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QCD radiative corrections have not been taken into account in these studies. They are likely to increase the Drell-Yan signal rates. Since all the physics backgrounds are very small after event selections are made, higher-order corrections to them are not expected to change our conclusions. The EHLQ-1 distribution functions were used for all simulations in this section
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The discrepancy between the theoretical widths determined from Eq. (5.20) and those from fitting the PYTHIA distributions corresponds to about a 0.5% Gaussian noise term that we have not yet understood. Since PYTHIA and gemfast widths agree within the expected detector resolution, this is not a matter of immediate concern
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