Table 1
Ancillary data and calculated BSC (blended source confidence) values for the KOIs studied in this paper.
| KOI | High-Res Im.a | Comp. | Sep. | Δm | BSC |
| Ref. | (<6′′) | arcsec. | mag (band) | % | |
|
|
|||||
| Group A − Eclipsing binaries | |||||
|
|
|||||
| 340.01 | L13 | 0b | 99.99 | ||
| 371.01 | L13 | 0b | 96.0 | ||
| 686.01 | LB14 | 0 | 99.9 | ||
| 3725.01 | LB14 | 0 | 99.7 | ||
| 3853.01 | LB14 | 0 | 99.6 | ||
|
|
|||||
| Group B − Fast rotators | |||||
|
|
|||||
| 12.01 | LB14 | 0 | 99.3 | ||
| 131.01 | LB12 | 1 | 5.54′′ | 3.48 (iSDSS) | − |
| 366.01 | LB14 | 0 | 99.3 | ||
| 625.01 | LB14 | 0 | 96.8 | ||
| 972.01 | CFOP | 0 | − | ||
| 3728.01 | LB14 | 0 | 99.6 | ||
|
|
|||||
| Group C − Unsolved cases | |||||
|
|
|||||
| 1463.01 | CFOP | 1 | 5.47′′ | 6.9 (Kep.) | − |
| 3890.01 | LB14 | 0 | 98.3 | ||
Notes. Uncertainties in the angular separation of the companions and in their magnitude difference have been omitted for clarification purposes. We refer to the corresponding references for more information about this.
LB12 = Lillo-Box et al. (2012), L13 = Law et al. (2014), LB14 = Lillo-Box et al. (2014c), CFOP = no reference found in the bibliography but companion tables of the UKIRT J-band survey by D. Ciardi are available in the CFOP.
The maximum angular separation explored in Law et al. (2014) is 2.5 arcsec.
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