27 November 2017 Optical design of the WFIRST Phase-A Wide Field Instrument
Author Affiliations +
Proceedings Volume 10590, International Optical Design Conference 2017; 105901Q (2017) https://doi.org/10.1117/12.2300295
Event: International Optical Design Conference - IODC 2017, 2017, Denver, United States
The WFIRST Wide-Field Infrared Survey Telescope TMA optical design provides 0.28-sq° FOV at 0.11” pixel scale to the Wide Field Instrument, operating between 0.48-2.0μm, including a spectrograph mode (1.0-2.0μm.) An Integral Field Channel provides 2-D discrete spectroscopy at 0.15” and 0.3” sampling from 0.42-2.0μm.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bert A. Pasquale, Bert A. Pasquale, Catherine T. Marx, Catherine T. Marx, Guangjun Gao, Guangjun Gao, Nerses Armani, Nerses Armani, Thomas Casey, Thomas Casey, "Optical design of the WFIRST Phase-A Wide Field Instrument", Proc. SPIE 10590, International Optical Design Conference 2017, 105901Q (27 November 2017); doi: 10.1117/12.2300295; https://doi.org/10.1117/12.2300295


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