Image Details
Caption: Fig. 8.
Pair statistics (Nc and Lc) are given for SSRS2 (﹩\left< z\right>=0.015﹩) and CNOC2 (﹩\left< z\right>=0.30﹩). Measurements are given for ﹩r^{\mathrm{max}\,}_{p}=20﹩ h−1 kpc (bottom), ﹩r^{\mathrm{max}\,}_{p}=50﹩ h−1 kpc (middle), and ﹩r^{\mathrm{max}\,}_{p}=100﹩ h−1 kpc (top). Best‐fit lines indicate evolution varying as ﹩( 1+z) ^{m}﹩. For ﹩r^{\mathrm{max}\,}_{p}=( 20,\ 50,\ 100) ﹩ h−1 kpc, values of m used are (1.44, 2.26, 1.66) for Nc and (1.34, 2.28, 1.70) for Lc. Increases in both Nc and Lc with redshift are seen for all three choices of ﹩r^{\mathrm{max}\,}_{p}﹩.
© 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.