Aperture masking interferometry research simulation

Haitao Wang; Qiufeng Luo; Weijun Fan; Xian Ling Zhang; ChunKan Tao; Yongtian Zhu; Bifang Zhou; Hanliang Chen

doi:10.1117/12.550301

20 October 2004 Aperture masking interferometry research simulation

Haitao Wang, Qiufeng Luo, Weijun Fan, Xian Ling Zhang, ChunKan Tao, Yongtian Zhu, Bifang Zhou, Hanliang Chen

Proceedings Volume 5491, New Frontiers in Stellar Interferometry; (2004) https://doi.org/10.1117/12.550301
Event: SPIE Astronomical Telescopes + Instrumentation, 2004, Glasgow, United Kingdom

Abstract

Aperture Masking Interferometry (AMI) is one of the high-resolution astronomical image observation technologies. It is also an important research way to the Optical Aperture Synthesis (OAS). The theory of OAS is simply introduced and AMI simulation method is raised. The mathematics model is built and the interferogram fringes are got. The aperture mask u-v coverage is discussed and one image reconstruction method is done. The reconstructed image result is got with CLEAN method. Shortcoming of this work is also referred and the future research work is mentioned at last.

Citation Download Citation

Haitao Wang, Qiufeng Luo, Weijun Fan, Xian Ling Zhang, ChunKan Tao, Yongtian Zhu, Bifang Zhou, and Hanliang Chen "Aperture masking interferometry research simulation", Proc. SPIE 5491, New Frontiers in Stellar Interferometry, (20 October 2004); https://doi.org/10.1117/12.550301

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