| Rev | Line |  | 
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| [400] | 1 | \relax | 
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|  | 2 | \citation{JECACLAL} | 
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|  | 3 | \citation{SPL} | 
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|  | 4 | \citation{HARP,MINERVA} | 
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|  | 5 | \citation{SIMONE1,DONEGA} | 
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|  | 6 | \citation{MEZZETTONF02,DONINI04} | 
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|  | 7 | \citation{LIPARIxsec} | 
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|  | 8 | \citation{GLOBES} | 
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|  | 9 | \citation{MEZZETTONF02} | 
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|  | 10 | \citation{T2K} | 
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|  | 11 | \@writefile{toc}{\contentsline {section}{\numberline {1}Introduction}{1}} | 
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|  | 12 | \@writefile{toc}{\contentsline {section}{\numberline {2}Fluxes}{1}} | 
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|  | 13 | \@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces The $\nu _\mu $ and the $\mathaccentV {bar}016{\nu }_\mu $ fluxes obtained by optimizing the SPL for a Super Beam case ("SB Opt.") are compared to those obtained with a focusing system designed for a Neutrino Factory ("NF Opt.").}}{1}} | 
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|  | 14 | \newlabel{fig:fluxComparison}{{1}{1}} | 
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|  | 15 | \@writefile{toc}{\contentsline {section}{\numberline {3}Physics potential}{1}} | 
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|  | 16 | \citation{T2K} | 
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|  | 17 | \citation{T2K} | 
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|  | 18 | \citation{VILLARS} | 
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|  | 19 | \bibcite{JECACLAL}{1} | 
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|  | 20 | \bibcite{SPL}{2} | 
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|  | 21 | \bibcite{HARP}{3} | 
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|  | 22 | \bibcite{MINERVA}{4} | 
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|  | 23 | \bibcite{SIMONE1}{5} | 
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|  | 24 | \bibcite{DONEGA}{6} | 
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|  | 25 | \bibcite{MEZZETTONF02}{7} | 
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|  | 26 | \bibcite{DONINI04}{8} | 
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|  | 27 | \bibcite{LIPARIxsec}{9} | 
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|  | 28 | \bibcite{GLOBES}{10} | 
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|  | 29 | \bibcite{T2K}{11} | 
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|  | 30 | \bibcite{VILLARS}{12} | 
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|  | 31 | \@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces Comparison of the sensitivity contours with the new optimized setup and the original SPL design after 5 years of running with positive focusing.}}{2}} | 
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|  | 32 | \newlabel{fig:SPLDmTheta13Comparison}{{2}{2}} | 
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|  | 33 | \@writefile{lof}{\contentsline {figure}{\numberline {3}{\ignorespaces Comparison of the sensitivity on combined $\theta _{13}$ and $\delta _{CP}$ after 5 years of positive focusing. The T2K sensitivity contour has been derived from reference \cite  {T2K}. No mass hierarchy nor octant hierarchy ambiguity has been considered.}}{2}} | 
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|  | 34 | \newlabel{fig:SPLCPSensi}{{3}{2}} | 
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