4. Spectral models

• 4.1. Overview of spectral components
  • 4.1.1. Absm: Morrison & McCammon absorption model
  • 4.1.2. Amol: interstellar dust absorption model
  • 4.1.3. Bb: blackbody model
  • 4.1.4. Cf: isobaric cooling flow differential emission measure model
  • 4.1.5. Cie: collisional ionisation equilibrium model
  • 4.1.6. Clus: projected cluster model
  • 4.1.7. Comt: comptonisation model
  • 4.1.8. CX: model for charge exchange plasmas
  • 4.1.9. Dabs: dust absorption model
  • 4.1.10. Dbb: disk blackbody model
  • 4.1.11. Delt: delta line model
  • 4.1.12. Dem: differential emission measure model
  • 4.1.13. Dust: dust scattering model
  • 4.1.14. Ebv: Galactic interstellar extinction model
  • 4.1.15. Etau: simple transmission model
  • 4.1.16. Euve: EUVE absorption model
  • 4.1.17. File: model read from a file
  • 4.1.18. Gain: Modify the energy scale of the model to compensate instrumental gain errors
  • 4.1.19. Gaus: gaussian line model
  • 4.1.20. Hot: collisional ionisation equilibrium absorption model
  • 4.1.21. Hyd: model with user-own hydrodynamical simulation
  • 4.1.22. Knak: segmented power law transmission model
  • 4.1.23. Laor: relativistic line broadening model
  • 4.1.24. Line: transmission model for a single spectral line
  • 4.1.25. Lpro: spatial broadening model
  • 4.1.26. Mbb: modified blackbody model
  • 4.1.27. Musr: User defined multiplicative model
  • 4.1.28. Neij: non-equilibrium ionisation jump model
  • 4.1.29. Pdem: DEM models
  • 4.1.30. Pion: SPEX photoionised plasma model
  • 4.1.31. Pow: power law model
  • 4.1.32. Reds: redshift model
  • 4.1.33. Refl: reflection model
  • 4.1.34. Rrc: radiative recombination continuum model
  • 4.1.35. Slab: thin slab absorption model
  • 4.1.36. Spei: relativistic line broadening model
  • 4.1.37. Spln: spline continuum model
  • 4.1.38. SSD: Shakura-Sunyaev disk model
  • 4.1.39. Tpho: Time-dependent, non-equilibrium, photoionised plasma model
  • 4.1.40. User: User defined model
  • 4.1.41. Vblo: rectangular velocity broadening model
  • 4.1.42. Vcom: Compton shoulder broadening model
  • 4.1.43. Vgau: gaussian velocity broadening model
  • 4.1.44. Vpro: velocity profile broadening model
  • 4.1.45. Warm: continuous photoionised absorption model
  • 4.1.46. Wdem: power law differential emission measure model
  • 4.1.47. Xabs: photoionised absorption model
• 4.2. Optimizing model performance
  • 4.2.1. Setting a maximum N
  • 4.2.2. Replacing secondary components by the file model
  • 4.2.3. Optimizing the number of threads