Speaker
Description
Quasars are perhaps the brightest extragalactic sources, and due to their brightness, they are visible at greater distances. By studying the distribution of quasars in the Universe, it is possible to determine whether there are large-scale inhomogeneities in the Universe or not. If the distribution of quasars is inhomogeneous at large distances, then the same can be stated about the Universe. At small distances, quasars either do not exist, or their number is very small. Therefore, the distribution of quasars at small distances is highly conditional, and we cannot draw any conclusions about the homogeneity of the Universe there.
Therefore, the distribution of quasars allows us to determine the distribution of matter over large distances, which we use to detect large-scale inhomogeneities in the Universe.