We are using the
AAT
Two-Degree Field
(2dF) to obtain redshifts for
> 25000 B < 21 QSOs in
two 75° × 5° declination strips
in the South Galactic Pole
and in an equatorial region at the North Galactic cap. The primary scientific aims
of the QSO survey are: (1) to obtain the primordial fluctuation power spectrum
out to COBE scales, (2) to determine the rate of QSO clustering evolution in the
non-linear and linear regimes and hence obtain new limits on the value of
and the bias parameter, (3) to apply a powerful geometric method to measure
.
A more detailed discussion of the above paragraph is available.
| The 2QZ team (Tue Jun 17 18:50:19 BST 2008 by RJS) |
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