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   PR # 22095
    We propose observations of a group of Vela-like ($\tau = {P\over     
    2\dot{P}} \sim$ 20,000 years) pulsars: PSR 1706-44, PSR 1823-13, PSR 
    1046-58, and PSR 1727-33. The goals of the observation will be to    
    detect pulsations at the radio period and determine the character-   
    istics of the high energy component of the spectrum. We will be      
    sensitive to pulsed fractions between $\geq$ 5\% (PSR 1706-44) and   
    $\geq$ 10\% (PSR 1727-33). The counts acquired will be sufficient to 
    place reasonable constraints on the spectrum. By exploiting the large
    FOV of the GIS a secondary goal will be to search for extended       
    emission from an associated supernova remnant. The study proposed    
    here will help fill in the gap in the X-ray database between the     
   young and intermediate aged   
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