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Biographical Info
My research focuses on reconstructing the formation conditions of the Milky Way using the positions, kinematics, ages, and chemical compositions of pulsating variable stars. I use data from proprietary surveys and publicly available databases, including (but not limited to) the Halo Outskirts With VAriable STars (HOWVAST), the Southern Stellar Stream Spectroscopic Survey (S⁵), and the Gaia mission. These projects are pivotal to lay the groundwork for exploiting the large amount of data upcoming in the next generation of large sky surveys.
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Biographical Info
As a member in the SDSS-V collaboration, I work mainly on developing and running the spectral analysis pipelines for the Milky Way Mapper (MWM). My research focuses on analysing the chemo-dynamical properties of star clusters and stellar populations in the Milky Way and nearby dwarf galaxies. I also developed a real-time extraction GUI software for a new IFU instrument (IFU-M) designed for use on the Magellan/Clay telescope.
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