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Beam Telescope Amplitude Cut
The multi-
stop events were distinguished
from single
stop events by applying a cut based on
the beam telescope amplitude
described in Section 5.3.2.
The light output
from the eight photo-multiplier tubes viewing
the four individual beam scintillators were normalized and summed.
The cut was imposed on this normalized sum.
The final pulse height spectra shown in Figure 5.7 is
obtained as follows. The ADC pulse heights from the four beam telescopes are
read out by a pair of top and bottom mounted photo-multiplier tubes. The eight ADC spectra thus obtained were normalized to 100. The normalization factors were 0.79, 1.12, 0.83, 0.81, 0.88, 0.86, 0.67 and 0.92 respectively. The final spectra was obtained by adding the individual ADC readouts multiplied by their respective normalization factors. Based on this final spectra a beam telescope cut was applied at 1069 to reject the multi-
peak.
The multi-pion background was about
our
signal and corresponds to the smaller second
peak in Figure 5.7.
The efficiency of passing the signal by
the beam telescope amplitude cut was determined from
analyzing the periodically recorded dedicated
runs. In such
runs, the random
coincident two-photon events are insignificant compared to the
two-photon events due to
decay by several orders of magnitude.
The
two-photon events are ideally expected to be unaffected by
the beam telescope amplitude cut. Following this procedure,
an individual beam telescope efficiency of selecting single pion events was
found to be
95%. An efficiency of
99% was obtained
for all four beam telescopes combined.
The beam telescope amplitude cut removed about
accidental
-
coincidences
arising from the multi-
stops.
As described in Section 5.3.2, from the 100 events attributed the random multi-
coincidences,
the remaining inefficiency in rejecting
the accidental coincidences was 100/
=
.
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Sugata Tripathi
2004-03-27