How to compute the <em>approximate SNR</em> of an AOT SWS01 observation



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How to compute the approximate SNR of an AOT SWS01 observation

 

The following algorithm may be used to compute the SNR to be expected for a source with a given flux density:

Determine the detector reset time required to achieve the desired SNR:
a) Convert the expected flux density at the desired wavelength to a detector signal (V/s), using the spectral response curves shown in Fig. gif (p. gif) to Fig. gif (p. gif).
b) Compute the expected SNR per resolution element, starting with the minimum detector reset time of sec, using the formula

where stands for the number of integrations per resolution element as given in Tab. gif, and taking the noise parameters from Tab. gif (p. gif).

If the expected SNR is less than requested, repeat the computation of the expected with the maximum detector reset time of sec, as indicated in Tab. gif.



SWS Consortium
Tue Jul 30 15:56:20 MET DST 1996