Table A.1.
Visual apparent magnitudes mV, bolometric corrections BCV, distances D (Bailer-Jones et al. 2018), and extinctions AV used to derive the luminosity.
| KIC | mV | BCV | D (pc) | AV | Reliable AV? | log L/L⊙ |
|---|---|---|---|---|---|---|
| 2710594 | 11.79 | 0.031 |
 |
0.21 | Y |
 |
| 3448365 | 9.92 | 0.031 |
 |
0.05 | N |
 |
| 4846809 | 12.36 | 0.035 |
 |
0.16 | Y |
 |
| 5114382 | 11.55 | 0.034 |
 |
0.27 | Y |
 |
| 5522154(*) | 10.44 | 0.028 |
 |
0.0 | N |
 |
| 5708550(*) | 11.93 | 0.03 |
 |
0.15 | Y |
 |
| 5788623 | 12.07 | 0.034 |
 |
0.12 | Y |
 |
| 6468146 | 9.96 | 0.035 |
 |
0.02 | N |
 |
| 6468987 | 12.67 | 0.034 |
 |
0.54 | Y |
 |
| 6678174(*) | 11.74 | 0.033 |
 |
0.21 | N |
 |
| 6935014 | 10.91 | 0.033 |
 |
0.15 | Y |
 |
| 6953103(*) | 12.56 | 0.035 |
 |
0.27 | Y |
 |
| 7023122 | 10.84 | 0.035 |
 |
0.05 | N |
 |
| 7365537(*) | 9.19 | 0.035 |
 |
0.0 | N |
 |
| 7380501 | 11.98 | 0.029 |
 |
0.46 | Y |
 |
| 7434470 | 12.02 | 0.031 |
 |
0.25 | Y |
 |
| 7583663 | 12.69 | 0.031 |
 |
0.21 | Y |
 |
| 7939065 | 12.14 | 0.035 |
 |
0.2 | Y |
 |
| 8364249 | 11.95 | 0.032 |
 |
0.25 | Y |
 |
| 8375138 | 11.02 | 0.032 |
 |
0.13 | N |
 |
| 8645874 | 9.92 | 0.035 |
 |
0.02 | N |
 |
| 8836473 | 12.78 | 0.035 |
 |
0.56 | Y |
 |
| 9480469 | 12.78 | 0.035 |
 |
0.31 | Y |
 |
| 9595743 | 12.09 | 0.035 |
 |
0.06 | Y |
 |
| 9751996 | 10.96 | 0.034 |
 |
0.1 | Y |
 |
| 10467146 | 12.66 | 0.034 |
 |
0.29 | Y |
 |
| 11080103 | 12.94 | 0.035 |
 |
0.2 | Y |
 |
| 11099031 | 10.02 | 0.025 |
 |
0.02 | N |
 |
| 11294808 | 11.73 | 0.03 |
 |
0.21 | Y |
 |
| 11456474 | 12.49 | 0.032 |
 |
0.2 | Y |
 |
| 11721304 | 11.71 | 0.034 |
 |
0.13 | Y |
 |
| 11754232 | 12.24 | 0.035 |
 |
0.08 | Y |
 |
| 11826272 | 10.21 | 0.031 |
 |
0.04 | N |
 |
| 11907454 | 11.38 | 0.032 |
 |
0.05 | Y |
 |
| 11917550 | 11.12 | 0.033 |
 |
0.05 | N |
 |
| 11920505 | 9.88 | 0.034 |
 |
0.0 | N |
 |
| 12066947 | 10.23 | 0.035 |
 |
0.0 | N |
 |
Notes. The ‘Reliable AV’ flag indicates whether a reliable estimation of the extinction could be made with the Bayerstar2019 extinction map. Stars for which no reliable estimation could be made according to the Bayerstar2019 map are relatively close by, and therefore the extinction is expected to be minimal. For the stars flagged with an asterisk (*) the luminosity is inconsistent with the pulsations, and its value is therefore not used in the modelling.
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