Hostname: page-component-76fb5796d-x4r87 Total loading time: 0 Render date: 2024-04-25T16:55:22.813Z Has data issue: false hasContentIssue false
  • English
  • Français

Two-point Correlation Function and Power Spectrum at Very Large Scales

Published online by Cambridge University Press:  26 May 2016

Z.-G. Deng  and
X.-Y. Xia
Z.-G. Deng
Affiliation:
Graduate School, CAS and Beijing Astrophysical Center, CAS-PKU, Beijing 100039, China
X.-Y. Xia
Affiliation:
Tianjin Normal University and Beijing Astrophysical Center, CAS-PKU, Tianjin 300074, China

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Subsamples of galaxies with different morphological types have been sorted out from Stromlo-APM redshift survey. Two-point correlation function for each subsample has been calculated. The two-point correlation functions for all subsamples show very large scale fluctuation. We show that the two-point correlation function with fluctuation could be fitted by a modified power spectrum with power excess at wave number comparable to the scale of the fluctuation.

Type
Part XII: Poster Papers
Information
Symposium - International Astronomical Union , Volume 201: New Cosmological Data and the Values of the Fundamental Parameters , 2005 , pp. 449 - 450
Copyright
Copyright © Astronomical Society of the Pacific 2005 

References

Broadhurst, T. J., Ellis, R. S., Koo, D. C. & Szalay, A. S. 1990, Nature, 343, 726.Google Scholar
Deng, Z. G., Xia, X. Y. & Fang, L. Z. 1994, ApJ, 431, 506.Google Scholar
Eisenstein, D. J., Hu, W., Silk, J. & Szalay, A. S. 1998, ApJL, L1.Google Scholar
Mo, H. J., Deng, Z. G., Xia, X. Y., Schiller, P. & Börner, G. 1992, A&A, 257, 1.Google Scholar
Landy, S. D., Schectman, S. A., Lin, H., Kirshner, R. P., Oemler, A. A. & Tucker, D. 1996, ApJL, L1.Google Scholar