Chebyshev1D¶

class
astropy.modeling.polynomial.
Chebyshev1D
(degree, domain=None, window=[1, 1], n_models=None, model_set_axis=None, name=None, meta=None, **params)[source] [edit on github]¶ Bases:
astropy.modeling.polynomial.PolynomialModel
Univariate Chebyshev series.
It is defined as:
\[P(x) = \sum_{i=0}^{i=n}C_{i} * T_{i}(x)\]where
T_i(x)
is the corresponding Chebyshev polynomial of the 1st kind.Parameters: degree : int
degree of the series
domain : list or None, optional
window : list or None, optional
If None, it is set to [1,1] Fitters will remap the domain to this window
**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 thefixed
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 thetied
property of a parameter may be used.bounds : dict
eqcons : list
A list of functions of length
n
such thateqcons[j](x0,*args) == 0.0
in a successfully optimized problem.ineqcons : list
A list of functions of length
n
such thatieqcons[j](x0,*args) >= 0.0
is a successfully optimized problem.Notes
This model does not support the use of units/quantities, because each term in the sum of Chebyshev polynomials is a polynomial in x  since the coefficients within each Chebyshev polynomial are fixed, we can’t use quantities for x since the units would not be compatible. For example, the third Chebyshev polynomial (T2) is 2x^21, but if x was specified with units, 2x^2 and 1 would have incompatible units.
Attributes Summary
inputs
outputs
Methods Summary
__call__
(x[, model_set_axis, …])Evaluate this model using the given input(s) and the parameter values that were specified when the model was instantiated. clenshaw
(x, coeffs)Evaluates the polynomial using Clenshaw’s algorithm. evaluate
(x, *coeffs)Evaluate the model on some input variables. fit_deriv
(x, *params)Computes the Vandermonde matrix. prepare_inputs
(x, **kwargs)This method is used in __call__
to ensure that all the inputs to the model can be broadcast into compatible shapes (if one or both of them are input as arrays), particularly if there are more than one parameter sets.Attributes Documentation

inputs
= ('x',)¶

outputs
= ('y',)¶
Methods Documentation

__call__
(x, model_set_axis=None, with_bounding_box=False, fill_value=nan, equivalencies=None) [edit on github]¶ Evaluate this model using the given input(s) and the parameter values that were specified when the model was instantiated.

static
clenshaw
(x, coeffs)[source] [edit on github]¶ Evaluates the polynomial using Clenshaw’s algorithm.

evaluate
(x, *coeffs)[source] [edit on github]¶ Evaluate the model on some input variables.

fit_deriv
(x, *params)[source] [edit on github]¶ Computes the Vandermonde matrix.
Parameters: x : ndarray
input
params : throw away parameter
parameter list returned by nonlinear fitters
Returns: result : ndarray
The Vandermonde matrix

prepare_inputs
(x, **kwargs)[source] [edit on github]¶ This method is used in
__call__
to ensure that all the inputs to the model can be broadcast into compatible shapes (if one or both of them are input as arrays), particularly if there are more than one parameter sets. This also makes sure that (if applicable) the units of the input will be compatible with the evaluate method.
