Bhagya Subrayan
Physics and Astronomy · Purdue University West Lafayette
Publications
64
Citations
260
Est. group size
~5
Recurring co-author estimate
Active years
7
Publishing since 2020
Bhagya Subrayan studies exploding stars (supernovae) and related transient phenomena, focusing on how these stellar explosions interact with surrounding material shed by the star before it died. This work combines observations across multiple wavelengths (X-ray, infrared, radio, ultraviolet) and telescopes, including the Hubble Space Telescope, to understand the properties of supernova progenitor stars and the environments they explode into.
Publication output has grown substantially over the last decade, rising from no recorded output before 2020 to a sharp increase in 2023-2026, with the most recent year showing the highest volume.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- The fate of the failed supernova candidate M31-2014-DS1
Monthly Notices of the Royal Astronomical Society · 2026
- SN 2024abfl: A Flat-plateau, Low-luminosity Type IIP Supernova with Early Circumstellar Matter Interaction
The Astrophysical Journal · 2026
- SN 2024iss: A double-peaked Type IIb supernova with evidence of circumstellar interaction
Astronomy and Astrophysics · 2026
- Late-time Hubble Space Telescope Ultraviolet Spectra of SN 2023ixf and SN 2024ggi Show Ongoing Interaction with Circumstellar Material
The Astrophysical Journal · 2026
- The Double-Peaked Calcium-Strong SN 2025coe: Progenitor Constraints from Early Interaction and Ejecta Asymmetries
arXiv (Cornell University) · 2026
- SN 2024abfl: A Flat-Plateau, Low-Luminosity Type IIP Supernova with Early CSM Interaction
arXiv (Cornell University) · 2026
- SN 2024abfl: A Flat-Plateau, Low-Luminosity Type IIP Supernova with Early CSM Interaction
arXiv (Cornell University) · 2026
- The Double-Peaked Calcium-Strong SN 2025coe: Progenitor Constraints from Early Interaction and Ejecta Asymmetries
arXiv (Cornell University) · 2026
- The fate of the failed supernova candidate M31-2014-DS1
arXiv (Cornell University) · 2026
- The fate of the failed supernova candidate M31-2014-DS1
arXiv (Cornell University) · 2026
- SN 2023zcu: A Type IIP SN with Early Flash Features
arXiv (Cornell University) · 2026
- SN 2023zcu: A Type IIP SN with Early Flash Features
arXiv (Cornell University) · 2026
- A multiwavelength view of the nearby Calcium-Strong Transient SN 2025coe in the X-Ray, Near-Infrared, and Radio Wavebands
Open MIND · 2026
- A multiwavelength view of the nearby Calcium-Strong Transient SN 2025coe in the X-Ray, Near-Infrared, and Radio Wavebands
arXiv (Cornell University) · 2026
- An infrared echo from a circumstellar disk in the hydrogen- and helium-poor SN 2024aecx
Open MIND · 2026
- arXiv (Cornell University)×30
- The Astrophysical Journal×14
- The Astrophysical Journal Letters×4
- Transient Name Server AstroNote×4
- Monthly Notices of the Royal Astronomical Society×2
- Braden Garretson
Physics and Astronomy · Purdue University West Lafayette
- S. Bose
Physics and Astronomy · The Ohio State University
- Danny Milisavljevic
Physics and Astronomy · Purdue University West Lafayette
- A. B. Davis
Physics and Astronomy · The Ohio State University
- K. Z. Stanek
Physics and Astronomy · The Ohio State University
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 20, 2026.
Claim or correct this profile