Question of the Referees:
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If there is a K partner to the 
(1.8) (fig. 4.6) at a mass of
about 1.9 to 2 GeV, decaying into 
, 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 (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 (1.8) or from a different state with
0 
quantum
numbers)?
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