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Constraining Dark Energy with Multiple Probes

Cosmological Background and Dark Energy Basics → Future Dark Energy Surveys and Forecasts

This path equips graduate students in cosmology with the theoretical and data-analysis skills needed to combine independent cosmological probes—Type Ia supernovae, BAO, weak lensing, RSD, galaxy clusters, and CMB—to constrain dark energy. It covers the underlying physics, probe-specific observables, systematics, and the statistical methods for joint analysis, culminating in a synthesis and forward look to future surveys.

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13 steps · 13 nodes · 3 stages

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Path Steps

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

Stage 1

Foundation

5 steps

Stage 2

Core Concepts

4 steps

Stage 3

Advanced Topics

4 steps

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