Paper
12 October 2004 Coronagraph contrast demonstrations with the high-contrast imaging testbed
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Abstract
Predictions of contrast performance for the Eclipse coronagraphic telescope are based on computational models that are tested and validated with laboratory experience. We review recent laboratory work in the key technology areas for an actively-corrected space telescope designed for extremely high contrast imaging of nearby planetary systems. These include apodized coronagraphic masks, precision deformable mirrors, and coronagraphic algorithms for wavefront sensing and correction, as integrated in the high contrast imaging testbed at JPL. Future work will focus on requirements for the Terrestrial Planet Finder coronagraph mission.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
John T. Trauger, Chris Burrows, Brian Gordon, Joseph Jacob Green, Andrew E. Lowman, Dwight Moody, Albert F. Niessner, Fang Shi, and Daniel Wilson "Coronagraph contrast demonstrations with the high-contrast imaging testbed", Proc. SPIE 5487, Optical, Infrared, and Millimeter Space Telescopes, (12 October 2004); https://doi.org/10.1117/12.552520
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Cited by 53 scholarly publications.
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KEYWORDS
Coronagraphy

Space telescopes

Photomasks

Wavefronts

Mirrors

Stars

Deformable mirrors

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