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
- [1] https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSmodelRdblur.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
- xsdiskline