Covariance matrix (statistical and systematic uncertainties combined) with the muon $p_{T}>35$ GeV. The units are in $10^{-4}$.

The DY pre-FSR cross section measurements for the combined dimuon and dielectron channels normalized to the Z-peak region in the full acceptance.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 20-30 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 30-45 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 45-60 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 60-120 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 120-200 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 200-1500 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

Lambda-Phi in the CS frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta-Phi in the CS frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta-Phi in the CS frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Tilde in the CS frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Tilde in the CS frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta in the HX frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta in the HX frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Phi in the HX frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Phi in the HX frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta-Phi in the HX frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta-Phi in the HX frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Tilde in the HX frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Tilde in the HX frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta in the PX frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta in the PX frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Phi in the PX frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Phi in the PX frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta-Phi in the PX frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta-Phi in the PX frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Tilde in the PX frame for the J/psi as a function of pT for 0.0 < |y| < 0.6.

Lambda-Tilde in the PX frame for the J/psi as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta in the CS frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta in the CS frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta in the CS frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Phi in the CS frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Phi in the CS frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Phi in the CS frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Theta-Phi in the CS frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta-Phi in the CS frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta-Phi in the CS frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Tilde in the CS frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Tilde in the CS frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Tilde in the CS frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Theta in the HX frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta in the HX frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta in the HX frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Phi in the HX frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Phi in the HX frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Phi in the HX frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Theta-Phi in the HX frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta-Phi in the HX frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta-Phi in the HX frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Tilde in the HX frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Tilde in the HX frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Tilde in the HX frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Theta in the PX frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta in the PX frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta in the PX frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Phi in the PX frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Phi in the PX frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Phi in the PX frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Theta-Phi in the PX frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Theta-Phi in the PX frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Theta-Phi in the PX frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Lambda-Tilde in the PX frame for the psi(2S) as a function of pT for 0.0 < |y| < 0.6.

Lambda-Tilde in the PX frame for the psi(2S) as a function of pT for 0.6 < |y| < 1.2.

Lambda-Tilde in the PX frame for the psi(2S) as a function of pT for 1.2 < |y| < 1.5.

Differential cross-section measurement for B+ production multiplied by the branching ratio to the J/PSI < MU+ MU- > K+ final state in B+ pT intervals in the B+ rapidity range 1.5<|y|<2.25 The first quoted uncertainty is statistical, the second uncertainty is systematic.

Differential cross-section measurement for B+ production multiplied by the branching ratio to the J/PSI < MU+ MU- > K+ final state in B+ pt intervals in the B+ rapidity (y) range 0<|y|<2.25. The first quoted uncertainty is statistical, the second uncertainty is systematic.

Differential cross-section measurement for B+ production multiplied by the branching ratio to the J/PSI < MU+ MU- > K+ final state in B+ rapidity intervals in the B+ pT range 9 GeV - 120 GeV. The first quoted uncertainty is statistical, the second uncertainty is systematic.

PT dependences of the differential multiplicities for 0.0080 < x_Bjorken < 0.0120 and 1.00 < Q^2 < 1.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0080 < x_Bjorken < 0.0120 and 1.50 < Q^2 < 2.10 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 1.00 < Q^2 < 1.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 1.50 < Q^2 < 2.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 2.50 < Q^2 < 3.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 1.00 < Q^2 < 1.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 1.50 < Q^2 < 2.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 2.50 < Q^2 < 3.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 3.50 < Q^2 < 5.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0350 and 1.00 < Q^2 < 1.20 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 1.20 < Q^2 < 1.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 1.50 < Q^2 < 2.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 2.50 < Q^2 < 3.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 3.50 < Q^2 < 6.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0500 and 1.50 < Q^2 < 2.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 2.50 < Q^2 < 3.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 3.50 < Q^2 < 6.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 6.00 < Q^2 < 10.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0700 < x_Bjorken < 0.1200 and 3.50 < Q^2 < 6.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0700 < x_Bjorken < 0.1200 and 6.00 < Q^2 < 10.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0045 < x_Bjorken < 0.0060 and 1.00 < Q^2 < 1.25 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0060 < x_Bjorken < 0.0080 and 1.00 < Q^2 < 1.30 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0060 < x_Bjorken < 0.0080 and 1.30 < Q^2 < 1.70 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0080 < x_Bjorken < 0.0120 and 1.00 < Q^2 < 1.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0080 < x_Bjorken < 0.0120 and 1.50 < Q^2 < 2.10 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 1.00 < Q^2 < 1.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 1.50 < Q^2 < 2.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 2.50 < Q^2 < 3.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 1.00 < Q^2 < 1.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 1.50 < Q^2 < 2.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 2.50 < Q^2 < 3.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 3.50 < Q^2 < 5.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0350 and 1.00 < Q^2 < 1.20 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 1.20 < Q^2 < 1.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 1.50 < Q^2 < 2.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 2.50 < Q^2 < 3.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 3.50 < Q^2 < 6.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0500 and 1.50 < Q^2 < 2.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 2.50 < Q^2 < 3.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 3.50 < Q^2 < 6.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 6.00 < Q^2 < 10.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0700 < x_Bjorken < 0.1200 and 3.50 < Q^2 < 6.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0700 < x_Bjorken < 0.1200 and 6.00 < Q^2 < 10.00 GeV^2 for Negative hadrons.

Fitted average PTs for positive hadrons.

Fitted average PTs for negative hadrons.

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 measured PHI* distributions for the dimuon events corrected back to the born level. The distributions are normalised to unity inidividually for each abs(yrap) bin and channel.

The measured PHI* distributions for the dimuon events corrected back to the dress level. The distributions are normalised to unity inidividually for each abs(yrap) bin and channel.

The measured PHI* distributions for the dimuon events corrected back to the bare level. The distributions are normalised to unity inidividually for each abs(yrap) bin and channel.

The combined normalised differential PHI* distributions at the Born level in the different rapidity ranges.

Expected and observed number of events with m_ll > 1300 GeV in the dielectron and dimuon channels. Yields given for different MS values correspond to the sum of signal and background events, with the signal obtained in the GRW formalism. All yields are normalized to the Z peak control region. The errors quoted originate from systematic uncertainties and limited MC statistics.

Expected and observed 95% C.L. lower limits on MS in the dielectron and dimuon channels, as well as for the combination of those channels without and with the diphoton channel in the GRW formalism. Separate results are provided for the different choices of flat priors.

Observed 95% C.L. lower limits on MS (in units of TeV), including systematic uncertainties, for ADD signal in the GRW, Hewett and HLZ formalisms with no K-factor applied to the signal. Separate results are provided for the different choices of flat priors.

Observed 95% C.L. lower limits on of TeV), including systematic uncertainties, for in the GRW, Hewett and HLZ formalisms with K-factors of 1.6 and 1.7 applied to the signal for the dilepton and diphoton channels, respectively. Separate results are provided for the different choices of flat priors.

Fiducial Upsilon(3S) production cross-section, where pT>4 GeV and |eta|<2.3 for both muons, as a function of Upsilon(3S) pT in the Upsilon(3S) rapidity (|y|) bins 0-1.2 and 1.2-2.25. The first uncertainty is statistical, the second is systematic.

Fiducial Upsilon(nS) production cross-section, where pT>4 GeV and |eta|<2.3 for both muons, as a function of Upsilon(nS) rapidity (|y|) in Upsilon(nS) PT ranging from 0 - 70 GeV. The first uncertainty is statistical, the second is systematic.

Inclusive Upsilon(1S) production cross-section as a function of Upsilon(1S) pT in the Upsilon(1S) rapidity (|y|) bins 0-1.2 and 1.2-2.25. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Inclusive Upsilon(2S) production cross-section as a function of Upsilon(2S) pT in the Upsilon(2S) rapidity (|y|) bins 0-1.2 and 1.2-2.25. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Inclusive Upsilon(3S) production cross-section as a function of Upsilon(3S) pT in the Upsilon(3S) rapidity (|y|) bins 0-1.2 and 1.2-2.25. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Inclusive Upsilon(nS) production cross-section as a function of Upsilon(nS) rapidity (|y|) in Upsilon(nS) PT ranging from 0 - 70 GeV. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Ratio of Upsilon(2S) to Upsilon(1S) inclusive cross-section as a function of Upsilon pT in the Upsilon rapidity (|y|) bins 0-1.2 and 1.2-2.25. The first uncertainty is statistical, the second is systematic.

Ratio of Upsilon(3S) to Upsilon(1S) inclusive cross-section as a function of Upsilon pT in the Upsilon rapidity (|y|) bins 0-1.2 and 1.2-2.25. The first uncertainty is statistical, the second is systematic.

Ratio of Upsilon(2S) and Upsilon(3S) to Upsilon(1S) inclusive cross-section as a function of Upsilon rapidity (|y|) in Upsilon pT 0 - 70 GeV. The first uncertainty is statistical, the second is systematic.

The Acceptance, Efficiency and Acceptance x Efficiency for the tau+muon channel as a function of Lambda and Tan(Beta).

The Acceptance, Efficiency and Acceptance x Efficiency for the tau+electron channel as a function of Lambda and Tan(Beta).

Number of tracks in vertex vs invariant mass of vertex (DATA) The number of tracks in the vertex vs the invariant mass of the vertex, for the data, and for the MH signal sample respectively. All selection cuts are applied, with the exceptions of those on the variables in the plot (Ntrk and mass), and the offline muon requirements.

Number of tracks in vertex vs invariant mass of vertex (SIGNAL) The number of tracks in the vertex vs the invariant mass of the vertex, for the data, and for the MH signal sample respectively. All selection cuts are applied, with the exceptions of those on the variables in the plot (Ntrk and mass), and the offline muon requirements.

95% CL upper limit on sigma.BR^2 vs c*tau The observed 95% CL upper limits on the cross-section for squark production, multiplied by the branching fraction for both squarks to decay to long-lived neutralinos, which in turn decay to mu+jets, given that we observed zero events in the signal region.

Expected upper limit on sigma.BR^2 vs c*tau The expected 95% CL upper limits on the cross-section for squark production, multiplied by the branching fraction for both squarks to decay to long-lived neutralinos, which in turn decay to mu+jets.

Observed and predicted dimuon invariant mass (m_mumu) distribution in the search region. The bin width is constant in log(m_mumu).

Expected and observed 95% CL limits on the cross-section times branching ratio (sigma*B) for Zprime_SSM production and the two E6-motivated Zprime models with lowest and highest sigma*B for the combination of the dielectron and dimuon channels.

Expected sigma*B for Zprime_SSM production and the two E6-motivated Zprime models with lowest and highest sigma*B.

Expected and observed 95% CL limits on sigma*B for Z* boson production for the combination of the dielectron and dimuon channels.

Expected sigma*B for Z* boson production.

Expected and observed 95% CL limits on M_{G*} versus k/Mbar_{Pl} for the combination of dielectron and dimuon channels.

Expected and observed 95% CL limits on M_{TS} versus eta_{TS} for the combination of dielectron and dimuon channels.

Expected and observed 95% CL limits on M_{pi_T} versus M_{rho_T,omega_T} for the combination of dielectron and dimuon channels.

Expected and observed 95% CL limits on M_A versus the coupling strength g-tilde for the combination of dielectron and dimuon channels.

Expected and observed 95% CL limits on g as a function of M_KK, for the combination of dielectron and dimuon channels.

Expected and observed upper limits on gammaprime within the Minimal Zprime Models parameterization, for the combination of dielectron and dimuon channels. The lower boundary corresponds to tan(theta) = 1.43 and the upper boundary to tan(theta) = -1.19. Two representative values of theta are tan(theta) = 0 and tan(theta) = -2 which correspond to the Z_{B-L} and Z_{3R} model at specific values of gammaprime respectively.

Distribution of the PT of the leading muon for E-MU events in the Signal Region, before the application of the leading lepton PT cut.

Distribution of the missing ET for all events in the Signal Region.

Distribution of MET-significnce, ie the missing ET/sqrt(scalar sum of PT of all leptons and jets), for all events in the Signal Region.

Distribution of the missing ET for E-E events in the Z Control Region.

Distribution of the missing ET for MU-MU events in the Z Control Region.

Distribution of the missing ET for E-E events in the Top Control Region.

Distribution of the missing ET for E-MU events in the Top Control Region.

Distribution of the missing ET for MU-MU events in the Top Control Region.

Distribution of the Jet Multiplicity for all events in the Top Control Region.

Distribution of the B-Jet Multiplicity for all events in the Top Control Region.

Distribution of the PT of the leading Jet for all events in the Top Control Region.

Distribution of the PT of the leading B-Jet for all events in the Top Control Region.

Observed and predicted W+W- transverse mass distribution in the E-E channel. Also tabulated are the predictions for a RS graviton of mass 1000 GeV and a bulk RS graviton with mass 600 GeV.

Observed and predicted W+W- transverse mass distribution in the E-MU channel. Also tabulated are the predictions for a RS graviton of mass 1000 GeV and a bulk RS graviton with mass 600 GeV.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the muon channel for rapidity |y| of 0-1.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the muon channel for rapidity |y| of 1-1.25.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the muon channel for rapidity |y| of 1.25-1.5.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the muon channel for rapidity |y| of 1.5-2.4.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the electron channel for rapidity |y| of 0-1.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the electron channel for rapidity |y| of 1-1.25.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the electron channel for rapidity |y| of 1.25-1.5.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the electron channel for rapidity |y| of 1.5-2.4.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the electron+muon channel for rapidity |y| of 0-1.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the electron+muon channel for rapidity |y| of 1-1.25.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the electron+muon channel for rapidity |y| of 1.25-1.5.

Statistical correlation (in percentage) of the unfolded AFB between the mass bins in the electron+muon channel for rapidity |y| of 1.5-2.4.

The distrubution of second leading jet pT for SR1 for the combined EE and MUMU channels. Tabulated are the observed Data rates and the Standard Model predictions as well as the distributions expected for two signal scenarios, both with an STOP mass of 250 GeV, and NEUTRALINO1 masses of 100 GeV and 220 GeV respectively. The last pT bin includes the number of overflow events for both data abd SM expectation.

The observed exclusion limits at 95% C.L. (using the CLs prescription) in the stop-neutralino1 mass plane, assuming direct stop pair production in the framework of GMSB models with light higgsinos.

The expected exclusion limits at 95% C.L. (using the CLs prescription) in the stop-neutralino1 mass plane, assuming direct stop pair production in the framework of GMSB models with light higgsinos.

The +1sigma contour around the median of the expected exclusion limits at 95% C.L. (using the CLs prescription) in the stop-neutralino1 mass plane, assuming direct stop pair production in the framework of GMSB models with light higgsinos.

The -1sigma contour around the median of the expected exclusion limits at 95% C.L. (using the CLs prescription) in the stop-neutralino1 mass plane, assuming direct stop pair production in the framework of GMSB models with light higgsinos.

The acceptance, using prompt leptons only, in the stop1-neutralino1 mass plane for SR1 and SR2.

The efficiancy in the stop1-neutralino1 mass plane for SR1 and SR2.

The total systematic uncertainty, including both theoretical and experimental uncertainties, in the stop1-neutralino1 mass plane for SR1 and SR2.

The CLs values in the stop1-neutralino1 mass plane for SR1 and SR2.

The number of generated MC events for each signal point in the stop1-neutralino1 mass plane before applying the dilepton filter efficiency. After that, 25K events per point are simulated.

The cross section of stop1-stop1 in the stop1-neutralino1 mass plane.

Toward $\sum p_\perp$ density vs $p_\perp^{\mu\mu}$.

Transverse $\sum p_\perp$ density vs $p_\perp^{\mu\mu}$.

Away $\sum p_\perp$ density vs $p_\perp^{\mu\mu}$.

Toward $\langle p_\perp \rangle$ vs $p_\perp^{\mu\mu}$.

Transverse $\langle p_\perp \rangle$ vs $p_\perp^{\mu\mu}$.

Away $\langle p_\perp \rangle$ vs $p_\perp^{\mu\mu}$.

Towards $+$ transverse $N_\text{chg}$ density vs $m_{\mu\mu}$, $p_\perp^{\mu\mu} < 5$ GeV.

Towards $+$ transverse $\sum p_\perp$ density vs $m_{\mu\mu}$, $p_\perp^{\mu\mu} < 5$ GeV.

Towards $+$ transverse $\langle p_\perp \rangle$ vs $m_{\mu\mu}$, $p_\perp^{\mu\mu} < 5$ GeV.

Toward $N_\text{chg}$.

Transverse $N_\text{chg}$.

Away $N_\text{chg}$.

Toward $p_\perp$.

Transverse $p_\perp$.

Away $p_\perp$.

Transverse $N_\text{chg}$, $p_\perp(\mu\mu) < 5$ GeV.

Transverse $p_\perp$, $p_\perp(\mu\mu) < 5$ GeV.

Differential J/$\psi$ production cross section at $\sqrt{s}=2.76$ TeV. J/$\psi$ production cross section at $\sqrt{s}=2.76$ TeV. The first uncertainty is statistical, the second one is $y$-correlated, the third one is uncorrelated. Polarization-related uncertainties are not included. The value for $-0.9<y<0.9$ refers to J/$\psi\rightarrow {\rm e}^+{\rm e}^-$, the remaining values to J/$\psi\rightarrow \mu^+\mu^-$.

The measured transverse asymmetry from the deuteron target as a function of the variable X. Mean values are also given for the variables Q**2[GeV^2], Y, Z, M[GeV], M**2[GeV^2], SIN(THETA), COS(THETA), COS(THETA)**2 and the transverse spin transfer coefficient DNN.

The measured transverse asymmetry from the deuteron target as a function of the variable Z. Mean values are also given for the variables Q**2[GeV^2], Y, X, M[GeV], M**2[GeV^2], SIN(THETA), COS(THETA), COS(THETA)**2 and the transverse spin transfer coefficient DNN.

The measured transverse asymmetry from the deuteron target as a function of the variable M. Mean values are also given for the variables Q**2[GeV^2], Y, Z, X, M**2[GeV^2], SIN(THETA), COS(THETA), COS(THETA)**2 and the transverse spin transfer coefficient DNN Note that the data in the last bin (>1.5) does not contribute to the X and Z distributions.

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.

Covariance matrix values between the rapidity bins for the electrons data sample.

Covariance matrix values between the rapidity bins for the combined data sample.

Covariance matrix values between the QT bins for the muons data sample.

Covariance matrix values between the QT bins for the electrons data sample.

Covariance matrix values between the QT bins for the combined data sample.

Efficiency as a function of the radial vertex position for displaced vertices in the signal MC sample MH, with squark mass 700 GeV and neutralino mass 494 GeV, in events that pass the trigger and primary vertex cuts and also requiring the reconstructed vertex to have at least 4 tracks, an invariant mass > 10 GeV and radial distance from the primary vertex > 4mm, and the event to contain a reconstructed muon with pT > 45 GeV.

Efficiency as a function of the radial vertex position for displaced vertices in the signal MC sample ML, with squark mass 700 GeV and neutralino mass 108 GeV, in events that pass the trigger and primary vertex cuts.

Efficiency as a function of the radial vertex position for displaced vertices in the signal MC sample ML, with squark mass 700 GeV and neutralino mass 108 GeV, in events that pass the trigger and primary vertex cuts and also requiring the reconstructed displaced vertex to have at least 4 tracks, an invariant mass > 10 GeV and radial distance from the primary vertex > 4mm.

Efficiency as a function of the radial vertex position for displaced vertices in the signal MC sample ML, with squark mass 700 GeV and neutralino mass 108 GeV, in events that pass the trigger and primary vertex cuts and also requiring the reconstructed vertex to have at least 4 tracks, an invariant mass > 10 GeV and radial distance from the primary vertex > 4mm, and the event to contain a reconstructed muon with pT > 45 GeV.

The invariant mass of reconstructed displaced vertices in the data after the trigger and muon requirements, and the background MC estimate scaled to the integrated luminosity of the data.

The distribution of numbner of tracks in reconstructed displaced vertices in the data after the trigger and muon requirements, and the background MC estimate scaled to the integrated luminosity of the data.

The distribution of radial position of reconstructed displaced vertices in the data after the trigger and muon requirements, and the background MC estimate scaled to the integrated luminosity of the data.

Observed and predicted missing ET distributions.

Observed 95% CL upper limits on the sneutrino cross section times its e-mu branching ratio.

Observed 95% CL upper limits on the zprime cross section times its e-mu branching ratio.

95% CL upper limits on lambdaprime_311 coupling as a function of the sneutrino mass for three values of lamdba_312.

RPV sneutrino signal selection efficiency as a function of the sneutrino mass.

The Zprime signal selection efficiency as a function of the Zprime mass.

Inclusive muon cross section from W+->mu+nu simulated with MC with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from W-->mu-nu simulated with MC with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from Z->mu+mu- simulated with MC with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV (the Z is defined as Z/gamma* with m_ll > 60 GeV): the error shown is due to the MC statistics.

Inclusive muon cross section from backgrounds: Z->tau tau, ttbar, Drell-Yan->mu+mu- (Drell-Yan is defined as Z/gamma* with m_ll < 60 GeV) simulated with Pythia with MRSTLO* pdf set for |eta| < 2.5 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from bbar+ccbar production and decays simulated with FONLL with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV: the error shown is the uncertainty due to scale variation, alpha_s+pdf using CTEQ6.6 error set and the heavy quark masses.

Inclusive muon cross section from bbar+ccbar simulated with FONLL removing the resummation term with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV?.

Inclusive muon cross section for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: (stat) statistical error, (sys) systematic error. The first systematic error is the intrinsic error of the measurement, the second is the error due to the luminosity.

Inclusive muon cross section after subtraction of W,Z, Drell-Yan and top background for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: (stat): statistical error, (sys): systematic error. The first systematic error is the intrinsic error of the measurement, the second the error due to the luminosity, the third is due to the subtraction of the background and is dominated by the error on the W, Z inclusive cross sections.

Inclusive muon cross section from W+->mu+nu simulated with MC with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from W-->mu-nu simulated with MC with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from Z->mu+mu- simulated with MC with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV (the Z is defined as Z/gamma* with m_ll > 60 GeV): the error shown is due to the MC statistics.

Inclusive muon cross section from backgrounds: Z->tau tau, ttbar, Drell-Yan->mu+mu- (Drell-Yan is defined as Z/gamma* with m_ll < 60 GeV) simulated with Pythia with MRSTLO* pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from bbar+ccbar production and decays simulated with FONLL with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: the error shown is the uncertainty due to scale variation, alpha_s+pdf using CTEQ6.6 error set and the heavy quark masses.

Inclusive muon cross section from bbar+ccbar simulated with FONLL removing the resummation term with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV.

Transverse mass after requiring one muon with pT>20 GeV, at least three jets with pT>60,25,25 GeV and dphi(jets,Etmiss)>0.2.

Effective mass after requiring one electron with pT>25 GeV, at least three jets with pT>60,25,25 GeV and dphi(jets,Etmiss)>0.2.

Effective mass after requiring one muon with pT>20 GeV, at least three jets with pT>60,25,25 GeV and dphi(jets,Etmiss)>0.2.

Missing transverse energy after requiring one electron with pT>25 GeV, at least four jets with pT>60,25,25,25 GeV and dphi(jets,Etmiss)>0.2.

Missing transverse energy after requiring one muon with pT>20 GeV, at least four jets with pT>60,25,25,25 GeV and dphi(jets,Etmiss)>0.2.

Transverse mass after requiring one electron with pT>25 GeV, at least four jets with pT>60,25,25,25 GeV and dphi(jets,Etmiss)>0.2.

Transverse mass after requiring one muon with pT>20 GeV, at least four jets with pT>60,25,25,25 GeV and dphi(jets,Etmiss)>0.2.

Effective mass after requiring one electron with pT>25 GeV, at least four jets with pT>60,25,25,25 GeV and dphi(jets,Etmiss)>0.2.

Effective mass after requiring one muon with pT>20 GeV, at least four jets with pT>60,25,25,25 GeV and dphi(jets,Etmiss)>0.2.

Effective mass in the electron plus three jets W+jets control region.

Effective mass in the muon plus three jets W+jets control region.

Effective mass in the electron plus three jets top control region.

Effective mass in the muon plus three jets top control region.

Number of b-tagged jets in the combined electron plus three jets W+jets and top control region.

Number of b-tagged jets in the combined muon plus three jets W+jets and top control region.

Effective mass in the electron plus four jets W+jets control region.

Effective mass in the muon plus four jets W+jets control region.

Effective mass in the electron plus four jets top control region.

Effective mass in the muon plus four jets top control region.

Effective mass in the 3-jet loose signal region (electron channel).

Effective mass in the 3-jet loose signal region (muon channel).

Effective mass in the 3-jet tight signal region (electron channel).

Effective mass in the 3-jet tight signal region (muon channel).

Effective mass in the 4-jet loose signal region (electron channel).

Effective mass in the 4-jet loose signal region (muon channel).

Effective mass in the 4-jet tight signal region (electron channel).

Effective mass in the 4-jet tight signal region (muon channel).

Expected 95% CL exclusion limits in the MSUGRA/CMSSM framework with the combined electron and muon channels.

Observed 95% CL exclusion limits in the MSUGRA/CMSSM framework with the combined electron and muon channels.

Inclusive J/psi production cross-section as a function of J/psi pT in the J/psi rapidity (|y|) bin 1.5<|y|<2. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Inclusive J/psi production cross-section as a function of J/psi pT in the J/psi rapidity (|y|) bin 0.75<|y|<1.5. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Inclusive J/psi production cross-section as a function of J/psi pT in the J/psi rapidity (|y|) bin |y|<0.75. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Non-prompt to inclusive production cross-section fraction fB as a function of J/psi pT for J/psi rapidity |y|<0.75 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0). The spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses, plus the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic, the third number is the uncertainty due to spin-alignment.}.

Non-prompt to inclusive production cross-section fraction fB as a function of J/psi pT for J/psi rapidity 0.75<|y|<1.5 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0). The spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses, plus the range of non-prompt cross-sections within lambda_theta = +/-0.1. The first uncertainty is statistical, the second uncertainty is systematic, the third number is the uncertainty due to spin-alignment.

Non-prompt to inclusive production cross-section fraction fB as a function of J/psi pT for J/psi rapidity 1.5<|y|<2 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0). The spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses, plus the range of non-prompt cross-sections within lambda_theta = +/-0.1. The first uncertainty is statistical, the second uncertainty is systematic, the third number is the uncertainty due to spin-alignment.

Non-prompt to inclusive production cross-section fraction fB as a function of J/psi pT for J/psi rapidity 2<|y|<2.4 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0). The spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses, plus the range of non-prompt cross-sections within lambda_theta =+/-0.1. The first uncertainty is statistical, the second uncertainty is systematic, the third number is the uncertainty due to spin-alignment.

Non-prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity |y|<0.75 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0), and the spin-alignment envelope spans the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic. Comparison is made to FONLL predictions.

Non-prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 0.75<|y|<1.5 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0), and the spin-alignment envelope spans the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic. Comparison is made to FONLL predictions.

Non-prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 1.5<|y|<2 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0), and the spin-alignment envelope spans the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic. Comparison is made to FONLL predictions.

Non-prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 2<|y|<2.4 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0), and the spin-alignment envelope spans the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic. Comparison is made to FONLL predictions.

Prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity |y|<0.75. The central value assumes unpolarised (lambda_theta = 0) prompt and non-prompt production, and the spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses. The first quoted uncertainty is statistical, the second uncertainty is systematic. Comparison is made to the Colour Evaporation Model prediction.

Prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 0.75<|y|<1.5. The central value assumes unpolarised (lambda_theta = 0) prompt and non-prompt production, and the spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses. The first quoted uncertainty is statistical, the second uncertainty is systematic. Comparison is made to the Colour Evaporation Model prediction.

Prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 1.5<|y|<2. The central value assumes unpolarised (lambda_theta = 0) prompt and non-prompt production, and the spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses. The first quoted uncertainty is statistical, the second uncertainty is systematic. Comparison is made to the Colour Evaporation Model prediction.

Prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 2<|y|<2.4. The central value assumes unpolarised (lambda_theta = 0) prompt and non-prompt production, and the spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses. The first quoted uncertainty is statistical, the second uncertainty is systematic. Comparison is made to the Colour Evaporation Model prediction.

Unweighted J/psi candidate yields in bins of $J/psi transverse momentum and rapidity. Uncertainties are statistical only.

Summary table of all sources of considered systematic uncertainty and statistical uncertainty (as a percentage) on the corrected inclusive J/psi production cross-section, for absolute J/psi rapidities within 2<|y|<2.4. The sources of systematic error shown are, in order, Acceptance, Muon recognition, Trigger, Fitting and the Total systematics. Also shown in the last error is the possible envelope of variation the central result due to uncertainty on spin-alignment of the J\psi.

Summary table of all sources of considered systematic uncertainty and statistical uncertainty (as a percentage) on the corrected inclusive J/psi production cross-section, for absolute J/psi rapidities within 1.5<|y|<2. The sources of systematic error shown are, in order, Acceptance, Muon recognition, Trigger, Fitting and the Total systematics. Also shown in the last error is the possible envelope of variation the central result due to uncertainty on spin-alignment of the J/psi.

Summary table of all sources of considered systematic uncertainty and statistical uncertainty (as a percentage) on the corrected inclusive J/psi production cross-section, for absolute J/psi rapidities within 0.75<|y|<1.5. The sources of systematic error shown are, in order, Acceptance, Muon recognition, Trigger, Fitting and the Total systematics. Also shown in the last error is the possible envelope of variation the central result due to uncertainty on spin-alignment of the J/psi.

Summary table of all sources of considered systematic uncertainty and statistical uncertainty (as a percentage) on the corrected inclusive J/psi production cross-section, for absolute rapidities within |y|<0.75. The sources of systematic error shown are, in order, Acceptance, Muon recognition, Trigger, Fitting and the Total systematics. Also shown in the last error is the possible envelope of variation the central result due to uncertainty on spin-alignment of the J/psi.

Breakdown of sources of systematic uncertainty on the non-prompt J/psi fraction measurements, for the bin |y|<0.75, as a function of the J/psi pT.

Breakdown of sources of systematic uncertainty on the non-prompt J/psi fraction measurements, for the bin 0.75<|y|<1.5, as a function of the J/psi pT.

Breakdown of sources of systematic uncertainty on the non-prompt J/psi fraction measurements, for the bin 1.75<|y|<2.0, as a function of the J/psi pT.

Breakdown of sources of systematic uncertainty on the non-prompt J/psi fraction measurements, for the bin 2.0<|y|<2.4, as a function of the J/psi pT.

The observed 95% CL upper limits on the cross section for p p --> zprime x BR(zprime -> e-mu) as a function of the zprime mass.

The dimuon yield from Z0 decays per unit rapidity and per unit minumum bias event as a function of centrality, and the nuclear modificationfactor RAA derived by using a POWHEG proton-proton reference.

The measured cross section ratio for W+jets in the muon channel as a function of corrected jet multiplicity.

The cross section times branching ratio for W+jets in the electron channel as a function of the leading jet PT.

The cross section times branching ratio for W+jets in the muon channel as a function of the leading jet PT.

The cross section times branching ratio for W+jets in the electron channel as a function of the next-to-leading jet PT.

The cross section times branching ratio for W+jets in the muon channel as a function of the next-to-leading jet PT.

UPSI(3S) differential cross sections for |y| < 2.

UPSI(1S) differential cross sections for |y| < 1.

UPSI(2S) differential cross sections for |y| < 1.

UPSI(3S) differential cross sections for |y| < 1.

UPSI(1S) differential cross sections for 1 < |y| < 2.

UPSI(2S) differential cross sections for 1 < |y| < 2.

UPSI(3S) differential cross sections for 1 < |y| < 2.

UPSI(1S) differential cross sections as a function of rapidity.

Ratio of upsilon cross sectis.on.

UPSI differential cross sections for |y| < 2.

UPSI differential cross sections for |y| < 1.

UPSI differential cross sections for 1< |y| < 2.

Differential inclusive cross J/PSI section for the |rapidity| range 1.6 to 2.4 for each prompt J/PSI polarization scenario considered.

Measured fractions of J/PSI mesons from B hadrons corrected for the prompt and non-prompt acceptances.

Measured fractions of J/PSI mesons from B hadrons corrected for the prompt and non-prompt acceptances.

Measured fractions of J/PSI mesons from B hadrons corrected for the prompt and non-prompt acceptances.

Differential prompt J/PSI cross section for the |rapidity| range 0 to 1.2 for each prompt J/PSI polarization scenario considered.

Differential prompt J/PSI cross section for the |rapidity| range 1.2 to 1.6 for each prompt J/PSI polarization scenario considered.

Differential prompt J/PSI cross section for the |rapidity| range 1.6 to 2.4 for each prompt J/PSI polarization scenario considered.

Differential non-prompt J/PSI cross section for the |rapidity| range 0 to 1.2.

Differential non-prompt J/PSI cross section for the |rapidity| range 1.2 to 1.6.

Differential non-prompt J/PSI cross section for the |rapidity| range 1.6 to 2.4.

Measured fiducial cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> e+e- final state.

Measured fiducial cross section times leptonic branching ratio for W+ production in the W+ -> mu+ nu final state.

Measured fiducial cross section times leptonic branching ratio for W- production in the W- -> mu- nubar final state.

Measured fiducial cross section times leptonic branching ratio for W+/- production in the combined W+ -> mu+ nu and W- -> mu- nubar final state.

Measured fiducial cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> mu+ mu- final state.

Measured total cross section times leptonic branching ratio for W+ production in the W+ -> e+ nu final state.

Measured total cross section times leptonic branching ratio for W- production in the W- -> e- nubar final state.

Measured total cross section times leptonic branching ratio for W+/- production in the combined W+ -> e+ nu and W- -> e- nubar final state.

Measured total cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> e+ e- final state.

Measured total cross section times leptonic branching ratio for W+ production in the W+ -> mu+ nu final state.

Measured total cross section times leptonic branching ratio for W- production in the W- -> mu- nubar final state.

Measured total cross section times leptonic branching ratio for W+/- production in the combined W+ -> mu+ nu and W- -> mu- nubar final state.

Measured total cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> mu+ mu- final state.

Measured total cross section times leptonic branching ratio for W+ production in the W+ -> l+ nu (l = e, mu) final states.

Measured total cross section times leptonic branching ratio for W- production in the W- -> l- nubar (l = e, mu) final states.

Measured total cross section times leptonic branching ratio for W+/- production in the combined W+ -> l+ nu and W- -> l- nubar (l = e, mu) final states.

Measured total cross section times leptonic branching ratio for Z/gamma* production in the combined Z/gamma* -> l+ l- (l = e, mu) final states.

Measured total cross-section ratio R_{W+/Z} = sigma (W+ -> e+ nu) / sigma (Z/gamma^* -> e+ e-).

Measured total cross-section ratio R_{W-/Z} = sigma (W- -> e- nubar) / sigma (Z/gamma^* -> e+ e-).

Measured total cross-section ratio R_{W+-/Z} = sigma (W+/- -> e+/- nu/nubar) / sigma (Z/gamma^* -> e+ e-).

Measured total cross-section ratio R_{W+/Z} = sigma (W+ -> mu+ nu) / sigma (Z/gamma^* -> mu+ mu-).

Measured total cross-section ratio R_{W-/Z} = sigma (W- -> mu- nubar) / sigma (Z/gamma^* -> mu+ mu-).

Measured total cross-section ratio R_{W+-/Z} = sigma (W+/- -> mu+/- nu/nubar) / sigma (Z/gamma^* -> mu+ mu-).

Measured total cross-section ratio R_{W+/Z} = sigma (W+ -> l+ nu) / sigma (Z/gamma^* -> l+ l-) where (l = e, mu).

Measured total cross-section ratio R_{W-/Z} = sigma (W- -> l- nubar) / sigma (Z/gamma^* -> l+ l-) where (l = e, mu).

Measured total cross-section ratio R_{W+-/Z} = sigma (W+/- -> l+/- nu/nubar) / sigma (Z/gamma^* -> l+ l-) where (l = e, mu).

Measured lepton asymmetry from W+ -> e+ nu and W- -> e- nubar, binned as a function pseudorapidity.

Measured lepton asymmetry from W+ -> e+ nu and W- -> e- nubar.

Measured lepton asymmetry from W+ -> mu+ nu and W- -> mu- nubar, binned as a function pseudorapidity.

Measured lepton asymmetry from W+ -> mu+ nu and W- -> mu- nubar.

Measured lepton asymmetry from W+ -> l+ nu and W- -> l- nubar (l = e, mu), binned as a function pseudorapidity.

Measured lepton asymmetry from W+ -> l+ nu and W- -> l- nubar (l = e, mu).

The COLLINS asymmetry for negatively charged hadrons as a function of X.

The COLLINS asymmetry for negatively charged hadrons as a function of Z.

The COLLINS asymmetry for negatively charged hadrons as a function of PT.

The SIVERS asymmetry for positively charged hadrons as a function of X.

The SIVERS asymmetry for positively charged hadrons as a function of Z.

The SIVERS asymmetry for positively charged hadrons as a function of PT.

The SIVERS asymmetry for negatively charged hadrons as a function of X.

The SIVERS asymmetry for negatively charged hadrons as a function of Z.

The SIVERS asymmetry for negatively charged hadrons as a function of PT.

The COLLINS asymmetry for positively charged hadrons as a function of Z for X > 0.05.

The COLLINS asymmetry for positively charged hadrons as a function of PT for X > 0.05.

The COLLINS asymmetry for negatively charged hadrons as a function of Z for X > 0.05.

The COLLINS asymmetry for negatively charged hadrons as a function of PT for X > 0.05.

The SIVERS asymmetry for positively charged hadrons as a function of Z for X > 0.032.

The SIVERS asymmetry for positively charged hadrons as a function of PT for X > 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of Z for X > 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of PT for X > 0.032.

The COLLINS asymmetry for positively charged hadrons as a function of W for X > 0.032.

The COLLINS asymmetry for negatively charged hadrons as a function of W for X > 0.032.

The SIVERS asymmetry for positively charged hadrons as a function of W for X > 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of W for X > 0.032.

The COLLINS asymmetry for positively charged hadrons as a function of W for X < 0.032.

The COLLINS asymmetry for negatively charged hadrons as a function of W for X < 0.032.

The SIVERS asymmetry for positively charged hadrons as a function of W for X < 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of W for X < 0.032.

The COLLINS asymmetry for positively charged hadrons as a function of X for W > 7.5 GeV.

The COLLINS asymmetry for negatively charged hadrons as a function of X for W > 7.5 GeV.

The SIVERS asymmetry for positively charged hadrons as a function of X for W > 7.5 GeV.

The SIVERS asymmetry for negatively charged hadrons as a function of X for W > 7.5 GeV.

The COLLINS asymmetry for positively charged hadrons as a function of X for W < 7.5 GeV.

The COLLINS asymmetry for negatively charged hadrons as a function of X for W < 7.5 GeV.

The SIVERS asymmetry for positively charged hadrons as a function of X for W < 7.5 GeV.

The SIVERS asymmetry for negatively charged hadrons as a function of X for W < 7.5 GeV.

The measured strange quark helicity distribution as a funxtion of X.

The XL dependence of the spin transfer from muons to the LAMBDABAR hyperon.

The X dependence of the spin transfer from muons to the LAMBDABAR hyperon.

The Collins and Sivers asymmetry as a function of X for 'ALL' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'ALL' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'ALL' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'ALL' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'ALL' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'ALL' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'ALL' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'ALL' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'ALL' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'ALL' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'ALL' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'ALL' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' positive pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' positivepions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' positive pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' negativepions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' positivekaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' negativekaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' neutral kaons from the 2002-2004 data.. Errors are statistical only.

Mean PT^2 values at forward rapidities (absolute value of y belongs to [1.2;2.2]), for different bins of centrality.

J/PSI invariant yield versus rapidity for 0-20%, 20-40%, 40-60%, 60-92% centrality, at mid rapidity :,-0.35<y<0.35 An up/down correction, to translate each point at the center of it's relative bin, have been applied to the data.

J/PSI invariant yield versus rapidity for 0-20%, 20-40%, 40-60%, 60-92% centrality,at forward rapidities (absolute value of y belongs to [1.2;2.2]). An up/down correction, to translate each point at the center of it's relative bin, have been applied to the data.

Nuclear modification factor Raa versus transverse momentum for 0-20%, 20-40%, 40-60%, 60-92% centrality, at mid rapidities :-0.35<y<0.35. An additional +- 10% (resp. +- 10%, +- 13%, +- 28%) global uncertainty, associated with the calculation of the number of binary collisions and the J/PSI yield in p+p, is not shown for the 0-20% (resp. 20-40%,40-60%, 60-92%) centrality bin.

Nuclear modification factor Raa versus transverse momentum for 0-20%, 20-40%, 40-60%, 60-92% centrality, at forward rapidities : absolute value of y belongs to [1.2;2.2] An additional +- 10% (resp. +- 10%, +- 13%, +- 28%) global uncertainty, associated with the calculation of the number of binary collisions and the J/PSI yield in p+p, is not shown for the 0-20% (resp. 20-40%,40-60%, 60-92%) centrality bin. An up/down correction, to translate each point at the center of it's relative bin, have been applied to the data.

Nuclear modification factor Raa versus rapidity for 0-20%, 20-40%, 40-60%, 60-92% centrality, at mid rapidities :,-0.35<y<0.35. An additional +- 10% (resp. +- 10%, +- 13%, +- 28%) global uncertainty, associated with the calculation of the number of binary collisions and the J/PSI yield in p+p, is not shown for the 0-20% (resp. 20-40%,40-60%, 60-92%) centrality bin.

Nuclear modification factor Raa versus rapidity for 0-20%, 20-40%, 40-60%, 60-92% centrality, at forward rapidities : absolute value of y belongs to [1.2;2.2] An additional +- 10% (resp. +- 10%, +- 13%, +- 28%) global uncertainty, associated with the calculation of the number of binary collisions and the J/PSI yield in p+p, is not shown for the 0-20% (resp. 20-40%,40-60%, 60-92%) centrality bin.

The number of participants Npart and the nuclear modification factor Raa versus centrality at mid rapidities :,-0.35<y<0.35. An additional +- 12% global uncertainty, associated with the calculation of the number of binary collisions and the J/PSI yield in p+p, is not shown.

The number of participants Npart and the nuclear modification factor Raa versus centrality at forward rapidities : absolute value of y belongs to [1.2;2.2] An additional +- 7% global uncertainty, associated with the calculation of the number of binary collisions and the J/PSI yield in p+p, is not shown.

Ratio of nuclear modification factors RAA(forward rapidity)/RAA(mid rapidity), versus centrality. For the two most central bins, mid rapidity points have been combined to form the ratio with the forward rapidity points. See previous tables. An additional globaluncertainty of +- 14% is not included.