No abstract

The X-ray Pulse Simulation and Inference (X-PSI) package is a software package designed to simulate rotationally-modulated surface X-ray emission from neutron stars and to perform Bayesian statistical inference on real or simulated pulse profile data sets. Model parameters of interest include neutron star mass and radius and the system geometry and properties of the hot emitting surface regions.

We study the effects of the time-variable properties of thermonuclear X-ray bursts on modeling their millisecond-period burst oscillations. We apply the pulse profile modeling technique that is being used in the analysis of rotation-powered millisecond pulsars by the Neutron Star Interior Composition Explorer (NICER) to infer masses, radii, and geometric parameters of neutron stars. By simulating and analyzing a large set of models, we show that overlooking burst time-scale variability in temperatures and sizes of the hot emitting regions can result in substantial bias in the inferred mass and radius. To adequately infer neutron star properties, it is essential to develop a model for the time variable properties or invest a substantial amount of computational time in segmenting the data into non-varying pieces. We discuss prospects for constraints from proposed future X-ray telescopes.