Synopsis
The XSPEC TBpcf model: ISM grain absorption.
Syntax
xstbpcf The xstbpcf model is a multiplicative model component.
Description
The model is described at [1] .
Example
>>> create_model_component("xstbpcf", "mdl")
>>> print(mdl)Create a component of the xstbpcf model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.nH thawed 1 0 1e+06 10^22 mdl.pcf thawed 0.5 0 1 mdl.redshift frozen 0 -1 10
ATTRIBUTES
The attributes for this object are:
| Attribute | Definition |
|---|---|
| nH | The equivalent hydrogen column (in units of 10^22 atoms/cm^2). |
| pcf | Partial covering fraction of the absorber. |
| redshift | The redshift of the absorber. |
Notes
The `set_xsabund` function changes the relative abundances of the elements, in particular the "wilm" setting.
References
XSPEC version
CIAO 4.18 comes with support for version 12.14.0k of the XSPEC models. This can be checked with the following:
% python -c 'from sherpa.astro import xspec; print(xspec.get_xsversion())' 12.14.0k
Bugs
See the bugs pages on the Sherpa website for an up-to-date listing of known bugs.