Presentation + Paper
9 September 2019 Testing the near-infrared optical assembly of the space telescope Euclid
Christof Bodendorf, Norbert Geis, Frank Grupp, Jennifer Kaminski, Reinhard Katterloher, Ralf Bender
Author Affiliations +
Abstract
Euclid is a space telescope currently developed in the framework of the ESA Cosmic Vision 2015-2025 Program. It addresses fundamental cosmological questions related to dark matter and dark energy. The lens system of one of the two scientific key instruments [a combined near-infrared spectrometer and photometer (NISP)] was designed, built-up and tested at the Max Planck Institute for Extraterrestrial Physics (MPE). We present the final imaging quality of this diffraction-limited optical assembly with two complementary approaches, namely a point-spread function- and a Shack- Hartmann sensor-based wavefront measurement. The tests are performed under space operating conditions within a cryostat. The large field of view of Euclid’s wide-angle objective is sampled with a pivot arm, carrying a measurement telescope and the sensors. A sequence of highly accurate movements to several field positions is carried out by a large computer controlled hexapod. Both measurement approaches are compared among one another and with the corresponding simulations. They demonstrate in good agreement a solely diffraction limited optical performance over the entire field of view.
Conference Presentation
© (2019) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christof Bodendorf, Norbert Geis, Frank Grupp, Jennifer Kaminski, Reinhard Katterloher, and Ralf Bender "Testing the near-infrared optical assembly of the space telescope Euclid", Proc. SPIE 11116, Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems II, 111160Y (9 September 2019); https://doi.org/10.1117/12.2529114
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KEYWORDS
Point spread functions

Cameras

Wavefronts

Sensors

Telescopes

Optical testing

Diffraction

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