The Usefulness and Limits of Coronagraphy in the Presence of Pinned Speckles
- 27 July 2004
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 612 (1) , L85-L88
- https://doi.org/10.1086/424381
Abstract
In this Letter we study the utility and limitations of ground-based coronagraphy with adaptive optics (AO). In very high AO correction regimes, residual speckles are pinned on the diffraction rings of the Airy pattern. We show that this effect is due to small errors in the complex wave in the focal plane, amplified by the coherent part of the wave. The statistics of these speckles are fairly well described by a modified Rician distribution. The variance of the speckles, at high flux and at photon-counting levels, finds simple expressions. The total variance can be partitioned into two contributions: one that can be suppressed by a coronagraph and one that cannot. Different regimes can be identified. These results enable us to analyze when a coronagraph can defeat the noise variance, and they provide a criterion for the effectiveness of such instruments.Keywords
This publication has 17 references indexed in Scilit:
- ForewordEAS Publications Series, 2004
- The Structure of High Strehl Ratio Point‐Spread FunctionsThe Astrophysical Journal, 2003
- Pupil densification of obstructed monolithic apertures for high-contrast coronagraphyEAS Publications Series, 2003
- Speckle Decorrelation and Dynamic Range in Speckle Noise–limited ImagingThe Astrophysical Journal, 2002
- Suppression of Speckle Noise by Speckle Pinning in Adaptive OpticsThe Astrophysical Journal, 2002
- Behavior of Remnant Speckles in an Adaptively Corrected Imaging SystemThe Astrophysical Journal, 2001
- Analysis of the technique of dark speckles for detection of exo-planetsJournal of Optics A: Pure and Applied Optics, 2000
- Photon statistics in partially compensated wave frontsJournal of the Optical Society of America A, 1999
- Speckle Noise and the Detection of Faint CompanionsPublications of the Astronomical Society of the Pacific, 1999
- The Telescope Point Spread FunctionPublications of the Astronomical Society of the Pacific, 1996