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13 September 2012 Manufacturing and testing of a convex aspherical mirror for ASSIST
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ASSIST is the testbed for the ESO Adaptive Optics Facility. The main objective of ASSIST is the characterization of the 1.2 meter deformable mirror which will replace the existing secondary of one of the 8 meter VLT telescopes. A large concave 1.65 meter diameter aspherical primary mirror combined with a 140 mm diameter convex aspherical secondary forms the main optical system of ASSIST. Two additional optical units provide the light sources and the wave front analyzing optics. Without having the possibility for checking the entire optical system as a whole, each individual mirror had to be manufactured and tested using reliable techniques. The secondary mirror for ASSIST (AM2) is made of an optically transparent material (BK7) with a specific and accurate backside radius in order to achieve a null test in transmission. Furthermore, not only the overall RMS surface error of AM2 is important, but due to the fact that it will be used in a setup that measures specific spatial frequencies, also the spatial frequencies of the surface error of AM2 is important. The aspherical surface is tested in double pass using an optical flat and an interferometer with a transmission sphere. Manufacturing of this asphere is mainly done by hand at the optical lab of NOVA-ASTRON. The final accuracy of the reflecting surface is within the required 50 nm RMS with a surface roughness of less than 2 nm RMS. This paper reports in more detail on manufacturing and testing of the a-spherical convex mirror.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rik ter Horst and Remko Stuik "Manufacturing and testing of a convex aspherical mirror for ASSIST", Proc. SPIE 8450, Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II, 84504X (13 September 2012);


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