The 2dF Galaxy Redshift Survey

• Aim for LCRS X 10 = 250,000 z’s

• Increase sky coverage to get fully 3D sample

  • Measure -Mpc power
  • Test Gaussian nature of linear fluctuations
  • Measure redshift-space distortions

• Increase sampling density

  • Spatial distribution for different galaxy types
  • Tests of theories for biased galaxy formation

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