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  Kepler planet host candidates imaging (Lillo-Box+, 2014)
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1.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)

Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  n_KOI (char) [AD] Active or Demoted KOI (Note G1)   (meta.note)
  KOI   [1/4512] KOI of Planet candidate (;meta.main)
  Type   [0/1] Isolated (0) or not (1) type (Note 1)   (meta.code)
  kepmag mag Kepler magnitude (phot.mag;em.opt)
  Dmmax mag Maximum contrast (with respect to the measured flux) (phot.mag)
  PBS0 % Prior probability of having a blended source (
  PBS14 % This paper high-resolution images improvements in the BSC parameter (
  Imp % (n) Corresponding improvement to PBS0 obtained with our high-resolution observations (
  PEB % (n) Probability of that source being an appropriate eclipsing binary (stat)
  PBB % (n) Probability of having a blended eclipsing binary (stat)

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