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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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 Astapovich Igor Stanislavovich 

General data:

11.01.1908 - 02.01.1976

Place of birth: Vovchansk city, Kharkov province, Russian Empire

Studied in: Moscow State University ( since 1940 M. V. Lomonosov Moscow State University) (?-1928); Leningrad State University (since 1991 St. Petersburg State University) (1928-1930);

Key interests: minor bodies of the Solar System, astronomy, space missions. PhD Thesis: Received the scientific degree of the candidate of physical mathematics. Sciences without defense of the dissertation (1935 P.K. Sternberg State Astronomical Institute, M. V. Lomonosov Moscow State University); ScD Thesis: Meteoric phenomena in the Earth's atmosphere (1962 Ulyanov-Lenin Kazan Order of the Red Banner of Labor State University);


Biography:

He was born January 11, 1908 according to the Gregorian calendar or December 29, 1907 according to the Julian calendar in Volochansk city of the Kharkiv province of the Russian Empire in the family of a teacher of physics and mathematics at the Teaching Seminary.

The childhood of a future scientist was held in Novgorod-Seversk of Chernigov province, where his father was an inspector of public schools, and after 1917 - an instructor of public education.

At the age of 13, the boy was interested in astronomy, and already in 1925, a 17-year-old boy was elected as a correspondent member of the Russian Society of Lovers of Myriodenium, founded in 1909 by N. A. Morozov in Moscow until his closure at the end of 1930.

After graduating from the Technical School in Nikolaev city, the young man entered the Faculty of Physics and Mathematics of the Moscow State University in the field of "astronomy"; in 1928, under family circumstances, he was forced to transfer to the Leningrad (now St. Petersburg) University, which graduated in 1930.

During 1928-1932 he worked at the Institute of Applied Geophysics and during 1931-1932 he headed the magneto-metric expedition of the Institute of Applied Physics in the territory of Eastern Siberia. Simultaneously with the winter periods of 1928-1930, he worked as a freelance scientist of a meteorite department at the Mineralogical Institute of the USSR Academy of Sciences in Leningrad under the direction of V. I. Vernadsky and A. E. Forsma.

Since November 1932 to 1933 (according to some data until 1934), he was the first director of the Tajik Astronomical Observatory in Stalinabad (Dushanbe), which he founded.

During 1934-1941 he worked as a senior researcher at the P. K. Sternberg State Astronomical Institute.

In 1935, without protection, he was awarded a Ph.D. degree in Physics and Mathematics.

Since 1937 he was Associate Professor at the Moscow University at the Department of Comet Astronomy. He was the first to create lectures on meteoric astronomy, which he read at Moscow University since 1937, at Saratov University - since 1938, in Ashgabat - since 1954, and later in Odessa and Kyiv Universities.

During 1942-1959 he worked as a senior researcher of the Physics and Technology Institute of the Turkmen Branch (since 1951, the Academy of Sciences of the Turkmen SSR), the USSR Academy of Sciences, the organizer of the Observatory and Astrophysical Laboratory in Ashgabat.

In May 1962, in the V. I. Ulyanov-Lenin Kazan Order of the Red Banner of Labor State University, the astronomer defended his doctoral dissertation, presenting to protect his monograph "Meteor phenomena in the atmosphere of the Earth", for which the Higher Attestation Commission in March 1963 awarded him a degree Doctor of Physics and Mathematics.

During 1959-1960, he was the head of the department of the Observatory of the I. I. Mechnikov Odessa State University, and since 1960-1973 he was a member of the T. G. Shevchenko Kyiv Order of Lenin State University. Since 1966 he was a professor at the Department of Astronomy of the T. G. Shevchenko Kyiv Order of Lenin State University.

Arriving in Odessa in 1959, he became one of the developers of the technology of observing artificial Earth conjoint.

Together with O. I. Kizimirchak (Polonskaya), N. A. Belyaev and A. K. Terent'eva first studied the perturbed motion of the Leonid meteor shower, a meteoric flow with a radiate in the constellation Lev (RA = 153°, Decl. = + 22°), which operates from November 14 to November 21, with a periodicity of 33 years, being generated by the Comet 55P/Tempel - Tuttle) during the period 1700-2000.

He suggested that the Earth's atmosphere has a radiant gas tail, which like comets, is always extended in the opposite direction from the Sun. His assumption was confirmed in 1949 by Fesenkov V. G.

The scientist was a member of the International Astronomical Union. He was awarded the Order of the "Badge of Honor", "Labor Red Banner", a medal "For Valiant Labor".

Died January 2, 1976,

He is the author and co-author of 10 monographs, over 400 scientific works on meteoric phenomena in the Earth's atmosphere. During the period 1942-1959, the astronomer collected an archive of observations of 40,000 meteors.

Small planet №2408 wears name of astronomer.




Main publications:
  1. Казимирчак-Полонская Е. И., Беляев Н. А., Астапович И. С., Терентьева А. К. Исследование возмущённого движения метеорного роя Леонид // Астрономический журнал. М., 1967. Т. 44. № 3. С. 616—629.
  2. Kazimirchak-Polonskaja E.I., Beljaev N.A., Astapovich I.S., Terenteva А. К. Investigation of perturbed motion of the Leonid meteor stream. In "Physics and dynamics of meteors. Eds. L. Kresak and P.M. Millman. Dordrecht-Holland, 1968. P. 449—475.
  3. Астапович И.С. Метеорные явления в атмосфере Земли. — М.: Физматгиз, 1958. — 640 с.
  4. Астапович И.С. Опыт методики обработки визуальных наблюдений метеоров // Труды института физики и геофизики АН Туркм. ССР // Изд-во АН Туркм. ССР. — Ашхабад. — 1956. — 2. — С. 5–121.



Sources:
  1  Кафедра астрономії та фізики космосу, Фізичний факультет, Київський національний університет імені Тараса Шевченка
  2  Колчинский И. Г., Корсунь А. А., Родригес М. Г. Астрономы: Биографический справочник. — Киев: Наук. думка, 1986.—510 с.-24-25
  3  Справочный биографический материал
  4  Терентьєва О. К. Ігор Станіславович Астапович // Астрономічна обсерваторія Київського національного університету імені Тараса Шевченка. 160 років / відп. ред. В. М. Єфіменко. – Київ, 2005. – 260 с.- C.155-158

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