Circumbinary exoplanets and brown dwarfs with the Laser Interferometer Space Antenna

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Table 3

Among the detected SSOs in all 4 yr scenarios we report the systems with the least massive CBP detected (x, A2), with the highest S∕N (y, B1), and with the CBP with longest period (z, C1).

	S∕N_DWD	d[kpc]	m₁ [M_⊙ ]	m₂ [M_⊙ ]	P_b [min]	i_b [deg]	M [M_J]	a [au]	i [deg]	P [yr]	ΔΩ [arcmin²]	K [m s⁻¹]
(x)	290	8.12	0.53585	0.53146	4.29	26.8	0.27	2.22	119.33	3.19	1.77	4.3
(y)	963	1.55	0.74955	0.47068	5.25	119.8	10.99	0.61	130.79	0.43	0.14	272.30
(z)	182	6.35	0.32285	0.30066	2.66	42.22	11.11	3.67	138.36	8.82	12.6	137.11

Notes. In this table the DWD S/N is denoted as S/N_DWD rather than S/N as in the text.

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