Anders, FriedrichCuevas Bullich, Aleix2022-10-062022-10-062022-02https://hdl.handle.net/2445/189706Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutor: Friedrich AndersIn 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 group5 p.application/pdfengcc-by-nc-nd (c) Cuevas, 2022http://creativecommons.org/licenses/by-nc-nd/3.0/es/Via LàctiaAgrupament vermellTreballs de fi de grauMilky WayRed clumpBachelor's thesesinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/openAccess