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J/A+A/547/A108
  Comparative modelling of cool giants spectra (Lebzelter+, 2012)
spectrum
  
    J/A+A/547/A108/table6Iron line selection for the M6 stellar parameter determination (26 rows)
    J/A+A/547/A108/table7Lines used in the A1 analysis to determine abundances for Star 1 (HR 1457) (32 rows)
    J/A+A/547/A108/table8Fe lines used in the A1 analysis to determine abundances for Star 3 (artificial star) (5 rows)
    J/A+A/547/A108/table9Lines used by the A2 participants (65 rows)
    J/A+A/547/A108/table10Lines analysed by the A5 team (60 rows)
    J/A+A/547/A108/table11Measured CO 3-0 lines in Star 4 (artificial star) from the T analysis (14 rows)
    J/A+A/547/A108/star1Observed optical spectrum for Albedaran (HR 1457) [spectrum](plot) (114979 rows)
    J/A+A/547/A108/star2Observed optical spectrum for Menkar (HR 911) [spectrum](plot) (114973 rows)
    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)
    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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