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Table 3
List of 25 eclipsing multiple candidates.
| Name | Inner binary | Number of | Inner period | Structure | Reference |
|---|---|---|---|---|---|
| period (d) | extraneous eclipses | change range (d)a | |||
| KIC 2835289 | 0.8577619 | 4 | 0.025 | hierarchical | Conroy et al. (2015) |
| KIC 2856960 | 0.2585073 | ~48 | 0.004 | hierarchical | Marsh et al. (2014) |
| KIC 4150611 | 1.5222786 | 23 + 160 | – | hierarchical+binary | Shibahashi & Kurtz (2012) |
| KIC 4247791 | 4.0497388 | 649 | <0.001 | double binary | Lehmann et al. (2012) |
| KIC 4862625 | 20.000249 | ~10c | <0.001 | circumbinary planet | Kostov et al. (2013) |
| KIC 5255552 | 32.448635 | 10 | 0.3 | hierarchical | Borkovits et al. (2015) |
| KIC 5897826 | 33.794718 | 68 | – | hierarchical | Carter et al. (2011) |
| KIC 5952403 | 0.9056778 | ~26 | 0.006 | hierarchical | Derekas et al. (2011) |
| KIC 6543674 | 2.3910305 | 2 | 0.0065 | hierarchical | Masuda et al. (2015) |
| KIC 6762829 | 18.795266 | ~13c | <0.005 | circumbinary planet | Orosz et al. (2012) |
| KIC 6964043 | 5.3626595 | 17 | 0.2 | hierarchical | Borkovits et al. (2015) |
| KIC 7289157 | 5.2664250 | ~12 | 0.02 | hierarchical | Borkovits et al. (2015) |
| KIC 7622486 | 2.2799960 | 31 | <0.005 | double binary | Zhang et al. (2017) |
| KIC 7668648 | 27.818590 | 10 + 5 | 0.13 | hierarchical | Borkovits et al. (2015) |
| KIC 7670485 | 8.4677064 | 1 | <0.001 | hierarchical | Zhang et al. (2017) |
| KIC 7941635 | 0.7627242 | 1? | <0.002 | hierarchical? | This paper |
| KIC 8572936 | 27.795808 | ~5c | <0.002 | circumbinary planet | Welsh et al. (2012) |
| KIC 8938628 | 6.8622157 | 6+4 | 0.01 | hierarchical | Borkovits et al. (2015) |
| KIC 9007918 | 1.3872069 | 1 | 0.0016 | hierarchical | Borkovits et al. (2016) |
| KIC 9632895 | 27.322046 | 3b | – | circumbinary planet | Welsh et al. (2015) |
| KIC 9837578 | 20.733749 | ~10c | <0.001 | circumbinary planet | Welsh et al. (2012) |
| KIC 10020423 | 7.4483776 | ~28 + 4c | <0.002 | circumbinary planet | Orosz et al. (2012b) |
| KIC 10091110 | 4.2185174 | ~89 | <0.002 | double binary | This paper |
| KIC 12351927 | 10.116148 | 3+1 | <0.003 | circumbinary planet | Kostov et al. (2014) |
| KIC 12644769 | 41.077587 | 7 | <0.003 | circumbinary planet | Marsh et al. (2014) |
Notes: (a) All the numbers with < are the estimated upper limit. The value is the whole variation range of the O−C curve. If the variation is sinusoidal, this value should be twice the amplitude of the sine curve. (b) Welsh et al. (2015). (c) Estimated from the outer planet period.
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