List of Tables

• Definition of the wavelength ranges of the SWS AOT bands
• Summary of SWS-FM detector properties for a reset time sec
• Grating noise parameters
• Fabry-Pérot noise parameters
• Merging of observations in AOT SWS06. The integration time in the last column shows which observation (SW or LW) determines the charged integration time
• Merging of observations in AOT SWS07. The integration time in the last column shows which observation determines the charged integration time
• Possible combinations of reset time , step size in scanner steps, and number of scans for each of the SWS AOT's
• Continuation of possible combinations of reset time , step size in scanner steps, and number of scans for each of the SWS AOT's
• AOT SWS02 observing times for sources of 0.1, 0.3, 1, 3, 10, 30, and 100 Jy. Wavelength intervals correspond to 10 resolution elements. In all cases SNR = 20 was requested, but may be exceeded.
• Continuation of AOT SWS02 observing times table.
• AOT SWS06 grating scan observing times for wavelength intervals corresponding to 80 resolution elements of sources of 0.3, 1, 3, 10, 30, and 100 Jy. In all cases a SNR = 20 per resolution element was requested, but may be exceeded.

• Continuation of AOT SWS06 grating scan observing times