Table 3
Best fit spectral parameters for the 17 brightest X-ray sources (more than 200 counts) identified as rotational variables; parameters are for a phabs*apec or phabs*(apec+apec) model.
| KIC_ID | SpT (a) | Counts (b) | Model | NH | kT | EM |
|---|---|---|---|---|---|---|
| (cm−2) | (keV) | (cm−3) | ||||
| 5 112 508 | M | 520 | Phabs*apec | ~0 | 0.83 | 1.31 × 1052 |
| 5 113 557 | F | 2088 | Phabs*apec | 1.46 × 1020 | 0.60 | 6.40 × 1050 |
| 5 653 243 | K | 316 | Phabs*apec | ~0 | 0.80 | 5.86 × 1052 |
| 6 761 532 | G | 226 | Phabs*apec | 3.60 × 1020 | 0.63 | 2.43 × 1052 |
| 7 018 708 | G | 2637 | Phabs*(apec+apec) | 6.80 × 1020 | 0.29, 1.04 | 1.93 × 1053, 2.24 × 1053 |
| 8 454 353 | M | 1291 | Phabs*apec | ~0 | 0.99 | 9.69 × 1051 |
| 8 517 303 | K | 1763 | Phabs*apec | 9.10 × 1020 | 1.06 | 1.10 × 1054 |
| 8 518 250 | K | 434 | Phabs*(apec+apec) | ~0 | 0.94, 0.23 | 1.24 × 1051, 1.88 × 1051 |
| 8 520 065 | F | 764 | Phabs*(apec+apec) | 2.33 × 1020 | 1.07, 0.54 | 4.30 × 1053, 3.42 × 1053 |
| 8 584 672 | K | 230 | Phabs*apec | ~0 | 0.83 | 1.21 × 1053 |
| 8 647 865 | F | 433 | Phabs*apec | ~0 | 0.49 | 1.60 × 1052 |
| 8 713 822 | K | 675 | Phabs*apec | 1.43 × 1020 | 1.05 | 2.58 × 1054 |
| 8 842 083 | K | 590 | Phabs*apec | 1.1 × 1021 | 0.76 | 7.01 × 1050 |
| 9 048 551 | K | 1634 | Phabs*apec | ~0 | 1.07 | 8.91 × 1051 |
| 9 048 949 | K | 844 | Phabs*apec | ~0 | 0.94 | 4.31 × 1051 |
| 9 048 976 | K | 285 | Phabs*apec | ~0 | 0.96 | 4.11 × 1051 |
| 11 971 335 | G | 696 | Phabs*apec | ~0 | 1.30 | 2.10 × 1053 |
Notes. (a) Spectral type has been evaluated from the Teff according to Pecaut & Mamajek (2013). (b)This is the sum of the counts in the three EPIC instruments.
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