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Observing the High-Energy Universe: X-ray and Gamma-ray Techniques

High-Energy Emission Processes → Spectral Fitting and Interpretation

This graduate-level learning path equips astrophysics students with the knowledge and skills to observe celestial sources in X-ray and gamma-ray bands. It covers the physics of high-energy emission, space-based detector technologies, data reduction (spectral extraction, background subtraction), source detection, and variability analysis, using real mission examples. The path emphasizes practical data analysis techniques essential for a career in high-energy astrophysics.

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12 steps · 12 nodes · 3 stages

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Path Steps

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

Stage 1

Foundation

4 steps

Stage 2

Core Concepts

4 steps

Stage 3

Advanced Topics

4 steps

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