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%an overview of our observing strategy including a discussion of:
%capabilities of the instrument
%selection of bands and fields
%allocation of time in each
%calibration observations
The MWA has observed 350 hours during the Fall 2013 EoR season. The two main observing variables are choice of 30MHz band and pointing. Total time is limited. Observations are thermal noise limited. After about 1000 hours on a particular sky location and tuning they become cosmic variance limited. Because 1000 hours per pointing is thought to be an achievable goal,