This would certainly speed up the rate of discovery from the images and get more people interested in astronomy.

Inside the project there must be an established data infrastructure running or ready to run. It probably has a raw layer and a transformed layer with well defined tabular schemas for the metadata of each image. It would be fun to see how both layers work and play around with the data.

Would the instrument itself have a fixed set of metadata attributes assigned to all imaging, or is it programmable and changeable during the service life?