The CRIRES spectrum of HD 101412

Identification labels:
Interval: 520.2-520.3 nm---->label: 256  26.00 34328  397

256: last 3 digits of wavelengths in nm  lambda=520.2256 nm
26.00 = Fe I  26=atomic number of the element (Fe), 00=charge (I)
34328=lower enrgy level in cm-1
397=per mil residual intensity of isolated line before broadening (rotational + instrumental)






Parameters: Teff=8300 K, log g=3.8 from Cowley et al., A&A 523, 65 (2010)
            vsini=9 km/sec from several lines in the  CRIRES spectra. 
            

                       abundances
                  star          sun
              C  -3.80        -3.52
              N  -3.50        -4.12 
              Mg -5.30        -4.46
              Si -5.55        -4.49
              Fe -5.10        -4.54



                         
 identified lines


Comments on identified lines: 

Fe I predicted at 15621.654 and 15631.948 A, are not observed.
The strong absorption at 10730 A should be C I blended with some artifact.
The strong absorption at 10754 A should be an artifact.
The strong absorption at 10832 A is He I 10830.250, 10830.341 A from the shell.
The strong absorption at 10919 A should be an artifact.

 Si I  10982.058 is observed only in phases 0.58 and 0.53
 Fe I  15769.423 is not observed in phase=0.53
 Fe I  15819.142 is not observed in phases 0.94, 0.53
 Fe I  15822.817 weak, is not observed in phase=0.53

IN DETAIL: