BBodyFreq¶
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class
sherpa.astro.models.
BBodyFreq
(name='bbodyfreq')[source] [edit on github]¶ Bases:
sherpa.models.model.RegriddableModel1D
A one-dimensional Blackbody model (frequency).
This model can be used when the independent axis is in frequency space.
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T
¶ The temperature if the blackbody, in Kelvin.
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ampl
¶ The amplitude of the blackbody component.
See also
Notes
The blackbody emission is calculated as a function of frequency (v) using Wien’s law (hv >> kT):
f(v) = ampl * 2 * h * v^3 * exp(-h * v / (k * T)) / c^2where T is the blackbody temperature in Kelvin, h is Planck’s constant, k is Boltzmann’s constant, and c the speed of light.
Attributes Summary
thawedparhardmaxes
thawedparhardmins
thawedparmaxes
thawedparmins
thawedpars
Methods Summary
apply
(outer, *otherargs, **otherkwargs)calc
(pars, xlo, *args, **kwargs)get_center
()guess
(dep, *args, **kwargs)Set an initial guess for the parameter values. regrid
(*arrays)reset
()set_center
(*args, **kwargs)startup
()Called before a model may be evaluated multiple times. teardown
()Called after a model may be evaluated multiple times. Attributes Documentation
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thawedparhardmaxes
¶
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thawedparhardmins
¶
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thawedparmaxes
¶
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thawedparmins
¶
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thawedpars
¶
Methods Documentation
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apply
(outer, *otherargs, **otherkwargs) [edit on github]¶
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calc
(pars, xlo, *args, **kwargs) [edit on github]¶
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get_center
() [edit on github]¶
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guess
(dep, *args, **kwargs)[source] [edit on github]¶ Set an initial guess for the parameter values.
Attempt to set the parameter values, and ranges, for the model to match the data values. This is intended as a rough guess, so it is expected that the model is only evaluated a small number of times, if at all.
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regrid
(*arrays) [edit on github]¶
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reset
() [edit on github]¶
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set_center
(*args, **kwargs) [edit on github]¶
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startup
() [edit on github]¶ Called before a model may be evaluated multiple times.
See also
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teardown
() [edit on github]¶ Called after a model may be evaluated multiple times.
See also
setup()
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