mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
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Files related to astronomical adaptive optics
Files | |
file | aoPaths.hpp |
Standardized paths for the mx::AO system. | |
file | basis.hpp |
Utilities for working with a modal basis. | |
file | fourierBasis.hpp |
Generating a fourier basis. | |
file | influenceFunctions.hpp |
Utilities for generating and analyzing deformable mirror influence functions. | |
file | pupil.hpp |
Utilities for specifying pupils. | |
file | zernikeBasis.hpp |
Generating a Zernike basis. | |
file | aoAtmosphere.hpp |
Provides a class to specify atmosphere parameters. | |
file | aoConstants.hpp |
Calculate and provide constants related to adaptive optics. | |
file | aoPSDs.hpp |
Spatial power spectra used in adaptive optics. | |
file | aoSystem.hpp |
Declares and defines an analytical AO system. | |
file | aoWFS.hpp |
Definitions of various analytic wavefront sensors. | |
file | clAOLinearPredictor.hpp |
Provides a class to manage closed loop gain linear predictor determination. | |
file | clGainOpt.hpp |
Provides a class to manage closed loop gain optimization. | |
file | fourierCovariance.hpp |
Calculation of the modal covariance in the Fourier basis. | |
file | jincFuncs.hpp |
The +/- Jinc functions for analyzing contrast. | |
file | speckleAmpPSD.hpp |
Calculates the PSD of speckle intensity given a modified Fourier mode amplitude PSD. | |
file | varmapToImage.hpp |
A utility to convert a wavefront variance map to an intensity image. | |
file | wfsNoisePSD.hpp |
Declares and defines a function to calculate the measurement noise PSD. | |
file | ccdDetector.hpp |
Provides a class to simulate a CCD. | |