1) General description of the beam Monte Carlo. (draft) This mini-document is not really a figure to present. It is a short description of the contents of the beam MC. The first page is about proton-aluminnum interactions, and the second is about other aspects of the code. A third page is added for some references on pion production. 2) General figure of the beamline geometry. 3) Expected spectrum on and off axis. This has two versions available. It is meant to address the question "What if your whole front site is mis-aimed compared to the far site?" Note that this is very different from the information on aiming from neutrino detectors or beam monitors. This is .NOT. an explicit error term in any calculation and the levels of mis-aiming on the plots are .NOT. given as representing 'reasonable cases.' In particular, the extra parts of the second version are huge compared to any reasonable estimate of possible mistakes. 4) Distribution of production points of parents of neutrinos. This is meant to address the question "What if the beamline components downstream of the target are not modeled properly?" Again, it is .NOT. put into any explicit error term. The point is that so much of the production is in the target that getting anything else wrong makes very little difference to the end result. The neutrinos here are those nu_mu with >0.5GeV which pass within 400m of SK. 5) Distribution of production points of neutrinos. The neutrinos here are those nu_mu with >0.5GeV which pass within 400m of SK. The point at which the plot starts to rise again is where the decay tunnel widens. The dotted line is for the subset of these neutrinos that are produced within 1m of the beam axis. This has the expected nearly exponential shape after the horns. 6) Systematic error as a function of neutrino momentum for (purely) Monte Carlo based extrapolation. This is the combination of several studies of beam MC with varied inputs. The errors are slightly larger than those for analysis using monitor data directly. For analysis with FD data below the pion monitor threshold, the low energy bins of this are necessary to supplement the monitor data. Sources of error considered are: - Nuclear model dependence of pi+ production. This uses the 64 nuclear model study and the fitted pion monitor data. - Nuclear extrapolation from Be to Al. This (a much smaller effect than the previous) is a study changing the nuclear corrrection factor in the MC. - Normalization of Kaon production. This uses the difference between pion cross section measurements from the Derrick experiment (our main source for pion production) and the Yamamoto paper (from which we get kaon production). This term is still being checked, but it is only large in the highest energy bin. - Magnetic field perturbations in the horn. - Proton profile and centering. - Mechanical sagging of the target. (This is probably over-estimated.)