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.

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 double-differential cross sections for prompt J/PSI production (assuming no polarisation) and production of J/PSI from b-hadron decays as a function of transverse momentum for the rapidity range 2.5-3.0. Also shown in the final column is the fraction (in %) of J/PSIs from the latter.

The double-differential cross sections for prompt J/PSI production (assuming no polarisation) and production of J/PSI from b-hadron decays as a function of transverse momentum for the rapidity range 3.0-3.5. Also shown in the final column is the fraction (in %) of J/PSIs from the latter.

The double-differential cross sections for prompt J/PSI production (assuming no polarisation) and production of J/PSI from b-hadron decays as a function of transverse momentum for the rapidity range 3.5-4.0. Also shown in the final column is the fraction (in %) of J/PSIs from the latter.

The double-differential cross sections for prompt J/PSI production (assuming no polarisation) and production of J/PSI from b-hadron decays as a function of transverse momentum for the rapidity range 4.0-4.5. Also shown in the final column is the fraction (in %) of J/PSIs from the latter.

The total integrated cross sections for UPSILON 1S 2S and 3S times their dimuon branching ratio in the rapidity range 2.0-4.5 and transverse momentum 0-15 GeV/c.

Differential production cross section for UPSILON 1S 2s and 3S mesons times their dimuon branching fraction as a function of transverse momentum ;.

Differential production cross section for UPSILON 1S 2s and 3S mesons times their dimuon branching fraction as a function of rapidity ;.

The double-differential cross section (times the dimuon decay probability) for the production of UPSILON 1S, 2S and 3S mesons as a function of their transverse momentum for the rapidity range 2.0-2.5, assuming no polarisation.

The double-differential cross section (times the dimuon decay probability) for the production of UPSILON 1S, 2S and 3S mesons as a function of their transverse momentum for the rapidity range 2.5-3.0, assuming no polarisation.

The double-differential cross section (times the dimuon decay probability) for the production of UPSILON 1S, 2S and 3S mesons as a function of their transverse momentum for the rapidity range 3.0-3.5, assuming no polarisation.

The double-differential cross section (times the dimuon decay probability) for the production of UPSILON 1S, 2S and 3S mesons as a function of their transverse momentum for the rapidity range 3.5-4.0, assuming no polarisation.

The double-differential cross section (times the dimuon decay probability) for the production of UPSILON 1S, 2S and 3S mesons as a function of their transverse momentum for the rapidity range 4.0-4.5, assuming no polarisation.

Ratios of the cross-sections for UPSILON(2S)->MU+MU- and UPSILON(3S)->MU+MU- with respect toe UPSILON(1S)->MU+MU- as a function of PT in the rapidity range 2.0-4.0 ;.

Ratios of the cross-sections for UPSILON(2S)->MU+MU- and UPSILON(3S)->MU+MU- with respect to UPSILON(1S)->MU+MU- as a function of rapidity in the rapidity range 2.0-4.0 ;.

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].

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.