Parameter constraints for accreting millisecond pulsars with synthetic NICER data

TL;DR

This paper adapts pulse profile modeling for accreting millisecond pulsars using synthetic NICER data, enabling more accurate parameter estimation and highlighting potential degeneracies in certain scenarios.

Contribution

It introduces modifications to the X-PSI code for AMPs, including accretion disc and atmosphere models, and tests parameter recovery with synthetic NICER data.

Findings

Accurate parameter constraints for large hotspots.

Degeneracy and bias in small hotspot, high inclination scenarios.

Foundation for future NICER and IXPE data analysis.

Abstract

Pulse profile modelling (PPM) is a technique for inferring mass, radius and hotspot properties of millisecond pulsars. PPM is now regularly used for analysis of rotation-powered millisecond pulsars (RMPs) with data from the Neutron Star Interior Composition ExploreR (NICER). Extending PPM to accreting millisecond pulsars (AMPs) is attractive, because they are a different source class featuring bright X-ray radiation from hotspots powered by accretion. In this paper, we present a modification of one of the PPM codes, X-PSI, so that it can be used for AMPs. In particular, we implement a model of an accretion disc and atmosphere model appropriate for the hotspots of AMPs, and improve the overall computational efficiency. We then test parameter recovery with synthetic NICER data in two scenarios with reasonable parameters for AMPs. We find in the first scenario, where the hotspot is large, that we are able to tightly and accurately constrain all parameters including mass and radius. In the second scenario, which is a high inclination system with a smaller hotspot, we find degeneracy between a subset of model parameters and a slight bias in the inferred mass and radius. This analysis of synthetic data lays the ground work for future analysis of AMPs with NICER data. Such an analysis could be complemented by future (joint) analysis of polarization data from the Imaging X-ray Polarimetry Explorer (IXPE).