Table 2
Trapezoidal occultation parameters for all Ks data.
| Parameter | Value | Error |
|---|---|---|
| T1 | 0.47146 | 0.00219 |
| T4 | 0.53102 | 0.00139 |
| T14 | 0.05956 | 0.00270 |
| T12 | 0.00528 | 0.00070 |
| δ | 0.00270 | 0.00014 |
Notes. All eclipse times are in the units of the orbital phase. Eclipse depth δ is the relative flux depression. The ingress and egress times, T1 and T4, can be converted into Barycentric Julian dates (TDB standard) using the following formulae, e.g., for the ingress: Ting[BJD]= Tcen + P× (n + T1), where n is the epoch number of the event of interest and Tcen = 2458355.50805 is the moment of the transit center and P = 1.6284300 d is the orbital period. Epochs are ‘as observed’, i.e., no correction was made due to orbital light time effect of 27 s.
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