| Quasar Clustering from SDSS DR5: Dependences on Physical Properties (2008) | |||||||||
Abstract | |||||||||
| Using a homogenous sample of 38,208 quasars with a sky coverage of $4000 {\rm deg^2}$ drawn from the SDSS Data Release Five quasar catalog, we study the dependence of quasar clustering on luminosity, virial black hole mass, quasar color, and radio loudness. At $z. Comment: Updated version; accepted for publication in ApJ | |||||||||
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