30 June 2001

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Table of Contents

The 2dF Galaxy Redshift Survey The 2dFGRS Team Benchmark Surveys Effective sizes of z-surveys The 2dF facility The Anglo-Australian Telescope 2dF on the AAT Configuring the fibers Data pipeline: real-time spectra 2dFGRS input catalogue 2dF Galaxy Redshift Survey Regions Directions of Survey Strips Magnitude Limit Mask Tiling the sky Sky Coverage of Survey Redshift Completeness Mask Sampling & Uniformity Data pipeline: real-time redshifts Redshift yield Completeness Redshift distribution Redshift cone plot - June 2001 Redshift cone plot - 100k Release Cone diagram: all declinations Cone diagram: 4-degree wedge Galaxy & QSO surveys Cosmology & LSS - goals Models vs Observations Effect of baryons on P(k) Cosmology from CMB observations The power spectrum Real and z-space power spectra

Power spectrum - detail Survey window function Effect of window Tests on mock data Fits to power spectrum CDM model fitting Consistency with other constraints Redshift-space distortions - theory Redshift-space distortions Beta and Omega Clustering and Luminosity Cosmology from beta and CMB Biasing, Omega and Inflation The Galaxy Population Galaxy Luminosity Function Spectral classification by PCA LFs by spectral type Infrared luminosity functions Bivariate Brightness Distribution Luminosity dependence of clustering 1 Luminosity dependence of clustering 2 Luminosity dependence of clustering 3 Luminosity dependence of clustering 4 Clustering by spectral type - early types Clustering by spectral type - late types Clusters and Environment Stellar populations & environment Radio Galaxies, AGN and more Emission-line galaxies Public Release of Data 2dFGRS - The Movie