What is it about
As the human race continues its quest to unveil the grandeur of the Universe, answers to several fundamental questions about the evolution of galaxies and the formation of stars in them remain elusive. As a cosmic detective, Professor Choudhury proactively hunts for answers by studying galaxies in our nearby Universe, i.e., those near the Milky Way and our local neighbourhood. These grand structures and celestial bodies near us are simply fossil records of the various physical processes involved in their formation and evolution events since the early phases of the Universe. Professor Choudhury is particularly interested in star-forming dwarf galaxies, whose chemical and physical environments are vital proxies of star formation and galaxy evolution events in the nascent phase of the Universe. To carry out these studies, he uses multiwavelength data from Big Sky Surveys and targeted observations from prominent space-based telescopes (e.g. India's AstroSat, NASA's Hubble Telescope) and ground-based optical telescopes worldwide. He employs image analysis techniques, mathematical and statistical techniques, and algorithms to analyse these data and uses physical models to interpret the associated astrophysical phenomena involved in the above processes. He has published several articles in the above domains in international journals of Astronomy and Astrophysics. Professor Choudhury leads his research projects in collaboration with some prolific research groups based in India, the USA, Australia, and South Korea.
Exciting results
By developing smart, robust, and versatile data analysis techniques, he has deciphered some of the global properties, like chemical enrichment maps and cluster formation history, of the most massive satellite galaxies of our Milky Way, the Magellanic Clouds. Estimating these properties is crucial in understanding the secular evolution of these satellites and their gravitational interaction history with the Milky Way. The results have implications on our understanding of star formation history, mass accumulation, and interaction history of similar systems in our Universe (minor galaxy merger events).
The Astronomy & Astrophysics Group
Professor Choudhury is establishing an Astronomy & Astrophysics research group at Ahmedabad University. Currently, two potential PhD Physics scholars, a Project Associate, an Undergraduate thesis student, and many other undergraduate students from various disciplines (physics, mechanical engineering, and computer science and engineering) are working with the research group. The group would focus on cutting-edge research in the aforementioned areas, involving observations and data analysis in the multiwavelength regimes, simulations/modelling, and developing new data analysis techniques/pipelines. The current science aims of the group are in synergy with the decadal missions of the international astronomy community and relevant in the era of Big Sky Surveys and next-generation space telescopes by ISRO, NASA and ESA. Professor Choudhury is interested in collaborating and applying interdisciplinary areas (e.g. big data analysis, image processing, high-performance computation) to science problems in Astronomy.
He is also setting up an Astronomy & Astrophysics teaching laboratory that would be used to provide hands-on experience to students on observations and data analysis. As an initial step, a pyramidal horn antenna for 21cm astronomy has been recently set up at the University, and more such facilities are under plan.