Show simple item record

dc.contributor.authorJovanovic, N.
dc.contributor.authorGuyon, O.
dc.contributor.authorLozi, J.
dc.contributor.authorCurrie, T.
dc.contributor.authorHagelberg, J.
dc.contributor.authorNorris, B.
dc.contributor.authorSingh, G.
dc.contributor.authorPathak, P.
dc.contributor.authorDoughty, D.
dc.contributor.authorGoebel, S.
dc.contributor.authorMales, J.
dc.contributor.authorKuhn, J.
dc.contributor.authorSerabyn, E.
dc.contributor.authorTuthill, P.
dc.contributor.authorSchworer, G.
dc.contributor.authorMartinache, F.
dc.contributor.authorKudo, T.
dc.contributor.authorKawahara, H.
dc.contributor.authorKotani, T.
dc.contributor.authorIreland, M.
dc.contributor.authorFeger, T.
dc.contributor.authorRains, A.
dc.contributor.authorBento, J.
dc.contributor.authorSchwab, C.
dc.contributor.authorCoutts, D.
dc.contributor.authorCvetojevic, N.
dc.contributor.authorGross, S.
dc.contributor.authorArriola, A.
dc.contributor.authorLagadec, T.
dc.contributor.authorKasdin, J.
dc.contributor.authorGroff, T.
dc.contributor.authorMazin, B.
dc.contributor.authorMinowa, Y.
dc.contributor.authorTakato, N.
dc.contributor.authorTamura, M.
dc.contributor.authorTakami, H.
dc.contributor.authorHayashi, M.
dc.date.accessioned2017-01-18T22:52:54Z
dc.date.available2017-01-18T22:52:54Z
dc.date.issued2016-07-26
dc.identifier.citationN. Jovanovic ; O. Guyon ; J. Lozi ; T. Currie ; J. Hagelberg ; B. Norris ; G. Singh ; P. Pathak ; D. Doughty ; S. Goebel ; J. Males ; J. Kuhn ; E. Serabyn ; P. Tuthill ; G. Schworer ; F. Martinache ; T. Kudo ; H. Kawahara ; T. Kotani ; M. Ireland ; T. Feger ; A. Rains ; J. Bento ; C. Schwab ; D. Coutts ; N. Cvetojevic ; S. Gross ; A. Arriola ; T. Lagadec ; J. Kasdin ; T. Groff ; B. Mazin ; Y. Minowa ; N. Takato ; M. Tamura ; H. Takami and M. Hayashi " The SCExAO high contrast imager: transitioning from commissioning to science ", Proc. SPIE 9909, Adaptive Optics Systems V, 99090W (July 26, 2016); doi:10.1117/12.2234294; http://dx.doi.org/10.1117/12.2234294en
dc.identifier.issn0277-786X
dc.identifier.doi10.1117/12.2234294
dc.identifier.urihttp://hdl.handle.net/10150/622018
dc.description.abstractSCExAO 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.
dc.language.isoenen
dc.publisherSPIE-INT SOC OPTICAL ENGINEERINGen
dc.relation.urlhttp://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2234294en
dc.rights© 2016 SPIE.en
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectExtreme AOen
dc.subjectAdaptive opticsen
dc.subjectHigh contrast imagingen
dc.subjectExoplanetsen
dc.subjectSparse aperture maskingen
dc.subjectCoronagraphsen
dc.subjectImageren
dc.subjectFiber injectionen
dc.titleThe SCExAO high contrast imager: transitioning from commissioning to scienceen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Steward Observen
dc.contributor.departmentUniv Arizona, Coll Opt Scien
dc.identifier.journalADAPTIVE OPTICS SYSTEMS Ven
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en
dc.eprint.versionFinal published versionen
refterms.dateFOA2018-08-13T23:23:12Z
html.description.abstractSCExAO 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.


Files in this item

Thumbnail
Name:
99090W.pdf
Size:
853.1Kb
Format:
PDF
Description:
FInal Published Version

This item appears in the following Collection(s)

Show simple item record