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New analysis techniques to reduce systematics due ... - CNGS - CERN

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Standard approach with near detec<strong>to</strong>r III<br />

Low energy beam<br />

Medium energy beam<br />

ν µ<br />

CC<br />

5000<br />

4000<br />

x 10 4 0 2 4 6 8 10 12 14<br />

GFLUKA<br />

MARS<br />

ν µ<br />

CC<br />

7000<br />

6000<br />

5000<br />

x 10 4 0 2 4 6 8 10 12 14<br />

GFLUKA<br />

BMPT<br />

MARS<br />

Malensek<br />

3000<br />

BMPT<br />

Malensek<br />

4000<br />

2000<br />

3000<br />

1000<br />

2000<br />

1000<br />

0<br />

0<br />

Near<br />

E ν<br />

GeV<br />

Near<br />

E ν<br />

GeV<br />

ν µ<br />

CC<br />

1.25<br />

1.2<br />

1.15<br />

1.1<br />

1.05<br />

1<br />

0.95<br />

0.9<br />

0.85<br />

0.8<br />

0.75<br />

0 2 4 6 8 10 12 14<br />

(F/N) / (F/N) nominal<br />

E ν<br />

GeV<br />

ν µ<br />

CC<br />

1.25<br />

1.2<br />

1.15<br />

1.1<br />

1.05<br />

1<br />

0.95<br />

0.9<br />

0.85<br />

0.8<br />

0.75<br />

0 2 4 6 8 10 12 14<br />

(F/N) / (F/N) nominal<br />

E ν<br />

GeV<br />

NNN Micha̷l SZLEPER Analysis <strong>techniques</strong> <strong>to</strong> <strong>reduce</strong> <strong>systematics</strong>... 4

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