Adaptive Phase Mask Coronagraph with Amplitude and Phase Modulation for High Dynamic Range Synchronous Detection: APM2 Coronagraph

被引:0
|
作者
Bourget, P. [1 ]
Mawet, D. [1 ]
Mardones, P. [1 ]
Schuhler, N. [1 ]
Pueyo, L. [2 ]
Girard, J. [1 ]
Haguenauer, P. [1 ]
Gonte, F. [1 ]
机构
[1] European So Observ, 3107 Alonso de Cordova Vitacura, Santiago, Chili, Chile
[2] Space Telescope Sci Inst, Baltimore, MD 21218 USA
关键词
High-contrast imaging; coronagraphy; polarization; high angular resolution; phase mask; adaptive optics; synchronous detection;
D O I
10.1117/12.2026211
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a new Adaptive Phase Mask (APM) coronagraph design enabling Amplitude and Phase Modulation control (APM). The Adaptive Phase mask coronagraph is a technique proposed to provide both high dynamic and high angular resolution imaging of faint sources around bright objects. Discriminating faint sources from static speckles is a challenging problem. Our new system is based on synchronous demodulation that allows high dynamic range detection of a faint target immersed in a background. The APM(2) uses the coherence of speckles to discriminate them from proper companions, using the mask itself as the electric field modulator. Synchronous detection in the radio frequency range is used to side-step the effect of atmospheric turbulence and enable the detection of low amplitude signals. The APM2 concept offers high dynamic range detection and provides a time- and cost-effective method to quantify the probability of presence of a faint object close to the central star.
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页数:8
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