Synopsis
The XSPEC TBfeo model: ISM grain absorption.
Syntax
xstbfeo The xstbfeo model is a multiplicative model component.
Description
The model is described at [1] .
Example
>>> create_model_component("xstbfeo", "mdl") >>> print(mdl)
Create a component of the xstbfeo 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.O frozen 1 -1e+38 1e+38 mdl.Fe frozen 1 -1e+38 1e+38 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). |
O | Oxygen abundance relative to Solar. |
Fe | Iron abundance relative to Solar. |
redshift | The redshift of the absorber. |
Notes
The `set_xsabund` function changes the relative abundances of the elements, in particular the "wilm" setting.
References
- [1] https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSmodelTbabs.html
Changes in CIAO
Changed in CIAO 4.17
The O and Fe parameters are now frozen by default to match XSPEC.
XSPEC version
CIAO 4.17 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.