hiciao high contrast instrument for the subaru next generation adaptive optics

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HiCIAO High Contrast Instrument for the Subaru Next Generation Adaptive Optics. TPF Coronagraph WS 2006.9.28 20:15-20:25 ( 6 min + 4 min). M. Tamura 1 , R. Suzuki 2 , K. Hodapp 2 , L. Abe 1 , H. Takami 3 , O. Guyon 3 , H. Suto 1 , S. Jacobson 2 , R. Kandori 1 , - PowerPoint PPT Presentation

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HiCIAOHigh Contrast Instrument for

the Subaru Next Generation Adaptive Optics

M. Tamura1, R. Suzuki2, K. Hodapp2, L. Abe1, H. Takami3, O. Guyon3, H. Suto1, S. Jacobson2, R.

Kandori1, J. Morino1, N. Murakami1, V. Stahlberger2 , A.

Tavrov1, H. Yamada2, J. Nishikawa1, N. Ukita1, J. Hashimoto1,

H. Izumiura4, M. Hayashi3, T. Nishimura3 1) NAOJ

2) UH Hilo, 3) Subaru Telescope, 4) Okayama

TPF Coronagraph WS 2006.9.28   20:15-20:25 ( 6 min + 4 min)

Diversity of proto-Planetary disks

Compact disk aroundmassive YSOs (BN)

Current Subaru AO Coronagraph Cs 36-act. AO + CIAO

First "dedicated" IR coronagraph on 8-m telescopes

Disk Morphology: spiral, banana-split Companion searches High-resolution Polarimetry: BN, bPic

Young very low-mass Companion

Bipolar structure only seen in Pol.Spiral disk around AB Aur Young BD around DH Tau

Nasmyth platformNasmyth platform

Tele

scop

eTele

scop

e

Com

mon

Com

mon

Opti

cs +

Opti

cs +

AO

AO

Mod

ule

Mod

ule

Coro

nag

rap

h

Coro

nag

rap

h

Mod

ule

Mod

ule

IR C

am

era

IR C

am

era

Mod

ule

Mod

ule

Hig

h

Hig

h

Con

trast

Con

trast

Op

tics

Op

tics

Mod

ule

Mod

ule

WarmWarm CoColdld

CoronagraphCoronagraphFocal masksFocal masksPupil stopsPupil stops

Differential Differential opticsoptics(Wollaston prisms)(Wollaston prisms)

HH AWAII AWAII 2-RG2-RG22k k 22kk HgCdTe arrayHgCdTe arrayASICS ControllerASICS Controller

FiltersFiltersCommon+DifferentialCommon+Differential

Pupil ViewerPupil ViewerIn/out positionIn/out position

188 actuators188 actuatorsAOAOFutureFuture::ComplementaryComplementaryMEM DM (32MEM DM (3232)32)

HiCIAO ConceptMerits

Modular styleFlexible coronagraphDifferential ImagingHigh performance array & ASIC controller

Observation Modes

DI Mode

PDI Mode SDI Mode

Spectral Differential Imaging Mode  FOV : 5"×5"  Filter : CH4 set, [FeII] set  Double Wollaston Prism  Coronagraph available  Contrast: 104 @0.1", 106   @1"

Direct Imaging Mode  FOV : 20"×20"  Pixel scale : 0.010"/pix  Wavelengths : 0.85 ~ 2.5μm  Filters : J, H, Ks, [FeII], Bgγ, H2, etc.  Strehl Ratio : 0.6(J) 、 0.7(H) 、 0.8(Ks)    Coronagraph available

Polarimetric Differential Imaging Mode  FOV : 10"×20"  Filter : J, H, Ks, [FeII], Bgγ, H2, etc.  Polarimetry with Wollaston Prism and Waveplate  Coronagraph available

Optics pictures from OFR (if available)

Optics ProgressLens manufacturing (Optics For Research)

Wollaston Prism manufacturing (Bernhard Halle)

Occulting Mask & Lyot Stop (Applied Image Group) Lenses

Various lensesWollaston prism YLF crystal

Filters (Barr Associate)

Mechanics Progress

Stages and controller( Newport )

Fore Optics

Local PC control

Stages and controller

Fore Optics

Mechanics Progress

Camera Optics

Optical bentch

Dewar

Schedule2006 Oct Cryo-test

Optics finish

Nov   Alignment

Dec   Final assembling

Mar   to the summit

Optical alignment

First light

2007

Lab test

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