LISA results obtained with the subtraction algorithm in different scenarios, indicated by colours. Left: characteristic strain of the total noise power spectral density $(\sqrt{f{S}_n(f)})$, including the instrumental and the DWD confusion noise, compared to the instrumental noise alone, in grey dashed lines. Right: number of resolvable sources in each of the considered scenarios. Hatches indicate how many of those are accreting. We find 56.4%, 20.1%, and 50.7%; of the resolvable systems to be accreting in the ‘low spins, strong tides’, ‘low spins, weak tides’, and ‘high spins, strong tides’ scenarios, respectively, as indicated by the boxed numbers.