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Large-Scale Structure of the Universe

Cosmological Principles and Expansion → Cosmic Web

This learning path guides undergraduate astronomy and physics students through the principles and methods used to describe the distribution of matter in the universe on large scales. It covers the statistical tools (correlation functions and power spectra), key cosmological phenomena (baryon acoustic oscillations and redshift-space distortions), and the cosmic web, grounding them in essential background in cosmology and survey astronomy.

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9 steps · 9 nodes · 3 stages

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Path Steps

9 steps · 3 stages. Click any step to inspect it and see it on the Path Map.

Stage 1

Foundation

3 steps

Stage 2

Core Concepts

3 steps

Stage 3

Advanced Topics

3 steps

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