Then and now: A new look at the eclipse timing variations of hierarchical triple star candidates in the primordial Kepler field, revisited by TESS

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Table A.6.

Orbital elements from moderately certain combined dynamical and LTTE solutions for systems.

KIC No.	P₁	P₂	a₂	e₂	ω₂	τ₂	f(m_C)	$\frac{m_{C}}{m_{ABC}}$ $\frac{m_{\mathrm{C}}}{m_{\mathrm{ABC}}}$	m_AB	m_C	$\frac{A_{dyn}^{meas}}{A_{LTTE}}$ $\frac{{\cal{A}}^{\mathrm{meas}}_{\mathrm{dyn}}}{{\cal{A}}_{\mathrm{LTTE}}}$
	(day)	(day)	(R_⊙)		(deg)	(MBJD)	(M_⊙)		(M_⊙)	(M_⊙)
5080652	4.14435547(8)	222.9(5)	251(28)	0.15(5)	350(7)	54865(15)	0.50(44)	0.49(15)	2.18(45)	2.10(133)	0.89
6877673	36.7593121(8)	3765(48)	1268(11)	0.18(1)	158(2)	53869(39)	0.0134(4)	0.193(2)	1.56(1)	0.37(1)	1.9
7837302	23.836787(2)	1381.3(9)	720(13)	0.265(8)	155(7)	56346(7)	0.010(2)	0.16(2)	2.20(13)	0.42(5)	7.1
9664215	3.3195332(1)	928(2)	537(18)	0.55(2)	182(3)	55758(6)	0.14(2)	0.39(1)	1.49(20)	0.93(14)	0.45
		5470(65)	321(31)a	0.40(7)	254(16)	56414(252)	0.015(4)	−	0.57^a	3:
10268809	24.708843(5)	4084(6)	1473(27)	0.636(6)	290(2)	56144(4)	0.17(2)	0.41(1)	1.52(11)	1.05(9)	4.61
10296163	9.29678473(3)	3408(3)	1274(68)	0.385(6)	2.6(8)	55953(5)	0.0036(8)	0.142(6)	2.05(38)	0.34(6)	0.31
12356914	27.308390(3)	1824(6)	942(15)	0.384(9)	106(3)	55863(8)	0.0052(5)	0.135(5)	2.92(15)	0.46(3)	7.8

Notes. ^(a)The fourth-body orbit is a pure LTTE solution; hence, the given value is a_ABCsin i₃ instead of a₃ and, similarly, instead of m_D, what is given is its minimum mass (for i₃ = 90°).

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