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24 September 2004 New improvements in reflecting-absorbing coatings for astronomy
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More and more complex telescopes and astronomical instruments require: (1) Mechanics with low diffusion/reflection properties in order to decrease the level of scattered light, especially for use in infrared. (2) Mirrors with high reflectivities, in order to improve the level of useful light and/or extend the useful spectrum, especially to the near UV(320 nm - 400 nm), SESO will present simultaneously here some results of its current developments concerning: (1) Solutions to increase the signal/noise ratio for systems operating in the infrared and needing a cryogenic cryostat assembly for the detection system, (2) A high efficiency reflective UV-coating.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Denis Fappani "New improvements in reflecting-absorbing coatings for astronomy", Proc. SPIE 5494, Optical Fabrication, Metrology, and Material Advancements for Telescopes, (24 September 2004);

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