Fig. 11 from Clustering Properties of Rest‐Frame UV‐Selected Galaxies. II. Migration of Star Formation Sites with Cosmic Time from GALEX and CFHTLS

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution

Export to PDF PPT Format

Clustering Properties of Rest‐Frame UV‐Selected Galaxies. II. Migration of Star Formation Sites with Cosmic Time from GALEX and CFHTLS

Authors: Sébastien Heinis, Bruno Milliard, Stéphane Arnouts, Jérémy Blaizot, David Schiminovich, Tamás Budavári, Olivier Ilbert, José Donas, Marie Treyer, Ted K. Wyder, Henry J. McCracken, Tom A. Barlow, Karl Forster, Peter G. Friedman, D. Christopher Martin, Patrick Morrissey, Susan G. Neff, Mark Seibert, Todd Small, Luciana Bianchi, Timothy M. Heckman, Young-Wook Lee, Barry F. Madore, R. Michael Rich, Alex S. Szalay, Barry Y. Welsh, Sukyoung K. Yi, and C. K. Xu

Heinis et al. 2007 The Astrophysical Journal Supplement Series 173 503.

Provider: AAS Journals

Caption: Fig. 11.

Bias of rest‐frame UV‐selected galaxies as a function of galaxy number density. The curves show the expected relation for the effective bias of dark matter halos at redshifts ﹩z=0,0.5,1,2,﹩ and 3, from bottom to top. We plot only independent samples here. The symbols are the same as in Fig. 10.

Other Images in This Article

Copyright and Terms & Conditions