Paper
31 October 1996 Single-grid pair Fourier telescope for imaging the sky in hard x-rays and gamma rays
Author Affiliations +
Abstract
Fourier telescopes are an effective approach for providing images of hard x-ray and gamma-ray sources found in the sky. Sufficient coverage of the (u,v) plane is a requirement for effective imaging. Unfortunately, this requirement is diametrically opposed to the requirements to minimize instrument weight and cost which translate into minimizing the number of grids. This paper reports on a telescope design incorporating only one real and imaginary set of grid pairs which provides superior imaging performance at a significantly reduced cost.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jonathan W. Campbell "Single-grid pair Fourier telescope for imaging the sky in hard x-rays and gamma rays", Proc. SPIE 2808, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VII, (31 October 1996); https://doi.org/10.1117/12.256007
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KEYWORDS
Telescopes

Spatial frequencies

Hard x-rays

Space telescopes

Sensors

Photons

Gamma radiation

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