Table 4
Final day- and nightside planet-star flux ratios and eclipse depths with their uncertainties and upper limits.
| Passband | Ns. flux ratio (%) | Ns. Tb (Κ) | Ds. flux ratio (%) | Eclipse depth (ppm) | Ds. Tb (Κ) |
|---|---|---|---|---|---|
| CHEOPS | <1.50 | <90 | 2100−2900 | ||
| TESS | <4 | <3000 | 6.1 ± 0.9 | 360 ± 50 | 3100−3500 |
| H | 17.3 ± 3.2 | 1000 ± 190 | 2100−3400 | ||
| Ks | 24.9 ± 1.9 | 1460 ± 110 | 2900−3400 | ||
| Spitzer 3.6 µm | <11 | <1900 | 34.9 ± 1.4 | 2040 ± 80 | 3000−3400 |
| Spitzer 4.5 µm | <12 | <1800 | 35.3 ± 1.5 | 2070 ± 80 | 2800−3200 |
Notes. The nightside estimates give an upper limit corresponding to the 99th posterior percentiles. The dayside estimates correspond to posterior medians with uncertainties based on the 16th and 84th posterior percentiles (except for CHEOPS, for which we only give the upper limit). The reported dayside brightness temperature values are lower and upper limits corresponding to 2.5th and 97.5th posterior percentiles.
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