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  Kepler planet host candidates imaging (Lillo-Box+, 2014)
    J/A+A/566/A103/table1(c)*Observational information, completeness, and detectability magnitudes (Note) (207 rows)
    J/A+A/566/A103/table3Photometry of the 23 active and 18 demoted KOIs with detected companions that are closer than 6arcsec in the new sample observed during 2012 and 2013 (100 rows)
    J/A+A/566/A103/table4(c)Sensitivity limit results (at 5σ level) for all observed tagets in the 2011, 2012 and 2013 observing seasons. (264 rows)
    J/A+A/566/A103/table7Results of the blended source probability prior and after the AstraLux images for 222 planet candidates around isolated KOIs from all 3 observing runs (Type=0) and KOIs with detected companions at 3-6" from the 2012 and 2013 observing runs (Type=1) (280 rows)
    J/A+A/566/A103/table10*Comparison between the improvements in the BSC parameter obtained by using the H11, A12 and our high-resolution images for all planet candidates involved (28 in H11 and 27 in A12) (Note) (33 rows)
    J/A+A/566/A103/table11Comparison between the blended source probabilities (PBS) obtained by using the L13 (Law et al. 2014ApJ...791...35L) and our high-resolution images for coincident planet candidates (167 rows)

       (c)  indicates tables which contain celestial coordinates 
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