VizieR

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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
Post annotation 		  
1.J/PASP/124/401/table1Iron Lines in Spectrum of BE Lyn (147 rows)
2.J/PASP/124/401/table2Lines of chemical elements in spectrum of BE Lyn (except iron) (242 rows)
3.J/PASP/124/401/refsReferences (22 rows)
4.J/PASP/124/401/table3Mean abundances of chemical elements in atmosphere of BE Lyn (34 rows)

Simple ConstraintList Of Constraints
 
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. ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc)
  (1+2)lambda 0.1nm Wavelength ((unassigned);phys.veloc.orbital;arith.diff;meta.bib.author)
  (1+4)Ion (char) Ion (Fe I or Fe II) ((unassigned);(unassigned);(unassigned);(unassigned))
  (1+2)loggf [-] Oscillator strength ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  (1+2)Elow eV Energy of low level ((unassigned);(unassigned);(unassigned);(unassigned);(unassigned))
  (1)EW 0.1pm Equivalent width (in mÅ) ((unassigned);(unassigned);(unassigned);phys.at.moment.magnetic;meta.main)
  (1+4)logN [-] Iron abundance (in the scale of logN(H)=12) ((unassigned);phys.veloc.orbital;arith.diff;phys.polarization.stokes.Q)
  (2)Ion  Ion numerial code (FeI=26.00) ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  (2)r_loggf  Reference for loggf, in refs.dat file ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.dispersion;€?**ucdid=0**?)
  (2+4)DlogN [-] Differential abundance, Be Lyn - Sun (in the scale of logN(H)=12) ((unassigned);phys.veloc.orbital;arith.diff;phys.polarization.stokes.Q)
  (2)logN* [-] BE Lyn abundance (in the scale of logN(H)=12) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

ALL cols		    
 (i)indexed column
  (2)logNS [-] (n) Sun abundance (in the scale of logN(H)=12) (time.equinox;(unassigned);arith.factor;phys.polarization.stokes.Q)
  (2)Bl*  (n) Be Lyn level of blending of the line in the synthetic spectra (1 = clean line, 0.0 = strong blended line) ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (2)n_Bl* (char) [h] h for hfs: hyperfine splitting ((unassigned);pos.wcs.naxis;arith.grad;phys.veloc.orbital)
  (2)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)
  (2)n_BlS (char) [h] h for hfs: hyperfine splitting ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.orbital)
  (2)D*  BE Lyn depth of the line in synthetic spectra ((unassigned);phys.veloc.orbital;arith.diff;phys.atmol.sWeight.nuclear;instr.offset)
  (2)DS  (n) Sun depth of the line in synthetic spectra ((unassigned);phys.veloc.orbital;arith.diff;phys.atmol.sWeight.nuclear;instr.offset)
  (2)dA(T) [-] Correction for abundance, by an effective temperature decrease of 200K ((unassigned);(unassigned);(unassigned);instr.beam)
  (2)dA(g) [-] Correction for abundance, by a gravity increase of 0.3dex ((unassigned);(unassigned);(unassigned);instr.beam)
  (2)dA(vt) [-] Correction for abundance, by a microturbulent velocity increase of 0.5km/s ((unassigned);(unassigned);(unassigned);instr.beam)
  (2)D  Depth of the line in convoluted synthetic spectra ((unassigned);(unassigned);(unassigned);phys.atmol.sWeight.nuclear;instr.offset)
  (2)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)
  (2)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);phys.veloc.orbital;arith.diff;instr.beam)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)Ref  Reference number ((unassigned);(unassigned);(unassigned);spect.line.veloc;arith)
  (3)Com (char) Reference ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.dispersion;€?**ucdid=0**?)
  (4)Z  Atomic number ((unassigned);(unassigned);(unassigned);spect.line.veloc;arith)
  (4)n  Number of line used ((unassigned);(unassigned);(unassigned);src.var)
  (4)e_DlogN [-] (n) rms uncertainty on DlogN ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (4)DlogN1 [-] Relative abundance in BL Lyn atmosphere, effective temperature increased by 100K ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)e_DlogN1 [-] (n) rms uncertainty on DlogN1 ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (4)DlogN2 [-] Relative abundance in BL Lyn atmosphere, surface gravity decreased by 0.3dex ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)e_DlogN2 [-] (n) rms uncertainty on DlogN2 ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (4)DlogN3 [-] Relative abundance in BL Lyn atmosphere, microturbulent velocity increased by 0.5km/s ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)e_DlogN3 [-] (n) rms uncertainty on DlogN3 ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (4)e_logN [-] (n) rms uncertainty on logN ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (4)logN1 [-] Absolute abundance in BL Lyn atmosphere, effective temperature increased by 100K ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)e_logN1 [-] (n) rms uncertainty on logN1 ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (4)logN2 [-] Absolute abundance in BL Lyn atmosphere, surface gravity decreased by 0.3dex ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)e_logN2 [-] (n) rms uncertainty on logN2 ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (4)logN3 [-] Absolute abundance in BL Lyn atmosphere, microturbulent velocity increased by 0.5km/s ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)e_logN3 [-] (n) rms uncertainty on logN3 ((unassigned);(unassigned);(unassigned);time.age;meta.main)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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The following problems were encountered in this VizieR run:
****Error execute query: UPDATE METAstat set nother=nother+1, tother=846445816 Where phase=3 and catid=61240401
**** 
**** --POSTGRES MSG db=0
**** 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 
****Error execute query: UPDATE METAstat set nother=nother+1, tother=846445816 Where phase=3 and catid=61240401
**** 
**** --POSTGRES MSG db=0
**** 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 
****Error execute query: UPDATE METAstat set nother=nother+1, tother=846445816 Where phase=3 and catid=61240401
**** 
**** --POSTGRES MSG db=0
**** 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/VR259536.err (2026-10-27T19:50:13)
-3
-source=J/PASP/124/401
-ref=VIZ6ae100773f5d0
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