Abstract
Observations of redshift-space distortions in spectroscopic galaxy surveys offer an attractive method for observing the build-up of cosmological structure, which depends both on the expansion rate of the Universe and our theory of gravity. In this paper, we present a formalism for forecasting the constraints on the growth of structure which would arise in an idealized survey. This Fisher matrix based formalism can be used to study the power and aid in the design of future surveys.
Original language | English |
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Pages (from-to) | 1348-1354 |
Number of pages | 7 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 397 |
Issue number | 3 |
DOIs | |
Publication status | Published - Aug 2009 |