DistortionModel | DataContainer | The 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. | |
ImageSize | float | Imag esize in pixels. | |
ListOfWavelengths | ListOfDouble | ListOfWavelengths | |
PixelScale | float | Size of the pixel in microns. | |
SimulatedPSFFile | DataContainer | This fits file corresponds to the PSF processed from the WFE. | |
WFE | WaveFrontErrorMap | WFE | |
XYFieldPos | ListOfDouble | This is the position in the FPA for which the PSF is processed. | |