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Table A.1

Relevant data for stars in our sample with periodic photometric modulation.

Star Sp. type m B m V ⟨ mVASAS ⟩ N meas Time span Ref.
(years)
HD 1388 G0 –4.89 ± 0.01 7.09 6.50 6.50 335 7.4 1, 5,
HD 10180 G1 –5.00 ± 0.03 7.95 7.32 7.32 524 8.8 2, 5
HD 21019 G2 –5.12 ± 0.02 6.90 6.20 6.20 331 8.1 2, 4
HD 2071 G2 –4.89 ± 0.03 7.95 7.27 7.27 641 8.4 1, 6
HD 1320 G2 –4.79 ± 0.03 8.63 7.98 7.95 614 9.0 1,3
HD 63765 G9 –4.77 ± 0.04 8.85 8.10 8.09 588 9.0 1, 5
HD 82558 K0 –4.01 ± 0.05 8.76 7.89 7.87 481 9.0 0, 7, 11
HD 155885 K1 –4.55 ± 0.02 5.96 5.08 4.96 562 8.6 3, 10
HD 224789 K1 –4.55 ± 0.03 9.12 8.24 8.23 489 9.0 1, 5
V660 Tau K2 13.66 12.60 12.63 275 7.0 18
HD 176986 K2.5 –4.90 ± 0.04 9.39 8.45 8.46 405 8.7 1, 5
HD 32147 K3 –4.92 ± 0.04 7.27 6.21 6.19 459 8.7 0, 9
HD 45088 K3 –4.48 ± 0.17 7.74 6.77 6.78 437 6.9 0, 7
HD 104067 K3 –4.77 ± 0.04 8.90 7.92 7.91 795 9.0 1, 7
HD 215152 K3 –4.92 ± 0.06 9.13 8.13 8.09 327 9.0 1, 5
V410 Tau K3 12.13 10.75 10.85 56 1.1 5
HD 131977 K4 –4.33 ± 0.13 6.83 5.72 5.66 228 8.3 0 9
HD 125595 K4 –4.82 ± 0.07 10.13 9.03 8.99 703 8.7 1, 6
HD 118100 K5 10.55 9.37 9.37 476 8.6 7
GJ9482 K7 –4.74 ± 0.05 11.80 10.38 10.38 524 8.8 0, 7
HD 113538 K9 –4.82 ± 0.07 10.43 9.06 9.05 994 8.8 0, 7
GJ846 M0 –4.84 ± 0.04 10.62 9.15 9.15 312 9.0 1, 7
GJ676A M0 –4.96 ± 0.04 11.03 9.59 9.60 789 8.7 1, 7
GJ229 M1 –4.91 ± 0.04 9.61 8.13 8.15 708 9.0 0, 7
HD 197481 M1 –4.05 ± 0.04 10.05 8.63 8.63 455 8.9 0, 4, 11
GJ514 M1 –5.10 ± 0.06 10.52 9.03 9.04 341 8.0 1,7
GJ239 M1 11.10 9.59 9.60 528 7.0 7
GJ205 M1.5 –4.96 ± 0.06 9.44 7.97 7.95 620 9.0 1, 7
GJ832 M1.5 –5.21 ± 0.07 10.18 8.67 8.67 482 8.9 1, 7
GJ536 M1.5 –5.22 ± 0.07 11.18 9.71 9.71 345 3.6 1, 7
GJ382 M2 –4.80 ± 0.06 10.76 9.26 9.25 494 9.0 1, 7
GJ588 M2.5 –5.34 ± 0.10 10.81 9.31 9.33 503 8.7 1, 7
GJ176 M2.5 –4.99 ± 0.07 11.49 9.95 10.01 413 7.0 1, 7
GJ752A M3 –5.16 ± 0.07 10.63 9.12 9.14 389 8.1 1, 7
GJ674 M3 –5.07 ± 0.08 10.97 9.41 9.39 537 8.7 1, 7
GJ680 M3 11.67 10.13 10.13 834 8.7 7
GJ408 M3 11.58 10.02 10.03 273 6.5 7
GJ877 M3 –5.33 ± 0.15 11.87 10.38 10.39 1049 9.0 0 ,7
GJ479 M3 –4.88 ±0.05 12.20 10.66 10.67 534 8.7 0, 7
GJ358 M3 –4.69 ± 0.10 12.21 10.69 10.72 994 9.0 1, 7
GJ273 M3.5 –5.52 ± 0.07 11.44 9.87 9.98 366 8.0 1, 7
GJ849 M3.5 –5.14 ± 0.04 11.87 10.37 10.36 424 8.9 1, 7
GJ729 M3.5 12.24 10.50 10.54 620 8.6 7
GJ896A M3.5 12.27 10.35 10.07 257 6.9 13, 14
GJ317 M3.5 –4.57 ± 0.11 13.2 11.98 12.07 561 9.0 0, 4, 16
GJ526 M4 –5.31 ± 0.07 9.92 8.43 8.45 281 6.5 1, 7
GJ628 M4 –5.47 ± 0.11 11.64 10.07 10.12 498 8.7 0, 17
GJ234 M4+M5.5 –4.60 ± 0.24 12.76 11.07 11.08 450 8.7 0, 7
GJ54.1 M4 13.89 12.07 12.09 435 9.0 7
LP 816-60 M4 13.03 11.46 11.44 413 8.5 7
GJ285 M4.5 –4.09 ± 0.06 12.83 11.23 11.24 530 8.7 0, 7
GJ447 M4.5 –5.73 ± 0.07 12.91 11.15 11.12 364 8.7 0, 17
GJ581 M5 –5.79 ± 0.03 12.17 10.57 10.57 687 8.7 1, 7
GJ551 M5.5 –5.65 ± 0.17 12.97 11.10 11.23 991 8.7 1, 8
GJ406 M6 15.54 13.51 13.51 331 8.0 17

Reference. For : 0) this work; 1) Suárez Mascareño et al. (2015); 2) Lovis et al. (2011); 3) Baliunas et al. (1995). For magnitudes: 4) Mermilliod (1986); 5) Høg et al. (2000); 6) Cousins & Stoy (1962); 7) Koen et al. (2010); 8) Jao et al. (2014); 9) Ducati (2002); 10) Torres et al. (2006); 11) Kiraga (2012); 12) Garcés et al. (2011); 13) Fabricius et al. (2002); 14) Jenkins et al. (2009); 15) Landolt (2009); 16) van Altena et al. (1995); 17) Landolt (1992); 18) Stauffer (1984).

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