Table 3
Inferred transit parameters for 55 Cnc e obtained using the light curves detrended by the classical (CM) and time-shift (TM) procedures and their 1σ uncertainties.
| Parameter | Symbol | Units | Value (CM) | Value (TM) | Bourrier et al. (2018a) | |
|---|---|---|---|---|---|---|
| Measured parameters | Orbital period | P | days |  |
 |
 |
| Transit epoch | T0 − 2 451 545 | BJD |  |
 |
 |
|
| Planet-to-star radius ratio | Rp∕Rs |  |
 |
 |
||
| Impact parameter | b |  |
 |
 |
||
| Transit duration | td | days |  |
 |
 |
|
| Eclipse depth | δecl | ppm |  |
 |
||
| Derived parameters | Transit depth |  |
ppm |  |
 |
 |
| Planetary radius | Rp | R⊕ |  |
 |
 |
|
| Scaled semimajor axis | a∕Rs |  |
 |
 |
||
| Semimajor axis | a | AU |  |
 |
 |
|
| Orbital inclination | i | deg |  |
 |
 |
|
Notes. The last column indicates the most recent values published in Bourrier et al. (2018a). All the 1σ uncertainties were derived using the distribution of the parameter posteriors. The impact parameter was completely determined by the input prior.
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