10 - H1 - Desy
10 - H1 - Desy
10 - H1 - Desy
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86 Calibration and tuning<br />
• Background BG.<br />
The third sample used to study the quality of MC simulation of the background<br />
clusters is selected by using photon candidates with low isolation z < 0.9 and no<br />
cut on the cluster radius of the photon candidate. In this phasespace, selected events<br />
are purely neutral hadron background.<br />
a. b. c.<br />
e<br />
p<br />
γ<br />
γ<br />
e e<br />
e<br />
p p<br />
p<br />
e<br />
p<br />
e<br />
p<br />
γ<br />
Figure 7.1: Feynman diagrams illustrating the Bethe-Heitler events (a and b) and deeply<br />
virtual Compton scattering (c).<br />
All the samples are statistically independent of the selection used for final results determination<br />
and provide a clean selection of electromagnetic clusters. The evaluation of<br />
the systematic uncertainty follows the method developed in [66]. MC cluster shape v is<br />
distorted by a stretching factor k:<br />
v ′ (k) = v · (1 + k ), (7.1)<br />
<strong>10</strong>0<br />
and its distribution is compared to the distribution measured in the data. An example<br />
of the comparison is presented in figure 7.2, where the FLF MC distribution in wheel<br />
CB1 is stretched against the data distribution measured in the BG sample. One may see<br />
that for negative k the MC distribution is shifted towards too low FLF values, while for<br />
positive k in the opposite direction. For k close to zero, both distributions are comparable,<br />
being at it best for k ≈ 2.<br />
For each factor k the χ 2 can be calculated between the data histogram and the stretched<br />
MC distribution:<br />
χ 2 = ∑ (b D i − b MC<br />
i ) 2 /(σD,i 2 + σ2 MC,i ), (7.2)<br />
i<br />
where b D i and b MC<br />
i denote the data and MC histogram content for bin i, σ its error and the<br />
sum runs over all non-empty histogram bins. The number of non-empty bins correspond<br />
to the number of degrees of freedom (NDF).<br />
Figure 7.2 shows the χ 2 (k)/NDF dependence for all six shower shape variables in CB1<br />
wheel as studied with the BG sample. A clear minima close to k = 0 can be observed<br />
in each case. The min(χ 2 ) is used for the correction applied to the MC simulation of the<br />
cluster shapes, while min(χ 2 )±NDF for the evaluation of its uncertainty. In case of DVCS<br />
and BH samples, error deduced by the χ 2 method is dominated by statistical error of both<br />
samples, which leads to an overestimated uncertainty of the cluster shapes description.