Galaxy clusters are a unique laboratory that trace the formation and evolution of structure on the largest scales in the universe. In addition, clusters host an array of complex internal physical processes from star-formation and active galactic nuclei to turbulent gas motions. The ability to accurately estimate total cluster mass based on observable signals is a challenging but essential ingredient to use the full potential of clusters for precise cosmological constraints or studies of cluster astrophysics.
In this dissertation, I present 152 GHz observations of galaxy clusters taken with the APEX-SZ imaging bolometer array. APEX-SZ is designed to image the small distortion in the Cosmic Microwave Background (CMB) due to the scattering of CMB photons off hot cluster electrons, known as the Sunyaev-Zel’dovich effect (SZE). A primary goal of APEX-SZ is to constrain power law scaling relations between the integrated SZE flux and cluster mass. I detail the extensive efforts taken to carefully clean and calibrate raw APEX-SZ data before parametrically modeling the sky signal, removing the effects of the instrumental response function in the final measurements. I explore and attempt to reduce the impact of potential systematic effects for each step in the data analysis process.
I present scaling relations between SZE flux and X-ray temperature, a proxy for total mass, along with the maximum likelihood regression parameters for the full data set and several interesting subsets. I compare to expectations from theory and numerical simulations and find that the APEX-SZ scaling relations are consistent with the gravitationally-dominated self-similar model of cluster evolution. Additionally, I find that the SZE scaling relation is insensitive to the dynamical state of the cluster, although the associated intrinsic astrophysical scatter does increase between relaxed and disturbed clusters.
|Advisor:||Halverson, Nils W.|
|Commitee:||Darling, Jeremy, DeWolfe, Oliver, Glenn, Jason, Shull, J. Michael|
|School:||University of Colorado at Boulder|
|Department:||Astrophysical and Planetary Sciences|
|School Location:||United States -- Colorado|
|Source:||DAI-B 73/04, Dissertation Abstracts International|
|Keywords:||APEX-SZ, Cosmic microwave background, Galaxy clusters, Observations, Sunyaev-zel'dovich effect|
Copyright in each Dissertation and Thesis is retained by the author. All Rights Reserved
The supplemental file or files you are about to download were provided to ProQuest by the author as part of a
dissertation or thesis. The supplemental files are provided "AS IS" without warranty. ProQuest is not responsible for the
content, format or impact on the supplemental file(s) on our system. in some cases, the file type may be unknown or
may be a .exe file. We recommend caution as you open such files.
Copyright of the original materials contained in the supplemental file is retained by the author and your access to the
supplemental files is subject to the ProQuest Terms and Conditions of use.
Depending on the size of the file(s) you are downloading, the system may take some time to download them. Please be