Neutron star mass-radius curves for all 21 models with unified crust. The gray regions indicate the 90% (light) and 50% (dark) CI constraints from the binary components of GW170817. The 1σ (68%) CI for the 2D posterior distribution in the mass-radii domain for the millisecond pulsar PSR J0030 + 0451 (cyan and green) Riley et al. (2019), Miller et al. (2019) as well as the PSR J0740 + 6620 (pink) Riley et al. (2021), Miller et al. (2021) from the NICER X-ray data are also shown. Additionally, we show the constraint obtained from HESS J1731-347 for 68.3% (95.4%) CIs in dashed dark red (solid dark red) Doroshenko et al. (2022).