2.47 & 3.16 & & 3.69 & 3.28 & 3.71 & 3.30 & 3.78 & 3.31\
& & Cln{$180^\circ,90^\circ$} & & 3.21 & 4.26 & 3.05 & 3.31 & 2.64 & 3.23 & & 3.27 & 2.94 & 3.36 & 3.49 & 4.15 & 3.38\
& & Frank & & 5.15 & 6.66 & 4.91 & 4.37 & 3.62 & 3.89 & & 2.81 & 3.36 & 2.83 & 4.72 & 5.24 & 4.30\
& beta & BVN & & 4.69 & 4.33 & 4.70 & 4.37 & 4.83 & 4.34 & & 2.00 & 2.27 & 1.98 & 2.20 & 1.92 & 2.21\
& & Cln{$0^\circ,270^\circ$} & & 4.97 & 4.63 & 5.01 & 4.27 & 4.64 & 4.29 & & 2.00 & 2.28 & 1.99 & 2.20 & 1.94 & 2.22\
& & Cln{$180^\circ,90^\circ$} & & 6.15 & 6.01 & 5.95 & 4.32 & 4.83 & 4.34 & & 2.51 & 2.83 & 2.40 & 2.23 & 1.96 & 2.24\
& & Frank & & 7.84 & 8.03 & 7.64 & 3.33 & 3.23 & 3.59 & & 3.60 & 4.07 & 3.47 & 2.88 & 2.61 & 2.64\

Cln{$\omega_1^\circ,\omega_2^\circ$}: The bivariate copulas are the Clayton rotated by 