Table 1
Photometry available for the counterpart identification and photo-z computation.
| Bands | Survey | Depth (AB mag) various indicators | Reference |
|---|---|---|---|
| FUV, NUV | GALEX | 19.9, 20.8 | Bianchi (2014) |
| u, g, r, i | KiDS | 24.2, 25.1, 25.0, 23.7 | Kuijken et al. (2019) |
| g, r, i, z, y | HSC | 26.8, 26.4, 26.4, 25.5, 24.7 | Aihara et al. (2018b) |
| g, r, i | LS8 | 24.0, 23.4, 22.5 | Dey et al. (2019) |
| z, J, H, K | KiDS/VIKING | 23.1, 22.3, 22.1, 21.5, 21.2 | Kuijken et al. (2019) |
| J, Ks | VISTA/VHS | 21.1, 19.8 | McMahon et al. (2013) |
| W1, W2, W3, W4 | LS8/WISE | 21.0, 20.1, 16.7, 14.5 | Meisner et al. (2019) |
Notes. For LS8, the required depth for DESI is listed. For Ls8/WISE, the listed depth is taken from Meisner et al. (2019) and is computed using WISE detected sources. Because the photometry we used is forced photometry at the position of optically detected sources, the depth is higher.
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