Microsoft PowerPoint - HiCIAOTamuraBerkeley070607f.ppt

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1 HiCIAO and exoplanet/disk searches on Subaru Berkeley Motohide Tamura NAOJ, Extrasolar Planet Project Office in collaboration with University of Hawaii, Hilo

2 Collaborators K. Hodapp 2, R. Suzuki 3, H. Takami 3, L. Abe 1, O. Guyon 3, H. Suto 1, S. Jacobson 2, R. Kandori 1, J. Morino 1, N. Murakami 1, V. Stahlberger 2, A. Tavrov 1, H. Yamada 2, J. Nishikawa 1, N. Ukita 1, J. Hashimoto 1, T. Nishimura 3 (1) NAOJ, (2) UH, (3) NAOJ/Subaru, (4) NAOJ/Okayama Figure Credit M. Fukagawa 5, T. Kudo 6, Y. Itoh 7, Z. Jiang 8, T. Hioki 7 (see Poster), R. Neuhäuser 9 (5) Nagoya U., (6) GUAS, (7) Kobe U., (8) PMO, (9) U. Jena

3 Subaru has an AO Coronagraph since act. AO + CIAO at CS First dedicated cold coronagraph on 8-m telescopes Diversity of proto- Planetary disks Young very low-mass Companion Compact disk around massive YSOs

4 NEW type of disk: HD banana split Herbig Ae star in Lupus (d=200pc) 1550 AU λ=1.65 micron Subaru/CIAO λ=24.5 micron Subaru/COMICS

5 Subaru is developing a new coronagraph - HiCIAO Warm Cold Telescope Common Optics + AO Module Coronagraph Module High Contrast Optics Module IR Camera Module Nasmyth platform 188 actuators AO near future ture: Complementary MEM DM ( ) Coronagraph Focal masks Pupil stops Differential optics (Wollaston prisms) Camera Hawaii 2-RG2 2k 2k array ASICS Sidecar Controller Filters Common+Differential Wollaston Prism

6 Specifications HiCIAO Focus Wavelength Pixel scale Detector ASIC Readout Observation modes Field of View Strehl Ratio Coronagraph Filters (as of first light) IR Nasmyth (with AO188) um /pix 2048x2048 HgCdTe (HAWAII-2RG) Sidecar (warm) Direct Imaging (DI) Polarimetric Differential Imaging (PDI) Spectral Differential Imaging (SDI) 20 x20 (DI), 20 x10 (PDI), 5.8 x5.8 (SDI) 0.6 (J), 0.7 (H), 0.8 (K) Occulting mask, Classical Lyot stop J, H, K (BB); CH4 set, [FeII] set (SDI)

7 HiCIAO Optics supports differential imaging direct imaging, polarization differential imaging, & spectral differential imaging Collimator Lyot Stop Camera Common Path Filter Filter & Detector Detector Wollaston Prism Differential Path Filter WPs made from YLF

8 AO Interface Nasmyth Floor HiCIAO Camera AO188 Optical Bench HiCIAO Foreoptics Electronics Racks ~1800 Support Frame ~1500 ~1400

9 Expected performances of HiCIAO/AO188 Resolution (FWHM): From ~0.1" w/ao36 to 0.03"~0.05"! Contrast: >One order better (>13 1") sensitivity Band J H Ks CH 4 low CH 4 high [FeII] 5σ (1 hour) Wavelength (µm) resolution FWHM (mas) CIAO CIAO

10 HiCIAO in the final assembling (in Hilo) Most recent image by Suzuki

11 Path to High-Contrast Extreme-AO System 1 st stage 2 nd stage 3 rd stage slow Focal Plane AO removes static speckles fast Focal Plane AO true extreme-ao Woofer AO 1st stage wavefront correction Tweeter AO 2 nd stage fine wavefront correction Coronagraph blocks starlight keeps planet light Near-IR camera science image SDI fast readout AO188 MEMs DM PIAAC HiCIAO put AO188 picture here put HiCIAO picture here

12 Schedule and Summary Development: quick (FY ) Sept 2006 Feb At present 2007 June 2007 Sep Concept design fixed PDR CDR final assembling Lab. test First Light (near) Future upgrades flexible instrument! 2 nd -stage MEMS-DM for Extreme AO (~1000 elements equivalent), already lab. demonstrated (Guyon). Extensive Surveys for exoplanets and disks Strategic observations in (100 nights) are proposed very soon. ~500 stars in total will be surveyed. ~300 stars for planets and ~200 stars for disks.

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