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http://hdl.handle.net/2445/189706
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DC Field | Value | Language |
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dc.contributor.advisor | Anders, Friedrich | - |
dc.contributor.author | Cuevas Bullich, Aleix | - |
dc.date.accessioned | 2022-10-06T16:52:53Z | - |
dc.date.available | 2022-10-06T16:52:53Z | - |
dc.date.issued | 2022-02 | - |
dc.identifier.uri | http://hdl.handle.net/2445/189706 | - |
dc.description | Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutor: Friedrich Anders | ca |
dc.description.abstract | In this work we use the Extreme Deconvolution algorithm to extract the underlying distribution function from an heterogeneous and noisy star sample of 10,941 Red Clumps from the GALAH+ DR3 survey. This algorithm allows us to describe the density probability function as a sum of Gaussians that we can interpret as distinct Galactic components. We are able to clearly distinguish the thin and thick disk components, and the hαmr group | ca |
dc.format.extent | 5 p. | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | eng | ca |
dc.rights | cc-by-nc-nd (c) Cuevas, 2022 | - |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ | * |
dc.source | Treballs Finals de Grau (TFG) - Física | - |
dc.subject.classification | Via Làctia | cat |
dc.subject.classification | Agrupament vermell | cat |
dc.subject.classification | Treballs de fi de grau | cat |
dc.subject.other | Milky Way | eng |
dc.subject.other | Red clump | eng |
dc.subject.other | Bachelor's theses | eng |
dc.title | Analysing the red-clump star population of the Milky Way with abundance-space extreme deconvolution | eng |
dc.type | info:eu-repo/semantics/bachelorThesis | ca |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | ca |
Appears in Collections: | Treballs Finals de Grau (TFG) - Física |
Files in This Item:
File | Description | Size | Format | |
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CUEVAS BULLICH ALEIX_5181446_assignsubmission_file_TFG-Cuevas-Bullich-Aleix.pdf | 2.25 MB | Adobe PDF | View/Open |
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