10 5 4.000 4.250 4.500 4.750 5.000 17 2 1 2 6.342e-03 9.42923e+00 9.31084e+00 9.07889e+00 8.92055e+00 8.37796e+00 17 2 1 3 9.081e-03 2.51795e+00 2.45309e+00 2.33849e+00 2.26163e+00 2.10889e+00 17 2 1 4 1.103e-01 8.95613e+00 8.82390e+00 8.68773e+00 8.60008e+00 8.42637e+00 17 2 1 5 2.509e-01 1.07267e+00 1.05861e+00 1.04157e+00 1.03812e+00 1.04183e+00 17 2 2 3 2.739e-03 2.93490e+00 2.90772e+00 2.96934e+00 3.04614e+00 2.93102e+00 17 2 2 4 1.103e-01 5.37919e+00 5.30217e+00 5.21127e+00 5.14678e+00 5.04976e+00 17 2 2 5 2.509e-01 6.44672e-01 6.35802e-01 6.24738e-01 6.21329e-01 6.22871e-01 17 2 3 4 1.103e-01 1.79311e+00 1.76267e+00 1.73430e+00 1.71909e+00 1.69002e+00 17 2 3 5 2.509e-01 2.14016e-01 2.11051e-01 2.08188e-01 2.08451e-01 2.07826e-01 17 2 4 5 1.406e-01 2.83835e+00 2.82361e+00 2.78853e+00 2.75038e+00 2.72817e+00 -1 %filename: cl_2_k1p8.dwns %Downsilons for the kappa-distribution with kappa = 1.8 %produced for the "KAPPA" database for astrophysical spectroscopy %E. Dzifcakova - 2024 Feb. -1