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Vadym Savanevych

Vadym Savanevych Mail
Western Center for Radio Technical Supervision, State Space Agency of Ukraine, Ukraine

Doctor of Technical Sciences, Professor, Head of Laboratory

Laboratory Checking and analysis of space situation


Scopus profile: link



 Selected Publications:

1. Savanevych, V. E., Khlamov, S. V., Vavilova, I. B., Briukhovetskyi, A. B., Pohorelov, A. V., Mkrtichian, D. E. et. al. (2018). A method of immediate detection of objects with a near-zero apparent motion in series of CCD-frames. Astronomy & Astrophysics, 609, A54. doi: 

2. Khlamov, S. V., Savanevych, V. E., Briukhovetskyi, O. B., Pohorelov, A. V. (2016). CoLiTec software - detection of the near-zero apparent motion. Proceedings of the International Astronomical Union, 12 (325), 349–352. doi: 

3. Khlamov, S., Savanevych, V., Briukhovetskyi, O., Oryshych, S. (2016). Development of computational method for detection of the object’s near-zero apparent motion on the series of ccd-frames. Eastern-European Journal of Enterprise Technologies, 2 (9 (80)), 41–48. doi: 

4. Pohorelov, A., Savanevych, V., Udovenko, S. (2016). An investigation of the reduction model power influence on the accuracy of the object’s position assessment using relative method. Eastern-European Journal of Enterprise Technologies, 4 (4 (82)), 42–49. doi: 

5. Vavilova, I. B., Yatskiv, Y. S., Pakuliak, L. K., Andronov, I. L., Andruk, V. M., Protsyuk, Y. I. et. al. (2016). UkrVO Astroinformatics Software and Web-services. Proceedings of the International Astronomical Union, 12 (325), 361–366. doi: 

6. Savanevych, V. E., Briukhovetskyi, A. B., Ivashchenko, Y. N., Vavilova, I. B., Bezkrovniy, M. M., Dikov, E. N. et. al. (2015). Comparative analysis of the positional accuracy of CCD measurements of small bodies in the solar system software CoLiTec and Astrometrica. Kinematics and Physics of Celestial Bodies, 31 (6), 302–313. doi: 

7. Savanevych, V. E., Briukhovetskyi, O. B., Sokovikova, N. S., Bezkrovny, M. M., Vavilova, I. B., Ivashchenko, Y. M. et. al. (2015). A new method based on the subpixel Gaussian model for accurate estimation of asteroid coordinates. Monthly Notices of the Royal Astronomical Society, 451 (3), 3287–3298. doi: