Poster + Paper
18 July 2024 Optical performance prediction of the AMASE-P system
Author Affiliations +
Conference Poster
Abstract
The AMASE-P project presents a bold exploration into the potential utilization of state-of-the-art commercial photographic lenses and CMOS detectors as integral components in spectrograph designs, thereby offering a cost-effective solution for astronomy instrumentation. In this contribution, we present the current optical design of the telescope and spectrograph system, and present the expected performance of the design, including the point spread function, spectral resolution, throughput, and signal-to-noise ratios. We also present the design of a telecentric corrector for the Canon 400mm f/2.8 III telephoto lens, which is necessary for coupling it to optical fibers.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Yiuhung Cheung, Chit-Ho Hui, Renbin Yan, Matthew A. Bershady, Sabyasachi Chattopadhyay, Man-Yin Leo Lee, Ziming Peng, Michael P. Smith, Yiwei Liu, and Egan Loubser "Optical performance prediction of the AMASE-P system", Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 130969Z (18 July 2024); https://doi.org/10.1117/12.3019778
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KEYWORDS
Signal to noise ratio

Spectrographs

Point spread functions

Spectral resolution

Telescopes

Diffraction gratings

Image analysis

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