An updated catalog of HIRES/Keck radial velocity measurements - Including Ca II H&K measurements

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Volume 702 (October 2025)

A&A, 702 (2025) A68

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Table B.1

Confirmed single massive planets.

Planet	∆ log L	RV_rms	Med_e_RV	Med_e_RVC	K	e_K	References
		[m s⁻¹]	[m s⁻¹]	[m s⁻¹]	[m s⁻¹]	[m s⁻¹]
HD 210277b	10.3766	2.9623	1.12	1.176	38.32	0.255	1
HD 16175b	8.6752	4.5107	1.505	1.553	94.0	11.0	2,3
HD 45350b	5.1638	3.6572	1.2	1.25	59.4	2.9	1
HD 222582b	3.7351	3.3887	1.385	1.4375	303.0	2.95	1
HD 117207b	3.1763	3.371	1.505	1.5705	27.44	0.715	1,3
HD 13931b	2.3411	4.0831	1.44	1.485	23.38	0.615	1,3
HD 175541b	2.2376	6.1661	1.29	1.363	13.76	0.735	1
HD 209458b	2.081	11.0145	1.75	1.794	84.9	1.25	1,4
HD 190007b	2.072	5.593	1.56	1.605	4.91	0.45	5
HD 114729b	2.0463	3.9543	1.6	1.66	18.1	1.0	1
HD 218566b	1.8617	3.7726	1.275	1.319	7.68	0.7	1
HD 10697b	1.7392	5.9151	1.49	1.545	114.583	1.1315	3, 6
HD 50554b	1.5839	5.2664	1.72	1.7605	90.8	3.35	1,3
HD 86081b	1.404	5.1901	1.7	1.719	205.53	0.78	7
HD 141937b	1.112	6.2162	1.835	1.8575	234.5	6.4	2, 8
HD 8574b	1.0349	6.7892	1.915	1.9585	58.3	1.55	1
HD 142245b	0.8778	5.8723	1.195	1.2125	24.8	2.6	2, 9
HD 88133b	0.8754	4.0489	1.425	1.466	32.93	0.73	10
HD 210702b	0.7562	3.7575	1.125	1.161	36.11	1.365	11
HD 224693b	0.7561	5.5276	2.34	2.366	39.96	0.68	7
HD 181234b	0.7045	2.8557	1.44	1.487	126.925	1.566	3, 6
HD 38801b	0.6873	8.7225	1.175	1.222	196.3	3.8	10
HD 189733b	0.6519	15.0117	1.04	1.069	204.7	2.55	4, 12
HD 109749b	0.5158	3.2765	1.34	1.371	29.2	1.1	7
HD 1502b	0.5012	12.7243	1.55	1.568	57.5	3.3	10
HD 179949b	0.467	7.8666	2.28	2.291	118.0	2.8	1
HD 52265b	0.4165	4.42201	1.59	1.62	41.14	0.69	1
HD 131496b	0.4111	6.5044	1.23	1.257	31.6	1.8	10
HD 94834b	0.3867	5.9949	1.27	1.299	20.7	2.9	10
HD 102956b	0.2596	6.6496	1.245	1.289	74.6	1.8	10
HD 10442b	0.2175	5.9408	1.8	1.8185	29.9	1.6	10
HD 72490b	0.2002	6.0459	1.45	1.5095	33.5	1.5	10
HD 152581b	0.1218	4.1966	1.44	1.449	36.2	1.3	10
HD 211810b	0.1055	3.5015	1.28	1.317	15.6	7.2	7
HD 130322b	0.0708	6.1316	1.42	1.473	111.1	2.35	1
HD 192263b	0.0341	8.2431	1.47	1.548	55.3	2.15	12
HD 231701b	−7.0E-4	6.9598	2.405	2.443	39.2	1.2	7
HD 17156b	−0.0155	3.5644	1.46	1.494	274.7	3.5	4, 7
HD 16417b	−0.0443	2.6798	1.045	1.064	5.0	0.4	13
HD 40979b	−0.0555	18.2648	2.21	2.247	107.9	4.0	1
HD 190228b	−0.112	3.9622	1.715	1.7415	92.936	1.2395	3, 6
HD 31253b	−0.1181	5.3455	1.555	1.596	10.8	1.8	1
HD 170469b	−0.1295	2.6718	1.52	1.577	10.2	1.3	1
10HD 168746b	−0.1305	3.5392	1.635	1.662	27.17	0.789	1
HD 4313b	−0.151	5.6019	1.415	1.4515	40.3	1.7	10
HD 206610b	−0.3093	10.2176	1.35	1.3765	35.4	1.0	10
HD 99109b	−0.3885	5.8102	1.42	1.477	12.98	0.875	1
HD 96167b	−0.5356	4.3132	1.45	1.504	21.5	1.4	10
HD 214823b	−0.5451	3.5182	1.775	1.8005	283.005	0.7795	3, 6
HD 164509b	−0.5612	5.4072	1.285	1.317	13.15	0.77	14
HD 136925b	−0.5987	5.2447	1.645	1.6825	11.4	0.995	1
HD 108863b	−0.6751	6.1651	1.2	1.243	47.4	1.5	10
HD 178911b	−0.7386	3.9829	1.28	1.315	342.69	0.82	1
HD 55696b	−0.7716	8.9351	2.06	2.085	76.7	3.9	3, 7
HD 149026b	−0.8982	7.0589	1.52	1.547	39.22	0.68	4, 7
HD 82886b	−0.9558	8.2932	1.62	1.679	28.7	2.1	2, 9
BD 103166b	−0.983	6.4099	2.06	2.092	60.2	1.5	1
HD 98219b	−1.2203	5.8728	1.29	1.34	42.0	2.1	10
HD 154345b	−1.2958	4.14601	1.45	1.4825	13.29	1.125	1,3
HD 149143b	−1.4233	7.4232	2.18	2.198	150.0	0.65	7
HD 185269b	−1.6229	6.5588	2.08	2.0945	93.3	1.4	10
HD 102195b	−1.8258	8.4974	1.17	1.203	66.9	3.4	12
HD 43691b	−1.9087	6.27601	1.72	1.748	130.06	0.84	7
HD 32963b	−2.0956	2.9379	1.355	1.3845	11.32	0.415	1,3
HD 73534b	−3.8289	4.6557	1.23	1.272	17.11	0.93	10
HD 179079b	−4.3308	4.0937	1.41	1.434	6.22	0.78	7
HD 49674b	−4.3493	5.8716	1.22	1.28	13.21	0.885	1
HD 180617b	−4.4358	5.7181	2.62	2.632	2.696	0.224	15
HD 87883b	−5.7473	2.3032	1.36	1.423	51.435	0.626	6
HD 46375b	−7.0105	3.5297	1.21	1.293	33.46	0.8	1
HD 45652b	−9.5988	14.3901	1.06	1.162	33.2	1.8	7

References. (1) Rosenthal et al. (2021); (2) Stassun et al. (2017); (3) Xiao et al. (2023); (4) Kokori et al. (2023); (5) Stalport et al. (2023); (6) Feng et al. (2022); (7) Ment et al. (2018); (8) Udry et al. (2002); (9) Johnson et al. (2011); (10) Luhn et al. (2019); (11) Teng et al. (2023); (12) Paredes et al. (2021); (13) O’Toole et al. (2009); (14) Giguere et al. (2011); (15) Burt et al. (2021).

Notes. RV_rms is the root mean square of the corrected RVs. Med_e_RV and Med_e_RVC represent the median uncertainties of the uncorrected and corrected RVs, respectively. K is the semi-amplitude of the Keplerian signal, with its associated uncertainty denoted as e_K.

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