astropy:docs

Chebyshev1D

class astropy.modeling.polynomial.Chebyshev1D(degree, domain=None, window=[-1, 1], n_models=None, model_set_axis=None, **params)[source] [edit on github]

Bases: astropy.modeling.polynomial.PolynomialModel

1D Chebyshev polynomial of the 1st kind.

Parameters:

degree : int

degree of the series

domain : list or None

window : list or None

If None, it is set to [-1,1] Fitters will remap the domain to this window

param_dim : int

number of parameter sets

**params : dict

keyword : value pairs, representing parameter_name: value

Other Parameters:
 

fixed : a dict

A dictionary {parameter_name: boolean} of parameters to not be varied during fitting. True means the parameter is held fixed. Alternatively the fixed property of a parameter may be used.

tied : dict

A dictionary {parameter_name: callable} of parameters which are linked to some other parameter. The dictionary values are callables providing the linking relationship. Alternatively the tied property of a parameter may be used.

bounds : dict

A dictionary {parameter_name: boolean} of lower and upper bounds of parameters. Keys are parameter names. Values are a list of length 2 giving the desired range for the parameter. Alternatively the min and max properties of a parameter may be used.

eqcons : list

A list of functions of length n such that eqcons[j](x0,*args) == 0.0 in a successfully optimized problem.

ineqcons : list

A list of functions of length n such that ieqcons[j](x0,*args) >= 0.0 is a successfully optimized problem.

Methods Summary

__call__(*inputs, **kwargs) Transforms data using this model.
clenshaw(x, coeff) Evaluates the polynomial using Clenshaw’s algorithm.
fit_deriv(x, *params) Computes the Vandermonde matrix.

Methods Documentation

__call__(*inputs, **kwargs)[source] [edit on github]

Transforms data using this model.

Parameters:

x : scalar, list or array

input

clenshaw(x, coeff)[source] [edit on github]

Evaluates the polynomial using Clenshaw’s algorithm.

fit_deriv(x, *params)[source] [edit on github]

Computes the Vandermonde matrix.

Parameters:

x : ndarray

input

params : throw away parameter

parameter list returned by non-linear fitters

Returns:

result : ndarray

The Vandermonde matrix

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