I am Associate Professor at
                Leiden Observatory, Leiden University, in the
                Netherlands. I am passionate about unravelling the
                mystery of how galaxy clusters, the largest and most
                massive gravitationally bound structures in our
                Universe, came into existence. Galaxy clusters and their
                surroundings, are also unique laboratories for
                determining the physics of particle acceleration,
                studying the effects of environment and feedback on
                galaxy evolution, and probing the origin of magnetic
                fields. Low-frequency radio telescopes play an essential
                role in addressing the scientific questions in this
                domain. The opportunity to lead at the forefront of
                low-frequency radio astronomy, with its accompanying
                fascinating technical and computational challenges,
                along with its vast potential for discovery, is
                something that is also incredibly exciting. 
              
              
My group at
                Leiden Observatory  focuses on two main topics.
                Firstly, we study cosmic rays and magnetic fields in
                galaxy clusters. We aim to understand how cosmic rays
                are accelerated and to unravel the origin of magnetic
                fields in these clusters. To achieve this, we observe
                clusters using large radio telescopes such as the VLA,
                GMRT, MeerKAT, and LOFAR. Additionally, we supplement
                these radio observations with X-ray data to study the
                hot plasma in clusters. Secondly, we work on developing
                low-frequency calibration and imaging techniques.
                Low-frequency observations are challenging due to
                ionospheric blurring effects, and our goal is to develop
                methods to mitigate this blurring. Currently, we are
                focused on observations in the decameter radio band, the
                last almost unexplored radio window. We are also
                developing techniques to create sub-arcsecond resolution
                images of large regions of sky, which presents both
                calibration and computational challenges.