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J/A+A/692/A212
  Metallicity of open clusters (Zhang+, 2024)
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2024A&A...692A.212Z
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Post annotation 		img(gal)
1.J/A+A/692/A212/table1(c)Radial velocities for the OCs studied here compared to those from the literature (1131 rows)
2.J/A+A/692/A212/tablea1(c)Basic information of OCs in the present samples (1121 rows)
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Simple ConstraintList Of Constraints
 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)[Fe/H] (char) indicates [Fe/H] values in tablea1 (meta.ref.url)
   (ALL)Cluster (char) (i) Name or identifier of the astronomical cluster being studied (meta.id;meta.main)
   (ALL)RA_ICRS "h:m:s" (i) Right ascension of the cluster (ICRS) (pos.eq.ra;meta.main)
   (ALL)DE_ICRS "d:m:s" (i) Declination of the cluster (ICRS) (pos.eq.dec;meta.main)
  (1)RV-LRS km/s (n) Radial velocity measured using low-resolution spectroscopy (LRS) LAMOST (phys.veloc;pos.heliocentric)
  (1)e_RV-LRS km/s (n) Uncertainty or error in the radial velocity measurement from low-resolution spectroscopy (LRS) (stat.error)
  (1)RV-HRS km/s (n) Radial velocity measured using high-resolution spectroscopy (HRS) LAMOST (phys.veloc;pos.heliocentric)
  (1)e_RV-HRS km/s (n) Uncertainty or error in the radial velocity measurement from high-resolution spectroscopy (HRS) (stat.error)
  (1)RV-GaiaDR3 km/s (n) Radial velocity obtained from the Gaia Data Release 3 (Gaia DR3) measurements (phys.veloc;pos.heliocentric)
  (1)e_RV-GaiaDR3 km/s (n) Uncertainty or error in the radial velocity measurement from Gaia Data Release 3 (Gaia DR3) (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)Rgc kpc Galactocentric distance of the cluster (pos.distance;pos.galactocentric)
  (2)Lz kpc.km/s Vertical component of angular momentum about the Z-axis (the axis perpendicular to the galactic plane) (phys.angMomentum)
  (2)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)
  (2)Rbirth kpc Birth radius, indicating the distance from the center of the cluster where stars formed (phys.size.radius)
  (2)[Fe/H]ANN  Metallicity of the cluster as determined by the ANN (Artificial Neural Network) method (phys.abund.Fe)
  (2)e_[Fe/H]ANN  Uncertainty or error associated with the [Fe/H]ANN metallicity measurement (stat.error;phys.abund.Fe)
  (2)[Fe/H]MCMC  Metallicity of the cluster determined using Markov Chain Monte Carlo (MCMC) method (phys.abund.Fe)
  (2)e_[Fe/H]MCMC  Uncertainty or error associated with the [Fe/H]MCMC metallicity measurement (stat.error;phys.abund.Fe)
  (2)Nmemb  Number of stars or members within the cluster used in the analysis (meta.number)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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