Presentation + Paper
13 December 2020 RAFTER: Ring Astrometric Field Telescope for Exo-planets and Relativity
Alberto Riva, Mario Gai, Alberto Vecchiato, Deborah Busonero, Mario Glilberto Lattanzi, Federico Landini, Zhaoxiang Qi, Zhenghong Tang
Author Affiliations +
Abstract
High precision astrometry aims at source position determination to a very small fraction of the diffraction image size, in high SNR regime. One of the key limitations to such goal is the optical response variation of the telescope over a sizeable FOV, required to ensure that bright reference objects to any selected target. The issue translates into severe calibration constraints, and/or the need for complex telescope and focal plane metrology. We propose an innovative system approach derived from the established TMA telescope concept, extended to achieve high filling factor of an annular field of view around the optical axis of the telescope. The proposed design is a very compact, 1 m class telescope compatible with modern CCD and CMOS detectors (EFL = 15 m). We describe the concept implementation guidelines and the optical performance of the current optical design. The diffraction limited FOV exceeds 1.25 square degrees, and the detector occupies the best 0.25 square degree with 66 devices.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alberto Riva, Mario Gai, Alberto Vecchiato, Deborah Busonero, Mario Glilberto Lattanzi, Federico Landini, Zhaoxiang Qi, and Zhenghong Tang "RAFTER: Ring Astrometric Field Telescope for Exo-planets and Relativity", Proc. SPIE 11443, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave, 114430P (13 December 2020); https://doi.org/10.1117/12.2576806
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Cited by 1 scholarly publication.
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