Path: SpacecraftEstimation/StellarModels
% Computes the angular resolution of the CCD. Assumes that the star is blurred so it fits within one pixel. This function ignores all real effects in a CCD such as dark current, blooming etc. ------------------------------------------------------------------------ Form: r = CCDRes( focalLength, wPixel, bits ) ------------------------------------------------------------------------ ------ Inputs ------ focalLength (1,1) Focal length (*) wPixel (1,1) Width of each cell bits (1,1) Number of bits per pixel * indicates any unit of length. ------- Outputs ------- r (1,1) Resolution (rad)
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