Image Details
Caption: Fig. 9.
Evolution of biasing parameters ﹩b_{\mathrm{cov}\,}﹩, ﹩r_{\mathrm{corr}\,}﹩, ﹩\epsilon _{\mathrm{scatt}\,}﹩, and ﹩\epsilon _{\mathrm{nl}\,}﹩ for galaxies (solid lines), dark halos (dotted lines), and the theoretical predictions by TS (long‐dashed lines).
© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.