Speaker
I. Kudzej
(Vihorlat Observatory, Humenné, Slovakia,)
Description
The capabilities of telescopes allow us to make the plotting of light curves a routine task. This one shifts the main attention of astronomer from the plotting to research. To achieve this goal, we developed a new tool for automated reduction of photometric observations, which includes the computational method for the brightness assessment of the investigated and comparison stars; brightness equalization of astronomical images using inverse median filter; light curve plotting and its processing using different tools.
Authors
V. E. Savanevych
(Western Radio Technical Surveillance Center, National Space Agency of Ukraine, Mukachevo, Ukraine,)
O. B. Briukhovetskyi
(Western Radio Technical Surveillance Center, National Space Agency of Ukraine, Mukachevo, Ukraine)
S. V. Khlamov
(Institute of Astronomy, V. N. Karazin Kharkiv National University, Kharkiv, Ukraine)
A. V. Pohorelov
(Kharkiv National University of Radioelectronics, Kharkiv, Ukraine,)
V. P. Vlasenko
(Western Radio Technical Surveillance Center, National Space Agency of Ukraine, Mukachevo, Ukraine,)
P. A. Dubovský
(Vihorlat Observatory, Humenné, Slovakia,)
I. Kudzej
(Vihorlat Observatory, Humenné, Slovakia,)
Š. Parimucha
(Faculty of Science, UPJŠ Коšice, Slovakia)
