CV Lattes
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Universidade de São Paulo (USP). Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG) (Institutional affiliation from the last research proposal) Birthplace: Brazil
bachelor's at Bacharelado em Física from Instituto de Física da Universidade de São Paulo (1995), master's at Astronomy from Universidade de São Paulo (1998) and doctorate at Astronomy from Universidade de São Paulo (2002). Has experience in Astronomy, focusing on Extragalactic Astrophysics, acting on the following subjects: aglomerados de galaxias, lentes gravitacionais, galáxias: interações, grupos fósseis and energia escura. (Source: Lattes Curriculum)
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The object of study of this research project are galaxy clusters in the context of the LSST survey, with extensive use of mass determination via weak gravitational lensing.Due to their privileged position at the top of the process of hierarchical formation of the structures of the Universe, clusters occupy an intersection between astrophysics and observational cosmology. On the one hand, …
Galaxy clusters are the object of study of this research project. We plan to do several studies in the context of the optical surveys: CODEX, S-PLUS and J-PAS, projecting for more future surveys such as the LSST.Due to their privileged position at the top of the process of hierarchical formation of the structures of the Universe, clusters occupy an intersection between astrophysics and o…
This project focus on galaxy clusters in the context of the J-PAS survey and preliminary surveys, such as S-PLUS. Clusters are on the pinnacle of the hierarchical structure formation process in the Universe. For that reason they lie in the crossroads between astrophysics and cosmology and thus are a rich source of information regarding dark matter and energy. One of the points of this p…
This project focus on galaxy clusters. Clusters are on the pinnacle of the hierarchical structure formation process in the Universe. For that reason they lie in the crossroads between astrophysics and observational cosmology. The amount and distribution of such objects carry information on the Universe that has formed then, including the dark energy. On the other hand, due to is almost c…
(Only some records are available in English at this moment)
This IC project focus on the use of weak-lensing techniques for the determination of the mass-richness relation of galaxy clusters using the CS82 survey data. This is a crucial step towards the determination of cosmological parameters through galaxy clusters count. Recently this kind of calibration has been done by the use of the stacking of the lensing signal of multiple systems in bins …
In our current understanding of the structure formation in the universe, dominated by cold dark matter, growth happens hierarchically, through fusions. Galaxy clusters have a special position in this scenario as they are the largest structures (dark matter halos) to have reach equilibrium. For reason not yet completely understood the radial density profile of those halos, over 5 decades i…
The goal of this project is to perform a analysis of the central region of the supercluster of galaxies SC0028-0001 through weak gravitational lensing techniques. This work in part of thorough analysis of this object that includes also dynamical and X-ray analysis. The ultimate goal of the whole project is to test whether the spheric collapse model provides a good description for the cen…
(Only some records are available in English at this moment)
| 2 / 2 | Ongoing grants |
| 4 / 4 | Completed research grants |
| 8 / 6 | Completed scholarships in Brazil |
| 14 / 12 | All research grants and scholarships |
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