Measuring the Luminosity Dependence of Quasar Clustering Using the 2DF QSO Redshift Survey

Details Measuring the Luminosity Dependence of Quasar Clustering Using the 2DF QSO Redshift Survey Measuring the Luminosity Dependence of Quasar Clustering Using the 2DF QSO Redshift Survey

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mas..conf...73l&link_type=abstract

MULTIWAVELENGTH AGN SURVEYS. Proceedings of the Guillermo Haro Conference 2003. Held 8-12 December 2003 in Cozumel, Mexico. Edit

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have been able to accurately measure the luminosity dependence of QSO clustering independently of any redshift evolution. Contrary to the results obtained from galaxy clustering studies, we find no evidence for any luminosity segregation in the QSO population. These results suggest that local astrophysical effects play an important role in QSO formation and have important implications for models of QSO formation and evolution.

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