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J/AJ/144/35
  Abundances of the eclipsing binary ZZ Boo (Kang+, 2012)
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2012AJ....144...35K
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Abundances of eclipsing binary ZZ Bootis
Post annotation 		  
1.J/AJ/144/35/table1Iron lines in the spectrum of ZZ Boo (125 rows)
2.J/AJ/144/35/linesLines of non-iron elements in the spectrmu of ZZ Boo (tables 3 and 4) (277 rows)
3.J/AJ/144/35/table5Mean abundances of chemical elements in the atmospheres of components of ZZ Boo (59 rows)
4.J/AJ/144/35/refsReferences (23 rows)

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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)
  (1+2+3)Ion (char) Iron line identifier (Fe I or Fe II) linkRole{abundances of this ion} (phys.atmol.ionStage)
  (1+2)lambda 0.1nm [4508/8825] Wavelength; in Å (em.wl)
  (1)EW-A 10-13m (n) Component A equivalent width; in mÅ (spect.line.eqWidth)
  (1)EW-B 10-13m (n) Component B equivalent width; in mÅ (spect.line.eqWidth)
  (1+2)log(gf) [-] [-4.2/0.645] Log of the oscillatory strength (phys.atmol.collStrength)
  (1)r_log(gf)  Reference to log(gf), in refs.dat file (meta.ref;pos.frame)
  (1+2)Elow eV Lower energy level Elow (phys.energy;phys.atmol.level)
  (1)logN-A [-] (n) Component A abundance (where log N(H)=12) (phys.abund)
  (1)logN-B [-] (n) Component B abundance (where log N(H)=12) (phys.abund)
  (2+3)Comp (char) Component: A for primary, B for secondary (meta.code.multip)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
   (2+4)Ref  (n) [1/27] Reference to log(gf), in refs.dat file (meta.ref)
  (2)f_Ref (char) Flag on Ref (h) (Note 1)   (meta.code)
  (2)logN [-] [0.8/9.7] ZZ Boo abundance (log N(H)=12) (phys.abund)
  (2)logNo [-] (n) [0.8/8.7] Solar abundance (phys.abund)
  (2)DlogN [Sun] [-0.573/0.993] Abundance relative to the Sun (phys.abund)
  (2)Bl   [0/1] ZZ Boo blending (1=clean line) (meta.note)
  (2)Bl0  (n) [0/1] Solar blending (1=clean line) (meta.note)
  (2)D   [0/1] ZZ Boo Depth in synthetic spectra (phot.flux.density;arith.ratio)
  (2)Do  (n) [0/1] Solar depth in synthetic spectra (phot.flux.density;arith.ratio)
  (2)e(T)  (n) ZZ Boo error in abundance for a change in effective temperatures ±100K (stat.error)
  (2)e(g)  (n) ZZ Boo error in abundance for a cja,ge in logg of +0.2dex (stat.error)
  (2)DC-best  ZZ Boo depth in best combined synthetic spectrum of the binary (phot.flux.density;arith.ratio)
  (2)DC-0.5  ZZ Boo depth with under-abundance by 0.5dex (phot.flux.density;arith.ratio)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)DC+0.5  ZZ Boo depth with over-abundance by 0.5dex (phot.flux.density;arith.ratio)
  (3)Z   [6/64] Atomic number (meta.id;meta.main)
  (3)NL   [1/76] Number of lines used (meta.id)
  (3)Ab-best [Sun] Best value abundance (ZZ Boo minus Solar) (phys.abund)
  (3)e_Ab-best [Sun] (n) error in Ab-best (stat.error)
  (3)Ab+100K [Sun] Abundance (ZZ Boo minus Solar) with effective temperature shifted by +100K) (phys.abund)
  (3)e_Ab+100K [Sun] (n) error in Ab+100K (stat.error)
  (3)Ab+0.2 [Sun] Abundance (ZZ Boo minus Solar) with surface gravity shifted by +0.2dex) (phys.abund)
  (3)e_Ab+0.2 [Sun] (n) error in Ab+0.2 (stat.error)
  (3)logN-best [-] Best value of ZZ Boo absolute mean abundance (phys.abund)
  (3)e_logN-best [-] (n) error in logN- (stat.error)
  (3)logN+100K [-] Absolute mean abundance of ZZ Boo with effective temperature shifted by +100K (phys.abund)
  (3)e_logN+100K [-] (n) error in logN+100K (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)logN+0.2 [-] Absolute mean abundance of ZZ Boo with surface gravity shifted by +0.2cm/s2) (phys.abund)
  (3)e_logN+0.2 [-] (n) error in logN-logg (stat.error)
  (4)BibCode (char) Bibliographic code (meta.bib.bibcode)
  (4)Aut (char) Authors's name (meta.bib.author)
  (4)Com (char) Comments (meta.note)

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