mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
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The square wave is parameterized by the central wavelength, width, and sampling (all in microns).
Definition at line 148 of file astroSpectra.hpp.
#include <astro/astroSpectra.hpp>
Public Attributes | |
realT | lam0 |
The central Wavelength in microns. More... | |
realT | fw |
The full width of the filter in microns. More... | |
realT | dlam |
The wavelength sampling to use in microns. More... | |
realT mx::astro::sqWaveFilter< _units, _rsr >::paramsT::dlam |
The wavelength sampling to use in microns.
Definition at line 152 of file astroSpectra.hpp.
Referenced by mx::astro::sqWaveFilter< _units, _rsr >::readSpectrum().
realT mx::astro::sqWaveFilter< _units, _rsr >::paramsT::fw |
The full width of the filter in microns.
Definition at line 151 of file astroSpectra.hpp.
Referenced by mx::astro::sqWaveFilter< _units, _rsr >::readSpectrum().
realT mx::astro::sqWaveFilter< _units, _rsr >::paramsT::lam0 |
The central Wavelength in microns.
Definition at line 150 of file astroSpectra.hpp.
Referenced by mx::astro::sqWaveFilter< _units, _rsr >::readSpectrum().