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20042009
most citedTheoretical Limits on Extrasolar Terrestrial Planet Detection with Coronagraphs

336 citations · 343 across the 5 of their papers we have counts for

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astro-ph20084 cited

Diversity among other worlds: characterization of exoplanets by direct detection

J. Schneider, A. Boccaletti, A. Aylward +34

The physical characterization of exoplanets will require to take spectra at several orbital positions. For that purpose, a direct imaging capability is necessary. Direct imaging re…

astro-ph2007

First Steps in Direct Imaging of Planetary Systems Like our Own: The Science Potential of 2-m Class Optical Space Telescopes

Karl Stapelfeldt, John Trauger, Weslay Traub +4

We summarize the scientific potential of high contrast optical space imaging for studies of extrasolar planets, debris disks, and planet formation. The unique scientific capabiliti…

astro-ph2006336 cited

Theoretical Limits on Extrasolar Terrestrial Planet Detection with Coronagraphs

O. Guyon, E. A. Pluzhnik, M. J. Kuchner +2

Many high contrast coronagraph designs have recently been proposed. In this paper, their suitability for direct imaging of extrasolar terrestrial planets is reviewed. We also devel…

astro-ph2005

Exoplanet Imaging with a Phase-induced Amplitude Apodization Coronagraph III. Hybrid Approach: Optical Design and Diffraction Analysis

E. A. Pluzhnik, O. Guyon, S. T. Ridgway +4

Properly apodized pupils can deliver point spread functions (PSFs) free of Airy rings, and are suitable for high dynamical range imaging of extrasolar terrestrial planets (ETPs). T…

astro-ph2005

Limits of Adaptive Optics for high contrast imaging

Olivier Guyon

The effects of photon noise, aliasing, wavefront chromaticity and scintillation on the point spread function (PSF) contrast achievable with ground based adaptive optics (AO) are ev…

astro-ph2004

Exoplanets imaging with a Phase-Induced Amplitude Apodization Coronagraph - I. Principle

Olivier Guyon, Eugene A. Pluzhnik, Raphael Galicher +3

Using 2 aspheric mirrors, it is possible to apodize a telescope beam without losing light or angular resolution: the output beam is produced by ``remapping'' the entrance beam to p…