Improving Pulsar Timing Precision with Single Pulses
Matthew Kerr

TL;DR
This paper introduces a novel pulsar timing method using basis pulses to reduce pulse-to-pulse variability, significantly improving timing precision and efficiency for large telescopes.
Contribution
It proposes a new technique to model and utilize single pulse variability, enhancing timing accuracy beyond traditional methods.
Findings
Achieved 25-40% improvement in TOA precision with high-time resolution data.
Demonstrated that the method produces Gaussian residuals, improving statistical reliability.
Halves the telescope time needed to reach a given timing precision.
Abstract
The measurement error of pulse times of arrival (TOAs) in the high S/N limit is dominated by the quasi-random variation of a pulsar's emission profile from rotation to rotation. Like measurement noise, this noise is only reduced as the square root of observing time, posing a major challenge to future pulsar timing campaigns with large aperture telescopes, e.g. the Five-hundred-metre Aperture Spherical Telescope and the Square Kilometre Array. We propose a new method of pulsar timing that attempts to approximate the pulse-to-pulse variability with a small family of 'basis' pulses. If pulsar data are integrated over many rotations, this basis can be used to measure sub-pulse structure. Or, if high-time resolution data are available, the basis can be used to 'tag' single pulses and produce an optimal timing template. With realistic simulations, we show that these applications can…
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