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Table A.2

Stellar and planetary parameters from the photodynamical modelling of the 2:1 resonance solution on Kepler long- and short-cadence data, the 6:2:1 resonance solution on Kepler data, the 3:2:1 resonance solution on Kepler data, the 3:2:1 resonance solution on Kepler data and the three KOINet transit light curves, and some corrections from investigating stellar evolution models in Sect. 5.4.

Parameter Kepler data Kepler data Kepler data Kepler & MESA
KOINet data
2:1 6:2:1 3:2:1 3:2:1 3:2:1
Kepler-82b
mbmS
207 ± 10
ab,corr 0.999927 ± 0.000011
0.1684 ± 0.0021 0.1683 ± 0.0020 0.1683 ± 0.0020 0.1683 ± 0.0020
26.44 ± 0.48 26.44 ± 0.48 26.44 ± 0.48 26.44 ± 0.48
eb
0 (fixed)
254.6 ± 1.3
0.079 ± 0.018
354.6 ± 1.3
RbRS

Kepler-82c
mcmb 0.156 ± 0.012 1.06 ± 0.14
32.2 ± 2.2 14.3 ± 1.3
ac,corr
0.2637 ± 0.0032 0.2626 ± 0.0032 0.2626 ± 0.0032 0.2626 ± 0.0032
51.84 ± 0.95 51.53 ± 0.94 51.53 ± 0.94 51.54 ± 0.94
ec
config. I 89.96 ± 0.18
config. II
config. I 1.6 ± 2.1
config. II 0.29 ± 0.10
− 0.507 ± 0.020
RcRS

Kepler-82f
mfmc
415 ± 23 20.9 ± 1.0 20.9 ± 1.0
PfPc
(d) 75.732 ± 0.012
0.5616 ± 0.0068 0.3395 ± 0.0041 0.3395 ± 0.0041
ef
config. I 86.30 ± 0.56
config. II
1.9 ± 2.2

Kepler-82
mS (M) 0.91 ±0.03 (fixed, Johnson et al. 2017)
RS (R)
c1,Kepler
c2,Kepler

Notes. Listed are the median values and 68.26% confidence interval from the MCMC posterior distribution. The osculating orbital elements are given at a reference time, BJD = 2 454 933.0. (*) Derived, not fitted parameters.

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