A preliminary examination of the Ultraviolet Spectrometer (UVS) data          
revealed no obvious detections of anything which might correspond with the    
impact phenomena. In order to investigate the possibility that more subtle    
impact-related events were present in the data and to establish a formal      
statistical upper limit for the non-detection of the impacts, we performed a  
statistical analysis as described in the DPS poster paper "Voyager 2          
UVS Observations of Jupiter During the Comet Shoemaker-Levy 9 Impact Events", 
by R. J. Vervack et al.                                                       
                                                                              
Our final conclusion in that paper was that no statistically significant      
detections were made for any of the impacts. The largest single candidate     
event observed corresponded to impact A, but the probability of observing     
random noise with the same spectral signature was determined to be            
approximately 8 per cent.                                                     
                                                                              
Jim Collins                                                                   
Lunar & Planetary Laboratory                                                  
901 Gould Simpson Building                                                    
University of Arizona                                                         
Tucson, Arizona 85721                                                         
(601) 621-8607                                                                
(601) 621-4493                                                                
collins@argus.lpl.arizona.edu                                                 
                                                                              
Latex and Postscript versions of this paper are available in the DOCUMENT     
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