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λ a [m]<br />

105<br />

100<br />

95<br />

90<br />

85<br />

80<br />

75<br />

OMs 11,12,27,33,71<br />

90% C.L.<br />

λ e = (23.9±0.6) m<br />

λ a = (88.8±3.2) m<br />

ρ = 0.79<br />

99.99% C.L.<br />

χ 2<br />

min /NDF = 268/228<br />

70<br />

20 21 22 23 24 25 26 27 28<br />

λe [m]<br />

Figure 29: Con<strong>to</strong>ur plot of the value yielded by comparing data time distributions with their simulated counterparts<br />

varying the parameters ¡£¢ and ¡¥¤§¦¨¦ .<br />

The dependence of ¢ on wavelength can be useful for other purposes though (simulation, computation<br />

of energy loss by Cherenkov emission) and is shown in the curve in Fig. 32, taken from<br />

[65].<br />

Distance(m)*count rate(/256Hz)<br />

10 5<br />

10 4<br />

1000<br />

100<br />

350nm-1950mA<br />

350nm-1480mA<br />

350nm-1200mA<br />

1σ<br />

0 50 100 150 200 250<br />

Distance (m)<br />

Figure 30: Distance © counting rate versus distance for DC lamp source emitting 350 nm pho<strong>to</strong>ns. The datapoints<br />

are well fitted by an exponential, as expected from Eq. 53<br />

42

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