The environmental dependence of galaxy clustering in the Sloan Digital Sky Survey
- 11 November 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 372 (4) , 1749-1754
- https://doi.org/10.1111/j.1365-2966.2006.10987.x
Abstract
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This publication has 36 references indexed in Scilit:
- The Scale Dependence of Relative Galaxy Bias: Encouragement for the “Halo Model” DescriptionThe Astrophysical Journal, 2006
- The Fourth Data Release of the Sloan Digital Sky SurveyThe Astrophysical Journal Supplement Series, 2006
- The environmental dependence of clustering in hierarchical modelsMonthly Notices of the Royal Astronomical Society, 2005
- The Dependence on Environment of Cold Dark Matter Halo PropertiesThe Astrophysical Journal, 2005
- Interpreting the Relationship between Galaxy Luminosity, Color, and EnvironmentThe Astrophysical Journal, 2005
- The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy typeMonthly Notices of the Royal Astronomical Society, 2005
- Halo models of large scale structurePhysics Reports, 2002
- Galaxy properties in low X-ray luminosity clusters atz=0.25Monthly Notices of the Royal Astronomical Society, 2002
- The evolution of galaxies in clusters. V - A study of populations since Z approximately equal to 0.5The Astrophysical Journal, 1984
- A survey of galaxy redshifts. V - The two-point position and velocity correlationsThe Astrophysical Journal, 1983