Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and a $\tilde{\chi}_1^\pm$ that decays to $W^\pm\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction to $q_i\bar{q}_j W\pm\tilde{\chi}_1^0$.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to bottom quarks ($\tilde{g}\to b\bar{b}\tilde{\chi}_1^0$). Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to top quarks ($\tilde{g}\to t\bar{t}\tilde{\chi}_1^0$). Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for light-flavor squark pair production, where the squarks decay to $q\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay and 1-fold degeneracy in the light-flavor squarks (corresponding to the inner set of curves in the limit plot). To get the theory cross section for other N-fold degeneracy assumptions (e.g. 8-fold for the outer curves in the limit plot), just multiply by N.

Exclusion limits at 95% CL for bottom squark pair production, where the squarks decay to $b\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for top squark pair production, where the squarks decay to $t\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for top squark pair production, where the squarks decay to $b\tilde{\chi}_1^\pm$ and the $\tilde{\chi}_1^0$ decay to $W^\pm\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for top squark pair production, where the squarks decay either to $b\tilde{\chi}_1^\pm\to bW^\pm\tilde{\chi}_1^0$ or to $t\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for top squark pair production, where the squarks decay to $c\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for the mono-$\phi$ model, in which a resonantly-produced colored scalar decays to a massive Dirac fermion and a quark. Signal cross sections are calculated at leading order in $\alpha_S$, assuming unity branching fraction for the given decay.

Cross section limits for $\mathrm{LQ}\to\mathrm{q}\nu$, where $q=u,\,d,\,s,\,\mathrm{or}\,c$. Limits are at the 95% confidence level. Theory cross sections are LO for vector LQ, and NLO for scalar LQ. Branching ratio is assumed to be 100% to $\mathrm{q}\nu$.

Cross section limits for $\mathrm{LQ}\to\mathrm{b}\nu$. Limits are at the 95% confidence level. Theory cross sections are LO for vector LQ, and NLO for scalar LQ. Branching ratio is assumed to be 100% to $\mathrm{b}\nu$.

Cross section limits for $\mathrm{LQ}\to\mathrm{t}\nu$. Limits are at the 95% confidence level. Theory cross sections are LO for vector LQ, and NLO for scalar LQ. Branching ratios are assumed to be $\mathcal{B}(\mathrm{LQ}\to\mathrm{t}\nu)=1-\beta$, and $\mathcal{B}(\mathrm{LQ}\to\mathrm{b}\tau)=\beta$.

Predictions and observations for monojet signal regions

Predictions and observations for signal regions with $250 \leq H_\mathrm{T} < 450$ GeV

Predictions and observations for signal regions with $450 \leq H_\mathrm{T} < 575$ GeV and $N_\mathrm{j}<7$

Predictions and observations for signal regions with $450 \leq H_\mathrm{T} < 575$ GeV and $N_\mathrm{j}\geq7$

Predictions and observations for signal regions with $575 \leq H_\mathrm{T} < 1200$ GeV and $N_\mathrm{j}^\mathrm{hi}<4$

Predictions and observations for signal regions with $575 \leq H_\mathrm{T} < 1200$ GeV and $4\leq N_\mathrm{j}^\mathrm{hi}<7$

Predictions and observations for signal regions with $575 \leq H_\mathrm{T} < 1200$ GeV and $N_\mathrm{j}\geq7$

Predictions and observations for signal regions with $1200 \leq H_\mathrm{T} < 1500$ GeV and $N_\mathrm{j}^\mathrm{hi}<4$

Predictions and observations for signal regions with $1200 \leq H_\mathrm{T} < 1500$ GeV and $4\leq N_\mathrm{j}^\mathrm{hi}<7$

Predictions and observations for signal regions with $1200 \leq H_\mathrm{T} < 1500$ GeV and $N_\mathrm{j}\geq7$

Predictions and observations for signal regions with $H_\mathrm{T} \geq 1500$ GeV and $N_\mathrm{j}<7$

Predictions and observations for signal regions with $H_\mathrm{T} \geq 1500$ GeV and $N_\mathrm{j}\geq7$

Covariance matrix for the 282 signal regions of the inclusive $M_\mathrm{T2}$ search

Correlation matrix for the 282 signal regions of the inclusive $M_\mathrm{T2}$ search

Bin number definitions for the $M_\mathrm{T2}$ covariance and correlation matrices

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 10$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 50$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 200$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct light squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 10$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, for a single light squark.

Exclusion limits at 95% CL for direct light squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 50$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, for a single light squark.

Exclusion limits at 95% CL for direct light squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 200$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, for a single light squark.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino is long-lived with $c\tau_0 = 10$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino is long-lived with $c\tau_0 = 50$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino is long-lived with $c\tau_0 = 200$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

The maximum chargino mass excluded at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 1$ to 2000 cm while the gluino mass is fixed to 1900 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$. If all kinematically allowed chargino masses are excluded, the curves, including 68 and 95% expected, tend to overlap. At short decay lengths, horizontal exclusion lines are obtained from the inclusive analysis, as this is not affected by track reconstruction inefficiencies, which may arise when the chargino decays before the CMS tracker, and therefore shows better sensitivity to scenarios with very small lifetime compared to the disappearing track search, based on median expected limits.

The maximum chargino mass excluded at 95% CL for direct squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 1$ to 2000 cm while the squark mass is fixed to 900 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, for a single light squark. If all kinematically allowed chargino masses are excluded, the curves, including 68 and 95% expected, tend to overlap. At short decay lengths, horizontal exclusion lines are obtained from the inclusive analysis, as this is not affected by track reconstruction inefficiencies, which may arise when the chargino decays before the CMS tracker, and therefore shows better sensitivity to scenarios with very small lifetime compared to the disappearing track search, based on median expected limits.

The maximum chargino mass excluded at 95% CL for direct squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 1$ to 2000 cm while the squark mass is fixed to 1500 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, and the eight light squarks' masses are assumed to be degenerate. If all kinematically allowed chargino masses are excluded, the curves, including 68 and 95% expected, tend to overlap. At short decay lengths, horizontal exclusion lines are obtained from the inclusive analysis, as this is not affected by track reconstruction inefficiencies, which may arise when the chargino decays before the CMS tracker, and therefore shows better sensitivity to scenarios with very small lifetime compared to the disappearing track search, based on median expected limits.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 1$ to 2000 cm while the stop mass is fixed to 1000 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$. If all kinematically allowed chargino masses are excluded, the curves, including 68 and 95% expected, tend to overlap. At short decay lengths, horizontal exclusion lines are obtained from the inclusive analysis, as this is not affected by track reconstruction inefficiencies, which may arise when the chargino decays before the CMS tracker, and therefore shows better sensitivity to scenarios with very small lifetime compared to the disappearing track search, based on median expected limits.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 5$ to 1000 cm while the gluino mass is fixed to 1600 GeV and the neutralino's mass is fixed to 1575 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 5$ to 1000 cm while the squark mass is fixed to 2000 GeV and the neutralino's mass is fixed to 1000 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, and the eight light squarks' masses are assumed to be degenerate.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 5$ to 1000 cm while the stop mass is fixed to 1100 GeV and the neutralino's mass is fixed to 1000 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Predictions and observations for 2016 disappearing track signal regions

Predictions and observations for 2017-2018 pixel track signal regions

Predictions and observations for 2017-2018 medium (M) and long (L) length track signal regions

Covariance matrix for the 68 signal regions of the disappearing tracks $M_\mathrm{T2}$ search

Correlation matrix for the 68 signal regions of the disappearing tracks $M_\mathrm{T2}$ search

Upper limits at 95% CL on the cross section times branching fraction for the process $H \to 2\gamma_d + X$ with $m_H$ = 800 GeV in the hadron-hadron final state.

Upper limits at 95% CL on the cross section times branching fraction for the process $H \to 2\gamma_d + X$ with $m_H$ = 800 GeV in the muon-hadron final state.

Upper limits at 95% CL on the cross section times branching fraction for the process $H \to 4\gamma_d + X$ with $m_H$ = 800 GeV in the muon-muon final state.

Upper limits at 95% CL on the cross section times branching fraction for the process $H \to 4\gamma_d + X$ with $m_H$ = 800 GeV in the muon-hadron final state.

Upper limits at 95% CL on the cross section times branching fraction for the process $H \to 4\gamma_d + X$ with $m_H$ = 800 GeV in the hadron-hadron final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 4\gamma_d + X$ process with $m_H$ = 125 GeV in the muon-muon final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 2\gamma_d + X$ process with $m_H$ = 125 GeV in the muon-muon final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 2\gamma_d + X$ process with $m_H$ = 800 GeV in the muon-muon final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 4\gamma_d + X$ process with $m_H$ = 800 GeV in the muon-muon final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 4\gamma_d + X$ process with $m_H$ = 125 GeV in the muon-hadron final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 2\gamma_d + X$ process with $m_H$ = 125 GeV in the muon-hadron final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 2\gamma_d + X$ process with $m_H$ = 800 GeV in the muon-hadron final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 4\gamma_d + X$ process with $m_H$ = 800 GeV in the muon-hadron final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 2\gamma_d + X$ process with $m_H$ = 125 GeV in the hadron-hadron final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 2\gamma_d + X$ process with $m_H$ = 800 GeV in the hadron-hadron final state.

Extrapolated signal efficiencies as a function of proper decay length of the dark photon for the $H \to 4\gamma_d + X$ process with $m_H$ = 800 GeV in the hadron-hadron final state.

Excitation function at pion c.m. angle THETA=49 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=57 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=63 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=69 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=75 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at THETA=81 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=87 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=93 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=99 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=104 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=110 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=117 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=123 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=130 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=138 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=148 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Excitation function at pion c.m. angle THETA=162 deg as function of incident photon energy E. The uncertainties are statistical and systematic, combined in quadrature.

Total cross section as a function of incident photon energy E.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ average transverse momentum vs multiplicity - SPDtracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ average transverse momentum vs multiplicity - SPDtracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ average transverse momentum vs multiplicity - SPDtracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ average transverse momentum vs multiplicity - SPDtracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ average transverse momentum vs multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ average transverse momentum vs multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ average transverse momentum vs multiplicity - SPDtracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ average transverse momentum vs multiplicity - SPDtracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ average transverse momentum vs multiplicity - SPDtracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ average transverse momentum vs multiplicity - SPDtracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ average transverse momentum vs multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ average transverse momentum vs multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ self-normalized yields vs self-normalized multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ self-normalized yields vs self-normalized multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ self-normalized yields vs self-normalized multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ self-normalized yields vs self-normalized multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets0815 multiplicity classes

$K^{0}_{S}$ transverse momentum spectra ratios SPDTracklets-to-V0M

$K^{0}_{S}$ transverse momentum spectra ratios SPDTracklets-to-V0M

$\Lambda+\bar{\Lambda}$ transverse momentum spectra ratios SPDTracklets-to-V0M

$\Lambda+\bar{\Lambda}$ transverse momentum spectra ratios SPDTracklets-to-V0M

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectra ratios SPDTracklets-to-V0M

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectra ratios SPDTracklets-to-V0M

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields vs multiplicity - SPDtracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields vs multiplicity - SPDtracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields vs multiplicity - SPDtracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields vs multiplicity - SPDtracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields vs multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields vs multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$, $K^{0}_{S}$ integrated yields vs multiplicity - SPDtracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$, $K^{0}_{S}$ integrated yields vs multiplicity - SPDtracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$, $K^{0}_{S}$ integrated yields vs multiplicity - SPDtracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$, $K^{0}_{S}$ integrated yields vs multiplicity - SPDtracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$, $K^{0}_{S}$ integrated yields vs multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$, $K^{0}_{S}$ integrated yields vs multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields (no extr.) vs multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields (no extr.) vs multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ integrated yields (no extr.) vs multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ integrated yields (no extr.) vs multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$, $\Omega^{-}+\bar{\Omega^{+}}$ integrated yields - INEL>0. V0M multiplicity dependent yields are already listed in Table 8c.

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$, $\Omega^{-}+\bar{\Omega^{+}}$ integrated yields - INEL>0. V0M multiplicity dependent yields are already listed in Table 8c.

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$, $\Omega^{-}+\bar{\Omega^{+}}$ integrated yields - INEL>0. V0M multiplicity dependent yields at 7 TeV are listed in the corresponding repository ("https://www.hepdata.net/record/77284").

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$, $\Omega^{-}+\bar{\Omega^{+}}$ integrated yields - INEL>0. V0M multiplicity dependent yields at 7 TeV are listed in the corresponding repository ("https://www.hepdata.net/record/77284").

$\Lambda+\bar{\Lambda}/K^{0}_{S}$, $\Xi^{-}+\bar{\Xi^{+}}/K^{0}_{S}$ - Tracklets08 multiplicity classes

$\Lambda+\bar{\Lambda}/K^{0}_{S}$, $\Xi^{-}+\bar{\Xi^{+}}/K^{0}_{S}$ - Tracklets08 multiplicity classes

$\Lambda+\bar{\Lambda}/K^{0}_{S}$, $\Xi^{-}+\bar{\Xi^{+}}/K^{0}_{S}$ - Tracklets0815 multiplicity classes

$\Lambda+\bar{\Lambda}/K^{0}_{S}$, $\Xi^{-}+\bar{\Xi^{+}}/K^{0}_{S}$ - Tracklets0815 multiplicity classes

$\Lambda+\bar{\Lambda}/K^{0}_{S}$, $\Xi^{-}+\bar{\Xi^{+}}/K^{0}_{S}$ - V0M multiplicity classes

$\Lambda+\bar{\Lambda}/K^{0}_{S}$, $\Xi^{-}+\bar{\Xi^{+}}/K^{0}_{S}$ - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}/K^{0}_{S}$ - Tracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}/K^{0}_{S}$ - Tracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}/K^{0}_{S}$ - Tracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}/K^{0}_{S}$ - Tracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}/K^{0}_{S}$ - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}/K^{0}_{S}$ - V0M multiplicity classes

$\Lambda+\bar{\Lambda}/2*$K^{0}_{S}$ transverse momentum spectrum - V0M multiplicity classes

$\Lambda+\bar{\Lambda}/2*$K^{0}_{S}$ transverse momentum spectrum $\it{N}_{tracklets}^{|\it{\eta}|<0.8}$ - multiplicity classes

$\Lambda+\bar{\Lambda}/2*$K^{0}_{S}$ transverse momentum spectrum $\it{N}_{tracklets}^{0.8<|\it{\eta}|<1.5}$ - multiplicity classes

Dependence of the overall signal efficiency on the pT of the long-lived Z' for Z' -> ee. The error bars indicate the total uncertainties.

Dependence of the overall signal efficiency on the transverse decay radius Rxy of the long-lived Z' for Z' -> emu. The error bars indicate the total uncertainties.

Dependence of the overall signal efficiency on the pT of the long-lived Z' for Z' -> emu. The error bars indicate the total uncertainties.

Dependence of the overall signal efficiency on the transverse decay radius Rxy of the long-lived Z' for Z' -> mumu. The error bars indicate the total uncertainties.

Dependence of the overall signal efficiency on the pT of the long-lived Z' for Z' -> mumu. The error bars indicate the total uncertainties.

Overall signal efficiency as a function of the mean proper lifetime (ctau) of the neutralino for the lambda121 scenario of the RPV SUSY model. The error bars indicate the total uncertainties.

Overall signal efficiency as a function of the mean proper lifetime (ctau) of the neutralino for the lambda122 scenario of the RPV SUSY model. The error bars indicate the total uncertainties.

95% CL upper limits on the squark-antisquark production cross-section as a function of the mean proper lifetime (ctau) of the neutralino for the lambda121 scenario of the RPV SUSY model and a 700 GeV squark. The uncertainties of the expected limit indicate the +-1sigma variations.

95% CL upper limits on the squark-antisquark production cross-section as a function of the mean proper lifetime (ctau) of the neutralino for the lambda122 scenario of the RPV SUSY model and a 700 GeV squark. The uncertainties of the expected limit indicate the +-1sigma variations.

95% CL upper limits on the squark-antisquark production cross-section as a function of the mean proper lifetime (ctau) of the neutralino for the lambda121 scenario of the RPV SUSY model and a 1600 GeV squark. The uncertainties of the expected limit indicate the +-1sigma variations.

95% CL upper limits on the squark-antisquark production cross-section as a function of the mean proper lifetime (ctau) of the neutralino for the lambda122 scenario of the RPV SUSY model and a 1600 GeV squark. The uncertainties of the expected limit indicate the +-1sigma variations.

Fraction of detector volume covered by the material veto as a function of z and Rxy of the displaced dilepton vertex.

Fraction of detector volume covered by the disabled pixel modules veto veto as a function of z and Rxy of the displaced dilepton vertex.

Observed Rxy distribution of vertices composed of two non-leptonic tracks in a control sample in the data and the predicted distribution obtained from the event mixing. The error bars indicate the statistical uncertainties.

Rxy distributions of Kshort vertices from the large radius tracking in the data and background MC samples. Data has been normalised such that the total number of Kshort from the standard tracking in the data agrees with the total number of Kshort from the standard tracking in the MC. The error bars indicate the statistical uncertainties.

Acceptance per decay as a function of the mean proper lifetime (ctau) of the neutralino for neutralino -> eenu. The error bars indicate the statistical uncertainties.

Acceptance per decay as a function of the mean proper lifetime (ctau) of the neutralino for neutralino -> emunu. The error bars indicate the statistical uncertainties.

Acceptance per decay as a function of the mean proper lifetime (ctau) of the neutralino for neutralino -> mumunu. The error bars indicate the statistical uncertainties.

Detection efficiency per decay as a function of the mean proper lifetime (ctau) of the neutralino for neutralino -> eenu. The error bars indicate the total uncertainties.

Detection efficiency per decay as a function of the mean proper lifetime (ctau) of the neutralino for neutralino -> emunu. The error bars indicate the total uncertainties.

Detection efficiency per decay as a function of the mean proper lifetime (ctau) of the neutralino for neutralino -> mumunu. The error bars indicate the total uncertainties.

Overall signal efficiency (acceptance times efficiency) per decay as a function of the mean proper lifetime (ctau) of the neutralino for neutralino -> eenu. The error bars indicate the total uncertainties.

Overall signal efficiency (acceptance times efficiency) per decay as a function of the mean proper lifetime (ctau) of the neutralino for neutralino -> emunu. The error bars indicate the total uncertainties.

Overall signal efficiency (acceptance times efficiency) per decay as a function of the mean proper lifetime (ctau) of the neutralino for neutralino -> mumunu. The error bars indicate the total uncertainties.

Detection efficiency per decay for Rxy < 22 mm as a function of the invariant mass and pT of the electron pair in LLP -> eeX.

Detection efficiency per decay for 22 <= Rxy < 38 mm as a function of the invariant mass and pT of the electron pair in LLP -> eeX.

Detection efficiency per decay for 38 <= Rxy < 73 mm as a function of the invariant mass and pT of the electron pair in LLP -> eeX.

Detection efficiency per decay for 73 <= Rxy < 111 mm as a function of the invariant mass and pT of the electron pair in LLP -> eeX.

Detection efficiency per decay for 111 <= Rxy < 145 mm as a function of the invariant mass and pT of the electron pair in LLP -> eeX.

Detection efficiency per decay for 145 <= Rxy < 300 mm as a function of the invariant mass and pT of the electron pair in LLP -> eeX.

Detection efficiency per decay for Rxy < 22 mm as a function of the invariant mass and pT of the electron and muon pair in LLP -> emuX.

Detection efficiency per decay for 22 <= Rxy < 38 mm as a function of the invariant mass and pT of the electron and muon pair in LLP -> emuX.

Detection efficiency per decay for 38 <= Rxy < 73 mm as a function of the invariant mass and pT of the electron and muon pair in LLP -> emuX.

Detection efficiency per decay for 73 <= Rxy < 111 mm as a function of the invariant mass and pT of the electron and muon pair in LLP -> emuX.

Detection efficiency per decay for 111 <= Rxy < 145 mm as a function of the invariant mass and pT of the electron and muon pair in LLP -> emuX.

Detection efficiency per decay for 145 <= Rxy < 300 mm as a function of the invariant mass and pT of the electron and muon pair in LLP -> emuX.

Detection efficiency per decay for Rxy < 22 mm as a function of the invariant mass and pT of the muon pair in LLP -> mumuX.

Detection efficiency per decay for 22 <= Rxy < 38 mm as a function of the invariant mass and pT of the muon pair in LLP -> mumuX.

Detection efficiency per decay for 38 <= Rxy < 73 mm as a function of the invariant mass and pT of the muon pair in LLP -> mumuX.

Detection efficiency per decay for 73 <= Rxy < 111 mm as a function of the invariant mass and pT of the muon pair in LLP -> mumuX.

Detection efficiency per decay for 111 <= Rxy < 145 mm as a function of the invariant mass and pT of the muon pair in LLP -> mumuX.

Detection efficiency per decay for 145 <= Rxy < 300 mm as a function of the invariant mass and pT of the muon pair in LLP -> mumuX.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 100 GeV and LLP -> ee.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 100 GeV and LLP -> emu.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 100 GeV and LLP -> mumu.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 250 GeV and LLP -> ee.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 250 GeV and LLP -> emu.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 250 GeV and LLP -> mumu.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 500 GeV and LLP -> ee.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 500 GeV and LLP -> emu.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 500 GeV and LLP -> mumu.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 750 GeV and LLP -> ee.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 750 GeV and LLP -> emu.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 750 GeV and LLP -> mumu.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 1000 GeV and LLP -> ee.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 1000 GeV and LLP -> emu.

Detection efficiency per decay as a function of the transverse decay radius Rxy and the dilepton pT for a LLP mass of 1000 GeV and LLP -> mumu.

Acceptance, detection efficiency, and overall signal efficiency in the Z' toy model for mZ' = 100 GeV, three mean proper lifetimes (ctau) and the three decay modes of the Z'.

Acceptance, detection efficiency, and overall signal efficiency in the Z' toy model for mZ' = 250 GeV, three mean proper lifetimes (ctau) and the three decay modes of the Z'.

Acceptance, detection efficiency, and overall signal efficiency in the Z' toy model for mZ' = 500 GeV, three mean proper lifetimes (ctau) and the three decay modes of the Z'.

Acceptance, detection efficiency, and overall signal efficiency in the Z' toy model for mZ' = 750 GeV, three mean proper lifetimes (ctau) and the three decay modes of the Z'.

Acceptance, detection efficiency, and overall signal efficiency in the Z' toy model for mZ' = 1000 GeV, three mean proper lifetimes (ctau) and the three decay modes of the Z'.

The double-differential Z + jets production cross-section as a function of |y_{jet}| in the 100 GeV < p_{T}^{jet} < 200 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The double-differential Z + jets production cross-section as a function of |y_{jet}| in the 200 GeV < p_{T}^{jet} < 300 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The double-differential Z + jets production cross-section as a function of |y_{jet}| in the 300 GeV < p_{T}^{jet} < 400 Gev range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The double-differential Z + jets production cross-section as a function of |y_{jet}| in the 400 GeV < p_{T}^{jet} < 1050 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The non-perturbative correction for the Z + jets production cross-section as a function of |y_{jet}| in the 25 GeV < p_{T}^{jet} < 50 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The non-perturbative correction for the Z + jets production cross-section as a function of |y_{jet}| in the 50 GeV < p_{T}^{jet} < 100 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The non-perturbative correction for the Z + jets production cross-section as a function of |y_{jet}| in the 100 GeV < p_{T}^{jet} < 200 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The non-perturbative correction for the Z + jets production cross-section as a function of |y_{jet}| in the 200 GeV < p_{T}^{jet} < 300 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The non-perturbative correction for the Z + jets production cross-section as a function of |y_{jet}| in the 300 GeV < p_{T}^{jet} < 400 Gev range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The non-perturbative correction for the Z + jets production cross-section as a function of |y_{jet}| in the 400 GeV < p_{T}^{jet} < 1050 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The correction for QED radiation effects for the Z + jets production cross-section as a function of |y_{jet}| in the 25 GeV < p_{T}^{jet} < 50 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The correction for QED radiation effects for the Z + jets production cross-section as a function of |y_{jet}| in the 50 GeV < p_{T}^{jet} < 100 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The correction for QED radiation effects for the Z + jets production cross-section as a function of |y_{jet}| in the 100 GeV < p_{T}^{jet} < 200 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The correction for QED radiation effects for the Z + jets production cross-section as a function of |y_{jet}| in the 200 GeV < p_{T}^{jet} < 300 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The correction for QED radiation effects for the Z + jets production cross-section as a function of |y_{jet}| in the 300 GeV < p_{T}^{jet} < 400 Gev range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

The correction for QED radiation effects for the Z + jets production cross-section as a function of |y_{jet}| in the 400 GeV < p_{T}^{jet} < 1050 GeV range. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

Correlation matrix for the bins of the Z + jets cross-section. The particle level phase space definition: - 66 GeV < m_{ee} < 116 GeV - |eta_{electron}| < 2.47 - p_{T}^{electron} > 20 GeV - anti-kt R=0.4 jets N>=1 - |y_{jet}| < 3.4 - p_{T}^{jet} > 25 GeV - Delta R(jet, electron) > 0.4

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 Z/gamma* production in the Z/gamma* -> e+ e- 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+ -> mu+ nu 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- -> mu- nu 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 Z/gamma* production in the Z/gamma* -> mu+ mu- final state.

Combined fiducial cross-section measurements for W+ boson production in the W+ -> l+ nu (l = e, mu) final state.

Combined fiducial cross-section measurements for W- boson production in the W- -> l- nu (l = e, mu) final state.

Combined fiducial cross-section measurements for W boson production in the W -> l nu (l = e, mu) final state.

Combined fiducial cross-section measurements for Z/gamma* production in the Z/gamma* -> l- l+ (l = e, mu) final state.

Combined total cross-section measurements for W+ boson production in the W+ -> l+ nu (l = e, mu) final state.

Combined total cross-section measurements for W- boson production in the W- -> l- nu (l = e, mu) final state.

Combined total cross-section measurements for W boson production in the W -> l nu (l = e, mu) final state.

Combined total cross-section measurements for Z/gamma* production in the Z/gamma* -> l- l+ (l = e, mu) final state.

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

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

Measured charge asymmetry in W-boson production A_{l} = ( sigma (W+ -> l+ nu) - sigma (W- -> l- nubar) ) / ( sigma (W+ -> l+ nu) + sigma (W- -> l- nubar) ) where l = e, mu.

The ratio of measured W+ cross-sections in the electron and muon decay channels R_{W+} = sigma (W+ -> e+ nu) / sigma (W+ -> mu+ nu)

The ratio of measured W- cross-sections in the electron and muon decay channels R_{W-} = sigma (W- -> e- nu) / sigma (W- -> mu- nu)

The ratio of measured W cross-sections in the electron and muon decay channels R_{W} = sigma (W -> e nu) / sigma (W -> mu nu)

The ratio of measured Z/gamma^* cross-sections in the electron and muon decay channels R_{Z/gamma^*} = sigma (Z/gamma^* -> e+ e-) / sigma (Z/gamma^* -> mu+ mu-)

Correlation coefficients among (W- -> l- nubar), (W+ -> l+ nu), (Z/gamma^* -> l+ l-) where (l = e, mu) excluding the common normalisation uncertainty due to the luminosity calibration.

$\langle \zeta \rangle$, central jet.

$\langle p_{T}^{rel} / GeV \rangle$, forward jet.

$\langle p_{T}^{rel} / GeV \rangle$, central jet.

$\langle r \rangle$, forward jet.

$\langle r \rangle$, central jet.

$\langle n_{ch} \rangle$, both jets.

$\langle \zeta \rangle$, combined jet.

$\langle p_{T}^{rel} / GeV \rangle$, both jets.

$\langle r \rangle$, both jets.

$n_{ch}$ , 100 GeV < Jet p_{T} < 200 GeV, both jets.

$n_{ch}$ , 200 GeV < Jet p_{T} < 300 GeV, both jets.

$n_{ch}$ , 300 GeV < Jet p_{T} < 400 GeV, both jets.

$n_{ch}$ , 400 GeV < Jet p_{T} < 500 GeV, both jets.

$n_{ch}$ , 500 GeV < Jet p_{T} < 600 GeV, both jets.

$n_{ch}$ , 600 GeV < Jet p_{T} < 700 GeV, both jets.

$n_{ch}$ , 700 GeV < Jet p_{T} < 800 GeV, both jets.

$n_{ch}$ , 800 GeV < Jet p_{T} < 900 GeV, both jets.

$n_{ch}$ , 900 GeV < Jet p_{T} < 1000 GeV, both jets.

$n_{ch}$ , 1000 GeV < Jet p_{T} < 1200 GeV, both jets.

$n_{ch}$ , 1200 GeV < Jet p_{T} < 1400 GeV, both jets.

$n_{ch}$ , 1400 GeV < Jet p_{T} < 1600 GeV, both jets.

$n_{ch}$ , 1600 GeV < Jet p_{T} < 2000 GeV, both jets.

$n_{ch}$ , 2000 GeV < Jet p_{T} < 2500 GeV, both jets.

$r$ , 100 GeV < Jet p_{T} < 200 GeV, both jets.

$r$ , 200 GeV < Jet p_{T} < 300 GeV, both jets.

$r$ , 300 GeV < Jet p_{T} < 400 GeV, both jets.

$r$ , 400 GeV < Jet p_{T} < 500 GeV, both jets.

$r$ , 500 GeV < Jet p_{T} < 600 GeV, both jets.

$r$ , 600 GeV < Jet p_{T} < 700 GeV, both jets.

$r$ , 700 GeV < Jet p_{T} < 800 GeV, both jets.

$r$ , 800 GeV < Jet p_{T} < 900 GeV, both jets.

$r$ , 900 GeV < Jet p_{T} < 1000 GeV, both jets.

$r$ , 1000 GeV < Jet p_{T} < 1200 GeV, both jets.

$r$ , 1200 GeV < Jet p_{T} < 1400 GeV, both jets.

$r$ , 1400 GeV < Jet p_{T} < 1600 GeV, both jets.

$r$ , 1600 GeV < Jet p_{T} < 2000 GeV, both jets.

$r$ , 2000 GeV < Jet p_{T} < 2500 GeV, both jets.

$\zeta$ , 100 GeV < Jet p_{T} < 200 GeV, both jets.

$\zeta$ , 200 GeV < Jet p_{T} < 300 GeV, both jets.

$\zeta$ , 300 GeV < Jet p_{T} < 400 GeV, both jets.

$\zeta$ , 400 GeV < Jet p_{T} < 500 GeV, both jets.

$\zeta$ , 500 GeV < Jet p_{T} < 600 GeV, both jets.

$\zeta$ , 600 GeV < Jet p_{T} < 700 GeV, both jets.

$\zeta$ , 700 GeV < Jet p_{T} < 800 GeV, both jets.

$\zeta$ , 800 GeV < Jet p_{T} < 900 GeV, both jets.

$\zeta$ , 900 GeV < Jet p_{T} < 1000 GeV, both jets.

$\zeta$ , 1000 GeV < Jet p_{T} < 1200 GeV, both jets.

$\zeta$ , 1200 GeV < Jet p_{T} < 1400 GeV, both jets.

$\zeta$ , 1400 GeV < Jet p_{T} < 1600 GeV, both jets.

$\zeta$ , 1600 GeV < Jet p_{T} < 2000 GeV, both jets.

$\zeta$ , 2000 GeV < Jet p_{T} < 2500 GeV, both jets.

$p_{T}^{rel} / GeV$ , 100 GeV < Jet p_{T} < 200 GeV, both jets.

$p_{T}^{rel} / GeV$ , 200 GeV < Jet p_{T} < 300 GeV, both jets.

$p_{T}^{rel} / GeV$ , 300 GeV < Jet p_{T} < 400 GeV, both jets.

$p_{T}^{rel} / GeV$ , 400 GeV < Jet p_{T} < 500 GeV, both jets.

$p_{T}^{rel} / GeV$ , 500 GeV < Jet p_{T} < 600 GeV, both jets.

$p_{T}^{rel} / GeV$ , 600 GeV < Jet p_{T} < 700 GeV, both jets.

$p_{T}^{rel} / GeV$ , 700 GeV < Jet p_{T} < 800 GeV, both jets.

$p_{T}^{rel} / GeV$ , 800 GeV < Jet p_{T} < 900 GeV, both jets.

$p_{T}^{rel} / GeV$ , 900 GeV < Jet p_{T} < 1000 GeV, both jets.

$p_{T}^{rel} / GeV$ , 1000 GeV < Jet p_{T} < 1200 GeV, both jets.

$p_{T}^{rel} / GeV$ , 1200 GeV < Jet p_{T} < 1400 GeV, both jets.

$p_{T}^{rel} / GeV$ , 1400 GeV < Jet p_{T} < 1600 GeV, both jets.

$p_{T}^{rel} / GeV$ , 1600 GeV < Jet p_{T} < 2000 GeV, both jets.

$p_{T}^{rel} / GeV$ , 2000 GeV < Jet p_{T} < 2500 GeV, both jets.

$n_{ch}$ , 100 GeV < Jet p_{T} < 200 GeV, more forward jet.

$n_{ch}$ , 200 GeV < Jet p_{T} < 300 GeV, more forward jet.

$n_{ch}$ , 300 GeV < Jet p_{T} < 400 GeV, more forward jet.

$n_{ch}$ , 400 GeV < Jet p_{T} < 500 GeV, more forward jet.

$n_{ch}$ , 500 GeV < Jet p_{T} < 600 GeV, more forward jet.

$n_{ch}$ , 600 GeV < Jet p_{T} < 700 GeV, more forward jet.

$n_{ch}$ , 700 GeV < Jet p_{T} < 800 GeV, more forward jet.

$n_{ch}$ , 800 GeV < Jet p_{T} < 900 GeV, more forward jet.

$n_{ch}$ , 900 GeV < Jet p_{T} < 1000 GeV, more forward jet.

$n_{ch}$ , 1000 GeV < Jet p_{T} < 1200 GeV, more forward jet.

$n_{ch}$ , 1200 GeV < Jet p_{T} < 1400 GeV, more forward jet.

$n_{ch}$ , 1400 GeV < Jet p_{T} < 1600 GeV, more forward jet.

$n_{ch}$ , 1600 GeV < Jet p_{T} < 2000 GeV, more forward jet.

$n_{ch}$ , 2000 GeV < Jet p_{T} < 2500 GeV, more forward jet.

$r$ , 100 GeV < Jet p_{T} < 200 GeV, more forward jet.

$r$ , 200 GeV < Jet p_{T} < 300 GeV, more forward jet.

$r$ , 300 GeV < Jet p_{T} < 400 GeV, more forward jet.

$r$ , 400 GeV < Jet p_{T} < 500 GeV, more forward jet.

$r$ , 500 GeV < Jet p_{T} < 600 GeV, more forward jet.

$r$ , 600 GeV < Jet p_{T} < 700 GeV, more forward jet.

$r$ , 700 GeV < Jet p_{T} < 800 GeV, more forward jet.

$r$ , 800 GeV < Jet p_{T} < 900 GeV, more forward jet.

$r$ , 900 GeV < Jet p_{T} < 1000 GeV, more forward jet.

$r$ , 1000 GeV < Jet p_{T} < 1200 GeV, more forward jet.

$r$ , 1200 GeV < Jet p_{T} < 1400 GeV, more forward jet.

$r$ , 1400 GeV < Jet p_{T} < 1600 GeV, more forward jet.

$r$ , 1600 GeV < Jet p_{T} < 2000 GeV, more forward jet.

$r$ , 2000 GeV < Jet p_{T} < 2500 GeV, more forward jet.

$\zeta$ , 100 GeV < Jet p_{T} < 200 GeV, more forward jet.

$\zeta$ , 200 GeV < Jet p_{T} < 300 GeV, more forward jet.

$\zeta$ , 300 GeV < Jet p_{T} < 400 GeV, more forward jet.

$\zeta$ , 400 GeV < Jet p_{T} < 500 GeV, more forward jet.

$\zeta$ , 500 GeV < Jet p_{T} < 600 GeV, more forward jet.

$\zeta$ , 600 GeV < Jet p_{T} < 700 GeV, more forward jet.

$\zeta$ , 700 GeV < Jet p_{T} < 800 GeV, more forward jet.

$\zeta$ , 800 GeV < Jet p_{T} < 900 GeV, more forward jet.

$\zeta$ , 900 GeV < Jet p_{T} < 1000 GeV, more forward jet.

$\zeta$ , 1000 GeV < Jet p_{T} < 1200 GeV, more forward jet.

$\zeta$ , 1200 GeV < Jet p_{T} < 1400 GeV, more forward jet.

$\zeta$ , 1400 GeV < Jet p_{T} < 1600 GeV, more forward jet.

$\zeta$ , 1600 GeV < Jet p_{T} < 2000 GeV, more forward jet.

$\zeta$ , 2000 GeV < Jet p_{T} < 2500 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 100 GeV < Jet p_{T} < 200 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 200 GeV < Jet p_{T} < 300 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 300 GeV < Jet p_{T} < 400 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 400 GeV < Jet p_{T} < 500 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 500 GeV < Jet p_{T} < 600 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 600 GeV < Jet p_{T} < 700 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 700 GeV < Jet p_{T} < 800 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 800 GeV < Jet p_{T} < 900 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 900 GeV < Jet p_{T} < 1000 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 1000 GeV < Jet p_{T} < 1200 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 1200 GeV < Jet p_{T} < 1400 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 1400 GeV < Jet p_{T} < 1600 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 1600 GeV < Jet p_{T} < 2000 GeV, more forward jet.

$p_{T}^{rel} / GeV$ , 2000 GeV < Jet p_{T} < 2500 GeV, more forward jet.

$n_{ch}$ , 100 GeV < Jet p_{T} < 200 GeV, more central jet.

$n_{ch}$ , 200 GeV < Jet p_{T} < 300 GeV, more central jet.

$n_{ch}$ , 300 GeV < Jet p_{T} < 400 GeV, more central jet.

$n_{ch}$ , 400 GeV < Jet p_{T} < 500 GeV, more central jet.

$n_{ch}$ , 500 GeV < Jet p_{T} < 600 GeV, more central jet.

$n_{ch}$ , 600 GeV < Jet p_{T} < 700 GeV, more central jet.

$n_{ch}$ , 700 GeV < Jet p_{T} < 800 GeV, more central jet.

$n_{ch}$ , 800 GeV < Jet p_{T} < 900 GeV, more central jet.

$n_{ch}$ , 900 GeV < Jet p_{T} < 1000 GeV, more central jet.

$n_{ch}$ , 1000 GeV < Jet p_{T} < 1200 GeV, more central jet.

$n_{ch}$ , 1200 GeV < Jet p_{T} < 1400 GeV, more central jet.

$n_{ch}$ , 1400 GeV < Jet p_{T} < 1600 GeV, more central jet.

$n_{ch}$ , 1600 GeV < Jet p_{T} < 2000 GeV, more central jet.

$n_{ch}$ , 2000 GeV < Jet p_{T} < 2500 GeV, more central jet.

$r$ , 100 GeV < Jet p_{T} < 200 GeV, more central jet.

$r$ , 200 GeV < Jet p_{T} < 300 GeV, more central jet.

$r$ , 300 GeV < Jet p_{T} < 400 GeV, more central jet.

$r$ , 400 GeV < Jet p_{T} < 500 GeV, more central jet.

$r$ , 500 GeV < Jet p_{T} < 600 GeV, more central jet.

$r$ , 600 GeV < Jet p_{T} < 700 GeV, more central jet.

$r$ , 700 GeV < Jet p_{T} < 800 GeV, more central jet.

$r$ , 800 GeV < Jet p_{T} < 900 GeV, more central jet.

$r$ , 900 GeV < Jet p_{T} < 1000 GeV, more central jet.

$r$ , 1000 GeV < Jet p_{T} < 1200 GeV, more central jet.

$r$ , 1200 GeV < Jet p_{T} < 1400 GeV, more central jet.

$r$ , 1400 GeV < Jet p_{T} < 1600 GeV, more central jet.

$r$ , 1600 GeV < Jet p_{T} < 2000 GeV, more central jet.

$r$ , 2000 GeV < Jet p_{T} < 2500 GeV, more central jet.

$\zeta$ , 100 GeV < Jet p_{T} < 200 GeV, more central jet.

$\zeta$ , 200 GeV < Jet p_{T} < 300 GeV, more central jet.

$\zeta$ , 300 GeV < Jet p_{T} < 400 GeV, more central jet.

$\zeta$ , 400 GeV < Jet p_{T} < 500 GeV, more central jet.

$\zeta$ , 500 GeV < Jet p_{T} < 600 GeV, more central jet.

$\zeta$ , 600 GeV < Jet p_{T} < 700 GeV, more central jet.

$\zeta$ , 700 GeV < Jet p_{T} < 800 GeV, more central jet.

$\zeta$ , 800 GeV < Jet p_{T} < 900 GeV, more central jet.

$\zeta$ , 900 GeV < Jet p_{T} < 1000 GeV, more central jet.

$\zeta$ , 1000 GeV < Jet p_{T} < 1200 GeV, more central jet.

$\zeta$ , 1200 GeV < Jet p_{T} < 1400 GeV, more central jet.

$\zeta$ , 1400 GeV < Jet p_{T} < 1600 GeV, more central jet.

$\zeta$ , 1600 GeV < Jet p_{T} < 2000 GeV, more central jet.

$\zeta$ , 2000 GeV < Jet p_{T} < 2500 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 100 GeV < Jet p_{T} < 200 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 200 GeV < Jet p_{T} < 300 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 300 GeV < Jet p_{T} < 400 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 400 GeV < Jet p_{T} < 500 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 500 GeV < Jet p_{T} < 600 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 600 GeV < Jet p_{T} < 700 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 700 GeV < Jet p_{T} < 800 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 800 GeV < Jet p_{T} < 900 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 900 GeV < Jet p_{T} < 1000 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 1000 GeV < Jet p_{T} < 1200 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 1200 GeV < Jet p_{T} < 1400 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 1400 GeV < Jet p_{T} < 1600 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 1600 GeV < Jet p_{T} < 2000 GeV, more central jet.

$p_{T}^{rel} / GeV$ , 2000 GeV < Jet p_{T} < 2500 GeV, more central jet.

The total uncertainty covariance matrix for the average number of tracks per jet $p_T$ bin. The covariance matrix is the sum of the covariance matrices for each source of systematic and statistical uncertainty. Note that the overall sign for the systematic uncertainty covariances is arbitrary.

The total uncertainty covariance matrix for the average fragmentation function per jet $p_T$ bin. The covariance matrix is the sum of the covariance matrices for each source of systematic and statistical uncertainty. Note that the overall sign for the systematic uncertainty covariances is arbitrary.

The total uncertainty covariance matrix for the average relative $p_T$ per jet $p_T$ bin. The covariance matrix is the sum of the covariance matrices for each source of systematic and statistical uncertainty. Note that the overall sign for the systematic uncertainty covariances is arbitrary.

The total uncertainty covariance matrix for the average r per jet $p_T$ bin. The covariance matrix is the sum of the covariance matrices for each source of systematic and statistical uncertainty. Note that the overall sign for the systematic uncertainty covariances is arbitrary.

The total uncertainty covariance matrix for the number of tracks. The first half of the bins on a given axis correspond to the more central jet while the second half correspond to the more forward jet. See Fig. 4 in the paper for more information about the binning. The covariance matrix is the sum of the covariance matrices for each source of systematic and statistical uncertainty. Note that the overall sign for the systematic uncertainty covariances is arbitrary.

The total uncertainty covariance matrix for the fragmentation function. The first half of the bins on a given axis correspond to the more central jet while the second half correspond to the more forward jet. See Fig. 4 in the paper for more information about the binning. The covariance matrix is the sum of the covariance matrices for each source of systematic and statistical uncertainty. Note that the overall sign for the systematic uncertainty covariances is arbitrary.

The total uncertainty covariance matrix for the relative $p_T$. The first half of the bins on a given axis correspond to the more central jet while the second half correspond to the more forward jet. See Fig. 4 in the paper for more information about the binning. The covariance matrix is the sum of the covariance matrices for each source of systematic and statistical uncertainty. Note that the overall sign for the systematic uncertainty covariances is arbitrary.

The total uncertainty covariance matrix for the r. The first half of the bins on a given axis correspond to the more central jet while the second half correspond to the more forward jet. See Fig. 4 in the paper for more information about the binning. The covariance matrix is the sum of the covariance matrices for each source of systematic and statistical uncertainty. Note that the overall sign for the systematic uncertainty covariances is arbitrary.