Model |
Description |
Ionized absorber. |
|
Extra absorption due to contamination on the ACIS filters. |
|
Gaussian line profile in wavelength space. |
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ASCA PSF mixing model. |
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APEC thermal plasma model. |
|
Additive table model. |
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Velocity broadened APEC thermal plasma model. |
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Blackbody spectrum, with redshift variant |
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Blackbody spectrum with norm proportional to surface area. |
|
E-folded broken power-law reflected from neutral matter |
|
E-folded broken power-law reflected from ionized matter |
|
Broken powerlaw. |
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Three-segment broken powerlaw. |
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Comptonization by relativistically moving matter. |
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Thermal bremsstrahlung, with redshift variant. |
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6th-order Chebyshev polynomial DEM using mekal and variants |
|
Compton scattering (non-relativistic) |
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Multi-temperature mekal. |
|
Cooling flow model. |
|
Calculate flux of other model components. |
|
Comptonized blackbody spectrum after Nishimura et al. 1986. |
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Comptonization spectrum after Lamb and Sanford 1979. |
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Thermal and bulk Comptonization for cylindrical accretion onto the polar cap of a magnetized neutron star. |
|
Comptonization spectrum after Poutanen and Svenson 1986. |
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Comptonization spectrum after Sunyaev and Titarchuk 1980. |
|
Thermal and bulk Comptonization of a seed blackbody-like spectrum. |
|
Comptonization spectrum after Titarchuk 1994. |
|
Energy-independent multiplicative factor. |
|
Convolution model to calculate photon flux. |
|
Non-physical model for low count background spectra. |
|
Powerlaw with high energy exponential rolloff. |
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Cyclotron absorption line. |
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Disk model. |
|
Multiple blackbody disk model. |
|
Irradiated inner and outer disk. |
|
Line emission from relativistic accretion disk. |
|
Disk model with gas pressure viscosity. |
|
Modified blackbody disk model. |
|
Accretion disk with power-law T(r). |
|
Accretion disk around a black hole. |
|
Dust scattering out of the beam. |
|
Absorption edge. |
|
Log-parabolic blazar model with vFv normalization. |
|
Paolo Coppi's hybrid hot plasma emission models. |
|
Equilibrium ionization collisional plasma model from Borkowski. |
|
Table model for exponential of -1 times the input. |
|
Low-energy exponential rolloff. |
|
Exponential decay |
|
Exponential factor. |
|
Multiple blackbody disk model with zero-torque inner boundary. |
|
Gaussian absorption line. |
|
Plasma emission, multi-temperature with gaussian distribution of emission measure. |
|
Simple gaussian line profile. |
|
Generalized single ionization NEI plasma model. |
|
GR accretion disk around a black hole. |
|
Gamma-ray burst model. |
|
Gaussian smoothing with an energy dependent sigma. |
|
Voigt absorption profiles for He I series. |
|
High energy cutoff. |
|
Simple reflection model good up to 15 keV. |
|
Reflection from ionized material. |
|
Convolve with the Laor model shape. |
|
Convolve with the Laor2 model shape. |
|
Multi-temperature blackbody model for thin accretion disk around a Kerr black hole. |
|
Accretion disk line shape with BH spin as a free parameter. |
|
Optically thick accretion disk around a Kerr black hole. |
|
Accretion disk line emission with BH spin as free parameter. |
|
Line from accretion disk around a black hole. |
|
Line from accretion disk with broken power-law emissivity around a black hole. |
|
Log-parabolic blazar model. |
|
Lorentzian line profile. |
|
Lorentzian smoothing with an energy dependent sigma. |
|
Voigt absorption profiles for H I or He II Lyman series. |
|
Mewe-Gronenschild-Kaastra thermal plasma (1992). |
|
Mewe-Kaastra-Liedahl thermal plasma (1995). |
|
Cooling flow model based on mekal. |
|
Multiplicative table model. |
|
Simple nonequilibrium ionization plasma model. |
|
Notch line absorption. |
|
Plane-parallel shock with ion and electron temperatures. |
|
Neutron star with hydrogen atmosphere |
|
Neutron star with hydrogen atmosphere for different g |
|
Neutron star H atmosphere with e- conduction and self-irradiation. |
|
Neutron star magnetic atmosphere. |
|
Neutron star with a magnetic atmosphere. |
|
Neutron star with a non-magnetic atmosphere. |
|
Pair plasma model. |
|
Thermally comptonized continuum. |
|
Colour temperature corrected disc and energetically coupled Comptonisation model for AGN. |
|
Convert absorption model into a partial covering absorption. |
|
Power-law distribution of neutral absorbers. |
|
Partial covering fraction absorption. |
|
Powerlaw with pegged normalization. |
|
Neutral Compton reflection with self-consistent Fe and Ni lines. |
|
Exponentially cut-off power-law reflected from neutral matter. |
|
Exponentially cut-off power-law reflected from ionized matter. |
|
Photo-electric absorption |
|
CCD pile-up model for Chandra |
|
Absorption model with power-law dependence on energy. |
|
Cut-off powerlaw observed through dense, cold matter. |
|
Positronium continuum. |
|
Simple photon power law. |
|
3-D to 2-D projection mixing model. |
|
Constant temperature, plane-parallel shock plasma model. |
|
Power-law distribution of neutral absorbers. |
|
Raymond-Smith thermal plasma. |
|
Convolve with the diskline model shape. |
|
Change correction norm for a spectrum (replaces old recornrm command). |
|
IR/optical/UV extinction from Cardelli et al. (1989) |
|
Recombination edge. |
|
reflection from neutral matter |
|
E-folded power-law reflected from an ionized relativistic disk. |
|
Non-equilibrium recombining collisional plasma. |
|
Sedov model with electron and ion temperatures. |
|
Comptonization of a seed spectrum. |
|
Multi-blackbody self-irradiated funnel model. |
|
Model for an optically-thin, spherically-symmetric thermal plasma. |
|
Smoothed absorption edge. |
|
Super-exponential cutoff absorption. |
|
Spline multiplicative factor. |
|
Synchrotron radiation from cut-off electron distribution. |
|
Synchrotron radiation from escape-limited electron distribution. |
|
Einstein Observatory SSS ice absorption. |
|
Step function convolved with gaussian. |
|
Suzaku PSF mixing model |
|
Absorption by partially ionized material with large velocity shear. |
|
Absorption due to the ISM including molecules and grains. |
|
UV reddening. |
|
Photoelectric absorption with variable abundances. |
|
Photoelectric absorption (Morrison & McCammon). |
|
Photoelectric absorption with low energy window. |
|
The reflected spectrum from a photo-ionized accretion disk. |
|
XMM PSF model |
|
Redshift an additive model. |
|
EUV ISM attenuation. |
|
Extinction by dust grains (Pei, 1992). |
|
UV/Optical attenuation by the intergalactic medium. |
|
Redshift a multiplicative model. |
|
Redshifted IR/optical/UV extinction from Cardelli et al. (1989) |
|
Extinction by dust grains in starburst galaxies. |
|
Redshifted absorption with variable iron abundance. |
|
Partial covering absorption by partially ionized material. |