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J/A+A/547/A108
  Comparative modelling of cool giants spectra (Lebzelter+, 2012)
spectrum
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1.J/A+A/547/A108/table6Iron line selection for the M6 stellar parameter determination (26 rows)
2.J/A+A/547/A108/table7Lines used in the A1 analysis to determine abundances for Star 1 (HR 1457) (32 rows)
3.J/A+A/547/A108/table8Fe lines used in the A1 analysis to determine abundances for Star 3 (artificial star) (5 rows)
4.J/A+A/547/A108/table9Lines used by the A2 participants (65 rows)
5.J/A+A/547/A108/table10Lines analysed by the A5 team (60 rows)
6.J/A+A/547/A108/table11Measured CO 3-0 lines in Star 4 (artificial star) from the T analysis (14 rows)
7.J/A+A/547/A108/star1Observed optical spectrum for Albedaran (HR 1457) [spectrum](plot) (114979 rows)
8.J/A+A/547/A108/star2Observed optical spectrum for Menkar (HR 911) [spectrum](plot) (114973 rows)
9.J/A+A/547/A108/star3Simulated observed H-band spectrum for Star 3 (T=4257K, logg=1.47, M=1.165M, [Fe/H]=-0.4) [spectrum](plot) (2101 rows)
10.J/A+A/547/A108/star4Simulated observed H-band spectrum for Star 4 (T=3280K, logg=0.06, M=1.509M, [Fe/H]=+0.1) [spectrum](plot) (2101 rows)

 
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Column  Constraint Explain   (UCD)
  (1+5)El (char) Element (Fe I or Fe II) (phys.atmol.element)
  (1+5)Elow eV Lower level excitation potential (phys.atmol.excitation;phys.atmol.level)
  (1+2+3+4+5+6)lambda nm Wavelength (em.wl)
  (1+2+3+4+5+6)log(gf)  gf value (stat.value;phys.absorption.coeff)
  (1+2+3+4+5)Source (char) Line data source (Note 1)   (meta.bib)
  (2+3)abund  Abundance (log(NH)=12.00) (phys.abund)
  (2+3+6)Elow cm-1 Lower level excitation potential (phys.atmol.excitation;phys.atmol.level)
  (2)Z  Atomic number (meta.id;meta.main)
  (4)EW1 0.1pm (n) Equivalent width Star 1 (HR 1457); in mÅ (spect.line.eqWidth)
  (4)EW2 0.1pm (n) Equivalent width Star 2 (HR 911); in mÅ (spect.line.eqWidth)
  (4)Ion  Species code following Kurucz's notation (phys.atmol.ionStage)

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(n) indicates a possible blank or NULL column(i)indexed column
  (4)n_Ion (char) [*] Line included in the final fit (meta.note)
  (5)EW 0.1pm Equivalent width in mÅ (spect.line.eqWidth)
  (6)Ident (char) Line identification (meta.id;spect.line)
  (6)logW/nu  Equivalent width over wavenumber (spect.line.eqWidth)
  (7+8+9+10)Flux  Flux normalized to continuum (see description) (phot.flux)
  (7+8+9+10)lambda 0.1nm [4900/9800] Air wavelength (see description) (em.wl)

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