Circumbinary exoplanets and brown dwarfs with the Laser Interferometer Space Antenna

Open Access

Table 1

Number of planetary detections depending by the different combinations of mass and semi-major axes distributions.

	DETECTIONS (4 yr)

	(A) (0.1–200 au)		(B) (0.1–200 au)		(C) log Normal_a (0.1–200 au)		(D) a^−0.61 (0.1–200 au)

	CBPs	BDs	CBPs	BDs	CBPs	BDs	CBPs	BDs
(1) (1M_⊕ – 0.08 M_⊙)	3 (0.011%)	79 (0.302%)	83 (0.317%)	2218 (8.482%)	18 (0.069%)	503 (1.924%)	28 (0.107%)	820 (3.136%)
(2) M^−1.31	6 (0.023%)	14 (0.054%)	30 (0.115%)	316 (1.209%)	5 (0.019%)	85 (0.325%)	13 (0.050%)	131 (0.501%)

Notes. In bold the minimal and maximal values for both CBPs and BDs. The percentage is computed over a total of 26 148 DWDs (visible during the nominal LISA mission length).

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