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VizieR

  
J/PASP/124/401
  Chemical composition of BE Lyn (Kim+, 2012)
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2012PASP..124..401K
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Objects
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1.J/PASP/124/401/table2Lines of chemical elements in spectrum of BE Lyn (except iron) (242 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. ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc)
  Ion  Ion numerial code (FeI=26.00) ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  lambda 0.1nm Wavelength ((unassigned);phys.veloc.orbital;arith.diff;meta.bib.author)
  loggf [-] Oscillator strength ((unassigned);(unassigned);(unassigned);(unassigned))
  r_loggf  Reference for loggf, in refs.dat file ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.dispersion;€?**ucdid=0**?)
  Elow eV Excitation potential ((unassigned);(unassigned);(unassigned);(unassigned))
  DlogN [-] Differential abundance, Be Lyn - Sun (in the scale of logN(H)=12) ((unassigned);phys.veloc.orbital;arith.diff;phys.polarization.stokes.Q)
  logN* [-] BE Lyn abundance (in the scale of logN(H)=12) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  logNS [-] (n) Sun abundance (in the scale of logN(H)=12) ((unassigned);phys.veloc.orbital;arith.diff;phys.polarization.stokes.Q)
  Bl*  (n) Be Lyn level of blending of the line in the synthetic spectra (1 = clean line, 0.0 = strong blended line) ((unassigned);phys.veloc.orbital;arith.diff;pos.eq.dec)
  n_Bl* (char) [h] h for hfs: hyperfine splitting ((unassigned);(unassigned);(unassigned);phys.veloc.orbital)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  BlS  (n) Sun level blending of the line in the synthetic spectra (1 = clean line, 0.0 = strong blended line) ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  n_BlS (char) [h] h for hfs: hyperfine splitting ((unassigned);(unassigned);(unassigned);phys.veloc.orbital)
  D*  BE Lyn depth of the line in synthetic spectra ((unassigned);(unassigned);(unassigned);phys.atmol.sWeight.nuclear;instr.offset)
  DS  (n) Sun depth of the line in synthetic spectra ((unassigned);(unassigned);(unassigned);phys.atmol.sWeight.nuclear;instr.offset)
  dA(T) [-] Correction for abundance, by an effective temperature decrease of 200K ((unassigned);phys.veloc.orbital;arith.diff;instr.beam)
  dA(g) [-] Correction for abundance, by a gravity increase of 0.3dex ((unassigned);(unassigned);(unassigned);instr.beam)
  dA(vt) [-] Correction for abundance, by a microturbulent velocity increase of 0.5km/s ((unassigned);phys.veloc.orbital;arith.diff;instr.beam)
  D  Depth of the line in convoluted synthetic spectra (pos.galactic.lon;(unassigned);stat.min;phys.atmol.sWeight.nuclear;instr.offset)
  dD1  Correction to the best depth of the line in the synthetic spectrum found by changing the abundance of the investigated chemical element by -0.5dex ((unassigned);(unassigned);(unassigned);instr.beam)
  dD2  Correction to the best depth of the line in the synthetic spectrum found by changing the abundance of the investigated chemical element by +0.5dex ((unassigned);(unassigned);(unassigned);instr.beam)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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usage  Display UCD1+    UCD1  

The following problems were encountered in this VizieR run:
****Error execute query: UPDATE METAstat set nother=nother+1, tother=846456001 Where phase=3 and catid=61240401
**** 
**** --POSTGRES MSG db=1
**** Report from: stdb_pg,     Status: STDB_ERR 
****ERROR:  invalid page in block 0 of relation base/16403/6104 
****ERROR:  invalid page in block 0 of relation base/16403/6104
If you can't find a solution, report to CDS and insert into your message the following details:

.errorfile=/tmp/VR476111.err (2026-10-27T22:39:59)
-3
-source=J/PASP/124/401/table2
-ref=VIZ6ae12841743cf
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