CollabMay03

SciFi Official Plots for 2003 May Collab. Meeting

1.Basic distribution in 2003 SciFi(DATA.vs.MC)
2.Q-square distributions
3.Comparison plots K2K-I.vs.2003
4.LG study (K2K-I)
5.Nsk estimation
6.Detector performance

1.Basic distribution in 2003 SciFi(DATA.vs.MC)

The dots and histogram correspond DATA and MC, respectively.
The hatched region of the histogram show quasi-elastic interaction in MC (Neut4.3 reweighted).

MRD3D

All track

1-track

2-trackQE

2-tracknonQE

MRD1L

2.Q-square distributions

MA(qe)=1.14, MA(1pi)=1.01, Q2min cut=0.2

3.Comparison plots K2K-I.vs.2003

New Geometry

The side view of FGD event display in 2003. The white rectangle is SciBar detector.

MRD3D

The hatched histogram and dots correspond 03a and K2K-I, respectively.
Both of the years are normalized by CT.

MRDALL

Q-square distributions (MRD3D)

Neut4.3 weighted, after Fit

4.LG study (K2K-I)

Basic distributions using LG-stopping events. The Dots are DATA, the histograms are MC, the hatched histogram shows QE events in MC.

6.Nsk estimation

Center value

------------------------------------------------------ SciFi ------------------------------------------------------ MRD events 4507 Efficiency of MRD events 0.265 CT 1.4952e19 p.o.t. ------------------------------------------------------ ------------------------------------------------------ SK ------------------------------------------------------ SK efficiency 0.785 CT 1.5221e19 p.o.t. ------------------------------------------------------ Flux ratio 1.9339e-3 ------------------------------------------------------ Nsk = 4507 * 0.785/0.265 * 1.5221e19/1.4952e19 * 1.9339e-3 = 26.31 +-0.4(stat.) +2.7 -3.0

Nsk error

------------------------------------------------------ Track selection +- 4% Al interaction +- 3% Spectrum shape +- 4% InEl/El +- 1.5% CC/NC +- 2% ------------------------------------------------------ Far/Near ratio +5.6% -7.1% SK eff +- 5.1% CT +- 1% ------------------------------------------------------ Total +10.3% -11.2% ------------------------------------------------------

Note:

WE USED InEl/El=30% AND FLUX ERROR FROM PIMON.
IF WE USE THE FLUX ERROR FROM SPECTRUM ANALYSIS AND InEl/El=20%, WE OBTAIN
Nsk = 26.31 +-0.4(stat.) +2.5 -2.7

5.Detector performance

Efficiency plot(cosmic ray)

Typical npix

The dots are DATA, the histogram is MC.

Npix distribution for muon and proton enriched samples

The dots are DATA, the histogram is MC.