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Table 3

Stars with X-ray activity level and derived rotation periods.

Name Spectral typea Teff log Lx log LxLbol Derived Prot
(K) (erg s−1) (days)
TYC 2710-691-1 −0.5 3867 ± 71 28.89 ± 0.12 − 3.61 ± 0.15 34.0 ± 6.0
GJ 9793 0.0 3881 ± 70 28.80 ± 0.18 − 3.82 ± 0.24 15.0 ± 3.0
NLTT 53166 0.0 3832 ± 70 28.58 ± 0.08 − 3.80 ± 0.12 55.0 ± 9.0
TYC 3720-426-1 0.0 3822 ± 70 29.18 ± 0.08 − 3.29 ± 0.17 8.0 ± 1.0
GJ 272 1.0 3747 ± 68 27.50 ± 0.21 − 4.71 ± 0.23 41.0 ± 7.0
GJ 895 1.5 3748 ± 68 27.20 ± 0.21 − 5.07 ± 0.23 24.0 ± 5.0
GJ 3014 1.5 3695 ± 69 27.95 ± 0.11 − 4.20 ± 0.15 24.0 ± 5.0
GJ 414B 2.0 3661 ± 68 27.52 ± 0.23 − 4.65 ± 0.24 62.0 ± 10.0
GJ 3117A 2.5 3549 ± 68 27.23 ± 0.19 − 4.78 ± 0.21 22.0 ± 4.0
GJ 70 2.5 3511 ± 68 27.41 ± 0.03 − 4.46 ± 0.14 46.0 ± 8.0
GJ 26 2.5 3484 ± 68 27.18 ± 0.17 − 4.66 ± 0.23 27.0 ± 5.0
GJ 408 2.5 3472 ± 68 26.93 ± 0.21 − 4.86 ± 0.26 58.0 ± 10.0
GJ 2128 2.5 3518 ± 68 27.60 ± 0.18 − 4.21 ± 0.24 85.0 ± 15.0
GJ 793 3.0 3461 ± 68 27.77 ± 0.03 − 3.99 ± 0.18 34.0 ± 6.0

Notes. Rotation values are from Suárez Mascareño et al. (2018), while Lx and Lbol values are computed in this work. (a)Spectral type = − 0.5–3.0 corresponds to K7.5–M3.0 spectral types.

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