Transform analysis of the high-resolution Shane-Wirtanen Catalog - The power spectrum and the bispectrum

The two- and three-point galaxy correlation functions in Fourier transform space for wavelengths corresponding to theta ranging from 1/2 deg to 70 deg have been examined in order to extract statistical information from the high-resolution (10 arcmin) Shane-Wirtanen data and, in particular, to gain information about the large-scale behavior of galaxy clustering. There is no evidence for any transition in behavior of the power spectrum corresponding to the break in the two-point function at 2.5 deg, but this characteristic scale does appear in the bispectrum.