ASTRONOMICAL IMAGE PROCESSING FOR HIGH-ACCURATE ASTROMETRY DATA

Автор(и)

  • A. M. Dmytrenko Department of Astronomy and Space Informatics, V.N.Karazin National University, Ukraine
  • V. S. Akhmetov Institute of Astronomy, V.N.Karazin National University, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.2017.30.114458

Ключові слова:

astrometry, survey, image processing, big-data

Анотація

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

2017-11-09

Номер

Розділ

Астроінформатика