Table 1
Characterization of the transiting planets and the transit candidate in the Kepler-160 planetary system.
| Fitted model parameters | Kepler-160 b | Kepler-160 c | New transit candidate |
|---|---|---|---|
| Epoch, T0 (BKJD) | 134.0320 |
171.4805 |
489.780 |
| Period, P (d) | 4.309397 |
13.699429 |
378.417 |
| Planet-star radius ratio, Rp∕Rs |  |
 |
 |
| Impact parameter, b | 0.19 |
0.26 |
0.34 |
| S∕N | 33.5 | 111.2 | 9.5 |
| Number of transits (with data) | 451 (399) | 106 (95) | 3 (3) |
| SDETLS | 125 | 117.2 | 16.3 |
| FPP3 | 3.90 × 10−7 | 1.45 × 10−3 | 1.81 × 10−3 |
| Derived parameters | |||
| Planetary radius, Rp | 1.715 |
3.76 |
1.91 |
| Semimajor axis, a |  |
 |
 |
 AU |
 AU |
 AU |
|
Notes. The values for T0, P, Rp ∕Rs, and b were obtained from an MCMC fitting procedure to the entire detrended Kepler light curve and using linear ephemerides. S/N values were computed from the detrended light curve after MCMC fitting and phase-folding. The number of transits and SDETLS were calculated with TLS. The FPP3 values were computed with vespa and take the statistical multiplicity boost of this system into account. Planetary radii were derived from the fitted values for (Rp ∕Rs) and the stellar radius of 
from Gaia DR2. The
a∕Rs ratios were computed from the global fitof 
and the fitted values for P, respectively. The values of a units of AU were calculated from
a∕Rs and using the Gaia DR2 value of Rs. The stellar limb-darkening parameters were found to be 
and 
.
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