Fig. 1: S/N detection map for KELT-20b.
LMU Munich, 2024 – ongoing
Using the FOCES spectrograph at Wendelstein Observatory, this work explores atmospheric compositions of three ultra-hot Jupiters (KELT-20b, KELT-9b, and WASP-189b) through high-resolution spectroscopy.
Fig. 2: VISit simulation of high density gradient gas filament under self gravity (left: initial, right: final)
SASTRA University & Duisburg-Essen, 2021–2022
This simulation-based study examined how embedding in larger environments affects the edge-effect in star-forming filaments, offering a fresh lens on filament stability.
Fig. 3: Decomposed rotational curve of NGC 1068
Tod’Aérs Fellowship, 2020–2021
Led a team that analytically studied the distribution of dark matter mass around 34 spiral galaxies using least-squares regression of rotational curves.
See PublicationSSERD Research Internship, 2020
Identified inverse correlation between sunspot area and flare activity parameters and built an ensemble boosting ML model with 79% accuracy to predict Solar Flare Index.
See Publication