Table A.1
Trapezoidal fit parameters to the nightly Ks datasets
| Set | T1 (phase) | T4 (phase) | T14 (phase) | T12 (phase) | δ (ΔF/F) | σfit (ΔF/F) | N |
|---|---|---|---|---|---|---|---|
| 1 | 0.47908 ± 0.00411 | 0.53234 ± 0.00468 | 0.05326 ± 0.00576 | 0.00766 ± 0.00128 | 0.00293 ± 0.00037 | 0.00356 ± 0.00012 | 699 |
| 2 | 0.46810 ± 0.00267 | 0.53204 ± 0.00180 | 0.06394 ± 0.00348 | 0.00633 ± 0.00102 | 0.00270 ± 0.00018 | 0.00300 ± 0.00005 | 2084 |
| 3 | 0.47169 ± 0.00310 | 0.53073 ± 0.00444 | 0.05903 ± 0.00426 | 0.00525 ± 0.00084 | 0.00279 ± 0.00022 | 0.00327 ± 0.00007 | 1732 |
| 123 | 0.47146 ± 0.00219 | 0.53102 ± 0.00139 | 0.05956 ± 0.00270 | 0.00528 ± 0.00070 | 0.00270 ± 0.00014 | 0.00317 ± 0.00004 | 4515 |
Notes: The ingress and egress phases (T1, T4) can be converted into Barycentric Julian Date (TDB standard) by the following formulae: Ting,egr[BJD]= Tcen + P × (n + T1/4), where n is the epoch number of the event of interest and Tcen = 2458355.50805 is the moment of the transit center, P = 1.6284300 d – see Sect. 4.1 for more details. The epochs are without correction for orbital light time effect.
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