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During my 1st year of PhD, my main focus has been the development of a software package called SPICE. This tool enables differentiable, fast spectra synthesis for stars with inhomogeneities, such as star spots or pulsations. I will present an overview of the implementation and underlying physical assumptions of this software. The presentation will include various use cases demonstrating the application of this tool to specific stellar phenomena. Additionally, I will cover preliminary results from a secondary research project examining the relationship between stellar ages and orbital characteristics within the Galactic Bulge. |
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