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Table 4.

Self-consistent Newtonian two-planet orbital fits initialized from the results of optimization Run 1 for both datasets (A and B).

Parameter Dataset A (Run 1) Dataset B (Run 1)


χν, best2 χν, min2 χν, max2 χν, best2 χν, min2 χν, max2
eb 0.18(3) 0.10(4) 0.29(5) 0.08(3) 0.03(5) 0.30(5)
Kb (d) 0.00041(3) 0.00034(3) 0.00034(3) 0.00047(4) 0.00035(3) 0.00035(4)
ωb (rad) 0.13(6) 5.85(4) 0.08(8) 5.65(3) 4.54(5) 5.74(6)
Pb (yr) 6.96(6) 7.03(4) 6.91(5) 8.14(3) 6.90(3) 7.06(6)
Mb (rad) 4.53(5) 0.10(33) 5.92(3) 1.39(8) 2.32(7) 4.56(8)
ec 0.85(5) 0.15(3) 0.12(4) 0.88(5) 0.26(4) 0.08(6)
Kc (d) 0.00046(4) 0.00071(5) 0.00078(4) 0.00058(5) 0.00343(6) 0.00146(9)
ωc (rad) 4.79(8) 6.19(4) 0.52(9) 4.44(7) 5.38(5) 3.98(7)
Pc (yr) 15.67(8) 20.51(6) 22.26(7) 17.57(6) 33.92(7) 27.19(6)
Mc (rad) 0.75(7) 3.43(6) 2.32(8) 5.33(5) 6.20(4) 1.82(5)
Pbin (d) 0.11037410(2) 0.11037411(3) 0.11037412(2) 0.11037409(2) 0.11037428(3) 0.11037413(3)
T0 (BJD-2400000) 54274.20851(5) 54274.20851(4) 54274.20834(5) 54274.20819(4) 54274.20500(9) 54274.20712(6)
mb (MJup) 12.32 10.09 10.60 12.68 10.33 10.69
mc (MJup) 7.97 10.68 10.56 8.98 38.12 17.66
χν2 5.76 7.07 7.38 5.53 6.97 7.31

Notes. Columns χν, best2 display the best-fitting curve parameters, whereas columns χν, min2 and χν, max2 contain parameters corresponding to the minimum- and maximum-reduced chi-square values of stable configurations, respectively. The term Mb, Mc is the resulting mean anomaly of the inner and outer orbits, with each configuration being set up in the N-body osculating frame at the osculating epoch T0. Digits in parentheses are for the uncertainty at the last significant place.

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