The Phase-Induced Amplitude Coronagraph (PIAA)

Olivier Guyon, Eugene A. Pluzhnik, Stephen T. Ridgway, Robert A. Woodruff, Celia Blain, Frantz Martinache, Raphael Galicher

Research output: Contribution to journalArticle

1 Scopus citations

Abstract

The Phase-Induced Amplitude Coronagraph (PIAAC) uses a lossless beam apodization, performed by aspheric mirrors, to produce a high contrast PSF. Thanks to the lossless apodization, this concept offers a unique combination of high theoretical throughput (≈100%), high angular resolution (λ/d), small inner working angle (≈1.5λ/d), low chromaticity and low sensitivity to pointing errors or angular star diameter. Together, these characteristics make the PRC an ideal choice for direct imaging of extrasolar terrestrial planets (ETPs) from space. We show that a visible telescope smaller than 4m would then achieve the goals of the TPF mission, while other coronagraphs considered for TPF require telescope diameters typically 2 to 3 times larger. On a large size (8m) space telescope, ETPs can be searched for around a significantly larger sample of stars, thus enabling a much higher scientific return.

Original languageEnglish (US)
Pages (from-to)385-391
Number of pages7
JournalProceedings of the International Astronomical Union
Volume1
Issue numberC200
DOIs
StatePublished - Jan 1 2005
Externally publishedYes

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Keywords

  • Planetary systems
  • Techniques: high angular resolution

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Cite this

Guyon, O., Pluzhnik, E. A., Ridgway, S. T., Woodruff, R. A., Blain, C., Martinache, F., & Galicher, R. (2005). The Phase-Induced Amplitude Coronagraph (PIAA). Proceedings of the International Astronomical Union, 1(C200), 385-391. https://doi.org/10.1017/S174392130600963X