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Synthesis Tutorial
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This tutorial demonstrates the forward modeling (synthesis) workflow for MUSE spectroscopic observations.

The method involves:

1. **VDEM (Velocity-Differential Emission Measure)**: The emission measure (plasma brightness) as a function of velocity, temperature, and space within the field of view
2. **Response Functions**: Instrument-specific functions describing how the telescope and spectrograph respond to emission at different wavelengths, velocities, and temperatures
3. **Synthesis**: Combining VDEM with response functions to produce synthetic spectra
4. **Analysis**: Calculating spectral moments and comparing with observations
