Table 3
Photospheric and chromospheric activity properties of the 18 seismic solar analogs derived from the photometric Kepler and spectroscopic Hermes observations.
# Star | KIC | Prot (days) | Sph (ppm) | ![]() |
log ![]() |
S/N(Ca) | ΔT (days) | N spec | |||||
|
|||||||||||||
1 | 3241581 | 26.3 ± 2.0 | 236.9 ± 3.8 | 0.182 ± 0.024 | − 4.868 ± 0.164 | 17.1 | 504 | 23 | |||||
2 | 3656476 | 31.7 ± 3.5 | 89.1 ± 1.6 | 0.168 | − 5.002 ± 0.100 | 24.5 | <1 | 1 | |||||
3 | 4914923 | 20.5 ± 2.8 | 139.1 ± 2.5 | 0.168 ± 0.014 | − 4.918 ± 0.100 | 26.6 | 34 | 6 | |||||
4 | 5084157 | 22.2 ± 2.8 | 270.8 ± 4.8 | 0.217 ± 0.107 | − 4.840 ± 0.580 | 11.0 | 33 | 9 | |||||
5 | 5774694 | 12.1 ± 1.0 | 2492.3 ± 61.2 | 0.269 ± 0.021 | − 4.581 ± 0.059 | 23.7 | 36 | 3 | |||||
6 | 6116048 | 17.3 ± 2.0 | 90.2 ± 1.9 | 0.157 ± 0.001 | − 4.984 ± 0.042 | 24.1 | 35 | 3 | |||||
7 | 6593461 | 25.7 ± 3.0 | 188.8 ± 3.6 | 0.260 ± 0.119 | − 4.550 ± 0.333 | 10.4 | 35 | 8 | |||||
8† | 7296438 | 25.2 ± 2.8 | 177.1 ± 3.0 | 0.162 | − 4.994 ± 0.151 | 20.4 | 35 | 3a | |||||
9 | 7680114 | 26.3 ± 1.9 | 50.2 ± 1.0 | 0.185 ± 0.019 | − 4.881 ± 0.164 | 19.4 | 35 | 3 | |||||
10 | 7700968 | 36.2 ± 4.2 | 88.9 ± 1.4 | 0.181 ± 0.010 | − 4.866 ± 0.123 | 19.8 | 35 | 3 | |||||
11 | 9049593 | 12.4 ± 2.5 | 290.8 ± 6.4 | 0.177 ± 0.016 | − 4.955 ± 0.200 | 18.4 | 35 | 3 | |||||
12 | 9098294 | 19.8 ± 1.3 | 292.7 ± 5.2 | 0.203 ± 0.031 | − 4.737 ± 0.136 | 19.5 | 35 | 3 | |||||
13 | 10130724 | 32.6 ± 3.0 | 155.0 ± 2.5 | 0.252 ± 0.067 | − 4.548 ± 0.246 | 10.6 | 34 | 5 | |||||
14 | 10215584 | 22.2 ± 2.9 | 138.3 ± 2.5 | 0.215 ± 0.049 | − 4.738 ± 0.211 | 17.4 | 35 | 4 | |||||
15 | 10644253 | 10.9 ± 0.9 | 549.4 ± 13.3 | 0.219 ± 0.014 | − 4.691 ± 0.059 | 30.1 | 180 | 12 | |||||
16 | 10971974 | 26.9 ± 4.0 | 309.9 ± 4.9 | 0.241 ± 0.066 | − 4.761 ± 0.312 | 10.0 | 35 | 3 | |||||
17† | 11127479 | 17.6 ± 1.8 | 115.9 ± 2.8 | 0.271 ± 0.169 | − 4.683 ± 0.482 | 10.2 | 35 | 4 | |||||
18 | 11971746 | 19.5 ± 2.1 | 90.5 ± 2.0 | 0.152 ± 0.028 | − 4.937 ± 0.217 | 16.6 | 34 | 7 |
Notes. The surface rotation periods, Prot, were measured by García et al. (2014) from the Kepler observations. The columns ΔT and Nspec corresponds respectively to the interval of time covered by the Hermes observations and the associated number of analyzed spectra. The two stars indicated by the symbol (†) a re candidates for hosting a planetary system from the Kepler Objects of Interest (KOI) list (source: MAST at https://archive.stsci.edu/kepler/).
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