Exomoon indicators in high-precision transit light curves

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Table A.1

Summary of our star, planet, and moon parameter grid.

								Case ID
									1a	1b	1c	1 d	1e	1f	1g	1h	1i	1j	1k	1l	1m	1n	1o	1p
								Parameter

								R_⋆ [R_⊙]	1	1	1	1	1	1	1	1	1	1	1	1	1	1	1	1
								M_⋆ [M_⊙]	1	1	1	1	1	1	1	1	1	1	1	1	1	1	1	1
								q₁	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6
								q₂	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4

								R_p	R_J	R_J	R_J	R_J	R_J	R_J	R_J	R_J	R_J	R_J	R_J	R_J	R_J	R_J	R_J	R_J
								M_p	M_J	M_J	M_J	M_J	M_J	M_J	M_J	M_J	M_J	M_J	M_J	M_J	M_J	M_J	M_J	M_J
								P_b [d]	30	30	30	30	30	30	30	30	30	30	30	30	30	30	30	30
								b_b	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1
								φ_b	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0

								R_s	0	0	0	0	R_⊕	R_⊕	R_⊕	R_⊕	0	0	0	0	R_⊕	R_⊕	R_⊕	R_⊕
								M_s	0	0	M_⊕	M_⊕	0	0	M_⊕	M_⊕	0	0	M_⊕	M_⊕	0	0	M_⊕	M_⊕
								P_s	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu
								φ_s	0-1	0-1	0-1	0-1	0-1	0-1	0-1	0-1	0-1	0-1	0-1	0-1	0-1	0-1	0-1	0-1
								i_s	0	0	0	0	0	0	0	0	0.2	0.2	0.2	0.2	0.2	0.2	0.2	0.2


Case ID
	2a	2b	2c	2d	3a	3b	3c	3d	4a	4b	4c	4d	5a	5b	5c	5d	6a	6b	6c	6d	7a	7b	7c	7d	8a	8b	8c	8d	9a	9b	9c	9d

Parameter

R_⋆ [R_⊙]	1	1	1	1	1	1	1	1	1	1	1	1	1	1	1	1	0.85	0.85	0.85	0.85	0.85	0.85	0.85	0.85	0.85	0.85	0.85	0.85	0.85	0.85	0.85	0.85
M_⋆ [M_⊙]	1	1	1	1	1	1	1	1	1	1	1	1	1	1	1	1	0.84	0.84	0.84	0.84	0.84	0.84	0.84	0.84	0.84	0.84	0.84	0.84	0.84	0.84	0.84	0.84
q₁	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.6	0.45	0.45	0.45	0.45	0.45	0.45	0.45	0.45	0.45	0.45	0.45	0.45	0.45	0.45	0.45	0.45
q₂	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.4	0.35	0.35	0.35	0.35	0.35	0.35	0.35	0.35	0.35	0.35	0.35	0.35	0.35	0.35	0.35	0.35

R_p	R_J	R_J	R_J	R_J	R_S	R_S	R_S	R_S	R_N	R_N	R_N	R_N	R_⊕	R_⊕	R_⊕	R_⊕	R_J	R_J	R_J	R_J	R_S	R_S	R_S	R_S	R_N	R_N	R_N	R_N	R_⊕	R_⊕	R_⊕	R_⊕
M_p	M_J	M_J	M_J	M_J	M_S	M_S	M_S	M_S	M_N	M_N	M_N	M_N	M_⊕	M_⊕	M_⊕	M_⊕	M_J	M_J	M_J	M_J	M_S	M_S	M_S	M_S	M_N	M_N	M_N	M_N	M_⊕	M_⊕	M_⊕	M_⊕
P_b [d]	30	30	58.31	58.41	30	30	58.31	58.41	30	30	58.31	58.41	30	30	58.31	58.41	30	30	58.31	58.41	30	30	58.31	58.41	30	30	58.31	58.41	30	30	58.31	58.41
b_b	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1	0.1
φ_b	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0

R_s	R_N	R_N	R_N	R_N	2 R_⊕	2 R_⊕	2 R_⊕	2 R_⊕	R_⊕	R_⊕	R_⊕	R_⊕	R_☾	R_☾	R_☾	R_☾	R_N	R_N	R_N	R_N	2 R_⊕	2 R_⊕	2 R_⊕	2 R_⊕	R_⊕	R_⊕	R_⊕	R_⊕	R_☾	R_☾	R_☾	R_☾
M_s	M_N	M_N	M_N	M_N	8 M_⊕	8 M_⊕	8 M_⊕	8 M_⊕	M_⊕	M_⊕	M_⊕	M_⊕	M_☾	M_☾	M_☾	M_☾	M_N	M_N	M_N	M_N	8 M_⊕	8 M_⊕	8 M_⊕	8 M_⊕	M_⊕	M_⊕	M_⊕	M_⊕	M_☾	M_☾	M_☾	M_☾
P_s	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu	P_Io	P_Eu
φ_s	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0	0
i_s	0.233	0.149	0.233	0.149	0.255	0.163	0.255	0.163	0.201	0.130	0.201	0.130	0.141	0.092	0.141	0.092	0.233	0.149	0.233	0.149	0.255	0.163	0.255	0.163	0.201	0.130	0.201	0.130	0.141	0.092	0.141	0.092

Notes. To preserve the orbital advancement per transit we changed the long planet orbit period from 60 d to the given values depending on the orbital period of the moon. The inclinations (i_s) tested in cases 1a–1p are 0 and 0.2 radians. For the other cases, the inclination is calculated as the smallest value needed to prevent occultations. The mass and radius of the Earth’s moon are referred to as M_☾ and R_☾, respectively.Subscripts S and N refer to Saturn and Neptune, respectively.

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