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/690/A262
  Phosphorus-rich stars. II. (Brauner+, 2024)
Post annotation
img(gal)
1.J/A+A/690/A262/linesLine list of the light and heavy elements including wavelength, excitation potential and oscillator strength (1661 rows)
2.J/A+A/690/A262/modifModifications applied on the original VALD log(gf) of transitions close to a line of interest (32 rows)
3.J/A+A/690/A262/lightabu(c)Abundances of the light (Z<30) elements (132 rows)
4.J/A+A/690/A262/uncert*Uncertainties associated with the heavy (Z>30) elements due to deviations in atmospheric parameters (Note) (22 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)
   (ALL)El (char) Element symbol + excitation state (phys.atmol.excitation)
  (1+2)lambda 0.1nm Wavelength in angstrom (em.wl)
  (1)n_lambda (char) [*] Note on lambda (Note 1)   (meta.note)
  (1+2)EP eV Excitation potential of the line (phys.atmol.excitation;spect.line)
  (1)log(gf) [-] Oscillator strength of the line (spect.line.intensity)
  (1)Mol/Isotope? (char) Is line a molecular line, indicating the molecule; or from isotope(s) (meta.code)
  (2)Line-to-improve 0.1nm (n) Wavelength in angstrom of the line to improve (em.wl)
  (2)Species-modified (char) Element symbol + excitation state of the modified species (phys.atmol.excitation)
  (2)log(gf)VALD [-] Oscillator strength of the line before modification (phys.atmol.oscStrength)
  (2)log(gf)MOD [-] Oscillator strength of the line after modification (phys.atmol.oscStrength)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)n_log(gf)MOD (char) [+] Note on log(gf)MOD (Note 1)   (meta.note)
  (3)Molecule? (char) Is abundance derived from molecular lines, indicating the molecule (meta.code)
  (3)Star (char) ID of the Star, 2MHHMMSSss+DDMMSSs (meta.id;meta.main)
  (3)l_[X/Fe] (char) Limit flag on [X/Fe] (meta.code.error;phys.abund)
  (3)[X/Fe] [-] (n) Abundance compared to solar (phys.abund)
  (3)sigma-std [-] (n) Line-to-line standard deviation (stat.stdev)
  (3)N  (n) Number of lines (meta.number)
  (3)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)
  (3)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)
  (3)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)
  (4)deltaTeff [-] Systematic uncertainty related to effective temperature (stat.error)
  (4)deltalogg [-] Systematic uncertainty related to surface gravity (stat.error)
  (4)deltamicrovel [-] Systematic uncertainty related to microturbulence velocity (stat.error.sys;phys.veloc.microTurb)
  (4)sigmaparam [-] The total uncertainty equal to the square root of the sum of the parameter deviations squared (stat.error)

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