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\@writefile{lof}{\contentsline {figure}{\numberline {9}{\ignorespaces Spectrum of detected quasi-elastic electron neutrino charged current events in a 0.5 MT detector at 2540 km from BNL. We have assumed 0.5 MW of beam power and 5 years of running. This plot is for $\Delta m^2_{32}= 0.0026 e\unhbox \voidb@x \hbox {V}^2$. We have assumed $\mathop {\mathgroup \symoperators sin}\nolimits ^2 2 \theta _{13} = 0.04$ and $\Delta m^2_{21}= 5\times 10^{-5} e\unhbox \voidb@x \hbox {V}^2$. The error bars correspond to the statistical error expected in the bin. A 10 \% energy resolution is assumed; this corresponds to the expected resolution due to both nuclear effects and the electron momentum reconstruction in the detector.}}{16}}
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\@writefile{lof}{\contentsline {figure}{\numberline {12}{\ignorespaces Schematic of the WIPP underground site and a location for the LANNDD detector. A water Cerenkov detector array could also be accommodated at the WIPP site. }}{20}}
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\@writefile{lof}{\contentsline {figure}{\numberline {22}{\ignorespaces Elevation view of the neutrino beam line to Homestake, South Dakota. For a nearer location a much smaller hill can be constructed. In this beam we assume a decay tunnel length of 200 m. For a shorter tunnel the cost of the hill will reduce as shown in table 4\hbox {}. }}{35}}
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\bibcite{rsvp}{31}