Statistical evidence for possible association between QSOs and bright galaxies

Details Statistical evidence for possible association between QSOs and bright galaxies Statistical evidence for possible association between QSOs and bright galaxies

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...138..408c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 138, no. 2, Sept. 1984, p. 408-414.

Astronomy and Astrophysics

Astrophysics

22

Astronomical Models, Galactic Clusters, Quasars, Cross Correlation, Density Distribution, Radio Spectra, Red Shift, Statistical Correlation, Visible Spectrum

Scientific paper

A statistical study has been made of QSO-bright galaxy correlations using the QSO catalog of Hewitt and Burbidge (1980) and the Second Reference Catalogue of Bright Galaxies (de Vaucouleurs et al., 1976). Both cross-correlation function techniques and the nearest neighbor method have been used. The results from all of these analyses shown in a series of tables provide strong statistical evidence for the association of QSOs at all redshifts with bright galaxies which have redshifts of not less than 0.05.

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