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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01gx41mn13b
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dc.contributor.advisorDaylan, Tansu-
dc.contributor.advisorWinn, Joshua-
dc.contributor.authorMurray, Emily-
dc.date.accessioned2023-07-20T17:18:12Z-
dc.date.available2023-07-20T17:18:12Z-
dc.date.created2023-05-01-
dc.date.issued2023-07-20-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01gx41mn13b-
dc.description.abstractWith the rapid rate of exoplanet discoveries, established exoplanet populations need to be continually revisited and updated. Identifying clusters of exoplanets based on major characteristics is a data- driven way to accomplish this. In this paper, I cluster exoplanets based on planetary mass, radius, insolation flux, and multiplicity, as well as stellar age, metallicity, multiplicity, and gravitational constant. However, examining clusters identified by single clustering algorithms does not provide information on how robust these clusters are. This paper presents an algorithm to match similar clusters found across different clustering algorithms and subsets of data. By comparing clusters based on how consistently they are identified across iterations of clustering, I determine the most robust patterns and evaluate which clustering algorithms are the most effective at identifying robust clusters.en_US
dc.format.mimetypeapplication/pdf
dc.language.isoenen_US
dc.titleEvaluating Clustering Algorithms as Applied to Exoplanet Populationsen_US
dc.typePrinceton University Senior Theses
pu.date.classyear2023en_US
pu.departmentAstrophysical Sciencesen_US
pu.pdf.coverpageSeniorThesisCoverPage
pu.contributor.authorid920228171
pu.mudd.walkinNoen_US
Appears in Collections:Astrophysical Sciences, 1990-2023

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