Table of Contents
The 2dF galaxy redshift survey
Outline
History of galaxy clustering
Meaning of clustering
PPT Slide
PPT Slide
The 2dF Galaxy Redshift Survey
The 2dF Galaxy Redshift Survey
2dFGRS Survey Team
2dFGRS parameters
2dFGRS geometry
Tiling strategy
Sampling: 2dF vs LCRS
Calibrating photometry
Photometric calibrations
Recalibrated number counts
Deep CCD photometry
The 2dF site
The 2dF facility
2dF on the AAT
Configuring fibres
Data pipeline: real-time X-corr z’s
Example spectra
Survey status - August 1999
Redshift yield
Completeness
Surface brightness selection
Bivariate Brightness Distribution
Survey mask
Selection mask
Stellar contamination
Survey rate
Cone diagram: all declinations
Cone diagram: 4-degree wedge
The big picture
Redshift distribution
Overall luminosity function
Spectral classification by PCA
LFs by spectral type
Galaxy distribution by type
2D correlations x(s, p)
Model comparison - I
Model comparison - II
Projected correlations X(r)
The CDM clustering problem
The CDM Mach-number problem
Numerical galaxy formation
Antibias in LCDM
Dark-matter haloes and bias
Correlations from smooth haloes
Halo occupations depend on mass
Summary
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