2. Analysis threads

• 2.1. Fitting a CCD spectrum
• 2.2. Modeling particle background
• 2.3. Fitting interstellar dust absorption
• 2.4. Import UV/Optical data
• 2.5. PION setup for AGN warm absorber
• 2.6. PION setup for emission and absorption features in AGN
• 2.7. Fitting two different spectra simultaneously
• 2.8. How to use the SPEX user model