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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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 Busarev Vladimir Vasilyevich 

General data:

Born: 1955

Place of birth: Alexandria city, Kirovohrad region, Ukrainian SSR

Studied in: M. V. Lomonosov Moscow State University (1977-1983);

Key interests: minor bodies of the Solar System, photometry, exploration of the Moon. PhD Thesis: Remote search for ilmenite-containing rocks on the Moon (1989 ); ScD Thesis: Study of the nature of asteroids by spectrophotometry (2012 );


Biography:

He was born in 1955 in the city of Alexandria city of Kirovograd region of the Ukrainian SSR.

During 1977-1983 he studied at the Faculty of Physics of M. V. Lomonosov Moscow State University.

During 1985-1988 he studied at the graduate school of the Faculty of Physics of M. V. Lomonosov Moscow State University.

Since 1989 he has grown from a junior to a leading researcher at the P. K. Sternberg State Astronomical Institute of M. V. Lomonosov Moscow State University.

In 1989 he defended his dissertation on "Remote search of ilmenite-containing rocks on the Moon" in "Astrophysics and stellar astronomy".

In 2012 he defended his doctoral dissertation on "Study of the nature of asteroids by spectrophotometry".

Scientific work began during his student years in the Department of Moon and Planetary Research of the P. K. Sternberg State Astronomical Institute of M. V. Lomonosov Moscow State University on the study of the Moon: study of photometric characteristics of the lunar surface on panoramic images "Moonlight-2"; performing spectral photographic observations of the Moon at the Central Asian Observatory of the P. K. Sternberg State Astronomical Institute, digital processing of the obtained images and their use to build distributions on the lunar surface of rocks that have resource value for the future lunar base.

In 1989 he began spectrophotometric observations of asteroids in the Main Belt, as well as the study of the characteristics of minerals, rocks and meteorites that are analogs of the matter of asteroids. In 2003, based on the study of the spectra of reflection of trans-Neptunian objects and analysis of data on the composition of cometary and meteorite matter, together with A.B. Makalkin (OY Schmidt Institute of Earth Physics, Russian Academy of Sciences) and V. A. Dorofeeva (V. I. Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences) bodies (more than 200 km) in the early solar system beyond the condensation of water ice due to the decay of short-lived (26<\sup>Al, etc.) for the first few million years.

Together with V. V. Prokofieva-Mikhailovskaya (Crimean Astrophysical Observatory) developed a new spectral-frequency method for studying asteroids and other non-atmospheric celestial bodies on a fairly long series of reflection spectra obtained during successive phases of rotation of each object. This method was able to establish the inhomogeneous distribution of carbonaceous-chondrite material and hydrosilicates (in the absorption band Fe3+<\sup>) on the asteroid 21 Lutetia, the object of study of the Rosetta spacecraft (ESA).

In 2011, he hypothesized the origin of primitive C-asteroids (and related types) and carbonaceous chondrites as fragments of stone-ice bodies from the zone of Jupiter's formation that underwent primary thermal evolution (with the collapse of 26<\sup>Al and other short-lived isotopes) and aqueous differentiation, and then ejected by Jupiter, in particular, in the main belt of asteroids. V.V. Busarev confirmed this hypothesis (spectral signs of the presence of atypical types of atypical hydrosilicates on asteroids). In 2011, similar features were found in the study of 4 Vesta (asteroid of basaltic composition) using the Dawn spacecraft (NASA).

He is currently engaged in spectrophotometry of asteroids approaching the Earth in order to study the chemical and mineral composition, possible origin and previous evolution of their matter.




Main publications:
  1. Solar analog spectra in asteroid observations / V. V. Bochkov, V. V. Busarev, L. G. Karachkina et al. // JENAM-2000: 9th European and 5th Euro-Asian Astronomical Society conference: abstracts. — Moscow, 2000. — P. 115—222.
  2. В. В. Бусарев, В. В. Прокофьева-Михайловская, В. В. Бочков, “Спектральный и спектрально-частотный методы исследования безатмосферных тел Солнечной системы”, УФН, 177:6 (2007), 663–675



Sources:
  1  Астрономы России 1917-2017/ науч. ред. А.М.Черепащук, Казань, Казан, фед. ун-т, 2017.- 568с- C.71

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