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Characterization of Pulsar Sources for X-ray Navigation

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arxiv 1711.08507 v1 pith:OGXJMUAW submitted 2017-11-22 astro-ph.IM astro-ph.HE

classification astro-ph.IMastro-ph.HE
keywords navigationx-raynicersextantdescribefactorspulsarpulse
verification ladder T0 review T1 audit T2 compute T3 formal
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The Station Explorer for X-ray Timing and Navigation Technology (SEXTANT) is a technology demonstration enhancement to the Neutron Star Interior Composition Explorer (NICER) mission, which is scheduled to launch in 2017 and will be hosted as an externally attached payload on the International Space Station (ISS). During NICER's 18-month baseline science mission to understand ultra-dense matter through observations of neutron stars in the soft X-ray band, SEXTANT will, for the first-time, demonstrate real-time, on-board X-ray pulsar navigation. Using NICER/SEXTANT as an example, we describe the factors that determine the measurement errors on pulse times of arrival, including source and background count rates, and pulse profile shapes. We then describe properties of the SEXTANT navigation pulsar catalog and prospects for growing it once NICER launches. Finally, we describe the factors affecting the prediction of pulse arrival times in advance, including variable interstellar propagation effect and red timing noise. Together, all of these factors determine how well a particular realization of an X-ray pulsar-based navigation system will perform.

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  1. Unlocking the hidden potential of pulsar astronomy

    astro-ph.IM 2025-06 conditional novelty 3.0 of 10

    This review and feasibility study shows that compact radio receivers can detect bright pulsars for navigation, timing, randomness, and space weather applications, with a 4-meter dish potentially achieving 10 km self-l...

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