Bias and beyond
Abstract
Description
It is becoming increasingly clear that galaxy bias is complicated, with evidence indicating that it can be time-dependent, morphology-dependent, scale-dependent, non-linear and non-deterministic. We discuss strategies for overcoming these complications and performing precision cosmological tests with upcoming redshift surveys.
4 pages, with 1 figure included. Links and more figures at http://www.sns.ias.edu/~max/biasframe.html or from max@ias.edu. To appear in ``Wide Field Surveys in Cosmology'', S. Colombi and Y. Mellier (eds), Editions Frontieres (1998)
4 pages, with 1 figure included. Links and more figures at http://www.sns.ias.edu/~max/biasframe.html or from max@ias.edu. To appear in ``Wide Field Surveys in Cosmology'', S. Colombi and Y. Mellier (eds), Editions Frontieres (1998)