Ph.D. in Physics (Astronomy & Astrophysics)
Very high energy (VHE) γ-ray astrophysicist with extensive experience in stereo Imaging Atmospheric Cherenkov Telescope (VERITAS) observations. Researching time-domain variability, broadband spectral modeling, and non-thermal emission from blazars, AGN, and relativistic jets using GammaPy and multiwavelength data from Fermi-LAT, Swift, XMM-Newton, and NuSTAR.
About
Very high energy (VHE) γ-ray astrophysics with the VERITAS stereo IACT array, focused on time-domain variability, broadband spectral modeling, and non-thermal emission from AGN, relativistic jets, and TeV blazars. Studies particle acceleration and transient phenomena in these sources.
End-to-end VHE data analysis with GammaPy — from event-level data to spectral and spatial likelihood modeling — including joint fits combining VERITAS, MAGIC, and LST-1 with Fermi-LAT, X-ray, and optical data. Cross-validated against the collaboration-level VEGAS pipeline.
Visiting Researcher with Prof. Luis C. Ho at the Kavli Institute for Astronomy and Astrophysics (KIAA), Peking University, Beijing, China (since June 2026). Previously a Postdoctoral Research Associate with Prof. Qi Feng on the VERITAS collaboration at the University of Utah (2024–2026), and held postdoctoral fellowships at the Center for Theoretical Physics PAS (Warsaw), the Indian Institute of Astrophysics (IIA, Bengaluru), and ARIES (Nainital). Ph.D. in Physics (Astronomy & Astrophysics) on multi-wavelength studies of TeV blazars, ARIES / DDU Gorakhpur University, India (2019).
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Kavli Institute for Astronomy and Astrophysics (KIAA)
Peking
University
Beijing, China