GASP
GASP (GAs Stripping Phenomena in galaxies with MUSE) is an ESO Large Program carried out with the MUSE Integral Field spectrograph on the Very Large Telescope to observe over a hundred galaxies.
I collect photons from galaxies and transform them into useful information about their contents.
I obtained my PhD in 2019 from the Federal University Santa Catarina (Brazil). I am now a postdoc in the GASP team, studying jellyfish and post-starburst galaxies. If you want to know more about me and my scientific activity, explore this website!
Projects
S-PLUS
The S-PLUS survey is mapping two thirds of the southern sky in twelve optical bands, including seven narrow band filters.
Intermediate redshift clusters
Using data from MUSE GTO datacubes, we have identified and characterized post-starburst and jellyfish galaxies in eight galaxy clusters at z~0.35. Integrated spectra of the full sample can be explored with this dashboard
SDSS + GALEX Synthesis
During my PhD, I have developed a method to combine spectroscopic and photometric information in the STARLIGHT spectral synthesis code. We have applied this method to a sample of galaxies with SDSS spectra and GALEX photometry (Werle et al. 2019, 2020). Results for a volume-limited sample (including only the NUV band) are available here .