International audienceContext. Direct imaging of exoplanets requires very high contrast levels, which are obtained using coronagraphs. But residual quasi-static aberrations create speckles in the focal plane downstream of the coronagraph which mask the planet. This problem appears in ground-based instruments as well as in space-based telescopes. Aims. An active correction of these wavefront errors using a deformable mirror upstream of the coronagraph is mandatory, but conventional adaptive optics are limited by differential path aberrations. Dedicated techniques have to be implemented to measure phase and amplitude errors directly in the science focal plane. Methods. First, we propose a method for estimating phase and amplitude aberrations ...
International audienceDetecting light from faint companions or protoplanetary disks lying close to t...
Context. The next generation of space-borne instruments dedicated to the direct detection of exoplan...
International audienceContext. Fewer than 1% of all exoplanets detected to date have been characteri...
International audienceContext. Direct imaging of exoplanets requires very high contrast levels, whic...
The Self-Coherent Camera is dedicated to the direct detection of exoplanets. This instrument can be ...
International audienceContext. Direct detection of exoplanets requires high dynamic range imaging. C...
Context. In the context of direct imaging of exoplanets, coronagraphs are commonly propose...
International audienceExtreme adaptive optics and coronagraphy are mandatory for direct imaging of e...
Direct imaging is a powerful tool for exoplanet atmosphere characterization. High performance of the...
International audienceDirect detection is a very promising field in exoplanet science. It allows the...
Context. In the context of exoplanet detection, the performance of coronagraphs is limited by wavefr...
International audienceContext: In the context of exoplanet detection, the performance of coronagraph...
Direct imaging of exoplanets is very challenging because the planet is 10 4 to 10 10 fainter than th...
Direct imaging of exoplanets requires high dynamical techniques as adaptive optics and coronagraphy ...
International audienceDirect imaging of exoplanets requires the detection of very faint objects orbi...
International audienceDetecting light from faint companions or protoplanetary disks lying close to t...
Context. The next generation of space-borne instruments dedicated to the direct detection of exoplan...
International audienceContext. Fewer than 1% of all exoplanets detected to date have been characteri...
International audienceContext. Direct imaging of exoplanets requires very high contrast levels, whic...
The Self-Coherent Camera is dedicated to the direct detection of exoplanets. This instrument can be ...
International audienceContext. Direct detection of exoplanets requires high dynamic range imaging. C...
Context. In the context of direct imaging of exoplanets, coronagraphs are commonly propose...
International audienceExtreme adaptive optics and coronagraphy are mandatory for direct imaging of e...
Direct imaging is a powerful tool for exoplanet atmosphere characterization. High performance of the...
International audienceDirect detection is a very promising field in exoplanet science. It allows the...
Context. In the context of exoplanet detection, the performance of coronagraphs is limited by wavefr...
International audienceContext: In the context of exoplanet detection, the performance of coronagraph...
Direct imaging of exoplanets is very challenging because the planet is 10 4 to 10 10 fainter than th...
Direct imaging of exoplanets requires high dynamical techniques as adaptive optics and coronagraphy ...
International audienceDirect imaging of exoplanets requires the detection of very faint objects orbi...
International audienceDetecting light from faint companions or protoplanetary disks lying close to t...
Context. The next generation of space-borne instruments dedicated to the direct detection of exoplan...
International audienceContext. Fewer than 1% of all exoplanets detected to date have been characteri...