Synopsis
The XSPEC rdblur convolution model: convolve with the diskline model shape
Syntax
xsrdblur The xsrdblur model is a convolution model component.
Description
The model is described at [1] .
Example
>>> create_model_component("xsrdblur", "mdl")
>>> print(mdl)Create a component of the xsrdblur model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.Betor10 frozen -2 -10 20 mdl.Rin_M frozen 10 6 10000 mdl.Rout_M frozen 1000 0 1e+07 mdl.Incl thawed 30 0 90 deg
ATTRIBUTES
The attributes for this object are:
| Attribute | Definition |
|---|---|
| Betor10 | The power law dependence of emissivity: see [1] for more details. |
| Rin_M | The inner radius, in units of GM^2/c. |
| Rout_M | The outer radius, in units of GM^2/c. |
| Incl | The inclination, in degrees. |
Notes
Unlike XSPEC, the convolution model is applied directly to the model, or models, rather than using the multiplication symbol.
References
Changes in CIAO
Added in CIAO 4.13
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.
See Also
- models
- xsdiskline