The SCExAO high contrast imager: Transitioning from commissioning to science

dc.contributor.authorJovanovic, Nemanja
dc.contributor.authorGuyon, Olivier
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.authorIreland, Michael
dc.coverage.spatialEdinburgh, United Kingdom
dc.date.accessioned2018-11-30T01:19:23Z
dc.date.available2018-11-30T01:19:23Z
dc.date.createdJune 26 - July 1 2016
dc.date.issued2016
dc.date.updated2018-11-29T08:20:23Z
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.format.mimetypeapplication/pdfen_AU
dc.identifier.isbn9781510601970
dc.identifier.urihttp://hdl.handle.net/1885/154045
dc.publisherSPIE - The International Society for Optical Engineering
dc.relation.ispartofseriesAdaptive Optics Systems V
dc.sourceProceedings of SPIE Volume 9909: The International Society for Optical Engineering
dc.titleThe SCExAO high contrast imager: Transitioning from commissioning to science
dc.typeConference paper
dcterms.accessRightsOpen Accessen_AU
local.contributor.affiliationJovanovic, Nemanja, Macquarie University
local.contributor.affiliationGuyon, Olivier, National Astronomical Observatory of Japan
local.contributor.affiliationLozi, J, National Astronomical Observatory of Japan
local.contributor.affiliationCurrie, T, National Astronomical Observatory of Japan
local.contributor.affiliationHagelberg, J, University of Hawaii
local.contributor.affiliationNorris, B, University of Sydney
local.contributor.affiliationSingh, G, Jet Propulsion Laboratory
local.contributor.affiliationPathak, P, National Astronomical Observatory of Japan
local.contributor.affiliationDoughty, D, National Astronomical Observatory of Japan
local.contributor.affiliationGoebel, S, National Astronomical Observatory of Japan
local.contributor.affiliationIreland, Michael, College of Science, ANU
local.contributor.authoruidIreland, Michael, u5544212
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020102 - Astronomical and Space Instrumentation
local.identifier.ariespublicationa383154xPUB4935
local.identifier.doi10.1117/12.2234294
local.identifier.scopusID2-s2.0-85001932779
local.identifier.thomsonID000387429700026
local.type.statusPublished Version

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