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PAHdb website C++ backend
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PAHEmissionModel Member List

This is the complete list of members for PAHEmissionModel, including all inherited members.

_approximate (defined in PAHEmissionModel)PAHEmissionModelstatic
_energy (defined in PAHEmissionModel)PAHEmissionModelstatic
_frequency (defined in PAHEmissionModel)PAHEmissionModelstatic
_nc (defined in PAHEmissionModel)PAHEmissionModelstatic
applyBlackbodyWithTemperature(double temperature) (defined in PAHEmissionModel)PAHEmissionModel
applyBlackbodyWithTemperatureForEach(const std::vector< double > &temperatures) (defined in PAHEmissionModel)PAHEmissionModel
applyCascadeWithEnergy(double energy, std::vector< double > &temperatures) (defined in PAHEmissionModel)PAHEmissionModel
applyTemperatureWithEnergy(double energy, std::vector< double > &temperatures) (defined in PAHEmissionModel)PAHEmissionModel
approximateFeatureStrength(double temperature, void *charge) (defined in PAHEmissionModel)PAHEmissionModelstatic
convertFromFrequencyToWavelength(std::vector< double > &grid) (defined in PAHEmissionModel)PAHEmissionModelstatic
convertFromFrequencyToWavelength(std::array< double, 2 > &grid) (defined in PAHEmissionModel)PAHEmissionModelstatic
convertFromFrequencyToWavelength(std::vector< std::vector< std::pair< double, double > > > &transitions) (defined in PAHEmissionModel)PAHEmissionModelstatic
convertFromWavelengthToFrequency(std::vector< double > &grid) (defined in PAHEmissionModel)PAHEmissionModelinlinestatic
convertFromWavelengthToFrequency(std::vector< std::vector< std::pair< double, double > > > &transitions) (defined in PAHEmissionModel)PAHEmissionModelinlinestatic
featureStrength(double temperature, void *transitions) (defined in PAHEmissionModel)PAHEmissionModelstatic
getGrid() const (defined in PAHEmissionModel)PAHEmissionModelinline
getSpectraAndConvolveWithDrudeOfFHWM(std::vector< std::vector< double > > &vector, double fwhm=15) (defined in PAHEmissionModel)PAHEmissionModel
getSpectraAndConvolveWithGaussianOfFHWM(std::vector< std::vector< double > > &vector, double fwhm=15) (defined in PAHEmissionModel)PAHEmissionModel
getSpectraAndConvolveWithLorentianOfFHWM(std::vector< std::vector< double > > &vector, double fwhm=15) (defined in PAHEmissionModel)PAHEmissionModel
getTransitions(std::vector< std::vector< std::pair< double, double > > > &transitions) (defined in PAHEmissionModel)PAHEmissionModel
heatCapacity(double temperature, void *transitions) (defined in PAHEmissionModel)PAHEmissionModelstatic
integralOverHeatCapacity(double temperature, void *transitions) (defined in PAHEmissionModel)PAHEmissionModelstatic
makeGrid(const std::vector< double > &frange, double step) (defined in PAHEmissionModel)PAHEmissionModelinline
makeGrid(double fmin, double fmax, double step) (defined in PAHEmissionModel)PAHEmissionModel
PAHEmissionModel() (defined in PAHEmissionModel)PAHEmissionModel
PAHEmissionModel(const std::vector< std::vector< std::pair< double, double > > > &transitions) (defined in PAHEmissionModel)PAHEmissionModel
printTransitions() (defined in PAHEmissionModel)PAHEmissionModel
setGrid(const std::vector< double > &grid) (defined in PAHEmissionModel)PAHEmissionModel
setTransitions(const std::vector< std::vector< std::pair< double, double > > > &transitions) (defined in PAHEmissionModel)PAHEmissionModel
shiftTransitions(double shift) (defined in PAHEmissionModel)PAHEmissionModel
solveApproximateInitialTemperatureFunc(double temperature, void *nc) (defined in PAHEmissionModel)PAHEmissionModelinlinestatic
solveInitialTemperatureFunc(double temperature, void *transitions) (defined in PAHEmissionModel)PAHEmissionModelinlinestatic
useApproximate(std::vector< int > &charges, std::vector< int > &carbons) (defined in PAHEmissionModel)PAHEmissionModelinline
From FY2025 onward the NASA Ames PAH IR Spectroscopic Database is being supported through the Laboratory Astrophysics Round 3 directed Work Package at NASA Ames.
From FY2023-2025 the NASA Ames PAH IR Spectroscopic Database was supported through the Laboratory Astrophysics Round 2 directed Work Package at NASA Ames.
From FY2019-2022 the NASA Ames PAH IR Spectroscopic Database was supported through a directed Work Package at NASA Ames titled: "Laboratory Astrophysics – The NASA Ames PAH IR Spectroscopic Database".
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