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The Subaru Coronagraphic Extreme Adaptive Optics Imager: First Results and On-Sky Performance

We present new on-sky results for the Subaru Coronagraphic Extreme Adaptive Optics imager (SCExAO) verifying and quantifying the contrast gain enabled by key components: the closed-loop coronagraphic low-order wavefront sensor (CLOWFS) and focal plane wavefront control ("speckle nulling"). SCExAO will soon be coupled with a high-order, Pyramid wavefront sensor which will yield > 90% Strehl ratio and enable 10^6--10^7 contrast at small angular separations allowing us to image gas giant planets at solar system scales. Upcoming instruments like VAMPIRES, FIRST, and CHARIS will expand SCExAO's science capabilities.

preprint2013arXivOpen access
Thayne CurrieOlivier GuyonFrantz MartinacheChristophe ClergeonMichael McElwainChristian ThalmannNemanja JovanovicGarima SinghTomoyuki Kudo
astro-ph.IMastro-ph.EP
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Thayne CurrieOlivier GuyonFrantz MartinacheChristophe ClergeonMichael McElwainChristian ThalmannNemanja JovanovicGarima SinghTomoyuki Kudo

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