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Table A.2

Multi-wavelength properties of the 144 MHz detected V-LoTSS × GCNS population sorted by increasing distance d. The symbols GBPGRP, SV, SV/SI, and log LX correspond to Gaia BP-RP colour, Stokes V flux density, fraction of circularly polarised radio emission, and logarithmic soft (0.1-2.4 keV) X-ray luminosity, respectively.

Common name Object(a) type Spectral type d(b) (pc) GBPGRP (b) (mag) SV (c) (mJy) SV /SI (c) (%) log LX(d) (erg s−1)
WX UMa Eruptive* M6V(1) 4.91 3.85 −0.86 ± 0.10 40 ± 9 27.56
GJ 1151 * M4.5V(2) 8.04 3.14 0.53 ± 0.07 40 ± 8 26.30(23)
GJ 450 * M1.5V(3) 8.77 2.16 0.40 ± 0.06 54 ± 23 27.82
LP 169-22 * M5.5V(4) 10.47 3.81 −0.64 ± 0.13 60 ± 29 < 26.48(23)
CW UMa Eruptive* M3.5V(5) 13.35 2.69 −1.53 ± 0.14 77 ± 10 28.76
YY Gem RS CVn M1Ve+M1Ve(6) 15.08 1.93 −0.87 ± 0.13 47 ± 10 29.88
HAT 182-00605 * M4V(7) 17.90 2.92 −0.73 ± 0.11 82 ± 25 28.53
LP 212-62 * M5V(8) 18.19 3.40 −6.63 ± 0.13 75 ± 3 27.58(23)
GJ 3861 Eruptive* M3.5V(9) 18.46 2.44 0.73 ± 0.08 79 ± 16 28.53
CR Dra * M1.5Ve(10) 20.15 2.17 0.34 ± 0.07 56 ± 26 29.56
σ2 CrB (TZ CrB) RS CVn F6V+G0V(11) 22.70 0.81 −6.07 ± 0.19 81 ± 4 30.71
BF Lyn BY Dra K3V+K3V(12) 23.44 1.24 1.37 ± 0.15 72 ± 13 30.22
GJ 3729 * M3.5V(13) 23.51 2.76 −1.61 ± 0.17 113±18 28.88
2MASS J09481615+5114518 * M4.5V(14) 35.97 3.53 1.86 ± 0.09 94 ± 8 27.45(23)
σ Gem RS CVn K1IIIe+dG/K(15) 36.87 1.35 1.27 ± 0.26 45 ± 13 31.07
LP 259-39 * M4V(16) 36.91 3.25 −0.39 ± 0.06 71 ± 24 < 29.27(23)
II Peg RS CVn K2IV+M0–3V(17) 39.12 1.38 2.66 ± 0.14 71 ± 8 31.17
2MASS J10534129+5253040 * M4V(18) 45.08 2.78 −0.86 ± 0.14 83 ± 25 29.45
BH CVn (HR 5110) RS CVn F2IV+K2IV(19) 46.89 0.65 1.12 ± 0.09 54 ± 11 30.75
2MASS J14333139+3417472 * M5V(20) 48.21 3.75 0.96 ± 0.11 65 ± 11 27.92(23)
EV Dra RS CVn G5V+K0V(21) 57.54 0.94 −2.59 ± 0.15 85 ± 9 30.44
HD 220242 * (F-type) F5V(22) 69.33 0.54 2.19 ± 0.29 78 ± 16 29.00

Notes. (a) Asterisks * denote M dwarfs unless specified otherwise. Eruptive* denotes eruptive variable stars classified by SIMBAD. (b) Distance d (derived from the parallaxes) and Gaίa colour GBP – GRP of each stellar systems are given by the Gaia Catalogue of Nearby Stars (Gaia Collaboration 2021b), which quotes measurements from Gaίa Early Data Release 3 (Gaia Collaboration 2021a). (c) Stokes V flux density SV and fraction of circularly polarised radio emission SV/SI are given by the V-LoTSS catalogue (Callingham et al. 2023). (d) X-ray luminosity XL of each stellar system is given by the Second ROSAT all-sky survey source catalogue (2RXS; Boller et al. 2016), unless specified otherwise. The derivation of the XL upper limit values for some stellar systems in our sample is described in detail in Callingham et al. (2021b).

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