The timing distribution of the background sources predicted to contribute to the signal region, compared to those for a representative signal model. The time is defined by the jet in the event with the largest $t_{\mathrm{jet}}$ passing the relevant selection. The distributions for the major backgrounds are taken from control regions and normalized to the predictions. The observed data is shown by the black points. No events are observed in data for $t_{\mathrm{jet}} > 3\,$ns (indicated with a vertical black line).

The product of the acceptance and efficiency in the $c\tau_{0}$ vs. $m_{\tilde{g}}$ plane for the GMSB model, after all requirements.

The product of the acceptance and efficiency in the $c\tau_{0}$ vs. $m_{\tilde{g}}$ plane for the GMSB model, after all requirements.

The observed upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed.

The observed upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The observed upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed.

The observed upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The observed and expected upper limits at $95\%$ CL on the gluino pair production cross section for a gluino GMSB model with $m_{\tilde{g}}=2400$ GeV. The one (two) standard deviation variation in the expected limit is shown in the inner green (outer yellow) band. The blue solid line shows the observed limit obtained by the CMS displaced jet search

The observed and expected upper limits at $95\%$ CL on the gluino pair production cross section for a gluino GMSB model with $m_{\tilde{g}}=2400$ GeV. The one (two) standard deviation variation in the expected limit is shown in the inner green (outer yellow) band. The blue solid line shows the observed limit obtained by the CMS displaced jet search

The distribution (normalized to unity) of number of ECAL cells hit in the jet for jets in a background enriched data sample (satisfying $|\eta| < 1.48$, $PV_{\rm track}^{\rm fraction} > 1/12$, $\mathrm{HEF} > 0.2$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$ and $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$) and for signal jets satisfying signal region requirements (except those on $E_{\mathrm{ECAL}}$ and $N^{\mathrm{cell}}_{\mathrm{ECAL}}$).

The distribution (normalized to unity) of number of ECAL cells hit in the jet for jets in a background enriched data sample (satisfying $|\eta| < 1.48$, $p_\mathrm{T}tf > 0.08$, $\mathrm{HEF} > 0.2$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$ and $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$) and for signal jets satisfying signal region requirements (except those on $E_{\mathrm{ECAL}}$ and $N^{\mathrm{cell}}_{\mathrm{ECAL}}$).

The distribution (normalized to unity) of $\mathrm{HEF}$ for a data sample enriched in beam halo and noise jets (satisfying $|\eta| < 1.48$, $p_\mathrm{T} > 30 \,\mathrm{GeV}$, $PV_{\rm track}^{\rm fraction} < 1/12$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$ and $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$) and for signal jets passing signal region selections (except on $\mathrm{HEF}$).

The distribution (normalized to unity) of $\mathrm{HEF}$ for a data sample enriched in beam halo and noise jets (satisfying $|\eta| < 1.48$, $p_\mathrm{T} > 30 \,\mathrm{GeV}$, $p_\mathrm{T}tf < 0.08$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$ and $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$) and for signal jets passing signal region selections (except on $\mathrm{HEF}$).

The distribution (normalized to unity) of $E_{\mathrm{HCAL}}$ for a data sample enriched in beam halo and noise jets (satisfying $|\eta| < 1.48$, $p_\mathrm{T} > 30 \,\mathrm{GeV}$, $PV_{\rm track}^{\rm fraction} < 1/12$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$ and $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$) and for signal jets passing signal region selections (except on $E_{\mathrm{HCAL}}$).

The distribution (normalized to unity) of $E_{\mathrm{HCAL}}$ for a data sample enriched in beam halo and noise jets (satisfying $|\eta| < 1.48$, $p_\mathrm{T} > 30 \,\mathrm{GeV}$, $p_\mathrm{T}tf < 0.08$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$ and $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$) and for signal jets passing signal region selections (except on $E_{\mathrm{HCAL}}$).

The distribution (normalized to unity) of $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}}$ for data sample enriched in jets from noise (satisfying $|\eta| < 1.48$, $p_\mathrm{T} > 30\,\mathrm{GeV}$, $PV_{\rm track}^{\rm fraction} > 1/12$, $\mathrm{HEF} > 0.2$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20 \,\mathrm{GeV}$ and $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$) and for signal jets passing signal region selections (except on $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}}$ and $t^{\mathrm{RMS}}_\mathrm{jet}$)

The distribution (normalized to unity) of $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}}$ for data sample enriched in jets from noise (satisfying $|\eta| < 1.48$, $p_\mathrm{T} > 30\,\mathrm{GeV}$, $p_\mathrm{T}tf > 0.08$, $\mathrm{HEF} > 0.2$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20 \,\mathrm{GeV}$ and $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$) and for signal jets passing signal region selections (except on $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}}$ and $t^{\mathrm{RMS}}_\mathrm{jet}$)

The distribution (normalized to unity) of $t^{\mathrm{RMS}}_\mathrm{jet}$ for data sample enriched in jets from noise (satisfying $|\eta| < 1.48$, $p_\mathrm{T} > 30\,\mathrm{GeV}$, $PV_{\rm track}^{\rm fraction} > 1/12$, $\mathrm{HEF} > 0.2$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20 \,\mathrm{GeV}$ and $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$) and for signal jets passing signal region selections (except on $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}}$ and $t^{\mathrm{RMS}}_\mathrm{jet}$)

The distribution (normalized to unity) of $t^{\mathrm{RMS}}_\mathrm{jet}$ for data sample enriched in jets from noise (satisfying $|\eta| < 1.48$, $p_\mathrm{T} > 30\,\mathrm{GeV}$, $p_\mathrm{T}tf > 0.08$, $\mathrm{HEF} > 0.2$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20 \,\mathrm{GeV}$ and $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$) and for signal jets passing signal region selections (except on $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}}$ and $t^{\mathrm{RMS}}_\mathrm{jet}$)

The distribution (normalized to unity) of $PV_{\rm track}^{\rm fraction}$ for a data sample enriched in main bunch backgrounds (satisfying $p_\mathrm{T} > 30\,\mathrm{GeV}$, $|\eta| < 1.48$, $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$, $|t_{\mathrm{jet}}| < 3\,\mathrm{ns}$ and $E_{\mathrm{ECAL}} >20\,\mathrm{GeV}$) and for signal jets passing signal selections (except on $PV_{\rm track}^{\rm fraction}$).

The distribution (normalized to unity) of $p_\mathrm{T}tf$ for a data sample enriched in main bunch backgrounds (satisfying $p_\mathrm{T} > 30\,\mathrm{GeV}$, $|\eta| < 1.48$, $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$, $|t_{\mathrm{jet}}| < 3\,\mathrm{ns}$ and $E_{\mathrm{ECAL}} >20\,\mathrm{GeV}$) and for signal jets passing signal selections (except on $p_\mathrm{T}tf$).

The distribution (normalized to unity) of $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}}$ for a data sample enriched in beam halo (satisfying $p_\mathrm{T} > 30\,\mathrm{GeV}$, $|\eta| < 1.48$, $PV_{\rm track}^{\rm fraction} < 1/12$, $\mathrm{HEF} < 0.2$, $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$ and $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$) and for signal jets passing signal selections (except on $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}}$)

The distribution (normalized to unity) of $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}}$ for a data sample enriched in beam halo (satisfying $p_\mathrm{T} > 30\,\mathrm{GeV}$, $|\eta| < 1.48$, $p_\mathrm{T}tf < 0.08$, $\mathrm{HEF} < 0.2$, $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$, $t_{\mathrm{jet}} < -3\,\mathrm{ns}$ and $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$) and for signal jets passing signal selections (except on $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}}$)

The distribution (normalized to unity) of $\mathrm{max}(\Delta \phi_{\mathrm{DT}})$ for a data sample enriched in cosmic muons (satisfying $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$, $p_\mathrm{T} > 30\,\mathrm{GeV}$, $|\eta| < 1.48$, $PV_{\rm track}^{\rm fraction} < 1/12$, $\mathrm{HEF} > 0.2$, $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$, $t_{\mathrm{jet}} > 3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$ and failing the HCAL noise rejection quality filters) and for signal jets passing signal selections (except on $\mathrm{max}(\Delta \phi_{\mathrm{DT}})$).

The distribution (normalized to unity) of $\mathrm{max}(\Delta \phi_{\mathrm{DT}})$ for a data sample enriched in cosmic muons (satisfying $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$, $p_\mathrm{T} > 30\,\mathrm{GeV}$, $|\eta| < 1.48$, $p_\mathrm{T}tf < 0.08$, $\mathrm{HEF} > 0.2$, $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$, $t_{\mathrm{jet}} > 3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$ and failing the HCAL noise rejection quality filters) and for signal jets passing signal selections (except on $\mathrm{max}(\Delta \phi_{\mathrm{DT}})$).

The distribution (normalized to unity) of $\mathrm{max}(\Delta \phi_{\mathrm{RPC}})$ for a data sample enriched in cosmic muons (satisfying $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$, $p_\mathrm{T} > 30\,\mathrm{GeV}$, $|\eta| < 1.48$, $PV_{\rm track}^{\rm fraction} < 1/12$, $\mathrm{HEF} > 0.2$, $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$, $t_{\mathrm{jet}} > 3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$ and failing the HCAL noise rejection quality filters) and for signal jets passing signal selections (except on $\mathrm{max}(\Delta \phi_{\mathrm{RPC}})$).

The distribution (normalized to unity) of $\mathrm{max}(\Delta \phi_{\mathrm{RPC}})$ for a data sample enriched in cosmic muons (satisfying $E^{\mathrm{CSC}}_\mathrm{ECAL}/E_{\mathrm{ECAL}} < 0.8$, $p_\mathrm{T} > 30\,\mathrm{GeV}$, $|\eta| < 1.48$, $p_\mathrm{T}tf < 0.08$, $\mathrm{HEF} > 0.2$, $t^{\mathrm{RMS}}_\mathrm{jet}/t_{\mathrm{jet}} < 0.4$, $t_{\mathrm{jet}} > 3\,\mathrm{ns}$, $E_{\mathrm{ECAL}} > 20\,\mathrm{GeV}$ and failing the HCAL noise rejection quality filters) and for signal jets passing signal selections (except on $\mathrm{max}(\Delta \phi_{\mathrm{RPC}})$).

Distribution of $t_{\mathrm{jet}}$ for jets with the full Run 2 dataset with no cleaning selection applied (a) and after all jet cleaning selections are applied (b) in events satisfying the trigger requirements and satisfying $p_T^\mathrm{miss} > 300$. The jets are required to pass an inverted selection of $PV_{\rm track}^{\rm fraction} > 1/12$ to enrich the sample in those originating from main and satellite bunch backgrounds. The cleaning selections are shown to reduce the backgrounds by many orders of magnitude.

Distribution of $t_{\mathrm{jet}}$ for jets with the full Run 2 dataset with no cleaning selection applied (a) and after all jet cleaning selections are applied (b) in events satisfying the trigger requirements and satisfying $p_T^\mathrm{miss} > 300$. The jets are required to pass an inverted selection of $PV_{\rm track}^{\rm fraction} > 0.08$ to enrich the sample in those originating from main and satellite bunch backgrounds. The cleaning selections are shown to reduce the backgrounds by many orders of magnitude.

Distribution of $t_{\mathrm{jet}}$ for jets with the full Run 2 dataset in events satisfying the trigger requirements and satisfying $p_T^\mathrm{miss} < 300$. The jets are required to pass an inverted selection of $PV_{\rm track}^{\rm fraction} > 1/12$ to enrich the sample in those originating from main and satellite bunch backgrounds (all other jet cleaning selections are applied). Clear contributions from jets from satellite bunch collisions can be seen peaked around -5, 5 and 10 ns.

Distribution of $t_{\mathrm{jet}}$ for jets with the full Run 2 dataset in events satisfying the trigger requirements and satisfying $p_T^\mathrm{miss} < 300$. The jets are required to pass an inverted selection of $PV_{\rm track}^{\rm fraction} > 0.08$ to enrich the sample in those originating from main and satellite bunch backgrounds (all other jet cleaning selections are applied). Clear contributions from jets from satellite bunch collisions can be seen peaked around -5, 5 and 10 ns.

Contribution to the delayed time of jets from the $\beta$ of the gluino is plotted against the delay contribution from the difference (assuming straight line paths) between the path taken by the gluino and the particle forming the jet from the path length for a particle travelling directly to the same position on the ECAL barrel for gluino $c\tau_{0} = 10$ m and mass of 1000 Gev (top) and 3000 GeV (bottom). The dominant contribution is shown to be the gluino $\beta$.

Contribution to the delayed time of jets from the $\beta$ of the gluino is plotted against the delay contribution from the difference (assuming straight line paths) between the path taken by the gluino and the particle forming the jet from the path length for a particle travelling directly to the same position on the ECAL barrel for gluino $c\tau_{0} = 10$ m and mass of 1000 Gev (top) and 3000 GeV (bottom). The dominant contribution is shown to be the gluino $\beta$.

Selection efficiencies for the GMSB model with $m_{\tilde{g}}=1000$ and various proper decay lengths

Selection efficiencies for the GMSB model with $m_{\tilde{g}}=1000$ and various proper decay lengths

Selection efficiencies for the GMSB model with $m_{\tilde{g}}=2400$ and various proper decay lengths

Selection efficiencies for the GMSB model with $m_{\tilde{g}}=2400$ and various proper decay lengths

Selection efficiencies for the GMSB model with $m_{\tilde{g}}=3000$ and various proper decay lengths

Selection efficiencies for the GMSB model with $m_{\tilde{g}}=3000$ and various proper decay lengths

The observed upper limits at $95\%$ CL for the gluino pair production cross section relative to the theoretical cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The observed upper limits at $95\%$ CL for the gluino pair production cross section relative to the theoretical cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected upper limits at $95\%$ CL for the gluino pair production cross section relative to the theoretical cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected upper limits at $95\%$ CL for the gluino pair production cross section relative to the theoretical cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected plus 1 $\sigma_{\mathrm{experiment}}$ upper limits at $95\%$ CL for the gluino pair production cross section relative to the theoretical cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected plus 1 $\sigma_{\mathrm{experiment}}$ upper limits at $95\%$ CL for the gluino pair production cross section relative to the theoretical cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected minus 1 $\sigma_{\mathrm{experiment}}$ upper limits at $95\%$ CL for the gluino pair production cross section relative to the theoretical cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected minus 1 $\sigma_{\mathrm{experiment}}$ upper limits at $95\%$ CL for the gluino pair production cross section relative to the theoretical cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected plus 1 $\sigma_{\mathrm{experiment}}$ upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected plus 1 $\sigma_{\mathrm{experiment}}$ upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected minus 1 $\sigma_{\mathrm{experiment}}$ upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

The expected minus 1 $\sigma_{\mathrm{experiment}}$ upper limits at $95\%$ CL for the gluino pair production cross section in the GMSB model, shown in the plane of $m_{\tilde{g}}$ and $c\tau_{0}$. A branching fraction of $100\%$ for the gluino decay to a gluon and a gravitino is assumed. The area below the thick black curve represents the observed exclusion region, while the dashed red lines indicate the expected limits and their $\pm 1$ standard deviation ranges from experimental uncertainties. The thin black lines show the effect of the theoretical uncertainties on the signal cross section.

Measured misidentification probability distribution as a function of track multiplicity for the EMJ-1 criteria group defined in Table 2. The red up-pointing triangles are for b jets while the blue down-pointing triangles are for light-flavor jets. The horizontal lines on the data points indicate the variable bin width.

The $H_\mathrm{T}$ distribution for the observed data events (black points) and the predicted background estimation (blue) for selection set 8 (SM QCD-enhanced), requiring at least two jets tagged by loose emerging jet criteria.

The number of associated tracks distribution for the observed data events (black points) and the predicted background estimation (blue) for selection set 8 (SM QCD-enhanced), requiring at least two jets tagged by loose emerging jet criteria.

The $H_\mathrm{T}$ distribution for the observed data events (black points) and the predicted background estimation (blue) for selection set 9 (SM QCD-enhanced), requiring at least one jet tagged by loose emerging jet criteria and large $p_\mathrm{T}^\mathrm{miss}$.

The number of associated tracks distribution for the observed data events (black points) and the predicted background estimation (blue) for selection set 9 (SM QCD-enhanced), requiring at least one jet tagged by loose emerging jet criteria and large $p_\mathrm{T}^\mathrm{miss}$.

Upper limits at 95% CL on the signal cross section for models with dark pion mass $(m_{\pi_\mathrm{DK}})$ of 5 GeV in the proper decay length $(c\tau_{\pi_\mathrm{DK}})$ versus dark mediator mass $(m_{\mathrm{X_{DK}}})$ plane.

Dark mediator mass exclusion limits at 95% CL derived from theoretical cross sections for models with dark pion mass $(m_{\pi_\mathrm{DK}})$ of 5 GeV in the proper decay length $(c\tau_{\pi_\mathrm{DK}})$ versus dark mediator mass $(m_{\mathrm{X_{DK}}})$ plane.

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The particle-level di-jet differential cross section. The systematic uncertainty on the data contains contributions from track finding efficiency, track transverse momentum resolution, calorimeter energy resolution, and unfolding uncertainties. For the theory, values are given for the underlying event and hadronization (UEH) correction uncertainty and the quadrature sum of the UEH and theoretical uncertainties. Both the UEH and theoretical uncertainties include contributions from factorization and renormalization scale uncertainties and PDF uncertainties. An 8.8% uncertainty common to all points due to the integrated luminosity determination is also present, but not included in the systematic values quoted below.

Values of gluon X1 and X2 obtained from the PYTHIA detector-level simulation for the same-sign di-jet topology compared to the gluon X distribution for inclusive jets. The inclusive distribution has been scaled down by a factor of 20 compared to the di-jet distributions.

Values of gluon X1 and X2 obtained from the PYTHIA detector-level simulation for the opposite-sign di-jet topology compared to the gluon X distribution for inclusive jets. The inclusive distribution has been scaled down by a factor of 20 compared to the di-jet distributions.

Di-jet A_LL asymmetry vs parton-level invariant mass for the same-sign di-jet topology. The systematic uncertainty on the mass includes contributions from jet energy scale, the correction to parton-level, and the difference between NLO and PYTHIA cross sections. The systematic uncertainty on the asymmetry includes contributions from trigger and reconstruction bias and residual transverse beam polarization components. A 6.5% uncertainty common to all points due to uncertainty on the measured beam polarizations is also present, but not included in the uncertainties quoted below.

Theoretical predictions for the di-jet A_LL asymmetry for the same-sign topology using the DSSV14 and NNPDFpol1.1 polarized PDF sets. The DSSV14 prediction is presented without uncertainty while the systematic uncertainty on the NNPDFpol1.1 prediction contains contributions from factorization and renormalization scale uncertainties and PDF uncertainties.

Di-jet A_LL asymmetry vs parton-level invariant mass for the opposite-sign di-jet topology. The systematic uncertainty on the mass includes contributions from jet energy scale, the correction to parton-level, and the difference between NLO and PYTHIA cross sections. The systematic uncertainty on the asymmetry includes contributions from trigger and reconstruction bias and residual transverse beam polarization components. A 6.5% uncertainty common to all points due to uncertainty on the measured beam polarizations is also present, but not included in the uncertainties quoted below.

Theoretical predictions for the di-jet A_LL asymmetry for the opposite-sign topology using the DSSV14 and NNPDFpol1.1 polarized PDF sets. The DSSV14 prediction is presented without uncertainty while the systematic uncertainty on the NNPDFpol1.1 prediction contains contributions from factorization and renormalization scale uncertainties and PDF uncertainties.

Observed and expected 95% CL upper limits on the product of cross section of a narrow resonance and the branching fraction $\sigma(gg \to X) B(X \to HH \to bbbb)$ for HPHP category. Theory curves corresponding to WED models with radion are superimposed.

Observed and expected 95% CL upper limits on the product of cross section of a narrow resonance and the branching fraction $\sigma(gg \to X) B(X \to HH \to bbbb)$ for HPLP category. Theory curves corresponding to WED models with radion are superimposed.

Observed and expected 95% CL upper limits on the product of cross section of a narrow resonance and the branching fraction $\sigma(gg \to X) B(X \to HH \to bbbb)$ for LPHP category. Theory curves corresponding to WED models with radion are superimposed.

Observed and expected 95% CL upper limits on the product of cross section and the branching fraction $\sigma(gg \to X) B(X \to HH \to bbbb)$ for HPHP, HPLP and LPHP categories combined. The one standard deviation on the 95% CL upper limit is also provided.

Inclusive jet $A_{LL}$ vs. parton jet $p_T$ for 0.5<|eta|<1.0.

The uncertainties on the parton jet pT values are strongly correlated across the bins. The point-to-point statistical and systematic uncertainties on the measured A_LL values given above are only weakly correlated among the bins. The correlation matrix for the quadrature sum of the point-to-point statistical and systematic uncertainties is given below. In that matrix, the order of the rows and columns matches the bin numbering above. In addition to the point-to-point statistical and systematic uncertainties, there are two systematic uncertainties that are common to all the measured A_LL values (and not included in the systematic uncertainty numbers quoted above): (a) +/-0.0005 vertical shift uncertainty from relative luminosity and (b) +/-6.5% vertical scale uncertainty from polarization.

$A_{LL}$ model predictions for |eta|<0.5.

$A_{LL}$ model predictions for 0.5<|eta|<1.0.

NLO cross sections and selection efficiencies (assuming $\beta$ = 1) for different signal points.

Selection efficiencies in % for the signal in the top squark search, estimated from the simulation.

The final $S_{\text{T}}$ distribution for the leptoquark search with the $\text{e}\tau_{\text{h}}$ and $\mu\tau_{\text{h}}$ channels combined. The last bin contains the overflow events.

The final $S_{\text{T}}$ distribution for the top squark search with the $\text{e}\tau_{\text{h}}$ and $\mu\tau_{\text{h}}$ channels combined. The last bin contains the overflow events.

The expected and observed combined upper limits on the third-generation LQ pair production cross section $\sigma$ times the square of the branching fraction, $\mathcal{B}^2$, at 95% CL, as a function of the LQ mass. These limits also apply to top squarks decaying directly via the coupling $\lambda^{\prime}_{333}$.

The expected and observed combined upper limits on the top squark pair production cross section $\sigma$ times the square of the branching fraction, $\mathcal{B}^2$, at 95% CL, as a function of the top squark mass. These limits apply to top squarks with a chargino-mediated decay through the coupling $\lambda^{\prime}_{3jk}$.

The expected and observed 95% CL upper limits on the branching fraction for the leptoquark decay to a tau lepton and a bottom quark, as a function of the leptoquark mass. A search for top squark pair production [EPJC 73(2013)2677] has the same kinematic signature as the leptoquark decay to a tau neutrino and a top quark. This search is reinterpreted to provide the expected and observed 95% CL upper limits for low values of $\mathcal{B}$, assuming the leptoquark only decays to third-generation fermions.

Number of data events (20.3 fb$^{-1}$), number of predicted events from the fit, statistical uncertainty on the fit, systematic uncertainty on the choice of control region, and on the choice of fit function versus inclusive $H_{\textrm{T}}^{\textrm{min}}$ lower bin edge for inclusive jet multiplicity $N_{\textrm{Jet}} \geq 6$. The total uncertainty is obtained by adding the three uncertainties linearly.

Number of data events (20.3 fb$^{-1}$), number of predicted events from the fit, statistical uncertainty on the fit, systematic uncertainty on the choice of control region, and on the choice of fit function versus inclusive $H_{\textrm{T}}^{\textrm{min}}$ lower bin edge for inclusive jet multiplicity $N_{\textrm{Jet}} \geq 7$. The total uncertainty is obtained by adding the three uncertainties linearly.

Number of data events (20.3 fb$^{-1}$), number of predicted events from the fit, statistical uncertainty on the fit, systematic uncertainty on the choice of control region, and on the choice of fit function versus inclusive $H_{\textrm{T}}^{\textrm{min}}$ lower bin edge for inclusive jet multiplicity $N_{\textrm{Jet}} \geq 8$. The total uncertainty is obtained by adding the three uncertainties linearly.

Upper limits on the visible cross section (cross section ($\sigma$) times acceptance ($A$) times efficiency ($\epsilon$)) at the 95% CL versus inclusive $H_{\textrm{T}}^{\textrm{min}}$ for $N_{\textrm{Jet}}\geq 3$.

Upper limits on the visible cross section (cross section ($\sigma$) times acceptance ($A$) times efficiency ($\epsilon$)) at the 95% CL versus inclusive $H_{\textrm{T}}^{\textrm{min}}$ for $N_{\textrm{Jet}}\geq 4$.

Upper limits on the visible cross section (cross section ($\sigma$) times acceptance ($A$) times efficiency ($\epsilon$)) at the 95% CL versus inclusive $H_{\textrm{T}}^{\textrm{min}}$ for $N_{\textrm{Jet}}\geq 5$.

Upper limits on the visible cross section (cross section ($\sigma$) times acceptance ($A$) times efficiency ($\epsilon$)) at the 95% CL versus inclusive $H_{\textrm{T}}^{\textrm{min}}$ for $N_{\textrm{Jet}}\geq 6$.

Upper limits on the visible cross section (cross section ($\sigma$) times acceptance ($A$) times efficiency ($\epsilon$)) at the 95% CL versus inclusive $H_{\textrm{T}}^{\textrm{min}}$ for $N_{\textrm{Jet}}\geq 7$.

Upper limits on the visible cross section (cross section ($\sigma$) times acceptance ($A$) times efficiency ($\epsilon$)) at the 95% CL versus inclusive $H_{\textrm{T}}^{\textrm{min}}$ for $N_{\textrm{Jet}}\geq 8$.

Mean reconstruction efficiencies $(\epsilon)$ and RMS of the reconstruction efficiencies for various black hole and string ball models.

Distributions of the b-tagging efficiency as a function of the mistag rate of charm jets for pp collisions in a PYTHIA simulation.

Distributions of the b-tagging efficiency as a function of the mistag rate of light jets for pPb collisions in a PYTHIA+HIJING simulation.

Distributions of the b-tagging efficiency as a function of the mistag rate of charm jets for pPb collisions in a PYTHIA+HIJING simulation.

Distributions of the Secondary Vertex Mass after applying the SSV tagger selection.

b-jet cross-sections in pPb, scaled by the Glauber nuclear overlap function, as well as a b-jet cross-section from a PYTHIA simulation from -2.5 < eta_CM < -1.5.

b-jet cross-sections in pPb, scaled by the Glauber nuclear overlap function, as well as a b-jet cross-section from a PYTHIA simulation from -1.5 < eta_CM < -0.5 (x 10^2).

b-jet cross-sections in pPb, scaled by the Glauber nuclear overlap function, as well as a b-jet cross-section from a PYTHIA simulation from -0.5 < eta_CM < 0.5 (x10^4).

b-jet cross-sections in pPb, scaled by the Glauber nuclear overlap function, as well as a b-jet cross-section from a PYTHIA simulation from 0.5 < eta_CM < 1.5 (x10^6).

b-jet RpA (PYTHIA) from 0.5 < eta_CM < 1.5.

b-jet RpA (PYTHIA) from -0.5 < eta_CM < 0.5.

b-jet RpA (PYTHIA) from -1.5 < eta_CM < -0.5.

b-jet RpA (PYTHIA) from -2.5 < eta_CM < -1.5.

b-jet Fraction.

b-jet RpA(PYTHIA).

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

BACKGROUND MINUS - Double W/Z tagged background variation downward (1 sigma) in HIGH purity bin estimated from a fit to data.

DATA - Double W/Z tagged events in LOW purity bin.

BACKGROUND - Double W/Z tagged background in LOW purity bin estimated from a fit to data.

BACKGROUND PLUS - Double W/Z tagged background variation upward (1 sigma) in LOW purity bin estimated from a fit to data.

BACKGROUND MINUS - Double W/Z tagged background variation downward (1 sigma) in LOW purity bin estimated from a fit to data.

Observed and expected 95% CL exclusions on the mass of various resonances.

Measured jet multiplicity distribution in the $W\mu\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured dilepton invariant mass distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured $E_{T}^{miss}$ distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured leading jet $p_{T}$ distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured jet multiplicity distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured transverse mass distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured $E_{T}^{miss}$ distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured leading jet $p_{T}$ distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured jet multiplicity distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured dilepton invariant mass distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured $E_{T}^{miss}$ distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured leading jet $p_{T}$ distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured jet multiplicity distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured distribution of the jet multiplicity for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of $E_{T}^{miss}$ for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of leading jet $p_{T}$ for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_{T}$ to $E_{T}^{miss}$ ratio for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the jet multiplicity for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the jet multiplicity for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ for SR9 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ to $E_{T}^{miss}$ ratio for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ to $E_{T}^{miss}$ ratio for SR9 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Observed and expected 95$\%$ CL limit on the fundamental Planck scale in $4+n$ dimensions, $M_D$, as a function of the number of extra dimensions. In the figure the two results overlap. The shaded areas around the expected limit indicate the expected $\pm 1\sigma$ and $\pm 2\sigma$ ranges of limits in the absence of a signal. The 95$\%$ CL observed limits after the suppression of the events with $\hat{s} > M_D^2$ is applied (truncated) are also given.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the scalar operator D1. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the vector operator D5. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the axial vector operator D8. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the tensor operator D9. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the gluon operator D11. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the gluon operator C5. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Observed 95% CL limits on the suppression scale M* as a function of the mediator mass Mmed, assuming a Z'-like boson in a simplified model and a DM mass of 50 GeV and 400 GeV. The width of the mediator is varied between Mmed/3 and Mmed/8pi.

Observed 95% CL upper limits on the product of couplings of the simplified model vertex in the plane of mediator and WIMP mass (Mmed versus m_chi).

Upper limits at 90% C.L. on the WIMP-nucleon scattering cross section as a function of m_chi for spin-independent interactions, for a coupling strength of unity or the maximum value that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

Upper limits at 90% C.L. on the WIMP-nucleon scattering cross section as a function of m_chi for spin-dependent interactions, for a coupling strength of unity or the maximum value that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

Upper limits at 90% C.L. on the WIMP-nucleon annihilation cross section as a function of m_chi, for a coupling strength of unity or the maximum value that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for degenerate squark/gluino masses.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 1/2 \times m_{\tilde{q}}$.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 1/4 \times m_{\tilde{q}}$.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 2 \times m_{\tilde{q}}$.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 4 \times m_{\tilde{q}}$.

Observed and expected 95$\%$ CL upper limit on $\sigma \times {\rm{BR}}(H \to {\rm{invisible}})$ as a function of the Higgs boson mass.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the scalar operator C1. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross section ratios for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Measured charged jet differential cross section ratios for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV.

Average charged particle multiplicity in charged jets.

Average charged particle multiplicity in charged jets.

Average charged particle multiplicity in charged jets.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average transverse momentum density distribution within a charged jet.

Average radius containing 80% of the total reconstructed jet transverse momentum.

Average radius containing 80% of the total reconstructed jet transverse momentum.

Average radius containing 80% of the total reconstructed jet transverse momentum.

Transverse momentum of particles in charged jet.

Transverse momentum of particles in charged jet.

Transverse momentum of particles in charged jet.

Transverse momentum of particles in charged jet.

Charged particle scaled pT spectra dN/dz.

Charged particle scaled pT spectra dN/dz.

Charged particle scaled pT spectra dN/dz.

Charged particle scaled pT spectra dN/dz.

Charged particle scaled pT spectra dN/dxi.

Charged particle scaled pT spectra dN/dxi.

Charged particle scaled pT spectra dN/dxi.

Charged particle scaled pT spectra dN/dxi.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV without UE subtraction.

Measured charged jet differential cross sections for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV without UE subtraction.

Average charged particle multiplicity in charged jets without UE subtraction.

Average charged particle multiplicity in charged jets without UE subtraction.

Average charged particle multiplicity in charged jets without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Average transverse momentum density distribution within a charged jet without UE subtraction.

Transverse momentum of particles in charged jet without UE subtraction.

Transverse momentum of particles in charged jet without UE subtraction.

Transverse momentum of particles in charged jet without UE subtraction.

Transverse momentum of particles in charged jet without UE subtraction.

Charged particle scaled pT spectra dN/dz without UE subtraction.

Charged particle scaled pT spectra dN/dz without UE subtraction.

Charged particle scaled pT spectra dN/dz without UE subtraction.

Charged particle scaled pT spectra dN/dz without UE subtraction.

Charged particle scaled pT spectra dN/dxi without UE subtraction.

Charged particle scaled pT spectra dN/dxi UE subtracted.

Charged particle scaled pT spectra dN/dxi without UE subtraction.

Charged particle scaled pT spectra dN/dxi without UE subtraction.

Mean $p_T$, leading in-jet charged particle.

Mean $p_T$, charged particle jets, $p^{ch.jet}_T > 5$ GeV, $|\eta^{ch.jet}| < 1.9$.

Charged jet rate, $p^\text{ch.jet}_T > 5$ GeV, $|\eta^{ch.jet}| < 1.9$.

Charged jet rate, $p^\text{ch.jet}_T > 30$ GeV, $|\eta^{ch.jet}| < 1.9$.

Jet $p_T$ spectrum, $|\eta^{ch.jet}| < 1.9$, $10 < N_\text{ch} \le 30$.

Jet $p_T$ spectrum, $|\eta^{ch.jet}| < 1.9$, $30 < N_\text{ch} \le 50$.

Jet $p_T$ spectrum, $|\eta^{ch.jet}| < 1.9$, $50 < N_\text{ch} \le 80$.

Jet $p_T$ spectrum, $|\eta^{ch.jet}| < 1.9$, $80 < N_\text{ch} \le 110$.

Jet $p_T$ spectrum, $|\eta^{ch.jet}| < 1.9$, $110 < N_\text{ch} \le 140$.

Intrajet ring $p_{T}$ density, $10 < N_\text{ch} \le 30$.

Intrajet ring $p_{T}$ density, $30 < N_\text{ch} \le 50$.

Intrajet ring $p_{T}$ density, $50 < N_\text{ch} \le 80$.

Intrajet ring $p_{T}$ density, $80 < N_\text{ch} \le 110$.

Intrajet ring $p_{T}$ density, $110 < N_\text{ch} \le 140$.

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Observed and expected 95% CL exclusions on the mass of various resonances. Systematic uncertainties are taken into account. For excited b quark the expected mass limit is below the range of this analysis. For the Axigluon/coloron and color-octet scalar only observed mass limits are computed.

Observed 95% CL upper limits on $\sigma B A$ as a function of resonance mass for several values of the width-to-mass ratio $\Gamma$ / M, computed for qq $\to$ G $\to$ qq.

Observed 95% CL upper limits on $\sigma B A$ as a function of resonance mass for several values of the width-to-mass ratio $\Gamma$ / M, computed for gg $\to$ G $\to$ gg.

Observed 95% CL upper limits on $\sigma B A$ for QBHs from the inclusive analysis. These limits are valid for the number of extra dimensions n considered in this paper, ranging from 1 to 6.

Observed 95% CL lower limits on ${M_{QBH}}^{min}$ for different numbers of extra dimensions n and several values of M$_{D}$.

Correction factors defined as the ratio of the full cross section obtained from Eqs. (5)-(7) to the cross section from the narrow-width approximation calculations, as a function of the resonance mass, for qq resonances and for eight different resonance widths in proton-proton collisions at $\sqrt{s}$=8 TeV.

Correction factors defined as the ratio of the full cross section obtained from Eqs. (5)-(7) to the cross section from the narrow-width approximation calculations, as a function of the resonance mass, for gg resonances and for eight different resonance widths in proton-proton collisions at $\sqrt{s}$=8 TeV.

Total cross sections (cross section), branching ratios (BR(gg)) and acceptances (A) for decays in gg, for the S8 model.

Total cross sections (cross section),next-to-next-to-leading order k-factors, branching ratios (BR(qqbar prime)) and acceptances for decays in q anti-q prime only (A) for the W prime model.

Total cross sections (cross section), branching ratios (BR(qqbar prime)) and acceptances for decays in q anti-q prime only (A) for the W* leptophobic model.

Total cross sections (cross section), branching ratios (BR(qqbar prime)) and acceptances for all decays (A) for the W* leptophilic model.

Total cross sections (cross section), branching ratios only involving q and g (BR(q/g)) and acceptances for all decays into jets for the QBH model from the QBH generator.

Total cross sections (cross section), branching ratios only involving q and g (BR(q/g)) and acceptances for all decays into jets for the QBH model from the BlackMax generator.

Observed limit on cross section times acceptance for each width and mass of Gaussian signal shape tested.

Observed limit on cross section times acceptance for each intrinsic width and mass of Breit-Wigner signal shape tested. The limits in this table correspond to the qq PDF.

Observed limit on cross section times acceptance for each intrinsic width and mass of Breit-Wigner signal shape tested. The limits in this table correspond to the qg PDF.

Observed limit on cross section times acceptance for each intrinsic width and mass of Breit-Wigner signal shape tested. The limits in this table correspond to the gg PDF.

Observed limit on cross section times acceptance for each intrinsic width and mass of Breit-Wigner signal shape tested. The limits in this table correspond to the q anti-q PDF.

Acceptance (A), efficiency (EPSILON), cross-section (SIG) and limits in number of events for the excited quark benchmark model, as a function of the signal mass M(q*). Uncertainties on the cross section are on the order of 1%. The limits include statistical uncertainties only. Expected limits include the 68% uncertainty band. Acceptance was calculated using parton-level quantities by imposing criteria that apply directly to kinematic selections (photon/jet |eta|, photon/jet transverse momentum, Delta(eta), Delta(R)). All other selections, which in general correspond to event and object quality criteria, were used to calculate the efficiency based on the events included in the acceptance.

Observed 95 PCT exclusion limit in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Expected 95 PCT exclusion limit in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Observed 95 PCT exclusion limit in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Number of MC signal events in the M(stop), M(neutralino) plane in gaugino universality scenario.

Number of MC signal events in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Number of MC signal events in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Cross section in the M(stop), M(neutralino) plane in gaugino universality scenario.

Cross section in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Cross section in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Acceptance in the 1LSR signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Acceptance in the 1LSR signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Efficiency in the 1LSR signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Efficiency in the 1LSR signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Total PCT systematic uncertainty in the 1LSR region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Total PCT systematic uncertainty in the 1LSR region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Acceptance in the 2LSR1 signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Acceptance in the 2LSR2 signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Efficiency in the 2LSR1 signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Efficiency in the 2LSR2 signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Total PCT systematic uncertainty in the 2LSR1 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Total PCT systematic uncertainty in the 2LSR2 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Acceptance in the 2LSR1 signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Acceptance in the 2LSR2 signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Efficiency in the 2LSR1 signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Efficiency in the 2LSR2 signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Total PCT systematic uncertainty in the 2LSR1 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Total PCT systematic uncertainty in the 2LSR2 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Acceptance in the 2LSR1 signal region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Acceptance in the 2LSR2 signal region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Efficiency in the 2LSR1 signal region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Efficiency in the 2LSR2 signal region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Total PCT systematic uncertainty in the 2LSR1 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Total PCT systematic uncertainty in the 2LSR2 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

expected CLs values for the 1LSR region in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values for the 1LSR region in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values for the 2LSR1 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values for the 2LSR1 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values for the 2LSR2 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values for the 2LSR2 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values combining the 1LSR and 2LSR1 regions in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values combining the 1LSR and 2LSR1 regions in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values combining the 1LSR and 2LSR2 regions in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values combining the 1LSR and 2LSR2 regions in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values for the best expected combination in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values for the best expected combination in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values for the 1LSR region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values for the 1LSR region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values for the 2LSR1 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values for the 2LSR1 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values for the 2LSR2 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values for the 2LSR2 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values combining the 1LSR and 2LSR1 regions in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values combining the 1LSR and 2LSR1 regions in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values combining the 1LSR and 2LSR2 regions in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values combining the 1LSR and 2LSR2 regions in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values for the best expected combination in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values for the best expected combination in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values for the 2LSR1 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

observed CLs values for the 2LSR1 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

expected CLs values for the 2LSR2 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

observed CLs values for the 2LSR2 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

expected CLs values for the best expected combination in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

observed CLs values for the best expected combination in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

(1) Number of generated MC events for the spin 1/2 top partner signal grid (2) Relative Cross section uncertainties for the spin 1/2 top partner signal grid.

(1) Acceptance of the same flavour selection for the spin 1/2 top partner signal grid (2) Selection efficiency of the same flavour selection for the spin 1/2 top partner signal grid (3) Product of the acceptance and efficiency of the same flavour selection for the spin 1/2 top partner signal grid (4) Relative experimental uncertainties on the acceptance times efficiency of the same flavour selection for the spin 1/2 top partner signal grid.

(1) Acceptance of the different flavour selection for the spin 1/2 top partner signal grid (2) Selection efficiency of the different flavour selection for the spin 1/2 top partner signal grid (3) Product of the acceptance and efficiency of the different flavour selection for the spin 1/2 top partner signal grid (4) Relative experimental uncertainties on the acceptance times efficiency of the different flavour selection for the spin 1/2 top partner signal grid.

(1) Observed CLs values for the scalar top signal grid (2) Expected CLs values for the scalar top signal grid.

(1) Observed CLs values for the spin 1/2 top partner signal grid (2) Expected CLs values for the spin 1/2 top partner signal grid.

Cross section limits [pb] for the scalar top signal grid.

Cross section limits [pb] for the spin 1/2 top partner signal grid.

Observed 95% CL limit for stop grid as a function of the scalar top and neutralino masses.

Observed 95% CL limit for stop grid as a function of the scalar top and neutralino masses, varying signal cross section of +1sigma.

Observed 95% CL limit for stop grid as a function of the scalar top and neutralino masses, varying signal cross section of -1sigma.

Expected 95% CL limit for stop grid as a function of the scalar top and neutralino masses.

Expected 95% CL limit for stop grid as a function of the scalar top and neutralino masses, varying the uncertainty of +1sigma.

Expected 95% CL limit for stop grid as a function of the scalar top and neutralino masses, varying the uncertainty of -1sigma.

Observed 95% CL limit for top partner grid as a function of the top partner and neutralino masses.

Observed 95% CL limit for top partner grid as a function of the top partner and neutralino masses, varying signal cross section of +1sigma.

Observed 95% CL limit for top partner grid as a function of the top partner and neutralino masses, varying signal cross section of -1sigma.

Expected 95% CL limit for top partner grid as a function of the top partner and neutralino masses.

Expected 95% CL limit for top partner grid as a function of the top partner and neutralino masses, varying the uncertainty of +1sigma.

Expected 95% CL limit for top partner grid as a function of the top partner and neutralino masses, varying the uncertainty of -1sigma.

The transverse momentum distribution of the 4th-leading lepton for events with at least 4 leptons and no Z-boson candidate.

Distribution of missing transverse momentum for events with at least 4 leptons and no Z-boson candidate.

Distribution of effective mass for events with at least 4 leptons and no Z-boson candidate.

Simplified Model (1) Number of generated events (2) Cross-section [pb] (3) CL_{S} [%] for SR1 (4) Acceptance [%] for SR1 (5) Efficiency [%] for SR1 (6) Uncertainty (not including MC statistics) for SR1 (7) CL_{S} [%] for SR2 (8) Acceptance [%] for SR2 (9) Efficiency [%] for SR2 (10) Uncertainty (not including MC statistics) for SR2.

MSUGRA/CMSSM Model (1) Number of generated events (2) Cross-section [pb] (3) CL_{S} [%] for SR1 (4) Acceptance [%] for SR1 (5) Efficiency [%] for SR1 (6) Uncertainty (not including MC statistics) for SR1 (7) CL_{S} [%] for SR2 (8) Acceptance [%] for SR2 (9) Efficiency [%] for SR2 (10) Uncertainty (not including MC statistics) for SR2.

Distribution of the variable ETmiss/sqrt(HT) for events with >= 7 jets each having transverse momentum > 80 GeV. The table gives the number of observed data events, the expected standard model backgroud prediction and the signal expected from the SUSY signal process.

Distribution of the variable ETmiss/sqrt(HT) for events with >= 9 jets each having transverse momentum > 55 GeV. The table gives the number of observed data events, the expected standard model backgroud prediction and the signal expected from the SUSY signal process.

Distribution of the variable ETmiss/sqrt(HT) for events with >= 8 jets each having transverse momentum > 80 GeV. The table gives the number of observed data events, the expected standard model backgroud prediction and the signal expected from the SUSY signal process.

Transverse momentum distribution of the sub-leading lepton in the signal region SR1a showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the 3rd-leading lepton in the signal region SR1a showing both data points with statistical errors only and the expected standard model background.

Missing transverse energy distribution in the signal region SR1a showing both data points with statistical errors only and the expected standard model background.

Mass distribution of Same Flavour Opposite Sign lepton pairs in the signal region SR1a showing both data points with statistical errors only and the expected standard model background.

Jet multiplicity distribution in the signal region SR1a showing both data points with statistical errors only and the expected standard model background.

Transverse mass distribution in the signal region SR1a showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the leading lepton in the signal region SR2 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the sub-leading lepton in the signal region SR2 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the 3rd-leading lepton in the signal region SR2 showing both data points with statistical errors only and the expected standard model background.

Missing transverse energy distribution in the signal region SR2 showing both data points with statistical errors only and the expected standard model background.

Jet multiplicity distribution in the signal region SR2 showing both data points with statistical errors only and the expected standard model background.

Transverse mass distribution in the signal region SR2 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the leading lepton in the validation region VR1 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the sub-leading lepton in the validation region VR1 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the 3rd-leading lepton in the validation region VR1 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the leading lepton in the validation region VR2 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the sub-leading lepton in the validation region VR2 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the 3rd-leading lepton in the validation region VR2 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the leading lepton in the validation region VR3 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the sub-leading lepton in the validation region VR3 showing both data points with statistical errors only and the expected standard model background.

Transverse momentum distribution of the 3rd-leading lepton in the validation region VR3 showing both data points with statistical errors only and the expected standard model background.

The efficiencies in the different signal regions across the MSSM Direct Gaugino grid of the Higgs mass parameter MU and gaugino massess M1 and M2.

The acceptance in the different signal regions across the MSSM Direct Gaugino grid of the Higgs mass parameter MU and gaugino massess M1 and M2.

The total absolute systematic uncertainty (in number of events) in the different signal regions, not including uncertainties from Monte Carlo statistics, across the MSSM Direct Gaugino grid of the Higgs mass parameter MU and gaugino massess M1 and M2.

The observed CL_s values in the different signal regions across the MSSM Direct Gaugino grid of the Higgs mass parameter MU and gaugino massess M1 and M2.

The cross-section across the MSSM Direct Gaugino grid of the Higgs mass parameter MU and gaugino massess M1 and M2.

The number of generated events across the MSSM Direct Gaugino grid of the Higgs mass parameter MU and gaugino massess M1 and M2.

The efficiencies in the different signal regions across the simplified models with and without intermediate sleptons.

The acceptance in the different signal regions across the simplified models with and without intermediate sleptons.

The total absolute systematic uncertainty (in number of events) in the different signal regions, not including uncertainties from Monte Carlo statistics, across the simplified models with and without intermediate sleptons.

The observed CL_s values in the different signal regions across the simplified models with and without intermediate sleptons.

The cross-section across the simplified models with and without intermediate sleptons.

The number of generated events across the simplified models with and without intermediate sleptons.

The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 20 - 30 %.

The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 30 - 40 %.

The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 40 - 50 %.

The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 50 - 60 %.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 38.36 - 44.21 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 44.21 - 50.94 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 50.94 - 58.70 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 58.70 - 67.64 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 67.64 - 77.94 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 77.94 - 89.81 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 89.81 - 103.5 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 103.5 - 119.3 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 119.3 - 137.4 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 137.4 - 158.3 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 158.3 - 182.5 GeV.

The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 182.5 - 210.3 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 38.36 - 44.21 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 38.36 - 44.21 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 44.21 - 50.94 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 44.21 - 50.94 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 50.94 - 58.70 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 50.94 - 58.70 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 58.70 - 67.64 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 58.70 - 67.64 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 67.64 - 77.94 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 67.64 - 77.94 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 77.94 - 89.81 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 77.94 - 89.81 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 89.81 - 103.5 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 89.81 - 103.5 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 103.5 - 119.3 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 103.5 - 119.3 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 119.3 - 137.4 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 119.3 - 137.4 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 137.4 - 158.3 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 137.4 - 158.3 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 158.3 - 182.5 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 158.3 - 182.5 GeV.

The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 182.5 - 210.3 GeV.

The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 182.5 - 210.3 GeV.

The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 0 - 10 %.

The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 10 - 20 %.

The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 20 - 30 %.

The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 30 - 40 %.

The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 40 - 50 %.

The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 50 - 60 %.

The covariance matrix for statistcal correlations for R = 0.2 and centrality range 0 - 10 %.

The covariance matrix for statistcal correlations for R = 0.3 and centrality range 0 - 10 %.

The covariance matrix for statistcal correlations for R = 0.4 and centrality range 0 - 10 %.

The covariance matrix for statistcal correlations for R = 0.5 and centrality range 0 - 10 %.

The covariance matrix for statistcal correlations for R = 0.2 and centrality range 10 - 20 %.

The covariance matrix for statistcal correlations for R = 0.3 and centrality range 10 - 20 %.

The covariance matrix for statistcal correlations for R = 0.4 and centrality range 10 - 20 %.

The covariance matrix for statistcal correlations for R = 0.5 and centrality range 10 - 20 %.

The covariance matrix for statistcal correlations for R = 0.2 and centrality range 20 - 30 %.

The covariance matrix for statistcal correlations for R = 0.3 and centrality range 20 - 30 %.

The covariance matrix for statistcal correlations for R = 0.4 and centrality range 20 - 30 %.

The covariance matrix for statistcal correlations for R = 0.5 and centrality range 20 - 30 %.

The covariance matrix for statistcal correlations for R = 0.2 and centrality range 30 - 40 %.

The covariance matrix for statistcal correlations for R = 0.3 and centrality range 30 - 40 %.

The covariance matrix for statistcal correlations for R = 0.4 and centrality range 30 - 40 %.

The covariance matrix for statistcal correlations for R = 0.5 and centrality range 30 - 40 %.

The covariance matrix for statistcal correlations for R = 0.2 and centrality range 40 - 50 %.

The covariance matrix for statistcal correlations for R = 0.3 and centrality range 40 - 50 %.

The covariance matrix for statistcal correlations for R = 0.4 and centrality range 40 - 50 %.

The covariance matrix for statistcal correlations for R = 0.5 and centrality range 40 - 50 %.

The covariance matrix for statistcal correlations for R = 0.2 and centrality range 50 - 60 %.

The covariance matrix for statistcal correlations for R = 0.3 and centrality range 50 - 60 %.

The covariance matrix for statistcal correlations for R = 0.4 and centrality range 50 - 60 %.

The covariance matrix for statistcal correlations for R = 0.5 and centrality range 50 - 60 %.

Transverse momentum distribution for the second leading lepton for events in the SR2 signal region for DATA and SM predictions.

Transverse momentum distribution for the third leading lepton for events in the SR1 signal region for DATA and SM predictions.

Transverse momentum distribution for the third leading lepton for events in the SR2 signal region for DATA and SM predictions.

Missing transverse energy for events in the SR1 signal region for DATA and SM predictions.

Missing transverse energy for events in the SR2 signal region for DATA and SM predictions.

Invariant mass of the same-flavour-opposite-sign (SFOS) lepton pair for events in the SR1 signal region for DATA and SM predictions.

The Cross Section in signal region SR1 for the SUSY pMSSM model with M1=100 GeV grid.

The Cross Section in signal region SR1 for the SUSY simplified model grid.

The Number of generated Events in signal region SR1 for the SUSY pMSSM model with M1=100 GeV grid.

The Number of generated Events in signal region SR1 for the SUSY simplified model grid.

The Efficiency in signal region SR1 for the SUSY pMSSM model with M1=100 GeV grid.

The Efficiency in signal region SR1 for the SUSY simplified model grid.

The Acceptance in signal region SR1 for the SUSY pMSSM model with M1=100 GeV grid.

The Acceptance in signal region SR1 for the SUSY simplified model grid.

The Acceptance*Efficiency in signal region SR1 for the SUSY pMSSM model with M1=100 GeV grid.

The Acceptance*Efficiency in signal region SR1 for the SUSY simplified model grid.

The Systematic Uncertainty of the data (excluding the Monte Carlo) in signal region SR1 for the SUSY pMSSM model with M1=100 GeV grid.

The Systematic Uncertainty of the data (excluding the Monte Carlo) in signal region SR1 for the SUSY simplified model grid.

CL values for the pMSSM with M1=100 GeV model grid for the SR1 signal region.

CL values for the simplified model model grid for the SR1 signal region.

Reconstructed distribution of the mass difference, DELTA(M), of the D*+- and its decay product (D0 PI+-) in different Z and PT bins.

Reconstructed distribution of the mass difference, DELTA(M), of the D*+- and its decay product (D0 PI+-) over the full Z and PT ranges.

Comparison of the reconstructed jet PT distribution with the reweighted Monte Carlo prediction.

Comparison of the reconstructed Z distribution with the reweighted Monte Carlo prediction.

The R ratios as a function of Z for D*+- jet production compared with various Monte Carlo predictions for the jet PT range 25-30 GeV.

The R ratios as a function of Z for D*+- jet production compared with various Monte Carlo predictions for the jet PT range 30-40 GeV.

The R ratios as a function of Z for D*+- jet production compared with various Monte Carlo predictions for the jet PT range 40-50 GeV.

The R ratios as a function of Z for D*+- jet production compared with various Monte Carlo predictions for the jet PT range 50-60 GeV.

The R ratios as a function of Z for D*+- jet production compared with various Monte Carlo predictions for the jet PT range 60-70 GeV.

The R ratios as a function of Z for D*+- jet production compared with various Monte Carlo predicitions for the jet PT range 25-70 GeV.

Comparisons of the D+- jet prodution rate over the PT and Z range with the POWHEG+PYTHIA predictions, showing also the c- and b- fractions.

Comparisons of the D+- jet prodution rate over the PT and Z range with the POWHEG+HERWIG predictions, showing also the c- and b- fractions.

The measured fraction of events, the gap fraction, surviving the veto cut of having no additional jets in the |rapidity| interval < 2.1 having a transverse momentum greater than Q, as a function of Q.

The measured fraction of events, the gap fraction, surviving the veto cut of having no events with the scalar sum of the transverse momentum of additional jets in the |rapidity| interval < 0.8 greater than Q, as a function of Q.

The measured fraction of events, the gap fraction, surviving the veto cut of having no events with the scalar sum of the transverse momentum of additional jets in the |rapidity| interval 0.8-1.5 greater than Q, as a function of Q.

The measured fraction of events, the gap fraction, surviving the veto cut of having no events with the scalar sum of the transverse momentum of additional jets in the |rapidity| interval 1.5-2.1 greater than Q, as a function of Q.

The measured fraction of events, the gap fraction, surviving the veto cut of having no events with the scalar sum of the transverse momentum of additional jets in the |rapidity| interval < 2.1 greater than Q, as a function of Q.

The correlation matrix (statistical) for the gap fraction measurement at different values of Q0 for the absolute rapditiy interval < 0.8.

The correlation matrix (statistical) for the gap fraction measurement at different values of Q0 for the absolute rapditiy interval 0.8 TO 1.5.

The correlation matrix (statistical) for the gap fraction measurement at different values of Q0 for the absolute rapditiy interval 1.5 TO 2.1.

The correlation matrix (statistical) for the gap fraction measurement at different values of Q0 for the absolute rapditiy interval < 2.1.

The correlation matrix (statistical) for the gap fraction measurement at different values of Qsum for the absolute rapditiy interval < 0.8.

The correlation matrix (statistical) for the gap fraction measurement at different values of Qsum for the absolute rapditiy interval 0.8 TO 1.5.

The correlation matrix (statistical) for the gap fraction measurement at different values of Qsum for the absolute rapditiy interval 1.5 TO 2.1.

The correlation matrix (statistical) for the gap fraction measurement at different values of Qsum for the absolute rapditiy interval < 2.1.

Observed and predicted jet multiplicity distribution for jets with PT > 55 Gev in the ET(C=MISSING)/SQRT(HT) region 2-3 GeV.

Observed and predicted jet multiplicity distribution for jets with PT > 80 Gev in the ET(C=MISSING)/SQRT(HT) region 1.5-2 GeV.

Observed and predicted jet multiplicity distribution for jets with PT > 80 Gev in the ET(C=MISSING)/SQRT(HT) region 2-3 GeV.

Observed and predicted jet multiplicity distribution for jets with PT > 55 Gev in the Top Control Region.

Observed and predicted jet multiplicity distribution for jets with PT > 80 Gev in the Top Control Region.

Observed and predicted jet multiplicity distribution for jets with PT > 55 Gev in the W Control Region.

Observed and predicted jet multiplicity distribution for jets with PT > 80 Gev in the W Control Region.

Observed and predicted jet multiplicity distribution for jets with PT > 55 Gev in the Z Control Region.

Observed and predicted jet multiplicity distribution for jets with PT > 80 Gev in the Z Control Region.

Observed and predicted distributions of the variable ET(C=MISSING)/SQRT(HT) for events with 7 ot more jets each having PT > 55 GeV.

Observed and predicted distributions of the variable ET(C=MISSING)/SQRT(HT) for events with 6 ot more jets each having PT > 80 GeV.

Observed and predicted distributions of the variable ET(C=MISSING)/SQRT(HT) for events with 8 ot more jets each having PT > 55 GeV.

Observed and predicted distributions of the variable ET(C=MISSING)/SQRT(HT) for events with 7 ot more jets each having PT > 80 GeV.

Observed and predicted jet multiplicity distribution for jets with PT > 55 Gev in the ET(C=MISSING)/SQRT(HT) region > 3 GeV.

Observed and predicted jet multiplicity distribution for jets with PT > 80 Gev in the ET(C=MISSING)/SQRT(HT) region > 3 GeV.

The distribution in Meff for the higher jet Pt cut (> 80 GeV) (scalar sum of the missing transverse momentum and the transverse momenta of all jets with pT > 40 GeV) for events with at least 4 jets after the application of all selection criteria (other than the Meff cut itself). The table shows the number of observed data points per 100 GeV bin plus the background prediction of the Standard-Model Monte-Carlo and its upper and lower 1-sigma error limits uncertainty band.

95% CL exclusion limit in the (Mgluino,Msquark) plane for the simplified model described in the paper. The gluino mass and the masses of the squarks of the first two generations are set to the values shown. The lightest neutralino is assigned mass of zero. All other supersymmetric particles, including the squarks of the third generation, are decoupled by being given masses of 5 TeV.

95% CL exclusion limit in the Squark-Gluino model, as in the previous table, but for a lightest neutralino assigned mass of 195 GeV.

95% CL exclusion limit in the Squark-Gluino model, as in the previous table, but for a lightest neutralino assigned mass of 395 GeV.

95% CL exclusion limit in M(0) and M(1/2) in the tan(beta)=10, A0=0, MU>0 slice of MSUGRA/CMSSM.

95% CL exclusion limit in the Universal Extra Dimensions model in 1/R v Lambda*R space.

95% CL exclusion limit in the Universal Extra Dimensions model in m_{g_KK} vs (m_{g_KK}-m_{gamma_KK}) space.

Distribution of the missing ET for data and the SM expectation in the one-lepton plus 2 jet channel.

Observed 95 PCT exclusion limit in the M(gluino), M(sbottom) plane obtained with the zero-lepton channel data.

Expected 95 PCT exclusion limit in the M(gluino), M(sbottom) plane obtained with the zero-lepton channel data.

Observed and expected 95 PCT CL upper limits on the gluino-mediated and stop pair production cross section as a function of the gluino mass for a stop mass od 180 GeV, for the one-lepton analysis.

Observed and expected 95 PCT CL upper limits on the gluino-mediated and stop pair production cross section as a function of the gluino mass for a stop mass od 210 GeV, for the one-lepton analysis.

Observed 95 PCT CL exclusion limits from the zero-lepton analysis on the MSUGRA/CMSSM scenario with tan(beta) = 40, A0 = 0 and MU > 0.

Expected 95 PCT CL exclusion limits from the zero-lepton analysis on the MSUGRA/CMSSM scenario with tan(beta) = 40, A0 = 0 and MU > 0.

Observed 95 PCT CL exclusion limits from the one-lepton analysis on the MSUGRA/CMSSM scenario with tan(beta) = 40, A0 = 0 and MU > 0.

Expected 95 PCT CL exclusion limits from the one-lepton analysis on the MSUGRA/CMSSM scenario with tan(beta) = 40, A0 = 0 and MU > 0.

Observed 95 PCT CL exclusion limits from the combined zero and one-lepton analyses on the MSUGRA/CMSSM scenario with tan(beta) = 40, A0 = 0 and MU > 0.

Expected 95 PCT CL exclusion limits from the combined zero and one-lepton analyses on the MSUGRA/CMSSM scenario with tan(beta) = 40, A0 = 0 and MU > 0.

The distribution in missing ET transverse momentum for events with at least 2 jets after the application of all the >=2 jet preselection cuts described in the paper. The table shows the number of observed data points per 50 GeV bin plus the background prediction of the Standard-Model Monte-Carlo and its upper and lower 1-sigma uncertainty band error limits.

95% CL exclusion limit in the (Mgluino,Msquark) plane for the simplified model described in the paper. The gluino mass and the masses of the squarks of the first two generations are set to the values shown. The lightest neutralino is assigned mass of zero. All other supersymmetric particles, including the squarks of the third generation, are decoupled by being given masses of 5 TeV.

95% CL exclusion limit in M(0) and M(1/2) in the tan(beta)=3, A0=0, MU>0 slice of MSUGRA/CMSSM.

95 PCT confidence lower limits to M(1/2).

CHI distribution for mass bin > 1200 GeV.

Centrality Ratio.

The proton plus antiproton fraction and differential production rate per hadronic Z0 decay.

Differential production rates of charged pions per Z0 decay into light (u,d,s) and c and b quarks. The errors are combined statistical and systematic.

Differential production rates of charged kaons per Z0 decay into light (u,d,s) and c and b quarks. The errors are combined statistical and systematic.

Differential production rates of charged protons plus antiprotons per Z0 decay into light (u,d,s) and c and b quarks. The errors are combined statistical and systematic.

Differential production rates of stable charged particles per Z0 decay intolight (u,d,s) and c and b quarks. The errors are combined statistical and syste matic.

Differential production rate for positive and negative charged pions into light quark jets from hadronic Z0 decays. Also shown are the normalization differences. The ratios are defined as:-. R(Q=PI+)=(1/2N(Q=Z0))*D(N(QUARK --> PI+) + N(QUARKBAR --> PI-))/DX. R(Q=PI-)=(1/2N(Q=Z0))*D(N(QUARK --> PI-) + N(QUARKBAR --> PI+))/DX.

Differential production rate for positive and negative charged kaons into light quark jets from hadronic Z0 decays. Also shown are the normalization differences. The ratios are defined as:-. R(Q=K+)=(1/2N(Q=Z0))*D(N(QUARK --> K+) + N(QUARKBAR --> K-))/DX. R(Q=K-)=(1/2N(Q=Z0))*D(N(QUARK --> K-) + N(QUARKBAR --> K+))/DX.

Differential production rate for positive and negative protons into light quark jets from hadronic Z0 decays. Also shown are the normalization differences.The ratios are defined as:-. R(Q=P+)=(1/2N(Q=Z0))*D(N(QUARK --> P+) + N(QUARKBAR --> PBAR))/DX. R(Q=PBAR)=(1/2N(Q=Z0))*D(N(QUARK --> PBAR) + N(QUARKBAR --> P+))/DX.

Measured angular distribution of the Lambda-Lambdabar pairs in all hadron events. Statistical errors only are given but the systematic errors are negigible. Data are read from the plot.

Measured rapidity difference os the Lambda and Lambdabars in the Lambda-Lambdabar pairs in all hadron events. Statistical errors only are given but the systematic errors are negigible. Data are read from the plot.

Scaled energy distribution of charged hadrons produced in Gluon jets in 'Mercedes' topology 3-JET events.

Subjet multiplicity-1 as a function of the jet resolution parameter ycut for Quark jets in 'Y' topology events.

Subjet multiplicity-1 as a function of the jet resolution parameter ycut for Gluon jets in 'Y' topology events.

Ratio of the sub-jet multiplicity-1 for gluon jets to the sub-jet multiplicity-1 for quark jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Total 1-jet rate for Quark jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Total 1-jet rate for Gluon jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Differential 1-jet rate for Quark jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Differential 1-jet rate for Gluon jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Splitting Function for Quark jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Splitting Function for Gluon jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Ratio of Splitting Functions for Gluon jets and Quark jets as a function ofthe jet resolution parameter ycut in 'Y' topology events.

Integral of event shape distribution over the specified interval.

Integral of event shape distribution over the specified interval.

Integral of event shape distribution over the specified interval.

Inclusive charged particle distributions, corrected to final state charged particles.

Rapidity, YS, w.r.t. Sphericity axis distribution. Axis definition is from corrected charged plus neutral particles.

Transverse momentum PTIN w.r.t. the Thrust axis. Axis definition is from corrected charged plus neutral particles.

Transverse momentum PTOUT w.r.t. the Thrust axis. Axis definition is from corrected charged plus neutral particles.

1-Thrust distribution. Axis definition is from corrected charged plus neutral particles.

Thrust Major distribution. Axis definition is from corrected charged plus neutral particles.

Thrust Minor distribution. Axis definition is from corrected charged plus neutral particles.

Oblateness distribution. Axis definition is from corrected charged plus neutral particles.

Wide Hemisphere Broadening, DBMAX. Axis definition is from charged corrected plus neutral particles.

Narrow Hemisphere Broadening, DBMIN. Axis definition is from charged corrected plus neutral particles.

Total Hemisphere Broadening, DBSUM. Axis definition is from charged corrected plus neutral particles.

Difference of the Hemisphere Broadening, DBDIFF. Axis definition is from charged corrected plus neutral particles.

2-jet rate for the Durham Algorithm.

3-jet rate for the Durham Algorithm.

4-jet rate for the Durham Algorithm.

5-jet rate for the Durham Algorithm.

2-jet rate for the Jade Algorithm.

3-jet rate for the Jade Algorithm.

4-jet rate for the Jade Algorithm.

5-jet rate for the Jade Algorithm.

Data corrected for finite acceptance and resolution of the detector and for intial state photon radiation. No corrections for hadronic effects are applied.. Errors include statistical and systematic uncertainties, added in quadrature.

Data corrected for finite acceptance and resolution of the detector and for intial state photon radiation. No corrections for hadronic effects are applied.. Errors include statistical and systematic uncertainties, added in quadrature.

Data corrected for finite acceptance and resolution of the detector and for intial state photon radiation. No corrections for hadronic effects are applied.. Errors include statistical and systematic uncertainties, added in quadrature.. YCUT is the cut off value used to define the jets in this case using the 'Durham' scheme.

Data corrected for finite acceptance and resolution of the detector and for intial state photon radiation. No corrections for hadronic effects are applied.. Errors include statistical and systematic uncertainties, added in quadrature.. YCUT is the cut off value used to define the jets in this case using the 'Durham' scheme.. D2 is the differential jet rate.

The scattering angle in the 4-jet centre-of-mass frame after all other cuts.

Number of events as a function of the average mass of the reconstructed dijet pairs for jet masses > 55 GeV.

Number of events as a function of the average mass of the reconstructed dijet pairs for jet masses > 77 GeV.

Number of events as a function of the average mass of the reconstructed dijet pairs for jet masses > 88 GeV.

Number of events as a function of the average mass of the reconstructed dijet pairs for jet masses > 104 GeV.

The observed 95% CL upper bounds on scalar pair production cross-section as a function of the scalar particle mass.