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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.
Australia-VO
Brazil-VO (BVO)
China-VO
CVO
VObs.it (aka DRACO) Italy
Euro-VO
The first European “hands-on” VO School was held at ESO Mar. 30 – Apr. 2, 2009 as part of the activities of the Euro-VO AIDA project (see http://www.euro-vo.org/aidahandson2009/). The aim of the school, targeted mostly at PhD students and young post-docs, was to expose European astronomers to the many available VO tools and services so that they could be used efficiently for research purposes. The school involved 40 students, out of the 75 who requested to participate, and 15 tutors and tool developers. Based on the input received from the participants during the hands-on and feedback sessions the school was a great success.
France VO
GAVO
HVO
Japan-VO
Korean VO
NVO
RVO
SVO
VO-India
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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