Clustering of quasars

Details Clustering of quasars Clustering of quasars

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sssmp..30..405f&link_type=abstract

Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 30, April 1987, p

Astronomy and Astrophysics

Astronomy

Galactic Clusters, Monte Carlo Method, Quasars, Red Shift

Scientific paper

The clustering of quasars has been analyzed by comparing the two-point correlation function, the cluster analysis curves, percolation parameters, and multiplicity function of three quasar samples with those of the corresponding Monte Carlos samples. No obvious clustering of quasars has been found. This indicates that in the z about 2 era the distribution of the visible matter had no obvious structure, which supports the cluster picture that the small-scale structure might be formed before or after the formation of the large-scale structure.

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