Using electromagnetic observations to aid gravitational-wave parameter estimation of compact binaries observed with LISA

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Table 1

Physical properties of verification binaries based on observations summarised in Nelemans (2011).

	S/N	m₁[M_⊙]	m₂[M_⊙]	d[kpc]		P_orb[s]	ι[°]	Ṗ_orb[s/s]	β[rad]	λ[rad]

J0651	10.7	0.55^a	0.25^a	~1^a	1.67	765.4 ± 7.9^a	^a	–	0.101	1.769
AM CVn	11.5	0.71^b	0.13^b	^c	1.49	1028.73^d	43 ± 2^c	–	0.653	2.974
HM Cnc	39.7	0.55^e	0.27^e	5^e	6.38	321.529^f	≈ 38^e	3.75 × 10^-11^f	₀ .082	2.102

Notes. The signal-to-noise ratio (S/N) listed in the second column is from GW data analysis, as explained in Sect. 3.

^(a)

Brown et al. (2011);

^(b)

Roelofs et al. (2006);

^(c)

Roelofs et al. (2007);

^(d)

Skillman et al. (1999);

^(e)

Roelofs et al. (2010);

^(f)

Strohmayer (2005);

^(*)

Eq. (3).

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