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Large-scale structure as a cosmological probe
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Cosmology with Large-Scale Structure - Lecture 1
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- 1 Large-scale structure as a cosmological probe
- 2 What we learn from LSS
- 3 Lecture plan
- 4 Statistical approach: Poisson clustering hypothesis
- 5 Bias: relating mass and light
- 6 Models for bias
- 7 High-peak bias
- 8 Testing the biased CDM linear P(k)
- 9 Projected clustering
- 10 1990: APM angular correlations, w(e)
- 11 Weighing the universe with horizons
- 12 The argument for A: 1990 LSS + CMB
