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
I am a Software and Systems Engineer specializing in astronomical instrumentation and large-scale observatory operations. Currently a Software Engineer at the National Radio Astronomy Observatory (NRAO), my career includes high-level software development with deep academic research in stellar astrophysics. Previously, I led software development of the operations team of the Gemini Observatory (NOIRLab) and served as Systems Engineer for the Giant Magellan Telescope Brazil Office (GMTBrO), where I coordinated national technical contributions to the global consortium. Grounded by a dual PhD in Stellar Astrophysics from IAG-USP and the University of Nice, alongside postdoctoral tenures at ESO Chile, I combine advanced data techniques -- including radiative transfer modeling, spectroscopy, and optical interferometry --and robust engineering to power current and next-generation astronomical systems.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 | Completed scholarships in Brazil |
| 1 | Completed scholarships abroad |
| 4 | All Scholarships |
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