Mapping the Circumgalactic Medium: Connecting Galaxies to their Environment

dc.contributor.advisorWerk, Jessica
dc.contributor.authorWilde, Matthew
dc.date.accessioned2022-09-23T20:42:33Z
dc.date.available2022-09-23T20:42:33Z
dc.date.issued2022-09-23
dc.date.submitted2022
dc.descriptionThesis (Ph.D.)--University of Washington, 2022
dc.description.abstractThe work presented in this dissertation provides the groundwork for understanding key unresolved questions in the study of galaxy evolution: the circumgalactic medium (CGM) and the role of environment. I present a new survey that has the power to drastically improve our understanding of the CGM and use it to estimate the size of the CGM as a function of galactic mass. In addition, a novel method to reconstruct the cosmic web using \textit{Physarum polycephalum} slime mold is presented and applied to the SDSS surveys. This cosmic web reconstruction was released publicly with SDSS DR17 and will allow exciting connections between galaxies and their environments to be illuminated, to distances greater than other previous catalogs.
dc.embargo.termsOpen Access
dc.format.mimetypeapplication/pdf
dc.identifier.otherWilde_washington_0250E_24808.pdf
dc.identifier.urihttp://hdl.handle.net/1773/49255
dc.language.isoen_US
dc.rightsCC BY
dc.subjectCGM
dc.subjectCircumgalactic Medium
dc.subjectData Science
dc.subjectGalaxy Evolution
dc.subjectSlime Mold
dc.subjectAstrophysics
dc.subject.otherAstronomy
dc.titleMapping the Circumgalactic Medium: Connecting Galaxies to their Environment
dc.typeThesis

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