CV Lattes
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Universidade de São Paulo (USP). Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG) (Institutional affiliation for the last research proposal) Birthplace: Brazil
Astrophysics PhD student at Swinburne University of Technology in Melbourne, Australia. Master of Science in Astronomy from the Institute for Astronomy, Geophysics and Atmospheric Sciences of the University of Sao Paulo. Bachelor of Science in Astronomy from the Institute for Astronomy, Geophysics and Atmospheric Sciences of the University of Sao Paulo (2018). Developed an academic internship in Centro de Estudios de Fisica del Cosmos de Aragon, in Teruel, Spain (July/2017) and in the Institute for Astrophysics of the University of Vienna, Austria (April/2019 - July/2019). (Source: Lattes Curriculum)
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One recent discovery has challenged our theoretical understanding of the life histories of galaxies. Ultra Diffuse Galaxies (UDGs) were found unexpectedly in extremely deep images of clusters of galaxies. Intriguingly, these are galaxies that have the sizes of giants but the luminosities of dwarfs.In this project, we will address problems in galaxy formation and evolution using observatio…
Recovering galaxies' formation histories and evolution using a combination of parametric and non-parametric fits of their multi-band-photometry is a novel and promising field in astronomy. Using multi band photometry of the galaxy NGC 3115, as observed with several telescopes at various wavelenghts, from ultraviolet to infrared data, we intend to mimic the study of multi-wavelength images…
Galaxy evolution can be studied either through spectroscopy or photometry. We plan to use both these methods to recover information about the formation of lenticular galaxies and to study how they relate to spiral galaxies. We will also study multi-band photometry of the Large Magellanic Cloud or of one field in the Strip 82, as observed by the Brazilian robotic telescope T80-South and it…
In this project, we propose to use MUSE/VLT data of the intriguing merging galaxy NGC 1487, in order to map its chemical distribution in a pixel-by-pixel manner, and to determine the mechanism that is producing inhomogeneities in its metal distribution, as suggested by previous Gemini data. Although gas flows could be responsible in producing flat and inverted metallicity gradients, the r…
IAG-USP is part of the Brazilian-Spanish collaboration JPAS (Javalambre Physics of the Accelerating Universe Astrophysical Survey), a photometric sky survey of 8000 square degrees of the sky done in 59 filters. The designs of the J-PAS camera and filter system allow mapping not only the positions and colors of hundreds of millions of galaxies in the sky, but to study their clustering prop…
| 3 / 3 | Completed scholarships in Brazil |
| 2 / 2 | Completed scholarships abroad |
| 5 / 5 | All Scholarships |
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