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Maire, Jérôme; Gagné, Jonathan; Lafrenière, David; Graham, James R.; Doyon, René
Proceedings of the International Astronomical Union, 06/2013, Volume: 8, Issue: S299Journal Article
Direct imaging and spectroscopy of exoplanets is a key element for understanding planet formation and migration. Such direct detections and characterizations remains technologically challenging, since a very high contrast ratio and small angular separation are involved, and futhermore speckle noise limits the high-contrast imaging performance. We further discuss a speckle subtraction and suppression technique that fully takes advantage of spectral and time-domain information on quasi-static speckles to measure the highest-fidelity photometry as well as accurate astrometry of detected companions.
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