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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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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 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...
Astronomical Net of Ukraine 
Добро пожаловать на портал! Терабайты видео, книг и другой астрономической научной и научно-популярной информации доступны для Вас! Вы также можете добавлять материалы - публиковать новости астрономии, статьи и т.п. Для этого достаточно пройти регистрацию. Давайте собирать информацию вместе!
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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 Malov Igor Fedorovich 

General data:

Born: 08.04.1941

Place of birth: Orikhovo-Zuyevo city, Moscow region, Russian SSR

Studied in: A. M. Gorky Kharkiv State University (since 1999 V. N. Karazin Kharkiv National University) (1963);


He was born on April 8, 1941 in Orikhovo-Zuyevo city of Moscow region of the Russian SSR.

In 1963 he graduated from A. M. Gorky Kharkiv State University.

Since 1963 he has been working at the Radio Astronomical Station of the Physical Institute of the USSR Academy of Sciences. He went from a research trainee to a senior researcher.

In 1992 he received the degree of Doctor of Physical and Mathematical Sciences.

He is a professor at the Pushchin State Institute of Natural Sciences.

He has been a member of the Board of the Eurasian Astronomical Society since 2000, a member of the International Astronomical Union.

The main scientific works relate to the fields of astrophysics and physics of pulsars. He is the author of about two hundred scientific papers, including co-author of two monographs.

In 1960-1970 he studied the mechanisms of acceleration of matter in hot stars and showed that in Wolf-Raye stars the main mechanism of acceleration is Thomson scattering of radiation by electrons.

Since the mid-1970s, he has been working on building a radio pulsar model based on available observational data.

He proposed mechanisms for the formation of characteristic features of the spectra of these objects (low-frequency blockage, linear part, high-frequency fracture, and observed in a number of pulsars increase in intensity at frequencies in the tens of GHz).

In collaboration with Yu.P. Shitov, V. A. Izvekova, A. D. Kuzmin, V. M. Malofeev, O. I. Malov and several German, Greek and Polish colleagues measured for the first time the basic parameters of radio emission of more than 200 pulsars, including flux density, spectrum, luminosity, shape of medium pulses. They compiled the largest catalog of pulsar spectra (335 objects), classified them.

I. F. Malov proposed the concept of dividing radio pulsars into two types depending on their periods, based on the differences in the scale of the magnetosphere in long-period and short-period pulsars.

I. F. Malov developed several methods for estimating the angle between the magnetic moment and the axis of rotation in pulsars. Co-authored with G. Z. Machabeli advanced and developed a drift model to explain the features of abnormal X-ray pulsars and sources with repetitive gamma radiation.

In early 2000, with the active participation of I. F. Malov the Training Center for Astrophysics and Radio Astronomy was established at the Pushkin State Astronomical Observatory to train undergraduates and graduate students in relevant specialties. He teaches two author's courses at this institute: "Mechanisms of cosmic radiation" and "Physics of stars and pulsars". Under his supervision, several master's and two candidate's dissertations were prepared.

  1  Астрономы России 1917-2017/ науч. ред. А.М.Черепащук, Казань, Казан. фед. ун-т, 2017.- 568с- C. 291
  2  МАЛОФЕЕВ Валерий Михайлович//Астрономы России 1917-2017/ науч. ред. А.М.Черепащук, Казань, Казан. фед. ун-т, 2017.- 568с- C. 292

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