Synopsis
The XSPEC c6vmekl model: differential emission measure using Chebyshev representations with multi-temperature mekal.
Syntax
xsc6vmekl The xsc6vmekl model is an additive model component.
Description
The model is described at [1] .
Example
>>> create_model_component("xsc6vmekl", "mdl")
>>> print(mdl)Create a component of the xsc6vmekl model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.CPcoef1 thawed 1 -1 1 mdl.CPcoef2 thawed 0.5 -1 1 mdl.CPcoef3 thawed 0.5 -1 1 mdl.CPcoef4 thawed 0.5 -1 1 mdl.CPcoef5 thawed 0.5 -1 1 mdl.CPcoef6 thawed 0.5 -1 1 mdl.nH frozen 1 1e-06 1e+20 cm^-3 mdl.He frozen 1 0 10 mdl.C frozen 1 0 10 mdl.N frozen 1 0 10 mdl.O frozen 1 0 10 mdl.Ne frozen 1 0 10 mdl.Na frozen 1 0 10 mdl.Mg frozen 1 0 10 mdl.Al frozen 1 0 10 mdl.Si frozen 1 0 10 mdl.S frozen 1 0 10 mdl.Ar frozen 1 0 10 mdl.Ca frozen 1 0 10 mdl.Fe frozen 1 0 10 mdl.Ni frozen 1 0 10 mdl.redshift frozen 0 -0.999 10 mdl.switch frozen 1 -3.40282e+38 3.40282e+38 mdl.norm thawed 1 0 1e+24
ATTRIBUTES
The attributes for this object are:
| Attribute | Definition |
|---|---|
| CPcoef1, CPcoef2, CPcoef3, CPcoef4, CPcoef5, CPcoef6 | Chebyshev polynomial coefficients. |
| nH | H density, in cm^-3. |
| He, C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, Fe, Ni | The abundance relative to Solar. |
| 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/XSmodelC6mekl.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.