Exploring Waveform Variations among Neutron Star Ray-tracing Codes for Complex Emission Geometries

Pulse profile modeling (PPM), the technique used to infer mass, radius, and geometric parameters for rotation-powered millisecond pulsars using data from the Neutron Star Interior Composition Explorer (NICER), relies on relativistic ray-tracing of thermal X-ray photons from hot spots on the neutron...

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Bibliografske podrobnosti
izdano v:The Astrophysical Journal
Main Authors: Devarshi Choudhury, Anna L. Watts, Alexander J. Dittmann, M. Coleman Miller, Sharon M. Morsink, Tuomo Salmi, Serena Vinciguerra, Slavko Bogdanov, Sebastien Guillot, Michael T. Wolff, Zaven Arzoumanian
Format: Artigo
Izdano: IOP Publishing 2024-01-01
Teme:
High energy astrophysics
Neutron stars
Gravitation
Pulsars
Millisecond pulsars
Rotation powered pulsars
Online dostop:https://doi.org/10.3847/1538-4357/ad7255
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https://doi.org/10.3847/1538-4357/ad7255

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