<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-09-21T02:02:37Z</responseDate><request verb="GetRecord" identifier="oai:www.repository.cam.ac.uk:1810/377285" metadataPrefix="uketd_dc">https://api.repository.cam.ac.uk/server/oai/request</request><GetRecord><record><header><identifier>oai:www.repository.cam.ac.uk:1810/377285</identifier><datestamp>2025-12-19T23:54:34Z</datestamp><setSpec>com_1810_214758</setSpec><setSpec>com_1810_256064</setSpec><setSpec>col_1810_219492</setSpec></header><metadata><uketd_dc:uketddc xmlns:uketd_dc="http://naca.central.cranfield.ac.uk/ethos-oai/2.0/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:uketdterms="http://naca.central.cranfield.ac.uk/ethos-oai/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://naca.central.cranfield.ac.uk/ethos-oai/2.0/ http://naca.central.cranfield.ac.uk/ethos-oai/2.0/uketd_dc.xsd">
   <dc:title>Hierarchical Bayesian Models for Investigating Astrophysical Systematics in Type Ia Supernova Cosmology</dc:title>
   <dc:identifier xsi:type="dcterms:DOI">https://doi.org/10.17863/CAM.114148</dc:identifier>
   <dc:creator>Ward, Sam</dc:creator>
   <uketdterms:advisor>Dhawan, Suhail</uketdterms:advisor>
   <uketdterms:advisor>Mandel, Kaisey</uketdterms:advisor>
   <dcterms:abstract>Type Ia supernovae (SNe Ia) are stellar explosions, and standardisable candles, used to
estimate luminosity distances and constrain cosmological parameters. With increasing
SN Ia sample sizes (≳ 1000 objects), systematic uncertainties in SN distance estimates now
dominate inferences in SN cosmology. The goal then is to improve SN Ia standardisation to
enhance their utility as cosmological probes. To do this, the astrophysics that drives observed
correlations between SN brightnesses, and their host galaxy properties, must be understood.
I review state-of-the-art studies of SN-host correlations in Chapter 1, which specifically
motivate the work in this thesis, and discuss statistical methods such as hierarchical Bayesian
modelling and Gaussian processes in Chapter 2, which are used extensively throughout.

In the subsequent Chapters, I explore two distinct avenues for better understanding
empirical SN-host correlations. The first involves the development of new hierarchical
Bayesian methods for rapidly inferring SN-host dust population distributions from SN
brightness measurements, without assuming any cosmology (Chapter 3). The second similarly
involves the development of various forward models for ‘SN siblings’: SNe that exploded
in the same host galaxy (Chapters 4, 5). This thesis thus contributes multiple fundamental
conceptual developments for SN Ia modelling, including: the intrinsic deviations formalism
for cosmology-independent hierarchical modelling of chromatic brightness measurements,
censored-data modelling for building a cosmological sample of SNe Ia that is consistent with
the forward model, and the relative intrinsic scatter hyperparameter, 𝜎Rel, for hierarchically
modelling and analysing siblings. Further developing and applying these models to future
larger samples of SNe Ia may lead to improvements in SN Ia standardisation for cosmology.

In Chapter 3, I build the publicly-available Bird-Snack model, to perform Bayesian
Inference of R𝑉 Distributions using SN Ia Apparent Colours at peaK. I use Gaussian processes
and a hierarchical Bayesian model to analyse optical-to-near-infrared light curves of 65
low-redshift SNe Ia with data near peak-brightness, and infer the host galaxy dust population
distributions without assuming any cosmology. I identify new best practices and avenues of
research for future hierarchical Bayesian analyses of larger samples.

In Chapter 4, I develop and model 𝜎Rel – the intrinsic scatter of siblings photometric
distance estimates relative to one another within a galaxy – to analyse a unique system of three SN Ia siblings in the nearby Cepheid-calibrator galaxy, NGC 3147. Their photometric
data include new Pan-STARRS-1 𝑔𝑟𝑖𝑧𝑦 light curves of the new sibling, SN 2021hpr, from
the Young Supernova Experiment. I develop a bespoke model that facilitates, for the first
time, a simultaneous fit to the siblings’ light curves, whilst marginalising over 𝜎Rel with
an informative hyperprior; this demonstrates how siblings can be robustly modelled to
study SN-host correlations. I then apply this model to infer the Hubble constant, further
demonstrating how siblings can be hierarchically modelled to infer cosmology.

In Chapter 5, I develop new publicly available methods to hierarchically analyse the
spectroscopic sample of 12 SN Ia sibling-pair galaxies from the Zwicky Transient Facility
survey. I use simulations to investigate the efficacy of various hyperprior choices for
constraining the siblings’ intrinsic scatter hyperparameters, and, for the first time, place
constraints on the correlation between photometric distance estimates to SN Ia siblings.

In Chapter 6, I summarise this thesis’ outcomes and present an outlook for future work.</dcterms:abstract>
   <uketdterms:institution>University of Cambridge</uketdterms:institution>
   <dcterms:issued>2024-08-30</dcterms:issued>
   <dc:type>Thesis</dc:type>
   <uketdterms:qualificationlevel>Doctoral</uketdterms:qualificationlevel>
   <uketdterms:qualificationname>Doctor of Philosophy (PhD)</uketdterms:qualificationname>
   <dc:language>eng</dc:language>
   <dcterms:isReferencedBy xsi:type="dcterms:URI">https://www.repository.cam.ac.uk/handle/1810/377285</dcterms:isReferencedBy>
   <dc:identifier xsi:type="dcterms:URI">https://www.repository.cam.ac.uk/bitstreams/2081b957-8246-435c-b7ae-4e6477ba5b55/download</dc:identifier>
   <uketdterms:checksum xsi:type="uketdterms:MD5">a817e14c1b92aa52bb41081cfffaf55c</uketdterms:checksum>
   <dcterms:license>https://www.repository.cam.ac.uk/bitstreams/ea4c51f3-3837-46d6-a0b0-270017e4fd98/download</dcterms:license>
   <uketdterms:checksum xsi:type="uketdterms:MD5">87eda9de84448d1f82354d60eee3eb5f</uketdterms:checksum>
   <dc:rights>https://www.rioxx.net/licenses/all-rights-reserved/</dc:rights>
   <dc:subject>Astronomy</dc:subject>
   <dc:subject>Astrostatistics</dc:subject>
   <dc:subject>Cosmology</dc:subject>
   <dc:subject>Hierarchical Bayes</dc:subject>
   <dc:subject>Supernovae</dc:subject>
</uketd_dc:uketddc>
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