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Simplified description of the correlations

Nel documento s = 7 TeV with the ATLAS detector (pagine 50-53)

preferable to have the JES uncertainties and correlations de-scribed by a reduced set of uncertainty components. This can the in situ methods, as they are convoluted with the corresponding weights.

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Fig. 40: Systematic (effective) relative uncertainties displayed as a function of jet pTfor anti-ktjets with R = 0.4 calibrated with the(a)EM+JES and the(b)LCW+JES calibration schemes for the reduced scheme with six nuisance parameters. Each curve can be interpreted as a 1σ JES systematic nuisance parameter, symmetric around zero. They represent eigenvectors of the covariance matrix (continuous lines) and the residual component (dashed line).

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Anti-(b) Difference between weaker and stronger correlation Fig. 41: In(a), the nominal JES correlation matrix is shown. The difference between the correlation matrices of the interpretations resulting in stronger and weaker correlations for anti-ktjets with R = 0.4 calibrated using the EM+JES calibration scheme in the central calorimeter region (η = 0.5) is depicted in(b).

be achieved by combining the least significant (weakest) nui-sance parameters into one component while maintaining a suf-ficient accuracy for the JES uncertainty correlations.

The total covariance matrix Ctotof the JES correction fac-tors can be derived from the individual components of the sta-tistical and systematic uncertainties:

Ctot=

Nsources

k=1

Ck, (14)

where the sum goes over the covariance matrices of the individ-ual uncertainty components Ck. Each uncertainty component sk is treated as fully correlated in pTand the covariance of the pT

bins i and j is given by Ci jk = skiskj. All the uncertainty compo-nents are treated as independent of one another, except for the photon and electron energy scales which are treated as corre-lated.16

A reduction of the number of nuisance parameters while re-taining the information on the correlations can be achieved by deriving the total covariance matrix in Eq. (14) and

diagonalis-16 A single systematic uncertainty source is assigned to account for both the photon and electron energy scales by first adding the pho-ton and electron scales linearly, deriving the full covariance matrix, and add it linearly to the covariance matrix of the other uncertainty components.

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Effective nuisance parameters for the statistical category

(a) Statistical and method components

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Effective nuisance parameters for the detector category

(b) Detector components

Effective nuisance parameters for the modelling category

(c) Modelling components

Effective nuisance parameters for the mixed category

(d) Mixed detector and modelling components

Fig. 42: Relative uncertainties for reduced (effective) components within a single category displayed as a fraction of jet pTfor anti-ktjets with R = 0.4, calibrated with the EM+JES scheme. The convention from Fig.40is followed here. The 54 nuisance pa-rameters that are input to the reduction for each of the categories are listed in Table10. The reduction is performed for all nuisance parameters belonging to any given category, which are statistical and method components (a), detector components (b), model-ling components (c), and mixed detector and modelmodel-ling components (d). Each of the curves can be interpreted as an effective 1σ JES systematic nuisance parameter, symmetric around zero. They represent eigenvectors of the covariance matrix (continuous lines) and the residual component (dashed line), for the specified category.

ing it:

Ctot= STD S.

Here D is a (positive definite) diagonal matrix, containing the eigenvalues σk2of the total covariance matrix, while the S ma-trix contains on its columns the corresponding (orthogonal) unitary eigenvectors Vk. A new set of independent uncertainty sources can then be obtained by multiplying each eigenvector by the corresponding eigenvalue. The covariance matrix can be re-derived from these uncertainty sources using:

Ci jtot=

Nbins

k=1

σk2VikVjk,

where Nbinsis the number of bins used in the combination.

A good approximation of the covariance matrix can be ob-tained by separating out only a small subset of Neff

eigenvec-tors that have the largest corresponding eigenvalues. From the remaining Nbins− Neffcomponents, a residual, left-over uncer-tainty source is determined, with an associated covariance ma-trix C0. The initial covariance matrix can now be approximated as:

Ctoti j

Neff k=1

σk2VikVjk+C0.

This approximation conserves the total uncertainty, while the precision on the description of the correlations can be directly determined by comparing the original full correlation matrix and the approximate one. The last residual uncertainty could in principle be treated either as correlated or as uncorrelated be-tween the pTbins. It is observed that treating this uncertainty source as uncorrelated in pT provides a better approximation of the correlation matrix. This is expected, as this residual

un-certainty source includes many orthogonal eigenvectors with small amplitudes and many oscillations, hence the small cor-relations. The original exact covariance matrix is thus decom-posed into a part with strong correlations and another one with much smaller correlations. It is this residual uncertainty source that incorporates the part with small correlations.

Figure40shows the obtained five eigenvectors σkVk and the residual sixth component, as a function of the jet pT. The pT-dependent sign of these eigenvectors allows to keep track of the (anti-)correlations of each component in different phase-space regions. This is necessary for a good description of the correlations of the total JES uncertainty. These six nuisance parameters are enough to describe the correlation matrix with sufficient precision at the level of percent. As explained above, the quadratic sum of these six components is identical to the quadratic sum of the original uncertainties shown in Fig. 37.

In the high-pTregion above 300 GeV, one eigenvector has a significantly larger amplitude than all the others, see the black curve in Fig.40, hence the strong correlations between the bins.

Approximately 60% to 80% of this component is due to the photon and electron energy scale uncertainties up to about 700 GeV (see Figs.37(c)and37(d)), while some other uncertainties contribute to it at higher pT.

Table 11: A summary of the various explored JES configura-tions. The precision of the reduction is defined by the largest deviation in correlations between the original full set of pa-rameters and the reduced version. The full pT phase space is considered in this determination. The values quoted are for jets in the region |η| < 1.2 for anti-kt with R = 0.4 calibrated with EM+JES scheme. The number of nuisance parameters quoted refers only to the parameters entering the reduction procedure, which are relevant to the in situ techniques.

Configuration Reduction Nparams Reduction

type precision (%)

All parameters none 54 100

global 6 97

category 11 95

Stronger correlations none 45 100

global 6 97

category 12 96

Weaker correlations none 56 100

global 6 97

category 12 95

Nel documento s = 7 TeV with the ATLAS detector (pagine 50-53)