BrokenPowerLaw1D¶
-
class
astropy.modeling.powerlaws.BrokenPowerLaw1D(amplitude=1, x_break=1, alpha_1=1, alpha_2=1, **kwargs)[source]¶ Bases:
astropy.modeling.Fittable1DModelOne dimensional power law model with a break.
- Parameters
- amplitudefloat
Model amplitude at the break point.
- x_breakfloat
Break point.
- alpha_1float
Power law index for x < x_break.
- alpha_2float
Power law index for x > x_break.
See also
Notes
Model formula (with \(A\) for
amplitudeand \(\alpha_1\) foralpha_1and \(\alpha_2\) foralpha_2):\[\begin{split}f(x) = \left \{ \begin{array}{ll} A (x / x_{break}) ^ {-\alpha_1} & : x < x_{break} \\ A (x / x_{break}) ^ {-\alpha_2} & : x > x_{break} \\ \end{array} \right.\end{split}\]Attributes Summary
This property is used to indicate what units or sets of units the evaluate method expects, and returns a dictionary mapping inputs to units (or
Noneif any units are accepted).Methods Summary
evaluate(x, amplitude, x_break, alpha_1, alpha_2)One dimensional broken power law model function
fit_deriv(x, amplitude, x_break, alpha_1, …)One dimensional broken power law derivative with respect to parameters
Attributes Documentation
-
alpha_1= Parameter('alpha_1', value=1.0)¶
-
alpha_2= Parameter('alpha_2', value=1.0)¶
-
amplitude= Parameter('amplitude', value=1.0)¶
-
input_units¶
-
param_names= ('amplitude', 'x_break', 'alpha_1', 'alpha_2')¶
-
x_break= Parameter('x_break', value=1.0)¶
Methods Documentation