2018
DOI: 10.1364/ao.57.002736
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Wide-band white light sparse-aperture Fizeau imaging interferometer testbed for a distributed small-satellites constellation

Abstract: Under the background of astronomical observation by a distributed small-satellites constellation, a Fizeau imaging interferometer testbed (FIIT) was designed and constructed at National Astronomical Observatories of the Chinese Academy of Sciences in the past four years that achieved wide-band white light (400-700 nm) phased imaging at laboratory with a field of view (FOV) ∼2  arcmin. This study presents the design of FIIT, which is mainly composed of a light source module for simulating infinite objects, thre… Show more

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Cited by 13 publications
(1 citation statement)
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“…The side view of the light path structure and the three-dimensional model (in CATIA software) are shown in Figure 1a,b, respectively. The system is divided into three main structural modules, namely the subaperture system, the beam steering and adjustment structure, and the synthetic imaging system [12]. The fast steering mirror (FSM) is the core component of the beam steering and adjustment structure.…”
Section: Structure and The Optical Path Of The Golay3 Systemmentioning
confidence: 99%
“…The side view of the light path structure and the three-dimensional model (in CATIA software) are shown in Figure 1a,b, respectively. The system is divided into three main structural modules, namely the subaperture system, the beam steering and adjustment structure, and the synthetic imaging system [12]. The fast steering mirror (FSM) is the core component of the beam steering and adjustment structure.…”
Section: Structure and The Optical Path Of The Golay3 Systemmentioning
confidence: 99%