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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 

 Isotov Yuri Ivanovich 

General data:

Born: 26.02.1952

Place of birth: Stalino city, Ukrainian SSR, (now Donetsk city, Donetsk region, Ukraine)

Studied in: T. G. Shevchenko Kyiv Order of Lenin State University (since 1999 Taras Shevchenko Kyiv National University) (1974);

Key interests: astrophysics, physics of extragalactics. PhD Thesis: Research of formation of of molecular hydrogen and conditions of star formation in communication with the primary chemical composition (1984 Institute of Astrophysics and Atmospheric Physics of the Academy of Sciences of the Estonian SSR); ScD Thesis: Physics of the blue compact dwarf galaxies and the problem of their formation (1992 Main Astronomical Observatory of the National Academy of Sciences of Ukraine);


Biography:

He was born on February 26, 1952, in Stalino city of the Ukrainian SSR, now the Donetsk city of Donetsk region of Ukraine.

After completing his studies at the physical faculty of the T. G. Shevchenko Kyiv Order of Lenin State University in 1974, in the field of astronomy, he worked for about 3 years at the Department of Astronomy and Space Physics of the T. G. Shevchenko Kyiv Order of Lenin State University.

Since 1977 he has been working at the Main Astronomical Observatory of the Academy of Sciences of the Ukrainian SSR (since 1991, the National Academy of Sciences of Ukraine.

In 1984 he defended his candidate's dissertation at the Institute of Astrophysics and Atmospheric Physics of the Academy of Sciences of the Estonian SSR on the topic "Investigation of the formation of molecular hydrogen and the conditions for the formation of stars in an environment with a primary chemical composition".

In 1992 he defended a doctoral dissertation at the Main Astronomical Observatory of the National Academy of Sciences of Ukraine in the specialty 01.03.02. - astrophysics, radio astronomy on the theme: "Physics of blue compact carnivorous galaxies and the problem of their formation".

In the 1990s, together with T.H. Thuan (USA), V.A. Lipovetsky and other colleagues from the Special Astrophysical Observatory conducted in-depth studies of blue compact galaxies found in the KISS (Kitt Peak Observatory) and Hamburg-SAO surveys containing active star-forming galaxies, studying the content of heavy elements and gas.

In 2000 he was elected a corresponding member of the National Academy of Sciences of Ukraine.

Since 2000, he has been in charge of the department of physics of vision and galaxies of the Main Astronomical Observatory of National Academy of Sciences of Ukraine.

2009 together with Shtanov Yu. V. and Guseva N. G. became the winner of the E. P. Fedorov prize of the National Academy of Sciences of Ukraine for the series of works "Blue Dwarf Galaxies and Problems of Dark Matter".

February 04, 2009 was elected academician of National Academy of Sciences of Ukraine in the field of astrophysics.

He worked as a senior researcher at the Main Astronomical Observatory of National Academy of Sciences of Ukraine in the Department of Physics of the Stars and Galaxies, then he was head of the department.

Awarded with certificates of honor of the Cabinet of Ministers of Ukraine and the Verkhovna Rada of Ukraine, winner of the award "Leader of Science of Ukraine 2016. Web of Science Award".

In April 2016 he moved to the Department of Astronomy and Astrophysics at the M. M. Bogolyubov Institute of Theoretical Physics of the National Academy of Sciences of Ukraine. Currently Senior Research Fellow at the position of Chief Scientist of the Department of Astrophysics and Elementary Particles.

His scientific interests are concentrated in the physics of extant galaxies. Known for the study of the physical and evolutionary properties of dwarf galaxies and star formation. He determined the amount of primary helium and the density of baryon matter in the universe. He proved the possibility of the formation of galaxies from primitive matter in the modern era. Established the existence of young galaxies at short distances from our galaxy. The galaxy he discovered was named Izot.

In 2005, he and American astronomer Trinh Tuan discovered the youngest galaxy.

He is author of more than 250 scientific papers, published mainly in leading international publications, such as "Nature" and "The Astrophysical Journal"

A group of researchers from five countries led by Yu. I. Izotov proved the reasons for the reionization of the universe.

Discovered the young galaxies in the local Universe and proved that their vision is formed in compact superstructures of stars that are 10 billion times brighter than the Sun.

He, together with I. G. Kolesnik based on the analysis of elemental processes in the primary substance of the universe has received new results on the concentration of molecular hydrogen and the characteristics of the first generation of vision.

In the 90's of the twentieth century. Yu. I. Izotov and N.G. Guseva, together with specialists from the USA, France and Germany, most accurately determined the content of primary helium, which was formed in the first minutes of existence of the Universe.




Main publications:
  1. Y.I. Izotov, T.X. Thuan, V.A. Lipovetsky The primordial helium abundance from a new sample of metal-deficient blue compact galaxies// Astrophysical Journal. -1994.- Vol.435. -P.647-667.
  2. Y.I. Izotov, T.X. Thuan, V.A. Lipovetsky The primordial helium abundance: systematic effects and a new determination// Astrophysical Journal Suppl. Ser. -1997. -Vol. 108. P. 1-39.
  3. Izotov Y.I., Lipovetsky V.A. Heavy element abundances in a new sample of low-metallicity blue compact galaxies // Astrophysical Journal. -1995 -Vol.445.-P.108-123
  4. Izotov Y.I., Thuan T.X. Reexaming the helium abundance of I Zw 18// Astrophysical Journal. -1998. - Vol.497. - P.227-237.



Sources:
  1  Pavlenko Ya. V., Vavilova I. B., Kostiuk Ò. Astronomy in Ukraine. Organizations and strategies in astronomy. — Springer-Verlag, 2005.—Vol. 6.—P. 22
  2  Áîòâ³íîâà Â.Â. Ïåðåë³ê äèñåðòàö³é íà çäîáóòòÿ â÷åíîãî ñòóïåíÿ äîêòîðà (êàíäèäàòà) ô³çèêî-ìàòåìàòè÷íèõ íàóê, âèêîíàíèõ â Ãîëîâí³é àñòðîíîì³÷í³é îáñåðâàòî𳿠Íàö³îíàëüíî¿ àêàäå쳿 íàóê Óêðà¿íè â 1944-1993ðð. //50 ðîê³â Ãîëîâí³é àñòðîíîì³÷í³é îáñåðâàòî𳿠/ ϳä ðåä. ßöê³âà ß.Ñ. - Êè¿â, 1994.-320ñ.- Ñ.305, 309
  3  dissercat.com
  4  http://www1.nas.gov.ua

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