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The SCExAO high contrast imager: transitioning from commissioning to science

SCExAO is the premier high-contrast imaging platform for the Subaru Telescope. It offers high Strehl ratios at near-IR wavelengths (y-K band) with stable pointing and coronagraphs with extremely small inner working angles, optimized for imaging faint companions very close to the host. In the visible, it has several interferometric imagers which offer polarimetric and spectroscopic capabilities. A recent addition is the RHEA spectrograph enabling spatially resolved high resolution spectroscopy of the surfaces of giant stars, for example. New capabilities on the horizon include post-coronagraphic spectroscopy, spectral differential imaging, nulling interferometry as well as an integral field spectrograph and an MKID array. Here we present the new modules of SCExAO, give an overview of the current commissioning status of each of the modules and present preliminary results.

Identiferoai:union.ndltd.org:arizona.edu/oai:arizona.openrepository.com:10150/622018
Date26 July 2016
CreatorsJovanovic, N., Guyon, O., Lozi, J., Currie, T., Hagelberg, J., Norris, B., Singh, G., Pathak, P., Doughty, D., Goebel, S., Males, J., Kuhn, J., Serabyn, E., Tuthill, P., Schworer, G., Martinache, F., Kudo, T., Kawahara, H., Kotani, T., Ireland, M., Feger, T., Rains, A., Bento, J., Schwab, C., Coutts, D., Cvetojevic, N., Gross, S., Arriola, A., Lagadec, T., Kasdin, J., Groff, T., Mazin, B., Minowa, Y., Takato, N., Tamura, M., Takami, H., Hayashi, M.
ContributorsUniv Arizona, Steward Observ, Univ Arizona, Coll Opt Sci, National Astronomical Observatory of Japan, Subaru Telescope (United States), National Astronomical Observatory of Japan, Subaru Telescope (United States), National Astronomical Observatory of Japan, Subaru Telescope (United States), National Astronomical Observatory of Japan, Subaru Telescope (United States), Univ. of Hawaii (United States), Univ. of Sydney (Australia), Jet Propulsion Lab. (United States), National Astronomical Observatory of Japan, Subaru Telescope (United States), National Astronomical Observatory of Japan, Subaru Telescope (United States), National Astronomical Observatory of Japan, Subaru Telescope (United States), Univ. of Arizona (United States), ETH Zürich (Switzerland), Jet Propulsion Lab. (United States), Univ. of Sydney (Australia), Univ. of Sydney (Australia), Observatoire de la Côte d'Azur (France), National Astronomical Observatory of Japan, Subaru Telescope (United States), The Univ. of Tokyo (Japan), National Astronomical Observatory of Japan (Japan), Australian National Univ. (Australia), Macquarie Univ. (Australia), Australian National Univ. (Australia), Australian National Univ. (Australia), Macquarie Univ. (Australia), Macquarie Univ. (Australia), Univ. of Sydney (Australia), Macquarie Univ. (Australia), Macquarie Univ. (Australia), Univ. of Sydney (Australia), Princeton Univ. (United States), Princeton Univ. (United States), Univ. of California, Santa Barbara (United States), National Astronomical Observatory of Japan, Subaru Telescope (United States), National Astronomical Observatory of Japan, Subaru Telescope (United States), Astrobiology Ctr. of NINS (Japan), National Astronomical Observatory of Japan (Japan), National Astronomical Observatory of Japan (Japan)
PublisherSPIE-INT SOC OPTICAL ENGINEERING
Source SetsUniversity of Arizona
LanguageEnglish
Detected LanguageEnglish
TypeArticle
Rights© 2016 SPIE
Relationhttp://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2234294

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