Image Details
Caption: Figure 2.
Panel (a) Comparison between f( W r ) of the models fits and the data. Panel (b) Comparison between the b W / b LRG at z = 0.6 from the models and the Bouché et al. (2006) data. The models cannot be distinguished by frequency data and by bias data at only one redshift.
© 2010. The American Astronomical Society. All rights reserved.