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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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 Belyakina Tamara Sergeevna 

General data:

14.01.1934 - 13.06.2016

Place of birth: Arsentievsky Vysilky village, Central Chernozem region, Russian Soviet Federative Socialist Republic (now Stanovlyansky district, Lipetsk region, Russian Federation)

Studied in: M. V. Lomonosov Moscow State University (1950-1956);

Key interests: stellar catalogues, non-stationary stars, stellar systems. PhD Thesis: Photometric studies of symbiotic stars (1972 );


Biography:

She was born on January 14, 1934 in the Arsentievsky Vysilki illage of Central Chernozem region of the Russian Soviet Federative Socialist Republic (now Stanovlya district of Lipetsk region of the Russian Federation).

In 1950 she graduated from high school in Pavlovsky Posad, Moscow region and entered the astronomy department of MV Lomonosov Moscow State University. After graduating from university in 1956 she was sent to work at the Crimean Astrophysical Observatory, where she spent her entire working life.

She was hired in the Department of Vision Physics, T. S. Belyakina participated in compiling catalogs of photovoltaic quantities and colors close to the Sun of stars and in determining the true dispersion of colors on a two-color chart in the UBV system. In the course of these works, she mastered all the intricacies of stellar electrophotometry. Then T. S. Belyakina took part in the spectral and spectrophotometric studies of New Hercules in 1960 and in the development of criteria for the spectral classification of metal stars (in particular, she together with the staff of the observatory I. M. Kopylov and E,. A. Vitrichenko performed a quantitative spectral classification for 26 "metal" Ami 23 standard stars of luminosity classes II-V in the spectral range A2-F5), thus mastering the technique of spectroscopic research. As a result, it was formed as an independent and multifaceted researcher of non-stationary stellar objects.

In the 1960s, T. S. Belyakina has done a long series of work on electrophotometry of symbiotic stars, which formed the basis of her PhD thesis "Photometric studies of symbiotic stars", successfully defended in 1972. These studies were included in the concept of symbiotic stars and other close binary systems in the later stages.

In the following years, T.S. Belyakina continued photometric and colorimetric studies of various nonstationary and peculiar objects: many symbiotic stars and related objects, New Swan 1975, PU Vul (Kuvano-Honda object), double system XX Oph, myrid NM and FG Sgr . Numerous publications on estimating the parameters of the components of these systems and tracking their variation over time have been devoted to many symbiotic stars, the XX Oph system, and especially PU Vul. The number of works published by T. S. Belyakina in Soviet and foreign publications exceeds six dozen.

She died on June 13, 2016 in the Nauchniy village.




Main publications:
  1. Belyakіna T.S., Bondar N.І., Chochol D., Chuvaev K.K., Efіmov Y.S., Gershberg R.E., Grygar J., Hrіc L., Krasnobabtsev V.І., Shakhovskoj N.N., Shenavrіn V.І. Kuwano-Honda pecular object (PU Vul) // Astron. and Astrophys. –1984. – V.132. – P.L12–L14.
  2. Белякина Т.С., Бондарь Н.И., Гершберг Р.Е., Ефимов Ю.С., Краснобабцев В.И., Петров П.П., Саванов И.С., Чуваев К.К., Шаховская Н.И., Шаховской Н.М., Шенаврин В.И. Исследование пекулярного объекта Кувано-Хонда (PU Vul). І. // Известия Крымск. астрофиз. обс. – 1985. – Т.72. – С.3–72.
  3. Belyakіna T.S., Bondar N.І., Chochol D., Chuvaev K.K., Efіmov Y.S., Gershberg R.E. , Grygar J., Hrіtz L., Krasnobabtsev V.І., Pііrola V., Poutanen M., Savanov І.S., Huovelіn J., Tuomіnen І., Shakhovskaya N.І., Shakhovskoj N.N., Shenavrіn V.І., Shcherbakov A.G. The Kuwano-Honda’s pecular object (PU Vulpeculae) іn 1983 -1986 // Astron. and Astrophys. – 1989. – V.223. – P.119–135.
  4. Белякина Т.С., Бондарь Н.И., Гершберг Р.Е., Гриц Л., Грыгыр Г., Ефимов Ю.С., Краснобабцев В.И., Пиирола В., Поутанен М.., Саванов И.С., Туоминен И., Хохол Д., Чуваев К.К., Шаховская Н.И., Шаховской Н.М., Шенаврин В.И., Щербаков А.Г. Исследование пекулярного объекта Кувано-Хонда (PU Vul). ІІ. // Известия Крымск. астрофиз. обс. – 1990. – Т.81. –С.28–112



Sources:
  1  Телескоп Zeiss-50 в Крыму. II/Т.М. Рачковская//Изв. Крымской Астрофиз. Обс. 109,No 2, С. 119(2013)
  2  Астрономы России 1917-2017/ науч. ред. А.М.Черепащук, Казань, Казан, фед. ун-т, 2017.- 568с- C.50

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