Table 1.
Atmospheric parameters of the giant stars in our sample.
Label | KIC | Teff | log g | [Fe/H] | vmicro | vbroad |
---|---|---|---|---|---|---|
(K) | (dex) | (dex) | (km s−1) | (km s−1) | ||
A | 4054905 (a) | 4790 ± 190 | ... | −0.72 ± 0.31 | 0.74 ± 0.75 | 57.6 ± 5.5 |
B | 4360072 | 5020 ± 210 | 2.79 ± 0.45 | −0.14 ± 0.23 | 0.57 ± 0.58 | 38.0 ± 3.3 |
C | 4473933 | 4530 ± 220 | 2.89 ± 0.59 | −0.41 ± 0.28 | 1.25 ± 0.80 | 49.8 ± 4.5 |
D | 4663623 (b) | 4812 ± 92 | 2.7 ± 0.2 | −0.13 ± 0.06 | ... | ... |
E | 5193386 (c) | 4780 ± 100 | 3.284± 0.014 | −0.36 ± 0.06 | ... | ... |
F | 5866138 | 4960 ± 120 | 3.04 ± 0.24 | 0.05 ± 0.13 | 1.40 ± 0.33 | 5.4 ± 1.6 |
G | 6307537 (a) | 4960 ± 240 | ... | −0.03 ± 0.43 | 2.0 ± 1.4 | 95.4 ± 8.1 |
H | 6757558 | 4590 ± 110 | 2.30 ± 0.31 | −0.04 ± 0.13 | 1.24 ± 0.40 | 4.9 ± 1.9 |
I | 7133286 (a) | 4500 ± 110 | ... | −0.60 ± 0.18 | 1.40 ± 0.58 | 31.1 ± 2.4 |
J | 7293054 (a) | 4790 ± 160 | ... | 0.11 ± 0.26 | 1.99 ± 0.86 | 26.1 ± 2.2 |
K | 7768447 | 4760 ± 160 | 2.96 ± 0.24 | 0.17 ± 0.25 | 3.0 ± 1.4 | 16.2 ± 2.8 |
L | 8435232 (a) | 4460 ± 130 | ... | −0.15 ± 0.24 | 2.00 ± 0.85 | 30.9 ± 3.0 |
M | 9153621 | 4760 ± 190 | 2.34 ± 0.39 | −0.35 ± 0.21 | 1.38 ± 0.55 | 16.6 ± 2.3 |
N | 9904059 | 4830 ± 160 | 2.83 ± 0.24 | 0.01 ± 0.26 | 1.05 ± 0.69 | 24.5 ± 2.3 |
O | 10015516 | 4830 ± 130 | 1.83 ± 0.22 | −0.43 ± 0.15 | 1.27 ± 0.35 | 23.6 ± 1.4 |
P | 10074700 (d) | 5070 ± 100 | 4.53 ± 0.20 | −0.40 ± 0.10 | ... | ... |
Q | 11235323 (a) | 4840 ± 200 | ... | −0.36 ± 0.25 | 2.6 ± 1.4 | 26.3 ± 3.0 |
Notes. For some systems, we added an extra step in the GSSP analysis or used different values.
For these SB2 systems, we fixed the value of log g during the spectroscopic analysis to that provided by the dynamical analysis (see Table 3).
KIC 4663623: atmospheric parameters from Gaulme et al. (2016a).
KIC 5193386: atmospheric parameters from APOGEE DR14 (Abolfathi et al. 2018).
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