Table 1.
Photometric bands and the corresponding instrument, central wavelength, and observed depth (3″).
| Band | Instrument/Telescope | λ[Å] | Depth [mag] |
|---|---|---|---|
| u* | MegaCam/CFHT | 3858 | 27.1 |
| g | HSC/Subaru | 4847 | 27.5 |
| r | HSC/Subaru | 6219 | 27.2 |
| i | HSC/Subaru | 7699 | 27.0 |
| z | HSC/Subaru | 8894 | 26.6 |
| Y | VIRCAM/VISTA | 10 216 | 26.1 |
| J | VIRCAM/VISTA | 12 525 | 25.9 |
| H | VIRCAM/VISTA | 16 466 | 25.5 |
| K | VIRCAM/VISTA | 21 557 | 25.2 |
Notes. The instruments we used are the Canada-France-Hawaii telescope (CFHT) and MegaCam instrument (Boulade et al. 1998), the Hyper Suprime-Cam (HSC) (Miyazaki et al. 2018), and the VIRCAM instrument on the VISTA telescope from the UltraVISTA survey (McCracken et al. 2012).
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