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J/A+A/546/A10
  Multiplicity in transiting planet-host stars (Lillo-Box+, 2012)
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2012A&A...546A..10L
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1.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)

Simple ConstraintList Of Constraints
 
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)
  KOI   [99/1574] KOI number (Note 2)   (meta.id;meta.main)
  Pl   [01/03] Planet candidate (Note 2)   (meta.code.multip)
  depth.c 10-6 Catalog planet-transit depth (in ppm) (phot.flux;arith.ratio)
  depth 10-6 New planet-transit depth (in ppm) (phot.flux;arith.ratio)
  e_depth 10-6 rms uncertainty on depth (in ppm) (stat.error;phys.absorption.opticalDepth)
  Rp/R*.c 10-2 Catalog planet-to-star radii ratio (phys.size;arith.ratio)
  e_Rp/R*.c 10-2 rms uncertainty on Rp/R*.c (stat.error)
  Rp/R* 10-2 New planet-to-star radii ratio assuming no limb-darkening (phys.size;arith.ratio)
  e_Rp/R* 10-2 rms uncertainty on Rp/R* (stat.error)
  Rp/R*.2 10-2 Planet-to-star radius assuming that the host is actually the secondary companion detected at less than 3 arcsec (phys.size;arith.ratio)
  e_Rp/R*.2 10-2 rms uncertainty on Rp/R*.2 (stat.error)
  Rp.c Rgeo Planet radii calculated by the Kepler team (Batalha et al., 2012, ApJS, submitted) (phys.size.radius)
  Rp Rgeo Planet radii assuming the new depth and no limb-darkening (Note 1)   (phys.size.radius)
  M  KOI original data from Borucki et al. 2011, Cat. J/ApJ/736/19 (meta.ref.url)

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