IVOA Executive Committee Meeting (FM32)

Sun May 24 2009 @ 16.00-18.00 CST

Logistics

Full Meeting: Salle de réunion - see website at http://cdsweb.u-strasbg.fr/interop2009/index.html

Agenda

1. Roll Call and Agenda
2. Minutes of TM31
3. Review of Actions
4. Approval of new IVOA Recommendation(s) [Standing Item]
5. ...
6. ...
7. ...
8. ...
9. Future Interop meetings
10. Schedule of other IVOA-related events (all)
11. Data and Venue of the next Exec meeting (telecon?)
12. AOB
13. Summary of Actions

Reports from the Projects

ArVO

Armenian Virtual Obesrvatory (ArVO), report 2009.05.17

ArVO group members at present are: A.M. Mickaelian (Principal Investigator), H.V. Astsatryan (Technical Manager), T.Yu. Magakian and L.K. Erastova (Project Scientists), L.A. Sargsyan, P.K. Sinamyan, and S.A. Ghazaryan (Scientific/Technical Assistants), and G.A. Mikayelyan (Web Master). Two more students from the Yerevan State University (YSU) are involved in the project, too.

Using the computer hardware (ArmCluster) and software possibilites at the Armenian Institute of Informatics and Automation Problems (IIAP), we have installed the full Digitized First Byurakan Survey (DFBS) database in Armenia, which is the copy of the same database created by the M.I.G.G. team in Rome and will serve for the Armenian students to work on new science projects. The Armenian VO server at the IIAP has been set up and soon will be open. The establishment and utilization of the Virtual Observatories standards in Armenia is being continued.

One of the recent works was the creation of Byurakan Observatory electronic plate database (BPD v1 contains data for some 11,000 plates) with full access by various parameters: sky area, observing project, telescope, observing mode, data of observations, observer, etc. The digitization works of the Byurakan archive plates are being continued. The digitized Byurakan plates will make up the main part of the Armenian astronomical data centre.

The low-dispersion spectra classification works have been started, too. It is planned that the users will have access to all 40,000,000 spectra and their suggested classification, which will allow to select objects of necessary types, make samples, study definite fields, etc. Developments for conducting scientific projects using the DFBS are in progress, including automatic search for UVX and late-type stars, variable objects, and new bright QSOs, optical identifications of radio, IR, and X-ray sources.

A new ISTC project (A-1606) on "Development of Armenian-Georgian Grid Infrastructure and applications in the Fields of High Energy Physics, Astrophysics and Quantum Physics" has been conducted in collaboration with 6 other Armenian and Georgian institutions, which includes the development of Armenian-Georgian VO based on the plate databases of Byurakan and Abastumani observatories.

AstroGrid

Australia-VO

Brazil-VO (BVO)

China-VO

CVO

VObs.it (aka DRACO) Italy

Euro-VO

France VO

GAVO

HVO

Japan-VO

Korean VO

NVO

RVO

SVO

VO-India

Reports from WGs & IGs(follows order as at http://www.ivoa.net/forum/)

Applications WG

Data Access Layer WG

Data Models WG

Grid and Web Services Working Group

Registry WG

Semantics/UCD WG

VOEvent

VOQL WG

VOTable WG

Astro-RG IG

Data Curation and Preservation IG

Theory IG

Stds & Process

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