High performance coronagraphy for direct imaging of exoplanets

Abstract

Abstract. Coronagraphy has recently been an extremely active field of research, with several high performance concepts proposed, and several new coronagraphs tested in laboratories and telescopes. Coronagraph concepts can be grouped in a few broad categories: Lyot-type coronagraphs, pupil apodization and nulling interferometers. Among existing coronagraph concepts, several approach the fundamental performance limit imposed by the physical nature of light. To achieve their full potential, coronagraphs require exquisite wavefront control and calibration. This has been, and still is, the main bottleneck for the scientifically productive use of coronagraphs on ground-based telescopes. New and promising wavefront sensing techniques suitable for high contrast imaging have however been developed in the last few years and are started to be realized in laboratories. I will review some of these enabling technologies, and show that coronagraphs are now ready for "prime time" on existing and future telescopes.

Medium-resolution integral-field spectroscopy for high-contrast exoplanet imaging

“…Subsequent post-processing algorithms (cADI, LOCI, PCA, AN-DROMEDA) aim to optimize the residual attenuation while conserving the planatery signal (see e.g. Guyon 2011;Mawet et al 2012; Chauvin 2016, for reviews).So far, direct imaging detections are generally limited to a specific part of the exoplanet population: Young gas giants in wide orbits that glow by radiating out the internal heat that remained from the time of their formation. These planets can be resolved from their host stars owing to their relatively large mutual angular separation and brightness at infrared wavelengths.…”

“…Subsequent post-processing algorithms (cADI, LOCI, PCA, AN-DROMEDA) aim to optimize the residual attenuation while conserving the planatery signal (see e.g. Guyon 2011;Mawet et al 2012; Chauvin 2016, for reviews).…”