Annotation
A certain modification of the algorithm of star observations with the photographic zenith tube makes it possible to use a CCD-matrix in the focal plane. The proposed algorithm minimizes the requirements to the equipment employed for the star image processing and data input into the computer.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
V.A. Krainov
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
Science News of the Faculty of Physics, Lomonosov Moscow State University
This new information publication, which is intended to convey to the staff, students and graduate students, faculty colleagues and partners of the main achievements of scientists and scientific information on the events in the life of university physicists.