The Efficiency of Geometric Samplers for Exoplanet Transit Timing Variation Models
Noah W. Tuchow, Eric B. Ford, Theodore Papamarkou, and Alexey Lindo

TL;DR
This paper evaluates the efficiency of various geometric MCMC samplers in modeling exoplanet transit timing variations, demonstrating that covariance-informed transformations significantly enhance sampling performance across different models.
Contribution
It systematically compares multiple geometric MCMC samplers for TTV models, highlighting the importance of covariance-based transformations for improved efficiency.
Findings
Transforming parameter space using covariance estimates improves sampler efficiency.
Differential Evolution Monte Carlo and Geometric adaptive Monte Carlo perform consistently well.
Hamiltonian Monte Carlo excels for near-Gaussian posteriors.
Abstract
Transit timing variations (TTVs) are a valuable tool to determine the masses and orbits of transiting planets in multi-planet systems. TTVs can be readily modeled given knowledge of the interacting planets' orbital configurations and planet-star mass ratios, but such models are highly nonlinear and difficult to invert. Markov chain Monte Carlo (MCMC) methods are often used to explore the posterior distribution for model parameters, but, due to the high correlations between parameters, nonlinearity, and potential multi-modality in the posterior, many samplers perform very inefficiently. Therefore, we assess the performance of several MCMC samplers that use varying degrees of geometric information about the target distribution. We generate synthetic datasets from multiple models, including the TTVFaster model and a simple sinusoidal model, and test the efficiencies of various MCMC…
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