With \approx 10000 QSO redshifts , the 2dF QSO Redshift Survey ( 2QZ ) is already the biggest individual QSO survey .
The aim for the survey is to have \approx 25000 QSO redshifts , providing an order of magnitude increase in QSO clustering statistics .
We first describe the observational parameters of the 2dF QSO survey .
We then describe several highlights of the survey so far ; we present new estimates of the QSO luminosity function and the QSO correlation function .
We also present the first estimate of the QSO power spectrum from the 2QZ catalogue , probing the form of the fluctuation power-spectrum out to the \approx 1000h ^ { -1 } Mpc scales only previously probed by COBE .
We find a power spectrum which is steeper than the prediction of standard CDM and more consistent with the prediction of \Lambda -CDM .
The best-fit value for the power spectrum shape parameter for a range of cosmologies is \Gamma = 0.1 \pm 0.1 .
Finally , we discuss how the complete QSO survey will be able to constrain the value of \Omega _ { \Lambda } by combining results from the evolution of QSO clustering and from a geometric test of clustering isotropy .