Impact of the PSR J0740+6620 radius constraint on the properties of high-density matter : Weighted Monte Carlo samples for neutron star observables

We provide weighted Monte Carlo samples for the, the natural logarithm of the sample weight when using two different measurements of J0740+6620 Radius, and when using no measurement of the radius, but just using the established mass measurement, the maximum Tolman-Oppenheimer-Volkoff (TOV) mass, the pressure divided by the speed of light squared at nuclear saturation, twice nuclear saturation, and six times nuclear saturation density, the dimensionless tidal deformability of a 1.4  and 2.0 solar mass NS, and the radius of a 1.4 and 2.0 solar mass NS, as well as the number of stable branches in the M-R curve, the central density of a maximum TOV mass star, the maximum speed of sound, the baryon density at the maximum speed of sound, and the speed of sound at the central density of a maximum TOV mass star.  See the README.md for more details.