Poster + Paper
13 December 2020 A white light collimator for Plato camera integration support
Author Affiliations +
Conference Poster
Abstract
A fiber fed, wide beam collimator was developed as a tool to support the Assembly, Integration and Verification (AIV) tasks associated to the integration of the ESA-PLATO telescope unit (TOU) to the focal plane, for the 26 cameras that are going to be assembled at the Centre Spatial de Liége (CSL). This collimator will work as source for the alignment process at ambient temperature, providing a white light beam that must comply with a series of critical requirements, namely high spatial uniformity over an clear aperture of 150 mm (better than 85%), Wavefront Error associated to focus aberration at the level of λ/30 rms and high flux stability over time (2% in 24h). This paper will present the steps taken towards the development, manufacture and integration of this collimator, as well as the tests devised to evaluate requirements compliance.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Manuel Abreu, David Castro Alves, Alexandre Cabral, João M.P. Coelho, Pedro Santos, L. Clermont, Ann Baeke, and B. Vandenbussche "A white light collimator for Plato camera integration support", Proc. SPIE 11443, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave, 114434T (13 December 2020); https://doi.org/10.1117/12.2561402
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KEYWORDS
Collimators

Cameras

Light

Manufacturing

Telescopes

Wavefronts

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