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/711/A215
  XP-TEAL. Balmer lines in open clusters (Carrasco+, 2026)
Post annotation
img(gal)
1.J/A+A/711/A215/tableb1(c)Color excess and interstellar absorptions derived for clusters in Hunt & Reffert, 2023A&A...673A.114H, Cat. J/A+A/673/114 (7135 rows)
2.J/A+A/711/A215/tableb2(c)Balmer lines widths for members of the clusters in Hunt & Reffert, 2023A&A...673A.114H, Cat. J/A+A/673/114 (608159 rows)
3.J/A+A/711/A215/tableb3Mastercurves used to determine the color excess in BP-RP (1972 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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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+2)Cluster (char) Name of the cluster (meta.id;meta.main)
  (1)RAJ2000 deg (i) Right ascension (J2000) of the cluster (pos.eq.ra;meta.main)
  (1)DEJ2000 deg (i) Declination (J2000) of the cluster (pos.eq.dec;meta.main)
  (1)E(BP-RP) mag Colour excess in BP-RP of the cluster based on the mastercurves in TableB3 (phot.color.excess)
  (1)AG mag Absorption of the cluster in Gaia G band predicted from EBPRP (phys.absorption)
  (1)AV mag Absorption of the cluster in Johnson V band predicted from EBPRP (phys.absorption)
  (1)E(H-K) mag Excess in H-K 2MASS colour (phot.color;em.IR.H;em.IR.K)
  (1)E(J-H) mag Excess in J-H 2MASS colour (phot.color.excess)
  (1)E(BP-K) mag Excess in BP-K Gaia-2MASS colour (phot.color.excess)
  (1)GoodEx   [0/1] Flag indicating if determination of E(BP-RP) is considered of good quality (meta.code.error)

ALL cols
    
 (i)indexed column
  (1)OC   [0/1] Flag indicating if the cluster is considered as open cluster (meta.code)
  (2)GaiaDR3  Gaia DR3 source identifier (meta.id;meta.main)
  (2)RA_ICRS deg (i) Right ascension (ICRS) at Ep=2016.0 of the star (pos.eq.ra;meta.main)
  (2)DE_ICRS deg (i) Declination (ICRS) at Ep=2016.0 of the star (pos.eq.dec;meta.main)
  (2)Gmag mag Gaia DR3 magnitude in G (phot.mag;em.opt)
  (2+3)BP-RP mag Gaia DR3 GBP–GRP colour (phot.color;em.opt.B;em.opt.R)
  (2+3)EWHa nm Equivalent width of the hydrogen alpha Balmer line (spect.line.eqWidth)
  (2)e_EWHa nm Standard error of EWHa (stat.error)
  (2)HaP  (n) P-value significance of the local extremum of the hydrogen alpha Balmer line (stat.fit.goodness)
  (2)HaD nm (n) Line width of the hydrogen alpha Balmer line relative to the LSF width (spect.line.width)
  (2)HaOrder (char) Detection order of the hydrogen alpha Balmer line (Note 1)   (phys.atmol)
  (2)HaRelEm (char) Relative emission of the hydrogen alpha Balmer line (phys.emissivity)
  (2+3)EWHb nm Equivalent width of the hydrogen beta Balmer line (spect.line.eqWidth)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)e_EWHb nm Standard error of EWHb (stat.error)
  (2)HbP  (n) P-value significance of the local extremum of the Hbeta line (stat.fit.goodness)
  (2)HbD  (n) Line width of the hydrogen beta Balmer line relative to the LSF width (spect.line.width)
  (2)HbOrder (char) Detection order of the hydrogen beta Balmer (Note 1)   (phys.atmol)
  (2)HbRelEm (char) Relative emission of the hydrogen beta Balmer line (phys.emissivity)
  (2+3)EWHg nm Equivalent width of the hydrogen gamma Balmer line (spect.line.eqWidth)
  (2)e_EWHg nm Standard error of EWHg (stat.error)
  (2)HgP  (n) P-value significance of the local extremum of the hydrogen gamma Balmer line (stat.fit.goodness)
  (2)HgD  (n) Line width of the hydrogen gamma Balmer line relative to the LSF width (spect.line.width)
  (2)HgOrder (char) Detection order of the hydrogen gamma Balmer line (Note 1)   (phys.atmol)
  (2)HgRelEm (char) Relative emission of the hydrogen gamma Balmer line (phys.emissivity)
  (2)OC (char) [F/T] Flag indicating if the cluster is considered open cluster (meta.code)
  (2)EmLit (char) [F/T] Flag indicating if the cluster is considered an emitter by the literature (meta.code)

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