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Table 1

Stellar parameters of the investigated sources.

RA (J2000) Dec (J2000) Gaia-DR3 Teff (K) log g [Fe/H] v sin i (km s−1) SpT Sub(a) N(b) < RV > (km s−1) Prot(c) (d) Rem.
58.615971 21.389748 51742471745296768 5624±111 4.40±0.11 −1.12±0.11 ≤8 G5V C 1 8.66±0.47 4.5480R ...
59.845396 22.571372 53335045618385536 4360±42 4.66±0.04 0.01±0.05 ≤8 K4V C 12 5.35±3.59 1.8839R RVvar
53.274270 22.134250 61554650949438208 5196±58 4.54±0.08 0.00±0.09 ≤8 K1V C 1 6.87±0.62 5.7660R ...
57.925378 21.668355 63730309584280960 5222±45 4.46±0.11 −1.02±0.07 ≤8 K0IV C 10 7.04±1.33 5.4447R RVvar
58.644969 21.883909 63795455648004608 3918±44 4.65±0.05 −1.15±0.06 9.0±1.7 K8V C 13 3.56±2.16 2.7745R RVvar
57.849460 22.113383 63849572235829248 4640±38 4.62±0.05 −1.03±0.06 ≤8 K3.5V C 2 6.83±0.49 6.4306R ...
58.470090 22.418532 63876402894075904 ... ... ... ... ... C ... ... 6.3353R SB2
56.892334 21.746810 63916431989200256 4956±48 4.56±0.05 −1.07±0.06 36.5±1.7 K2.5V C 2 8.07±0.46 7.5554R ...
57.399503 22.151421 63958801843006208 4052±74 4.68±0.11 −1.03±0.10 66.3±2.9 K6V C 1 3.38±1.84 0.2471R ...

Notes. The full table is available at the CDS. (a)Subsample the target belongs to: C=Cantat; H=Hunt; R=Rebull. (b)N is the number of observation epochs. (c)The rotation periods reported by Rebull et al. (2016) are flagged with R; those measured in this work with TESS data are indicated with T.

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