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