Mass–radius relations for non-rotating stars for the CL EOS with ρ_u = ρ₀, the CL EOS with two crust models connected at ρ_u = ρ₀: the catalysed crust from Douchin & Haensel (2001) (CLC EOS) and the accreted crust from Haensel & Zdunik (2008) (CLCacc EOS). For reference we plot the M–R relation obtained for the DH EOS. The horizontal lines correspond to the highest observed maximum mass for PSR J1614–2230 and PSR J0348+0432.