An active coronagraph using a liquid crystal array for exoplanet imaging: principle and testing

Author(s): Xi Zhang, De-Qing Ren, Yong-Tian Zhu and Jiang-Pei Dou.


“High-contrast imaging coronagraphs, used for the detection of exoplanets, have always adopted passive coronagraph optical components. It is therefore impossible to actively optimize the coronagraphs to achieve their best performance. To solve this problem, we propose a novel high-contrast imaging coronagraph which combines a liquid crystal array (LCA) for active pupil apodization and a deformable mirror (DM) for phase correction. The LCA we use is an amplitude-only spatial light modulator. The LCA is well calibrated and compensates for its amplitude non-uniformity and nonlinear intensity responsivity. We measured the imaging contrasts of the coronagraph system with the LCA only and without the DM deployed. Imaging contrasts of 10-4 and 10-5 can be reached at an inner working angular distance of 2.5 and 5λ/D, respectively. A simulation shows that the phase errors on the coronagraph pupil limit the contrast performance. The contrast could be further improved if a DM is deployed to correct the phase errors induced by the LCA and coronagraph optics.”

Link to Publications Page

Publication: Research in Astronomy and Astrophysics, (subscription required)

Issue/Year/DOI: Res. Astron. Astrophys., Vol. 12, Issue 5,(2012)

This entry was posted on Tuesday, May 1st, 2012 and is filed under All, LC-R 1080, Spatial Light Modulators. You can follow any responses to this entry through the RSS 2.0 feed. Both comments and pings are currently closed.

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