Currently pursuing a Ph.D. degree in Astronomy at the Institute of Astronomy, Geophysics and Atmospheric Sciences of the University of São Paulo (IAG/USP) supervised by Prof. Claudia Lucia Mendes de Oliveira. Participated in an undergraduate research in the S-PLUS collaboration, cosupervised by Ph.D. Felipe de Almeida Fernandes, on the determination of stellar atmospheric parameters using photometry (FAPESP grant 2021/09528-4). Recently working on the characterization of substructures of accreted stars in the galactic halo using photometric metallicities. Topics of interest: Photometry; Determination of Stellar Parameters; Structure and Formation of the Galaxy. (Source: Lattes Curriculum)
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The lambda-Cold Dark Matter (lambda-CDM) cosmological model predicts a hierarchical formation process of the structures present in the universe, in such a way that galaxies like ours must have started their histories much smaller than they are today but were then formed through cannibalization of lower mass systems. With the advent of the Gaia survey, especially, more recently, its 3rd da…
It's undeniable that knowing stellar parameters (effective temperature, surface gravity, and metallicity) is important for many fields in astronomy. One way to obtain these parameters is through multi-band photometry, like the one provided by the S-PLUS survey. The outstanding characteristic of S-PLUS is the use of 12 filters, including 5 broad-bands and 7 narrow-bands centered in key spe…
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