The shape of the two-point correlation function - Evidence for a double power law

Details The shape of the two-point correlation function - Evidence for a double power law The shape of the two-point correlation function - Evidence for a double power law

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...398..429c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 398, no. 2, p. 429-440.

Statistics

Computation

15

Computational Astrophysics, Galactic Clusters, Statistical Correlation, Universe, Angular Correlation, Infrared Astronomy Satellite, Power Spectra, Red Shift, Sky Surveys (Astronomy)

Scientific paper

The two-point galaxy correlation functions for three samples of galaxies are studied to determine a suitable model based on a Chi-square analysis. A double-power-law model is shown to generally describe the samples over the large range of separations, and the fit obtained agrees with studies based on redshift separations. The analysis suggests that the double power law is geometrical, and the function for galactic clusters is the same as that for large-scale galactic formations.

Affiliated with

Also associated with

No associations

Rating

The shape of the two-point correlation function - Evidence for a double power law does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The shape of the two-point correlation function - Evidence for a double power law, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The shape of the two-point correlation function - Evidence for a double power law will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1869626