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ON THE FON ASTROPLATE PROJECT ACCOMPLISHMENT

V. M. AndrukMain Astronomical Observatory of National Academy of Sciences,L. K. PakuliakMain Astronomical Observatory of National Academy of SciencesИ. ЭглитисInstitute of Astronomy, University of LatviaQ. YuldoshevUlugh Beg Astronomical Institute of the Uzbekistan Academy of SciencesA. Sh. Mullo-AbdolovInstitute of Astrophysics of the Academy of Sciences of Republic TajikistanS. V. ShatokhinaMain Astronomical Observatory of National Academy of SciencesO. M. YizhakevychMain Astronomical Observatory of National Academy of SciencesYu. I. ProtsyukResearch Institute Mykolaiv Astronomical ObservatoryH. RelkeV. S. AkhmetovM. M. MuminovAndijan State UniversitySh. A. EhgamberdievUlugh Beg Astronomical Institute of the Uzbekistan Academy of SciencesГ. И. КохироваInstitute of Astrophysics of the Academy of Sciences of Republic Tajikistan
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Аннотация

The plan of the photographic survey of thenorthern sky (FON) was proposed in 1976 in Golosiiv ob-servatory (now MAO NAS of Ukraine) by I. Kolchinskyand A. Onegina. The final project of the Compiled FONACcatalog (FON Astrographic Catalog) is based on the digitaldata of photographic plates exposed at four observatories.They are MAO NAS of Ukraine (Kyiv, Ukraine), Kitabastronomical observatory (Tashkent, Uzbekistan), Hissarastronomical observatory (Dushanbe, Tajikistan), and Bal-done observatory (Latvia)). The total amount of plates is5700. The result is expected to be the catalog of positionsand B-magnitudes of stars covered the declination areafrom -20 to 90 degrees. The estimated mean epoch of thecatalog is ~1987. The limiting B-magnitude is ~17.5 m . Thereference system for positions is Tycho-2. B-magnitudesare being obtained in the system of photoelectric standards.The resulted data of photometric reduction are corrected forthe photometric color equation in B magnitudes. The com-plement for the photometric content of the catalog is U andV magnitudes of stars being obtained from the processingof 5400 plates from the glass collection of 1.2 m Schmidttelescope in Baldone. Photometric data of bright stars withV < 8.5 m U, B,V magnitudes cannot be obtained from pho-tographic material, so those objects will gain photometricdata from photoelectric catalogs. The catalog will be com-plemented with proper motions from GAIA.

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