EmissionGaussian¶
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class
sherpa.astro.optical.EmissionGaussian(name='emissiongaussian')[source]¶ Bases:
sherpa.models.model.ArithmeticModelGaussian function for modeling emission.
It is for use when the independent axis is in Angstroms.
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fwhm¶ The full-width half-maximum of the model in km/s.
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pos¶ The center of the gaussian, in Angstroms.
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flux¶ The normalisation of the gaussian.
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skew¶ The skew of the gaussian.
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limit¶ The model is only evaluated for points that lie within limit sigma of pos. It is a hidden parameter, with a default value of 4.
See also
AbsorptionGaussian,EmissionLorentz,EmissionVoigt,LogEmissionNotes
The functional form of the model for points is:
f(x) = flux * exp(-0.5 * d(x)^2) / s2 if skew = 1 = 2 * flux * exp(-0.5 * d2(x)^2) / (s2 * (1 + skew)) otherwise d(x) = (x - pos) / s d2(x) = d(x) if x <= pos = d(x) / skew otherwise s2 = 2.50662828 * s s = pos * fwhm / (2.9979e5 * 2.354820044)
and for integrated data sets the low-edge of the grid is used.
The calculation is only done for those points that are in the range:
|x - pos| < limit * sigma
Outside this range the model is set to 0.
Attributes Summary
thawedparhardmaxesthawedparhardminsthawedparmaxesthawedparminsthawedparsMethods Summary
apply(outer, \*otherargs, \*\*otherkwargs)calc(p, x[, xhi])get_center()guess(dep, \*args, \*\*kwargs)Set an initial guess for the parameter values. reset()set_center(\*args, \*\*kwargs)startup()teardown()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)¶
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get_center()¶
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guess(dep, *args, **kwargs)¶ 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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reset()¶
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set_center(*args, **kwargs)¶
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startup()¶
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teardown()¶
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