I have a Bachelor's and a Master's degree in Astronomy from the Institute of Astronomy, Geophysics and Atmospheric Sciences of the University of São Paulo (IAG/USP). Currently, I am a PhD student at the Max Planck Institute for Astronomy, working with the characterization of exoplanets, more specifically warm Jupiters, using radial velocity and transit data. I have experience in the area of #8203;#8203;Stellar Astrophysics, precise characterization of solar twins, chemical abundances with neural networks and detection of exoplanets with radial velocity. (Source: Lattes Curriculum)
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The objective of the project is to study spectra of solar twin stars in order to identify and analyze spectroscopic chemical signatures of planetary material. We will extend the sample of solar twins which were previously analyzed with high precision, to better characterize how rare the chemical composition of the Sun is and to study the evolution of chemical abundances in the Galactic di…
The project aims to study the chemical element lithium in the interior of metal rich solar analogs stars, in order to verify the prediction of a greater destruction of this element inside stars with larger metallic content, due to the deepening of the convective zone in more metal-rich stars.
The objective of the project is to study the radial velocity method in Astronomy, which is important for the detection of new exoplanets and for the confirmation and characterization of exoplanets detected with the transit technique. We will use data from the literature to study different planetary orbits, and also data gathered by our group SAMPA for the detection of planets around solar…
Solar twins were important to develop a manual method of precise differential chemical abundances, allowing to achieve a precision at the 0.01 - 0.02 dex level. In this project we aim to use solar twins to develop an automatic code to achieve the same level of precision that is achieved with the manual line-by-line differential method, or perhaps even better, at the 0.01 dex or sub-0.01 d…
This project has the aim of using improved tools for the characterization of exoplanets through data obtained with the radial velocity and transit techniques. We will employ the versatile code Juliet using known exoplanets in the literature, for which there are public data available. In this way, the student will benefit by learning cutting-edge tools, and also the group at STScI will ben…
| 3 / 3 | Completed scholarships in Brazil |
| 2 / 2 | Completed scholarships abroad |
| 5 / 5 | All Scholarships |
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CV Lattes
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