Measuring pulsar profile variations with 2-D Gaussian process regression
Michael J. Keith, Ren\'ee Spiewak, Andrew G. Lyne, Patrick Weltevrede, Danai Antonopoulou, Ben Stappers

TL;DR
This study introduces an efficient 2-D Gaussian process model to analyze pulsar profile variations, revealing new correlations with spin-down rates and complex profile shape dynamics in multiple pulsars.
Contribution
We develop a computationally efficient 2-D Gaussian process approach that improves detection of correlated pulsar profile variations and uncover new spin-down related shape changes.
Findings
Detected significant profile variations in 21 of 26 pulsars
Confirmed known spin-down correlations in 11 pulsars
Discovered new spin-down correlated shape changes in 7 pulsars
Abstract
Time-correlated variations in the pulse profiles of radio pulsars provide insights into changes in their magnetospheres. For a small number of pulsars (~20), these variations have been shown to correlate with spin-down rate. Many of these profile changes involve small (few percent) variations in the relative intensity of different profile components, and hence tools such as Gaussian process regression have been employed to separate the time-correlated profile variation from intrinsic noise. In this paper, we present a computationally efficient approximation of a 2-D Gaussian process model that enhances sensitivity by simultaneously tracking time- and phase-correlated signals. Applying this model to 26 pulsars observed at the Jodrell Bank Observatory, we detect significant profile shape variations in 21 pulsars. Using principal component analysis, we confirm spin-down correlated shape…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Scientific Research and Discoveries
