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Scale-Dependence of Bias from APM-BGC Sample

Published online by Cambridge University Press:  25 May 2016

L. Z. Fang ,
Z. G. Deng  and
X. Y. Xia
L. Z. Fang
Affiliation:
Dept. of Physics, University of Arizona, Tucson, USA
Z. G. Deng
Affiliation:
Dept. of Physics, Graduate School, USTC, P. R. China
X. Y. Xia
Affiliation:
Dept. of Physics, Tianjin Normal University, P.R. China

Extract

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Applying a discrete wavelet transformation (DWT)1 to the spiral (SP) and elliptical+lenticular (EL) galaxies in A PM bright galaxy catalog (APMBGC)2, we investigated the scale-dependence of bias parameter b in the linear bias model

Type
IV. Structure Formation and Dark Matter
Information
Symposium - International Astronomical Union , Volume 183: Cosmological Parameters and the Evolution of the Universe , 1999 , pp. 271
Copyright
Copyright © Kluwer 1999 

References

1. Fang, L.Z. & Pando, J. 1997, The 5th Current Topics of Astrofundamental Physics, eds. Sanchez, N. & Zichichi, A., World Scientific; 1996, ApJ, 459, 1 Google Scholar
2. Loveday, L. (1996) MNRAS, 278, 1025 CrossRefGoogle Scholar