2018, Bauer, Jens, Ulitschka, Melanie, Pietag, Fred, Arnold, Thomas

Aluminum mirrors offer great potential for satisfying the increasing demand in high-performance optical components for visible and ultraviolet applications. Ion beam figuring is an established finishing technology and in particular a promising technique for direct aluminum figure error correction. For the machining of strongly curved or arbitrarily shaped surfaces as well as the correction of low-to-mid spatial frequency figure errors, the usage of a high-performance ion beam source with low tool width is mandatory. For that reason, two different concepts of ion beam generation with high ion current density and narrow beam width are discussed. (1) A concave ion beam extraction grid system is used for apertureless constriction of ion beams in the low millimeter range. An oxygen ion beam with a full-width at half-maximum (FWHM) of 4.0 mm with an ion current density of 29.8  mA  /  cm2 was achieved. (2) For even smaller ion beams, a conic aperture design with a submillimeter-sized exit opening was tested. A nitrogen ion beam with an FWHM down to 0.62 mm with an ion current density of 4.6  mA  /  cm2 was obtained. In situ ion current density mapping is performed by scanning Faraday probe measurements. Special interest is set on the data evaluation for submillimeter ion beam analysis.

2017, Schubert, Matthias, Kentischer, Thomas, von der Lühe, Oskar

Journal of astronomical telescopes, instruments, and systems : JATIS 3 (2017), Nr. 04

2015, Swift, Jonathan J., Bottom, Michael, Johnson, John A., Wright, Jason T., McCrady, Nate, Wittenmyer, Robert A., Plavchan, Peter, Riddle, Reed, Muirhead, Philip S., Herzig, Erich, Myles, Justin, Blake, Cullen H., Eastman, Jason, Beatty, Thomas G., Barnes, Stuart I., Gibson, Steven R., Lin, Brian, Zhao, Ming, Gardner, Paul, Falco, Emilio, Criswell, Stephen, Nava, Chantanelle, Robinson, Connor, Sliski, David H., Hedrick, Richard, Ivarsen, Kevin, Hjelstrom, Annie, de Vera, Jon, Szentgyorgyi, Andrew

The Miniature Exoplanet Radial Velocity Array (MINERVA) is a U.S.-based observational facility dedicated to the discovery and characterization of exoplanets around a nearby sample of bright stars. MINERVA employs a robotic array of four 0.7-m telescopes outfitted for both high-resolution spectroscopy and photometry, and is designed for completely autonomous operation. The primary science program is a dedicated radial velocity survey and the secondary science objective is to obtain high-precision transit light curves. The modular design of the facility and the flexibility of our hardware allows for both science programs to be pursued simultaneously, while the robotic control software provides a robust and efficient means to carry out nightly observations. We describe the design of MINERVA, including major hardware components, software, and science goals. The telescopes and photometry cameras are characterized at our test facility on the Caltech campus in Pasadena, California, and their on-sky performance is validated. The design and simulated performance of the spectrograph is briefly discussed as we await its completion. New observations from our test facility demonstrate sub-mmag photometric precision of one of our radial velocity survey targets, and we present new transit observations and fits of WASP-52b—a known hot-Jupiter with an inflated radius and misaligned orbit. The process of relocating the MINERVA hardware to its final destination at the Fred Lawrence Whipple Observatory in southern Arizona has begun, and science operations are expected to commence in 2015.