Table E.1.
Optical and NIR ground-based photometry.
| Time | Exposure | Instrument | Magnitude | Band |
|---|---|---|---|---|
| since Tb (hr) | time (s) | (AB) | ||
| 16.7 | 360 | VLT/X-shooter | > 23.1 | z |
| 16.81 | 930 | GTC/OSIRIS+ | > 23.9 | z |
| 16.96 | 600 | VLT/HAWK-I | 23.29±0.13 | Y |
| 12.31 | 1080 | NOT/NOTCam | 21.82±0.17 | J |
| 16.61 | 480 | VLT/HAWK-I | 22.50±0.08 | J |
| 38.64 | 2700 | NOT/NOTCam | > 21.5 | J |
| 16.74 | 480 | VLT/HAWK-I | 22.44±0.06 | H |
Notes.z-band photometry is calibrated against the Pan-STARRS catalogue, while Y, J, and H are calibrated against the VISTA Hemisphere Survey (McMahon et al. 2021). Upper limits are given at the 3σ levels. No correction has been made for the small Galactic foreground extinction (AJ = 0.026, AH = 0.016; Schlafly & Finkbeiner 2011).
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