Accurate sky identification is one of the most important functions of an automated telescope
mount. The more accurately the robotic telescope is navigated to the investigated part of the …

In general, astronomical images are made by the charge-coupled device (CCD)[Smith 2010]
or other cameras/sensors. Also, such astronomical images can be received from other …

The paper deals with a computational method for detection of the solar system minor bodies
(SSOs), whose inter-frame shifts in series of CCD-frames during the observation are …

Joint scientific experiments are the main way of international cooperation in the field of
science. One of the ways to organize joint research is providing remote groups of scientists …

We investigated two variable stars AH Tau and ZZ Cas. They are eclipsing binaries of W
UMa and $\beta $ Lyr types. The period changes with time. The reason for steady changes …

In this work we have presented the computational algorithm for determining the primary
orbits and discovery of the different asteroids using the Väisälä method. The first step of the …

The very fast technological progress provokes the creation of a big volume of the
astronomical data, which is fed in the different forms. There are various directions in science …

The biography of Vladimir Platonovich Tsesevich (11.11. 1907-28.10. 1983), a leader of the
astronomy in Odessa from 1944 to 1983, is briefly reviewed, as well as the directions of …

Old, digitized astronomical images taken before the human spacefaring age offer a unique
view of the sky devoid of known artificial satellites. In this paper, we have carried out the first …

In our research, we have studied 6 close binary stellar systems which are eclipsing variables
of $\beta $ Lyrae and W Ursae Majoris types of variability. We have studied their OC curves …