A transdimensional sampling framework for pulsar timing noise modelling
Valentina Di Marco, Nir Guttman, Matthew T. Miles, Andrew Zic, Ryan M. Shannon, Eric Thrane

TL;DR
This paper introduces tPTABilby, a transdimensional Bayesian framework for pulsar noise analysis that improves model selection and parameter estimation, validated through simulations and real data application.
Contribution
It presents a novel transdimensional sampling method integrated into a pulsar noise analysis framework, enabling flexible, unified noise modeling and model selection.
Findings
Accurately recovers known noise models in simulations.
Demonstrates consistent results with existing PTA analyses.
Provides a robust, flexible approach for pulsar noise characterization.
Abstract
A careful characterisation of the noise processes in pulsar timing data is a prerequisite for pulsar timing array experiments. While single-pulsar noise analyses are crucial for both gravitational-wave searches and astrophysical studies, they are often computationally intensive and rely on running and comparing multiple fixed noise models. We present tPTABilby, a transdimensional Bayesian inference framework for single-pulsar noise analysis built on the Bilby library. The method flexibly models a wide range of noise processes like radiometer noise, pulse-phase jitter, intrinsic red noise, dispersion measure variations, and chromatic interstellar medium effects. By employing transdimensional sampling, tPTABilby simultaneously infers the number and type of active noise sources, providing a unified treatment of model selection and parameter estimation. We validate the methodology through…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Radio Astronomy Observations and Technology · Scientific Research and Discoveries
