Fraction of systems that merge within a Hubble time, f_merge, that remain bound after SN, f_bound, and that are disrupted by the SN kick, f_disrupt, in six post-CE evolutionary scenarios of binaries with the 1.4 M_⊙ and 5.0 M_⊙ companions. The six scenarios are as follows: (i) no mass transfer after the CE and SN kicks; (ii) our default scenario of non-conservative (β = 1.0) mass transfer with final mass M₁ = 2.0 M_⊙ and SN kicks; (iii) same as the default scenario (ii) but with slower NS kicks from a Maxwellian with σ_kick = 50 km s⁻¹; (iv) same as the default scenario but assuming an orbital separation after the CE that is smaller by one-third; (v) same as (iv) but with an orbital separation that is smaller by two-thirds; (vi) same as the default scenario but assuming a final mass of M₁ = 1.6 M_⊙.