Cosmological distances scale: Part 10. The global Anisotropy

Abstract

A brief overview of the history of the origin and development of the cosmological distance scale based on redshift is given. Statistical aspects of the problem of calibration of scales of this type are considered and their analogy with the problems of calibration of measurement tools is shown. The analysis of the first data on the basis of which the “accelerated expansion of the Universe” was detected. The Consequences of Anisotropy for Distance Scale is analyzed.