bachelor's at Bacharelado em Física from Instituto de Física - USP (2006), master's at Astronomy from Instituto de Astronomia, Geofísica e Ciências Atmosféricas - USP (2009) and doctorate at Astronomy from Instituto de Astronomia, Geofísica e Ciências Atmosféricas - USP (2012). Has experience in Astronomy, acting on the following subjects: active galactic nuclei and spectroscopy. (Source: Lattes Curriculum)
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Galactic nuclei provide fundamental information about the formation and evolution of galaxies. Most, if not all, massive galaxies host supermassive black holes (SMBHs) at their nuclei, with masses between one million and ten billion solar masses. Correlations between the masses of the SMBHs and certain parameters of the host galaxies suggest a possible co-evolution between the galaxies an…
Light curves are astronomical data used for the study of the brightness variability of stars, which can potentially result in the discovery of exoplanets, due to the eclipses (detected in the light curves) caused by the passage of the exoplanets between the observed star and the observer. Light curves show high-frequency noise that can make it difficult to detect eclipses and to determine…
In this project, we propose to study data cubes from two statistically complete samples of galaxies. The first of them will be composed by objects of morphological types E+S0 and the second by objects of types Scd+Sd. The galaxies of types E+S0, in general, have high mass, little gas, low star formation, are dominated by classical bulges and often show nuclear activity. However, the ones …
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