A quick test was made to assess the consistency of the combined
counting experiment and mass measurement with the top production
cross section of [17]. Many simulated experiments
were generated by varying the measured and theoretical parameters
within errors and then picking a number of observed signal
and background events from appropriate Poisson distributions.
The fraction of such experiments which yielded
observed
events is then a measure of the consistency of the measured results
with the standard model cross section.
For this calculation, the standard cuts were used, and all seven
channels were combined together. The luminosities from the channels
were averaged to yield
(with the standard
12% luminosity error). The backgrounds were summed over
all channels; this was then divided by the
luminosity
to define an effective background cross section of 0.080
0.012 pb.
The values of efficiency times branching ratio for the signal
were summed
across all channels for each top mass. The results are tabulated
below.

The relative errors for these four points were averaged to obtain a mean relative error of 8.7%.
The detailed procedure used is a follows. For each simulated event:
from the gaussian distribution
.
0.012 pb. Multiply this with the luminosity
to obtain the expected number of background events
.
from an asymmetric gaussian distribution
with mean 199 GeV/
. For the 50% of trials which are below
the mean, take the width to be 30 GeV/
; for the upper half, take
the width to be 24 GeV/
.
to a cross section by interpolating
between the values from [17].
Smear the resulting value with a gaussian error
of 30%.
> 200 GeV/
use the 200 GeV/
point, and similarly
for
< 140 GeV/
.
Smear this with a gaussian error of 8.7%. Multiply together
the top cross section, top efficiency, and luminosity
to
obtain the expected number of signal events
.
or
is nonpositive, reject this experiment
and go on to the next (less than 0.1% of experiments were thus
rejected).
. Do the same for the number of signal events
(using
).
To obtain the final result, sum the contents of the histogram
bins for
and divide by the total number of accepted
experiments. Out of a total of 10000 experiments which were generated,
9992 were accepted, and 891 had
.
Thus, assuming the standard model cross section and the measured
mass, the probability of seeing at least 17 events is 8.9%.
A similar calculation was made in [147], except that all the channels were kept separate and allowed to vary independently. The result from that calculation for the probability of seeing at least 17 events was 6.6%.