IVOA SPM 2006, Moscow1 History and current status Chenzhou CUI National Astronomical Observatories, Chinese Academy of Sciences The Chinese V IRTUAL O BSERVATORY
IVOA SPM 2006, Moscow2 Content Infrastructure and facilities in CAS Principles and goals for the China-VO Activities and outputs Future directions Roles of small VO projects
IVOA SPM 2006, Moscow3 IT infrastructure in CAS 2001 year2005 year Network Core net bandwidth 1Gbps2.5Gbps Backbone net bandwidth 2MbpsN*155Mbps+5Gbps International Links 55Mbps620Mbps+17.5Gbps Computing and Storage Rpeak 0.13 TFlop/s 5.3 TFlop/s Storage 2.1TB182TB Rmax 0.05 TFlop/s4.193 TFlop/s
IVOA SPM 2006, Moscow4 Lenovo 6800 Rank124 SiteCAS ManufacturerLenovo Computer DeepComp 6800, Itanium2 1.3 GHz, QsNet CountryChina Year2003 Processors1024 Rmax4193 Rpeak Nmax Nhalf0 Operating SystemLinux ArchitectureCluster
IVOA SPM 2006, Moscow5 NAOC –Beijing –Changchun –Urumchi –Kunming Purple Mountain Obs. (Nanjing) Shanghai Obs. –Qinghai Station Observatories in CAS Optical: 2.4m Radio: 50m
IVOA SPM 2006, Moscow6 Development of China-VO Advanced research platform for Chinese astronomers Import data and technologies from IVOA partners Share Chinese datasets with international astronomers Bring up a group of VO-oriented astronomers, engineers and students Education outreach
IVOA SPM 2006, Moscow7 R&D Focuses China-VO Platform Uniform Data Access System VO-compliant projects VO-enabled facilities VO-based Public Education
IVOA SPM 2006, Moscow st VO workshop in China “ China-VO ” kicked off “ China-VO ” became a member of the IVOA China-VO system design the 2nd VO workshop IVOA Small Projects Meeting VOFilter 1.0 released China-VO VOFilter 2.0 released China-VO VO-DAS project began SkyMouse 1.0 released China-VO IVOA interoperability meeting, Beijing History and Events
IVOA SPM 2006, Moscow9 China-VO Meeting (2001, Beijing) VO is important, we should involve…
IVOA SPM 2006, Moscow10 China-VO in 2002 “China-VO” initiated China-VO PI (Yongheng Zhao) attended the VO conference in Garching, ESO Dr. Jim Gray (NVO, Microsoft Research) visited the China- VO China-VO became a member of the IVOA
IVOA SPM 2006, Moscow11 China-VO 2003, Beijing
IVOA SPM 2006, Moscow12 Small project meeting, Beijing November 2003: Beijing, China Main topics: –Advantages and disadvantages of small projects. –The role of small projects in the IVOA. –R&D focus of small projects. –Collaboration among small projects and with big VO projects. –Implementation of IVOA standards and infrastructures developed by other VO projects. 39 participants from Korea, Japan, India, Europe, UK and China (including Taiwan)
IVOA SPM 2006, Moscow13 Brief Review
IVOA SPM 2006, Moscow14
IVOA SPM 2006, Moscow15 China-VO 2004, Wuhan, Hubei
IVOA SPM 2006, Moscow16 China-VO 2005 (Weihai, Shandong)
IVOA SPM 2006, Moscow17 China-VO 2006 Theme: the coming e-science era for astronomy research Date: November 29th – December 3rd Place: Guangxi Normal Univ., Guilin, Guangxi
IVOA SPM 2006, Moscow18 China-VO Architecture
IVOA SPM 2006, Moscow19
IVOA SPM 2006, Moscow20 Two XSLT transforms VOFilter –an XML filter for OpenOffice.org Calc to open VOTable files – VOTable2XHTML –a stylesheet to transform VOTable data into HTML/XHTML format –
IVOA SPM 2006, Moscow Touch the sky with your mouse An intelligent client for VO services A commodity for astronomers and students A Smart On-line Astronomical Information Collector
IVOA SPM 2006, Moscow22 VO Data Access Service (VO-DAS) Based on comparative mature Grid middle-wares, for example Globus Toolkit and OGSA-DAI, the VO-DAS system will provide VO-compliant, uniform access interfaces for different kinds of astronomical resources existing as VO services, databases, file systems and even data mining algorithms and other applications. From Aug 14th, VO-DAS project has been turned from design stage to coding stage. A preview version will be available by the end of the year. The first public release will be in the IVOA 2007 Spring Interoperability meeting.
IVOA SPM 2006, Moscow23 VO-DAS
IVOA SPM 2006, Moscow24 Astrophysical Integrated Research Environment (AIRE) Provide a web-based collaborative research environment Radio : Interferometry …, AIPS, AIPS++, Difmap… Optical : Photometry …, IRAF, MIDAS … X-ray : Coded-mask …, HEADAS …. Contributed by Tsinghua University
IVOA SPM 2006, Moscow25 Partners National Astronomical Observatories (NAOC) Purple Mountain Astronomical Observatory (Nanjing) Shanhai Astronomical Observatory Tsinghua University Peking University Beijing Normal University Nanjing University University of Science and Technology of China Beijing Planetarium Huazhong Normal University Computer Network and Information Center, CAS Tianjing University
IVOA SPM 2006, Moscow26 Topology
IVOA SPM 2006, Moscow27 Roles of Small VO Projects a.Bridging a)Bridging IVO Standards and Best Practice b)Bridging VO and Domestic Community b.Servicing a)User training b)VO-enabled projects
IVOA SPM 2006, Moscow28 Large sky Area Multi-Object fibre Spectroscopy Telescope Clear aperture: 4m Field of view: 5° Focal plane: 1.75m Focal length:20m Number of fibers:4000 Spectral ranges:370 ~ 900nm Spectral resolution:1 ~ 0.25nm Sky coverage:Declination -10 to+90 A meridian reflecting Schmidt telescope VO-enabled LAMOST
IVOA SPM 2006, Moscow29 VO-enabled LAMOST VO-enabled –LAMOST data –LAMOST Spectral Analysis Pipeline
IVOA SPM 2006, Moscow30 Beijing-Arizona-Taiwan-Connecticut Sky Survey Started in 1995 data archived on CD- ROM and hard disks 700 GB images 0.6/0.9 m Schmidt telescope 15 intermediate-band filters
IVOA SPM 2006, Moscow31 Catalog is available at VizieR now Image archive access system is under developing BATC Data Release Current Interface
IVOA SPM 2006, Moscow32 Q & A ? The Chinese V IRTUAL O BSERVATORY