10   5
  4.000  4.250  4.500  4.750  5.000
 17  2   1   2 6.342e-03 4.83741e+00 4.56453e+00 4.19501e+00 3.89837e+00 3.52793e+00
 17  2   1   3 9.081e-03 1.26080e+00 1.16690e+00 1.05086e+00 9.69128e-01 8.79839e-01
 17  2   1   4 1.103e-01 4.69126e+00 4.59167e+00 4.41705e+00 4.11916e+00 3.66647e+00
 17  2   1   5 2.509e-01 5.64148e-01 5.60827e-01 5.49927e-01 5.27182e-01 4.89125e-01
 17  2   2   3 2.739e-03 1.59863e+00 1.54789e+00 1.46460e+00 1.37306e+00 1.23172e+00
 17  2   2   4 1.103e-01 2.81475e+00 2.75486e+00 2.65057e+00 2.47602e+00 2.21757e+00
 17  2   2   5 2.509e-01 3.38262e-01 3.36314e-01 3.29955e-01 3.15822e-01 2.91866e-01
 17  2   3   4 1.103e-01 9.38158e-01 9.18264e-01 8.83530e-01 8.25201e-01 7.37946e-01
 17  2   3   5 2.509e-01 1.12759e-01 1.12058e-01 1.09844e-01 1.05283e-01 9.68631e-02
 17  2   4   5 1.406e-01 1.49256e+00 1.47059e+00 1.43607e+00 1.40289e+00 1.38453e+00
-1
%filename: cl_2_k33.dwns
%Downsilons for the kappa-distribution with kappa = 33
%produced for the "KAPPA" database for astrophysical spectroscopy
%E. Dzifcakova - 2024 Feb.
-1