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  Impact of stellar multiplicity on planetary systems I. (Kraus+, 2016)
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1.J/AJ/152/8/table7System properties for candidate binary systems (463 rows)

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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Gr (char) Group type (M=Masking, B=PSF fitting binary, T=PSF fitting triple, or I=Imaging) (
  KOI  Kepler Object of Interest number (;meta.main)
  I/PSF  (n)Number of Keck/NIRC2 imaging or PSF-fitting (table 5 or 6) (meta.number)
  Iml  (n)Number of Keck/NIRC2 imaging detection limits (table4) (meta.number)
  NRMl  (n)Number of Keck/NIRC2 NRM detection limits (table2) (meta.number)
  NRMc (char) Indicates a Keck/NIRC2 NRM candidate companion (table3) (meta.ref.url)
  l_Mass2 (char) [<] Upper limit flag on Mass2 (meta.code.error)
  Mass2 Msun [0.099/1.597] Secondary mass (Msec) (phys.mass)
  l_M2/M1 (char) [<] Upper limit flag on M2/M1 (meta.code.error)
  M2/M1   [0.068/1.021] Ratio of secondary to primary masses (q) (phys.mass;arith.ratio)
  Sep AU [4.7/12439.1] Separation (pos.angDistance)

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