Table 1
Ancillary data and calculated blended source confidence values for the three KOIs studied in this paper.
| KOI | High-res im.a | Comp. | Sep. | ΔmKep | BSCb | ||
| Ref. | (<6′′) | arcsec. | mag | (%) | |||
|
|
|||||||
| 554 | CFOP | B | 5.65′′ | 1.68 | – | ||
| 1074 | CFOP | 0 | – | – | – | ||
| 3728 | LB14 | 0 | – | – | 99.6% | ||
Notes.
LB14 = Lillo-Box et al. (2014a), 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 blended source confidence parameter (BSC) provides the probability that no chance-aligned eclipsing binaries are responsible for the detected transit signal given a high spatial resolution image while taking into account its sensitivity limits (see Lillo-Box et al. 2014a).
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