Best‐fit correlation lengths, ﹩r_{0}﹩, in this work and from other studies. For this work (filled symbols), the fits were performed with γ fixed at 1.8. The solid line shows the "stable clustering" prediction (e.g., Peebles 1993) for ﹩\gamma =1.8﹩ with ﹩r_{0}=9.0﹩ Mpc at ﹩z=0﹩. The results of the other work have been transformed to ﹩h=0.6﹩ and proper coordinates. Error bars on the solid points are based only on bootstrap resampling and therefore represent lower limits to the true uncertainties. The error bars on the Le Fevre et al. (1996) points are likely incorrect; see text. It should be noted that the other work is heterogeneous, with galaxies selected in many different ways, in different magnitude and redshift ranges, with different assumed or fit values of γ, and in different cosmographic models. See the original references for details. The dotted and dashed lines show theoretical predictions.