27 November 2017 Optical design of the WFIRST Phase-A Wide Field Instrument
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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
Abstract
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, Catherine T. Marx, Guangjun Gao, Nerses Armani, 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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