VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/AJ/156/286
  The LEECH exoplanet imaging survey (Stone+, 2018)
ReadMe+ftp
2018AJ....156..286S
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Post annotation 		img(gal)
1.J/AJ/156/286/table3Best-fit age, mass, and metallicity for observed stars in the Field-B/A sublist (35 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)
  Name (char) Star name (meta.id;meta.main)
  Age Myr [50/1646] Best-fit age (time.age;meta.modelled)
  b_Age16-84 Myr [14/1249] Lower value of age in the interval between 16% and 84% in the cumulative distribution function of the posterior probability distribution (time.age;stat.min)
  B_Age16-84 Myr [81/1723] Upper value of age in the interval between 16% and 84% in the cumulative distribution function of the posterior probability distribution (time.age;stat.max)
  b_Age2.5-97.5 Myr [7/1045] Lower value of age in the interval between 2.5% and 97.5% in the cumulative distribution function of the posterior probability distribution (time.age;stat.min)
  B_Age2.5-97.5 Myr [124/5477] Upper value of age in the interval between 2.5% and 97.5% in the cumulative distribution function of the posterior probability distribution (time.age;stat.max)
  Mass Msun [1.5/4.5] Best-fit mass (phys.mass;meta.modelled)
  b_Mass16-84 Msun [1.4/4.4] Lower value of mass in the interval between 16% and 84% in the cumulative distribution function of the posterior probability distribution (phys.mass;stat.min)
  B_Mass16-84 Msun [1.5/4.5] Upper value of mass in the interval between 16% and 84% in the cumulative distribution function of the posterior probability distribution (phys.mass;stat.max)
  b_Mass2.5-97.5 Msun [1.4/4.3] Lower value of mass in the interval between 2.5% and 97.5% in the cumulative distribution function of the posterior probability distribution (phys.mass;stat.min)
  B_Mass2.5-97.5 Msun [1.5/4.5] Upper value of mass in the interval between 2.5% and 97.5% in the cumulative distribution function of the posterior probability distribution (phys.mass;stat.max)
  logZ [Sun] [-0.26/0.04] Best-fit metallicity log10(Z/Z☉) (phys.abund.Z;meta.modelled)
  b_logZ16-84 [Sun] [-0.27/-0.11] Lower value of metallicity in the interval between 16% and 84% in the cumulative distribution function of the posterior probability distribution (phys.abund.Z;stat.min)
  B_logZ16-84 [Sun] [-0.13/0.09] Upper value of metallicity in the interval between 16% and 84% in the cumulative distribution function of the posterior probability distribution (phys.abund.Z;stat.max)
  b_logZ2.5-97.5 [Sun] [-0.3/-0.17] Lower value of metallicity in the interval between 2.5% and 97.5% in the cumulative distribution function of the posterior probability distribution (phys.abund.Z;stat.min)
  B_logZ2.5-97.5 [Sun] [-0.04/0.19] Upper value of metallicity in the interval between 2.5% and 97.5% in the cumulative distribution function of the posterior probability distribution (phys.abund.Z;stat.max)

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