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Table A.1
Observation log of the γ Dor stars.
| KIC | N | Observation times | S/N | RV |
|---|---|---|---|---|
| (km s−1) | ||||
| 2 575 161 | 3 | 2019 | 160 | − 9.3 ± 0.8 |
| 2 710 594 | 4 | 2011 | 80 | − 37 ± 2 |
| 2 846 358 | 4 | 2017 | 70 | 2.7 ± 0.8 |
| 3 331 147 | 3 | 2019 | 115 | − 20.0 ± 0.9 |
| 3 448 365 | 4 | 2011, 2014 | 205 | − 30 ± 2 |
| 3 626 325 | 3 | 2019 | 65 | − 24 ± 1 |
| 3 648 936 | 3 | 2019 | 110 | 2 ± 2 |
| 3 744 571 | 4 | 2013 | 35 | − 23 ± 1 |
| 3 942 392 | 3 | 2012 | 170 | − 28.8 ± 0.9 |
| 4 255 166 | 3 | 2019 | 80 | − 25.6 ± 0.8 |
| 4 567 531 | 3 | 2019 | 85 | − 29 ± 2 |
| 4 659 837 | 2 | 2019 | 40 | SB1 |
| 4 757 184 | 4 | 2011 | 60 | − 24.7 ± 0.8 |
| 4 846 809 | 3 | 2013 | 25 | 0 ± 1 |
| 5 018 590 | 4 | 2012 | 150 | − 19 ± 2 |
| 5 113 797 | 2 | 2011 | 170 | 15 ± 3 |
| 5 114 382 | 4 | 2011 | 40 | 15 ± 2 |
| 5 450 503 | 3 | 2019 | 115 | − 23 ± 2 |
| 5 522 154 | 3 | 2011 | 105 | − 24 ± 3 |
| 5 646 058 | 3 | 2019 | 55 | − 10 ± 2 |
| 5 708 550 | 4 | 2011 | 75 | − 15 ± 2 |
| 5 788 623 | 4 | 2013 | 45 | − 4 ± 2 |
| 5 887 983 | 3 | 2019 | 60 | − 9 ± 3 |
| 5 954 264 | 2 | 2010 | 185 | − 33.0 ± 0.8 |
| 6 064 932 | 2 | 2019 | 60 | − 3.5 ± 0.8 |
| 6 131 093 | 4 | 2017 | 110 | 5.6 ± 0.7 |
| 6 292 398 | 8 | 2011–2020 | 105 | SB1(a) |
| 6 301 745 | 3 | 2019 | 100 | − 39 ± 4 |
| 6 468 146 | 7 | 2011, 2014, 2019 | 225 | SB1(b) |
| 6 468 987 | 4 | 2013, 2014 | 30 | − 27.6 ± 0.7 |
| 6 519 869 | 2 | 2011 | 85 | 2.5 ± 0.3 |
| 6 678 174 | 4 | 2011 | 60 | − 13.6 ± 0.9 |
| 6 935 014 | 5 | 2011 | 80 | − 9 ± 1 |
| 6 953 103 | 4 | 2013, 2014 | 30 | 7 ± 2 |
| 7 023 122 | 4 | 2011 | 100 | − 18.1 ± 0.8 |
| 7 215 607 | 2 | 2019 | 90 | 7.4 ± 0.3 |
| 7 365 537 | 3 | 2011 | 170 | − 30 ± 2 |
| 7 380 501 | 4 | 2011 | 40 | − 6 ± 1 |
| 7 434 470 | 4 | 2013 | 35 | SB1(c) |
| 7 583 663 | 3 | 2013, 2014 | 30 | − 29 ± 4 |
| 7 661 054 | 4 | 2012 | 95 | − 17.8 ± 0.2 |
| 7 694 191 | 4 | 2019 | 80 | SB1 |
| 7 939 065 | 4 | 2013 | 45 | − 22 ± 3 |
| 8 123 127 | 3 | 2019 | 60 | 2 ± 2 |
| 8 197 761 | 13 | 2015 | 100 | SB1(d) |
| 8 355 130 | 2 | 2010 | 105 | 9.4 ± 0.6 |
| 8 364 249 | 4 | 2011 | 50 | − 23 ± 4 |
| 8 375 138 | 4 | 2011 | 90 | − 4 ± 2 |
| 8 651 452 | 3 | 2019 | 80 | − 16 ± 3 |
| 8 871 304 | 16 | 2010 | 195 | SB1 |
| 9 210 943 | 5 | 2011, 2014 | 80 | − 28 ± 3 |
| 9 419 182 | 4 | 2011, 2019 | 115 | 0 ± 2 |
| 9 480 469 | 4 | 2013, 2014 | 30 | − 18 ± 3 |
| 9 490 067 | 2 | 2017 | 40 | − 0.6 ± 0.2 |
| 9 595 743 | 4 | 2013 | 50 | − 9 ± 1 |
| 9 716 358 | 4 | 2009 | 60 | 6.1 ± 0.4 |
| 9 962 653 | 19 | 2017, 2019 | 215 | SB1 |
| 10 224 094 | 4 | 2011 | 50 | − 7.2 ± 0.5 |
| 10 256 787 | 13 | 2012, 2013, 2014 | 50 | 6 ± 1 |
| 10 317 467 | 3 | 2019 | 110 | 6.9 ± 0.4 |
| 10 467 146 | 4 | 2013, 2014 | 35 | SB1(b) |
| 10 470 294 | 3 | 2019 | 70 | − 17 ± 7 |
| 11 080 103 | 4 | 2013, 2014 | 25 | 4 ± 1 |
| 11 099 031 | 4 | 2011 | 155 | − 17 ± 1 |
| 11 294 808 | 4 | 2011 | 55 | − 9 ± 2 |
| 11 456 474 | 4 | 2013, 2014 | 25 | − 11 ± 2 |
| 11 607 017 | 3 | 2019 | 40 | − 26 ± 4 |
| 11 612 274 | 2 | 2018 | 90 | 1 ± 2 |
| 11 721 304 | 4 | 2011 | 45 | 1.1 ± 0.7 |
| 11 826 272 | 11 | 2011, 2015, 2019 | 130 | − 9.6 ± 0.6 |
| 11 907 454 | 4 | 2011 | 70 | SB1 |
| 11 917 550 | 4 | 2011 | 75 | 10 ± 2 |
| 11 920 505 | 13 | 2011, 2016, 2019 | 245 | − 25 ± 1 |
| 12 066 947 | 3 | 2011 | 115 | 9 ± 2 |
| 12 117 689 | 3 | 2019 | 95 | − 24 ± 6 |
| 12 458 189 | 4 | 2011 | 80 | − 35 ± 1 |
| 12 643 786 | 4 | 2011 | 55 | 1 ± 2 |
| γ Dor- δ Sct hybrids | ||||
| 2 168 333 | 8 | 2014-2020 | 150 | − 7 ± 6 |
| 3 241 199 | 3 | 2019 | 75 | − 6 ± 11 |
| 5 294 571 | 2 | 2017 | 50 | − 15 ± 10 |
| 5 608 334 | 3 | 2012 | 125 | − 17 ± 6 |
| 7 106 648 | 4 | 2018 | 135 | − 12 ± 4 |
| 7 748 238 | 6 | 2014 | 195 | − 23 ± 2 |
| 7 770 282 | 27 | 2011–2019 | 240 | 7 ± 1 |
| 7 977 996 | 4 | 2019, 2020 | 55 | 13 ± 11 |
| 8 645 874 | 5 | 2011, 2019 | 125 | SB1 |
| 8 836 473 | 4 | 2013, 2014 | 25 | − 26 ± 1 |
| 9 651 065 | 2 | 2019 | 50 | − 22 ± 1 |
| 9 751 996 | 8 | 2011, 2019 | 50 | − 51.7 ± 0.2 |
| 11 754 232 | 12 | 2013, 2014 | 50 | SB1(b) |
| 12 365 420 | 5 | 2019, 2020 | 35 | 7 ± 4 |
| SB2, SB3 or higher order binaries | ||||
| 3 222 854 | 10 | 2013, 2014, 2015 | SB2(b) | |
| 4 480 321 | 58 | 2011–2020 | SB3(e) (hybrid) | |
| 5 219 533 | 50 | 2010–2019 | SB3(e) (hybrid) | |
| 6 467 639 | 12 | 2013, 2014 | SB3(b) (hybrid) | |
| 6 764 812 | 3 | 2019 | SB2 | |
| 6 778 063 | 9 | 2013, 2014 | SB3(b) (hybrid) | |
| 7 385 783 | 3 | 2019 | SB2 | |
| 8 324 305 | 3 | 2011, 2019, 2020 | SB2 | |
| 8 975 515 | 32 | 2010–2020 | SB2(e) | |
| 10 080 943 | 25 | 2011, 2013, 2014 | SB2(f) (hybrid) | |
| low S/N spectra | ||||
| 5 254 203 | 4 | 2013, 2014 | 15 | |
| 7 746 984 | 2 | 2014 | 20 | |
| 9 533 489 | 3 | 2013, 2014 | 20 | |
Notes. N is the total number of spectra, and S/N is the combined signal-to-noise ratio in the continuum region between 5440 and 5442 Å. The last column contains the RV of single stars or the type of spectroscopic binary.
References. (a) Niemczura et al. (2015); (b)Van Reeth et al. (2015);(c)Li et al. (2020); (d)Murphy et al. (2018); (e)Lampens et al. (2018); (f)Tkachenko et al. (2013).
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