Including the new NICER PSR J0437 radius pushes inferred neutron star radii down by about 0.2-0.3 km and strengthens Bayesian evidence for a negative trace anomaly in heavy stars.
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Implications of latest NICER data for the neutron star equation of state
Including the new NICER PSR J0437 radius pushes inferred neutron star radii down by about 0.2-0.3 km and strengthens Bayesian evidence for a negative trace anomaly in heavy stars.