The CARTA system is a tool for visualising and anaylsing large-scale astronomical imagery. As the volume of data produced from modern radio telescopy continues to increase rapidly, a robust and scalable architectural solution is required to perform these computations in near real-time. We investigate a data flow model as this solution.

Videos



Visit the video on YouTube to like and join the discussion in the comment section.

Images



The CARTA Interface

CARTA use cases

General data flow diagram

Component diagram

Performance testing results

A Dask task graph