graduation at F sica from Universidade de São Paulo (1998), master's at Astronomy from Universidade de São Paulo (2001) and doctorate at Astronomy from Universidade de São Paulo (2005). He is currently full professor at Universidade Cruzeiro do Sul. Has experience in Astronomy, focusing on Astronomy, acting on the following subjects: infrared, seyfert, galaxy:ism, computação científica and ism. (Source: Lattes Curriculum)
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The integrated spectra of stellar systems contain an abundance of information, and its analysis can reveal fundamental parameters such as metallicity, age and star formation history. A method widely used to analyze these spectra is the spectral fitting technique, based on modeling the galaxy spectra with a combination of stellar population spectra from a given library. Despite being a pow…
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The nuclear activity phenomenon is a result of the gas and star feeding of supermassiveblack holes (SMBHs) hosted in the central region of galaxies. One of the greatest current challenges is to understand how active galactic nuclei (AGNs) can be fed during their lifetime. The search for universal feeding mechanisms has been made searching for morphological signatures in the central kpc re…
Synthetic stellar spectra are widely used in many different applications in astronomy, from determining atmospheric parameters to being used as ingredients to the study of the stellar population of galaxies. One of the main input parameters of spectral synthesis codes that generate these spectra are the atomic and molecular line lists, which contain the atomic parameters of the absorpti…
Libraries of stellar spectra are fundamental tools for the study of stellar popu-lations. Despite the significant improvement of recent libraries, there is still a lot tobe done in order to have libraries that are able to generate models that can reproducethe observed stellar population spectra of real galaxies. Theoretical stellar libraries areparticularly interesting for stellar populat…
Starburst features in the optical are nowadays well known, but the use of this knowledge is not always possible (e.g. objects heavily obscured). In this case the near-IR is of unprecedented value. Recent models show that TP-AGB stars should dominate the NIR spectra of populations 0.3 to 2 Gyr old. We propose here to take advantage of the ideal coverage of the IRTF Spex instrumentto create…
| 1 / 1 | Ongoing research grants |
| 12 / 8 | Completed research grants |
| 6 / 2 | Completed scholarships in Brazil |
| 2 / 2 | Completed scholarships abroad |
| 21 / 13 | All research grants and scholarships |
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CV Lattes
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