V2V3ToIdeal¶
-
class
jwst.transforms.
V2V3ToIdeal
(v3idlyangle, v2ref, v3ref, vparity, name='V2idl', **kwargs)[source]¶ Bases:
astropy.modeling.core.Model
Performs the transform from telescope V2,V3 to Ideal coordinate system. The two systems have the same origin - V2_REF, V3_REF.
Note: This model has no schema implemented - add if needed.
Attributes Summary
inputs
coorinates in the telescope (V2,V3) frame. outputs
x and y coordinates in the telescope Ideal frame. param_names
v2ref
v3idlyangle
v3ref
vparity
Methods Summary
__call__
(v2, v3[, model_set_axis, …])Evaluate this model using the given input(s) and the parameter values that were specified when the model was instantiated. evaluate
(v2, v3, v3idlyangle, v2ref, v3ref, …)param xidl, yidl: Coordinates in Ideal System [in arcsec] Attributes Documentation
-
inputs
= ('v2', 'v3')¶ coorinates in the telescope (V2,V3) frame.
Type: (‘v2’, ‘v3’)
-
outputs
= ('xidl', 'yidl')¶ x and y coordinates in the telescope Ideal frame.
Type: (‘xidl’, ‘yidl’)
-
param_names
= ('v3idlyangle', 'v2ref', 'v3ref', 'vparity')¶
-
v2ref
¶
-
v3idlyangle
¶
-
v3ref
¶
-
vparity
¶
Methods Documentation
-
__call__
(v2, v3, model_set_axis=None, with_bounding_box=False, fill_value=nan, equivalencies=None)¶ Evaluate this model using the given input(s) and the parameter values that were specified when the model was instantiated.
-