Differential production cross-sections for prompt $D^{+} + D^{-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

Differential production cross-sections for prompt $D_{s}^{+} + D_{s}^{-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

Differential production cross-sections for prompt $D_{s}^{+} + D_{s}^{-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

Differential production cross-sections for prompt $D^{*+} + D^{*-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

Differential production cross-sections for prompt $D^{*+} + D^{*-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

The ratios of differential production cross-sections, $R_{13/5}$, for prompt $D^{0} + \bar{D}^{0}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

The ratios of differential production cross-sections, $R_{13/5}$, for prompt $D^{0} + \bar{D}^{0}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

The ratios of differential production cross-sections, $R_{13/5}$, for prompt $D^{+} + D^{-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

The ratios of differential production cross-sections, $R_{13/5}$, for prompt $D^{+} + D^{-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

The ratios of differential production cross-sections, $R_{13/5}$, for prompt $D_{s}^{+} + D_{s}^{-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

The ratios of differential production cross-sections, $R_{13/5}$, for prompt $D_{s}^{+} + D_{s}^{-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

The ratios of differential production cross-sections, $R_{13/5}$, for prompt $D^{*+} + D^{*-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

The ratios of differential production cross-sections, $R_{13/5}$, for prompt $D^{*+} + D^{*-}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D^{+}$ and $D^{0}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D^{+}$ and $D^{0}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D_{s}^{+}$ and $D^{0}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D_{s}^{+}$ and $D^{0}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D^{*+}$ and $D^{0}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D^{*+}$ and $D^{0}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D_{s}^{+}$ and $D^{+}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D_{s}^{+}$ and $D^{+}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D^{*+}$ and $D^{+}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D^{*+}$ and $D^{+}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D_{s}^{+}$ and $D^{*+}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

The ratios of differential production cross-section-times-branching fraction measurements for prompt $D_{s}^{+}$ and $D^{*+}$ mesons in bins of $(p_{\mathrm{T}}, y)$. The first uncertainty is statistical, and the second is the total systematic. All values are given in percent.

Summary of results for cross-section of non-prompt $J/\psi$ decaying to a muon pair for 8 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of prompt $\psi(2S)$ decaying to a muon pair for 7 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of prompt $\psi(2S)$ decaying to a muon pair for 8 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of non-prompt $\psi(2S)$ decaying to a muon pair for 7 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of non-prompt $\psi(2S)$ decaying to a muon pair for 8 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $J/\psi$ decaying to a muon pair as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $J/\psi$ decaying to a muon pair as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $\psi(2S)$ decaying to a muon pair as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $\psi(2S)$ decaying to a muon pair as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Mean weight correction factor for $J/\psi$ under the "longitudinal" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "transverse zero" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "transverse positive" spin-alignment transverse positive hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "transverse negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "longitudinal" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "transverse zero" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "transverse positive" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "transverse negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "longitudinal" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "transverse zero" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "transverse positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "transverse negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "longitudinal" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "transverse zero" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "transverse positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "transverse negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

psi(2S) double-differential cross section times branching fraction and the corresponding scaling factors to obtain the cross sections for different polarization scenarios (azimuthal polarization parameter in the center of mass helicity frame lambda_theta^HX = +1, -1, +0.03) as a function of pT for |y| < 1.2.

Ratio of psi(2S) to J/psi differential cross section times branching fractions assuming unpolarized productions as a function of pT for |y| < 1.2.

Inclusive Jet cross section with R = 0.5 in the rapidity bin 1.5 < |y| < 2. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.5 in the rapidity bin 2 < |y| < 2.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.5 in the rapidity bin 2.5 < |y| < 3. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 0 < |y| < 0.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 0.5 < |y| < 1. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 1 < |y| < 1.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 1.5 < |y| < 2. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 2 < |y| < 2.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 2.5 < |y| < 3. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 0 < |y| < 0.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 0.5 < |y| < 1. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 1 < |y| < 1.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 1.5 < |y| < 2. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 2 < |y| < 2.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 2.5 < |y| < 3. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Double Differential distributions for B/S0 production.

PT distributions for B0 production.

PT distributions for B+ production.

PT distributions for B/S0 production.

Rapidity distributions for B0 production.

Rapidity distributions for B+ production.

Rapidity distributions for B/S0 production.

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].

Inclusive Jet Cross Section for |rapidity| 1.5 TO 2.0 as a function of the jet transverse momentum. The (sys) error is the total systematic error, including the luminosity uncertainty of 2.2%.

Inclusive Jet Cross Section for |rapidity| 2.0 TO 2.5 as a function of the jet transverse momentum. The (sys) error is the total systematic error, including the luminosity uncertainty of 2.2%.

DiJet Cross Section for |rapidity| < 0.5 as a function of the dijet invariant mass. The (sys) error is the total systematic error, including the luminosity uncertainty of 2.2%.

DiJet Cross Section for |rapidity| 0.5 TO 1.0 as a function of the dijet invariant mass. The (sys) error is the total systematic error, including the luminosity uncertainty of 2.2%.

DiJet Cross Section for |rapidity| 1.0 TO 1.5 as a function of the dijet invariant mass. The (sys) error is the total systematic error, including the luminosity uncertainty of 2.2%.

DiJet Cross Section for |rapidity| 1.5 TO 2.0 as a function of the dijet invariant mass. The (sys) error is the total systematic error, including the luminosity uncertainty of 2.2%.

DiJet Cross Section for |rapidity| 2.0 TO 2.5 as a function of the dijet invariant mass. The (sys) error is the total systematic error, including the luminosity uncertainty of 2.2%.

Double differential cross section for UPSI(1S) production times the dimuon branching fraction as a function of PT for the rapidity region 3.0-3.5. The second systematic (sys) error is due to the unknown polarisation of the UPSI(1S).

Double differential cross section for UPSI(1S) production times the dimuon branching fraction as a function of PT for the rapidity region 3.5-4.0. The second systematic (sys) error is due to the unknown polarisation of the UPSI(1S).

Double differential cross section for UPSI(1S) production times the dimuon branching fraction as a function of PT for the rapidity region 4.0-4.5. The second systematic (sys) error is due to the unknown polarisation of the UPSI(1S).

Double differential cross section for UPSI(2S) production times the dimuon branching fraction as a function of PT for the rapidity region 2.0-2.5. The second systematic (sys) error is due to the unknown polarisation of the UPSI(2S).

Double differential cross section for UPSI(2S) production times the dimuon branching fraction as a function of PT for the rapidity region 2.5-3.0. The second systematic (sys) error is due to the unknown polarisation of the UPSI(2S).

Double differential cross section for UPSI(2S) production times the dimuon branching fraction as a function of PT for the rapidity region 3.0-3.5. The second systematic (sys) error is due to the unknown polarisation of the UPSI(2S).

Double differential cross section for UPSI(2S) production times the dimuon branching fraction as a function of PT for the rapidity region 3.5-4.0. The second systematic (sys) error is due to the unknown polarisation of the UPSI(2S).

Double differential cross section for UPSI(2S) production times the dimuon branching fraction as a function of PT for the rapidity region 4.0-4.5. The second systematic (sys) error is due to the unknown polarisation of the UPSI(2S).

Double differential cross section for UPSI(3S) production times the dimuon branching fraction as a function of PT for the rapidity region 2.0-2.5. The second systematic (sys) error is due to the unknown polarisation of the UPSI(3S).

Double differential cross section for UPSI(3S) production times the dimuon branching fraction as a function of PT for the rapidity region 2.5-3.0. The second systematic (sys) error is due to the unknown polarisation of the UPSI(3S).

Double differential cross section for UPSI(3S) production times the dimuon branching fraction as a function of PT for the rapidity region 3.0-3.5. The second systematic (sys) error is due to the unknown polarisation of the UPSI(3S).

Double differential cross section for UPSI(3S) production times the dimuon branching fraction as a function of PT for the rapidity region 3.5-4.0. The second systematic (sys) error is due to the unknown polarisation of the UPSI(3S).

Double differential cross section for UPSI(3S) production times the dimuon branching fraction as a function of PT for the rapidity region 4.0-4.5. The second systematic (sys) error is due to the unknown polarisation of the UPSI(3S).

Ratios of cross section with respect to the UPSI(1S) cross section as a function of PT in the rapidity range 2.0-4.4. The second systematic (sys) error is due to the unknown polarisation of the three states.

The (unpolarised) acceptance corrected J/PSI cross section times branching ratio to MU+ MU- for (PROMPT) and NON-PROMPT) production in the |rapidity| bin 1.6-2.1.

The (unpolarised) acceptance corrected J/PSI cross section times branching ratio to MU+ MU- for (PROMPT) and NON-PROMPT) production in the |rapidity| bin 2.1-2.4.

The (unpolarised) acceptance corrected PSI(2S) cross section times branching ratio to MU+ MU- for (PROMPT) and NON-PROMPT production in the |rapidity| bin 0.0-1.2.

The (unpolarised) acceptance corrected PSI(2S) cross section times branching ratio to MU+ MU- for (PROMPT) and NON-PROMPT production in the |rapidity| bin 1.2-1.6.

The (unpolarised) acceptance corrected PSI(2S) cross section times branching ratio to MU+ MU- for (PROMPT) and NON-PROMPT production in the |rapidity| bin 1.6-2.4.

The uncorrected visible J/PSI cross section times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 0.0-0.9.

The uncorrected visible J/PSI cross section times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 0.9-1.2.

The uncorrected visible J/PSI cross section times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 1.2-1.6.

The uncorrected visible J/PSI cross section times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 1.6-2.1.

The uncorrected visible J/PSI cross section times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 2.1-2.4.

The uncorrected visible PSI(2S) cross section times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 0.0-1.2.

The uncorrected visible PSI(2S) cross section times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 1.2-1.6.

The uncorrected visible PSI(2S) cross section times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 1.6-2.4.

The ratio between the PSI(2S) and J/PSI cross sections times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 0.0-1.2.

The ratio between the PSI(2S) and J/PSI cross sections times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 1.2-1.6.

The ratio between the PSI(2S) and J/PSI cross sections times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the |rapidity| bin 1.6-2.4.

The ratio between the PSI(2S) and J/PSI cross sections times branching ratio to MU+ MU- for PROMPT and NON-PROMPT production in the integrated |rapidity| bin 0.0-2.4.

The non-prompt fraction (FB) of J/PSI times branching ratio to MU+ MU- from B-HADRON decays in the |rapidity| bin 0.0-0.9.

The non-prompt fraction (FB) of J/PSI times branching ratio to MU+ MU- from B-HADRON decays in the |rapidity| bin 0.9-1.2.

The non-prompt fraction (FB) of J/PSI times branching ratio to MU+ MU- from B-HADRON decays in the |rapidity| bin 1.2-1.6.

The non-prompt fraction (FB) of J/PSI times branching ratio to MU+ MU- from B-HADRON decays in the |rapidity| bin 1.6-2.1.

The non-prompt fraction (FB) of J/PSI times branching ratio to MU+ MU- from B-HADRON decays in the |rapidity| bin 2.1-2.4.

The non-prompt fraction (FB) of PSI(2S) times branching ratio to MU+ MU- from B-HADRON decays in the |rapidity| bin 0.0-1.2.

The non-prompt fraction (FB) of PSI(2S) times branching ratio to MU+ MU- from B-HADRON decays in the |rapidity| bin 1.2-1.6.

The non-prompt fraction (FB) of PSI(2S) times branching ratio to MU+ MU- from B-HADRON decays in the |rapidity| bin 1.6-2.4.

The difference between the J/PSI cross section times branching ratio to MU+ MU- for non-prompt production calculated for four different polarization scenarios and the zero polarization values. The notation is (-1,CS), (+1,CS), (-1,HX), (+1,HX), where CS(HX) is the Collins-Soper (Helicity) frame and -1(+1) refer to full longitudinal (transverse) polarization.

The difference between the J/PSI cross section times branching ratio to MU+ MU- for non-prompt production calculated for four different polarization scenarios and the zero polarization values. The notation is (-1,CS), (+1,CS), (-1,HX), (+1,HX), where CS(HX) is the Collins-Soper (Helicity) frame and -1(+1) refer to full longitudinal (transverse) polarization.

The difference between the J/PSI cross section times branching ratio to MU+ MU- for non-prompt production calculated for four different polarization scenarios and the zero polarization values. The notation is (-1,CS), (+1,CS), (-1,HX), (+1,HX), where CS(HX) is the Collins-Soper (Helicity) frame and -1(+1) refer to full longitudinal (transverse) polarization.

The difference between the J/PSI cross section times branching ratio to MU+ MU- for non-prompt production calculated for four different polarization scenarios and the zero polarization values. The notation is (-1,CS), (+1,CS), (-1,HX), (+1,HX), where CS(HX) is the Collins-Soper (Helicity) frame and -1(+1) refer to full longitudinal (transverse) polarization.

The difference between the J/PSI cross section times branching ratio to MU+ MU- for non-prompt production calculated for four different polarization scenarios and the zero polarization values. The notation is (-1,CS), (+1,CS), (-1,HX), (+1,HX), where CS(HX) is the Collins-Soper (Helicity) frame and -1(+1) refer to full longitudinal (transverse) polarization.

The difference between the PSI(2S) cross section times branching ratio to MU+ MU- for non-prompt production calculated for four different polarization scenarios and the zero polarization values. The notation is (-1,CS), (+1,CS), (-1,HX), (+1,HX), where CS(HX) is the Collins-Soper (Helicity) frame and -1(+1) refer to full longitudinal (transverse) polarization.

The difference between the PSI(2S) cross section times branching ratio to MU+ MU- for non-prompt production calculated for four different polarization scenarios and the zero polarization values. The notation is (-1,CS), (+1,CS), (-1,HX), (+1,HX), where CS(HX) is the Collins-Soper (Helicity) frame and -1(+1) refer to full longitudinal (transverse) polarization.

The difference between the PSI(2S) cross section times branching ratio to MU+ MU- for non-prompt production calculated for four different polarization scenarios and the zero polarization values. The notation is (-1,CS), (+1,CS), (-1,HX), (+1,HX), where CS(HX) is the Collins-Soper (Helicity) frame and -1(+1) refer to full longitudinal (transverse) polarization.

Total J/PSI cross section from the di-electron data. The first error is statistical, the second is a systematic error. The second systematic errors is related to the unknown polarization. Only the one from the Helicity Frame is quoted here. It has the biggest influence in this rapidity range. Data updated from the erratum.

Total J/PSI cross section from the di-muon data. The first error is statistical, the second is a systematic error. The second systematic errors is related to the unknown polarization. Only the one from the Collins Soper Frame is quoted here. It has the biggest influence in this rapidity range.