Universidade de São Paulo (USP). Instituto de Física (IF) (Institutional affiliation from the last research proposal) Birthplace: Brazil
Gabriela Satie Sato-Polito in research grants and scholarships supported by FAPESP.
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In the Halo Model (HM), the fundamental objects that we employ to describe matter distribution in the Universe are the structures which have already experience gravitational collapse: galaxy clusters, galaxy groups, even field galaxies. From a cosmological perspective, the large-scale structure of the Universe is characterized by the positions and velocities of those collapsed regions. Si…
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