The Vera Rubin Observatory will soon begin operations.
The largest digital camera ever built will be used to regularly scan the entire sky.
I imagine this could result in the discovery of vast numbers of new variable stars, as well as improved light curves for already known ones.
Are there any plans or discussions within AAVSO/VSX regarding:
How the variable star data might be incorporated into the VSX?
Whether Rubin data will lead to automatic submissions?