HiCIAO High Contrast Instrument for the Subaru Next Generation Adaptive Optics M. Tamura 1, R. Suzuki 2, K. Hodapp 2, L. Abe 1, H. Takami 3, O. Guyon 3,

Slides:



Advertisements
Similar presentations
The SPHERE/ZIMPOL polarimeter for extra-solar planetary systems Hans Martin SCHMID, ETH Zurich and many collaborators in the SPHERE consortium IPAG Grenoble,
Advertisements

What is HiCIAO ? Near-infrared high contrast imaging instrument with a linear polarimetor at the 8.2m Subaru telescope. Targets: exoplanets and proto-planetary.
Standard stars for the ZIMPOL polarimeter
Strategic Exploration of Exoplanets and Disks with Subaru: SEEDS Nobuhiko Kusakabe, Motohide Tamura, Ryo Kandori, Tomoyuki Kudo, Jun Hashimoto, SEEDS/HiCIAO/AO188.
Subaru Explorations of Exoplanets and Disks with its IR Coronagraph in Shanghai :00-9:30 Motohide Tamura National Astronomical Observatory of.
ESO, 27 Nov 09 SPHERE – the high contrast challenge Markus Kasper, ESO 1 1.
High Contrast AO Imaging at the MMT with ARIES SDI Laird Close, Beth Biller, Eric Nielsen Don McCarthy & MMT AO Group (Steward Obs)
Instrumentation at the Subaru Telescope - next 10 years - Naruhisa Takato and Tomonori Usuda (Subaru Telescope)
NIR INSTRUMENT FOR GLAO Takashi Hattori, Iwata Ikuru (Subaru Telescope)
1 HICIAO-Assembly-Procedure Prepared for HICIAO CDR Author: Vern Stahlberger Institute for Astronomy Date:
HiCIAO: High Contrast Instrument for next generation Adaptive Optics For Subaru 8.2m telescope Based on a previous Japan/MEXT grant (Tokutei) PI & CoPIs:
Ben R. Oppenheimer, Sasha Hinkley, Anand Sivaramakrishnan, Remi Soummer, Douglas Brenner Ian Parry, David King, Steve Medlen PROJECT 1640.
FMOS: the fiber multiple-object spectrograph IV current status of OHS-based spectrograph Kyoto University : F.Iwamuro, T.Maihara, K.Ohta, S.Eto, M.Sakai.
Meeting of the Blue Dot Team, UCL, London, sept Single Aperture Concepts.
Anthony Boccaletti Observatoire de Paris LESIA. Several instruments dedicated to Exoplanet detection and characterization with High Contrast Imaging since.
PI type instruments Yosuke Minowa Naruhisa Takato, Ikuru Iwata (New Development group, Subaru Telescope) Subaru User’s Meeting 2013 (2014/01/21)
Maximizing GSMT Science Return with Scientific Figures of Merit.
Polarimetry Christoph Keller. Polarimetry Requirements Polarization sensitivity: amount of fractional polarization that can be detected above a (spatially.
Thermal Infrared Observation using Adaptive Secondary Mirror (ASM) Hiroshi TERADA (Subaru Telescope)  Ground-based Thermal IR w/AO  Subaru Thermal IR.
VLBI: Visible Light Broadband Imager Instrument Conceptual Design Presentation Tom Berger Lockheed Martin Solar and Astrophysics Lab.
NGAO Instrumentation Overview September 2008 Updated Sean Adkins.
Pupil Remapping for high dynamical range imaging Olivier Guyon Subaru Telescope National Astronomical Observatory of Japan Hilo, HI Michelson.
Recent & planned high-contrast work on the WCS and P3K Gene Serabyn Nov. 12, 2007.
NGAO Instrumentation Cost Drivers and Cost Savings September 2008 Sean Adkins.
F444W F300M F277W F356W F480M F335M F360M F460M F410M F430M LWF1 LWF2 LWF3 LWF4 LWF5 LWF6 LWF7 LWF8 LWF9 LWF10 LWF11 LWF12 F322W2 LWF F250M Imaging pupil.
James Webb Space Telescope and its Instruments George Rieke (MIRI Expert) & Marcia Rieke (NIRCam Expert) Steward Observatory, University of Arizona The.
An Optimized Pupil Coronagraph: A New Way To Observe Extrasolar Planets This work was performed for the Jet Propulsion Laboratory, California Institute.
Near Infrared Tunable Filter System for ATST Big Bear Solar Observatory & Solar Research Center, NJIT Aug. 25, 2003.
IRCS-HRU Subaru IRCS High Resolution Unit Hiroshi TERADA (NAOJ, Hawaii)
Masahiro Konishi (IoA, UTokyo), SWIMS Team S W I M S.
Big Bear Solar Observatory NST Main Features  All reflecting, off-axis Gregory optical configuration  PM: 1.6 m clear aperture with f/2.4  Figuring.
B.Delabre November 2003ANGRA DOS REIS - BRAZIL ESO 2 nd GENERATION INSTRUMENTATION – OPTICAL DESIGNS ESO VLT SECOND GENERATION INSTRUMENTATION Optical.
RAS E-ELT meeting 9th May 08 Fraser Clarke Towards EPICS; high contrast spectroscopy Fraser Clarke N Thatte, G Salter, M Tecza C Verinaud, M Kasper (EPICS.
1 FRIDA Engineering Status 17/05/07 Engineering Status May 17, 2007 F.J. Fuentes InFraRed Imager and Dissector for Adaptive Optics.
Oct 17, 2001SALT PFIS Preliminary Design Review Optical Integration and Test Plan 1 Southern African Large Telescope Prime Focus Imaging Spectrograph Optical.
Infrared Wavefront Sensor (IR-WFS) Yutaka Hayano Internal Meeting on Future Instrument Projects at Subaru April 26, 2010.
NIRCam ETU Testing at LMATC, Palo Alto Kailash C. Sahu.
Near Infrared Spectro-polarimeter (NIRSP) Conceptual Design Don Mickey Jeff Kuhn Haosheng Lin.
Current Status of SPICA Focal Plane Instruments October 19, 2009 Hideo Matsuhara (ISAS/JAXA) & FPI team.
1 A. Boccaletti Pasadena, Sept th Imaging EGPs with JWST/MIRI and VLT/SPHERE valuable experiences for TPF-C A. Boccaletti, P. Baudoz D. Rouan + coronagraphic.
Discriminating Migration Mechanisms of Tilted or Eccentric Planetary Systems Norio Narita (NAOJ/University of Hawaii)
SCI (SPICA coronagraph instrument) Keigo Enya & SCI team.
From NAOS to the future SPHERE Extreme AO system T. Fusco 1, G. Rousset 1,2, J.-L. Beuzit 3, D. Mouillet 3, A.-M. Lagrange 3, P. Puget 2 and many others.
Observational Studies for Understanding Planetary Migration Norio Narita National Astronomical Observatory of Japan.
Aligned, Tilted, Retrograde Exoplanets and their Migration Mechanisms Norio Narita (JSPS Fellow) National Astronomical Observatory of Japan.
High Contrast Imaging with Focal Plane Wavefront Sensing and PIAA for Subaru Telescopes Olivier Guyon Basile Gallet
The SPICA Coronagraph Project A BE 1 /E NYA 2 /T ANAKA 2 /N AKAGAWA 2 /M URAKAMI 1 N ISHIKAWA 1 /T AMURA 1 /F UJITA 3 /I TOH 3 /K ATAZA 2 /G UYON 4 AND.
Kyoto 3DII (3DII) + AO Apr 26 HST 1.What is 3DII? 2.Purposes of 3DII + AO188 3.What is needed for this? 4.Present status 5.Cass or Nasmyth in future?
Molecules in the atmosphere of extrasolar planets, Paris, nov Direct Imaging of Extrasolar Planets Overview of Ground & Space Programs Anthony.
Hubble Space Telescope Coronagraphs John Krist JPL.
AO188/LGS Status and Schedule 1 Yutaka Hayano January 31, 2008.
The FMOS Facility for the SUBARU telescope Gavin Dalton Oxford/RAL.
Discriminating Planetary Migration Mechanisms by Direct Imaging Norio Narita National Astronomical Observatory of Japan on behalf of SEEDS/HiCIAO/AO188.
Current Status of SPICA FPI Mechanical I/F & resources April 6 th 2010 Hideo Matsuhara (ISAS/JAXA) & FPI team.
Kailash C. Sahu NIRCam: Status Update 1m Cold, space-facing side
JTPF Japanese Terrestrial Planet Finder JTPF Japanese Terrestrial Planet Finder M. Tamura (NAOJ) JTPF Working Group TPF-C coronagraph WS :15-15:30.
Page 1 Adaptive Optics in the VLT and ELT era Wavefront sensors, correctors François Wildi Observatoire de Genève.
Keck Observatory Overview Peter Wizinowich W. M. Keck Observatory AOSC May 31, 2004.
（ 1: Kobe University, 2: Nagoya University, 3: NAOJ) ☆ Abstract ☆ We obtained a high spatial resolution (FWHM ~ 0.1”) near-infrared image of XZ Tau, a.
IFS prototype – PM3 LAM, 13/06/2003 Prototype testing at CRAL Tests at room temperature in the visible.
Astronomical Observational Techniques and Instrumentation
Introduction NICMOS (Near-Infrared Camera and Multi-Object Spectroscopy) was installed on the Hubble Space Telescope during SM2 in 1997 and has been the.
Page 1 Lecture 16 Extreme Adaptive Optics: Exoplanets and Protoplanetary Disks Claire Max AY 289 March 7, 2016 Based in part on slides from Bruce Macintosh.
Focal Plane Instrumentation at Big Bear Solar Observatory
Pyramid sensors for AO and co-phasing
Adaptive optics Now: Soon: High angular resolution
An IFU slicer spectrometer for SNAP
He Sun Advisor: N. Jeremy Kasdin Mechanical and Aerospace Engineering
Infrared Instrumentation for Small Telescopes
The Installation & Characterization of the Coronagraphic Upgrade to the Extreme Adaptive Optics Test Bed Darrius Robinson.
Presentation transcript:

HiCIAO High Contrast Instrument for the Subaru Next Generation Adaptive Optics 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, J. Morino 1, N. Murakami 1, V. Stahlberger 2, A. Tavrov 1, H. Yamada 2, J. Nishikawa 1, N. Ukita 1, J. Hashimoto 1, H. Izumiura 4, M. Hayashi 3, T. Nishimura 3 1)NAOJ 2) UH Hilo, 3) Subaru Telescope, 4) Okayama TPF Coronagraph WS :15-20:25 （ 6 min + 4 min)

Diversity of proto- Planetary disks Compact disk around massive 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 AurYoung BD around DH Tau

Nasmyth platform Telescope Common Optics + AO Module Coronagraph Module IR Camera Module High Contrast Optics Module Warm Cold Coronagraph Focal masks Pupil stops Differential optics (Wollaston prisms) HAWAII 2-RG 2k  2k HgCdTe array ASICS Controller Filters Common+Differential Pupil Viewer In/out position 188 actuators AO Future: Complementary MEM DM (32  32) HiCIAO Concept  Merits  Modular style  Flexible coronagraph  Differential Imaging  High 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: 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 Progress Lens manufacturing (Optics For Research) Wollaston Prism manufacturing (Bernhard Halle) Occulting Mask & Lyot Stop (Applied Image Group) Lenses Various lenses Wollaston 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

Schedule OctCryo-test Optics finish Nov Alignment Dec Final assembling Mar to the summit Optical alignment First light 2007 Lab test

Feedback: Privacy Policy Feedback
Do Not Sell My Personal Information
About project: SlidePlayer Terms of Service

© 2025 SlidePlayer.com. Inc. All rights reserved.