activity
20042008
most citedWavefront error correction and Earth-like planet detection by Self-Coherent Camera in space

78 citations · 99 across the 4 of their papers we have counts for

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6 papers · 1 filter

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-ph200878 cited

Wavefront error correction and Earth-like planet detection by Self-Coherent Camera in space

R. Galicher, P. Baudoz, G. Rousset

In the context of exoplanet detection, the performance of coronagraphs is limited by wavefront errors. To efficiently correct for these aberrations with a deformable mirror, it is…

astro-ph20081 cited

Theory and laboratory tests of the multi-stage phase mask coronagraph

P. Baudoz, R. Galicher, J. Baudrand +1

A large number of coronagraphs have been proposed to overcome the ratio that exists between the star and its planet. The planet finder of the Extremely Large Telescope, which is ca…

astro-ph200716 cited

Expected Performance of a Self-Coherent Camera

R. Galicher, P. Baudoz

Residual wavefront errors in optical elements limit the performance of coronagraphs. To improve their efficiency, different types of devices have been proposed to correct or calibr…

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-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…