Eric Limburg

Boswil, Schwitzerland

After a first demonstration of the new functionality of the Lunar Occultation Workbench (LOW), version 4.0 at ESOP XXI in Naples, a second one will be given at ESOP XXII in Trebur. The new highlights to be demonstrated this time will be:

* improved functionality for setting up graze expeditions, e.g. showing graze site events,
* greater flexibility and versatility for calculating predictions of occultations, e.g. Messier, NGC/IC objects, multiple sites, double/variable stars, and ‘CCD’ magnitudes,
* new functionality for reducing total and grazing occultations.

LOW 4.0 is likely to become avialable before the end of 2003.
 
 
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