Synopsis
The XSPEC rfxconv convolution model: angle-dependent reflection from an ionized disk
Syntax
xsrfxconv The xsrfxconv model is a convolution model component.
Description
The model is described at [1] .
Example
>>> create_model_component("xsrfxconv", "mdl") >>> print(mdl)
Create a component of the xsrfxconv model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.rel_refl thawed -1 -1 1e+06 mdl.redshift frozen 0 0 4 mdl.Fe_abund frozen 1 0.5 3 mdl.cosIncl frozen 0.5 0.05 0.95 mdl.log_xi thawed 1 1 6
ATTRIBUTES
The attributes for this object are:
Attribute | Definition |
---|---|
rel_refl | The relative reflection normalization. If negative then only the reflected component is returned. |
redshift | The redshift of the source. |
Fe_abund | The iron abundance relative to the solar abundance, as set by the set_xsabund function. All other elements are assumed to have Solar abundances. |
cosIncl | The cosine of the inclination angle in degrees. |
log_xi | The ionization parameter used by the table models. |
Notes
Unlike XSPEC, the convolution model is applied directly to the model, or models, rather than using the multiplication symbol.
The precision of the numerical integration can be changed by using the set_xsxset function to set the value of the RFXCONV_PRECISION keyword, which defines the fractional precision. The default is 0.01 (1%).
References
- [1] https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSmodelRfxconv.html
Changes in CIAO
Added in CIAO 4.13
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.
See Also
- models
- xsxilconv