Bit,
EXCELLENT.
Wide open, for an ideally perfect lens, is the best. This isn't due to diffraction as the article mentions, but is a result of a simple thing called Dawes Law. It states that the larger the optic, all things being equal, the better the angular resolution. In other words, the larger diameter of the optic, the more you'll resolve. That's why the largest observatories are still going for bigger and bigger mirrors. If the Hubble space telescope used a mirror as large as the earth based ones, you'll see a tremendous, tremendous difference.
If you ever look through a small scope, say a 4 inch diameter at a tight cluster, it'll look like a small fuzzy cloud. But if you were to take a 8 inch diameter scope at the same object, you'll realize that the fuzzy cloud is actually about a million stars all clustered up together. Larger diameter for better resolution, all things being equal.
Stopping down to f/8 or two stops from max....here's what's going on. At f/8, it appears sharper, but there is a loss in resolution. You're gaining depth of field and apparent sharpness, but you're losing resolution since the virtual diameter of the lens is smaller. At two stops from max, since we're using a "practical" optics (commercially available camera lens), we're just using the "good" part of the lens. If the lens was made to a critically high precision with a perfect figure, then you would have the best performance wide open. Very very few lenses do this. High end t-scope optics, however, DO do this. Going from a 4 inch diameter to a 6 inch diameter yields highly noticable results.
Also, even with the highest available technology and glass, the fastest the t-scope guys can make a lens with a 4 inch diameter, with all the tricks thrown in and be nearly nearly perfect in color correction is f/5. Any faster and you WILL see CA. With a 5 inch, it's f/6. With a 6 inch, f/7. 7 inch, f/7. 8 inch, f/8. There's only so much that you can do while bending light.
Surprising answer?
Percy