Registration of star transits on semiconductor matrix in real time
Tolstoy A. L.1,2, Petrov S. D.1, Smirnov S. S.1, Trofimov D. A.1, Grachev S. I.1
1St. Petersburg State University, St. Petersburg, Russia
2Institute of Applied Astronomy, Russian Academy of Sciences, Saint-Petersburg, Russia
Email: st063510@student.spbu.ru

PDF
In this paper, we consider the problem of using CMOS matrices to record the transit of stars on a transit instrument. Reasoning is given that indicates the relevance of this task, as well as a project for the modernization of a transit instrument and the current results of work on the development of technologies for creating a modernized transit instrument. The paper also considers the problem of specific image artifacts and proposes a method for calibrating images that removes these artifacts. Keywords: image calibration, fixed-pattern noise correction.
  1. A. El Gamal, EE392B: Introduction to Image Sensors and Digital Cameras, Lecture Notes, Lecture 7: Fixed Pattern Noise, URL: https://isl.stanford.edu/ abbas/ee392b/lect07.pdf
  2. S. Howell. Handbook of CCD Astronomy (Cambridge: Cambridge University Press, 2006), p. 77-82. DOI: 10.1017/CBO9780511807909
  3. T. Zhang, X. Li, J. Li, Z. Xu. Appl. Sci., 10 (11), 369 (2020). DOI: 10.3390/app10113694
  4. Y. Cao, Z. He, J. Yang, Y. Cao, M.Y.Y. Yang. IEEE Photon. J., 9 (5), 1 (2017). DOI: 10.1109/JPHOT.2017.2752000
  5. T. Zhang, X. Li, J. Li, Z. Xu. Sensors, 20 (19), 5567 (2020). DOI: 10.3390/s2019556
Publisher:

Ioffe Institute

Institute Officers:

Director: Sergei V. Ivanov

Contact us:

26 Polytekhnicheskaya, Saint Petersburg 194021, Russian Federation
Fax: +7 (812) 297 1017
Phone: +7 (812) 297 2245
E-mail: post@mail.ioffe.ru