VizieR

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

VizieR

  
J/AJ/145/167
  Abundances of LX Per (Kang+, 2013)
ReadMe+ftp
2013AJ....145..167K
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Objects
Post annotation 		  
1.J/AJ/145/167/linesLines of non-iron elements in the spectrum of LX Per (tables 5 and 6) (233 rows)

Simple ConstraintList Of Constraints
 
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)
  M  Mean abundance for this element (meta.ref.url)
  Ion (char) Elemental line identification (phys.atmol.ionStage)
  lambda 0.1nm [4497/9238] Line wavelength; in Å (em.wl;spect.line)
  C (char) hotter (table5) or cooler (table6) component (meta.code.multip)
  loggf [-] Log of the oscillator strength (phys.atmol.oscStrength)
  f_loggf (char) [h] Flag on loggf (h) (Note 1)   (meta.code)
  r_loggf (char) Reference for loggf; in refs.dat file (meta.ref;pos.frame)
  Elow eV Excitation energy of lower level (phys.energy;phys.atmol.level)
  logN [-] Derived abundance in LX Per (H=12) (phys.abund)
  logNo [-] (n) Derived abundance in the Sun (H=12) (phys.abund)
  Abun [Sun] LX Per abundance relative to the Sun (phys.abund)
  Bl   [0/1] Blending in LX Per (1=clean line) (meta.note)
  Blo  (n) [0/1] Blending in the Sun (1=clean line) (meta.note)
  D   [0/1] LX Per depth in synthetic spectrum (phot.flux.density;arith.ratio)
  Do  (n) [0/1] Solar depth in synthetic spectrum (phot.flux.density;arith.ratio)
  e(g) [-] LX Per error in abundance for a change in logg of +0.2dex (stat.error)
  e(T) [-] LX Per error in abundance for a change in effective temperature of +100K (stat.error)

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