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Rudrani Kar Chowdhury
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Welcome to my homepage

I am a postdoctoral fellow at The University of Hong Kong. I completed my doctoral studies from Presidency University, India. My research focuses on the massive black hole activity onto their surrounding gas, stars and large scale properties of host galaxies. environment using semi-analytical models and cosmological simulations. I employ semi-analytical models and cosmological simulations to explore these complex interactions and to better understand galaxy evolution and the role of black holes within their cosmic environments

My contribution to the field

Feedback from Active Galactic Nuclei

I am interested in investigating the nature and impact of active supermassive black holes on their host galaxy properties through AGN feedback. For more details, click 
here

Synthetic X-ray Observation Pipeline

I have developed a synthetic Chandra observation pipeline starting from post-processed cosmological simulation data and detailed model of diffuse  X-ray emission from galaxy groups and clusters. For more information, click
here

Tidal Disruption Event of First Stars

For the first time, we have proposed a unique method to observe the elusive first stars of the universe, by looking at their tidal disruption event signatures with JWST and upcoming Roman telescope. For more details, click  
here
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