In this article, we present the new product and its description developed by the CoLiTec
(Collection Light Technology) project (Khlamov & Savanevych 2020), called CoLiTecVS …

This computational method is based on the analytical selection of the typical form of the
object's image, as well as on the choice of spe cial parameters for the transfer function of the …

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 …

A computational method for the automated formation of a typical form of a digital image of
the investigated objects on a series of digital frames has been developed. Due to the …

We presented the overview and realization of recognition prospects into processing of the
astronomical images using the Sobel filter in this research. It was designed for the border …

Modern astronomical systems and telescopes allow taking a lot of frames of considerable
sky area in one night. This is a big amount of the raw data sets that should be processed …

In this paper we presented the new algorithm for pixelization of astronomical data in celestial
sphere. This algorithm is used for partition and analysis of the large astronomical catalogues …

In this paper we presented the results of cloud computing and analysis of orbital parameters
of the satellite fragments that formed by first India anti-satellite (ASAT) missile against a" live" …

The appearance of" blurred" digital images is a consequence of the violation of the
immobility of the camera during the shooting of the objects under study. To this end, a …

In this paper we presented the new algorithm for astrometric reduction of the images
received from modern large telescopes with very wide field of view. This algorithm is based …