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mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
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#include "../../catch2/catch.hpp"#include <vector>#include <Eigen/Dense>#include "../../../include/math/func/gaussian.hpp"#include "../../../include/improc/imageXCorrDiscrete.hpp"#include "../../../include/improc/eigenCube.hpp"#include "../../../include/ioutils/fits/fitsFile.hpp"Go to the source code of this file.
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| SCENARIO ("Verify X-Corr with center of light calculation", "[improc::imageXCorrDiscrete]") | |
| SCENARIO | ( | "Verify X-Corr with center of light calculation" | , |
| "" | [improc::imageXCorrDiscrete] | ||
| ) |
Scenario: centroiding Gaussians with center of light
Verify center of light calculation
Definition at line 21 of file imageXCorrDiscrete_test.cpp.
References mx::improc::imageCenterOfLight(), mx::improc::imageXCorrDiscrete< _ccImT >::m_ccIm, mx::improc::imageXCorrDiscrete< _ccImT >::m_refIm, mx::improc::imageXCorrDiscrete< _ccImT >::refIm(), and mx::fits::fitsFile< dataT >::write().