S. V. Shatokhina

Main Astronomical Observatory

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V. M. Andruk

Main Astronomical Observatory

O. M. Yizhakevych

Main Astronomical Observatory

Yu. I. Protsyuk

Mykolaiv Observatory

L. K. Pakuliak

Main Astronomical Observatory

L. V. Kazantseva

Taras Shevchenko National University of Kyiv

ИЭ

И. Эглитис

University of Latvia

V. V. Golovnia

Main Astronomical Observatory

H. Relke

Mykolaiv Observatory

M. Eglīte

Riga Stradiņš University

V. V. Golovnya

Main Astronomical Observatory

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Main Astronomical Observatory

National Academy of Sciences of Ukraine

Mykolaiv Observatory

Taras Shevchenko National University of Kyiv

Academy of Sciences Republic of Uzbekistan

Astronomical Observatory

Ulugh Beg Astronomical Institute

Andijan State University

ASTER

Pulkovo Observatory

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POSITIONAL CATALOGUES OF SATURN’S AND JUPITER’S MOONS

DOAJ (DOAJ: Directory of Open Access Journals) (2014)

O. M. Yizhakevych V. M. Andruk I. Pakuliak V. Lukianchuk S. V. Shatokhina

Jupiter (rocket family)

10.18524/1810-4215.2014.27.81225

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Citations (2)

First results of MAO NASU SS bodies photographic archive digitizing

HAL (Le Centre pour la Communication Scientifique Directe) (2012)

L. K. Pakuliak V. Andruk S. V. Shatokhina V. V. Golovnya O. M. Yizhakevych

MAO NASU glass archive encloses about 1800 photographic plates with planets and their satellites (including near 80 images of Uranus, Pluto and Neptune), about 1700 plates with minor planets and about 900 plates with comets. Plates were made during 1949-1999 using 11 telescopes of different focus, mostly the Double Wide-angle Astrograph (F/D=2000/400) and the Double Long-focus Astrograph (F/D=5500/400) of MAO NASU. Observational sites are Kiev (Ukraine), Lviv (Ukraine), Biurakan (Armenia), Abastumani (Georgia), Mt. Maidanak (Uzbekistan), Quito (Equador).

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Astrometric positions of the external planets and their satellites.

S. V. Shatokhina

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Citations (3)

Photographic Survey of the Northern Sky: hidden reserves

Yu. I. Protsyuk V. M. Andruk L. K. Pakuliak V. V. Golovnia S. V. Shatokhina

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Processing results of digitized photographic observations of Pluto from the collections of the Ukrainian Virtual Observatory

Kinematics and Physics of Celestial Bodies (2015)

L. V. Kazantseva S. V. Shatokhina Yu. I. Protsyuk O. E. Kovylianska V. M. Andruk

Pluto

Ephemeris

Virtual Observatory

10.3103/s0884591315010031

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Citations (17)

ON THE “SOLAR SYSTEM SMALL BODIES” ASTROPLATE PROJECT OF THE UKRAINIAN VIRTUAL OBSERVATORY

Odessa Astronomical Publications (2019)

S. V. Shatokhina O. M. Yizhakevych Yu. I. Protsyuk L. V. Kazantseva L. K. Pakuliak

The UkrVO Joint Digital Archive of astro-plates and the newest digitized data processing services al-lowed us to form a new approach for the creation of catalogsof astrometric and photometric characteristics of the SolarSystem bodies. Given this, the main goal of this approachwas not only to complete the processing with the best possi-ble accuracy of high-quality and unprocessed earlier photo-graphic observations of the Solar System bodies but also tofind new original data from these observations.As a result, more than 6,500 new astrometric positionsand stellar magnitudes of asteroids, and 3,036 positions ofouter planets (Pluto, Uranus, Neptune, Saturn, Jupiter) andtheir satellites have been determined. Most of the posi-tions obtained from observations of large stellar surveysof the northern sky FON (Kyiv and Kitab parts) and othersurveys (MEGA, Equatorial Catalog).The number of new obtained positions of asteroids iscomparable to the total number of all positions of aster-oids obtained at the Main Astronomical Observatory ofthe NAS of Ukraine in 1949-1996. The accuracy of newpositions is higher than in traditional determinations fromphotographic observations, but it cannot be comparable tothe accuracy of modern CCD observations.Contrary to traditional classic definitions, digitized im-ages of plates have produced a large number of faint aster-oids down to 17.5 magnitudes, which were discovered inthe early 21st century. For some of them, observations areeither completely absent or not enough over the certain timeinterval preceding the moments of their official discoveries.These data can be obtained from photographic observationsonly. Based on our observations, about 300 such asteroidswere found. The collection of missing data on positionsover certain time intervals and their analysis can be usefulnot only for modern ephemeris calculations but also forstudying the evolution of asteroid orbits over time.The cooperation between UkrVO and the observatory inBaldone of the University in Latvia, astronomical and astro-physical institutes of Uzbekistan and Tajikistan make it pos-sible to expand this work by involving numerous additionalarchives of digitized observations and processing servicesand thus obtaining new original data about the Universe.

Neptune

Uranus

Pluto

Ecliptic

10.18524/1810-4215.2019.32.181732

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Citations (1)

COMPILATION OF CATALOG OF STELLAR EQUATORIAL COORDINATES AND B-MAGNITUDES USING UKRVO PLATE DATABASE

DOAJ (DOAJ: Directory of Open Access Journals) (2014)

V. N. Andruk V. V. Golovnya G. A. Ivanov E. M. Izhakevich L. K. Pakuliak

10.18524/1810-4215.2014.27.80985

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