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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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SERVICE 

 Logvinenko Sergey Valentinovich 

General data:

Born: 11.04.1956

Place of birth: Makeyevka city, Donetsk region, Ukrainian SSR

Studied in: Moscow Institute of the Order of Lenin and the Order of the Red Banner of Labor of Railway Engineers (2019 Russian University of Transport, Moscow City) (1973-1978);

Key interests: decameter radio astronomy, astrophysics, instruments and devices. PhD Thesis: Automation of spectral radio astronomical research on the RT-22 FIAN radio telescope based on distributed control structures (1997 );


Biography:

He was born on April 11, 1956 in the city of Makeyevka, Donetsk region of the Ukrainian SSR.

After graduating from school in 1973, he entered the Faculty of Automation and Computing of the Moscow Institute of the Order of Lenin and the Order of the Red Banner of Labor of Railway Engineers.

After graduating from the institute in 1978 he joined the Pucshino Radio Astronomical Station of the Lebedev Institute of Physics, where he worked as an electronics engineer to head of the laboratory of technical sciences in 1997. He is a member of the Scientific Council of the Observatory and Astronomical Center Lebedev Institute, a member of the Scientific Council on Astronomy of the Russian Academy of Sciences in the section "Radio Telescopes and Methods".

The main area of ​​activity is the creation of radio telescope control systems, work on the development of digital receiving equipment and their integration into the control and data collection systems of radio telescopes PJSC FIAN. He is the author of more than 30 scientific papers. Constantly participates in the maintenance and modernization of the observatory's radio telescopes.

Since the 1980s, S.V. Logvinenko led several stages of modernization of the automation system of the RT-22 FIAN radio telescope. Participated in the creation of the first automation system based on the M-6000 computer, then transferred this system to the line of computers SM-2M.

In the late 1990s, together with O. Iþ Malov, D.A. Teplykh and V. Mþ Malofeev discovered radio radiation in a number of peculiar gamma and X-ray pulsars, including the famous Heming pulsar, which is very important for identifying the energy source and radiation mechanisms of these space objects.

In 1997 he defended his dissertation for the degree of Candidate of Technical Sciences in specialty 01.03.02 (astrophysics, radio astronomy) "Automation of spectral radio astronomical research on the radio telescope RT-22 FIAN based on distributed control structures." Later, using the ideology of distributed systems, they created a radio telescope control system based on IBM PC computers.

In 2010, S.V. Logvinenko supplemented the control system of the RT-22 FIAN radio telescope with the possibility of working in the international project "Radio Astron" as a ground-based monitoring station (in this status, the radio telescope has been operating successfully for over 5 years).

In recent years, S. V. Logvinenko pays a lot of attention to the development of digital receivers for observations on radio telescopes. Thus, the RT-22 radio telescope operates and manufactures under its leadership a 2048-channel digital spectrum analyzer of the autocorrelation type with a band of 50 MHz, a 2048-channel BPF-type spectrum analyzer with a band of 50 MHz with two independent inputs and an 8192-channel digital spectrum analyzer also with two independent inputs. The BSA FIAN radio telescope has a digital receiver for pulsar observations, as well as a multi-channel digital receiver for the 128-beam pattern of this radio telescope; two digital pulsar receivers are used on the DKR-1000 radio telescope for observations in two frequency bands. Since 2007, the RATAN-600 radio telescope of the Special Astrophysical Observatory has been manufactured by S.V. Logvinenko spectrum analyzer with a band of 60 MHz. He also developed a number of programs for processing the results of scientific observations, maintenance and control of radio telescopes.

He was awarded a number of diplomas of the Russian Academy of Sciences and the Diploma of the Moscow Regional Duma.




Sources:
  1  Àñòðîíîìû Ðîññèè 1917-2017/ íàó÷. ðåä. À.Ì.×åðåïàùóê, Êàçàíü, Êàçàí. ôåä. óí-ò, 2017.- 568ñ- C. 276
  2  ÌÀËÎÔÅÅ Âàëåðèé Ìèõàéëîâè÷//Àñòðîíîìû Ðîññèè 1917-2017/ íàó÷. ðåä. À.Ì.×åðåïàùóê, Êàçàíü, Êàçàí. ôåä. óí-ò, 2017.- 568ñ- C. 292

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