Synopsis
The XSPEC vvapec model: APEC emission spectrum.
Syntax
xsvvapec The xsvvapec model is an additive model component.
Description
The model is described at [1] , with xsapec describing how it is implemented in Sherpa.
Example
>>> create_model_component("xsvvapec", "mdl")
>>> print(mdl)Create a component of the xsvvapec model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.kT thawed 6.5 0.0808 68.447 keV mdl.H frozen 1 0 1000 mdl.He frozen 1 0 1000 mdl.Li frozen 1 0 1000 mdl.Be frozen 1 0 1000 mdl.B frozen 1 0 1000 mdl.C frozen 1 0 1000 mdl.N frozen 1 0 1000 mdl.O frozen 1 0 1000 mdl.F frozen 1 0 1000 mdl.Ne frozen 1 0 1000 mdl.Na frozen 1 0 1000 mdl.Mg frozen 1 0 1000 mdl.Al frozen 1 0 1000 mdl.Si frozen 1 0 1000 mdl.P frozen 1 0 1000 mdl.S frozen 1 0 1000 mdl.Cl frozen 1 0 1000 mdl.Ar frozen 1 0 1000 mdl.K frozen 1 0 1000 mdl.Ca frozen 1 0 1000 mdl.Sc frozen 1 0 1000 mdl.Ti frozen 1 0 1000 mdl.V frozen 1 0 1000 mdl.Cr frozen 1 0 1000 mdl.Mn frozen 1 0 1000 mdl.Fe frozen 1 0 1000 mdl.Co frozen 1 0 1000 mdl.Ni frozen 1 0 1000 mdl.Cu frozen 1 0 1000 mdl.Zn frozen 1 0 1000 mdl.Redshift frozen 0 -0.999 10 mdl.norm thawed 1 0 1e+24
ATTRIBUTES
The attributes for this object are:
| Attribute | Definition |
|---|---|
| kT | The temperature of the plasma, in keV. |
| H, He, Li, Be, B, C, N, O, F, Ne, Na, Mg, Al, Si, P, S, Cl, Ar, K, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn | The abundance of the element in solar units. |
| Redshift | The redshift of the plasma. |
| norm | The normalization of the model: see [1] for an explanation of the units. |
References
- [1] https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSmodelApec.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.