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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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 Moiseyev Ivan Grigorovich 

General data:

31.07.1921 - 16.10.2008

Studied in: Moscow Order of Lenin Energy Institute (since 2005 Federal State Budget Educational Institution of Higher Education "National Research Institute" MEI "", Moscow City) (1953);

Key interests: decameter radio astronomy, astrophysics, extragalactic astronomy, solar physics, instruments and devices


Biography:

He was born on July 31, 1921.

In 1953 he graduated from the Moscow Energy Institute with a degree in radio engineering and in the same year by distribution he was sent to the Crimean Astrophysical Observatory of the USSR Academy of Sciences to the position of junior non-researcher. He worked his way up to the head of the department.

In 1963 he defended his dissertation for the degree of Candidate of Physical and Mathematical Sciences at M. V. Lomonosov Moscow State University.

Together with Vvedensky V. A., Pogribny B. M., Semenov Y. M., Stezhka P. M. developed a modernized control system for a 22-meter radio telescope of millimeter waves in the Crimean Astrophysical Observatory of the then USSR Academy of Sciences on the basis of computers. In the automatic mode, which is the main, the drives of fast movement on the computer command perform the re-installation of the antenna during the transition from one object of observation to another and rough aiming of the antenna at the source. Slow motion devices perform accurate guidance and observation of the selected object, the motion of which is also set by the computer.

Together with Skulachev D. P., Nesterov M. S., Efanov S. V., Strukov I. A., Korogod V. Vю conducted observations in early 1986 on a wave of 8.2 mm 171 radio sources with a limit of about 0 , 1 Jan (3σ).

He died on October 16, 2008 in the Katsiveli urban village.

The main scientific works relate to the fields of astrophysics, solar physics. He is one of the founders of radio astronomy at the Crimean Astrophysical Observatory. With his participation in 1955 the first radio telescope of the meter wave range was made at the Crimean Astrophysical Observatory, on which regular observations of the Sun were started. In 1957 he headed the first radio astronomy group. To study the lower layers of the solar atmosphere in 1956 began to make a second radio telescope at 10 cm, test observations which began to be conducted in 1957. Radio astronomical methods of observation gave new, previously unknown, information about the upper layers of the solar atmosphere, limited availability. The next radio astronomical instrument of the Crimean Astrophysical Observatory in 1957 was a radio spectrograph operating in the range from 2 to 3 m. flashes. and with flares and other rapidly changing optical processes in the Sun.

He headed the Department of Radio Astronomy established at the Crimean Astrophysical Observatory since 1962. With his participation in 1966, the 22-meter RT-22 radio telescope was built and put into operation in Simeiz, one of the five best instruments in the world. Research has been launched:

a) the study of solar radiation in a wide range of waves up to millimeters,

b) observation of the variability of galactic and extragalactic sources of radio radiation,

c) measurement of ultrafine structure of compact sources of cosmic radio radiation by the method of radio interferometry with ultralong bases.

In 1969 he participated in the organization and conduct of the first intercontinental observations on RT-22 by radio interferometry with ultralong bases for the study of the size and ultrafine structure of cosmic radio sources. The experiment was successful, on the basis of Crimea-Hystek (USA) a record angular resolution of 0.0004 "was obtained.

In 1987 he was awarded the USSR State Prize for work in the field of radio engineering. He is the author of about 50 scientific papers.




Main publications:
  1. Модернизированная система управления РТ22 КАО /Введенский В. А., Моисеев И. Г., Погребной Б.М., Семенов Ю. Н., Стежка П. Н.// Изв. Крым. астофиз. обсерв., 1988, 78, С. 201-205
  2. Наблюдения на волне 8,2 мм. с высокой чувствительностью полной выборки фнегалактических радиоисточников/ Моисеев И. Г. , Нестеров Н. С., Ефанов С. В. , Струков И. А., Корогод В. В., Скулачев Д. П.//Изв. Крым. астофиз. обсерв. , 1988, 78. С. 112-122
  3. Extreme kinematic misalignment in IllustrisTNG galaxies: the origin, structure and internal dynamics of galaxies with a large-scale counterrotation/Sergey Khoperskov, Igor Zinchenko, Branislav Avramov, Sergey Khrapov, Peter Berczik, Anna Saburova, Maryna Ishchenko, Alexander Khoperskov, Claudia Pulsoni, Yulia Venichenko, Dmitry Bizyaev, Alexei V. Moiseev,2020.-p 20



Sources:
  1  Реферативный журнал. 51 астрономия., М.: ВИНИТИ, 1988, №12, С.148, 162
  2  Астрономы России 1917-2017/ науч. ред. А.М.Черепащук, Казань, Казан. фед. ун-т, 2017.- 568с- C.317

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