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Stellar Coronograph with Phase Mask

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Roddier, F., Roddier, C.·1997·Publications of the Astronomical Society of the Pacific

Abstract

The detection of faint light sources very close to a bright star is primarily limited by light scattered by the Earth's atmosphere. This source of scattered light can now be reduced by means of adaptive optics, or totally eliminated by using a telescope in space. Then diffraction by the telescope aperture becomes the primary source of scattered light. Whereas a classical Lyot coronograph can reduce the amount of light diffracted away from the star, it becomes inefficient very close to the star. Instead of forming the stellar image on an opaque mask, it is proposed here to use a small phase plate which produces a 180 degrees phase shift on the core of the stellar image. Light diffracted outside the core is then eliminated by destructive interference. Applied to the Hubble Space Telescope, the technique would easily allow detection of a stellar companion 0.3" away from a star and at least 8 magnitude fainter.

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Metadata

Authors
Roddier, F., & Roddier, C.
Venue
Publications of the Astronomical Society of the Pacific
Published
1997-07
Volume
109
Pages
815
ISSN
  • 0004-6280 (ISSN-L)
  • 1538-3873
OpenAlex
W2020245669
Cited by
239
References
0
FWCI
2.51
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Stellar Coronograph with Phase Mask. https://app.cochat.ai/papers/10.1086/133949
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Roddier, F., & Roddier, C. (1997). Stellar Coronograph with Phase Mask. Publications of the Astronomical Society of the Pacific. https://doi.org/10.1086/133949

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