An upper limit on the frequency of short-period black hole companions to Sun-like stars

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Table 3.

Results for all targets for which observations were obtained, as is described in Sections 3–5.

TIC ID	Telescope	Epochs	P_orb	K	f_M	M_2, min	q_min	SB2	p_BH, 3	p_BH, 8
			[days]	[km s⁻¹]	[M_⊙]	[M_⊙]
1947924	Gaia RVs	29	1.95	36.7	0.010	0.33	0.17	N	0.02	0.01
3103024	Gaia RVs	11	2.06	35.2	0.009	0.34	0.17	N	0.02	0.01
5769943	NTT	2	1.35	98.1 ± 24.8	0.132 ± 0.127	0.60 ± 0.15	0.47 ± 0.12	N	0.11	0.04
7264195	Gaia RVs	38	0.42	201.2	0.351	0.77	0.67	N	0.21	0.08
13205508	Gaia RVs	36	1.51	28.2	0.003	0.23	0.12	N	0.01	0.00
18750830	INT	6	0.40	45.7 ± 1.9	0.004 ± 0.001	0.19 ± 0.01	0.14 ± 0.01	Y	0.01	0.00
19124199	NTT	4	1.84	37.9 ± 3.6	0.010 ± 0.003	0.28 ± 0.03	0.19 ± 0.02	N	0.02	0.01
21586667	INT	3	1.70	84.2 ± 2.0	0.105 ± 0.008	0.64 ± 0.01	0.40 ± 0.01	N	0.10	0.04
24358586	Gaia RVs	28	2.03	64.8	0.057	0.44	0.36	N	0.06	0.02
26516212	Gaia SB1	25	2.63	19.8 ± 3.2	0.002 ± 0.001	0.19 ± 0.03	0.10 ± 0.02	N	0.01	0.00
⋮	⋮	⋮	⋮	⋮	⋮	⋮	⋮	⋮	⋮	⋮

Notes. The column f_M contains the mass function. This table contains 250 rows and is sorted by TIC ID. The full table is available at the Centre de Données astronomiques de Strasbourg (CDS).

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