T. Kato, U.I. Safronova, A.S. Shlyaptseva, M. Cornille, J. Dubau and J. Nilsen 1997, ADNDT 67, 225
COMPARISON OF SATELLITE SPECTRA FOR H-LIKE Fe AND He-LIKE Fe, Ca, AND S CALCULATED BY THREE DIFFERENT METHODS

  Aa2 is the autoionizing rate to 1s2 2s2 2p 2P3/2

 C-like ion: Z=26
   Table VB        calculated by Cornille and Dubau (AUTOLSJ code)

lower level    upper level               lambda(A) Qd(1/s)   Ar(1/s)    Aa2(1/s)   SumAa(1/s) Br

1s2s2 2p3 3D 1  1s2 2s2 2p2 3P 0	  1.8905  3.828E+13  2.644E+14  3.404E+13  3.843E+14  0.375
1s2s2 2p3 3D 1  1s2 2s2 2p2 3P 2	  1.8948  6.410E+12  4.430E+13  3.404E+13  3.843E+14  0.063
1s2s2 2p3 3D 2  1s2 2s2 2p2 3P 1	  1.8925  8.484E+13  2.010E+14  5.290E+13  4.098E+14  0.321
1s2s2 2p3 3D 2  1s2 2s2 2p2 1D 2	  1.8988  4.360E+12  1.032E+13  5.290E+13  4.098E+14  0.016
1s2s2 2p3 3D 3  1s2 2s2 2p2 3P 2	  1.8926  2.652E+14  1.633E+14  1.485E+14  4.260E+14  0.255
1s2s2 2p3 3D 3  1s2 2s2 2p2 1D 2	  1.8973  7.848E+13  4.834E+13  1.485E+14  4.260E+14  0.075
1s2s2 2p3 3S 1  1s2 2s2 2p2 3P 0	  1.8866  5.200E+12  2.506E+13  6.055E+13  2.558E+14  0.029
1s2s2 2p3 3S 1  1s2 2s2 2p2 3P 1	  1.8893  8.992E+13  4.336E+14  6.055E+13  2.558E+14  0.495
1s2s2 2p3 3S 1  1s2 2s2 2p2 3P 2	  1.8909  2.758E+13  1.330E+14  6.055E+13  2.558E+14  0.152
1s2s2 2p3 3S 1  1s2 2s2 2p2 1D 2	  1.8956  4.570E+12  2.204E+13  6.055E+13  2.558E+14  0.025
1s2s2 2p3 3P 0  1s2 2s2 2p2 3P 1	  1.8884  3.947E+13  2.232E+14  1.092E+14  3.917E+14  0.361
1s2s2 2p3 3P 2  1s2 2s2 2p2 3P 2	  1.8892  2.620E+14  3.045E+14  1.308E+14  3.906E+14  0.401
1s2s2 2p3 3P 2  1s2 2s2 2p2 1D 2	  1.8939  5.008E+13  5.823E+13  1.308E+14  3.906E+14  0.077
1s2s2 2p3 3P 1  1s2 2s2 2p2 3P 2	  1.8886  1.336E+14  3.637E+14  9.179E+13  3.385E+14  0.485
1s2s2 2p3 3P 1  1s2 2s2 2p2 1S 0	  1.8976  1.279E+13  3.480E+13  9.179E+13  3.385E+14  0.046
1s2s2 2p3 1D 2  1s2 2s2 2p2 3P 2	  1.8854  4.020E+12  4.270E+12  1.655E+14  3.807E+14  0.005
1s2s2 2p3 1D 2  1s2 2s2 2p2 1D 2	  1.8900  4.568E+14  4.847E+14  1.655E+14  3.807E+14  0.552
1s2s2 2p3 1D 2  1s2 2p4     1D 2	  1.9490  4.760E+12  5.050E+12  1.655E+14  3.807E+14  0.006
1s2s2 2p3 1P 1  1s2 2s2 2p2 1D 2	  1.8872  1.552E+14  3.931E+14  1.291E+14  3.268E+14  0.401
1s2s2 2p3 1P 1  1s2 2s2 2p2 1S 0	  1.8915  9.840E+13  2.493E+14  1.291E+14  3.268E+14  0.254