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10 - H1 - Desy

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1<strong>10</strong> Cross section building<br />

contribution of higher Q 2 values was subtracted by correcting each bin i of data input<br />

vector:<br />

y ′ i<br />

obs = yi obs × yi obs,MC,Q2<br />

y i obs,MC<br />

(8.22)<br />

The correction affects mainly cross section in the backward region with its maximum value<br />

of 5%. The ratio y obs,MC,Q2 /y obs,MC is presented in figure 8.8 as a function of pseudorapidity<br />

of the photon candidate.The final results are correctly quoted in the photoproduction<br />

range of Q 2 < 1 GeV 2 .<br />

)<br />

γ<br />

(η<br />

obs,MC,Q2<br />

y<br />

)<br />

γ<br />

(η<br />

obs,MC<br />

y<br />

1<br />

0.98<br />

0.96<br />

0.94<br />

-1 0 1 2<br />

γ<br />

η<br />

Figure 8.8: The Q 2 selection correction factor as a function of pseudorapidity of the<br />

photon candidate.<br />

8.3 Error matrix evaluation<br />

The final error matrix E x consists of three components and is built in the following way:<br />

E x = E u + E mc + ∑ i<br />

E i sys (8.23)<br />

where E u is the covariance matrix of the unfolding output bins calculated with the equation<br />

8.12, E mc is the error originating from the limited statistics of MC used to determine<br />

the migration matrix and E i sys is the error due to particular systematic effects i. Both<br />

E mc and E sys are calculated using error propagation rules [99] shortly explained in this<br />

section.<br />

Considering n η functions η i , building vector ⃗η and depending on n θ variables θ: η i (θ 1 , · · ·θ nθ )<br />

the covariance matrix U ij = cov|η i , η j | can be approximated by the first order in the Taylor

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