Exclusion limit for BrHZX_BrXee

Exclusion limit for BrHZX_BrXmumu

Exclusion limit for BrHZX_BrXll

Exclusion limit for cah

Exclusion limit for cZh

Exclusion limit for kappa

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.

Z0 total and fiducial production cross sections times branching fractions.

W+ to W- ratios of total and fiducial production cross sections times branching fractions.

(W+ + W-) to Z0 ratios of total and fiducial production cross sections times branching fractions.

The fiducial and acceptance corrected UPSI(3S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range < 2.4. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(3S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(1S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range < 0.4. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(1S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(2S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range < 0.4. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(2S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(3S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range < 0.4. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(3S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(1S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 0.4 to 0.8. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(1S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(2S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 0.4 to 0.8. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(2S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(3S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 0.4 to 0.8. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(3S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(1S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 0.8 to 1.2. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(1S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(2S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 0.8 to 1.2. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(2S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(3S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 0.8 to 1.2. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(3S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(1S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 1.2 to 1.6. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(1S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(2S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 1.2 to 1.6. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(2S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(3S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 1.2 to 1.6. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(3S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(1S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 1.6 to 2.0. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(1S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(2S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 1.6 to 2.0. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(2S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(3S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 1.6 to 2.0. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(3S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(1S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 2.0 to 2.4. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(1S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(2S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 2.0 to 2.4. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(2S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(3S) production cross sections (times di-muon branching ratio) as a function of PT for the |rapidity| range 2.0 to 2.4. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(3S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(1S) production cross sections (times di-muon branching ratio) as a function of rapidity for PT < 50 GeV/c. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(1S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(2S) production cross sections (times di-muon branching ratio) as a function of rapidity for PT < 50 GeV/c. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(2S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The fiducial and acceptance corrected UPSI(3S) production cross sections (times di-muon branching ratio) as a function of rapidity for PT < 50 GeV/c. Note these are integrated cross sections and the acceptance-corrected cross sections assume the UPSI(3S) are unpolarized with the variations due to the 4 extreme polarization scenarios shown in the last 4 columns. The fiducial cross sections do not need to make any assumptions on the polarizations scenarios. The luminosity uncertainty of 4% is not included in the systematic errors.

The ratios of the UPSI(3S) to UPSI(1S) fiducial and acceptance cross sections as a function of PT for the |rapidiy| range < 2.4.

The ratios of the UPSI(2S) to UPSI(1S) fiducial and acceptance cross sections as a function of PT for the |rapidiy| range < 2.4.

The ratios of the UPSI(3S) to UPSI(2S) fiducial and acceptance cross sections as a function of PT for the |rapidiy| range < 2.4.

The acceptance-corrected UPSI(1S) production cross section, integrated and differential in PT, times the respective dimuon branching fraction, integrated over the rapidity range |y| < 1.2. The first (sys) error is the quadratic sum of all systematic uncertainties excluding that associated with the polarization of the UPSI(1S) which is shown separately as the second (sys) value. The latter has been obtained by calculating the acceptance with the +68 and -68% CL as given by the measured UPSI(1S) polarization [see. PRL 110 (2013) 081802].

The acceptance-corrected UPSI(2S) production cross section, integrated and differential in PT, times the respective dimuon branching fraction, integrated over the rapidity range |y| < 1.2. The first (sys) error is the quadratic sum of all systematic uncertainties excluding that associated with the polarization of the UPSI(2S) which is shown separately as the second (sys) value. The latter has been obtained by calculating the acceptance with the +68 and -68% CL as given by the measured UPSI(2S) polarization [see. PRL 110 (2013) 081802].

The acceptance-corrected UPSI(3S) production cross section, integrated and differential in PT, times the respective dimuon branching fraction, integrated over the rapidity range |y| < 1.2. The first (sys) error is the quadratic sum of all systematic uncertainties excluding that associated with the polarization of the UPSI(3S) which is shown separately as the second (sys) value. The latter has been obtained by calculating the acceptance with the +68 and -68% CL as given by the measured UPSI(3S) polarization [see. PRL 110 (2013) 081802].

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed AK7 jets, for the mean PT of the two leading jets in the range 500-600 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed AK7 jets, for the mean PT of the two leading jets in the range 600-800 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed AK7 jets, for the mean PT of the two leading jets in the range 800-1000 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed AK7 jets, for the mean PT of the two leading jets in the range 1000-1500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 220-300 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 300-450 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 450-500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 500-600 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 600-800 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 800-1000 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 1000-1500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 220-300 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 300-450 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 450-500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 500-600 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 600-800 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 800-1000 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 1000-1500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 220-300 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 300-450 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 450-500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 500-600 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 600-800 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 800-1000 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 1000-1500 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Total nonprompt X(3872) fraction without acceptance corrections.

Differential cross section for prompt P P --> X + anything times branching fraction X-> J/PSI pi+ pi-.

Cross section for prompt P P --> X + anything times branching fraction X-> J/PSI pi+ pi-.

Dipion invariant-mass spectrum for X(3872) ->J/PSI pi+pi- decays corrected for acceptance and efficiency, dividing by the total cross section for 0.5 < M(PI+PI-) < 0.78 GEV.