Table 3
Mapping between the input (columns) and output (lines) parameters of the model.
| e, i, ωp | a | d | T | tp | RP, Ag | wR | Ω | |
|
|
||||||||
| α, fT, ν | x | |||||||
| rorbit1, θ1 | ||||||||
| Date1 | x | x | ||||||
| Date2 | x | x | x | |||||
| rorbit2, θ2 | x | x | x | |||||
| CR 1 | x | x | ||||||
| CR 2 | x | x | x | |||||
| Pz, ΦPz1 | x | x | x | |||||
| ΦPz 2 | x | x | x | x | ||||
| ϕ North | x | x | ||||||
| υ orb | x | x | x | x | x | |||
Notes. An “x” indicates that the given input parameter(s) is required for computing that output parameter(s). Example: calculating the relative angular separation (line 4) and the absolute contrast ratio (line 7) only requires six input parameters: e, i, ωp, a, RPlanet, and Ag.
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