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Table A.2
Observation log of the SPB stars.
| KIC | N | Observation times | S/N | RV |
|---|---|---|---|---|
| (km s−1) | ||||
| 3 240 411 | 6 | 2012, 2016, 2018 | 145 | − 37 ± 8 |
| 3 756 031 | 5 | 2012, 2016 | 90 | 11 ± 4 |
| 3 839 930 | 3 | 2010 | 175 | − 29 ± 1 |
| 3 865 742 | 3 | 2019 | 55 | − 12 ± 12 |
| 5 941 844 | 1 | 2016 | 110 | − 11 ± 2 |
| 6 462 033 | 1 | 2019 | 65 | 3.7 ± 0.7 |
| 6 780 397 | 10 | 2012 | 135 | SB1 |
| 7 760 680 | 4 | 2012, 2014 | 140 | − 50 ± 2 |
| 8 057 661 | 6 | 2019 | 65 | − 36 ± 10 |
| 8 087 269 | 4 | 2013 | 50 | 96 ± 46 |
| 8 381 949 | 3 | 2010 | 100 | − 111 ± 10 |
| 8 459 899 | 122 | 2010 | 720 | − 10 ± 3 |
| 8 714 886 | 3 | 2010 | 90 | 25.0 ± 0.8 |
| 8 766 405 | 2 | 2010 | 180 | 43 ± 17 |
| 9 964 614 | 6 | 2010, 2016, 2017 | 80 | − 137 ± 4 |
| 10 285 114 | 4 | 2009, 2012 | 135 | 37 ± 19 |
| 10 536 147 | 5 | 2019 | 70 | − 18 ± 11 |
| 11 360 704 | 3 | 2010, 2012 | 105 | − 24 ± 13 |
| 11 971 405 | 5 | 2010, 2015 | 245 | − 27 ± 7 |
| 12 258 330 | 4 | 2010, 2017, 2018 | 170 | − 37 ± 7 |
| SB2 | ||||
| 4 930 889 | 27 | 2010–2015 | SB2(a) | |
| 6 352 430 | 29 | 2010, 2011, 2012 | SB2(b) | |
| low S/N spectra | ||||
| 9 715 425 | 3 | 2019 | 20 | |
Notes. N is the total number of spectra, and S/N is the combined signal-to-noise ratio in the continuum region between 4960 and 4962 Å. The last column contains the RV of single stars or the type of spectroscopic binary.
References. (a) Pápics et al. (2017); (b) Pápics et al. (2013).
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