Compilation of Discoveries of Substellar Companions around Giant Stars

This is, to the best of my knowledge, a list of all credible planets orbiting giant stars. Typically, only refereed publications are considered.
Planets orbiting subgiant stars are not included.

The table is now sortable (click on the column headers) and downloadable in cvs format!

99 substellar companions in 90 systems
click here to download data in cvs format

#namehipV-+K-+sptypefeh-+mstar-+m2sini-+period-+tzero-+ecc-+omega-+mf-+a2-+Krv-+referencetelescoperemarks




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1iota Dra b754583.290.671K2 III0.111.050.360.368.7510.720.070.072452015.360.160.160.7130.0080.00892.50.70.75.227e-71.27306.03.83.8Frink et al. 2002; Kane et al. 2010Hamilton (Lick)Additional linear trend. Updated elements here
2Pollux b378261.16-0.936K0 IIIb0.071.862.90.30.3589.73.53.52452337.952700.060.040.04277886.2e-90.6e-90.6e-91.690.030.0346.91.51.5Reffert et al. 2006Hamilton (Lick)similar elements by Hatzes et al. 2006
3HD 11977 b89284.682.590G5 III-0.162.316.54621.62.42.42452906.610100.30.030.0335.55.85.81.890.0050.005Setiawan et al. 2005;Soto et al. 2015FEROS; later HARPS and CHIRONupdated elements
4HD 47536 b316885.252.383K1 III-0.650.040.040.980.080.084.00.40.4434.92.62.62453040.830300.30.10.1268.617.317.31.120.0050.005Setiawan et al. 2003; Soto et al. 2015FEROS; Coralie; HARPS; CHIRONsecond planet most likely not real
5HD 13189 b100857.573.997K2 II4.52.52.51466471.66.06.02452327.920.220.20.270.060.06160.712.012.02.26e-70.37e-70.37e-71.5-2.2173.39.89.8Hatzes et al. 2005Tautenburg; McDonald; HET
6epsilon Tau b208893.531.422K0 III0.170.040.042.70.10.17.60.20.2594.95.35.30.1510.0230.0231.930.030.0395.91.81.8Sato et al. 2007HIDES (Okayama)
7HD 104985 b589525.783.274G9 III-0.352.38.3199.5050.0850.0852451927.53.33.30.0900.0090.009203.55.75.70.953e-70.022e-70.022e-70.95166.81.31.3Sato et al. 2003; Sato et al. 2008aHIDES (Okayama)
8NGC2423 No.3 b9.450.140.090.092.40.20.210.6714245321321210.210.070.071810100.180e-62.10137.69.19.1Lovis & Mayor 2007Coralie; HARPS
9NGC4349 No.127 b10.88-0.120.040.043.90.30.319.8678245411434340.190.070.076119190.442e-62.381881313Lovis & Mayor 2007Coralie; HARPS
104 UMa b425274.591.734K1 III-0.250.040.041.230.150.157.11.61.6269.30.430.020.022.05e-70.24e-70.24e-7216.8Döllinger et al. 2007Tautenburg
11HD 17092 b7.744.807K0 III0.222.30.30.34.60.30.3359.92.42.42452970.012.312.30.1660.0620.062347.413.413.42.001e-80.11e-80.11e-81.290.050.0582.43.23.2Niedzielski et al. 2007HET
1211 Com b602024.722.282G8 III-0.350.090.092.70.30.319.41.51.5326.030.320.322452899.61.61.60.2310.0050.00594.81.51.58.68e-70.21e-70.21e-71.290.050.05302.82.62.6Liu et al. 2008Xinglong; OAO
1318 Del b1035275.513.366G6 III-0.0520.0230.0232.310.3993.33.23.2245167218180.080.010.01166.16.56.51.743e-70.054e-70.054e-72.6119.41.31.3Sato et al. 2008aHIDES (Okayama)
14xi Aql b979384.712.171K0 III-0.2050.0390.0392.22.8136.750.250.252453001.71.41.4000.0399e-70.0031e-70.0031e-70.6865.41.71.7Sato et al. 2008aHIDES (Okayama)circular orbit fixed
15HD 81688 b464715.403.056K0 III-IV-0.3590.0200.0202.12.7184.020.180.182452335.41.11.1000.0385e-70.0019e-70.0019e-70.8158.580.970.97Sato et al. 2008aHIDES (Okayama)circular orbit fixed
1614 And b1160765.222.331K0 III-0.240.030.032.20.20.14.8185.840.230.232452861.41.51.5001.936e-60.0079e-60.0079e-60.83100.01.31.3Sato et al. 2008bHIDES (Okayama)circular orbit fixed
1781 Cet b122475.653.266G5 III-0.060.030.032.40.40.15.3952.78.88.82452486.26.26.0.2060.0290.029175.06.96.92.30e-60.15e-60.15e-62.562.81.51.5Sato et al. 2008bHIDES (Okayama)
18HD 102272 b574288.696.259K0 III-0.260.080.081.95.90.20.2127.580.300.302452146.564640.050.040.0411858580.6140.0010.001155.55.65.6Niedzielski et al. 2009aHET
19HD 102272 c574288.696.259K0 III-0.260.080.081.92.60.40.4520.26262454135.52602600.680.060.0632010101.570.050.05591111Niedzielski et al. 2009aHET
20HD 240210 b8.33K3 III-0.180.120.120.820.150.155.21501.752.332.332454486.8810.9310.930.150.020.02277.597.777.771.16161.893.493.49Niedzielski et al. 2009bHET
21BD +20 2457 b9.75K2 III-1.000.070.072.81.51.521.42379.632.012.012454677.0328.1928.190.150.030.03207.6421.9921.991.45322.359.579.57Niedzielski et al. 2009bHETdynamical stability unclear
22BD +20 2457 c9.75K2 III-1.000.070.072.81.51.512.47621.9910.2010.202453866.9527.9927.990.180.060.06126.0216.5416.542.01160.037.217.21Niedzielski et al. 2009bHETdynamical stability unclear
23HD 173416 b918526.057G8 III2.00.30.32.70.30.3323.62.22.22453465.88.38.30.210.040.0425411114.38e-50.51e-50.51e-51.160.060.0651.82.02.0 Liu et al. 2009CES (Xinglong); HIDES (Okayama)
2442 Dra b903444.833K1.5 III-0.460.050.050.980.050.053.880.850.85479.16.26.22452757.43.73.70.380.060.06218.710.610.65.29e-80.62e-80.62e-81.190.010.01110.57.07.0Döllinger et al. 2009aTautenburgRV amplitude has changed considerably; see comment in Hrudková et al. 2017
25HD 139357 b763115.977K4 III-0.130.050.051.350.240.249.762.152.151125.79.09.02452466.73.23.20.100.020.02235.410.610.64.79e-70.57e-70.57e-72.360.020.02161.23.23.2Döllinger et al. 2009aTautenburg
2611 UMi b747935.0240.0050.005K4 III0.040.040.041.800.250.2511.202.472.47516.223.253.252452861.042.062.060.080.030.03117.6321.0621.063.61e-70.44e-70.44e-71.540.070.07189.707.157.15Döllinger et al. 2009bTautenburg
27HD 32518 b240036.4360.0050.005K1 III-0.150.040.041.130.180.183.040.680.68157.540.380.382452950.2913.6613.660.010.030.03306.11126.71126.712.20e-80.24e-80.24e-80.590.030.03115.834.674.67Döllinger et al. 2009bTautenburg
28HD 110014 b617404.657K2 III0.142.0913.672.32.3936.444.544.52453842.0206.6206.60.060.090.09119.5584.284.22.50.080.08de Medeiros et al. 2009; Soto et al. 2015FEROS; HARPS; Coraliesecond planet signal could be real
29HD 119445 b668926.30G6 III0.040.180.183.90.40.437.62.62.6410.20.60.62452873.95.65.60.0820.0070.007160.54.34.32.975e-60.058e-60.058e-61.710.060.06413.52.62.6Omiya et al. 2009BOES (BOAO) + HIDES (OAO)
30HD 145457 b792196.574.122K0 III-0.140.090.091.90.30.32.9176.300.390.39245351813130.1120.0350.03530026266.3e-90.86e-90.86e-90.7670.63.13.1Sato et al. 2010HDS (Subaru) + HIDES (OAO)
31HD 180314 b945766.614.312K0 III0.200.090.092.60.30.322396.030.620.622453565.03.13.10.2570.0100.010303.12.32.31.465e-60.046e-60.046e-61.4340.83.33.3Sato et al. 2010HDS (Subaru) + HIDES (OAO)
32gamma1 Leo b505832.01K0 - K4 III-0.510.050.051.230.210.218.781.01.0428.51.251.25245123613.513.50.1440.0460.046206.79.29.21.190.020.02208.34.34.3 Han et al. 2010BOES (Bohyunsan)
33HD 1690 b16929.176.018K1 III-0.320.060.061.090.150.156.10.90.95331.71.72454449550.640.040.04122881.81e-70.84e-70.84e-71.30.020.021902929Moutou et al. 2011HARPSlinear trend -7.2+/- 0.4 m/s
34nu Oph b880483.321.2250.3060.306K0 III+0.060.10.12.720.150.1522.3529.90.10.12452035.02.42.40.1270.0040.0048.900.030.031.286e-61.78288.4Quirrenbach et al. 2011Hamilton (Lick)similar elements by Sato et al. 2012
35nu Oph c880483.321.2250.3060.306K0 III+0.060.10.12.720.150.1524.5318477245307617170.1900.0070.0079.660.040.041.684e-65.89175.4Quirrenbach et al. 2011Hamilton (Lick)similar elements by Sato et al. 2012
36HD 175679 b929686.14G8 III-0.142.70.30.337.31366.85.75.72453263.97.67.60.3780.0080.008346.41.31.36.18e-61.7e-61.7e-63.360.120.12380.23.23.2Wang et al. 2012Xinglong; OAO
37HD 240237 b1148408.19K2 III-0.260.070.071.690.420.425.3745.713.813.82454292.528.328.30.40.10.1108.121.821.81.991.512.812.8Gettel et al. 2012aHET
38BD +48 738 b9.14K0 III-0.200.070.070.740.390.390.91392.65.55.52454457.728.528.50.20.10.1358.931.131.11.031.92.62.6Gettel et al. 2012aHET
39HD 96127 b542327.43K2 III-0.240.100.100.910.250.254.0647.316.816.82453969.931.031.00.30.10.1162.018.218.21.4104.810.610.6Gettel et al. 2012aHET
40BD +20 274 b9.366.169K5 III-0.460.070.070.80.20.24.2578.25.45.42453921.033.233.20.210.060.06108.538.138.11.3121.46.46.4Gettel et al. 2012bHET
41HD 219415 b8.946.421K0 III-0.040.090.091.00.10.11.02093.332.732.72453461.457.757.70.400.090.09207.012.312.33.218.22.22.2Gettel et al. 2012bHET
42epsilon CrB b781594.141.349K2 III-0.0940.0010.0011.70.10.16.70.30.3417.90.50.52451235.339.739.70.110.330.33133.133.333.39.227e-81.3129.42.02.0Lee et al. 2012a BOES (BOAO)
43HD 66141 b393114.391.40.30.3K2 III-0.3230.0340.0341.10.10.16.00.30.3480.50.50.52451320.84.84.80.070.030.0322.13.53.51.545e-71.20.10.1146.22.72.7Lee et al. 2012bBOES (BOAO)
44Kepler-56 b10.2270.0180.018K III0.200.160.161.320.130.130.0470.0470.04710.50342940.000250.000250.10420.001740.00174Steffen et al. 2013Kepler
45Kepler-56 c10.2270.0180.018K III0.200.160.161.320.130.130.200.1970.19721.405050.000360.000360.16760.00280.0028Steffen et al. 2013Kepler
4675 Cet b117915.363.2070.2720.272G3 III:0.000.040.042.490.270.023.0691.93.63.6245221354540.1170.0480.04816528283.95e-50.62e-50.62e-52.138.32.02.0Sato et al. 2012HIDES (Okayama)
47omicron UMa b417043.351.3390.2020.202G4 II-III-0.090.020.023.090.070.074.11630353524534001701700.1300.0650.0655842426.3e-51.2e-51.2e-53.933.62.12.1Sato et al. 2012HIDES (Okayama)
48omicron CrB b750495.512.9340.3220.322K0 III-0.290.030.032.130.230.011.5187.830.540.54245221117170.1910.0850.0857936366.2e-41.6e-41.6e-40.8332.252.82.8Sato et al. 2012HIDES (Okayama)
49kappa CrB b776554.792.4230.2420.242K0 III-IV+0.100.040.041.510.190.191.61251151524518601801800.0730.0490.04921051511.69e-50.25e-50.25e-52.623.61.11.1Sato et al. 2012HIDES (Okayama)
50HD 208527 b1082966.42.2M1 III-0.090.160.161.60.40.49.91.71.7875.55.85.82450745.345.745.70.080.040.04278.019.519.53.375e-72.10.20.2155.43.23.2Lee et al. 2013BOES (BOAO)
51HD 220074 b1152186.42.0M2 III-0.250.250.251.20.30.311.11.81.8672.13.73.72451158.231.731.70.140.050.05323.08.58.58.314e-71.60.10.1230.85.05.0Lee et al. 2013BOES (BOAO)
52BD +15 2940 b784079.056.525K00.280.070.071.10.20.21.1137.480.340.342453464.516160.260.100.1030233330.53942.74.44.4Nowak et al. 2013HET
53HD 233604 b10.297.979K5-0.360.040.041.50.30.36.6192.000.220.22245302277770.050.030.0328143430.747177.84.34.3Nowak et al. 2013HETK5 questionable
54tau Gem b346934.411.6810.2540.254K2 III0.140.10.12.30.30.320.6305.50.10.12453270.714.814.80.0310.00090.0009137.40.30.31.36e-61.17350.2Mitchell et al. 2013Hamilton (Lick)
5591 Aqr b1148554.241.5970.2360.236K0 III-0.030.10.11.40.10.13.2181.40.10.12453472.124.524.50.00270.0260.026177.30.80.81.44e-80.7091.5Mitchell et al. 2013Hamilton (Lick)
56HD 112410 b632426.860.010.014.4060.0160.016G8 III-0.310.090.091.540.050.059.18124.62455376.20.23118.20.565287.5Jones et al. 2013FEROS
57HD 2952 b26115.933.629K0 III0.000.040.042.540.090.121.6311.61.91.7245011254640.1290.0850.0996448565.7e-101.9e-102.7e-101.226.33.43.8Sato et al. 2013HIDES (Okayama)
58HD 120084 b669035.913.572G7 III+0.090.050.052.390.30.064.520823524245077461800.660.100.141179121.4e-80.5e-81.8e-84.3531133Sato et al. 2013HIDES (Okayama)
59omega Ser b775785.214.107G8 III-0.240.020.022.170.290.211.7277.020.510.52245002238270.1060.0690.07913252349.0e-101.8e-102.1e-101.131.82.32.3Sato et al. 2013HIDES (Okayama)
60Kepler-91 b12.88410.1360.0210.021K3 III0.110.070.071.310.100.101.090.200.206.2465800.0000820.0000820.0660.0170.0132501001000.07260.00190.0019931717Lillo-Box et al. 2014Keplerlum. class might be III-IV (R = 6.30 R_Sun)
61Sand 364 b9.86.7K3 III-0.020.040.041.350.050.051.540.240.24121.7100.3050.3052456240.93.73.70.350.080.08273.5112.8112.8167.425.855.85Brucalassi et al. 2014HARPS; Coralie; Sophie; HETmember of M67
62HIP 105854 b1058545.642.9940.2320.232K2 III0.310.180.182.10.10.18.20.20.2184.20.50.52455262.42.42.40.020.030.03343.24.94.90.810.030.03178.110.010.0 Jones et al. 2014FEROS; CHIRON
63eta Cet b53643.460.9220.2500.250K1 III0.070.10.11.70.10.12.550.160.16407.52.72.72454025.030.120.050.05245.49.59.51.2849.4Trifonov et al. 2014Lickdynamically stable 2 planet system; possibly in 2:1 MMR
64eta Cet c53643.460.9220.2500.250K1 III0.070.10.11.70.10.13.260.170.17739.94.84.82454124.910.080.040.0468.222.322.31.9151.6Trifonov et al. 2014Lickdynamically stable 2 planet system; possibly in 2:1 MMR
65HD 14067 b106576.414.0970.0360.036G9 III-0.100.080.082.40.20.29.00.90.9285029043024500928625860.6970.0510.045102.15.35.11.10e-70.15e-70.16e-75.30.40.6100.14.84.9Wang et al. 2014Xinglong; OAO
66Kepler-432 b12.4640.0580.05810.1210.0170.017K2 III-0.020.060.061.350.100.105.840.050.0552.5011340.000070.0001072456841.060.030.030.4780.0040.00468.40.70.70.3030.0070.007294.62.12.1Ortiz et al. 2015; Ciceri et al. 2015; Quinn et al. 2015Kepler; RVsecond planet present
67HIP 67851 b678516.173.7510.2360.236K0 III0.000.100.101.630.220.221.380.150.1588.90.10.12452997.816.716.70.050.040.04138.160.060.00.460.020.0245.51.61.6Jones et al. 2015a; Jones et al. 2015bFEROS; CHIRONupdated orbital parameters after announcement of second planet
68HIP 67851 c678516.173.7510.2360.236K0 III0.000.100.101.630.220.225.980.760.762131.888.388.32452684.1235.7235.70.170.060.06166.520.520.53.820.230.2369.03.33.3Jones et al. 2015bFEROS; CHIRON
69TYC 1422-614-1 b10.217.7280.0310.031K0 III-0.200.080.081.150.180.182.510.120.12198.440.640.64245284340400.070.040.046246460.68790.00150.001582.23.73.7Niedzielski et al. 2015aHRS; HARPS-Ntwo planet system
70TYC 1422-614-1 c10.217.7280.0310.031K0 III-0.200.080.081.150.180.1810.100.140.14569.22.12.1245261730300.0490.0140.01412420201.39160.00330.0033232.83.33.3Niedzielski et al. 2015aHRS; HARPS-Ntwo planet system
71HD 145934 b8.56.1450.0150.015K0 III1.7480.1050.1052.282.262.26273010010024514303703700.0530.0530.05321562624.600.140.1422.92.62.6Feng et al. 2015 HIRES (Keck)
72HIP 65891 b658916.754.4530.0230.023K0 III0.160.100.102.500.210.216.000.490.491084.523.223.22456014.849.349.30.130.050.05355.515.515.52.810.090.0964.92.42.4Jones et al. 2015bFEROS; CHIRON
73HIP 107773 b1077735.623.2920.2500.250K1 III0.030.100.102.420.270.271.980.210.21144.30.50.52456202.312.812.80.090.060.06166.032.632.60.720.030.0342.72.72.7Jones et al. 2015bFEROS; CHIRON
74BD +49 828 b9.380.020.026.5710.0210.021K0 III-0.190.060.061.520.220.221.60.20.425901803002455479.51702000.350.100.2417030324.20.200.3218.82.06.2Niedzielski et al. 2015bHET
75HD 95127 b537338.150.010.015.0220.0180.018K0 III-0.180.050.051.200.220.225.010.440.61482552453200.550500.110.060.154040371.280.010.01116916Niedzielski et al. 2015bHET
76HD 216536 b9.230.020.026.4960.0180.018K0 III-0.170.090.091.360.380.381.470.120.20148.60.70.72453587.511110.380.100.1227020210.6090.0020.0025048Niedzielski et al. 2015bHET
77HD 155233 b840566.8134.4930.0360.036K1 III+0.100.070.071.500.200.202.00.50.5885636324551124124120.030.200.209590902.070.100.1032.28.78.7Wittenmyer et al. 2016aUCLESlinear trend 15.4+/-6.5 m/s/yr
78HD 11755 b92426.873.7600.2800.280G5 III-0.740.020.020.90.10.16.51.01.0433.73.23.22457018.214.014.00.190.100.10155.312.612.61.080.040.04191.310.210.2Lee et al. 2015BOES (BOAO)
79HD 12648 b108006.984.7430.0310.031G5 III-0.570.020.021.20.10.12.90.40.4133.60.50.52452324.757.657.60.040.160.1699.3140.7140.70.540.020.02102.08.48.4Lee et al. 2015BOES (BOAO)
80HD 24064 b184516.753.1300.3940.394K0 III-0.490.060.061.00.10.19.41.31.3535.63.03.02455278.311.811.80.350.080.08250.86.36.31.290.050.05251.09.39.3Lee et al. 2015BOES (BOAO)
818 UMi b731366.834.5150.0200.020K0 III-0.030.020.021.80.10.11.50.20.293.44.54.52454108.522.822.80.060.180.1891.084.684.60.490.030.0346.14.04.0Lee et al. 2015BOES (BOAO)
82HD 33844 b242757.294.9450.0180.018K0 III0.270.090.091.780.180.181.920.110.11547.96.46.42454578.50500.160.070.0719062621.590.010.0132.92.22.2Wittenmyer et al. 2016bAAT; Keck; FEROS2 planet system in 5:3 MMR
83HD 33844 c242757.294.9450.0180.018K0 III0.270.090.091.780.180.181.680.160.16924.332.532.52454356.2812810.090.080.08530302.250.030.0324.02.22.2Wittenmyer et al. 2016bAAT; Keck; FEROS2 planet system in 5:3 MMR
84HD 11343 b85417.885.2900.0290.029K2 III/IV-0.150.080.081.170.280.285.51.01.01560.253.953.92459346.993.493.40.160.060.06293.915.215.22.80.250.2587.46.46.4Jones et al. 2016CHIRON; FEROS; UCLES
85HD 135760 b748907.054.6390.0160.016K1 III+0.200.130.131.740.210.212.40.30.3822.316.816.82459820.4379.8379.80.070.070.07181.993.993.92.10.090.0936.52.72.7Jones et al. 2016FEROS; UCLES
86HD 155233 b840566.814.4930.0360.036K1 III+0.080.070.071.690.140.142.60.30.3818.812.112.12460282.0192.1192.10.040.040.04120.071.971.92.00.060.0640.53.13.1Jones et al. 2016CHIRON; FEROS
87HD 181342 b951247.555.2510.0200.020K0 III+0.200.080.081.890.110.112.90.20.2562.16.06.02459915.554.354.30.100.070.07311.835.835.81.650.040.0446.51.81.8Jones et al. 2016CHIRON; FEROS; UCLES
88HD 5583 b7.65.2210.0200.020K0 III-0.500.180.181.010.10.15.780.530.53139.350.220.212456021.517180.0760.0230.0701263300.530.020.02225.84.04.5Niedzielski et al. 2016aHET; HARPS-N (Tapas)
89BD +15 2375 b10.317.7180.0170.017-0.220.080.081.080.140.141.0610.270.27153.220.440.442457680.56307000.0010.0010.2555172400.5760.0270.02738.31.02.3Niedzielski et al. 2016aHET; HARPS-N (Tapas)
90TYC 3667-1280 b9.867.1000.0170.017-0.080.050.051.870.170.175.40.40.426.4680.0050.0052456320.13.33.70.0360.0140.04324050500.210.010.01242.41.21.0Niedzielski et al. 2016bHET; HARPS-N (Tapas)
91HD 47366 b316746.114.0550.2900.290K1 III-0.020.090.091.810.130.131.750.170.20363.32.42.52450122.55710.0890.0600.079100.71.100.1.2140.0290.03033.62.83.6Sato et al. 2016HIDES (Okayama); Xinglong; AATmultiple system; possibly retrograde
92HD 47366 c316746.114.0550.2900.290K1 III-0.020.090.091.810.130.131.860.150.16684.74.95.02450445.62.55.0.2780.0940.067132.20.17.1.8530.0450.04530.12.02.1Sato et al. 2016HIDES (Okayama); Xinglong; AATmultiple system; possibly retrograde
93EPIC 211351816.01 b12.6110.0310.03110.0350.0210.021K III+0.380.080.081.160.120.121.100.110.118.40800.00020.00022457416.8080.0070.00710388Grunblatt et al. 2016K2, Keck, APFinflated hot Jupiter
94nu Oct b1070893.7430.0150.0151.4580.3060.306K1 III/IV+0.180.040.041.612.110.020.02414.82.63.62452136.0.0860.0360.043350.25.8.1.2760.0050.00738.741.20.9Ramm et al. 2009; Ramm et al. 2016HERCULES, Mt. John Observatoryplanet in 2.6 AU spectroscopic binary; dynamical fit
95HD 59686 Ab366165.452.9220.3000.300K2 III0.150.10.11.90.20.26.920.240.18299.360.310.262451531.060.050.020.03121.24281.08600.00070.0006136.94.63.8Ortiz et al. 2016Hamilton (Lick)planet in 13.6 AU spectroscopic binary; dynamical fit
96HD 175370 b926687.190.010.014.2240.0170.017K2 III-0.520.070.071.020.160.164.20.70.7347.73.13.12456276.38380.150.100.10171.37.37.0.980.050.05122.13.13.Hrudková et al. 2017Tautenburg and HERMES/MercatorKepler; masses are for the RGB phase; 22 AU spectroscopic binary
97HD 86950 b491297.460.010.015.0380.0180.018K1 III0.040.100.101.660.250.253.60.70.71270.57.57.2454245.161.161.0.170.160.16243.70.70.2.720.080.0849.12.12.Wittenmyer et al. 2017AAT; FEROS; CHIRON
98HD 222076 b1166307.475.1270.0270.027K0 III0.050.100.101.070.250.251.560.110.11871.19.19.2454264.189.189.0.080.050.05241.60.60.1.830.030.0331.92.32.3Wittenmyer et al. 2017AAT; FEROS; CHIRON
99HD 120457 b675376.440.0050.0054.1960.0360.036K1 III0.150.080.082.410.160.1611.10.60.62592.5116.1116.12456293.329.929.90.590.040.04120.75.35.32.2e-74.960.240.24113.24.04.0Jones et al. 2017FEROS; CHIRONupper mass limit 0.22 M_Sun from astrometry


e-mail: sreffert@lsw.uni-heidelberg.de