mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
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A class to register images using the Fourier cross correlation with a peak fit. More...
A class to register images using the Fourier cross correlation with a peak fit.
Definition in file imageXCorrFFT.hpp.
#include "../mxError.hpp"
#include "../mxException.hpp"
#include "../math/ft/fftT.hpp"
#include "../math/ft/mftT.hpp"
#include "../math/ft/ftUtils.hpp"
#include "../math/ft/fftwEnvironment.hpp"
#include "../math/fit/fitGaussian.hpp"
#include "eigenImage.hpp"
#include "imageUtils.hpp"
#include "imageTransforms.hpp"
#include "imageXCorr.hpp"
Go to the source code of this file.
Classes | |
class | mx::improc::imageXCorrFFT< _realImageT > |
Find the optimum shift to align two images using the FFT cross correlation. More... | |
Namespaces | |
namespace | mx |
The mxlib c++ namespace. | |