Correlations between the stellar, planetary, and debris components of exoplanet systems observed by Herschel

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Table 4

Summary table of all exoplanets in each system.

Name	Planet	Mass (Msini)	Semi-major axis	Eccentricity	Reference
		[M_Jup]	[AU]		Orbit	Discovery

HD 1237	b	3.37 ± 0.09	0.4947 ± 0.0083	0.511 ± 0.017	1	1
HD 3651	b	0.229 ± 0.0148	0.2947 ± 0.0049	0.596 ± 0.036	2	3
HD 4308	b	0.0477 ± 0.0028	0.1192 ± 0.00199	0.000	4	4
υ And	b	0.669 ± 0.026	0.05939 ± 0.00099	0.013	5	6
	c	1.919 ± 0.088	0.830 ± 0.0138	0.224 ± 0.026	5	7
	d	4.12 ± 0.165	2.525 ± 0.042	0.267 ± 0.0196	5	7
q¹ Eri	b	0.93 ± 0.24	2.022 ± 0.082	0.16	8	8
τ Ceti	b	0.0063 ± 0.0025	0.105 ± 0.005	0.16	9	9
	c	0.0098	0.195 ± 0.009	0.03	9	9
	d	0.0113 ± 0.0054	0.374 ± 0.020	0.08	9	9
	e	0.0135 ± 0.0066	0.552 ± 0.023	0.05	9	9
	f	0.0208 ± 0.0110	1.350 ± 0.080	0.03	9	9
GJ 86	b	4.00 ± 0.137	0.1142 ± 0.0019	0.0416 ± 0.0072	8	10
ι Hor	b	2.05 ± 0.2	0.924 ± 0.0161	0.14 ± 0.13	8	11
HD 19994	b	1.33 ± 0.105	1.306 ± 0.022	0.266 ± 0.014	2	12
HD 20794	b	0.00849 ± 0.00096	0.1207 ± 0.002	0	13	13
	c	0.0074 ± 0.00135	0.2036 ± 0.0034	0	13	13
	d	0.0148 ± 0.00181	0.3498 ± 0.0058	0	13	13
ϵ Eri	b	1.05 ± 0.188	3.38 ± 0.32	0.25 ± 0.23	8	14
HD 33564	b	9.13 ± 0.37	1.124 ± 0.0196	0.340 ± 0.02	15	15
HD 39091	b	10.09 ± 0.38	3.35 ± 0.104	0.6405 ± 0.0072	8	16
HD 40307	b	0.01291 ± 0.00084	0.04689 ± 0.00078	0	17	17
	c	0.0211 ± 0.00118	0.0801 ± 0.00133	0	17	17
	d	0.0281 ± 0.00162	0.1324 ± 0.0022	0	17	17
HD 69830	b	0.0316 ± 0.00172	0.0782 ± 0.0013	0.100 ± 0.04	18	18
	c	0.0368 ± 0.0025	0.1851 ± 0.0031	0.130 ± 0.06	18	18
	d	0.0563 ± 0.0052	0.627 ± 0.0122	0.070 ± 0.07	18	18
55 Cnc	b	0.801 ± 0.027	0.1134 ± 0.00189	0.0040 ± 0.003	19	6
	c	0.1646 ± 0.0066	0.2373 ± 0.004	0.070 ± 0.02	19	20
	d	3.54 ± 0.122	5.475 ± 0.094	0.0200 ± 0.008	19	20
	e	0.0262 ± 0.00123	0.01544 ± 0.00026	0	19	21
	f	0.173 ± 0.0106	0.774 ± 0.0129	0.320 ± 0.05	19	22
47 UMa	b	2.546 ± 0.096	2.101 ± 0.035	0.032 ± 0.014	23	24
	c	0.546 ± 0.071	3.57 ± 0.111	0.098 ± 0.071	23	25
HD 99492	b	0.106 ± 0.0117	0.1219 ± 0.002	0.254 ± 0.092	8	26
	c	0.36 ± 0.02	5.4 ± 0.1	0.106 ± 0.006	27	27
HD 102365	b	0.0510 ± 0.0081	0.4633 ± 0.0078	0.34 ± 0.14	28	28
61 Vir	b	0.0161 ± 0.00184	0.05006 ± 0.00083	0.12 ± 0.11	29	29
	c	0.0334 ± 0.0038	0.2169 ± 0.0036	0.140 ± 0.06	29	29
	d	0.0716 ± 0.0093	0.4745 ± 0.008	0.350 ± 0.09	29	29
70 Vir	b	7.46 ± 0.25	0.4836 ± 0.0081	0.4007 ± 0.0035	8	30
τ Boo	b	4.17 ± 0.142	0.04800 ± 0.0008	0.023 ± 0.015	31	6
α Cen B	b	0.00356 ± 0.00028	0.0419 ± 0.0007	0	32	32
GJ 581	b	0.0499 ± 0.0023	0.04061 ± 0.00087	0.031 ± 0.014	33	34
	c	0.0168 ± 0.00119	0.0729 ± 0.00157	0.070 ± 0.06	33	35
	d	0.0191 ± 0.0022	0.2177 ± 0.0047	0.250 ± 0.09	33	35
	e	0.00613 ± 0.00071	0.02846 ± 0.00061	0.320 ± 0.09	33	17
ρ CrB	b	1.064 ± 0.053	0.2257 ± 0.0038	0.057 ± 0.028	8	36
14 Her	b	5.21 ± 0.3	2.934 ± 0.084	0.3690 ± 0.005	37	38
HD 154345	b	0.957 ± 0.061	4.21 ± 0.105	0.044	39	40
μ Ara	b	1.746 ± 0.069	1.527 ± 0.029	0.128 ± 0.017	41	42
	c	1.89 ± 0.22	5.34 ± 0.4	0.099 ± 0.063	41	43
	d	0.0346 ± 0.00199	0.0928 ± 0.00177	0.172 ± 0.04	41	44
	e	0.543 ± 0.03	0.940 ± 0.018	0.067 ± 0.0122	41	41,45
HD 176051	b	1.5 ± 0.3	19.1	0.2667 ± 0.0022	46	46
16 Cyg B	b	1.640 ± 0.083	1.660 ± 0.028	0.681 ± 0.017	8	47
HD 189567	b	0.0316 ± 0.0034	0.1099 ± 0.0018	0.23 ± 0.14	48	48
HD 192310	b	0.0531 ± 0.0028	0.3223 ± 0.0054	0.130 ± 0.04	13	49
	c	0.0736 ± 0.0098	1.184 ± 0.024	0.32 ± 0.11	13	13
GJ 832	b	0.644 ± 0.075	3.40 ± 0.153	0.12 ± 0.11	50	50
HD 210277	b	1.273 ± 0.051	1.131 ± 0.0189	0.476 ± 0.017	8	51
GJ 876	b	1.95 ± 0.122	0.2081 ± 0.0065	0.0324 ± 0.0013	52	53,54
	c	0.612 ± 0.021	0.1296 ± 0.0022	0.25591 ± 0.00093	52	55
	d	0.0184 ± 0.00123	0.02081 ± 0.00035	0.207 ± 0.055	52	56
	e	0.0392 ± 0.0051	0.333 ± 0.0105	0.055 ± 0.012	52	52
51 Peg	b	0.461 ± 0.0164	0.05211 ± 0.00087	0.013 ± 0.012	8	57
HD 217107	b	1.401 ± 0.048	0.0750 ± 0.00125	0.1267 ± 0.0052	5	58
	c	2.62 ± 0.15	5.33 ± 0.2	0.517 ± 0.033	5	59

Reference. (1) Naef et al. (2001); (2) Wittenmyer et al. (2009); (3) Fischer et al. (2003); (4) Udry et al. (2006); (5) Wright et al. (2009); (6) Butler et al. (1997); (7) Butler et al. (1999); (8) Butler et al. (2006); (9) Tuomi et al. (2013); (10) Queloz et al. (2000); (11) Kürster et al. (2000); (12) Mayor et al. (2004); (13) Pepe et al. (2011); (14) Hatzes et al. (2000); (15) Galland et al. (2005); (16) Jones et al. (2002); (17) Mayor et al. (2009); (18) Lovis et al. (2006); (19) Endl et al. (2012); (20) Marcy et al. (2002); (21) McArthur et al. (2004); (22) Fischer et al. (2008); (23) Gregory & Fischer (2010); (24) Butler & Marcy (1996); (25) Fischer et al. (2002); (26) Marcy et al. (2005); (27) Meschiari et al. (2011); (28) Tinney et al. (2011); (29) Vogt et al. (2010); (30) Marcy & Butler (1996); (31) Brogi et al. (2012); (32) Dumusque et al. (2012); (33) Forveille et al. (2011); (34) Bonfils et al. (2005); (35) Udry et al. (2007); (36) Noyes et al. (1997); (37) Wittenmyer et al. (2007); (38) Butler et al. (2003); (39) Wright et al. (2008); (40) Wright et al. (2007); (41) Pepe et al. (2007); (42) Butler et al. (2001); (43) McCarthy et al. (2004); (44) Santos et al. (2004); (45) Goździewski et al. (2007); (46) Muterspaugh et al. (2010); (47) Cochran et al. (1997); (48) Mayor et al. (2011); (49) Howard et al. (2011); (50) Bailey et al. (2009); (51) Marcy et al. (1999); (52) Rivera et al. (2010); (53) Delfosse et al. (1998); (54) Marcy et al. (1998); (55) Marcy et al. (2001); (56) Rivera et al. (2005); (57) Mayor & Queloz (1995); (58) Fischer et al. (1999); (59) Vogt et al. (2005).

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