260 likes | 268 Views
Drivers, Status and Planning. Overview. The need for a new research infrastructure in astronomy AVO Work Program Status Future The International VO Alliance. The winds of change.
E N D
Drivers, Status and Planning P.Quinn TIVO June10-14 2002
Overview • The need for a new research infrastructure in astronomy • AVO • Work Program • Status • Future • The International VO Alliance P.Quinn TIVO June10-14 2002
The winds of change “Internet computing and Grid technologies promise to change the way we tackle complex problems. They will enable large-scale aggregation and sharing of computational, data and other resources across institutional boundaries. And harnessing these new technologies effectively will transform scientific disciplines ranging from high-energy physics to the life sciences.” Dr. Ian Foster, Co-leader GLOBUS Project P.Quinn TIVO June10-14 2002
Particle Physics Problems CMS ATLAS ~8-10 PetaBytes /year/on tape ~1 PetaByte/year/on disk ~8000 kSI95 (~300,000 PC2000) The LHC Detectors LHCb P.Quinn TIVO June10-14 2002
What has this to do with astronomy? • Astronomy has become a BIG international science • Gemini, VLT, ALMA, SKA, NGST, ELTs • Astronomy projects involve • International coordinated research efforts • Distributedmulti-wavelength teams, resources and data • Data volumes with doubling times < 12 months • Astronomy service organizations need to • provide their communities with access to software tools, high quality raw and processed data in the face of desktop computing power and network bandwidths with doubling times > 18 months P.Quinn TIVO June10-14 2002
T2 < 12 months Science Data Volume ESO/STECF Science Archive Facility P.Quinn TIVO June10-14 2002
Projected Growth T2 < 12 months P.Quinn TIVO June10-14 2002
VO Astronomical Strategies PROBLEM SOLUTION Slow CPU growth Distributed Computing Limited storage Distributed Data Limited bandwidth Information Hierarchies - Move only what you need Data diversity Interoperability P.Quinn TIVO June10-14 2002
3675440 5075 491854017 1092374 954229.737 years 1662.448 years 1.502416e+21 4.260259e+18 49.31 TFLOPs/sec Distributed Computing at Work • Virtual and collaborative exploration of the Universe Total Last 24 Hours Users Results received Total CPU time Floating Point Operations P.Quinn TIVO June10-14 2002
Information Society Technologies GRID startups (today~40M Euro) [3.6B Euro 2003-2007] Applications EGSO GRIA CROSSGRID AVO EUROGRID GRIP GRIDLAB GRIDSTART DATAGRID Middleware& Tools DAMIEN DATATAG Underlying Infrastructures Industry / business Science An Integrated European Approach P.Quinn TIVO June10-14 2002
The AVO Proposal • EU RTD Proposal submitted 15 February 2001 following OPTICON recommendations for a European VO effort (similar effort in the US [NVO] proposed by Decadal Report) • ESO PI (Quinn) + STECF(Benvenuti), CDS (Genova), TERAPIX (Mellier), ASTROGRID (Lawrence) and Jodrell Bank (Diamond) + NVO affiliates • Asked for funds for a three year Phase-A study of an Astrophysical Virtual Observatory – 7.2 Million € (50% from EU and 50% from organizations) • Focus on • Multi-wavelength science case demonstrations (ASTROVIRTEL basis) • Interoperability demonstrations (CDS/All) • Technology assessments and testbeds (ASTROGRID/ESO) P.Quinn TIVO June10-14 2002
AVO STATUS • AVO approved with EU funds ~2 Million € (total budget ~ 4M €) • Contract start on 15 November 2001 - 3 Year Phase A study • 9 NEW POSITIONS for 3 years over 6 institutions - total 18 FTE (~ 50 people) • Total VO funding AVO+NVO+ASTROGRID = $21 million (US) • 3 Year target : • Build VO 1.0 among the 6 partner archive sets by • Defining and executing trial science cases • Defining, developing and deploying new interoperability standards and tools • Developing and deploying new Grid-based services P.Quinn TIVO June10-14 2002
AVO Work Program P.Quinn TIVO June10-14 2002
AVO Science WG Selection of preliminary science cases in June’02 See Piero’s talk on ASTROVIRTEL development P.Quinn TIVO June10-14 2002
Interoperability • Major step forward : VOTable 1.0 • See F.Ochsenbein talk P.Quinn TIVO June10-14 2002
Technology • Scalable storage and computing (see talk by Andreas Wicenec on NGAST) • Web services prototypes (ASTROGRID talk by Andy Lawrence) • Tool prototypes : QUERATOR (talk by F. Pierfederici) P.Quinn TIVO June10-14 2002
VO Challenges AVO: the promise Bob Fosbury JENAM 2001 (1) To take the data collected by teams for specific projects and manage/massage it in such a way as to be of general use Comments - • If the data in an archive are neither well-calibrated nor well-described, they are of little value for the AVO • If the data are in good order, the AVO is unnecessary — it is just a layer of middle-men • If I were a funding agency, why should I support the ‘middle-man’ when I could fund the original science project? P.Quinn TIVO June10-14 2002
A VO RoadmapQuinn ADASS’01 • To address Bob’s comments the international VO effort needs to define a unified and astronomically accepted roadmap for the next three years • Without a publicly visible direction, accountability and receptiveness to requirements we will fail - • This roadmap must be in defined/produced by the next international VO meeting P.Quinn TIVO June10-14 2002
The International Virtual Observatory Alliance P.Quinn TIVO June10-14 2002
IVOA • IS NOT ANOTHER PROJECT • IS an alliance of existing and future national and international projects to • Define the common ground needed to make an operational and scientifically effective IVO • Reach agreement on standards and interoperability • Allow the international scientific communities resident in the national projects, and elsewhere, a global channel for comment, criticism and guidance P.Quinn TIVO June10-14 2002
An Agreed Roadmap - 1 January 2002Initiate international dialog on interoperability. OPTICON Interoperability Working Group meeting, Strasbourg. + Discussion/revision draft VOTable std. April 15, 2002 Reach agreement on VOTable 1.0. June 10-14, 2002 Formation of IVOA P.Quinn TIVO June10-14 2002
Early Progress • VOTable: A Proposed XML Format for Astronomical Tables • Roy Williams, California Institute of Technology, USA NVO • François Ochsenbein, Observatoire Astronomique de Strasbourg, France AVO • Clive Davenhall, University of Edinburgh, UK AVO • Daniel Durand, Canadian Astronomy Data Centre, Canada CADC • Pierre Fernique, Observatoire Astronomique de Strasbourg, France AVO • David Giaretta, Rutherford Appleton Laboratory, UK STARLINK • Robert Hanisch, Space Telescope Science Institute, USA NVO • Tom McGlynn, NASA Goddard Space Flight Center, USA NVO • Alex Szalay, Johns Hopkins University, USA NVO • Andreas Wicenec, European Southern Observatory, Germany AVO • Version 1.0 (15 Apr 2002) • Document repository: http://cdsweb.u-strasbg.fr/doc/VOTable/ • Comments: VOTable@us-vo.org P.Quinn TIVO June10-14 2002
An Agreed Roadmap - 2 January 2003Coordinated initial science demonstrations by IVOA members January, 2003 IVOA agreement on initial suite of interoperability Standards and tools May 2003 Working Published Web Services August 2003 Coordinated intermediate science demonstrations including international access at IAU General Assembly P.Quinn TIVO June10-14 2002
An Agreed Roadmap - 3 October 2003 Astronomical Query Language January 2004 Coordinated intermediate demonstrations + Grid May 2004 Resource Discovery 1.0 July 2004 IVO 2005+ roadmap October 2004 Compound Web Services and Ontology Service 1.0 January 2005 Coordinated complex science demonstrations P.Quinn TIVO June10-14 2002
An Invitation The ASTROGRID, AVO and NVO projects take the opportunity of the Munich VO meeting to formally announce the IVOA and would like to extend an invitation to all VO projects to join this alliance for the pursuit of an international virtual observatory and the expansion of astronomical research capabilities in the 21st century. P.Quinn TIVO June10-14 2002
ESO Archive Policy http://archive.eso.org/Archive_Access_Policy.html ESO is fully aware of the importance of international collaborations in achieving the scientific goals and break-throughs necessary for astronomy to advance in the 21st century. The scientific potential of facilities like ALMA and OWL will only be realized by coordinated international efforts and the free exchange of astronomical ideas and data. To this end, ESO is preparing to provide open international access to all its archival data. Before this can happen, the ESO data holdings must be of a uniform high quality, in a form appropriate for recalibration and archival research and be supported by adequate operational manpower. ESO is taking the lead in Europe in defining data quality and interoperability standards through its coordination and funding efforts for an Astrophysical Virtual Observatory. The aim of the AVO is to provide the European and global astronomical community with an archival and data handling resource that can meet the needs of 21st century astronomy. The AVO program aims to join data from ESO telescopes with space and ground archives from Europe in an AVO Phase A facility by the end of 2003. From this time, ESO data will start to become freely available to the international astronomical community in a phased manner, following standards for data centers in the global virtual observatory and the availability of new VLT instruments. P.Quinn TIVO June10-14 2002