Synopsis
The XSPEC vrnei model: non-equilibrium recombining collisional plasma.
Syntax
xsvrnei The xsvrnei model is an additive model component.
Description
The model is described at [1] . The set_xsxset and get_xsxset functions are used to set and query the XSPEC XSET parameters, in particular the keyword "NEIVERS".
Example
>>> create_model_component("xsvrnei", "mdl")
>>> print(mdl)Create a component of the xsvrnei model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.kT thawed 0.5 0.0808 79.9 keV mdl.kT_init thawed 1 0.0808 79.9 keV mdl.H frozen 1 0 1 mdl.He frozen 1 0 10000 mdl.C frozen 1 0 10000 mdl.N frozen 1 0 10000 mdl.O frozen 1 0 10000 mdl.Ne frozen 1 0 10000 mdl.Mg frozen 1 0 10000 mdl.Si frozen 1 0 10000 mdl.S frozen 1 0 10000 mdl.Ar frozen 1 0 10000 mdl.Ca frozen 1 0 10000 mdl.Fe frozen 1 0 10000 mdl.Ni frozen 1 0 10000 mdl.Tau thawed 1e+11 1e+08 5e+13 s/cm^3 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. |
| kT_init | The initial temperature of the plasma, in keV. |
| H | The H abundance: it should be set to 0 to switch on and 1 to switch off the free-free continuum. |
| He, C, N, O, Ne, Mg, Si, S, Ar, Ca, Fe, Ni | The abundance of the element, with respect to Solar. |
| Tau | The ionization timescale in units of s/cm^3. |
| 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/XSmodelRnei.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.