The distribution of quasars on the large scale and the super large scale

Details The distribution of quasars on the large scale and the super large scale The distribution of quasars on the large scale and the super large scale

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...311..578z&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 311, Dec. 15, 1986, p. 578-588. Research supported by the Chinese Academy o

Statistics

Computation

7

Computational Astrophysics, Density Distribution, Quasars, Big Bang Cosmology, Cluster Analysis, Red Shift, Statistical Correlation, Universe

Scientific paper

Using the two-point correlation function, cluster analysis (including change of size and number of the maximum connected region), percolation parameter calculation, multiplicity function analysis, and other statistical methods, testing three quasar samples and two quasar candidate samples, the authors obtain in all cases the consistent conclusion that there is possibly some very weak clustering when the distance between the quasar is ≡100 Mpc, and there is no clustering on the super large scale, i.e., the universe above the supercluster is uniform and structureless.

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