1     2p6                               1  S    0.0          0.000          0.000
      2     2p5.3s                            3  P    2.0    5848620.000    5855680.500
      3     2p5.3s                            1  P    1.0    5864000.000    5871661.500
      4     2p5.3s                            3  P    0.0    5950710.000    5956518.000
      5     2p5.3s                            3  P    1.0    5960270.000    5967008.000
      6     2p5.3p                            3  S    1.0    6092810.000    6099089.000
      7     2p5.3p                            3  D    2.0    6121010.000    6128677.500
      8     2p5.3p                            3  D    3.0    6134030.000    6141047.500
      9     2p5.3p                            1  P    1.0    6143140.000    6150493.500
     10     2p5.3p                            3  P    2.0    6157770.000    6164853.500
     11     2p5.3p                            3  P    0.0    6201860.000    6211008.000
     12     2p5.3p                            3  D    1.0    6218510.000    6225625.000
     13     2p5.3p                            3  P    1.0    6244720.000    6250816.500
     14     2p5.3p                            1  D    2.0    6247750.000    6254324.500
     15     2p5.3p                            1  S    0.0    6352630.000    6382883.000
     16     1s.2s2.2p6.3s                     3  S    1.0   57735005.000   57735005.000
     17     1s.2s2.2p6.3s                     1  S    0.0   57775332.000   57775332.000
     18     1s.2s2.2p6.3p                     3  P    0.0   57995519.000   57995519.000
     19     1s.2s2.2p6.3p                     3  P    1.0   58000359.000   58000359.000
     20     1s.2s2.2p6.3p                     3  P    2.0   58019716.000   58019716.000
     21     1s.2s2.2p6.3p                     1  P    1.0   58043106.000   58043106.000
 -1
%filename: fe_17d.elvlc
%Energy levels (below ionization): Shirai,T., Sugar,J., Musgrove,A., Wiese,W.L., 2000, J.Phys.Chem.Ref.Data, Monograph 8
%Energy levels (above ionization): Mendoza, C., Kallman, T.R., Bautista, M.A., Palmeri, P., 2004, A&A, 414, 377
%Comment: some energy levels from the NIST database, version 2.0, have been renumbered
        in order to match the identification given by Bhatia and Doschek
        and their theoretical energy levels. In particular, the following changes
        have been made:
                        NIST  -->  CHIANTI
                         12   -->     9
                         13   -->    12
                          9   -->    13
%Comment: the theoretical energies from Mendoza et al have been used as experimental ones.
%Comment: the LS notation for energy levels has been taken from Mendoza et al.
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Enrico Landi - Jan 2005