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Table 5.3 gives a summary of the various selection
steps required to select the final charged current event sample.
It is interesting to note that for the Monte Carlo events the
by far largest individual reason for loss of acceptance stems
from the FLT. This is not a surprise, however, considering that
the Monte Carlo events have been generated starting at a very low
of
. The
cut at the FLT
corresponds to a cut at about
to
.
Table 5.3:
Acceptance of the different trigger and selection steps.
Shown are only numbers for runs for which the
detector was in a good state (see section 5.5.2).
| Trigger Level |
MC |
Data |
Data |
Data |
| |
% accepted |
% accepted |
% accepted |
# remaining |
| |
of total |
in this step |
of total |
|
| Level-1 |
69.8 |
100.0 |
100.0 |
107560345 |
| Level-2 |
63.2 |
2.1 |
2.1 |
2283932 |
| Level-3 |
63.2 |
3.5 |
|
81540 |
| Vertex Req. |
62.4 |
6.4 |
|
5288 |
| Spark |
62.4 |
33.5 |
|
1770 |
| Beam-Wall |
58.0 |
39.2 |
|
693 |
| Cosmic & Halo |
58.0 |
29.4 |
|
204 |
| Vertex Cut |
50.3 |
87.7 |
|
179 |
| Neutral Current |
45.8 |
51.4 |
|
92 |
| Photoproduction |
44.7 |
53.3 |
|
49 |
|
|
|
|
|
|
Next: Muon Finder
Up: Charged Current Event Selection
Previous: Background from Photoproduction Events
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Els de Wolf
1999-12-20