VizieR

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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/631/A43
  Late-type stars FeI & FeII NLTE line formation (Mashonkina+, 2019)
Post annotation
img(gal)
1.J/A+A/631/A43/stars(c)List of studied stars (41 rows)
2.J/A+A/631/A43/table2LTE and NLTE abundances of three halo stars (151 rows)
3.J/A+A/631/A43/table4LTE and NLTE abundances of the dSph stars (38 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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Column  Constraint Explain   (UCD)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1)FileName (char) Name of the table with data for this star (meta.id;meta.table)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)SimbadName (char) Designation understandable by the Simbad data-base (meta.id)
  (1+3)Star (char) Star designation (meta.id;meta.main)
  (2)Eexc eV Excitation energy (phys.atmol.excitation)
  (2)El (char) Atom (meta.id;spect.line)
  (2)epsLTE1  (n) HD 84937 LTE abundance (log eps(H)=12) (phys.abund)
  (2)epsLTE2  (n) HD 140283 LTE abundance (log eps(H)=12) (phys.abund)
  (2)epsLTE3  (n) HD 122563LTE abundance (log eps(H)=12) (phys.abund)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)epsNLTEB1  (n) HD 84937 NLTE abundance (log eps(H)=12), B18 recipe (phys.abund)
  (2)epsNLTEB2  (n) HD 140283 NLTE abundance (log eps(H)=12), B18 recipe (phys.abund)
  (2)epsNLTEB3  (n) HD 122563NLTE abundance (log eps(H)=12), B18 recipe (phys.abund)
  (2)epsNLTEY1  (n) HD 84937 NLTE abundance (log eps(H)=12), YBK18 (phys.abund)
  (2)epsNLTEY2  (n) HD 140283 NLTE abundance (log eps(H)=12), YBK18 (phys.abund)
  (2)epsNLTEY3  (n) HD 122563NLTE abundance (log eps(H)=12), YBK18 (phys.abund)
  (2)EW1 0.1pm (n) Equivalent width in HD 84937 (spect.line.eqWidth)
  (2)EW2 0.1pm (n) Equivalent width in HD 140283 (spect.line.eqWidth)
  (2)EW3 0.1pm (n) Equivalent width in HD 122563 (spect.line.eqWidth)
  (2)Ion (char) Ion (phys.atmol.ionStage)
  (2)lambda 0.1nm Wavelength (em.wl)
  (2)loggf  Adopted gf-value (phys.absorption.coeff)
  (3)e_epsL1  Dispersion of FeI LTE abundance (stat.error)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)e_epsL2  Dispersion of FeII LTE abundance (stat.error)
  (3)e_epsN1  Dispersion of FeI NLTE abundance (stat.error)
  (3)e_epsN2  Dispersion of FeII NLTE abundance (stat.error)
  (3)epsL1  Mean FeI LTE abundance (log eps(H)=12) (phys.abund)
  (3)epsL2  Mean FeII LTE abundance (log eps(H)=12) (phys.abund)
  (3)epsN1  Mean FeI NLTE abundance (log eps(H)=12) (phys.abund)
  (3)epsN2  Mean FeII NLTE abundance (log eps(H)=12) (phys.abund)
  (3)[Fe/H]  Metallicity (phys.abund.Fe)
  (3)logg [cm/s2] Surface gravity (phys.gravity)
  (3)NFeI  Number of FeI lines (meta.number)
  (3)NFeII  Number of FeII lines (meta.number)
  (3)Teff K Effective temperature (phys.temperature.effective)
  (3)xi km/s Microturbulent velocity (phys.veloc)

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