Definition at line 9 of file SpectralFitter.h.
 
◆ SpectralFitter()
      
        
          | SpectralFitter::SpectralFitter  | 
          ( | 
          std::vector< double > &  | 
          spectrum,  | 
        
        
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          std::vector< std::vector< double > > &  | 
          pool  | 
        
        
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          ) | 
           |  | 
        
      
 
 
◆ fitSpectrum()
      
        
          | void SpectralFitter::fitSpectrum  | 
          ( | 
           | ) | 
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◆ getNonZeroIndices()
      
        
          | const std::vector< unsigned int > & SpectralFitter::getNonZeroIndices  | 
          ( | 
           | ) | 
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◆ getNorm()
  
  
      
        
          | const double & SpectralFitter::getNorm  | 
          ( | 
           | ) | 
           const | 
         
       
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inline   | 
  
 
 
◆ getWeights()
  
  
      
        
          | const std::vector< double > & SpectralFitter::getWeights  | 
          ( | 
           | ) | 
           const | 
         
       
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inline   | 
  
 
 
◆ setPool()
  
  
      
        
          | void SpectralFitter::setPool  | 
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          std::vector< std::vector< double > > &  | 
          pool | ) | 
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inline   | 
  
 
 
◆ setSpectrum()
  
  
      
        
          | void SpectralFitter::setSpectrum  | 
          ( | 
          std::vector< double > &  | 
          spectrum | ) | 
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inline   | 
  
 
 
◆ setUncertainties()
  
  
      
        
          | void SpectralFitter::setUncertainties  | 
          ( | 
          std::vector< double > &  | 
          uncertainties | ) | 
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inline   | 
  
 
 
The documentation for this class was generated from the following files:
 
  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".