Summary

• 2dF survey status

  • Over 50,000 redshifts (20% of survey)
  • Expect 100,000 March 2000
  • 250,000 March 2001

• Preliminary results

  • Luminosity functions by spectral type
  • Correlations and redshift-space distortions

• Future issues

  • Clustering on 100-Mpc scales
  • Gaussian nature of density field
  • Clustering by spectral type and luminosity
  • Detailed tests of halo-based bias models

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