A review arguing that the galaxy distribution's fractal dimension is best measured with the structure function, and that the canonical correlation length understates the clustering scale.
New 3D data indicate that at large separations (r >100h −1 Mpc) the fractal dimension approaches the limitD(r) = 3
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Fractal properties of the cosmic web
A review arguing that the galaxy distribution's fractal dimension is best measured with the structure function, and that the canonical correlation length understates the clustering scale.