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\paragraph{Parameters - orbit-sizes, mass-ratios, eccentricities}  \label{par:_f_a_q_e_}  For the binary runs the authors make simplifying first assumption that the function $f(a,q,e)$ is separable and assign 3 ad-hoc analyitic formulae for the functions to $f(a)$ - initial orbit-sizes, $f(q)$ - initial mass ratios and $f(e)$ -initial - initial  eccentricities respectively. All parameters for the BSE code are kept at the defaults and in order to handle brown dwarfs below $0.08 M_{\odot}$ the authors use an extra data grid due to Baraffe et al. (1998).