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A robust technique for estimating cosmological parameters
Martin A. Hendry
Dept. of Physics and Astronomy, Glasgow University, U.K.
The impact of observational selection e ects on the estimation of
cosmological parameters from galaxy redshift surveys is a topic of
considerable interest - and some controversy - in cosmology. We
present a new, non-parametric, technique for extracting informa-
tion from galaxy surveys which circumvents a number of prob-
lematic issues a ecting traditional, parametric, methods. Our
ROBUST technique builds on the C-method and allows deter-
mination of cosmological parameters free of almost any model as-
sumptions concerning the galaxy luminosity function and spatial
clustering. We also describe a related technique which provides
a non-parametric test of completeness in ux-limited galaxy sur-
veys.
We illustrate ROBUST by estimating the Hubble parameter and
linear bias parameter from recent redshift-distance data. We also
discuss applications to the study of the galaxy luminosity function
and testing the homogeneity of the Universe on large scales.
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