ON THE FON ASTROPLATE PROJECT ACCOMPLISHMENT

• Main Authors: V. M. Andruk, L. K. Pakuliak, I. Eglitis, Q. Yuldoshev, A. Mullo-Abdolov, S. V. Shatokhina, O. M. Yizhakevych, Yu. I. Protsyuk, H. Relke, V. S. Akhmetov, M. M. Muminov, Sh. A. Ehgamberdiev, G. Kokhirova
• Format: Article
• Language: English
• Published: Odessa I. I. Mechnykov National University 2019-10-01
• Series: Odessa Astronomical Publications
• Subjects: зоряні каталоги, обробка оцифрова- них зображень, фотометрія, система ubv
• Online Access: http://oap.onu.edu.ua/article/view/181558

The plan of the photographic survey of the northern sky (FON) was proposed in 1976 in Golosiiv ob- servatory (now MAO NAS of Ukraine) by I. Kolchinsky and A. Onegina. The final project of the Compiled FONAC catalog (FON Astrographic Catalog) is based on the digital data of photographic plates exposed at four observatories. They are MAO NAS of Ukraine (Kyiv, Ukraine), Kitab astronomical observatory (Tashkent, Uzbekistan), Hissar astronomical observatory (Dushanbe, Tajikistan), and Bal- done observatory (Latvia)). The total amount of plates is 5700. The result is expected to be the catalog of positions and B-magnitudes of stars covered the declination area from -20 to 90 degrees. The estimated mean epoch of the catalog is ~1987. The limiting B-magnitude is ~17.5 m . The reference system for positions is Tycho-2. B-magnitudes are being obtained in the system of photoelectric standards. The resulted data of photometric reduction are corrected for the photometric color equation in B magnitudes. The com- plement for the photometric content of the catalog is U and V magnitudes of stars being obtained from the processing of 5400 plates from the glass collection of 1.2 m Schmidt telescope in Baldone. Photometric data of bright stars with V < 8.5 m U, B,V magnitudes cannot be obtained from pho- tographic material, so those objects will gain photometric data from photoelectric catalogs. The catalog will be com- plemented with proper motions from GAIA.