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SimulatedPSF Overview

Query Form

Attribute nameAttribute typeDocstringUnit
DistortionModelDataContainerThe telescope distortion at the field position specified by the X, Y values in the wavefront image, and calculated the four coefficients of the affine transformation. This is the RAYFILE used in the Lance Miller code.
ImageSizefloatImag esize in pixels.
ListOfWavelengthsListOfDoubleListOfWavelengths
PixelScalefloatSize of the pixel in microns.
SimulatedPSFFileDataContainerThis fits file corresponds to the PSF processed from the WFE.
WFEWaveFrontErrorMapWFE
XYFieldPosListOfDoubleThis is the position in the FPA for which the PSF is processed.

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