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Negative log-likelihood difference in $\text{c}_{\varphi\text{Q}}^{3}$ where the other Wilson coefficients are fixed to 0.

Negative log-likelihood difference in $\text{c}_{\varphi\text{t}}$ where the other Wilson coefficients are fixed to 0.

Negative log-likelihood difference in $\text{c}_{\varphi\text{tb}}$ where the other Wilson coefficients are fixed to 0.

Negative log-likelihood difference in $\text{c}_{\text{tW}}$ where the other Wilson coefficients are fixed to 0.

Negative log-likelihood difference in $\text{c}_{\text{bW}}$ where the other Wilson coefficients are fixed to 0.

Negative log-likelihood difference in $\text{c}_{\text{tZ}}$ where the other Wilson coefficients are fixed to 0.

Negative log-likelihood difference in $\text{c}_{\text{t}\varphi}$ where the other Wilson coefficients are simultaneously fit.

Negative log-likelihood difference in $\text{c}_{\varphi\text{Q}}^{-}$ where the other Wilson coefficients are simultaneously fit.

Negative log-likelihood difference in $\text{c}_{\varphi\text{Q}}^{3}$ where the other Wilson coefficients are simultaneously fit.

Negative log-likelihood difference in $\text{c}_{\varphi\text{t}}$ where the other Wilson coefficients are simultaneously fit.

Negative log-likelihood difference in $\text{c}_{\varphi\text{tb}}$ where the other Wilson coefficients are simultaneously fit.

Negative log-likelihood difference in $\text{c}_{\text{tW}}$ where the other Wilson coefficients are simultaneously fit.

Negative log-likelihood difference in $\text{c}_{\text{bW}}$ where the other Wilson coefficients are simultaneously fit.

Negative log-likelihood difference in $\text{c}_{\text{tZ}}$ where the other Wilson coefficients are simultaneously fit.

Negative log-likelihood difference in $\text{c}_{\varphi\text{t}}, \text{c}_{\varphi\text{Q}}^{-}$ where the other Wilson coefficients are fixed to 0.

Negative log-likelihood difference in $\text{c}_{\varphi\text{Q}}^{3}, \text{c}_{\varphi\text{Q}}^{-}$ where the other Wilson coefficients are fixed to 0.

Negative log-likelihood difference in $\text{c}_{\text{tW}}, \text{c}_{\text{tZ}}$ where the other Wilson coefficients are fixed to 0.

$\Delta\phi$ projection of balance function in low $p_{T}$ in 0-10% centrality

$\Delta\phi$ projection of balance function in low $p_{T}$ in 30-40% centrality

1D $\Delta\eta$ projection of balance function in low $p_{T}$ in 70-80% centrality

$\Delta\eta$ projection of balance function in low $p_{T}$ in 0-40 $N_{trk}$

$\Delta\eta$ projection of balance function in low $p_{T}$ in 120-150 $N_{trk}$

$\Delta\eta$ projection of balance function in low $p_{T}$ in 270-300 $N_{trk}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 0-40 $N_{trk}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 120-150 $N_{trk}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 270-300 $N_{trk}$

The width of balance function in $<|\Delta\eta|>$ in low $p_{T}$ for PbPb collisions

Balance function width in low $p_{T}$ PbPb relative $<|\Delta\eta|>/<|\Delta\eta|>_{N_{ch}<65}$

The width of balance function in $<|\Delta\eta|>$ in low $p_{T}$ for pPb collisions

Balance function width in low $p_{T}$ in pPb relative $<|\Delta\eta|>/<|\Delta\eta|>_{N_{ch}<24}$

The width of the balance function in $<|\Delta\phi|>$ in low $p_{T}$ for PbPb collisions

Balance function width in low $p_{T}$ in PbPb for relative $<|\Delta\phi|>/<|\Delta\phi|>_{N_{ch}<65}$

The width of the balance function in $<|\Delta\phi|>$ in low $p_{T}$ for pPb collisions

Balance function width in low $p_{T}$ in pPb for relative $|\Delta\phi|/<|\Delta\phi|>_{N_{ch}<24}$

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in pPb for 0-40 $N_{trk}$

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in pPb for 120-150 $N_{trk}$

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in pPb for 270-300 $N_{trk}$

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in pPb for $N_{trk}$ 0-40

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in pPb for $N_{trk}$ 120-150

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in pPb for $N_{trk}$ 270-300

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in pPb for $N_{trk}$ 0-40

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in pPb for $N_{trk}$ 120-150

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in pPb for $N_{trk}$ 270-300

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for $N_{trk}$ 0-40

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for $N_{trk}$ 120-150

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for $N_{trk}$ 270-300

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for low $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for high $p_{T}$

Average width of the balance function in $\Delta \phi$ with $p_{T}$ for low $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for high $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for low $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for high $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for low $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for high $p_{T}$

The JEC, JER, and total systematic uncertainties in unfolded cross sections as functions of transverse momentum, for 1.5<|y|<2. The total systematic uncertainty includes also the luminosity, jet identification and trigger efficiency uncertainties.

The unfolded measured particle-level inclusive jet cross section as functions of jet pT (markers), for |y|<0.5, compared to the NLO perturbative QCD prediction (histogram), using the CT14NLO PDF set, with muR = muF = HT, and corrected for the NP effects. The experimental and theoretical systematic uncertainties are shown.

The unfolded measured particle-level inclusive jet cross section as functions of jet pT (markers), for 0.5<|y|<1, compared to the NLO perturbative QCD prediction (histogram), using the CT14NLO PDF set, with muR = muF = HT, and corrected for the NP effects. The experimental and theoretical systematic uncertainties are shown.

The unfolded measured particle-level inclusive jet cross section as functions of jet pT (markers), for 1<|y|<1.5, compared to the NLO perturbative QCD prediction (histogram), using the CT14NLO PDF set, with muR = muF = HT, and corrected for the NP effects. The experimental and theoretical systematic uncertainties are shown.

The unfolded measured particle-level inclusive jet cross section as functions of jet pT (markers), for 1.5<|y|<2, compared to the NLO perturbative QCD prediction (histogram), using the CT14NLO PDF set, with muR = muF = HT, and corrected for the NP effects. The experimental and theoretical systematic uncertainties are shown.

Ratios (points) of the unfolded measured cross sections to the NLO theoretical predictions, using the CT14NLO PDF set, with mu = pT, for |y|<0.5. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NLO theoretical predictions, using the CT14NLO PDF set, with mu = pT, for 0.5<|y|<1. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NLO theoretical predictions, using the CT14NLO PDF set, with mu = pT, for 1<|y|<1.5. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NLO theoretical predictions, using the CT14NLO PDF set, with mu = pT, for 1.5<|y|<2. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NLO theoretical predictions, using the CT14NLO PDF set, with mu = HT, for |y|<0.5. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NLO theoretical predictions, using the CT14NLO PDF set, with mu = HT, for 0.5<|y|<1. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NLO theoretical predictions, using the CT14NLO PDF set, with mu = HT, for 1<|y|<1.5. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NLO theoretical predictions, using the CT14NLO PDF set, with mu = HT, for 1.5<|y|<2. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NNLO theoretical predictions, using the CT14NNLO PDF set, with mu = HT, for |y|<0.5. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NNLO theoretical predictions, using the CT14NNLO PDF set, with mu = HT, for 0.5<|y|<1. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NNLO theoretical predictions, using the CT14NNLO PDF set, with mu = HT, for 1<|y|<1.5. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NNLO theoretical predictions, using the CT14NNLO PDF set, with mu = HT, for 1.5<|y|<2. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NNLO theoretical predictions, using the NNPDF31NNLO PDF set, with mu = HT, for |y|<0.5. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NNLO theoretical predictions, using the NNPDF31NNLO PDF set, with mu = HT, for 0.5<|y|<1. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NNLO theoretical predictions, using the NNPDF31NNLO PDF set, with mu = HT, for 1<|y|<1.5. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

Ratios (points) of the unfolded measured cross sections to the NNLO theoretical predictions, using the NNPDF31NNLO PDF set, with mu = HT, for 1.5<|y|<2. The vertical error bars show the statistical experimental uncertainty. The systematic experimental uncertainty, the total theoretical uncertainty, and the individual sources of theoretical uncertainty are shown.

The effect of aS(MZ) variation, for |y|<0.5. The NNLO theoretical cross section predictions using the NNPDF31NNLO PDF with m = HT, calculated for different choices of aS (0.108, 0.110, 0.112, 0.114, 0.116, 0.117, 0.118, 0.119, 0.120, 0.122, and 0.124), are divided by the benchmark NNLO prediction for aS = 0.118 and the same choice of PDF set, muR, and muF. Also shown is the experimental unfolded measurement divided by the same benchmark prediction. The width of the unity line corresponds to the statistical uncertainty from the MC integration for the determination of the NNLO prediction. The error bars on the unfolded data correspond to the total experimental statistical and systematic uncertainty added in quadrature.

The effect of aS(MZ) variation, for 0.5<|y|<1. The NNLO theoretical cross section predictions using the NNPDF31NNLO PDF with m = HT, calculated for different choices of aS (0.108, 0.110, 0.112, 0.114, 0.116, 0.117, 0.118, 0.119, 0.120, 0.122, and 0.124), are divided by the benchmark NNLO prediction for aS = 0.118 and the same choice of PDF set, muR, and muF. Also shown is the experimental unfolded measurement divided by the same benchmark prediction. The width of the unity line corresponds to the statistical uncertainty from the MC integration for the determination of the NNLO prediction. The error bars on the unfolded data correspond to the total experimental statistical and systematic uncertainty added in quadrature.

The effect of aS(MZ) variation, for 1<|y|<1.5. The NNLO theoretical cross section predictions using the NNPDF31NNLO PDF with m = HT, calculated for different choices of aS (0.108, 0.110, 0.112, 0.114, 0.116, 0.117, 0.118, 0.119, 0.120, 0.122, and 0.124), are divided by the benchmark NNLO prediction for aS = 0.118 and the same choice of PDF set, muR, and muF. Also shown is the experimental unfolded measurement divided by the same benchmark prediction. The width of the unity line corresponds to the statistical uncertainty from the MC integration for the determination of the NNLO prediction. The error bars on the unfolded data correspond to the total experimental statistical and systematic uncertainty added in quadrature.

The effect of aS(MZ) variation, for 1.5<|y|<2. The NNLO theoretical cross section predictions using the NNPDF31NNLO PDF with m = HT, calculated for different choices of aS (0.108, 0.110, 0.112, 0.114, 0.116, 0.117, 0.118, 0.119, 0.120, 0.122, and 0.124), are divided by the benchmark NNLO prediction for aS = 0.118 and the same choice of PDF set, muR, and muF. Also shown is the experimental unfolded measurement divided by the same benchmark prediction. The width of the unity line corresponds to the statistical uncertainty from the MC integration for the determination of the NNLO prediction. The error bars on the unfolded data correspond to the total experimental statistical and systematic uncertainty added in quadrature.

Unfolded correlation matrix for |y|<0.5.

Unfolded correlation matrix for 0.5<|y|<1.

Unfolded correlation matrix for 1<|y|<1.5.

Unfolded correlation matrix for 1.5<|y|<2.

Normalised inclusive single-particle distributions of charged hadrons in different intervals of W and Q**2 with corresponding values of X(Bjorken). Additional systematic error of 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons in different intervals of W and Q**2 with corresponding values of X(Bjorken). Additional systematic error of 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons in different intervals of W and Q**2 with corresponding values of X(Bjorken). Additional systematic error of 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons in different intervals of W and Q**2 with corresponding values of X(Bjorken). Additional systematic error of 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons in different intervals of W and Q**2 with corresponding values of X(Bjorken). Additional systematic error of 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons in different intervals of W and Q**2 with corresponding values of X(Bjorken). Additional systematic error of 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons in different intervals of W and Q**2 with corresponding values of X(Bjorken). Additional systematic error of 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons in different intervals of W and Q**2 with corresponding values of X(Bjorken). Additional systematic error of 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons in different intervals of W and Q**2 with corresponding values of X(Bjorken). Additional systematic error of 4 PCT.

Additional inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of W. Additional systematic error 4 PCT.

Additional inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of W. Additional systematic error 4 PCT.

Additional inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of W. Additional systematic error 4 PCT.

Additional inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of W. Additional systematic error 4 PCT.

Additional inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of W. Additional systematic error 4 PCT.

Additional inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of W. Additional systematic error 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of Q**2. Additional systematic error 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of Q**2. Additional systematic error 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of Q**2. Additional systematic error 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of Q**2. Additional systematic error 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of Q**2. Additional systematic error 4 PCT.

Normalised inclusive single-particle distributions of charged hadrons as a function of XL and PT**2 in different intervals of Q**2. Additional systematic error 4 PCT.

Mean values of PT**2 in different XL intervals in different regions of W**2. Additional systematic error 2 PCT.

Mean values of PT**2 in different XL intervals in different Q**2 regions. Additional systematic error 2 PCT.

Mean value of PT**2 in different XL intervals in different intervals of W**2 and Q**2. Corresponding values of X(Bjorken) as shown. Additional systematic error 2 PCT.

Mean value of PT**2 in different XL intervals in different intervals of W**2 and Q**2. Corresponding values of X(Bjorken) as shown. Additional systematic error 2 PCT.

Mean value of PT**2 in different XL intervals in different intervals of W**2 and Q**2. Corresponding values of X(Bjorken) as shown. Additional systematic error 2 PCT.

Mean value of PT**2 in different XL intervals in different intervals of W**2 and Q**2. Corresponding values of X(Bjorken) as shown. Additional systematic error 2 PCT.

Mean value of PT**2 in different XL intervals in different intervals of W**2 and Q**2. Corresponding values of X(Bjorken) as shown. Additional systematic error 2 PCT.

Mean value of PT**2 in different XL intervals in different intervals of W**2 and Q**2. Corresponding values of X(Bjorken) as shown. Additional systematic error 2 PCT.

Average forward multipicities for positive, negative and all charged hadrons. Additional systematic error 1 PCT.

Average forward multipicities for positive, negative and all charged hadrons. Additional systematic error 1 PCT.

Average forward multipicities for positive, negative and all charged hadrons. Additional systematic error 1 PCT.

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Mean values of Q**2 and y.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $\phi^*$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $\phi^*$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Integrated fiducial cross section for the DY process measured in the muon channel. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of dimuon invariant mass. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of rapidity in the centre-of-mass frame for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of rapidity in the centre-of-mass frame for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $\phi^*$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $\phi^*$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Integrated cross section for the DY process measured in the muon channel. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Forward-backward ratios for $15<m_{\mu\mu}<60$ GeV. Quoted uncertainties are the quadratic sum of the statistical and systematic uncertainties.

Forward-backward ratios for $60<m_{\mu\mu}<120$ GeV. Quoted uncertainties are the quadratic sum of the statistical and systematic uncertainties.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of dimuon invariant mass.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of rapidity in the centre-of-mass frame for $15<m_{\mu\mu}<60$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of rapidity in the centre-of-mass frame for $60<m_{\mu\mu}<120$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $p_{\textrm{T}}$ for $15<m_{\mu\mu}<60$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $p_{\textrm{T}}$ for $60<m_{\mu\mu}<120$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $\phi^*$ for $15<m_{\mu\mu}<60$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $\phi^*$ for $60<m_{\mu\mu}<120$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of rapidity in the centre-of-mass frame, putting together low and high masses. Each bin is labeled lm_i or hm_i, where lm stands for $15<m_{\mu\mu}<60$ GeV, hm stands for $60<m_{\mu\mu}<120$ GeV, and i is the corresponding bin number in rapidity in the centre-of-mass frame. The global normalisation uncertainty of 3.5% is not included. Data from Figure [3, 4, 4].

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $p_{\textrm{T}}$, putting together low and high masses. Each bin is labeled lm_i or hm_i, where lm stands for $15<m_{\mu\mu}<60$ GeV, hm stands for $60<m_{\mu\mu}<120$ GeV, and i is the corresponding bin number in $p_{\textrm{T}}$. The global normalisation uncertainty of 3.5% is not included. Data from Figure [3, 4, 4].

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $\phi^*$, putting together low and high masses. Each bin is labeled lm_i or hm_i, where lm stands for $15<m_{\mu\mu}<60$ GeV, hm stands for $60<m_{\mu\mu}<120$ GeV, and i is the corresponding bin number in $\phi^*$. The global normalisation uncertainty of 3.5% is not included. Data from Figure [3, 4, 4].

The asymmetry $A_{\mu}$ extracted from the differential cross sections.

Unfolded measurements of AFB in each M-|y| bin (e+e-).

Covariance matrix of Drell-Yan AFB in muon channel for |y|<1 for cos(theta)<0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for |y|<1 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for |y|<1 for cos(theta)>0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for |y|<1 for cos(theta)>0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1<|y|<1.25 for cos(theta)<0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1<|y|<1.25 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1<|y|<1.25 for cos(theta)>0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1<|y|<1.25 for cos(theta)>0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1.25<|y|<1.5 for cos(theta)<0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1.25<|y|<1.5 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1.25<|y|<1.5 for cos(theta)>0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1.25<|y|<1.5 for cos(theta)>0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1.5<|y|<2.4 for cos(theta)<0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1.5<|y|<2.4 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1.5<|y|<2.4 for cos(theta)>0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in muon channel for 1.5<|y|<2.4 for cos(theta)>0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for |y|<1 for cos(theta)<0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for |y|<1 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for |y|<1 for cos(theta)>0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for |y|<1 for cos(theta)>0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1<|y|<1.25 for cos(theta)<0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1<|y|<1.25 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1<|y|<1.25 for cos(theta)>0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1<|y|<1.25 for cos(theta)>0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1.25|y|<1.5 for cos(theta)<0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1.25|y|<1.5 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1.25|y|<1.5 for cos(theta)>0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1.25|y|<1.5 for cos(theta)>0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1.5<|y|<2.4 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1.5<|y|<2.4 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1.5<|y|<2.4 for cos(theta)>0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 1.5<|y|<2.4 for cos(theta)>0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 2.4<|y|<5 for cos(theta)<0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 2.4<|y|<5 for cos(theta)<0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 2.4<|y|<5 for cos(theta)>0 and cos(theta)<0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Covariance matrix of Drell-Yan AFB in electron channel for 2.4<|y|<5 for cos(theta)>0 and cos(theta)>0. The covariance matrix is built in 2 dimensions, 14x14(mass) for cos(theta), --, -+, +-, ++ combination where + means positive cos(theta) and - implies the negative cos(theta).

Fig. 7. The 95% CL exclusion limit on $\sigma (pp \to H)\mathcal{B}(H \to \mu\mu\gamma)$, with $m_{\mu\mu}$ < 20 GeV, for a Higgs-like particle, as a function of the mass hypothesis, $m_{H}$.

The (Z to l+l-l'+l'-) branching ratio. The first systematic uncertainty is detector systematics, the second is theoretical uncertainty, and the third is luminosity uncertainty. The theoretical prediction is from MadGraph5_aMC@NLO.

The total (P P to Z Z) cross section. The first systematic uncertainty is detector systematics, the second is theoretical uncertainty, and the third is luminosity uncertainty. The theoretical predictions are MATRIX generated at NNLO and POWHEG generated at NLO plus the gluon-gluon initial state contribution from MCFM. Both use NNPDF3.0 PDFs and fixed scales mu_F = mu_R = 0.5m[l+l-l'+l'-].

The $\gamma$ differential transverse momentum cross-section in an inclusive $\gamma+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ selection for central rapidities $\vert y_{\gamma} \vert > 1.4$.

The Z boson differential transverse momentum cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ over $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq1$ selection.

The $\gamma$ boson differential transverse momentum cross-section in an inclusive $\gamma+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ over $Z+\mathrm{jets}$, $N_{\mathrm{jets}} \geq1$ selection for central rapidities $\vert y_{\gamma} \vert < 1.4$.

The Z boson differential transverse momentum over $H_{\mathrm{T}}$ cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ selection.

The Z boson differential transverse momentum over $H_{\mathrm{T}}$ cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq3$ selection.

The log (base 10) of the Z boson differential transverse momentum over the leading jet transverse momentum cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ selection.

The log (base 10) of the Z boson differential transverse momentum over the leading jet transverse momentum cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq3$ selection.

Differential cross-section ratio of Z over $\gamma$ as a function of the total transverse momentum cross-section and for central bosons ($\vert y_{\mathrm{V}}\vert < 1.4$) in an inclusive $ N_{\mathrm{jets}}\geq 1 $ selection.

Differential cross-section ratio of Z over $\gamma$ as a function of the total transverse momentum cross-section and for central bosons ($\vert y_{\mathrm{V}}\vert < 1.4$) in a $ H_{\mathrm{T}}$% > 300 GeV, N_{\mathrm{jets}}\geq 1 $ selection.

Differential cross-section ratio of Z over $\gamma$ as a function of the total transverse momentum cross-section and for central bosons ($\vert y_{\mathrm{V}}\vert < 1.4$) in an inclusive $ N_{\mathrm{jets}}\geq 2 $ selection.

Differential cross-section ratio of Z over $\gamma$ as a function of the total transverse momentum cross-section and for central bosons ($\vert y_{\mathrm{V}}\vert < 1.4$) in an inclusive $ N_{\mathrm{jets}}\geq 3 $ selection.

Observed and expected 95% CL upper limits on the product of cross section of a narrow resonance and the branching fraction $\sigma(gg \to X) B(X \to HH \to bbbb)$ for HPHP category. Theory curves corresponding to WED models with radion are superimposed.

Observed and expected 95% CL upper limits on the product of cross section of a narrow resonance and the branching fraction $\sigma(gg \to X) B(X \to HH \to bbbb)$ for HPLP category. Theory curves corresponding to WED models with radion are superimposed.

Observed and expected 95% CL upper limits on the product of cross section of a narrow resonance and the branching fraction $\sigma(gg \to X) B(X \to HH \to bbbb)$ for LPHP category. Theory curves corresponding to WED models with radion are superimposed.

Observed and expected 95% CL upper limits on the product of cross section and the branching fraction $\sigma(gg \to X) B(X \to HH \to bbbb)$ for HPHP, HPLP and LPHP categories combined. The one standard deviation on the 95% CL upper limit is also provided.

Differential cross section as a function of the transverse momentum PT of the leading other jet. The first uncertainty is the statistical one, the second uncertainty is the combined systematic uncertainty including luminosity, jet energy scale, sample purity, model dependence and jet energy resolution and trigger efficiency correction.

Differential cross section as a function of the transverse momentum PT of the subleading other jet. The first uncertainty is the statistical one, the second uncertainty is the combined systematic uncertainty including luminosity, jet energy scale, sample purity, model dependence and jet energy resolution and trigger efficiency correction.

Differential cross section as a function of the pseudorapidity ETA of the leading b-jet. The first uncertainty is the statistical one, the second uncertainty is the combined systematic uncertainty including luminosity, jet energy scale, sample purity, model dependence and jet energy resolution and trigger efficiency correction.

Differential cross section as a function of the pseudorapidity ETA of the subleading b-jet. The first uncertainty is the statistical one, the second uncertainty is the combined systematic uncertainty including luminosity, jet energy scale, sample purity, model dependence and jet energy resolution and trigger efficiency correction.

Differential cross section as a function of the pseudorapidity ETA of the leading other jet. The first uncertainty is the statistical one, the second uncertainty is the combined systematic uncertainty including luminosity, jet energy scale, sample purity, model dependence and jet energy resolution and trigger efficiency correction.

Differential cross section as a function of the pseudorapidity ETA of the subleading other jet. The first uncertainty is the statistical one, the second uncertainty is the combined systematic uncertainty including luminosity, jet energy scale, sample purity, model dependence and jet energy resolution and trigger efficiency correction.

Differential cross section as a function of the azimuthal angle DeltaPhi between the two other jets, normalized to the total number of selected events. The first uncertainty is the statistical one, the second uncertainty is the combined systematic uncertainty including luminosity, jet energy scale, sample purity, model dependence and jet energy resolution and trigger efficiency correction.

Differential cross section as a function of the normalized PT balance DELTARELPT between the third and the fourth jet, normalized to the total number of selected events. The first uncertainty is the statistical one, the second uncertainty is the combined systematic uncertainty including luminosity, jet energy scale, sample purity, model dependence and jet energy resolution and trigger efficiency correction.

Differential cross section as a function of the azimuthal angle between the two dijet planes (leading-subleading b- and leading-subleading other jets), normalized to the total number of selected events. The first uncertainty is the statistical one, the second uncertainty is the combined systematic uncertainty including luminosity, jet energy scale, sample purity, model dependence and jet energy resolution and trigger efficiency correction.

Inclusive Jet Cross Section for |rapidity| 1.5 TO 2.0 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.7). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| 2.0 TO 2.5 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.7). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| 2.5 TO 3.0 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.7). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| 3.2 TO 4.7 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.7). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| < 0.5 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.4). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| 0.5 TO 1.0 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.4). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| 1.0 TO 1.5 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.4). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| 1.5 TO 2.0 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.4). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| 2.0 TO 2.5 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.4). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| 2.5 TO 3.0 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.4). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Inclusive Jet Cross Section for |rapidity| 3.2 TO 4.7 as a function of the jet transverse momentum. Jets are clustered with the anti-kt algorithm ( R = 0.4). The (sys) error is the total systematic error, including the luminosity uncertainty of 2.7%.

Correlation matrix of systematic uncertainties for $\sigma^{\pm}$. The statistical and integrated luminosity uncertainties are not included. The first and the last eleven indices correspond to the systematic uncertainites of $W^+$ ($\sigma^+_{1-11}$) and $W^-$ ($\sigma^-_{1-11}$) cross sections, respectively, in 11 muon pseudorapidity bins. The values are expressed as percentages.

Correlation matrix of statistical uncertainties for $\sigma^{\pm}$. The first and the last eleven indices correspond to the statistical uncertainites of $W^+$ ($\sigma^+_{1-11}$) and $W^-$ ($\sigma^-_{1-11}$) cross sections, respectively, in 11 muon pseudorapidity bins. The values are expressed as percentages.

Correlation matrix of systematic uncertainties for $\mathcal{A}$. The values are expressed as percentages.

Normalized dijet cross section differential in DeltPhi_{dijet} for 500<p_{T}^{max}<700 GeV region. The error bars on the data points include statistical and systematic uncertainties. The (sys) error is the total systematic error.

Normalized dijet cross section differential in DeltPhi_{dijet} for 700<p_{T}^{max}<900 GeV region. The error bars on the data points include statistical and systematic uncertainties. The (sys) error is the total systematic error.

Normalized dijet cross section differential in DeltPhi_{dijet} for 900<p_{T}^{max}<1100 GeV region. The error bars on the data points include statistical and systematic uncertainties. The (sys) error is the total systematic error.

Normalized dijet cross section differential in DeltPhi_{dijet} for p_{T}^{max}>1100 GeV region. The error bars on the data points include statistical and systematic uncertainties. The (sys) error is the total systematic error.

Normalized $t\bar{t}$ differential cross section measurements with respect to the $p^{W}_{T}$ variable at a center-of-mass energy of 7 TeV (combination of electron and muon channels).

Normalized $t\bar{t}$ differential cross section measurements with respect to the $E^{miss}_{T}$ variable at a center-of-mass energy of 8 TeV (combination of electron and muon channels).

Normalized $t\bar{t}$ differential cross section measurements with respect to the HT variable at a center-of-mass energy of 8 TeV (combination of electron and muon channels).

Normalized $t\bar{t}$ differential cross section measurements with respect to the $S_T$ variable at a center-of-mass energy of 8 TeV (combination of electron and muon channels).

Normalized $t\bar{t}$ differential cross section measurements with respect to the $p^{W}_{T}$ variable at a center-of-mass energy of 8 TeV (combination of electron and muon channels).

Covariance matrix for the normalized $t\bar{t}$ differential cross section measurements with respect to the $E_{T}^{miss}$ variable at a center-of-mass energy of 7 TeV. Both statistical and systematic effects are considered.

Covariance matrix for the normalized $t\bar{t}$ differential cross section measurements with respect to the $H_{T}$ variable at a center-of-mass energy of 7 TeV. Both statistical and systematic effects are considered.

Covariance matrix for the normalized $t\bar{t}$ differential cross section measurements with respect to the $S_{T}$ variable at a center-of-mass energy of 7 TeV. Both statistical and systematic effects are considered.

Covariance matrix for the normalized $t\bar{t}$ differential cross section measurements with respect to the $p^{W}_{T}$ variable at a center-of-mass energy of 7 TeV. Both statistical and systematic effects are considered.

Covariance matrix for the normalized $t\bar{t}$ differential cross section measurements with respect to the $E_{T}^{miss}$ variable at a center-of-mass energy of 8 TeV. Both statistical and systematic effects are considered.

Covariance matrix for the normalized $t\bar{t}$ differential cross section measurements with respect to the $H_{T}$ variable at a center-of-mass energy of 8 TeV. Both statistical and systematic effects are considered.

Covariance matrix for the normalized $t\bar{t}$ differential cross section measurements with respect to the $S_{T}$ variable at a center-of-mass energy of 8 TeV. Both statistical and systematic effects are considered.

Covariance matrix for the normalized $t\bar{t}$ differential cross section measurements with respect to the $p^{W}_{T}$ variable at a center-of-mass energy of 8 TeV. Both statistical and systematic effects are considered.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of $\Delta \phi^{\gamma\gamma}$ as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of ||$y^{\gamma\gamma}$|| as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of $N_\rm{jets}$ as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of $p_\rm{T}^\rm{j1}$ as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of |$y^{\gamma\gamma}-y^{\rm{j1}}$| as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of $m_\rm{jj}$ as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of $\Delta \eta^{\rm{jj}}$ as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of $\Delta \phi^{\gamma\gamma,\rm{jj}}$ as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of $\Delta \phi^{\rm{jj}}$ as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Values of the pp $\to$ H $\to \gamma\gamma$ differential cross sections as a function of |$\eta^{\gamma\gamma}-(\eta^{\rm{j1}}+\eta^{\rm{j2}})/2$| as measured in data. For each observable the fit to $m_{\gamma\gamma}$ is performed simultaneously in all the bins. Since the signal mass is profiled for each observable, the best fit $\hat{m}_{\rm{H}}$ varies from observable to observable.

Covariance matrix of total experimental uncertainties (statistical and systematic uncertainties added in quadrature) of absolute double differential fiducial cross section. The bin index is PT_i + 10*y_j.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

Factorization ratio, $r_{2}$, as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

Factorization ratio, $r_{3}$, as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

Factorization ratio, $r_{2}$, as a function of event multiplicity in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

Factorization ratio, $r_{3}$, as a function of event multiplicity in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 50-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 50-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 50-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 50-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 3.0<$\eta_b$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 3.0<$\eta_b$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 3.0<$\eta_b$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 4.4<$\eta_b$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 4.4<$\eta_b$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 4.4<$\eta_b$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^{a}, \eta^{b}){\cdot(-\eta^{a}, -\eta^{b})}}$ a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for multiplicity bin $120<=N_{trk}^{offline}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^{a}, \eta^{b}){\cdot(-\eta^{a}, -\eta^{b})}}$ a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for multiplicity bin $150<=N_{trk}^{offline}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^{a}, \eta^{b}){\cdot(-\eta^{a}, -\eta^{b})}}$ a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for multiplicity bin $185<=N_{trk}^{offline}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^{a}, \eta^{b}){\cdot(-\eta^{a}, -\eta^{b})}}$ a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for multiplicity bin $220<=N_{trk}^{offline}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^a, \eta^b)\cdot{r_2(-\eta^{a}, -\eta^{b})}}$ as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for a given multiplicity class in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^a, \eta^b)\cdot{r_2(-\eta^{a}, -\eta^{b})}}$ as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for a given multiplicity class in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^a, \eta^b)\cdot{r_2(-\eta^{a}, -\eta^{b})}}$ as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for a given multiplicity class in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^a, \eta^b)\cdot{r_2(-\eta^{a}, -\eta^{b})}}$ as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for a given multiplicity class in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

$F^{\eta}_2$ as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

$F^{\eta}_3$ as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

$F^{\eta}_4$ as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

$F^{\eta}_2$ as a function of event multiplicity in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

Correlation matrix for the asymmetries as a function of $p_\text{T}^\mathrm{t\bar{t}}$ in the fiducial phase space. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $m_\mathrm{t\bar{t}}$ in the fiducial phase space, using three bins in $m_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $m_\mathrm{t\bar{t}}$ in the fiducial phase space, using three bins in $m_\mathrm{t\bar{t}}$. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $m_\mathrm{t\bar{t}}$ in the fiducial phase space, using six bins in $m_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $m_\mathrm{t\bar{t}}$ in the fiducial phase space, using six bins in $m_\mathrm{t\bar{t}}$. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $|y_\mathrm{t\bar{t}}|$ in the full phase space. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $|y_\mathrm{t\bar{t}}|$ in the full phase space. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $p_\text{T}^\mathrm{t\bar{t}}$ in the full phase space. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $p_\text{T}^\mathrm{t\bar{t}}$ in the full phase space. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $m_\mathrm{t\bar{t}}$ in the full phase space, using three bins in $m_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $m_\mathrm{t\bar{t}}$ in the full phase space, using three bins in $m_\mathrm{t\bar{t}}$. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $m_\mathrm{t\bar{t}}$ in the full phase space, using six bins in $m_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $m_\mathrm{t\bar{t}}$ in the full phase space, using six bins in $m_\mathrm{t\bar{t}}$. Both statistical and systematic effects are considered.

Systematic covariance matrix for the 12 bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$.

Values of the 6 bins of the normalized differential cross section as a function of $\cos\varphi$.

Statistical covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\varphi$.

Systematic covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\varphi$.

Values of the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$.

Statistical covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$.

Systematic covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$.

Values of the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$.

Statistical covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$.

Systematic covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$.

Values of the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$.

Statistical covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$.

Systematic covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$.

Values of $A_{\Delta\phi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{\cos\varphi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{c1c2}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{c1c2}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{c1c2}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{P}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{P}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{P}^{\rm{CPV}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{\Delta\phi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{\cos\varphi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{c1c2}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{c1c2}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{c1c2}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{P}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{P}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{P}^{\rm{CPV}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{\Delta\phi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $|y_\mathrm{t\bar{t}}|$.

Values of $A_{\cos\varphi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $|y_\mathrm{t\bar{t}}|$.

Values of $A_{c1c2}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{c1c2}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{c1c2}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $|y_\mathrm{t\bar{t}}|$.

Values of $A_{P}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{P}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $|y_\mathrm{t\bar{t}}|$.

Values of $A_{P}^{\rm{CPV}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $|y_\mathrm{t\bar{t}}|$.

Upper limits at 95% CL on the gluon-gluon fusion cross section for a heavy Higgs boson as a function of its mass and its width relative to a SM-like Higgs boson.

Upper limits at 95% CL on the VBF cross section for a heavy Higgs boson as a function of its mass and its width relative to a SM-like Higgs boson.

Fully corrected average charged particle scalar Sum(pT) per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransMAX region.

Fully corrected average charged particle multiplicity per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransMIN region.

Fully corrected average charged particle scalar Sum(pT) per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransMIN region.

Fully corrected average charged particle multiplicity per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransDIF region.

Fully corrected average charged particle scalar Sum(pT) per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransDIF region.

Measurement of $m_{t}$ as a function of the number of jets with pT>30 GeV.

Measurement of $m_{t}$ as a function of the pT of the b jet assigned to the hadronic decay branch.

Measurement of $m_{t}$ as a function of the pseudorapidity of the b jet assigned to the hadronic decay branch.

Measurement of $m_{t}$ as a function of the $\Delta R$ between the b jets.

Measurement of $m_{t}$ as a function of the $\Delta R$ between the light-quark jets.

The combined $\sqrt{s}$ = 7 and 8 TeV measurements of $m_{t}$ for each of the top-antitop decay channels and the combined result.

For the tu$\gamma$ signal channel, the total number of observed selected events in the data (N$_{obs}$), the SM expectations (N$_{SM}$), the efficiencies ($\epsilon$), and the upper limits on the cross sections $\sigma_{fid}$ at the 95% CL in the fiducial region, without and with a requirement on the presence of a single accompanying b jet.

For the tc$\gamma$ signal channel, the total number of observed selected events in the data (N$_{obs}$), the SM expectations (N$_{SM}$), the efficiencies ($\epsilon$), and the upper limits on the cross sections $\sigma_{fid}$ at the 95% CL in the fiducial region, without and with a requirement on the presence of a single accompanying b jet.

Systematic covariance matrix for the 6 bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$.

Values of the 12 bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$.

Statistical covariance matrix for the 12 bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$.

Systematic covariance matrix for the 12 bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$.

Values of $A_{\mathrm{C}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\mathrm{C}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\mathrm{C}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$ and $M_\mathrm{t\bar{t}}$.

Values of $A^{\mathrm{lep}}_{\mathrm{C}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A^{\mathrm{lep}}_{\mathrm{C}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A^{\mathrm{lep}}_{\mathrm{C}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $12\times3$ bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{\mathrm{C}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\mathrm{C}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\mathrm{C}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A^{\mathrm{lep}}_{\mathrm{C}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A^{\mathrm{lep}}_{\mathrm{C}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A^{\mathrm{lep}}_{\mathrm{C}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $12\times3$ bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{\mathrm{C}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\mathrm{C}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{\mathrm{C}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\Delta|y_\mathrm{t}|$ and $|y_\mathrm{t\bar{t}}|$.

Values of $A^{\mathrm{lep}}_{\mathrm{C}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A^{\mathrm{lep}}_{\mathrm{C}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A^{\mathrm{lep}}_{\mathrm{C}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $12\times3$ bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\Delta|\eta_{\ell}|$ and $|y_\mathrm{t\bar{t}}|$.

Normalized differential ttbar cross sections as a function of the jet multiplicity for jets with pt > 60GeV, along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space of the ttbar decay products and the additional jets.

Absolute differential ttbar cross sections as a function of the jet multiplicity for jets with pt > 100GeV, along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space of the ttbar decay products and the additional jets.

Normalized differential ttbar cross sections as a function of the jet multiplicity for jets with pt > 100GeV, along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space of the ttbar decay products and the additional jets.

Absolute differential ttbar cross sections as a function of the pt of the leading additional jet in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the pt of the leading additional jet in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the eta of the leading additional jet in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the eta of the leading additional jet in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the pt of the subleading additional jet in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the pt of the subleading additional jet in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of |eta| of the subleading additional jet in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of |eta| of the subleading additional jet in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the invariant mass of the two leading additional jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the invariant mass of the two leading additional jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the angle DeltaR between the two leading additional jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the angle DeltaR between the two leading additional jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the observable HT, along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the observable HT, along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the pt of the leading additional jet j1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at the particle level in the full phase space of the ttbar system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of pt of the leading additional jet j1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at the particle level in the full phase space of the ttbar system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of |eta| of the leading additional jet j1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at the particle level in the full phase space of the ttbar system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of |eta| of the leading additional jet j1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at the particle level in the full phase space of the ttbar system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of the pt of the subleading additional jet j2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at the particle level in the full phase space of the ttbar system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of pt of the subleading additional jet j2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at the particle level in the full phase space of the ttbar system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of |eta| of the subleading additional jet j2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at the particle level in the full phase space of the ttbar system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of |eta| of the subleading additional jet j2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at the particle level in the full phase space of the ttbar system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of the invariant mass of the two leading additional jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of tt system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of the invariant mass of the two leading additional jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of tt system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of the angle DeltaR between the two leading additional jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of tt system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of the angle DeltaR between the two leading additional jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of tt system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of the observable HT, along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of tt system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of the observable HT, along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of tt system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of the pt of the leading additional b-jet b1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the pt of the leading additional b-jet b1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of |eta| of the leading additional b-jet b1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of |eta| of the leading additional b-jet b1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the pt of the subleading additional b-jet b2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the pt of the subleading additional b-jet b2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of |eta| of the leading additional b-jet b2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of |eta| of the leading additional b-jet b2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the invariant mass of the two leading additional b-jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the invariant mass of the two leading additional b-jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the angle DeltaR between the two leading additional b-jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Normalized differential ttbar cross sections as a function of the angle DeltaR between the two leading additional b-jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the visible phase space.

Absolute differential ttbar cross sections as a function of the pt of the leading additional b-jet b1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of the pt of the leading additional b-jet b1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of |eta| of the leading additional b-jet b1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of |eta| of the leading additional b-jet b1 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of the pt of the subleading additional b-jet b2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of the pt of the subleading additional b-jet b2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of |eta| of the leading additional b-jet b2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of |eta| of the leading additional b-jet b2 in the event (not coming from the top quark decay products), along with their statistical, systematic, and total uncertainties. The results are presented at particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of the invariant mass of the two leading additional b-jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of the invariant mass of the two leading additional b-jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Absolute differential ttbar cross sections as a function of the angle DeltaR between the two leading additional b-jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Normalized differential ttbar cross sections as a function of the angle DeltaR between the two leading additional b-jets in the event (not coming from the top quark decay products), along with their statistical and systematic uncertainties. The results are presented at the particle level in the full phase space of the tt system, corrected for acceptance and branching fractions.

Gap fraction $f(p_T^{\rm jet})$ as function of leading additional jet transverse momentum $p_T^{\rm jet}$.

Gap fraction $f(p_T^{\rm jet})$ as function of leading additional jet transverse momentum $p_T^{\rm jet}$ in the region $|\eta|<0.8$.

Gap fraction $f(p_T^{\rm jet})$ as function of leading additional jet transverse momentum $p_T^{\rm jet}$ in the region $0.8<|\eta|<1.5$.

Gap fraction $f(p_T^{\rm jet})$ as function of leading additional jet transverse momentum $p_T^{\rm jet}$ in the region $1.5<|\eta|<2.4$.

Gap fraction $f(p_T^{\rm jet_2})$ as function of subleading additional jet transverse momentum $p_T^{\rm jet_2}$.

Gap fraction $f(p_T^{\rm jet_2})$ as function of subleading additional jet transverse momentum $p_T^{\rm jet_2}$ in the region $|\eta|<0.8$.

Gap fraction $f(p_T^{\rm jet_2})$ as function of subleading additional jet transverse momentum $p_T^{\rm jet_2}$ in the region $0.8<|\eta|<1.5$.

Gap fraction $f(p_T^{\rm jet_2})$ as function of subleading additional jet transverse momentum $p_T^{\rm jet_2}$ in the region $1.5<|\eta|<2.4$.

Gap fraction $f(H_T)$ as function of $H_T$.

Gap fraction $f(H_T)$ as function of $H_T$ in the region $|\eta|<0.8$.

Gap fraction $f(H_T)$ as function of $H_T$ in the region $0.8<|\eta|<1.5$.

Gap fraction $f(H_T)$ as function of $H_T$ in the region $1.5<|\eta|<2.4$.

Statistical covariance matrix for the absolute differential cross-section as a function of the number of jets with pt>30 GeV (see also table B.1).

Statistical covariance matrix for the normalized differential cross-section as a function of the number of jets with pt>30 GeV.

Statistical covariance matrix for the absolute differential cross-section as a function of the number of jets with pt>60 GeV (see also table B.1).

Statistical covariance matrix for the normalized differential cross-section as a function of the number of jets with pt>60 GeV.

Statistical covariance matrix for the absolute differential cross-section as a function of the number of jets with pt>100 GeV (see also table B.1).

Statistical covariance matrix for the normalized differential cross-section as a function of the number of jets with pt>100 GeV.

Signal selection efficiency as a function of mA.

Expected +2 sigma uncertainty band exclusion limit for Type-I models, as a function of tan beta and cos(beta-alpha).

Expected +1 sigma uncertainty band exclusion limit for Type-I models, as a function of tan beta and cos(beta-alpha).

Expected exclusion limit for Type-I models, as a function of tan beta and cos(beta-alpha).

Expected -1 sigma uncertainty band exclusion limit for Type-I models, as a function of tan beta and cos(beta-alpha).

Expected -2 sigma uncertainty band exclusion limit for Type-I models, as a function of tan beta and cos(beta-alpha).

Observed exclusion limit for Type-I models, as a function of tan beta and cos(beta-alpha).

Expected +2 sigma uncertainty band exclusion limit for Type-II models, as a function of tan beta and cos(beta-alpha).

Expected +1 sigma uncertainty band exclusion limit for Type-II models, as a function of tan beta and cos(beta-alpha).

Expected exclusion limit for Type-II models, as a function of tan beta and cos(beta-alpha).

Expected -1 sigma uncertainty band exclusion limit for Type-II models, as a function of tan beta and cos(beta-alpha).

Expected -2 sigma uncertainty band exclusion limit for Type-II models, as a function of tan beta and cos(beta-alpha).

Observed exclusion limit for Type-II models, as a function of tan beta and cos(beta-alpha).