The project aims to characterize the images of black holes using image-domain feature extraction of the black holes shadow parameters. In short, we want to be able to use the observed accretion flow, or photon ring, around the black hole as a proxy for the size of the black hole. This project lies within the area of astronomy and astrophysics.
Recent News
- Advanced EHT Data Analysis: Time Domain Methods II, Session 2 February 16, 2021
- Now Available: CASPER Workshop and BH PIRE DSP School 2019 Presentations February 4, 2021
- Advanced EHT Data Analysis: Time Domain Methods I, Session 1 January 19, 2021
- Leading Astrophysicist Receives Swinburne Lifetime Achievement Award December 9, 2020
- Astrophysics Empowered by the EHT: Kerr Black Holes and Beyond, Session 5 November 25, 2020
- EVOLUTION: The Genius Equation November 23, 2020
- Astrophysics Empowered by the EHT: Subgrid Plasma Physics, Session 4 November 11, 2020
- Astrophysics Empowered by the EHT: GRMHD Simulations, Session 2 October 30, 2020