In the last 3 years, extreme adaptive optics (XAO) systems entered into operation. They explore a new regime in terms of inner working angle and contrast. After introducing the science case and technical requirements, we will review the architecture of XAO systems, before presenting a few selected science highlights obtained on disks and planet formation with instruments such as SPHERE, GPI, SCEXAO and MagAO.Acknowledgments: D. Mawet, D. Mouillet, A-M. Lagrange, J-L. Beuzi
The Optimal Optical Coronagraph Workshop at the Lorentz Center in September 2017 in Leiden, the Neth...
The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is a multipurpose high-contrast...
The SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) instrument aims at detecting extr...
This paper deals with adaptive optics in the framework of very high-contrast astronomical imaging. S...
To directly detect exoplanets and protoplanetary disks, the development of high accuracy wavefront s...
As adaptive optics (AO) matures, it becomes possible to envision AO systems oriented towards specifi...
We show end-to-end extreme adaptive optics (XAO) simulation results for EPICS (Exo-Planets Imag...
International audienceWhile most confirmed exoplanets were discovered by indirect techniques such as...
Ground based adaptive optics is a potentially powerful technique for direct imaging detection of ext...
The next generation of extremely large telescopes (ELTs) have the potential to image habitable rocky...
EAS Publications Series, Astronomy with High Contrast Imaging, eds. C. Aime and R. Soummer, 12, pp. ...
Large segmented aperture ground and space based telescopes are undergoing development to enable dire...
High contrast imaging opportunties abound in astronomy, and some carry such intrinsic interest that ...
Post-processing of images delivered by the eXtreme Adaptive Optics (XAO) instrumentation is a crucia...
The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is a multipurpose high-contrast...
The Optimal Optical Coronagraph Workshop at the Lorentz Center in September 2017 in Leiden, the Neth...
The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is a multipurpose high-contrast...
The SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) instrument aims at detecting extr...
This paper deals with adaptive optics in the framework of very high-contrast astronomical imaging. S...
To directly detect exoplanets and protoplanetary disks, the development of high accuracy wavefront s...
As adaptive optics (AO) matures, it becomes possible to envision AO systems oriented towards specifi...
We show end-to-end extreme adaptive optics (XAO) simulation results for EPICS (Exo-Planets Imag...
International audienceWhile most confirmed exoplanets were discovered by indirect techniques such as...
Ground based adaptive optics is a potentially powerful technique for direct imaging detection of ext...
The next generation of extremely large telescopes (ELTs) have the potential to image habitable rocky...
EAS Publications Series, Astronomy with High Contrast Imaging, eds. C. Aime and R. Soummer, 12, pp. ...
Large segmented aperture ground and space based telescopes are undergoing development to enable dire...
High contrast imaging opportunties abound in astronomy, and some carry such intrinsic interest that ...
Post-processing of images delivered by the eXtreme Adaptive Optics (XAO) instrumentation is a crucia...
The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is a multipurpose high-contrast...
The Optimal Optical Coronagraph Workshop at the Lorentz Center in September 2017 in Leiden, the Neth...
The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is a multipurpose high-contrast...
The SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) instrument aims at detecting extr...