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Description

  AOT SWS06 allows the user to observe up to 64 wavelength ranges, with SWS in the grating mode. The wavelength range(s) may be chosen anywhere in the SWS grating range, i.e., between 2.38 and 45.2 tex2html_wrap_inline2404 m, under the restriction  that each range falls within one of the AOT bands  (Tab. 2.1, p. gif). The sum of the ranges chosen can cover the entire SWS wavelength range. The spectrum is sampled in a flexible and fastest possible way. Wavelength ranges are specified by giving the vacuum wavelengths of beginning and end of each range, and the source's heliocentric radial velocity . A specific wavelength within the desired wavelength range is being referred to as the reference wavelength    of that range. It is important that while selecting this wavelength one should avoid lines and make sure that it is representative for the average continuum flux density, rather than that it is close to the centre of the wavelength range. In SWS06, reference scans are made only when the grating scan takes longer than the nominal interval between reference scans.

AOT SWS06 is executed the following way: The telescope is pointed to the target position. Then for each wavelength range (or pair of merged ranges) the following sequence of steps is taken:

AOT SWS06 is used for a single observation of one target.


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Next: AOT SWS06 sample time-line Up: AOT SWS06: Grating Scan Previous: AOT SWS06: Grating Scan

SWS Consortium
Wed Aug 7 17:20:29 MET DST 1996