Synopsis
The XSPEC cpflux convolution model: calculate photon flux
Syntax
xscpflux The xscpflux model is a convolution model component.
Description
The model is described at [1] .
Example
>>> create_model_component("xscpflux", "mdl") >>> print(mdl)
Create a component of the xscpflux model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.Emin frozen 0.5 0 1e+06 keV mdl.Emax frozen 10 0 1e+06 keV mdl.Flux thawed 1 0 1e+10
ATTRIBUTES
The attributes for this object are:
Attribute | Definition |
---|---|
Emin | Minimum energy over which the photon flux is calculated. |
Emax | Maximum energy over which the photon flux is calculated. |
Flux | photon flux in photon/cm^2/s |
Notes
Unlike XSPEC, the convolution model is applied directly to the model, or models, rather than using the multiplication symbol.
See [1] for the meaning and restrictions, in particular the necessity of freezing the amplitude, or normalization, of the emission component (or components) at 1.
References
- [1] https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSmodelCpflux.html
Changes in CIAO
Added in CIAO 4.13
XSPEC version
CIAO 4.16 comes with support for version 12.13.1e of the XSPEC models. This can be checked with the following:
% python -c 'from sherpa.astro import xspec; print(xspec.get_xsversion())' 12.13.1e
Bugs
See the bugs pages on the Sherpa website for an up-to-date listing of known bugs.