"Somewhere, something incredible is waiting to be known | क्वचित् किमपि अद्भुतं ज्ञातुं प्रतीक्षते |کہیں، کوئی نایاب شے پائے جانے کے انتظار میں ہے۔ " - Carl Sagan
I am a Senior AI Engineer at Temus, with a PhD in Astrophysics and a strong background in data-driven science and machine learning methods. Previously, I was a full-time researcher at Harvard & Smithsonian and a postdoctoral fellow at the University of New South Wales, Australia. I completed my PhD at the Center for Astrophysics and Supercomputing, Swinburne University of Technology, Australia, and hold an integrated Bachelor's and Master's degree in Engineering Physics from IIT (BHU) Varanasi, India.
My work spans AI/ML, Data Science, and Astrophysics, with experience taking data-driven solutions from research and experimentation to production. At Temus, I work on enterprise AI, including RAG-based systems, scalable data pipelines, foundation models, and production-grade AI/ML solutions across cloud platforms, including AWS and Azure. I have also applied AI and machine learning to high-dimensional genomic data and developed risk-scoring algorithms for cybersecurity.
My research experience has been largely observation- and data-driven, focusing on supermassive black holes, galaxy evolution, gravitational lensing, and cosmology. As part of the Astro 3D Galaxy Evolution with Lenses (AGEL) collaboration, I led projects applying advanced data analysis and physics-based modeling to astronomical datasets, using gravitational lenses to study galaxy evolution and test cosmological theories.
News
Spoke at Nasopharyngeal Carcinoma Singapore Symposium (NPCSS), "From Sequence to Signal: Using AI for Genomic Pattern Discovery". Link
Spoke at AstroAI Workshop 2025, "Gravitational Lensing and the Need for AI-Accelerated Lens Modeling". Link
Spoke to ABC News about India's role in the Axiom 4 Space Mission. Link
Sahu et al. 2024 ApJ, 970, 86
"Cosmography with the Double Source Plane Strong Gravitational Lens AGEL150745+052256"
Sahu et al. 2025, ApJ, 991, 72
Gravitational Lensing
Gravitational lensing is the deflection of light coming from a background source by a foreground mass concentration along the same line of sight. As a result, multiple distorted and magnified images of the background source are formed. Strong lensing, where multiple images of the background source are formed, is caused by massive objects such as galaxies or clusters with a radially varying (differential) mass distribution. I use gravitational lenses to study galaxy evolution models and cosmology. See Sahu et al. (2024), Sahu et al. (2025)
Co-evolution of Black Holes and Host Galaxies