Reproducing the observational parameters of the MW and the Andromeda galaxy (M31) by modeling their merger
Investigating the origin of dwarf galaxies in the Vast Polar Structure (VPOS) of the Milky Way from the tidal tail ejected from the major merger at M31.
Investigating the timing argument calculation in the context of the major merger of the M31.
Analyzing the rotation curve of the Milky Way to deduce the distribution of the dark matter in the galaxy.
Mapping and modeling the orbits of dwarf galaxies and globular clusters within the Milky Way to understand their origins and interactions.
Calculating the polarisation of Stars in the Kepler field from their polarimetric observations.