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¹Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098XH Amsterdam, The Netherlands
²Department of Physics and Astronomy, University of New Hampshire, Durham, New Hampshire 03824, USA
³SRON, Niel Bohrweg 4, 2033 CA Leiden, The Netherlands
⁴Technische Universität Darmstadt, Department of Physics, 64289 Darmstadt, Germany
⁵ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany
⁶Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany
⁷Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
⁸Department of Physics, University of Helsinki, P.O. Box 64, FI-00014 University of Helsinki, Finland

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Articles Citing

Equation-of-state-informed pulse profile modeling

Magnetic Field Effects on the Structure of Neutron Stars

Equation-of-state-informed pulse profile modeling

Characterizing the quark-hadron mixed phase in compact star cores: Sensitivity to nuclear saturation and quark-model parameters at finite temperature

Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2−604207

Astrophysics Equation of State Inference with Bayesian Chiral Effective Field Theory Uncertainties

A NICER View of PSR J0030+0451: Updated Constraints from 6 yr of NICER Observations

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