIS | GOODS-N |
---|---|---|---|---|---|---|---|---|
CFHT MegaCam/u | 26.4 | 26.4 | × | 27.7 | 27.6 | 27.4 | 27.0 | 26.6 |
Subaru HSC/g | 27.5 | 27.5 | × | 28.1 | 28.1 | 27.5 | 26.5 | – |
Subaru HSC/r | 27.5 | 27.5 | × | 27.8 | 27.8 | 27.1 | 26.1 | 27.8 |
Subaru HSC/i | 27.0 | 27.0 | × | 27.6 | 27.6 | 26.8 | 25.9 | 24.9 |
Subaru HSC/z | 26.5 | 26.5 | × | 27.2 | 27.2 | 26.3 | 25.1 | 24.5 |
Subaru HSC/y | 25.1 | – | × | 26.5 | 26.5 | 25.3 | 24.4 | 23.8 |
Spitzer IRAC/[3.6 μm] | 24.8 | 24.8 | 23.9 | 25.3 | 25.3 | 24.6 | 24.2 | 25.3 |
Spitzer IRAC/[4.5 μm] | 24.7 | 24.7 | 23.8 | 25.3 | 25.1 | 24.4 | 24.2 | 25.1 |
Euclid VIS/IE | 28.2 | 27.95 | 27.7 | |||||
Euclid NISP/YE | 26.3 | 26.05 | 25.8 | |||||
Euclid NISP/JE | 26.5 | 26.25 | 26.0 | |||||
Euclid NISP/HE | 26.4 | 26.15 | 25.9 | |||||
Rubin/u | × | 26.8 | × | × | ||||
Rubin/g | × | 28.4 | × | × | ||||
Rubin/r | × | 28.5 | × | × | ||||
Rubin/i | × | 28.3 | × | × | ||||
Rubin/z | × | 28.0 | × | × | ||||
Rubin/y | × | 26.8 | × | × |
Notes. Unless noted below, depths are quoted as the median 5σ limiting AB magnitude measured in 2″ empty apertures. Cells marked with ‘×’ indicate fields that are inaccessible by the designated facility. Cells marked with a dash (–) have no data taken at the time of publication. The Euclid depths are those expected for point sources by the end of the mission. Expected depths for Rubin data from Foley et al. (2018). The u band depths in SXDS and VVDS are from Sawicki et al. (2019), and the depths in AEGIS are from Gwyn (2012). The Subaru HSC and CFHT MegaCam depths for COSMOS are from Weaver et al. (2022). The HSC depths for SXDS, VVDS, and AEGIS are the average over each field provided by Aihara et al. (2022).
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