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

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

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...259..474f&link_type=abstract

Astrophysical Journal, Part 1, vol. 259, Aug. 15, 1982, p. 474-481.

Astronomy and Astrophysics

Astrophysics

46

Astronomical Catalogs, Fourier Transformation, Galactic Clusters, Power Spectra, Spectral Correlation, Statistical Analysis, Data Reduction, High Resolution, Spectral Resolution

Scientific paper

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.

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