My primary research interest is to understand the physical processes responsible for X-ray emission and its interaction with the surrounding environment in X-ray binaries (XRBs). I pursue this by studying X-ray light curves, power density spectra (PDS), and energy spectra of both black hole (BH) and neutron star (NS) systems, focusing primarily on the X-ray band. More broadly, my work aims to investigate the physics of accretion flows around compact objects across multiple spectral states and to constrain the geometry and physical properties of the accretion disk, corona, and relativistic reflection regions through a combination of broadband X-ray spectral and timing analyses. In addition, I am also interested in understanding the ionized outflows in active galactic nuclei (AGN), which I study through high-resolution X-ray spectroscopy. For these studies, I utilize data from multiple missions such as AstroSat, NICER, NuSTAR, Chandra, XMM-Newton, and XRISM.