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Universidade de São Paulo (USP). Instituto de Física (IF) (Institutional affiliation from the last research proposal) Birthplace: Brazil
Graduated at Physics from Universidade de São Paulo (2006), master's (2009) and PhD (2013) at Astronomy from Universidade de São Paulo. My work is on Cosmology, particularly in statistical tests to constrain cosmological parameters, universes locally inhomogeneous, modified gravitational theories and alternative models to explain the acceleration of the universe. (Source: Lattes Curriculum)
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Whole-sky surveys are revolutionizing the way research is conducted in cosmology. In order to extract the maximum scientific output, standard methods used in the analyses need to be refined so systematic errors are not included. The Dark Energy Survey will map the sky in the optical bandwidth and will detect 200 million galaxies and 100 thousand galaxy clusters, aiming at providing a bett…
Galaxy clusters probe the high-end limit of the halo mass function, where their abundance is very sensitive to how structures formed in the Universe and therefore to cosmological parameters. In order to take full advantage of these objects, one must connect the observed cluster richness, i.e. the number of galaxies in a cluster, with the mass of the halo where the cluster resides. This is…
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