Spectral modelsΒΆ
For more information on the definition of spectral components and the different types, see Different types of spectral components. Currently the following models are implemented in SPEX:
- Absm: Morrison & McCammon absorption model
- Amol: interstellar dust absorption model
- APEC: collisional ionisation equilibrium model (External)
- Bb: blackbody model
- Cf: isobaric cooling flow differential emission measure model
- Cie: collisional ionisation equilibrium model
- Clus: projected cluster model
- Comt: comptonisation model
- CX: model for charge exchange plasmas
- Dabs: dust absorption model
- Dbb: disk blackbody model
- Delt: delta line model
- Dem: differential emission measure model
- Dust: dust scattering model
- Ebv: Galactic interstellar extinction model
- Etau: simple transmission model
- Euve: EUVE absorption model
- File: model read from a file
- Gain: Modify the energy scale of the model to compensate instrumental gain errors
- Gaus: gaussian line model
- Hot: collisional ionisation equilibrium absorption model
- Hyd: model with user-own hydrodynamical simulation
- Knak: segmented power law transmission model
- Laor: relativistic line broadening model
- Line: transmission model for a single spectral line
- Lpro: spatial broadening model
- Mbb: modified blackbody model
- Musr: User defined multiplicative model
- Neij: non-equilibrium ionisation jump model
- Pdem: DEM models
- Pion: SPEX photoionised plasma model
- Pow: power law model
- Reds: redshift model
- Refl: reflection model
- Rrc: radiative recombination continuum model
- Slab: thin slab absorption model
- Spei: relativistic line broadening model
- Spln: spline continuum model
- SSD: Shakura-Sunyaev disk model
- Tpho: Time-dependent, non-equilibrium, photoionised plasma model
- User: User defined model
- Vblo: rectangular velocity broadening model
- Vcom: Compton shoulder broadening model
- Vgau: gaussian velocity broadening model
- Vpro: velocity profile broadening model
- Warm: continuous photoionised absorption model
- Wdem: power law differential emission measure model
- Xabs: photoionised absorption model