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Table A.2

Results for the 89 stars of our HARPS RV survey.

Stellar characteristics Survey results.
Name HIP ST TBL Nm RV BVS RV- ⟨FWHM⟩ ⟨ log ⟩ V
HD /BD/CD BVS
A rms ⟨U⟩ A rms ⟨U⟩ corr.
(day) (ms −1) (ms −1) (km s−1)
HD 105 490 G0V 4606 36 236.8 61.1 4.2 310.7 9.8 72.9 −0.67 22.6 −4.316 A
HD 984 1134 F7V 867 21 301.9 84.6 16.4 571.8 38.2 137.4 −0.46 59.7 −4.368 A
HD 987 1113 G8V 2621 19 502.6 116.8 2.5 393.6 6.4 103.1 −1.08 13.0 −4.088 A
HD 1466 1481 F8V 4400 19 135.8 39.6 7.4 189.8 17.6 55.9 −0.66 32.3 −4.344 A
HD 3221 2729 K4V 4014 5 4793.4 1794.3 68.6 3115.1 172.5 1447.8 −0.54 203.6 −4.474 −
HD 6569 5191 K1V 8 4 24.0 11.4 1.5 17.8 3.8 7.5 −1.49 9.6 −4.228 A
HD 7661 5938 K0V 1525 29 96.0 28.1 1.2 50.5 3.3 12.5 −1.42 9.2 −4.325 A
HD 10008 7576 K0V 4021 17 20.5 6.2 1.0 17.5 2.7 5.2 0.44 7.5 −4.358 A
HD 16765 12 530 F71V 926 27 173.0 47.2 11.0 402.9 27.9 93.1 −0.42 48.5 −4.475 A
HD 17925 13 402 K1V 1470 40 113.6 30.5 1.1 58.7 3.1 17.4 −0.87 10.0 −4.310 A
HD 18599 13 754 K2V 1055 16 115.9 38.9 1.5 54.3 3.9 17.6 −1.46 9.8 −4.310 A
HD 19668 14 684 K0V 4402 20 143.1 33.2 1.8 91.9 4.7 26.0 −0.95 11.8 −4.284 A
HD 24916 18 512 K4V 792 22 24.3 7.4 0.8 36.7 2.2 11.6 0.46 7.8 −4.536 A
HD 25457 18 859 F6V 4089 78 187.2 49.5 3.3 345.4 7.7 60.2 −0.66 28.2 −4.355 A
HD 26923 19 859 G0IV 4010 47 50.2 12.7 1.1 24.7 3.1 5.6 1.12 8.0 −4.487 A
HD 29391 21 547 F0IV 3996 81 1476.1 326.2 28.4 2564.3 72.1 487.8 − 101.4 P
HD 30447 22 226 F3V 792 19 194.1 47.2 47.7 7048.7 106.6 1728.3 − 120.7 −4.447 P
HD 35650 25 283 K6V 1195 13 48.3 15.3 1.2 43.6 3.0 12.3 −0.67 9.4 −4.359 A
HD 37572 26 373 K0V 2826 34 347.1 75.4 1.7 223.6 4.4 52.8 −1.28 15.6 −4.165 A
HD 39060 27 321 A6V 3702 5108 755.5 341.4 58.9 − P
HD 41593 28 954 K0V 1194 15 69.5 19.8 1.1 59.4 2.9 16.7 −0.66 9.1 −4.370 A
HD 43989 30 030 G0V 4433 17 819.0 238.6 15.6 743.7 34.3 197.6 −0.83 64.2 −4.209 A
HD 44627 30 034 K1V 4892 23 670.6 177.7 3.2 428.6 8.1 110.9 − 19.1 −4.018 A
HD 45081 29 964 K4V 4020 17 852.4 252.1 5.0 911.0 13.0 246.9 − 24.8 −3.887 A
HD 45270 30 314 G1V 2827 19 137.4 51.8 3.1 193.3 8.4 59.2 −0.76 27.6 −4.335 A
HD 59967 36 515 G3V 1065 25 65.3 19.7 1.4 41.6 3.6 10.5 −0.99 9.0 −4.328 A
HD 61005 36 948 G8V 2369 33 186.5 48.8 2.5 127.4 6.3 32.7 −1.16 14.5 −4.261 A
HD 63608 37 923 K0V 1069 36 80.7 22.2 1.1 49.1 3.0 11.7 −0.63 8.0 −4.323 A
HD 77825 44 526 K2V 283 6 47.0 18.3 1.4 46.5 3.4 14.9 −1.09 9.6 −4.314 A
HD 82558 46 816 K1V 1092 24 296.0 79.7 7.1 475.6 17.5 124.1 −0.43 42.0 −3.990 A
HD 89449 50 564 F6IV 1227 28 129.9 41.4 4.3 351.6 9.1 113.6 −0.26 25.3 −4.971 A
HD 90905 51 386 F5V 2551 24 125.6 40.8 1.9 187.7 5.0 49.0 −0.74 15.0 −4.345 A
HD 92945 52 462 K1V 4533 38 182.3 40.5 1.5 86.2 3.9 23.8 −1.37 10.3 −4.261 A
HD 95086 53 524 A8III 1532 103 1279.0 268.8 14.8 2594.0 36.3 511.1 − 45.4 P
HD 95650 53 985 M2V 4046 12 23.8 7.6 3.1 46.1 7.3 13.6 − 8.0 −4.330 −
HD 99211 55 705 A7V 3068 112 818.0 149.4 86.8 49 704.0 214.7 5222.3 − 183.4 P
HD 102458 57 524 G4V 2964 26 988.5 307.7 10.0 1358.4 23.8 431.7 − 43.6 −3.994 A
HD 103743 58 241 G4V 1065 30 102.2 32.1 2.6 141.6 6.6 35.1 −0.79 14.9 −4.308 A
HD 105690 59 315 G5V 2975 133 269.4 61.3 2.3 193.7 5.4 44.0 −0.91 15.1 −4.276 A
HD 106906 59 960 F5V 1230 46 5290.4 1285.7 32.9 9949.8 83.3 2272.4 − 74.0 −4.574 B
HD 108767 60 965 K0V 1201 18 47.9 12.4 0.7 25.3 2.0 7.7 0.21 8.2 −4.381 A
HD 116434 65 426 A2V 439 58 6273.2 1223.2 1235.6 − P
HD 118100 66 252 K5V 720 10 534.7 155.6 6.4 139.5 15.6 43.0 −3.48 16.5 −4.108 A
HD 131399 72 940 A1V 189 87 19 478.2 6381.7 16.4 1287.6 39.3 237.0 − 43.1 B
HD 141943 − G2V 2648 58 861.4 222.8 10.3 1169.7 25.3 269.6 −0.66 53.0 −4.025 A
HD 146464 79 958 K3V 51 5 872.1 352.1 5.0 546.2 12.3 220.6 −1.55 25.8 −4.163 A
HD 146624 79 881 A0V 4762 335 232.7 39.8 29.2 70 472.6 72.9 6163.4 − 65.1 P
HD 152555 82 688 F8V 1135 22 225.0 64.8 6.1 283.2 15.9 69.9 −0.74 26.3 −4.294 A
HD 159492 86 305 A5IV 4751 90 612.4 124.9 20.8 2413.2 52.1 359.7 − 79.4 P
HD 164249 88 399 F6V 1113 25 56.9 14.6 6.9 134.2 17.0 36.7 −0.24 29.8 −4.765 A
HD 169178 − K0V 1123 19 354.7 135.7 1.8 85.6 4.7 25.0 − 10.7 −4.234 A
HD 171488 91 043 G2V 1111 18 2190.4 717.7 13.1 2249.5 33.2 680.4 −1.0 58.2 −3.988 A
HD 172555 92 024 A7V 2975 262 1883.8 329.6 70.6 94 415.3 185.8 6148.5 − 172.4 P
HD 174429 92 680 G9IV 4572 42 3362.3 970.2 26.0 1167.7 60.0 320.7 −1.77 109.9 A
HD 177171 93 815 F6V 144 21 21 233.2 5931.1 53.4 − −4.047 B
HD 181321 95 149 G2V 3757 28 2610.2 683.2 3.9 244.0 9.6 59.1 − 19.5 −4.243 B
HD 181327 95 270 F6V 3496 56 63.1 16.3 3.8 156.8 9.0 30.6 −0.26 28.8 −4.577 A
HD 183414 96 334 G3V 3097 68 247.9 63.6 2.4 214.0 6.2 58.3 −1.01 16.0 −4.236 A
HD 186704 97 255 G0V 451 4 345.8 168.8 4.7 77.1 11.9 29.3 − 22.3 −4.308 T
HD 188228 98 495 A0V 4315 194 1398.7 319.2 150.2 211 414.9 368.1 18 294.0 − 148.0 P
HD 189245 98 470 F7V 4285 46 646.2 119.4 21.0 5149.4 43.1 757.5 − 104.2 −4.304 P
HD 191089 99 273 F5V 1025 26 107.1 22.8 15.7 300.0 37.3 78.4 − 57.0 −4.526 P
HD 197481 102 409 M1V 5619 55 667.6 144.0 3.2 470.1 8.0 101.2 −1.37 16.2 −4.289 A
HD 197890 102 626 K3V 13 3 922.1 376.6 85.2 3975.6 217.1 1713.8 − 216.2 −4.277 −
HD 202917 105 388 G7V 4438 20 436.1 124.6 5.0 438.1 12.4 134.8 −0.84 23.0 −3.984 A
HD 206860 107 350 G0V 1332 22 122.1 35.8 2.8 180.9 6.7 51.4 − 16.1 −4.387 A
HD 206893 107 412 F5V 542 15 185.6 45.5 10.8 361.3 21.3 68.2 − 50.7 −4.630 P
HD 207575 107 947 F6V 2391 39 227.6 49.3 9.5 389.5 19.9 97.6 − 49.1 −4.332 P
HD 213845 111 449 F7V 4436 79 220.4 44.2 9.6 454.3 25.8 82.6 − 52.3 −4.703 P
HD 215641 112 491 G8V 1639 78 101.5 20.5 1.2 84.4 3.4 12.2 0.22 8.3 −4.460 A
HD 216956 113 368 A3V 4929 834 382.4 44.3 27.0 − P
HD 217343 113 579 G5V 2727 26 276.6 96.9 2.7 298.7 6.6 85.6 −1.08 19.3 −4.215 A
HD 217987 114 046 M2V 5109 130 63.8 18.5 0.9 39.5 2.3 8.2 0.95 5.8 −4.899 A
HD 218396 114 189 A5V 2727 124 3616.3 924.5 38.5 7376.0 95.5 2191.3 − 62.3 P
HD 218860 114 530 G8V 1137 18 137.1 36.2 2.1 82.8 5.4 18.6 −1.3 11.7 −4.240 A
HD 221575 116 258 K2V 869 16 45.7 12.2 1.4 33.4 3.7 12.0 −0.54 8.8 −4.438 A
HD 223340 − K1V 868 10 54.4 17.3 1.7 42.2 4.4 10.7 −1.34 9.8 −4.337 A
HD 224228 118 008 K2V 2815 31 35.4 8.8 1.0 31.5 2.8 7.5 0.32 7.8 −4.356 A
− 6276 G9V 1201 20 95.6 27.3 1.6 91.0 4.2 27.6 −0.65 9.4 −4.321 A
− 116 384 K7V 733 8 104.3 41.2 1.7 60.2 4.5 19.2 −1.18 8.6 −4.455 A
− 17 157 K7V 1457 6 67.5 22.3 1.4 37.1 3.6 14.9 − 8.1 −4.577 A
− 23 309 M0V 4030 16 245.4 64.1 2.3 116.1 5.9 33.0 −1.83 11.7 −3.816 A
− 31 878 K7V 435 11 84.3 31.6 1.6 48.3 4.1 16.1 −1.86 8.5 −4.276 A
− 36 985 M2V 789 20 670.1 247.4 2.1 58.8 5.4 14.7 − 8.1 −4.316 B
− 44 722 K7V 90 4 8.0 3.4 1.5 10.7 3.8 4.0 −0.49 7.6 −4.550 A
− 46 634 G5V 281 3 38.2 16.1 1.4 32.6 3.5 13.9 −1.0 9.8 −4.321 A
− 51 317 M2V 4541 139 17.7 3.6 1.2 24.5 3.2 3.5 −0.38 4.8 −5.032 A
BD+20 2465 − M5V 3983 40 63.5 16.1 1.2 33.6 3.1 6.5 −0.61 6.7 −4.026 A
CD-46 1064 − K3V 1185 12 477.8 134.9 8.7 211.2 21.6 68.7 −1.53 17.4 −4.204 A

Notes. Spectral type (ST) are taken from the CDS database. The survey results include the time baseline (TBL), the number of computed spectra Nm, the amplitude corresponding to the difference between the maximum and the minimum of the RV(A), rms and mean uncertainty ⟨U⟩ on the RV and BVS measurements, the RV−BVS correlation factor (slope of the best linear fit), the mean FWHM (⟨FWHM⟩), and the mean log (⟨ log ⟩). V stands for the dominant source of RV variations, with A for stellar activity (spots), P for pulsations, B for binary and, T for long-term trend.

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