<?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>2026-09-25T02:59:04Z</responseDate><request verb="GetRecord" identifier="oai:www.repository.cam.ac.uk:1810/241039" metadataPrefix="uketd_dc">https://api.repository.cam.ac.uk/server/oai/request</request><GetRecord><record><header><identifier>oai:www.repository.cam.ac.uk:1810/241039</identifier><datestamp>2024-06-27T12:32:36Z</datestamp><setSpec>com_1810_198332</setSpec><setSpec>com_1810_256064</setSpec><setSpec>col_1810_214775</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>Blind and pointed Sunyaev-Zel'dovich observations with the Arcminute Microkelvin Imager</dc:title>
   <dc:identifier xsi:type="dcterms:DOI">10.17863/CAM.16580</dc:identifier>
   <dc:creator>Shimwell, Timothy William</dc:creator>
   <dcterms:abstract>In this thesis I discuss my work on the Arcminute Microkelvin Imager (AMI). I focus on the detection of Sunyaev-Zel’dovich (SZ) signatures at 14-18GHz.
Once the background science and operation of the instrument are described I proceed to present my contribution to the calibration of AMI, including: primary beam measurements; refinements to the known antenna geometry and flagging geostationary satellite interference. This is followed by an outline of the software that I have developed to subtract sources from visibilities, concatenate data from multiple observations, simulate data, and perform jack-knife tests to evaluate the magnitude of systematic errors.
The Bayesian analysis that I use to obtain parameter estimates and to quantify the significance of putative SZ detections is described. I perform realistic simulations of clusters and use these to characterise
the analysis. I then, for the first time, apply the analysis to data from the AMI blind cluster survey. I identify several previously unknown
SZ decrements.
Finally, I conduct pointed observations towards a high luminosity subsample of eight clusters from the Local Cluster Substructure Survey
(LoCuSS). For each of these I provide probability distributions of parameters such as mass, radius,  and temperature. I compare my
results to those in the literature and find an overall agreement.</dcterms:abstract>
   <uketdterms:institution>University of Cambridge</uketdterms:institution>
   <dcterms:issued>2011-11-08</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>
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   <dcterms:isReferencedBy xsi:type="dcterms:URI">https://www.repository.cam.ac.uk/handle/1810/241039</dcterms:isReferencedBy>
   <dc:identifier xsi:type="dcterms:URI">https://apollo8-f-pro.lib.cam.ac.uk/bitstreams/b1d449dc-5013-4c49-9672-80108e0a4409/download</dc:identifier>
   <uketdterms:checksum xsi:type="uketdterms:MD5">96f8c58b27aed6a9af5f374f42c41bb2</uketdterms:checksum>
   <dcterms:license>https://apollo8-f-pro.lib.cam.ac.uk/bitstreams/26b2e9aa-ce44-4906-8b8d-03527ce2d29c/download</dcterms:license>
   <uketdterms:checksum xsi:type="uketdterms:MD5">0b1a12d4eb169023d6d65183e2d7aac9</uketdterms:checksum>
   <dc:rights>https://www.rioxx.net/licenses/all-rights-reserved/</dc:rights>
   <dc:subject>Observationjal cosmology</dc:subject>
   <dc:subject>Interferometry</dc:subject>
</uketd_dc:uketddc>
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