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J/A+A/546/A10
  Multiplicity in transiting planet-host stars (Lillo-Box+, 2012)
img(gal)
    J/A+A/546/A10/table3(c)Estimated spectral types for objects with i-z>0.21 (11 rows)
    J/A+A/546/A10/table4(c)Observing information of the 41 non-isolated objects in our sample (59 rows)
    J/A+A/546/A10/multiplePhotometric and astrometric results for companions detected in our KOI sample, closer than 3'' (table5) and between 3-6'' (table6) (93 rows)
    J/A+A/546/A10/table7(c)Spectral-energy-distribution fitting results for the medium-distance companions with 2MASS counterparts (29 rows)
    J/A+A/546/A10/table8*New planet-transit depth and relative radii to the parent star accounting for the blended objects in the Kepler images (Note) (23 rows)

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       (c)  indicates tables which contain celestial coordinates 
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