Synopsis
The XSPEC cglumin convolution model: calculate luminosity
Syntax
xscglumin The xscglumin model is a convolution model component.
Description
The model is described at [1] .
Examples
Example 1
>>> create_model_component("xscglumin", "mdl")
>>> print(mdl)Create a component of the xscglumin 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.Distance frozen 10 0 1e+06 kpc mdl.lg10Lum thawed 40 -100 100 cgs
Example 2
With the following definitions:
>>> xscglumin.cglumin >>> xsphabs.absmdl >>> xspowerlaw.plmdl >>> xsgaussian.gmdl >>> srcmdl = plmdl + gmdl
then the model can be applied in a number of ways, such as:
>>> mdl1 = cglumin(absmdl * srcmdl) >>> mdl2 = absmdl * cglumin(srcmdl) >>> mdl3 = absmdl * (plmdl + cglumin(gmdl))
ATTRIBUTES
The attributes for this object are:
| Attribute | Definition |
|---|---|
| Emin | Minimum energy over which the luminosity is calculated. |
| Emax | Maximum energy over which the luminosity is calculated. |
| Distance | Distance to the source in kpc. |
| lg10Lum | log (base 10) of the luminosity in erg/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
Changes in CIAO
Added in CIAO 4.16
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.