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Table C.2

Parameters of the DUNES_DB stars with d ≤ 15 pc and 15 pc <d ≤ 20 pc.

HIP Teff log g [Fe/H] Flag Lbol Ref. Prot (d) t Gyro) tHK
(K) (cm/s2) (dex) (L) or lower limit (Gyr) (Gyr)

FGK stars (d ≤ 15 pc)

1599 5960 4.45 −0.17 S 1.224 −4.855 1 14.01 ± 0.97 2.20 4.03
3765 4977 4.57 −0.22 S 0.283 −4.852 2 39.02 ± 0.25 5.41 3.98
7751 4993 4.54 −0.23 S 0.304 −4.94 3
7918 5891 4.36 + 0.06 S 1.405 −4.987 4 21.10 ± 0.12 3.56 6.36
7981 5189 4.52 −0.04 S 0.439 −4.912 2 39.60 ± 0.43 6.04 4.99
10644 5684 4.36 −0.45 P 1.118 −4.644 4 11.57 ± 0.35 1.30 1.47
12114 4866 4.66 + 0.00 S 0.257 −4.958 2 44.90 ± 0.53 6.66 5.82
12843 6273 4.20 −0.04 P 2.585 −4.524 1 2.92 ± 0.36 0.71
14879 6275 4.40 −0.19 S 4.923 −4.901 1 11.58 ± 1.39 2.12 4.79
15457 5755 4.52 + 0.11 S 0.838 −4.42 2 7.53 ± 0.18 0.46 0.35
15510 5415 4.55 −0.34 S 0.637 −4.998 1 32.42 ± 0.55 5.51 6.56
16852 6014 4.08 −0.06 S 3.060 −5.053 4 17.06 ± 0.95 3.13 7.59
22449 6457 4.15 −0.01 S 2.708 −4.788 4 5.83 ± 0.18 3.04
23693 6165 4.38 −0.20 P 1.414 −4.49 3 3.91 ± 0.37 0.40 0.57
27072 6331 4.28 −0.10 P 2.291 −4.817 1 5.91 ± 0.66 3.45
37279 6578 3.99 + 0.01 S 6.605 −4.777 2 3.21 ± 0.59 2.89
47080 5539 4.48 + 0.33 S 0.822 −4.638 2 21.86 ± 0.10 2.39 1.42
56997 5514 4.50 −0.04 S 0.618 −4.546 2 14.62 ± 0.65 1.31 0.82
57443 5630 4.51 −0.28 S 0.806 −4.957 1 25.90 ± 0.47 4.27 5.80
57757 6125 4.12 + 0.14 S 3.483 −4.99 5 10.27 ± 1.37 2.62 6.41
59199 7042 4.21 −0.14 P 4.175 −5.373 6 >3.26 (21.7)
61317 5890 4.40 −0.17 S 1.178 −4.851 4 15.11 ± 0.89 2.32 3.96
61941 6797 4.25 −0.13 P 8.346 −4.50 6 6.31 ± 0.37 0.61
64394 6065 4.43 + 0.04 S 1.381 −4.745 2 11.48 ± 0.49 1.59 2.49
64924 5646 4.57 + 0.10 S 0.820 −5.001 2 32.29 ± 0.78 5.50 6.62
70497 6315 4.29 −0.10 P 4.034 −4.591 4 4.26 ± 0.21 2.25 1.08
72659 5549 4.63 −0.10 S 0.611 −4.363 2 6.49 ± 0.31 0.31 0.23
73695 5851 4.30 −0.19 S 1.552 −4.602 4 12.85 ± 0.13 1.31 1.16
77257 5899 4.17 + 0.01 S 2.077 −5.004 2 19.73 ± 0.96 3.40 6.67
78072 6265 4.08 −0.15 S 2.863 −5.113 4 >5.2 (11.42)
80686 6029 4.46 −0.19 P 1.301 −4.65 3 8.25 ± 1.00 1.02 1.52
89937 6034 4.27 −0.65 P 1.942 −4.9 6 7.13 ± 0.35 4.78
93017 5834 4.33 −0.19 P 1.515 −4.874 2 16.18 ± 0.31 2.53 4.34
99825 5105 4.48 −0.03 S 0.405 −5.048 1 47.33 ± 0.78 7.74 7.50
102485 6590 4.26 −0.05 P 3.705 −4.404 1 0.94 ± 0.06 0.31
105858 6089 4.38 −0.68 P 1.400 −4.491 1 2.93 ± 0.57 0.57
109176 6448 4.25 0.12 P 3.303 −5.06 7 4.61 ± 0.39 7.72
113283 4555 4.53 −0.01 S 0.181 −4.467 1 16.03 ± 0.03 0.88 0.49
116771 6180 4.09 −0.10 S 3.319 −5.112 4 >8.58 (6.67) > 2.27
FGK stars (15 pc <d 20 pc)

5862 6128 4.36 + 0.16 S 1.913 −4.861 1 13.63 ± 0.68 2.17 4.12
17651 6654 4.11 + 0.09 P 4.930 −4.684 1 2.74 ± 0.40 1.83
36366 7086 4.13 −0.25 P 5.351 −4.66 6 2.50 ± 0.36 1.61
44248 6556 4.01 + 0.04 P 5.249 −4.548 8 2.62 ± 0.09 0.83
46509 6486 4.22 −0.01 P 3.369 −4.828 4 2.66 ± 0.52 3.61
48113 5940 4.05 + 0.14 S 2.618 −5.042 4 22.30 ± 0.89 3.91 7.39
61174 6784 4.06 −0.05 P 4.873 −5.173 6 >1.12 (59.15)
64241 6376 4.26 −0.21 P 4.625 −4.53 2 2.26 ± 0.20 0.74
67153 6745 3.88 −0.09 P 5.857 −4.56 6 2.42 ± 0.22 0.90
71284 6727 4.32 −0.35 S 3.112 −5.476 4 >9.34 (7.32)
75312 5949 4.15 −0.06 S 2.631 −4.828 2 13.60 ± 0.38 2.07 3.61
77760 5840 3.94 −0.49 S 2.962 −5.042 2 15.50 ± 1.59 2.91 7.39
88745 6089 4.18 −0.53 S 1.867 −5.02 9 11.52 ± 0.20 2.60 6.98
104858 6250 4.40 −0.07 P 4.450 −4.905 8 10.36 ± 1.32 2.12 4.86
112447 6181 3.93 −0.24 S 4.387 −5.276 4 >4.55 (12.67) > 1.23

Notes. Teff, log g, and [Fe/H] are averages from Fuhrmann (2008), Gray et al. (2003), Gray et al. (2006), Holmberg et al. (2009), Santos et al. (2004), Sousa et al. (2008), Takeda et al. (2005), and Valenti & Fischer (2005). “S” and “P” in Col. 5 mean that the determination is spectroscopic or photometric. log g for HIP 104858 assigned according to its spectral type.

Reference. : (1) Gray et al. (2006); (2) Baliunas et al. (1996); (3) Martínez-Arnáiz et al. (2010); (4) Duncan et al. (1991); (5) Hall et al. (2007); (6) computed from ROSAT X-ray data using Eq. (A1) from Mamajek & Hillenbrand (2008); (7) Saffe et al. (2005); (8) Gray et al. (2003); (9) Wright et al. (2004). Determination of Prot from the Rossby number and valid if 0.4 <BV< 1.4 and (Noyes et al. 1984).

(†)

When a lower limit of the period is given, the number in parentheses is the value of vsini (km s-1) used to estimate it.

(‡)

The (BV) value is slightly outside the valid range of the Noyes et al. (1984) calibration for Prot. Gyrochronology age calibration valid if BV> 0.5 (Mamajek & Hillenbrand 2008). Chromospheric age calibration valid in the interval (Mamajek & Hillenbrand 2008).

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