ASTRONOMICAL IMAGE PROCESSING FOR HIGH-ACCURATE ASTROMETRY DATA
DOI:
https://doi.org/10.18524/1810-4215.2017.30.114458Ключові слова:
astrometry, survey, image processing, big-dataАнотація
This article presents the main results of the initial processing of some of the astronomical images obtained from the archive of the digitized photographics survey of the whole sky SuperCOSMOS. Using of the median filtering and gausian convolution procedure with the adaptive kernel allows to carry out the initial processing of astronomical images without calibration frames. After the initial processing, the photocenters of the celestial objects were identified by various methods. It has been concluded that after the use of the mathematical methods for the initial processing of the digitized photographics images, the position of objects is calculated with a higher random and systematic precision.
Посилання
Akhmetov V., Fedorov P., Velichko A. et al.: 2017, MNRAS, 469, 1315.
Delabie T., De Schutter J., Vandenbussche B.: 2015, JAnSc, 61, 60.
Gaia Collaboration: 2016, A&A, 595, A1.
Gaia Collaboration: 2016, A&A, 595, A2.
Hambly N., Davenhall A., Irwin M. et al.: 2001a, MNRAS, 326, 1315.
Hambly N., Irwin M., MacGillivray H.: 2001, MNRAS, 326, 1295.
Hambly N., Miller L., MacGillivray H. et al.: 1998, MNRAS, 298, 897.
Juric M., Kantor J., Lim K.-T. et al.: 2015, arXiv pre-print:1502.07915.
Popowicz A., Smolka B.: 2015, MNRAS, 452, 809.
Vavilova I. et al.: 2012, Kinematics and Physics of Celestial Bodies, 28, N2, 85.
##submission.downloads##
Опубліковано
Номер
Розділ
Ліцензія
Авторське право (c) 2017 Odessa Astronomical Publications
Ця робота ліцензується відповідно до Creative Commons Attribution-NonCommercial 4.0 International License.
Відповідно Закону України про авторське право і суміжні права N 3792-XII від 23 грудня 1993 року