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Table A.2

Best-fit models in a linear-combination fit with filling factors and the difference ΔICa IRT of the models.

Stars Inactive model More active model ΔICa IRT
Model Filling factor Model Filling factor (Å)
Wolf 1056 #047 0.8 #050 0.2 1.02 0.047
GJ 47 #047 0.81 #050 0.19 0.86 0.047
BD+70 68 #047 0.4 #080 0.6 1.18 0.033
GJ 70 #079 0.72 #049 0.28 1.18 0.067
G 244-047 #042 0.66 #049 0.34 1.08 0.071
VX Ari #079 0.66 #049 0.34 2.04 0.067
Ross 567 #042 0.73 #049 0.27 1.25 0.071
GJ 226 #047 0.92 #064 0.08 0.66 0.189
GJ 258 #047 0.87 #064 0.13 1.08 0.189
GJ 1097 #042 0.63 #049 0.37 1.29 0.071
GJ 3452 #042 0.76 #049 0.24 1.22 0.071
G 234-057⋆ #080 0.9 #139 0.1 3.58 0.389
GJ 357 #042 0.74 #049 0.26 1.24 0.071
GJ 360⋆ #080 0.82 #132 0.17 5.13 0.215
GJ 386 #047 0.81 #050 0.19 1.21 0.047
LP 670-017 #042 0.49 #080 0.51 2.23 0.039
GJ 399 #079 0.8 #065 0.2 1.31 0.093
Ross 104 #079 0.71 #049 0.29 1.46 0.067
LP 733-099⋆ #079 0.68 #149 0.32 16.13 0.598
Ross 905 #042 0.7 #049 0.3 1.05 0.071
GJ 443 #047 0.37 #080 0.63 1.09 0.033
Ross 690 #079 0.82 #065 0.18 1.39 0.093
Ross 695 #042 0.73 #049 0.27 1.41 0.071
Ross 992 #079 0.68 #049 0.32 1.43 0.067
θ Boo B #047 0.8 #050 0.2 0.83 0.047
Ross 1047 #047 0.88 #064 0.12 1.01 0.189
LP 743-031 #047 0.43 #080 0.57 2.12 0.033
G 137-084 #029 0.39 #080 0.61 1.39 0.038
EW Dra #047 0.44 #080 0.56 0.96 0.033
GJ 625 #042 0.74 #049 0.26 1.02 0.071
GJ 1203 #047 0.81 #050 0.19 0.98 0.047
LP 446-006 #047 0.8 #050 0.2 1.08 0.047
Ross 863 #079 0.8 #060 0.2 1.87 0.102
GJ 2128 #042 0.75 #049 0.25 1.13 0.071
GJ 671 #042 0.7 #049 0.3 1.44 0.071
G 204-039 #029 0.36 #080 0.64 1.73 0.038
TYC 3529-1437-1⋆ #079 0.75 #149 0.25 14.25 0.598
Ross 145 #042 0.69 #049 0.31 1.27 0.071
G 155-042 #042 0.68 #049 0.32 1.44 0.071
Ross 730 #029 0.8 #049 0.2 1.89 0.070
HD 349726 #029 0.8 #049 0.2 1.91 0.070
GJ 793 #112 0.22 #080 0.78 1.93 0.050
Wolf 896 #047 0.89 #064 0.11 0.67 0.189
Wolf 906 #079 0.79 #065 0.21 1.09 0.093
LSPM J2116+0234 #079 0.78 #060 0.22 1.54 0.102
Wolf 926 #047 0.79 #050 0.21 1.05 0.047
BD-05 5715 #047 0.43 #080 0.57 1.66 0.033
Wolf 1014 #042 0.7 #049 0.3 1.43 0.071
G 273-093 #047 0.85 #050 0.15 0.92 0.047
Wolf 1051 #042 0.32 #080 0.68 1.44 0.039

Notes. The line of Na I D 2 and the bluest Ca II IRT line are weighted by a factor of 12 compared to Hα as described in Sect. 4.1. Asterisks identify active stars in the stellar sample. The combinations for GJ 360 and TYC 3529-1437-1 are illustrated in Fig. 12.

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