Collaboration status between ASIAA and Subaru Shiang-Yu Wang ( 王祥宇 ) Institute of Astronomy and Astrophysics Academia Sinica.

Slides:



Advertisements
Similar presentations
4D2U theater at NAOJ 4D Digital Universe Project Today & Future
Advertisements

(Radio) Astronomy in Taiwan
The 3 rd workshop on Large Mm/Submm Telescopes in the ALMA Era March 10, 09:00 – 18:10 March 11, 09:00 – 17:40 COSMOS Lodge Conference Room.
Taiwan America Occultation Survey TAOS 2002/8/28 TAOS photometry using IRAF Shao-Er Chuang Department of Earth sciences, National Taiwan Normal University,
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The March to Early.
OPTICON Board Meeting, Porto, OPTICON WP4 Interferometry Status Report D. Mourard presented by A. Chelli.
ASIAA Research Highlights and Prospects with HSC Keiichi Umetsu, ASIAA SAC HSC Science Workshop
Weak Lensing Study of DM sub halos in Coma Cluster T. Futamase Astronomical Institute, Tohoku University, Sendai, Japan 29 th Apr. Collaborators:
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array.
Current Status of Lulin Observatory Hung-Chin Lin Taiwan.
M2FS: Michigan/Magellan Fiber System. M2FS (Michigan/Magellan Fiber System) Fiber-fed MOS w/2 independent and identical spectrograph arms 256 total fibers.
Science Specification Table 12 keV keV for neutral particles 40.5 cm 2 image plane Electronic Noise 3 keV FWHM Proton Dead Layer
Ch 25 1 Chapter 25 Optical Instruments © 2006, B.J. Lieb Some figures electronically reproduced by permission of Pearson Education, Inc., Upper Saddle.
Berkeley workshop summary Redundancy : dual detector Field of view : 3”x6” Spectrograph length goal: < 400 mm Isostatic mount on the base plate with control.
Status of the Korean ALMA project Jongsoo Kim Korea Astronomy and Space Science Institute.
2008 Decmeber 5 ALMA-JT Science Meeting 1 ALMA Project News Koh-Ichiro Morita ALMAJ Project Scientist.
Masahiro Konishi (IoA, UTokyo), SWIMS Team S W I M S.
SKA-Japan Industry Forum [SKA-Japan Workshop 2010] EMC & Microwave Systems November 05, 2010.
LSST Scheduler status Francisco Delgado Sr. Software Engineer Telescope & Site.
Hanoi, Aug. 6-12, 2006 Pascal Vernin 1 Antares Status report P.Vernin CEA Saclay, Dapnia On behalf of the Antares collaboration P.Vernin
Japanese Plans for the IYA 2009 Kaz Sekiguchi National Astronomical Observatory of Japan.
14-16 January, 2009Subaru User’s Meeting (NAOJ) Possible Collaboration between Seoul National University and Subaru Myungshin Im (CEOU/Astronomy Seoul.
Mark Bowen Acting Theme Leader – Technologies for Radio Astronomy CSIRO Astronomy and Space Science 14 October 2010 Australia Telescope Users Committee.
Presentation EddiCam consortium, FF, Madrid 13/06/2002 Eddington programmatic status Fully approved by SPC as part of ESA’s science program as project.
The Hard X-ray Modulation Telescope Mission
SIMCorBSIMCorB 1 Policies and Procedures n Data administration and quality assurance standards, policies, and procedures (8.2.1) n User requirements for.
ASIAA NTU PHYS J.H.P.Wu & AMiBA Team To remove the ground pickup and electronic DC component in the data, we tracked the source- (P1) and tail- (P2) patches.
EA ARC Ken Tatematsu East-Asian ARC Manager. ARC organization Difference between ARCS: NA: concentrated in Charlottesville Europe: distributed in different.
A Search for Hydroxlyamine (NH 2 OH) Towards IRC+10216, Orion-S, Orion(KL), SgrB2(N), SgrB2(OH), W512M, W3(IRS5) R. L. Pulliam NRAO / North American ALMA.
Astronomy & Astrophysics Advisory Committee (AAAC) May 11, 2006 Vladimir Papitashvili Antarctic Sciences Section Office of Polar Programs National Science.
(Radio) Astronomy in Taiwan Jeremy Lim Institute of Astronomy & Astrophysics, Academia Sinica (ASIAA), Taiwan Taiwan (22.5 million) Malaysia (23 million)
Status of LIGO Data Analysis Gabriela González Department of Physics and Astronomy Louisiana State University for the LIGO Scientific Collaboration Dec.
Report from Subaru Advisory Committee The main issues of the current SAC: ・ Extensive (strategic) program of Subaru telescope ・ International collaborations.
Upgrade plan of the MOA 1.8-m telescope F. Abe MOA collaboration 19 Jan. 2009, 13th Microlensing Paris.
SWIIMS A New NIR MOS Spectrograph for TAO 6.5m Telescope K. Motohara, M. Konishi, S. Sako, N. Mitani, T. Aoki, K. Asano, M. Doi, T. Handa, K. Kawara, K.
Suggested Subaru-NAOJ/Princeton Consortium: Overview Michael Strauss, Ed Turner, Jim Gunn January 25, 2007.
Report on the Second Asian Radio Astronomy School 2008 Tomoya Hirota (Mizusawa-VERA, NAOJ) 1.
Academia Sinica National Taiwan University AMiBA System Performance Kai-yang Lin 1,2 and AMiBA Team 1,2,3 1 Institute of Astronomy and Astrophysics, Academia.
ALMA Common Software Basic Track A walk through ACS functionality.
Current Status of the Lulin Observatory Hung-Chin Lin ( 林宏欽 ), Wen-Ping Chen ( 陳文屏 ), K. H. Chang ( 張光祥 ), Ming-Hsin Chang (張明新), Yung-Hsin Chang (張永欣),
The North American ALMA Science Center North America’s ALMA Regional Center The North American ALMA Science Center acts as the gateway to ALMA for North.
Data Analysis Software Development Hisanori Furusawa ADC, NAOJ For HSC analysis software team 1.
ALMA Polarization Commissioning and Verification Status Kouichiro Nakanishi (Joint ALMA Observatory/NAOJ) on behalf of ALMA Polarization Commissioning.
Array for Microwave Background Anisotropy AMiBA SZ Science AMiBA Team NTU Physics Figure 4. Simulated AMiBA deep surveys of a 1deg 2 field (no primary.
JTPF Japanese Terrestrial Planet Finder JTPF Japanese Terrestrial Planet Finder M. Tamura (NAOJ) JTPF Working Group TPF-C coronagraph WS :15-15:30.
HSC development in Taiwan Shiang-Yu Wang ( 王祥宇 ) Institute of Astronomy and Astrophysics Academia Sinica.
Why Collaboration?  Better science through collaboration If you want to do a big survey, you need to benefit (or persuade) many scientists. (Democratic.
AS NTU Introductory Atronomy Spring MAR Modern Telescopes Best to surf the web Recommend search engine: Select search for.
Update on Activities in Suspensions for Advanced LIGO Norna A Robertson University of Glasgow and Stanford University LSC meeting, Hanford, Aug 20 th 2002.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array.
Space Part 06, Beijing, China, April 21, Lobster-Eye (LE) Novel Wide Field X-ray Telescopes FOV of 100 sq. deg. and more easily possible (classical.
ALMA and the Call for Early Science The Atacama Large (Sub)Millimeter Array (ALMA) is now under construction on the Chajnantor plain of the Chilean Andes.
E-MERLIN & EVLA P.J.DiamondP.J.Diamond MERLIN/VLBI National Facility Jodrell Bank Observatory University of Manchester MERLIN/VLBI National Facility Jodrell.
ALMA’s Roots in Three Scientific Visions Paul Vanden Bout NRAO The Dusty & Molecular Universe – Paris 28/10/04.
Status Report of Taiwan Two Meter Telescope Yi Chou Graduate Institute of Astronomy National Central University 2016/1/ 兩岸天文儀器會議.
ALMA Project Status Adrian Russell. Where is ALMA? El llano de Chajnantor ALMA.
ALMA Common Software Basic Track Project Lifecycle.
ETC Block Diagram. Source Spectrum is derived from: Spectra Type –Stellar (50 stellar types) –Galaxies (elliptical, spiral) –QSO Luminosity Profile –point.
Brenna Flaugher, PMG, April 6, 2007 DECam Funding Need Profile (Dec 06) (then yr $, Overhead included) This gave a technically driven schedule resulting.
A Search for High Redshift Galaxies behind Gravitationally Lensing Clusters Kazuaki Ota (Kyoto U) Johan Richard (Obs.Lyon), Masanori Iye (NAOJ), Takatoshi.
ALMA and FP6 Opportunities and strategy Funded project – construction phase FP6 timeframe 2003 – Good timing - first science planned for.
Seeing the Invisible: Observing the Dark Side of the Universe Sarah Bridle University College London.
Joint Astrophysics Projects with CNRS Andreas Kelz Astrophysikalisches Institut Potsdam Meeting Leibniz Association / CNRS, Berlin,
Item 2 - Information Security and Privacy Protection Technology in RFID Applications Nai-Wei Lo Assistant Professor Department of Information Management.
Dashboard upcoming features A Hales, ALMA and M Chavan, ESO
Homework #4 What is the maximum resolution of your eyes (assume the wavelength range that your eyes are sensitive to is 300 – 700 nm and that your iris.
ATACAMA CCAT : The Cornell-Caltech Atacama Telescope
The influence of Dark Energy on the Large Scale Structure Formation
Subaru Weak Lensing Survey: Hyper Suprime-Cam
Globus-M2 will be constructed by the end of 2015
Presentation transcript:

Collaboration status between ASIAA and Subaru Shiang-Yu Wang ( 王祥宇 ) Institute of Astronomy and Astrophysics Academia Sinica

Hyper SuprimeCam Fits the interests of ASIAA both in the technical and science aspects Discussions for the collaboration began in late 2006 Funding for HSC-Taiwan secured in 2008 MOU signed Oct 2008

Technical participation in HSC Mechanical Shutter (ASRD) Filter exchanger (ASRD) CCD procurement and test Lens testing system (GEOS) Data reduction software? Fit the needs of the project Learn new technology from the development Brought in the local companies to help

Mechanical shutter Major change of the allowed dimensions in Aug Prototyping stopped Activity transferred to NAOJ New prototype under tests.

Filter exchanger Separated filter exchanger unit is designed to solve the space and weight constrain

Specification for FEU Number of filters: 6 filters Minimum operational life of filter: 40,000 cycles Minimum time between maintenance: 4,000 cycles Max time between two visits in different filters: 10 min (goal 5 min) Accommodate SH filter Filter glass aperture: ϕ 600mm Filter glass thickness: 28mm position reproducibility : 50 micron Weight: 240+/-40 kg

FEU centering mechanism

Lens testing system Test the lens with two different configurations

Expected Schedule Complete detailed design of FEU in March 2009 First CCD chip to be delivered in March 2009 Lens testing system completed in Feb 2010 Delivery of FEU in mid 2010

Scientific interests Enhance the collaboration between Japanese and Taiwanese astronomers to use the Subaru telescope Participate in the HSC survey Mini workshop held in Dec 2008

Interests on HSC survey Enrich the existing research topics –Weak lensing survey (Umestu, Nishioka) –High z galaxies study (Lin, Hsieh, Wang) –GRB & SNa study (Huang, Urata) –Solar system (Abe) Synergy with on-going projects in Taiwan: –AMiBA –ALMA –TAOS –PanSTARRS

Interests on HSC survey Enrich the existing research topics –Weak lensing survey (Umestu, Nishioka) –High z galaxies study (Lin, Hsieh, Wang) –GRB & SNa study (Huang, Urata) –Solar system (Abe) Synergy with on-going projects in Taiwan: –AMiBA –ALMA –TAOS –PanSTARRS

AMiBA (Array for Microwave background Anisotropy) SZE interferometer 13 elements implemented in 2009 Increasing the photon- collecting area by a factor of ~7.4 Angular resolution is 2 arcmin (10’ FoV)

Simulated AMiBA and Subaru Surveys Subaru WL AMiBA13 SZE ng=30 arcmin^-2 zs=1  g)=0.4

TAOS (Taiwan America Occultation Survey) 4 Robotic telescopes for the search of stellar occultation by KBO and EDOs.