mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
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Go to the source code of this file.
Functions | |
SCENARIO ("compiling psdFilter", "[sigproc::psdFilter]") | |
SCENARIO ("filtering with psdFilter", "[sigproc::psdFilter]") | |
SCENARIO | ( | "compiling psdFilter" | , |
"" | [sigproc::psdFilter] | ||
) |
Scenario: compiling psdFilter
Verify compilation and initilization of the 3 ranks for psdFilter.
Definition at line 22 of file psdFilter_test.cpp.
SCENARIO | ( | "filtering with psdFilter" | , |
"" | [sigproc::psdFilter] | ||
) |
Verify filtering and noise normalization Conducts random noise tests, verifying that the resultant rms is within 2% of expected value on average over many trials. Results are usually better than 1%, but 2% makes sure we don't get false failures.
Definition at line 218 of file psdFilter_test.cpp.
References mx::sigproc::augment1SidedPSD(), mx::sigproc::augment1SidedPSDFreq(), mx::sigproc::frequencyGrid(), mx::improc::eigenCube< dataT >::image(), mx::astro::constants::k(), mx::sigproc::normPSD(), mx::improc::eigenCube< dataT >::pixel(), and mx::math::vectorVariance().