IdealToV2V3¶

class jwst.transforms.IdealToV2V3(v3idlyangle, v2ref, v3ref, vparity, name='idl2V', **kwargs)[source]¶

Bases: astropy.modeling.core.Model

Performs the transform from Ideal to telescope V2,V3 coordinate system. The two systems have the same origin: V2_REF, V3_REF.

Note: This model has no schema implemented - add schema if needed.

Attributes Summary

`n_inputs`	The number of inputs.
`n_outputs`	The number of outputs.
`param_names`	Names of the parameters that describe models of this type.
`v2ref`
`v3idlyangle`
`v3ref`
`vparity`

Methods Summary

__call__(*inputs[, model_set_axis, …])

Evaluate this model using the given input(s) and the parameter values that were specified when the model was instantiated.

evaluate(xidl, yidl, v3idlyangle, v2ref, …)

param xidl: Coordinates in Ideal System [in arcsec]

Attributes Documentation

n_inputs = 2¶: The number of inputs.

n_outputs = 2¶: The number of outputs.

param_names = ('v3idlyangle', 'v2ref', 'v3ref', 'vparity')¶

Names of the parameters that describe models of this type.

The parameters in this tuple are in the same order they should be passed in when initializing a model of a specific type. Some types of models, such as polynomial models, have a different number of parameters depending on some other property of the model, such as the degree.

When defining a custom model class the value of this attribute is automatically set by the Parameter attributes defined in the class body.

v2ref = Parameter('v2ref', value=nan)¶

v3idlyangle = Parameter('v3idlyangle', value=nan)¶

v3ref = Parameter('v3ref', value=nan)¶

vparity = Parameter('vparity', value=nan)¶

Methods Documentation

__call__(*inputs, model_set_axis=None, with_bounding_box=False, fill_value=nan, equivalencies=None, inputs_map=None, **new_inputs)¶: Evaluate this model using the given input(s) and the parameter values that were specified when the model was instantiated.

static evaluate(xidl, yidl, v3idlyangle, v2ref, v3ref, vparity)[source]¶

Parameters

xidl (ndarray-like) – Coordinates in Ideal System [in arcsec]
yidl (ndarray-like) – Coordinates in Ideal System [in arcsec]
v3idlyangle (float) – Angle between Ideal Y-axis and V3 [ in deg]
v2ref (ndarray-like) – Coordinates in V2, V3 [in arcsec]
v3ref (ndarray-like) – Coordinates in V2, V3 [in arcsec]
vparity (int) – Parity.

Returns

v2, v3 – Coordinates in the (V2, V3) telescope system [in arcsec].

Return type

ndarray-like