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
- A Makeover for M87: Machine-learning technique provides a clearer look at the supermassive black hole April 13, 2023
- New PIRE Webinar on Composable Architecture March 15, 2023
- New Webinar: Performing Large Scale Parameter Surveys with OSG Services September 12, 2022
- How We Get a Picture of a Black Hole – UArizona Black Hole Team August 17, 2022
- Horizon Scale Physics Around Sagittarious A* May 13, 2022
- New Immersive Fly-through Experience May 12, 2022
- From the Possibility to the Certainty of a Supermassive Black Hole March 29, 2022
- A View of Sagittarius A* Across the Radio Band February 8, 2022
BH PIRE research and education are conducted with major support from the National Science Foundation under Grant No. 1743747.