Table B.3
Flux zero-point corrections applied to the LH photometry during photo-z fitting or stellar mass estimates.
| LH | |||||
|---|---|---|---|---|---|
| Filter | Template set | ||||
| EAZY | Brown | Ananna | Masses | ||
| u | 1.115 | 1.102 | 1.107 | 1.121 | |
| g | 0.989 | 0.978 | 0.94 | 0.904 | |
| r | 1.008 | 0.987 | 0.946 | 0.911 | |
| z | 0.99 | 1.006 | 0.992 | 0.981 | |
| gRCS | 0.921 | 0.915 | 0.879 | 0.873 | |
| rRCS | 0.963 | 0.947 | 0.904 | 0.889 | |
| iRCS | 0.931 | 0.941 | 0.906 | 0.9 | |
| zRCS | 0.919 | 0.935 | 0.921 | 0.927 | |
| J | 1.117 | 1.11 | 1.08 | 1.16 | |
| K | 1.113 | 1.071 | 1.109 | 1.126 | |
| 3.6 μm SERVS | 0.962 | 0.952 | 0.969 | 0.933 | |
| 4.5 μm SERVS | 1.0 | 0.94 | 1.0 | 0.908 | |
| 3.6 μm SWIRE | 1.0 | 0.977 | 1.0 | 0.954 | |
| 4.5 μm SWIRE | 1.019 | 0.967 | 1.0 | 0.941 | |
| 5.8 μm SWIRE | 1.04 | 0.977 | 1.0 | ||
| 8.0 μm SWIRE | 1.2 | 1.039 | 1.0 | ||
Notes. Values quoted are multiplicative corrections applied to the observed fluxes and flux uncertainties. The three photo-z template sets consist of the “EAZY” (Brammer et al. 2008), “Brown” (Brown et al. 2014, 2019), and “Ananna” (Ananna et al. 2017)libraries as described in Sect. 3.1. If a filter was not included in the SED fitting for a specific template set, we do not provide a corresponding value.
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