28 July 2000 Holographic telescope design for narrowband imaging in the far ultraviolet
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We report on the status of a novel imaging spectrometer design based on aberration-corrected holographic gratings. The goal of the work is to develop optical designs with high spatial resolution and high sensitivity over a narrow wavelength bandpass, thus effectively creating a narrow-band imaging capability. Ideally the narrow-band capability can be used to observe astrophysical phenomena at key diagnostic lines short-ward the short-wavelength transmission cut-off of lithium fluoride (1050 angstroms) while simultaneously controlling the intense geocoronal Lyman alpha emission at 1216 angstroms. For example OVI 1032, 1038 angstroms emission from a fast shock can be observed with arc-second resolution over a 5 arc-minute field of view.
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Erik Wilkinson, Erik Wilkinson, Remy Indebetouw, Remy Indebetouw, } "Holographic telescope design for narrowband imaging in the far ultraviolet", Proc. SPIE 4013, UV, Optical, and IR Space Telescopes and Instruments, (28 July 2000); doi: 10.1117/12.394025; https://doi.org/10.1117/12.394025

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