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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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 Yakovina Larisa Yakimivna 

General data:

Born: 02.06.1948

Place of birth: Kyiv City, Kyiv region, Ukrainian SSR

Studied in: T. G. Shevchenko Kyiv Order of Lenin State University (since 1999 Taras Shevchenko Kyiv National University) (1966-1971);

Key interests: informatic technologies. PhD Thesis: Analysis of the chemical composition of the atmospheres of red giants by the synthetic spectrum (1986 Main Astronomical Observatory of Academy of Science Ukrainian SSR);


Biography:

She was born on June 2, 1948 in the Kyiv city of Kyiv region of Ukrainian SSR.

In 1971, she graduated from the astronomy department of the physics department of the Kyiv Order of Lenin State University named after T. G. Shevchenko, which she entered in 1966 after graduating from secondary school No. 145 in Kyiv. Received the specialty "astronomer" with specialization in "astrophysics".

Since August 1971 to September 1974, she worked as an engineer at the Lenin Arsenal plant.

From October 1974 to May 1978, she worked as a junior researcher at the department of integrated use of water resources of the Ukrainian SSR, UnishKIVR of the Ministry of Water Management of the USSR.

From November 1973 to November 1977, she studied at the postgraduate course of the Main Astronomical Observatory of the Academy of Sciences of the Ukrainian SSR without a break from production (correspondence postgraduate course).

In 1977, the program for entering numerical arrays in the computer code "Minsk-22" was developed in the BESM-6 computer with control of the entered information.

From May 15, 1978, she worked as an engineer at the Computing and Research Center of the Main Astronomical Observatory of the Academy of Sciences of the Ukrainian SSR. She dealt with issues of computer use for automating the processing of atomic and molecular spectra of stars of late spectral classes. In Assembler, she wrote a program for inserting perforated lenses from the AMF-2 microphotometer into the EC-1022 computer, and it was registered in the algorithm and program fund. At the beginning of 1982, the debugging of a complex of programs for digital processing of spectrograms of stars of late spectral classes with the help of a computer was completed, and together with A. V. Shavrina, a complex of programs for calculating synthetic spectra of cold stars taking into account absorption in molecular stars was completed. With the help of these programs, in 1982, a number of problems were solved to determine the chemical composition of the atmospheres of red giants. Together with A. V. Shavrina and M. E. Boyarchuk, the content of lithium in the atmospheres of 8 stars was determined; together with M. Ya. Orlov and A. V. Shavrina, the content of sodium in the atmosphere of the M-giant β Pegasi was determined. The fact of the presence of the chromospheric line NeI λ 5876Å in the spectra of 6 M-giants has been established. The issue of the possibility of separating blends in the spectra of red giants is considered.

Since September 1979 she worked as an engineer of the Laboratory of Experimental Astrophysics of Astrospectroscopy of the Main Astronomical Observatory of the Academy of Sciences of the Ukrainian SSR, and Since 1981 in the same position in the Department of Planetary Physics, and Since February 1982 as a junior researcher of the department (according to other data started working in this position since 1981), since February 1988 - as a research associate.

In 1986 (according to other data, in April 1985), she defended her candidate's thesis "Analysis of the chemical composition of the atmospheres of red giants using the synthetic spectrum method" at the Main Astronomical Observatory of the Academy of Sciences of the Ukrainian SSR.

After defending her thesis, she devoted a significant part of her life to the study of the star γ Leo in the Leo constellation. Together with A. V. Shavrina, she worked on determining the nitrogen and carbon content in the atmosphere by molecular spectra.

In December 2009, she worked part-time as a senior researcher under contract #4/9 "Cosmomicrophysics" at the Laboratory of Astroinformatics.

About 60 of her works have been published in leading domestic and foreign publications.

In July 2011, she left the Main Astronomical Observatory of the National Academy of Sciences of Ukraine due to her retirement.

From September 2011 to December 2012, she worked in the Department of Physics of Stars and Galaxies of the Main Astronomical Observatory of the National Academy of Sciences of Ukraine as a contract researcher (in 2012, she went to the Department of Solar Physics and was dismissed as an employee of this department at the end of the contract).




Main publications:
  1. Боярчук М. Е., Шаврина А. В., Яковина Л. А. (1983) Содержание лития в атмосферах M-гигантов с учетом молекулярного поглощения. Астрофизика, 19 (2). pp. 265-272.
  2. Шаврина А. В., Яковина Л. А. Химический состав атмосфер М-сверхгигантов α Sco и α Her А//Астрометрия и астрофизика, 1973, №19, С. 87-98
  3. Яковина Л. А. Сглаживание звездных спектров методом Уиттекера//Астрономия и астрофизика, вып. 31, 1977, С.78-84
  4. Яковина Л. А. Программа ввода числовых массивов в коде ЭВМ -"Минск-22" в ЭВМ БЭСМ-6 с контролем вводимой информации, РФАП, КИекв, 1977, рег. №4873



Sources:
  1  Ботвінова В.В. Перелік дисертацій на здобуття вченого ступеня доктора (кандидата) фізико-математичних наук, виконаних в Головній астрономічній обсерваторії Національної академії наук України в 1944-1993рр. //50 років Головній астрономічній обсерваторії / Під ред. Яцківа Я.С. - Київ, 1994.-320с.- С.310
  2  Список дисертацій, захищених співробітниками ГАО/Головна астрономічна обсерваторія Національної академії наук України: від ідеї створення до міжнародного визнання/За редакцією Я. С. Яцківа.-Київ: Наукова думка, 2018.-376 с.-С.332
  3  Київський національний університет імені Тараса Шевченка. Кафедра астрономії та фізики космосу. Випускники
  4  Яковіна Лариса Якимівна. Архів ГАО НАН України, Опис №3-К, том 3 (прод), Справа № 229, 2012, 68 с.

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