Member of the Scientific Operations team of the Gemini Observatory (AURA). Researcher in the field of Stellar Astrophysics and Astronomical Instrumentation. He has a postdoctoral degree at the European Southern Observatory (ESO Chile) and the Institute of Astronomy, Geophysics and Atmospheric Sciences of the University of São Paulo (IAG-USP), where he also acted as Systems Engineer at the Giant Magellan Telescope Brazil Office (GMTBrO). He holds a double-degree PhD from IAG-USP (Brazil) and the University of Nice Sophia Antipolis (UNS, France). The research is focused on the study of peculiar hot stars employing multiple observational techniques (spectroscopy, polarimetry, optical interferometry) and radiative transfer modeling. Keywords: stellar astrophysics - circumstellar environment - astrophysical disks - astronomical instrumentation - systems engineering. (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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