Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-24T01:18:47.841Z Has data issue: false hasContentIssue false
  • English
  • Français

Color and magnitude dependence of galaxy clustering

Published online by Cambridge University Press:  12 October 2016

Volker Müller
Volker Müller*
Affiliation:
Leibniz-Institut für Astrophysik Potsdam D-14482 Potsdam, Germany email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A quantitative study of the clustering properties of galaxies in the cosmic web as a function of absolute magnitude and colour is presented using the SDSS Data Release 7 galaxy redshift survey. We compare our results with mock galaxy samples obtained with four different semi-analytical models of galaxy formation imposed on the merger trees of the Millenium simulation.

Keywords

Cosmology: obserations - cosmology: theory - galaxies: statistics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S308: The Zeldovich Universe: Genesis and Growth of the Cosmic Web , June 2014 , pp. 293 - 294
Copyright
Copyright © International Astronomical Union 2016 

References

Blanton, M., Schlegel, D., Strauss, M., et al. 2005, ApJ, 129, 2562 Google Scholar
Croton, D., Springel, V., White, s., et al. 2006, MNRAS, 365, 11 Google Scholar
De Lucia, G. & Blaizot, J. 2007, MNRAS, 375, 2 Google Scholar
Font, A., Bower, R., McCarchy, I., et al. 2008, MNRAS, 193, 353 Google Scholar
Guo, Q., White, S., Boylan-Kolchin, M., et al. 2011, MNRAS, 413, 101 CrossRefGoogle Scholar
Müller, V., Hoffmann, K., & Nuza, S. E. 2011, Baltic Astronomy, 20, 259 Google Scholar