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Table 1

Fundamental parameters of the stars in the sample.

Star SpT Te f f (K) (G) B(S) (mag) V(S) (mag) 2MASS-KS (mag) θLD (mas) ref. θLD
GJ 1 (*) M2V 3355 10.02 8.61 4.50 0.812 ± 0.005 2
GJ 15 A (*) M2V 3352 10.12 8.13 4.02 1.005 ± 0.005 1
GJ 79 M0V 10.32 8.88 5.18
GJ 169 M0.5V 3815 9.69 8.30 4.88
GJ 176 M2.5V 11.49 9.95 5.61 0.452 ± 0.020 2
GJ 205 (*) M1.5Ve 9.44 7.84 4.04 0.943 ± 0.004 1
GJ 229 M1V 9.61 8.13 4.17
GJ 273 (†) M3.5V 3024 11.44 9.87 4.86 0.763 ± 0.010 2
GJ 338 B (†) M0V 9.05 7.63 4.14 0.856 ± 0.016 1
GJ 393 (*) M2V 3291 11.15 9.63 5.31 0.564 ± 0.021 4
GJ 406 (*) M6Ve 15.54 13.51 6.08 0.582 ± 0.020 2
GJ 411 (†) M2+V 3511 8.96 7.52 3.34 S 1.432 ± 0.013 1
GJ 412 A (†) M1V 3382 10.27 8.80 4.77 0.764 ± 0.017 1
GJ 447 (*) M4V 3093 12.91 11.11 5.65 0.524 ± 0.029 2
GJ 488 M0V 3738 9.89 8.47 4.88
GJ 526 (*) M2V 3425 9.89 8.49 4.42 0.835 ± 0.014 1
GJ 536 M0V 3638 11.18 9.71 5.68
GJ 551 (*) M5.5Ve 2829 12.95 11.01 4.38 1.103 ± 0.007 2
GJ 570 B M1.5V 9.56 8.07 3.80
GJ 581 (*) M3V 3110 12.14 10.56 5.84 0.476 ± 0.007 2
GJ 628 (†) M3V 11.64 10.07 5.08 0.661 ± 0.014 2
GJ 674 (*) M3V 3275 10.97 9.41 4.86 0.737 ± 0.037 2
GJ 687 (*) M3V 3192 10.65 9.15 4.55 0.859 ± 0.014 1
GJ 699 (†) M4V 3099 11.24 9.51 4.52 1.004 ± 0.040 3
GJ 725 A (†) M3V 3352 10.43 8.93 4.43 0.937 ± 0.008 1
GJ 725 B (†) M3.5V 3180 11.32 9.78 5.00 0.851 ± 0.015 1
GJ 729 (†) M3.5Ve 3117 12.19 10.43 5.37 0.642 ± 0.020 2
GJ 752 A M3V 3236 10.63 9.12 4.67 0.836 ± 0.051 5
GJ 809 (*) M1V 3474 10.46 8.58 4.62 0.722 ± 0.008 1
GJ 825 M1V 8.09 6.68 3.10
GJ 832 (*) M2/3V 3310 10.18 8.69 4.50 0.814 ± 0.010 2
GJ 876 (*) M3.5V 3185 11.75 10.18 5.01 0.705 ± 0.009 2
GJ 880 (†) M1.5V 3398 10.14 8.64 4.52 0.744 ± 0.004 1
GJ 887 (†) M2V 3376 8.83 7.39 3.46 1.390 ± 0.040 3
GJ 908 M1V 3619 10.43 8.99 5.04

Notes. In the last two columns, we show the limb-darkened angular diameter of the stars extracted from the literature and its references. (G) Values extracted from Gaia Data Release 3 (Gaia Collaboration 2023). (S) Values extracted from SIMBAD. (*), (†) stars considered and rejected by Salsi et al. 2021 (see Sect. 3.2). 1: Boyajian et al. (2012); 2: Rabus et al. (2019); 3: Ségransan et al. (2003); 4: Schaefer et al. (2018); 5: Berger et al. (2006).

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