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J/A+A/281/465
  Chemical Composition of alf UMi and V473 Lyr (Andrievsky+ 1994)
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1994A&A...281..465A
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1.J/A+A/281/465/table1Observational data (9 rows)
2.J/A+A/281/465/table2Residual intensities for hydrogen line profiles (30 rows)
3.J/A+A/281/465/table3Chemical composition of Alpha UMi (33 rows)
4.J/A+A/281/465/table4Chemical composition of HR7308 (35 rows)
5.J/A+A/281/465/annexEquivalent widths of lines in the spectra (441 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)Name (char) Star name (meta.id;meta.main)
  (1)Date (char) Observation date (time.epoch)
  (1)HDJ d Julian day (time.epoch)
  (1)Phase   [0,1[ Phase (see n_Phase) (time.phase)
  (1)n_Phase   [1,2] Phase calculated according to: 1: Arellano Ferro (1984MNRAS.209..481A) 2: Eggen (1985AJ.....90.1297E) (meta.note)
  (1)Emulsion (char) Photographic emulsion used (instr.plate.emulsion)
  (1)Region (char) 0.1nm Spectral region (min/max wavelength) (instr.bandwidth)
  (1)Exp min Exposure time (time.duration;obs.exposure)
  (1)S/N  Signal-to-noise ratio (stat.snr)
  (2)Dlambda 0.1nm Distance from center of line (em.wl;arith.diff)

ALL cols		    
 (i)indexed column
  (2)Hbeta1  Residual intensity for hydrogen line profile of Alpha UMi (spect.line.intensity)
  (2)Hgamma1  Residual intensity for hydrogen line profile of Alpha UMi (spect.line.intensity)
  (2)Hbeta2a  Residual intensity for hydrogen line profile of HR7308(1990) (spect.line.intensity)
  (2)Hgamma2a  Residual intensity for hydrogen line profile of HR7308(1990) (spect.line.intensity)
  (2)Hbeta2b  Residual intensity for hydrogen line profile of HR7308(1990) (spect.line.intensity)
  (2)Hgamma2b  Residual intensity for hydrogen line profile of HR7308(1992) (spect.line.intensity)
  (2)Hdelta2b  Residual intensity for hydrogen line profile of HR7308(1992) (spect.line.intensity)
  (3+4+5)Ion (char) Element and ionisation level (phys.atmol.element)
  (3+4+5)Elem (char) Show all values for this element (meta.ref)
  (3)NL  Number of lines used for this study (meta.number)
  (3)(E/H)  Mean abundance relative to logN(H) = 12 (Note G1)   (phys.abund)
  (3)[E/H] [Sun] Mean abundance relative to solar value (phys.abund)
  (3)e_[E/H] [Sun] (n) rms uncertainty on [E/H] (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)B+L [Sun] (n) [E/H] Result of Boyarchuck & Luybimkov (1981IzKry..64....3B) (phys.abund)
  (3)L+B [Sun] (n) [E/H] Luck & Bond (1986PASP...98..442L) (phys.abund)
  (3)GIR [Sun] (n) [E/H] Giridhar (1985, Proc. Coll. IAU 82, 100) (phys.abund)
  (3)SR+J [Sun] (n) [E/H] Sanwal, Rautela & Joshi (1988Ap&SS.140..131S) (phys.abund)
  (4)NLa  (n) Number of lines used for the 1990 value (meta.number)
  (4)(E/H)a  (n) Mean abundance, 1990 value (Note G1)   (phys.abund)
  (4)[E/H]a [Sun] (n) (E/H) with respect to solar 1990 value, 1990 value (phys.abund)
  (4)e_[E/H]a [Sun] (n) rms uncertainty on [E/H], 1990 value (stat.error)
  (4)NLb  (n) Line number used for average 1992 value (meta.number)
  (4)(E/H)b  (n) Mean abundance, average 1992 value (Note G1)   (phys.abund)
  (4)[E/H]b [Sun] (n) (E/H) with respect to solar, average 1992 value (phys.abund)
  (4)e_[E/H]b [Sun] (n) rms uncertainty on [E/H], average 1992 value (stat.error)
  (5)Lambda 0.1nm Wavelength (em.wl)
  (5)EW1 pm (n) Alpha UMi equivalent width (spect.line.eqWidth)
  (5)EW2a pm (n) HR7308(1990) equivalent width (spect.line.eqWidth)
  (5)EW2b pm (n) HR7308(1992) equivalent width (spect.line.eqWidth)

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