Objectif The direct detection of young and warm extrasolar giant planets in the habitable zone of nearby cool stars is one of the major goals of future ground-based high-contrast imaging (HCI) instruments. The motive is to study the physical and chemical properties of exoplanetary atmospheres and search for evidences of biosignatures. Direct imaging is the required technique to characterize exoplanets with spectroscopy of their atmospheres. However, the ability to resolve planet signal above bright stellar halo is still a challenge. A coronagraph is an optic, which suppresses the diffraction effects of the telescope by blocking the starlight but wavefront errors arising due to Earth’s atmospheric turbulence scatter starlight over the science region of interest and bury faint planet photons in stellar/speckle noise. Most of these errors are mitigated by the dedicated Extreme Adaptive Optics instruments. However, under the AO/ExAO WF residuals, imaging and characterizing exoplanets at small angles require achieving detection limit 10 to 100 times better than the state of the art. No existing ground-based HCI instruments have successfully disentangled the planet signals from stellar residuals at small angles. The proposal seek to develop and demonstrate wavefront sensing and control techniques that will enhance the planet detection sensitivity at small angles and will aid the existing HCI instruments in directly imaging young Jovian-like exoplanets at small angles around nearby stars. This research proposal will also enable next generation of exoplanets characterization instruments with the European Extremely Large Telescope to perform low resolution spectroscopy of Neptune or Super-Earth exoplanets in the HZ of low mass stars (for example M-type). Champ scientifique natural sciencesphysical sciencesastronomyplanetary sciencesplanetsexoplanetologynatural sciencesphysical sciencesastronomyobservational astronomyinfrared astronomynatural sciencesphysical sciencesastronomyplanetary sciencesplanetsgiant planetssuper-Earthsnatural sciencesearth and related environmental sciencesatmospheric sciencesmeteorologyatmospheric circulationatmospheric turbulencenatural sciencesphysical sciencesopticsspectroscopy Programme(s) H2020-EU.1.3. - EXCELLENT SCIENCE - Marie Skłodowska-Curie Actions Main Programme H2020-EU.1.3.2. - Nurturing excellence by means of cross-border and cross-sector mobility Thème(s) MSCA-IF-2017 - Individual Fellowships Appel à propositions H2020-MSCA-IF-2017 Voir d’autres projets de cet appel Régime de financement MSCA-IF-EF-ST - Standard EF Coordinateur OBSERVATOIRE DE PARIS Contribution nette de l'UE € 173 076,00 Adresse AVENUE DE L OBSERVATOIRE 61 75014 Paris France Voir sur la carte Région Ile-de-France Ile-de-France Paris Type d’activité Higher or Secondary Education Establishments Liens Contacter l’organisation Opens in new window Site web Opens in new window Participation aux programmes de R&I de l'UE Opens in new window Réseau de collaboration HORIZON Opens in new window Coût total € 173 076,00