VizieR

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

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
 Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/A+A/692/A212
  Metallicity of open clusters (Zhang+, 2024)
ReadMe+ftp
2024A&A...692A.212Z
Similar Catalogs
Post annotation 		img(gal)
1.J/A+A/692/A212/tablea1Basic information of OCs in the present samples (1121 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)
  Cluster (char) Name or identifier of the astronomical cluster being studied (meta.id;meta.main)
  RA_ICRS "h:m:s" (i) Right ascension of the cluster (ICRS) (pos.eq.ra;meta.main)
  DE_ICRS "d:m:s" (i) Declination of the cluster (ICRS) (pos.eq.dec;meta.main)
  Rgc kpc Galactocentric distance of the cluster (pos.distance;pos.galactocentric)
  Lz kpc.km/s Vertical component of angular momentum about the Z-axis (the axis perpendicular to the galactic plane) (phys.angMomentum)
  Rguiding kpc Guiding radius, which indicates the effective distance from the center of the cluster at which stars are significantly influenced by the cluster's gravitational field (phys.size.radius)
  Rbirth kpc Birth radius, indicating the distance from the center of the cluster where stars formed (phys.size.radius)
  [Fe/H]ANN  Metallicity of the cluster as determined by the ANN (Artificial Neural Network) method (phys.abund.Fe)
  e_[Fe/H]ANN  Uncertainty or error associated with the [Fe/H]ANN metallicity measurement (stat.error;phys.abund.Fe)
  [Fe/H]MCMC  Metallicity of the cluster determined using Markov Chain Monte Carlo (MCMC) method (phys.abund.Fe)
  e_[Fe/H]MCMC  Uncertainty or error associated with the [Fe/H]MCMC metallicity measurement (stat.error;phys.abund.Fe)
  Nmemb  Number of stars or members within the cluster used in the analysis (meta.number)

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