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Question of the Referees:


If there is a K partner to the tex2html_wrap_inline2264 (1.8) (fig. 4.6) at a mass of about 1.9 to 2 GeV, decaying into tex2html_wrap_inline2754 , will you have sensitivity to this?

Up to what mass will you be able to separate Primakoff excitations from diffractive production? In particular, is it possible to extract an electromagnetic excitation strength for the tex2html_wrap_inline2264 (1.8)? What essential improvements are anticipated by Compass relative to the current Protvino set up for this particular state (i.e., will you improve the information on the question of whether there is a rho omega decay, and if so whether this is from the same tex2html_wrap_inline2264 (1.8) or from a different state with 0 tex2html_wrap_inline2272 quantum numbers)?


Lars Schmitt
Wed May 22 16:44:09 METDST 1996