Best fit values of $\sigma(gg\to H\to ZZ)$, $\sigma_i/\sigma_{gg\mathrm{F}}$, and $\mathrm{B}^f/\mathrm{B}^{ZZ}$ relative to their SM prediction from the combined analysis of the $\sqrt{s}$=7 and 8 TeV data. The results are shown for the combination of ATLAS and CMS, and also separately for each experiment, together with their total uncertainties and their breakdown into the four components described in the text. The expected uncertainties in the measurements are also shown.

Best fit values of $\sigma(gg\to H\to WW)$, $\sigma_i/\sigma_{gg\mathrm{F}}$, and $\mathrm{B}^f/\mathrm{B}^{WW}$ from the combined analysis of the $\sqrt{s}$=7 and 8 TeV data. The values involving cross sections are given for $\sqrt{s}$=8 TeV, assuming the SM values for $\sigma_i(7 \mathrm{TeV})/\sigma_i(8 \mathrm{TeV})$. The results are shown for the combination of ATLAS and CMS, and also separately for each experiment, together with their total uncertainties and their breakdown into the four components described in the text. The expected uncertainties in the measurements are also shown.

Best fit values of $\sigma(gg\to H\to WW)$, $\sigma_i/\sigma_{gg\mathrm{F}}$, and $\mathrm{B}^f/\mathrm{B}^{WW}$ relative to their SM prediction from the combined analysis of the $\sqrt{s}$=7 and 8 TeV data. The results are shown for the combination of ATLAS and CMS, and also separately for each experiment, together with their total uncertainties and their breakdown into the four components described in the text. The expected uncertainties in the measurements are also shown.

Best fit values of $\kappa_{gZ}= \kappa_{g}\cdot\kappa_{Z} / \kappa_{H}$ and of the ratios of coupling modifiers, as defined in the most generic parameterisation described in the context of the $\kappa$ framework, from the combined analysis of the $\sqrt{s}$=7 and 8 TeV data. The results are shown for the combination of ATLAS and CMS and also separately for each experiment, together with their total uncertainties and their breakdown into the four components described in the text. The uncertainties in $\lambda_{tg}$ and $\lambda_{WZ}$, for which a negative solution is allowed, are calculated around the overall best fit value. The expected total uncertainties in the measurements are also shown. For those parameters with no sensitivity to the sign, only the absolute values are shown.

Measured global signal strength $\mu$ and its total uncertainty, together with the breakdown of the uncertainty into its four components as defined in the text. The results are shown for the combination of ATLAS and CMS, and separately for each experiment. The expected uncertainty, with its breakdown, is also shown.

Measured signal strengths $\mu$ and their total uncertainties for different Higgs boson production processes. The results are shown for the combination of ATLAS and CMS, and separately for each experiment, for the combined $\sqrt{s}$=7 and 8 TeV data. The expected uncertainties in the measurements are also displayed. These results are obtained assuming that the Higgs boson branching fractions are the same as in the SM.

Measured signal strengths $\mu$ and their total uncertainties for different Higgs boson decay channels. The results are shown for the combination of ATLAS and CMS, and separately for each experiment, for the combined $\sqrt{s}$=7 and 8 TeV data. The expected uncertainties in the measurements are also displayed. These results are obtained assuming that the Higgs boson production process cross sections at $\sqrt{s}$ = 7 and 8 TeV are the same as in the SM.

Results of the ten-parameter fit of $\mu_F^f = \mu_{gg\mathrm{F}+ttH}^f$ and $\mu_V^f = \mu_{\mathrm{VBF}+VH}^f$ for each of the five decay channels. The results are shown for the combination of ATLAS and CMS, together with their measured and expected uncertainties. The measured results are also shown separately for each experiment.

Results of the six-parameter fit of the global ratio $\mu_V/\mu_F = \mu_{\mathrm{VBF}+VH}/\mu_{gg\mathrm{F}+ttH}$ together with $\mu_F^f$ for each of the five decay channels. The results are shown for the combination of ATLAS and CMS, together with their measured and expected uncertainties. The measured results are also shown separately for each experiment.

Fit results allowing BSM loop couplings, assuming that $|\kappa_{V}| \le$ 1, where $\kappa_{V}$ denotes $\kappa_{Z}$ or $\kappa_{W}$, and that $\mathrm{B_{BSM}} \ge$ 0. The results for the combination of ATLAS and CMS are reported with their measured and expected uncertainties. Also shown are the results from each experiment. For the parameters with both signs allowed, the other 1$\sigma$ interval is shown on a second line. For those parameters with no sensitivity to the sign, only the absolute values are shown.

Fit results allowing BSM loop couplings, assuming that there are no additional BSM contributions to the Higgs boson width, i.e. $\mathrm{B_{BSM}}=0$. The results for the combination of ATLAS and CMS are reported with their measured and expected uncertainties. Also shown are the results from each experiment. For the parameters with both signs allowed, the other 1$\sigma$ interval is shown on a second line. When a parameter is constrained and reaches a boundary, namely $\mathrm{B_{BSM}}$ = 0, the uncertainty is not indicated. For those parameters with no sensitivity to the sign, only the absolute values are shown.

Fit results for the parameterisation assuming the absence of BSM particles in the loops ($\mathrm{B_{BSM}}$=0). The results with their measured and expected uncertainties are reported for the combination of ATLAS and CMS, together with the individual results from each experiment. For the parameters with both signs allowed, the other 1$\sigma$ CL interval is shown on a second line. When a parameter is constrained and reaches a boundary, namely $|\kappa_\mu|$ = 0, the uncertainty is not indicated. For those parameters with no sensitivity to the sign, only the absolute values are shown.

Summary of fit results for a parameterisation probing the ratios of coupling modifiers for up-type versus down-type fermions. The results for the combination of ATLAS and CMS are reported together with their measured and expected uncertainties. Also shown are the results from each experiment. The parameter $\kappa_{uu}$ is positive definite since $\kappa_H$ is always assumed to be positive. For the parameter $\lambda_{du}$, for which both signs are allowed, the other 1$\sigma$ CL interval is shown on a second line. Negative values for the parameter $\lambda_{Vu}$ are excluded by more than 4$\sigma$.

Summary of fit results for a parameterisation probing the ratios of coupling modifiers for leptons versus quarks. The results for the combination of ATLAS and CMS are reported together with their measured and expected uncertainties. Also shown are the results from each experiment. The parameter $\kappa_{qq}$ is positive definite since $\kappa_H$ is always assumed to be positive. For the parameter $\lambda_{lq}$, for which there is no sensitivity to the sign, only the absolute values are shown. Negative values for the parameter $\lambda_{Vq}$ are excluded by more than 4$\sigma$.

Correlation matrix obtained from the fit combining the ATLAS and CMS data using the generic parameterisation with 23 parameters, $\sigma_i\cdot\mathrm{B}^f$ for each specific channel $i\to H\to f$. Only 20 parameters are shown because the other three, corresponding to the $H\to ZZ$ decay channel for the $WH$, $ZH$, and $ttH$ production processes, are not measured with a meaningful precision.

Correlation matrix obtained from the fit combining the ATLAS and CMS data using the generic parameterisation with nine parameters, $\sigma(gg\to H\to ZZ)$, $\sigma_i/\sigma_{gg\mathrm{F}}$, and $\mathrm{B}^f/\mathrm{B}^{ZZ}$.

Correlation matrix obtained from the fit combining the ATLAS and CMS data using the generic parameterisation with seven parameters, $\kappa_{gZ}=\kappa_{g}\cdot\kappa_{Z} / \kappa_{H}$ and the ratios of coupling modifiers.

Expected correlation matrix obtained from the fit combining ATLAS and CMS pre-fit Asimov data sets using the generic parameterisation with 23 parameters, $\sigma_i\cdot\mathrm{B}^f$ for each specific channel $i\to H\to f$. Only 20 parameters are shown because the other three, corresponding to the $H\to ZZ$ decay channel for the $WH$, $ZH$, and $ttH$ production processes, are not measured with a meaningful precision.

Expected correlation matrix obtained from the fit combining ATLAS and CMS pre-fit Asimov data sets using the generic parameterisation with nine parameters, $\sigma(gg\to H\to ZZ)$, $\sigma_i/\sigma_{gg\mathrm{F}}$, and $\mathrm{B}^f/\mathrm{B}^{ZZ}$.

Expected correlation matrix obtained from the fit combining ATLAS and CMS pre-fit Asimov data sets using the generic parameterisation with seven parameters, $\kappa_{gZ}=\kappa_{g}\cdot\kappa_{Z} / \kappa_{H}$ and the ratios of coupling modifiers.

ATLAS+CMS combined best-fit and 68% and 95% CL negative log-likelihood contours in the ($\kappa_{g}$,$\kappa_{\gamma}$) plane.

ATLAS best-fit and 68% and 95% CL negative log-likelihood contours in the ($\kappa_{g}$,$\kappa_{\gamma}$) plane.

CMS best-fit and 68% and 95% CL negative log-likelihood contours in the ($\kappa_{g}$,$\kappa_{\gamma}$) plane.

Best-fit and 68% and 95% CL negative log-likelihood contours in the ($\kappa_{F}$,$\kappa_{V}$) plane.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow\gamma\gamma$ channel.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow ZZ$ channel.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow WW$ channel.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow\tau\tau$ channel.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow bb$ channel.

ATLAS best-fit and 68% and 95% CL negative log-likelihood contours in the ($\kappa_{F}$,$\kappa_{V}$) plane.

CMS best-fit and 68% and 95% CL negative log-likelihood contours in the ($\kappa_{F}$,$\kappa_{V}$) plane.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow\gamma\gamma$ channel, assuming $\kappa_{F}>0$.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow ZZ$ channel, assuming $\kappa_{F}>0$.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow WW$ channel, assuming $\kappa_{F}>0$.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow\tau\tau$ channel, assuming $\kappa_{F}>0$.

Best-fit and 68% CL negative log-likelihood contour in the ($\kappa_{F}$,$\kappa_{V}$) plane for the $H\rightarrow bb$ channel, assuming $\kappa_{F}>0$.

Best-fit and 68% and 95% CL negative log-likelihood contours in the ($\mu^{f}_{gg\mathrm{F}+ttH}$,$\mu^{f}_{\mathrm{VBF}+VH}$) plane for the $H\rightarrow\gamma\gamma$ channel.

Best-fit and 68% and 95% CL negative log-likelihood contours in the ($\mu^{f}_{gg\mathrm{F}+ttH}$,$\mu^{f}_{\mathrm{VBF}+VH}$) plane for the $H\rightarrow ZZ$ channel.

Best-fit and 68% and 95% CL negative log-likelihood contours in the ($\mu^{f}_{gg\mathrm{F}+ttH}$,$\mu^{f}_{\mathrm{VBF}+VH}$) plane for the $H\rightarrow WW$ channel.

Best-fit and 68% and 95% CL negative log-likelihood contours in the ($\mu^{f}_{gg\mathrm{F}+ttH}$,$\mu^{f}_{\mathrm{VBF}+VH}$) plane for the $H\rightarrow\tau\tau$ channel.

Best-fit and 68% and 95% CL negative log-likelihood contours in the ($\mu^{f}_{gg\mathrm{F}+ttH}$,$\mu^{f}_{\mathrm{VBF}+VH}$) plane for the $H\rightarrow bb$ channel.

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.

Normalized differential W+W- cross section as a function of the leading lepton pT. Both statistical and systematic uncertainties are included. Results are computed in a fiducial region defined by requiring zero jets at particle level with varying jet pT thresholds and requiring prompt leptons with pT > 20 GeV and abs(eta) < 2.5, before final-state radiation.

Normalized differential W+W- cross section as a function of the dilepton system. Both statistical and systematic uncertainties are included. Results are computed in a fiducial region defined by requiring zero jets at particle level with varying jet pT thresholds and requiring prompt leptons with pT > 20 GeV and abs(eta) < 2.5, before final-state radiation.

Normalized differential W+W- cross section as a function of the invariant mass. Both statistical and systematic uncertainties are included. Results are computed in a fiducial region defined by requiring zero jets at particle level with varying jet pT thresholds and requiring prompt leptons with pT > 20 GeV and abs(eta) < 2.5, before final-state radiation.

Normalized differential W+W- cross section as a function of the angular separation between leptons. Both statistical and systematic uncertainties are included. Results are computed in a fiducial region defined by requiring zero jets at particle level with varying jet pT thresholds and requiring prompt leptons with pT > 20 GeV and abs(eta) < 2.5, before final-state radiation.

Measured cWWW/LAMBDA^2, cW/LAMBDA^2, and cB/LAMBDA^2 coupling constants.

Measured 95% CL interval of the cWWW/LAMBDA^2, cW/LAMBDA^2, and cB/LAMBDA^2 coupling constants.

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).

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.

Event yields for the same-sign dilepton mu+mu category.

Event yields for the same-sign dilepton mu+e category.

Event yields for the multilepton event categories Explanation of categories: C1 - 3 lepton, 0 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 600 to 1000 C2 - 3 lepton, 0 tau, 0 OSSF, >=1 b-tag, ST in 600 to 1000 C3 - 3 lepton, 0 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 1000 to 1500 C4 - 3 lepton, 0 tau, 0 OSSF, >=1 b-tag, ST in 1000 to 1500 C5 - 3 lepton, 0 tau, 1 OSSF, 0 b-tag, off-Z, ST in 600 to 1000 C6 - 3 lepton, 0 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 600 to 1000 C7 - 3 lepton, 1 tau, 0 OSSF, >=1 b-tag, ST in 600 to 1000 C8 - 3 lepton, 1 tau, 0 OSSF, >=1 b-tag, ST in 1000 to 1500 C9 - 3 lepton, 0 tau, 0 OSSF, 0 b-tag, ST in 600 to 1000 C10 - 3 lepton, 0 tau, 1 OSSF, 0 b-tag, off-Z, ST in 1000 to 1500 C11 - 3 lepton, 0 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 1000 to 1500 C12 - 3 lepton, 0 tau, 1 OSSF, >=1 b-tag, on-Z, ST in 600 to 1000 C13 - 3 lepton, 0 tau, 0 OSSF, 0 b-tag, ST in 1000 to 1500 C14 - 3 lepton, 1 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 600 to 1000 C15 - 3 lepton, 1 tau, 0 OSSF, 0 b-tag, ST in 600 to 1000 C16 - 3 lepton, 1 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 1000 to 1500 C17 - 4 lepton, 1 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 600 to 1000 C18 - 4 lepton, 0 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 600 to 1000 C19 - 3 lepton, 1 tau, 0 OSSF, 0 b-tag, ST in 100 to 1500 C20 - 4 lepton, 0 tau, 2 OSSF, >=1 b-tag, off-Z, ST in 600 to 1000 C21 - 3 lepton, 0 tau, 1 OSSF, >=1 b-tag, on-Z, ST in 1000 to 1500 C22 - 3 lepton, 0 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 300 to 600 C23 - 3 lepton, 0 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 1500 to 2000 C24 - 3 lepton, 1 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 600 to 1000 C25 - 3 lepton, 0 tau, 1 OSSF, 0 b-tag, off-Z, ST in 600 to 1000 C26 - 4 lepton, 1 tau, 1 OSSF, >=1 b-tag, off-Z, ST in 300 to 600 Note: "n/a" signifies a category which does not contribute for a given signal hypothesis.

Event yields for the all-hadronic event categories.

Event yields for the opposite sign dilepton event categories.

Cross section limits for all branching ratio combinations.

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.

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 $p_{T}$-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.

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'-].

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.

Observed and expected limits for the FCNC couplings at $\sqrt{s}=7$, $8$ TeV, and for combined $7+8$ TeV data.

Observed and expected limits for the FCNC branching ratios at $\sqrt{s}=7$, $8$ TeV, and for combined $7+8$ TeV data.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side in pPb collisions as a function of multiplicity with individual track pT between 0.3 to 3.0 GeV/c.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions as a function of multiplicity with individual track pT between 0.3 to 3.0 GeV/c.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions as a function of centrality with individual track pT between 0.3 to 3.0 GeV/c, where the average multiplicity value is plotted on figure in order to compare with pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side, p-going side in pPb collisions as a function of multiplicity with individual track pT between 0.3 to 3.0 GeV/c.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions as a function of multiplicity with individual track pT between 0.3 to 3.0 GeV/c.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions as a function of centrality with individual track pT between 0.3 to 3.0 GeV/c, where the average multiplicity value is plotted on figure in order to compare with pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going and p-going direction in pPb collisions and in PbPb collisions as a function DeltaEta for multiplicity [185,220) with individual track pT between 0.3 to 3.0 GeV/c. Data points are plotted at the bin center.

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%.