Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/44585
Title: Dynamical modelling of dwarf spheroidal galaxies using Gaussian-process emulation
Authors: Gration, Amery
Wilkinson, Mark I.
First Published: 29-Mar-2019
Publisher: Oxford University Press (OUP), Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2019, 485 (4), pp. 4878-4892
Abstract: We present a novel and efficient method for fitting dynamical models of stellar kinematic data for dwarf spheroidal galaxies (dSph). Our approach is based on Gaussian-process emulation (GPE), which is a sophisticated form of curve fitting that requires fewer training data than alternative methods. We use a set of validation tests and diagnostic criteria to assess the performance of the emulation procedure. We have implemented an algorithm in which both the GPE procedure and its validation are fully automated. Applying this method to synthetic data, with fewer than 100 model evaluations we are able to recover a robust confidence region for the three-dimensional parameter vector of a toy model of the phase-space distribution function of a dSph. Although the dynamical model presented in this paper is low-dimensional and static, we emphasize that the algorithm is applicable to any scheme that involves the evaluation of computationally expensive models. It therefore has the potential to render tractable previously intractable problems, for example, the modelling of individual dSphs using high-dimensional, time-dependent N-body simulations.
DOI Link: 10.1093/mnras/stz605
ISSN: 0035-8711
eISSN: 1365-2966
Links: https://academic.oup.com/mnras/article/485/4/4878/5420835
http://hdl.handle.net/2381/44585
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2019, Oxford University Press (OUP), Royal Astronomical Society. Deposited with reference to the publisher’s open access archiving policy. (http://www.rioxx.net/licenses/all-rights-reserved)
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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