Synopsis
The XSPEC gadem model: plasma emission, multi-temperature with gaussian distribution of emission measure.
Syntax
xsgadem The xsgadem model is an additive model component.
Description
The model is described at [1] . The set_xsabund and get_xsabund functions change and return the current settings for the relative abundances of the metals. See the xsapec documentation for settings relevant to the APEC model (i.e. when switch=2 ).
Example
>>> create_model_component("xsgadem", "mdl") >>> print(mdl)
Create a component of the xsgadem model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.Tmean frozen 4 0.01 20 keV mdl.Tsigma thawed 0.1 0.01 100 keV mdl.nH frozen 1 1e-06 1e+20 cm^-3 mdl.abundanc frozen 1 0 10 mdl.Redshift frozen 0 -0.999 10 mdl.switch frozen 2 -3.40282e+38 3.40282e+38 mdl.norm thawed 1 0 1e+24
ATTRIBUTES
The attributes for this object are:
Attribute | Definition |
---|---|
Tmean | The mean temperature for the gaussian emission measure distribution, in keV. |
Tsigma | The sigma of the temperature distribution for the gaussian emission measure, in keV. |
nH | H density, in cm^-3. |
abundanc | The metal abundance of the plasma, as defined by the set_xsabund function. |
Redshift | The redshift of the plasma. |
switch | If 0, the mekal code is run to evaluate the model; if 1 then interpolation of the mekal data is used; if 2 then interpolation of APEC data is used. See [1] for more details. This parameter can not be thawed. |
norm | The normalization of the model. |
References
- [1] https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSmodelGadem.html
XSPEC version
CIAO 4.16 comes with support for version 12.13.1e of the XSPEC models. This can be checked with the following:
% python -c 'from sherpa.astro import xspec; print(xspec.get_xsversion())' 12.13.1e
Bugs
See the bugs pages on the Sherpa website for an up-to-date listing of known bugs.
See Also
- models
- xsvgadem