VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/ApJ/934/110
  Abundance analysis of 4 HES metal-poor stars (Shejeelammal+, 2022)
Post annotation
img(gal)
1.J/ApJ/934/110/table11Lines used to derive the elemental abundance from spectral synthesis (31 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  lambda 0.1nm [4118.7/7800.3] Wavelength, Angstroms (em.wl)
  El (char) Element (phys.atmol.element)
  Elow eV [0/4.1] Energy, lower level (phys.energy;phys.atmol.level)
  loggf [-] [-2.3/0.7] Log, statistical weight*oscillator strength (stat.weight;phys.atmol.oscStrength)
  Ab-HE0457 [-] (n) [-0.2/4.5] Derived absolute abundance for line, HE 0457-1805 (phys.abund)
  Ab-HE0920 [-] (n) [-0.5/4.5] Derived absolute abundance for line, HE 0920-0506 (phys.abund)
  Ab-HE1241 [-] (n) [-1.6/3.6] Derived absolute abundance for line, HE 1241-0337 (phys.abund)
  Ab-HE1327 [-] (n) [-1.2/3.7] Derived absolute abundance for line, HE 1327-2116 (phys.abund)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
Adapt form
Display your selection only Reset to default columns
usage  Display UCD1+    UCD1  
elapse time 0

Cite/acknowledge VizieR catalogue
Rules of usage of VizieR data

© UDS/CNRS

Contact