Paper
9 July 2018 Simulation and experimental study on the detection of binary stars with non-redundant aperture masking
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Abstract
The non-redundant aperture masking techniques transforms telescope into a Fizeau interferometer by a simple action of placing an aperture mask over the pupil, the limited resolution set by atmospheric fluctuations can be overcome by closure phase techniques to obtain diffraction-limited images. For binary stars, the closure phases can not only eliminate the influence of atmospheric fluctuations on ground-based optical telescope, but also have a functional relationship with contrast and angular separation of binary stars. In this paper, basing on the mathematical model of non-redundant aperture masking detecting binary stars, we carry out the computer simulation and laboratory experiment by using the Golay-6 mask.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yanqiang Wang, Zhen Wu, Qian Li, Teng Xu, Mingming Xu, Huatao Zhang, and Yonghui Hou "Simulation and experimental study on the detection of binary stars with non-redundant aperture masking", Proc. SPIE 10701, Optical and Infrared Interferometry and Imaging VI, 1070127 (9 July 2018); https://doi.org/10.1117/12.2311604
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Cited by 1 scholarly publication.
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KEYWORDS
Stars

Point spread functions

Data processing

Atmospheric optics

Telescopes

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