Show simple item record

Files in this item

Thumbnail

Item metadata

dc.contributor.advisorThomas, Len
dc.contributor.advisorNewman, Ken B.
dc.contributor.authorEmpacher, Fanny
dc.coverage.spatial246en_US
dc.date.accessioned2024-04-19T12:39:50Z
dc.date.available2024-04-19T12:39:50Z
dc.date.issued2024-06-11
dc.identifier.urihttps://hdl.handle.net/10023/29716
dc.description.abstractState-space models (SSMs) are a popular and flexible framework for modelling time series due to their ability to separate changes in the underlying state of a system from the noisy observations made on these states. This thesis explores methods for estimating states and model parameters in non-linear and non-Gaussian Bayesian SSMs. We focus on models of wildlife population dynamics, in particular a case study of the UK grey seal population. Calculation of the likelihood is fundamental to Bayesian analysis, but direct calculation is typically intractable for non-linear non-Gaussian SSMs. We use a class of simulation-based methods, Sequential Monte Carlo (SMC), which build on repeated importance sampling of simulated states to deliver an unbiased estimate of the likelihood. We find that variance of the estimated likelihood can be high and explore techniques for variance reduction. For parameter inference, we use particle marginal Metropolis-Hastings (PMMH), which embeds the SMC likelihood within a Markov chain Monte Carlo (MCMC) algorithm. Careful balance is needed between computational effort expended on the SMC step and the number of MCMC samples. A much faster alternative is the Kalman filter, designed for linear and Gaussian SSMs. We applied the Kalman filter to an approximation of the seal model. The posterior distribution obtained was often close to the true posterior, while reducing computation time by a factor of 1790. We show the seal model suffers from identifiability issues which cannot be resolved by increasing the accuracy of the observations or allowing more flexibility in the underlying biological process with random effects. However, estimation of underlying states (i.e., population sizes) is unaffected by these issues. A reduction in PMMH computation time can be achieved by exploiting the structure of the state model: separately estimating likelihood components in each of the 4 seal regions led to a 5-fold increase in speed.en_US
dc.description.sponsorship"This work was supported by the Engineering and Physical Sciences Research Council, via a Doctoral Training Partnership grant to the University of St Andrews; and by the University of St Andrews (School of Mathematics and Statistics)."--Funding Acknowledgementsen
dc.language.isoenen_US
dc.rightsCreative Commons Attribution-NonCommercial 4.0 International*
dc.rights.urihttp://creativecommons.org/licenses/by-nc/4.0/*
dc.subjectBayesian inferenceen_US
dc.subjectSequential Monte Carlo methodsen_US
dc.subjectPopulation dynamicsen_US
dc.subjectHalichoerus grypusen_US
dc.subjectState-space modelsen_US
dc.subjectParticle filtersen_US
dc.subjectKalman filteren_US
dc.titleEfficient methods for fitting nonlinear non-Gaussian state space models of wildlife population dynamicsen_US
dc.typeThesisen_US
dc.contributor.sponsorEngineering and Physical Sciences Research Council (EPSRC)en_US
dc.contributor.sponsorUniversity of St Andrews. School of Mathematics and Statisticsen_US
dc.type.qualificationlevelDoctoralen_US
dc.type.qualificationnamePhD Doctor of Philosophyen_US
dc.publisher.institutionThe University of St Andrewsen_US
dc.identifier.doihttps://doi.org/10.17630/sta/860


The following licence files are associated with this item:

    This item appears in the following Collection(s)

    Show simple item record

    Creative Commons Attribution-NonCommercial 4.0 International
    Except where otherwise noted within the work, this item's licence for re-use is described as Creative Commons Attribution-NonCommercial 4.0 International