Hi, Rod, et al.! For decades, most of my work responsibilities were Optical Testing. Our (very large) group was even called "Test and Technology Center", serving commercial and government programs.
Mostly interferometry, radiometry, alignments, scattered light, baffling, coatings, mirror supports, materials, and field support of instrument operations.
Right around 1/20-wave, the design, build and calibration of the Test Sets DOMINATED the difficulty of the task. Even factory-fresh interferometers (Zygo, WYKO, etc.) were certified to "only" 1/20-wave. They (very reasonably) assumed that the user would either use as-is (with that uncertainty affecting knowledge of the reported test wavefront), OR that he would calibrate the test cavity...
The Later, highly-desirable option, meant either having NBS-traceable references (typically concave spherical mirrors and flats), or doing absolute-cal in-house... an extraordinarily laborious procedure, developed by one of our own seasoned scientists (my boss!) So, you go to the NBS heritage... and they reference my boss!
Consequently, when I see "interferometrically tested" and superb numbers... I can't help but wonder about the traceability of the equipment. The computer will dutifully spit out all kinds of PV, RMS, Strehl, Zernikes, energy within a circle, impulse response, more. But that is always the combo of the tested article (e.g. telescope mirror), AND interferometer, nulling optics, mounting, etc. Even with laborious "back-outs" of the test-set, the residual uncertainties can be quite significant.
Yet, most houses seem to just USE the interferometer, it they're lucky enough to have one, and report the output. If asked, they proudly say they use a ~Brand Name~ interferometer.
Enter the challenge of parsing mirrors A, B, C... At small fractional-wave shoot-outs, the test environment dominates. Yet, many/most suppliers just flatly/proudly state 1/20-wave, ~diffraction-limited~ etc.; I can't help but wonder.
Even Hubble was delivered as... the most perfect telescope ever made. Tom
29-inch Dob in a dome
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