My current research focuses on establishing observational constraints on the
origins of the chemical elements in the Galaxy and the Universe through spectroscopic
analysis of low-metallicity stars. Below you can find an interactive plot with a few selected
synthetic spectra for stars with different metallicities ([Fe/H] - upper panel) and different carbon
abundances ([C/Fe] - lower panel). All the spectra have the same effective temperature (Teff = 5250K)
and surface gravity (logg=2.5). More details soon!
Access the simple jupyter notebook with the code to generate this plot: