HIGHLIGHTS
SUMMARY
High-contrast imaging (HCI) detections are mostly limited to about a dozen very young and luminous giant exoplanets (e_g, Marois et_al 2010; Lagrange et_al 2009; Macintosh et_al 2015) due to the challenging contrast requirements at a ? 1 NASA Hubble Fellow Exoplanet Orbit Database: http://exoplanets.org/ fraction of an arcsecond angular distance from the star which could be a billion times brighter than the exoplanet. Significant advances in HCI technology are needed to address two major scientific questions: the architectures of outer planetary systems, which remain essentially unexplored (e_g, Dressing and amp; Charbonneau 2015 . . .
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