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/700/L13
  Variable stars in Galactic open clusters (Hunt+, 2025)
Post annotation
img(gal)
1.J/A+A/700/L13/tableb1(c)Variable star classifications (34762 rows)
2.J/A+A/700/L13/tableb2(c)Absolute dereddened cluster photometry (173294 rows)
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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)
   (ALL)GaiaDR3  Gaia DR3 source ID (meta.id;meta.main)
   (ALL)Cluster (char) Host cluster name (meta.id.parent)
  (1)Class (char) Gaia DR3 best variability classification (Rimoldini et al., 2023A&A...674A..14R, See Cat. I/358) (meta.code.class)
  (1)fCep   [0/1] Flag indicating if star is in Gaia DR3 Cepheid table (meta.code)
  (1)fRB   [0/1] Flag indicating if star is in Gaia DR3 eclipsing binary table (meta.code)
  (1)fLPV   [0/1] Flag indicating if star is in Gaia DR3 long-period variable table (meta.code)
  (1)fMSOsc   [0/1] Flag indicating if star is in Gaia DR3 main sequence oscillators table (meta.code)
  (1)frotmod   [0/1] Flag indicating if star is in Gaia DR3 rotation modulation table (meta.code)
  (1)fRRLyr   [0/1] Flag indicating if star is in Gaia DR3 RR Lyrae table (meta.code)
  (1)fShortTS   [0/1] Flag indicating if star is in Gaia DR3 short-timescale variability table (meta.code)

ALL cols
    
 (i)indexed column
   (ALL)_RA deg (i) Positions from Gaia DR3 (right ascension part) (pos.eq.ra;meta.main)
   (ALL)_DE deg (i) Positions from Gaia DR3 (declination part) (pos.eq.dec;meta.main)
  (2)GMAG mag Absolute dereddened G-band magnitude (phot.mag.reddFree)
  (2)BP-RP mag Absolute dereddened BP-RP color (phys.magAbs)
  (2)logAge [yr] Log of host cluster age (log base 10) (Note 1)   (time.age)
  (2)Ext mag Extinction of host cluster (Note 1)   (phys.absorption)
  (2)Dist pc Distance to host cluster based on parallax (Note 1)   (pos.distance)

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