At Institute of Space Technology, I contribute to research investigating cosmic ray properties and flux variations, supporting data collection, processing, and preliminary statistical analysis of detector output using Python.
I'm building an automated fitter for SDSS spectra of OB stars that detects and fits spectral lines, aiming to make measurements consistent and reproducible across many spectra.
I built a PostgreSQL database of 6,336 confirmed exoplanets from the NASA Exoplanet Archive and connected it to Python for analytical queries and visualizations. I also published the project, including its documentation, on GitHub.
My projects include a Python spectral-data fitter, numerical N-body simulations validated against ephemeris data, and a browser-based planetarium that renders the night sky from astronomical catalogs.
