Jets from supermassive black holes change over time, but existing imaging methods have had difficulty resolving that variability at high resolution. The new method represents the observations as a video and learns how the source changes across time while processing observations from different dates together.

The researchers demonstrated the approach using multi-epoch observations of the blazar 3C 345 made with the Very Long Baseline Array, a network of radio telescopes. They report improved resolution and dynamic range compared with traditional methods, allowing them to estimate the plasma's local, instantaneous velocity in the jet.