Inferred M − R (left) and M − Λ (right) curves for the 68% CI corresponding to the EOS posterior along with the sources also at 68% (solid lines). The light blue and green patches correspond to the latest mass and radius measurements of the pulsar J0740+6620 (Fonseca et al. 2021; Riley et al. 2021a; Miller et al. 2021a). The black dashed lines represent the most probable EOS. The brown dashed curve on the left panel denotes the 90% of J0437–4715. Additionally, the blue dashed curve on the right panel denotes the 90% of the heavier component of GW170817.