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DATACENTRES, DATABASES & CATALOGUES
Main actors in astronomy research in the country  There are 7 Research Institutes in the structure of the National Academy of Sciences of Ukraine (NAS of Ukraine), 2 Research Institutes in the structure of the Ministry of Education and Science, Youth and Sport of Ukraine (MESYS of Ukraine); 15 astronomical observatories and Departments in the structure of the Universities of the MESYS of Ukraine; 1 Private Astronomical Observatory play a main role in the development and teaching Astronomy in Ukraine.
 
The XPM Catalog  Absolute proper motions of 280 million stars distributed all over the sky without gaps in the magnitude range 10m < V <20m on the basis of combined data from 2MASS and USNO-A2.0 catalogues.
 
MAO NASU Plate Archive   Digital archive of MAO NAS of Ukraine (GPA) comprises data of about 26 thousands of direct photographic plates, obtained with 14 instruments in 9 observational sites, and more than 2000 digital images of different resolution available via GPA search pages.
 
Mykolaiv AO Plate Archive   Digital archive of Mykolaiv Aastronomical Observatory (MykAO) includes astronomical data obtained during observations with photo plates and CCD frames. The digitization of the archive is near its completion. Digitized images are available via a web browser and Aladin.
 
AO LNU Plate Archive   Astronomical Observatory of Lviv National University (AO LNU) is the owner of valuable archive that stores approximately 8 000 of photographic plates from 1939, including nearly 6 000 direct images of the northern sky. The archive is partly digitized and images are available via the joint search pages of AO LNU and MAO NASU.
 
IRA UTR-2 catalogue of RS   The very-low frequency sky survey of discrete sources has been obtained in the Institute of Radio Astronomy of the Ukrainian National Academy of Sciences (Kharkov, Ukraine) with the UTR-2 radio telescope at a number of the lowest frequencies used in contemporary radio astronomy within the range from 10 to 25 MHz.
 
Mykolaiv AO stellar catalogues   27 astrometric stellar catalogues of Mykolaiv Aastronomical Observatory (MykAO) in VOTable format are available for downloading
 
AO KNU Historic Plate Archive   AO KNU glass collection contains about 20 thousand photographic plates. Historical part of the archive was received during 1898-1946 and now is being digitized.
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ASTRO INFO NET
The Role of Data Science in Astronomy and Interstellar Exploration 
Space has always been a fascinating frontier for humans. From the first satellite, Sputnik 1, in 1957, to the amazing Mars rovers, our adventures in space show our love for discovery, creativity, and courage. Exploring space is a big dream, always pushing us to learn more and go further. Nowadays, data science is making a meaningful contribution to space technology. It's changing how we think about space. Being able to gather, understand, and use lots of data has helped us get to know the universe better and has changed how we explore and move through space...
 
GRID-based Virtual Observatory VIRGO.UA 
VO VIRGO.UA for cosmology and astrophysics is a segment of VO «Infrastructure»- a virtual organization, which deals with ensuring the provision of standards for Grid Services for virtual organizations, to ensure reliability functioning of the Ukrainian power grid, Grid training for users and administrators of the Grid sites, as well as the creation of technical conditions UNG for entry into the international grid community...
 
WDC-Ukraine 
WDC-Ukraine is a part of World Data Center System of the International Council of Science (ICSU). Among the basic tasks of WDC-Ukraine there is collection, handling and storage of science data and giving access to it for usage both in science research and study process. That include contemporary tutoring technologies and resources of e-libraries and archives; remote access to own information resources for the wide circle of scientists from the universities and science institutions of Ukraine...
 
IVOA NEWSLETTER
US VAO Data Discovery Portal 
Find datasets from thousands of astronomical collections known to the VO and over wide areas of the sky. This includes important collections from archives around the world. Feedback on your experience with the tool is appreciated -- please send your comments, suggestions, and questions to the VAO Help Desk.
 
US VAO Cross-Comparison Tool 
Perform fast positional cross-matches between an input table of up to 1 million sources and common astronomical source catalogs, such as 2MASS, SDSS DR7 and USNO-B. Feedback on your experience with the tool is appreciated -- please send your comments, suggestions, and questions to the VAO Help Desk.
 
VOPlot v1.8 Beta 
VOPlot v1.8Beta includes many enhancements and bug fixes. To name a few v1.8Beta supports multi-grid plots for 2D Scatter-Plot which allows the user to have multiple plots having grid size from 1x1 to 3x3 in a single window. Paginated view is added to see data in tabular format which allows user to navigate systematically. Provision to label Lat/Long lines is also added. Users can now plot a cumulative histogram for all histogram types. VOPlot 1.8Beta shows the metadata of a FITS file instantaneously while the actual loading happens in background. VOPlot v1.8Beta also provides better handling of "faulty data" while parsing an ASCII file.
 


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 Berczik Peter Peterovich 

General data:

Born: 16.09.1964

Place of birth: Uzhhorod city, Transcarpathian region, Ukrainian SSR

Studied in: T. G. Shevchenko Kyiv Order of Lenin and the Order of the October Revolution State University (since 1999 Taras Shevchenko Kyiv National University) (1989);

Key interests: astrophysics, physics of extragalactics, radiophysics. PhD Thesis: Triaxial models of large-scale gas formation in galaxies (1993 Main Astronomical Observatory of the National Academy of Sciences of Ukraine); ScD Thesis: Self-consistent simulation of the chemical and dynamic evolution of galaxies (2010 Main Astronomical Observatory of the National Academy of Sciences of Ukraine);


Biography:

He was born September 16, 1964 in Uzhhorod city of Transcarpathian region of Ukrainian SSR on the border with Hungary.

In 1989 graduated from T. G. Shevchenko Kyiv Order of Lenin and the Order of the October Revolution State University.

in 1993 defended his Ph.D. thesis "Three-dimensional models of large-scale gas formations in galaxies" majoring in astrophysics, radio astronomy in Main Astronomical Observatory of the National Academy of Sciences of Ukraine.

In 1994, he became the head of the Astro-Space Information and Computing Center, which was created on the basis of the computer-measurement center of the Main Astronomical Observatory of the National Academy of Sciences of Ukraine.

Since the end of September 1995 he has been working at the Main Astronomical Observatory of the National Academy of Sciences of Ukraine as Senior Researcher.

In 2000, 2003 he was elected to the Council of the Ukrainian Astronomical Association.

In 2010 (according to other data in 2009), he defended a doctoral dissertation in the Main Astronomical Observatory of the National Academy of Sciences of Ukraine on the specialty "01.03.02 - Astrophysics, Radio Astronomy" on the topic "Self-consistent modeling of chemical and dynamic evolution of galaxies".

Since January 1, 2012 he has been working as a Deputy Director of Main Astronomical Observatory of the National Academy of Sciences of Ukraine for scientific work.

In 2014, he became the laureate of the State Prize of Ukraine in the field of science and technology for the work "The structure and evolution of the universe on the galactic and cosmological scales, the latent mass and dark energy: theoretical models and observational results" among the co-authors.

Since 2019 he headed the Department of Physics of Stars and Galaxies of Main Astronomical Observatory of the National Academy of Sciences of Ukraine.

He is actively working at the university observatories of USA, Germany, China and Japan.

The frequency of interaction of globular clusters (several tens of passes per billion years within the central zone of 100 pc) with the center of the Galaxy, found in 2023 by employees of the Department of Physics of Stars and Galaxies of the Main Astronomical Observatory of the National Academy of Sciences of Ukraine M.V. Ishchenko, M.O. Sobolenko and P.P. Bertzik, turned out to be such that it does not explain the relative high mass of the nuclear star cluster of the Galaxy. Several tens of globular clusters of galaxies are likely to experience several close encounters and even possible collisions during their lifetime, which can significantly affect their individual dynamical evolution and possibly even their stellar content.




Main publications:
  1. Жук О. І., Новосядлий Б. С. Будова та еволюція Всесвіту на галактичних та космологічну их масштабах, прихована маса і темна енергія: теоретичні моделі та спостережні результати.- 10с.
  2. Shulga V.M., Zhdanov V.I., Alexandrov A.N., Berczik P.P., Pavlenko E.P., Pavlenko Ya.V.,Pilyugin L.S., Tsvetkova V.S. Dark energy and dark matter in the Universe: in three volumes / Editor V. Shulga. — Vol. 2. Dark matter: Astrophysical aspects of the problem. Publisher: K. : Akademperiodyka, 2014. — 356 p.
  3. САМОУЗГОДЖЕНЕ МОДЕЛЮВАННЯ ХІМІЧНОЇ ТА ДИНАМІЧНОЇ ЕВОЛЮЦІЇ ГАЛАКТИК/Берцик П. П. автореф. докт. дис. - К.: 2010.
  4. Берцик Петер Петерович. Трехосные модели крупномасштабных тазовых образований в галактиках : Дис...канд.физ.-мат.наук: 01.03.02 / АН Украины. — К., 1992. — 133с.



Sources:
  1  aspirant.kiev.ua
  2  aspirantura.org.ua
  3  mao.kiev.ua
  4  lib.ua-ru.net

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