Realization of Vilnius UPXYZVS photometric system for AltaU42 CCD camera at the MAO NAS of Ukraine

• Опубліковано в: : Кинематика и физика небесных тел
• Дата: 2005
• Автори: Vid'machenko, A.P., Andruk, V.M., Samoylov, V.S., Delets, O.S., Nevodovsky, P.V., Ivashchenko, Yu.M., Kovalchuk, G.U.
• Формат: Стаття
• Мова: English
• Опубліковано: Головна астрономічна обсерваторія НАН України 2005
• Теми: MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
• Онлайн доступ: https://nasplib.isofts.kiev.ua/handle/123456789/79720
• Назва журналу: Digital Library of Periodicals of National Academy of Sciences of Ukraine
• Цитувати: Realization of Vilnius UPXYZVS photometric system for AltaU42 CCD camera at the MAO NAS of Ukraine / A.P. Vid'machenko, V.M. Andruk, V.S. Samoylov, O.S. Delets, P.V. Nevodovsky, Yu.M. Ivashchenko, G.U. Kovalchuk // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 551-556. — Бібліогр.: 9 назв. — англ.

The description of two-inch glass filters of the Vilnius UPXYZVS photometric system, which are made at the Main Astronomical Observatory of NAS of Ukraine for AltaU42 CCD camera with format of 2048×2048 pixels, is presented in the paper. Reaction curves of instrumental system are shown. Estimations of minimal star’s magnitudes for each filter’s band in comparison with the visual V one are obtained. New software for automation of CCD frames processing is developed in program shell of LINUX/MIDAS/ROMAFOT. It is planned to carry out observations with the purpose to create the catalogue of primary UPXYZVS CCD standards in selected field of the sky for some radio-sources, globular and open clusters, etc. Numerical estimations of astrometric and photometric accuracy are obtained.