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                           Cha p te r
                                    T e n

                                        ξ = instrument efficiency (no units)
                                     R(σ) = responsivity of the system (A/W)
                                                                  2
                                        Θ = instrument throughput (cm  sr)
                                        F =  noise reduction apodization factor (no units);
                                            equal to 1 if no apodization is used
                             Being incoherent, the various sources of noise are added in an
                          RSS manner in Eq. (10.11).
                          10.7.15 Signal-to-Noise Ratio
                          Finally, the signal-to-noise ratio SNR is given by:
                                                        P()σ
                                               SNR()σ =                       (10.31)
                                                       NESR


                     10.8  Instrument Line Shape and Spectral Resolution
                          The ILS (instrument line shape) is the response of the spectrometer to
                          a monochromatic spectral stimulus. This is illustrated schematically
                          in Fig. 10.10. A distinct ILS spanning from σ = –∞ to +∞ exists for each
                          wave-number σ′, although it changes from one σ′ to the next in a slow
                          and progressive manner. The ILS at a given wave number σ′ repre-
                          sents the noiseless spectrum that would be obtained if the spectrom-
                          eter were submitted to monochromatic radiation—for example, that
                          of a laser at λ′ = 1/σ′. The ILS function ILS (σ) is thus characterized
                                                              σ′
                          by two indices, σ and σ′, as illustrated in Fig. 10.10.
                             An observed spectrum  S observed (σ) is the convolution of the ILS
                          functions with the spectral distribution of photon incidence B(σ).
                                                 ∞
                                             σ
                                                      −
                                      S observed () = ∫  B(σ σ′ ) ILS σσ′ (σ′  d ) σ′  (10.32)
                                                             −
                                                 −∞
                             If the spectral features or variations of B(σ) are much wider than
                          the width of the ILS peak, then S observed (σ) will be very similar to B(σ).

                                   IR Stimulus



                                                                      ILS σ′  (σ)
                                                 Spectrometer


                                      σ′   σ                                  σ
                                                                         0
                          FIGURE 10.10  Monochromatic IR stimulus and instrumental response
                          function (ILS).
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