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Table 1.

Sample of HARPS low-mass binary candidates.

ID Sp. Type N MG BP − RP
46 Cet K2III 9 −0.232 1.408
66 Vir K2V 27 3.509 0.563
BD-06 6318 M2.5Vk 9 8.884 2.330
BD-19 4341 K0IV 9 2.767 0.887
BO Mic K3V(e) 11 5.382 1.190
CD-23 16484 K6.5V 9 7.341 1.627
CD-29 4446 M1Ve 17 8.268 2.136
CD-31 18409 K6+Vk: 27 7.366 1.616
CD-32 7774 K0 12 5.445 1.017
CD-35 15144 K3V 28 6.073 1.220
CD-40 14067 K6.5Vk: 30 7.509 1.662
CD-42 862 K0 8 6.230 1.166
CD-45 7872 M1.0 12 8.556 2.243
HD 3221 K4Ve 13 5.867 1.461
HD 4457 K2V 44 6.098 1.160
HD 22663 K1III 10 −0.218 1.226
HD 24706 K2III 8 0.359 1.363
HD 49050 K2/3(III) 20 −0.929 1.360
HD 49091 K3III 13 −3.403 1.418
HD 49334 K1III 10 −1.207 1.248
HD 96118 K3III+A/F 8 −3.932 1.169
HD 101886 K1III 10 −0.608 1.103
HD 11938 K4Vk: 31 6.427 1.354
HD 127124 K0V 33 5.814 1.108
HD 138799 K1/2(V) 41 5.463 0.993
HD 139084 K0V 14 4.678 0.967
HD 160346 K3-V 94 5.999 1.174
HD 178445 K6.5V 13 7.223 1.644
HD 191797 K0V 39 5.995 1.092
HD 211188 K2V 20 5.887 1.083
HD 219630 K6+Vk: 16 7.234 1.639
KW Lup K2V 23 5.933 1.330
L 440-30 M2.5+V 24 14.491 1.046
L 590-10 M1 13 8.247 1.952
PM J21214-6655 K7V 29 7.485 1.830
PX Vir K1V 21 5.737 1.062
Ross 193 M3Vnne 8 9.605 2.696
Wolf 359 M6Ve 72 14.128 4.185
Wolf 414 M4V 11 10.156 2.777
Wolf 1051 M3.0Ve 9 9.511 2.528
WW PsA M4IVe 28 9.143 2.775

Notes. The columns (from left to right) correspond to the star ID, the spectral type, the number of HARPS spectral observations N, the absolute magnitude MG (obtained from Gaia DR3; Gaia Collaboration 2023), and the color index BP − RP (Gaia mission).

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