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J/AJ/152/8/table7 Impact of stellar multiplicity on planetary systems I. (Kraus+, 2016)
System properties for candidate binary systems (463 rows)
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ColumnValue  Explain   (UCD)
47recno 47  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)

GrB  Group type (M=Masking, B=PSF fitting binary, T=PSF fitting triple, or I=Imaging) (
KOI2542  Kepler Object of Interest number (linked to stellar parameters in table1 ) (;meta.main)

I/PSF 1  Number of Keck/NIRC2 imaging or PSF-fitting (table 5 or 6) (meta.number)
Iml 1  Number of Keck/NIRC2 imaging detection limits (table4) (meta.number)
NRMl 1  Number of Keck/NIRC2 NRM detection limits (table2) (meta.number)
NRMc   Indicates a Keck/NIRC2 NRM candidate companion (table3) (meta.ref.url)

l_Mass2    [<] Upper limit flag on Mass2 (meta.code.error)
Mass2 0.182 Msun [0.099/1.597] Secondary mass (Msec) (phys.mass)
l_M2/M1    [<] Upper limit flag on M2/M1 (meta.code.error)
M2/M1 0.628   [0.068/1.021] Ratio of secondary to primary masses (q) (phys.mass;arith.ratio)
Sep 85.7 AU [4.7/12439.1] Separation (pos.angDistance)
elapse time 0

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