astropy:docs

Polynomial2D

class astropy.modeling.polynomial.Polynomial2D(degree, x_domain=[-1, 1], y_domain=[-1, 1], x_window=[-1, 1], y_window=[-1, 1], n_models=None, model_set_axis=None, **params)[source] [edit on github]

Bases: astropy.modeling.polynomial.PolynomialModel

2D Polynomial model.

Represents a general polynomial of degree n:

P(x,y) = c_{00} + c_{10}x + ...+ c_{n0}x^n + c_{01}y + ...+ c_{0n}y^n
+ c_{11}xy + c_{12}xy^2 + ... + c_{1(n-1)}xy^{n-1}+ ... + c_{(n-1)1}x^{n-1}y

Parameters:

degree : int

highest power of the polynomial, the number of terms is degree+1

x_domain : list or None

domain of the x independent variable

y_domain : list or None

domain of the y independent variable

x_window : list or None

range of the x independent variable

y_window : list or None

range of the y independent variable

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.
fit_deriv(x, y, *params) Computes the Vandermonde matrix.
invlex_coeff()
mhorner(x, y, coeff) Multivariate Horner’s scheme

Methods Documentation

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

Transforms data using this model.

Parameters:

x : scalar, list or array

input

y : scalar, list or array

input

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

Computes the Vandermonde matrix.

Parameters:

x : ndarray

input

y : ndarray

input

params : throw away parameter

parameter list returned by non-linear fitters

Returns:

result : ndarray

The Vandermonde matrix

invlex_coeff()[source] [edit on github]
mhorner(x, y, coeff)[source] [edit on github]

Multivariate Horner’s scheme

Parameters:

x, y : array

coeff : array of coefficients in inverse lexical order

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