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
A seasoned Software Engineer at the National Radio Astronomy Observatory (NRAO), I specialize in Astronomical Instrumentation and Operations. Prior to joining NRAO, I served as an Operator at the Gemini-North Observatory (NOIRLab) and led the team's software development efforts. My academic journey includes postdoctoral research at the European Southern Observatory (ESO Chile) and the Institute of Astronomy, Geophysics, and Atmospheric Sciences of the University of São Paulo (IAG-USP). At IAG-USP, I also held the position of Systems Engineer at the Giant Magellan Telescope Brazil Office (GMTBrO), coordinating Brazil's technical involvement in the consortium. I earned my doctorate from IAG-USP (Brazil) and the University of Nice Sophia Antipolis (UNS, France) in Stellar Astrophysics. The thesis focused on the study of peculiar hot stars through the application of multiple observational techniques (spectroscopy, polarimetry, optical interferometry) and radiative transfer modeling. Keywords: software engineering -- astronomical instrumentation -- systems engineering -- stellar astrophysics. (Source: Lattes Curriculum)
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Since FAPESP entered the GMT Project and since the creation of the GMTBrO (GMT Brazil Office), we've been trying to collaborate with other members on the conception of the instruments to be installed in Giant Magellan Telescope (GMT). For the GMACS Spectrograph the chosen candidate will be trained in the Instrumentation and Systems Engineering areas. This professional will establish a lin…
Among hot stars, one class has been extensively studied by modern techniques: the Be stars. Mainly due to interferometry, which is capable of angularly resolving their circumstellar environment and even their photosphere, much progress have been achieved to our understanding of physical processes of great astrophysical interest such as stellar rotation, dynamical processes in astrophysica…
The project intends to determine physical parameters and chemical abundances for a sample of galactic planetary nebulae with bipolar morphology, and use these results to model the objects using a photoionization code. The project has two complimentary parts: new observational data will be collected for a sample of bipolar nebulae and the results, combined to data from the literature, will…
Among hot stars, one class has been extensively studied by modern techniques: the Be stars. Mainly due to interferometry, which is capable of angularly resolving their circumstellar environment and even their photosphere, much progress have been achieved to our understanding of physical processes of great astrophysical interest such as stellar rotation, dynamical processes in astrophysica…
| 3 / 3 | Completed scholarships in Brazil |
| 1 / 1 | Completed scholarships abroad |
| 4 / 4 | All Scholarships |
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