mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
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A spectrum from the astroFilt filter library.
Definition at line 68 of file astroSpectra.hpp.
#include <astro/astroSpectra.hpp>
Public Types | |
typedef std::string | paramsT |
The astroFilters are parameterized by name. More... | |
Static Public Member Functions | |
static int | readSpectrum (std::vector< realT > &rawLambda, std::vector< realT > &rawSpectrum, const std::string &path, const paramsT ¶ms) |
Static Public Attributes | |
static constexpr realT | wavelengthUnits = static_cast<realT>(1e6) |
Convert from um to SI m. More... | |
static constexpr realT | fluxUnits = static_cast<realT>(1) |
No conversion is performed on filter transmission. More... | |
typedef std::string mx::astro::astroFilter< _units, _rsr >::paramsT |
The astroFilters are parameterized by name.
Definition at line 76 of file astroSpectra.hpp.
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inlinestatic |
[out] | rawLambda | the raw wavelength vector. This should be an empty vector on input. |
[out] | rawSpectrum | the raw spectrum. This should be an empty vector on input. |
[in] | path | the full path to the file. |
[in] | params | the parameters are passed in case needed to construct the spectrum |
Definition at line 91 of file astroSpectra.hpp.
References mx::ioutils::readColumns().
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staticconstexpr |
No conversion is performed on filter transmission.
Definition at line 82 of file astroSpectra.hpp.
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staticconstexpr |
Convert from um to SI m.
Definition at line 79 of file astroSpectra.hpp.