Kinematic distributions of single l + > 5-jet events in data (points), compared to MC simulation normalized to the number of events observed in data. Shown are pT spectra for muons (a) and electrons (b), and jet spectra for the channels $\mu$+jets (c) and e+jets (d). The reconstructed mtg distribution is shown for the $\mu$+jets channel in (e) and for e+jets in (f).

Kinematic distributions of single l + > 5-jet events in data (points), compared to MC simulation normalized to the number of events observed in data. Shown are pT spectra for muons (a) and electrons (b), and jet spectra for the channels $\mu$+jets (c) and e+jets (d). The reconstructed mtg distribution is shown for the $\mu$+jets channel in (e) and for e+jets in (f).

Kinematic distributions of single l + > 5-jet events in data (points), compared to MC simulation normalized to the number of events observed in data. Shown are pT spectra for muons (a) and electrons (b), and jet spectra for the channels $\mu$+jets (c) and e+jets (d). The reconstructed mtg distribution is shown for the $\mu$+jets channel in (e) and for e+jets in (f).

Reconstructed mass spectrum for the $tg$ system in data (points), along with a fit of the background $f(m)$ to the data in the $\mu$+jets channel (a) and $e$+jets channel (b). The reconstructed masses correspond to the results of kinematic fits for the jet-quark assignments that provide the best match to the $t^{*}\bar{t}^{*}$ hypothesis. Also shown are the expectations of $t^*$ signals for $m_{t^*}=750$ and 850 GeV normalized to the integrated luminosity of the data. Information about the fit: F = 501885/(1+exp((x+251.828)/112.311)) where x = $M_{tg}$.

Reconstructed mass spectrum for the $tg$ system in data (points), along with a fit of the background $f(m)$ to the data in the $\mu$+jets channel (a) and $e$+jets channel (b). The reconstructed masses correspond to the results of kinematic fits for the jet-quark assignments that provide the best match to the $t^{*}\bar{t}^{*}$ hypothesis. Also shown are the expectations of $t^*$ signals for $m_{t^*}=750$ and 850 GeV normalized to the integrated luminosity of the data. Information about the fit: F = 62101.5/(1+exp((x+6.58811)/107.886)) where x = $M_{tg}$.

The observed (solid line) and expected (dashed line) 95%CL upper limits for the product of the inclusive $t^{*}\bar{t}^{*}$ production cross section and the branching fraction $B(t^{*}{\rightarrow}tg)$, as a function of the $t^{*}$ mass, for the combined lepton data. The ranges for ${\pm}1$ and ${\pm}2$ standard deviations for the expected limits are shown by the bands.

The leptonic asymmetry dependence on the invariant mass of top-antitop system ($m_{t\bar{t}}$) in the fiducial volume.

The leptonic asymmetry dependence on the longitudinal boost of the top-antitop system ($\beta_z^{t\bar{t}}$) in the fiducial volume.

The leptonic asymmetry dependence on the transverse momentum of the top-antitop system ($p_T^{t\bar{t}}$) in the fiducial volume.

The top-antitop inclusive asymmetry in the fiducial volume.

The top-antitop asymmetry dependence on the invariant mass of top-antitop system ($m_{t\bar{t}}$) in the fiducial volume.

The top-antitop asymmetry dependence on the longitudinal boost of the top-antitop system ($\beta_z^{t\bar{t}}$) in the fiducial volume.

The top-antitop asymmetry dependence on the transverse momentum of the top-antitop system ($p_T^{t\bar{t}}$) in the fiducial volume.

The measured fiducial cross sections are corrected to the dressed level. The ratio of $C_{WZ}^{\textrm{dressed}}/C_{WZ}^{\textrm{Born}}$ factors presented in this table can be used to correct fiducial integrated cross sections from dressed to Born level.

Cross section extrapolated to total phase space and all W and Z boson decays. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the theory uncertainty and the third is the luminosity uncertainty.

The total cross section is measured at dressed level and can also be corrected to Born level use this acceptance correction factor.

Ratio of fiducial cross sections measured for $W^{+} Z$ and $W^{-} Z$ production. The first systematic uncertainty is the combined systematic uncertainty excluding the luminosity uncertainty, the second is the luminosity uncertainty.

Observed and expected upper limits at $95\%$ CL in fb on the fiducial cross section $\sigma^{\mathrm{fid.}}_{W^{\pm} Zjj \textrm{-EW} \rightarrow \ell^{'} \nu \ell \ell}$, multiplied by the $W$ and $Z$ branching ratios in a single leptonic channel with muons or electrons in the VBS fiducial phase space. Values obtained with or without subtraction of the $tZj$ contribution are presented. The $1$ $\sigma$ and $2$ $\sigma$ uncertainty intervals around the expected limits are also indicated.

Observed and expected upper limits at $95\%$ CL in fb on the fiducial cross section $\sigma^{\mathrm{fid.}}_{W^{\pm} Zjj \textrm{-EW} \rightarrow \ell^{'} \nu \ell \ell}$, multiplied by the $W$ and $Z$ branching ratios in a single leptonic channel with muons or electrons in the aQGC fiducial phase space. Values obtained with or without subtraction of the $tZj$ contribution are presented. The $1$ $\sigma$ and $2$ $\sigma$ uncertainty intervals around the expected limits are also indicated.

Expected and observed one-dimensional 95% Confidence Level intervals on the anomalous couplings parameters. Anomalous couplings are introduced as form factors using a cut-off scale $\Lambda_{\mathrm{co}}$.

Expected and observed one-dimensional intervals at 95% Confidence Level on the Effective Field Theory (EFT) parameters.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Measured normalised fiducial cross section in all $\ell'^\pm \nu \ell^+ \ell^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding theory and luminosity uncertainties, the second is the luminosity uncertainty. The last bin is a cross section for all events above the lower end of the bin.

Ratio of $W^{+}Z$ over $W^{-}Z$ differential fiducial cross sections measured in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The last bin is a cross section for all events above the lower end of the bin.

Ratio of $W^{+}Z$ over $W^{-}Z$ differential fiducial cross sections measured in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The last bin is a cross section for all events above the lower end of the bin.

Ratio of $W^{+}Z$ over $W^{-}Z$ differential fiducial cross sections measured in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The last bin is a cross section for all events above the lower end of the bin.

Ratio of $W^{+}Z$ over $W^{-}Z$ differential fiducial cross sections measured in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The last bin is a cross section for all events above the lower end of the bin.

Ratio of $W^{+}Z$ over $W^{-}Z$ differential fiducial cross sections measured in all $\ell'^\pm \nu \ell^+ \ell'^-$ channels combined, where $\ell, \ell' = e, \mu$.

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.

Vertex-level efficiency if no re-tracking is performed, as a function of the vertex radial position for an RPV SUSY model of squark production with $\tilde{q}\to q[\tilde{\chi}_1^0\to\mu qq]$, where $m(\tilde{q}) = 700$ GeV, $m(\tilde{\chi}_1^0) = 494$ GeV and $c\tau(\tilde{\chi}_1^0)$ = 175 mm. The result with re-tracking is tabulated in http://hepdata.cedar.ac.uk/view/ins1362183/d1.

Upper limits (95% CL) on the number of DV+muon displaced vertices in 20.3 fb$^{-1}$ and the corresponding vertex-level efficiencies (from Auxiliary Figure 7a) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider squark or gluino pair production, with masses in GeV as indicated, with either $\tilde{q}\to q[\tilde{\chi}_1^0\to\mu qq]$ or $\tilde{g}\to qq[\tilde{\chi}_1^0\to\mu qq]$ decays, respectively.

Upper limits (95% CL) on the number of DV+muon displaced vertices in 20.3 fb$^{-1}$ and the corresponding vertex-level efficiencies (from Auxiliary Figure 7b) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider squark or gluino pair production, with masses in GeV as indicated, with either $\tilde{q}\to q\tilde{\chi}_1^0$ or $\tilde{g}\to qq\tilde{\chi}_1^0$ decays, respectively.

Upper limits (95% CL) on the number of DV+electron displaced vertices in 20.3 fb$^{-1}$ and the corresponding vertex-level efficiencies (from Auxiliary Figure 7c) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider squark or gluino pair production, with masses in GeV as indicated, with either $\tilde{q}\to q[\tilde{\chi}_1^0\to e qq]$ or $\tilde{g}\to qq[\tilde{\chi}_1^0\to e qq]$ decays, respectively.

Upper limits (95% CL) on the number of DV+electron displaced vertices in 20.3 fb$^{-1}$ and the corresponding vertex-level efficiencies (from Auxiliary Figure 7d) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider squark or gluino pair production, with masses in GeV as indicated, with either $\tilde{q}\to q\tilde{\chi}_1^0$ or $\tilde{g}\to qq\tilde{\chi}_1^0$ decays, respectively.

Upper limits (95% CL) on the number of dilepton $e^+e^-$ displaced vertices in 20.3 fb$^{-1}$ and the corresponding vertex-level efficiencies (from Auxiliary Figure 5a) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to ee\nu]$ decays and masses in GeV as indicated. A dash indicates results omitted due to limited statistical precision.

Upper limits (95% CL) on the number of dilepton $e^{\pm}\mu^{\mp}$ displaced vertices in 20.3 fb$^{-1}$ and the corresponding vertex-level efficiencies (from Auxiliary Figure 5b) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to e\mu\nu]$ decays and masses in GeV as indicated.

Upper limits (95% CL) on the number of $\mu^+\mu^-$ displaced vertices in 20.3 fb$^{-1}$ and the corresponding vertex-level efficiencies (from Auxiliary Figure 5c) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to \mu\mu\nu]$ decays and masses in GeV as indicated. A dash indicates results omitted due to limited statistical precision.

Upper limits (95% CL) on the number of dilepton ($e^+e^-+e^{\pm}\mu^{\mp}+\mu^+\mu^-$) displaced vertices in 20.3 fb$^{-1}$ and the corresponding vertex-level efficiencies (from Auxiliary Figure 5d) for two GGM SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to Z\tilde{G}]$ decays, $m(\tilde{g})$ = 1100 GeV and $m(\tilde{\chi}_1^0)$ = 400 GeV.

Upper limits (95% CL) on the number of dilepton ($e^+e^-+e^{\pm}\mu^{\mp}+\mu^+\mu^-$) displaced vertices in 20.3 fb$^{-1}$ and the corresponding vertex-level efficiencies (from Auxiliary Figure 5d) for two GGM SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to Z\tilde{G}]$ decays, $m(\tilde{g})$ = 1100 GeV and $m(\tilde{\chi}_1^0)$ = 1000 GeV.

Upper limits (95% CL) from the dilepton $e^+e^-+e^{\pm}\mu^{\mp}$ channels on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 6a) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to e\mu\nu/ee\nu]$ decays and masses in GeV as indicated. For comparison, the production cross-sections for $m(\tilde{g})$ = 600 GeV and 1300 GeV are $1280\pm230$ fb and $1.7\pm0.7$ fb, respectively.

Upper limits (95% CL) from the dilepton $e^{\pm}\mu^{\mp}+\mu^+\mu^-$ channels on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 6b) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to e\mu\nu/\mu\mu\nu]$ decays and masses in GeV as indicated. For comparison, the production cross-sections for $m(\tilde{g})$ = 600 GeV and 1300 GeV are $1280\pm230$ fb and $1.7\pm0.7$ fb, respectively. A dash indicates results omitted due to limited statistical precision.

Upper limits (95% CL) from the dilepton $e^+e^-+e^{\pm}\mu^{\mp}+\mu^+\mu^-$ channels on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 6c) for two GGM SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to Z\tilde{G}]$ decays, $m(\tilde{g})$ = 1100 GeV and $m(\tilde{\chi}_1^0)$ = 400 GeV. For comparison, the production cross-section for $m(\tilde{g})$ = 1100 GeV is $7.6\pm2.8$ fb.

Upper limits (95% CL) from the dilepton $e^+e^-+e^{\pm}\mu^{\mp}+\mu^+\mu^-$ channels on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 6c) for two GGM SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to Z\tilde{G}]$ decays, $m(\tilde{g})$ = 1100 GeV and $m(\tilde{\chi}_1^0)$ = 1000 GeV. For comparison, the production cross-section for $m(\tilde{g})$ = 1100 GeV is $7.6\pm2.8$ fb.

Upper limits (95% CL) from the DV+jets channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 8a) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider squark pair production, with $\tilde{q}\to q\tilde{\chi}_1^0$ decays, $m(\tilde{q})$ = 700 GeV and $m(\tilde{\chi}_1^0)$ = 494 GeV. For comparison, the production cross-section for $m(\tilde{q})$ = 700 GeV is $124\pm17$ fb. A dash indicates where the limit-setting procedure did not converge.

Upper limits (95% CL) from the DV+jets channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 8b) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider squark pair production, with $\tilde{q}\to q\tilde{\chi}_1^0$ decays, $m(\tilde{q})$ = 1000 GeV and $m(\tilde{\chi}_1^0)$ = 108 GeV. For comparison, the production cross-section for $m(\tilde{q})$ = 1000 GeV is $11.9\pm1.5$ fb. A dash indicates where the limit-setting procedure did not converge.

Upper limits (95% CL) from the DV+$E_T^{miss}$ channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 9a) for two GGM SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to Z\tilde{G}]$ decays, $m(\tilde{g})$ = 1100 GeV and a $\tilde{\chi}_1^0$ mass in GeV as indicated. For comparison, the production cross-section for $m(\tilde{g})$ = 1100 GeV is $7.6\pm2.8$ fb.

Upper limits (95% CL) from the DV+jets channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 9b) for two GGM SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to Z\tilde{G}]$ decays, $m(\tilde{g})$ = 1100 GeV and a $\tilde{\chi}_1^0$ mass in GeV as indicated. For comparison, the production cross-section for $m(\tilde{g})$ = 1100 GeV is $7.6\pm2.8$ fb. A dash indicates where the limit-setting procedure did not converge.

Upper limits (95% CL) from the DV+$E_T^{miss}$ channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 10a) for four split-SUSY models as a function of the $\tilde{g}$ proper decay distance $c\tau$. The models consider gluino pair production, with $[\tilde{g}\to g/qq \tilde{\chi}_1^0]$ decays, $\tilde{g}$ masses in GeV as indicated and $m(\tilde{\chi}_1^0)$ = 100 GeV. For comparison, the production cross-sections for $m(\tilde{g})$ = 400 GeV, 800 GeV and 1400 GeV are $18700\pm2800$ fb, $149\pm31$ fb and $0.71\pm0.32$ fb, respectively.

Upper limits (95% CL) from the DV+jets channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 10b) for four split-SUSY models as a function of the $\tilde{g}$ proper decay distance $c\tau$. The models consider gluino pair production, with $[\tilde{g}\to g/qq \tilde{\chi}_1^0]$ decays, $\tilde{g}$ masses in GeV as indicated and $m(\tilde{\chi}_1^0)$ = 100 GeV. For comparison, the production cross-sections for $m(\tilde{g})$ = 400 GeV, 800 GeV and 1400 GeV are $18700\pm2800$ fb, $149\pm31$ fb and $0.71\pm0.32$ fb, respectively. A dash indicates where the limit-setting procedure did not converge or the limit is greater than $10^8$ fb.

Upper limits (95% CL) from the DV+$E_T^{miss}$ channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 10c) for three split-SUSY models as a function of the $\tilde{g}$ proper decay distance $c\tau$. The models consider gluino pair production, with $[\tilde{g}\to tt \tilde{\chi}_1^0]$ decays, $\tilde{g}$ masses in GeV as indicated and $m(\tilde{\chi}_1^0)$ = 100 GeV. For comparison, the production cross-sections for $m(\tilde{g})$ = 600 GeV, 1000 GeV and 1400 GeV are $1270\pm230$ fb, $22\pm6$ fb and $0.71\pm0.32$ fb, respectively.

Upper limits (95% CL) from the DV+jets channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 10d) for three split-SUSY models as a function of the $\tilde{g}$ proper decay distance $c\tau$. The models consider gluino pair production, with $[\tilde{g}\to tt \tilde{\chi}_1^0]$ decays, $\tilde{g}$ masses in GeV as indicated and $m(\tilde{\chi}_1^0)$ = 100 GeV. For comparison, the production cross-sections for $m(\tilde{g})$ = 600 GeV, 1000 GeV and 1400 GeV are $1270\pm230$ fb, $22\pm6$ fb and $0.71\pm0.32$ fb, respectively. A dash indicates where the limit-setting procedure did not converge.

Upper limits (95% CL) from the DV+$E_T^{miss}$ channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 10e) for four split-SUSY models as a function of the $\tilde{g}$ proper decay distance $c\tau$. The models consider gluino pair production, with $[\tilde{g}\to tt \tilde{\chi}_1^0]$ decays, $\tilde{g}$ masses in GeV as indicated and $m(\tilde{\chi}_1^0)$ = $m(\tilde{g}) - 480$ GeV. For comparison, the production cross-sections for $m(\tilde{g})$ = 500 GeV, 800 GeV and 1400 GeV are $4450\pm700$ fb, $149\pm31$ fb and $0.71\pm0.32$ fb, respectively.

Upper limits (95% CL) from the DV+jets channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 10f) for four split-SUSY models as a function of the $\tilde{g}$ proper decay distance $c\tau$. The models consider gluino pair production, with $[\tilde{g}\to tt \tilde{\chi}_1^0]$ decays, $\tilde{g}$ masses in GeV as indicated and $m(\tilde{\chi}_1^0)$ = $m(\tilde{g}) - 480$ GeV. For comparison, the production cross-sections for $m(\tilde{g})$ = 500 GeV, 800 GeV and 1400 GeV are $4450\pm700$ fb, $149\pm31$ fb and $0.71\pm0.32$ fb, respectively. A dash indicates where the limit-setting procedure did not converge.

Observed 95% CL exclusion contour in the $m(\tilde{g})$-$c\tau$ plane for the split-SUSY model with gluino production, $[\tilde{g}\to g/qq \tilde{\chi}_1^0]$ decays and $m(\tilde{\chi}_1^0)$ = 100 GeV. These results are obtained from the DV+$E_T^{miss}$ and DV+jets channels, see http://hepdata.cedar.ac.uk/view/ins1362183/d34 for details.

Expected 95% CL exclusion contour in the $m(\tilde{g})$-$c\tau$ plane for the split-SUSY model with gluino production, $[\tilde{g}\to g/qq \tilde{\chi}_1^0]$ decays and $m(\tilde{\chi}_1^0)$ = 100 GeV. These results are obtained from the DV+$E_T^{miss}$ and DV+jets channels, see http://hepdata.cedar.ac.uk/view/ins1362183/d34 for details.

Observed 95% CL exclusion contour in the $m(\tilde{g})$-$c\tau$ plane for the split-SUSY model with gluino production, $[\tilde{g}\to tt \tilde{\chi}_1^0]$ decays and $m(\tilde{\chi}_1^0)$ = 100 GeV. These results are obtained from the DV+$E_T^{miss}$ and DV+jets channels, see http://hepdata.cedar.ac.uk/view/ins1362183/d34 for details.

Expected 95% CL exclusion contour in the $m(\tilde{g})$-$c\tau$ plane for the split-SUSY model with gluino production, $[\tilde{g}\to tt \tilde{\chi}_1^0]$ decays and $m(\tilde{\chi}_1^0)$ = 100 GeV. These results are obtained from the DV+$E_T^{miss}$ and DV+jets channels, see http://hepdata.cedar.ac.uk/view/ins1362183/d34 for details.

Observed 95% CL exclusion contour in the $m(\tilde{g})$-$c\tau$ plane for the split-SUSY model with gluino production, $[\tilde{g}\to g/qq \tilde{\chi}_1^0]$ decays and $m(\tilde{\chi}_1^0)$ = $m(\tilde{g})$ - 480 GeV. These results are obtained from the DV+$E_T^{miss}$ and DV+jets channels, see http://hepdata.cedar.ac.uk/view/ins1362183/d34 for details.

Expected 95% CL exclusion contour in the $m(\tilde{g})$-$c\tau$ plane for the split-SUSY model with gluino production, $[\tilde{g}\to g/qq \tilde{\chi}_1^0]$ decays and $m(\tilde{\chi}_1^0)$ = $m(\tilde{g})$ - 480 GeV. These results are obtained from the DV+$E_T^{miss}$ and DV+jets channels, see http://hepdata.cedar.ac.uk/view/ins1362183/d34 for details.

Upper limits (95% CL) from the DV+$E_T^{miss}$ channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 11a) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider squark or gluino pair production, with masses in GeV as indicated, with either $\tilde{q}\to q[\tilde{\chi}_1^0\to \nu qq]$ or $\tilde{g}\to qq[\tilde{\chi}_1^0\to \nu qq]$ decays, respectively. For comparison, the production cross-sections for $m(\tilde{g})$ = 700 GeV, $m(\tilde{q})$ = 700 GeV and $m(\tilde{q})$ = 1000 GeV are $430\pm80$ fb, $124\pm17$ fb and $11.9\pm1.5$ fb, respectively.

Upper limits (95% CL) from the DV+$E_T^{miss}$ channel on the production cross-section and the corresponding event-level efficiencies (from Auxiliary Figure 11b) for four RPV SUSY models as a function of the $\tilde{\chi}_1^0$ proper decay distance $c\tau$. The models consider squark pair production, with $\tilde{q}\to q\tilde{\chi}_1^0$ decays and masses in GeV as indicated. For comparison, the production cross-sections for $m(\tilde{q})$ = 700 GeV and 1000 GeV are $124\pm17$ fb and $11.9\pm1.5$ fb, respectively.

Vertex mass distributions in data and one RPV SUSY signal model, for vertices with 3, 4 and $\geq$5 tracks in the DV+muon channel. The entries are the number of DVs in each bin, not normalized according to bin size. The signal model is for squark pair production, with $\tilde{q}\to q[\tilde{\chi}_1^0\to\mu qq]$ decays, $m(\tilde{q})$ = 700 GeV, $m(\tilde{\chi}_1^0)$ = 494 GeV and $c\tau(\tilde{\chi}_1^0)$ = 175 mm.

Vertex mass distributions in data and one GGM SUSY signal model, for vertices with 3, 4 and $\geq$5 tracks in the DV+jets channel. The entries are the number of DVs in each bin, not normalized according to bin size. The signal model is for gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to Z\tilde{G}]$ decays, $m(\tilde{g})$ = 1100 GeV, $m(\tilde{\chi}_1^0)$ = 400 GeV and $c\tau(\tilde{\chi}_1^0)$ = 175 mm.

Vertex mass distributions in data and one RPV SUSY signal model, for vertices with 3, 4 and $\geq$5 tracks in the DV+electron channel. The entries are the number of DVs in each bin, not normalized according to bin size. The signal model is for squark pair production, with $\tilde{q}\to q[\tilde{\chi}_1^0\to e qq]$ decays, $m(\tilde{q})$ = 700 GeV, $m(\tilde{\chi}_1^0)$ = 494 GeV and $c\tau(\tilde{\chi}_1^0)$ = 175 mm.

Vertex mass distributions in data and one split-SUSY signal model, for vertices with 3, 4 and $\geq$5 tracks in the DV+$E_T^{miss}$ channel. The entries are the number of DVs in each bin, not normalized according to bin size. The signal model is for gluino pair production, with $[\tilde{g}\to g/qq \tilde{\chi}_1^0]$ decays, $m(\tilde{g})$ = 1400 GeV, $m(\tilde{\chi}_1^0)$ = 100 GeV and $c\tau(\tilde{g})$ = 175 mm.

Vertex mass distributions in data and one RPV SUSY signal model, for vertices with 0, 1 and $\geq$2 charged leptons in the dilepton $e^+e^-$ channel. The entries are the number of DVs in each bin, not normalized according to bin size. The signal model is for gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to e\mu\nu/ee\nu]$ decays, $m(\tilde{g})$ = 1300 GeV, $m(\tilde{\chi}_1^0)$ = 50 GeV and $c\tau(\tilde{\chi}_1^0)$ = 30 mm.

Vertex mass distributions in data and one RPV SUSY signal model, for vertices with 0, 1 and $\geq$2 charged leptons in the dilepton $e^{\pm}\mu^{\mp}$ channel. The entries are the number of DVs in each bin, not normalized according to bin size. The signal model is for gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to e\mu\nu/ee\nu]$ decays, $m(\tilde{g})$ = 1300 GeV, $m(\tilde{\chi}_1^0)$ = 50 GeV and $c\tau(\tilde{\chi}_1^0)$ = 30 mm.

Vertex mass distributions in data and one RPV SUSY signal model, for vertices with 0, 1 and $\geq$2 charged leptons in the dilepton $\mu^+\mu^-$ channel. The entries are the number of DVs in each bin, not normalized according to bin size. The signal model is for gluino pair production, with $\tilde{g}\to qq[\tilde{\chi}_1^0\to e\mu\nu/\mu\mu\nu]$ decays, $m(\tilde{g})$ = 1300 GeV, $m(\tilde{\chi}_1^0)$ = 50 GeV and $c\tau(\tilde{\chi}_1^0)$ = 30 mm.

Numbers of events satisfying each selection criterion in turn for the DV+muon channel, using the model listed in http://hepdata.cedar.ac.uk/view/ins1362183/d44. The ''Filter and trigger'' line includes the requirements placed on the primary vertex.

Numbers of events satisfying each selection criterion in turn for the DV+electron channel, using the model listed in http://hepdata.cedar.ac.uk/view/ins1362183/d44. The ''Filter and trigger'' line includes the requirements placed on the primary vertex.

Numbers of events satisfying each selection criterion in turn for the DV+jets channel, using the model listed in http://hepdata.cedar.ac.uk/view/ins1362183/d44. The ''Filter and trigger'' line includes the requirements placed on the primary vertex.

Numbers of events satisfying each selection criterion in turn for the DV+$E_T^{miss}$ channel, using the model listed in http://hepdata.cedar.ac.uk/view/ins1362183/d44. The ''Filter and trigger'' line includes the requirements placed on the primary vertex.

Numbers of events satisfying each selection criterion in turn for the dilepton $e^+e^-$ channel, using the model listed in http://hepdata.cedar.ac.uk/view/ins1362183/d44. The ''Trigger'' line includes the event-level cosmic-muon veto and the requirements placed on the primary vertex, but not the offline filter selection. This is included in the ''Lepton reconstruction and DV match'' line, along with all other requirements placed on offline-reconstructed leptons. About 20,000 events of the full sample are analyzed, which contain an equal mixture of $\tilde{\chi}_1^0 \to e^{\pm}\mu^{\mp}\nu$ and $\tilde{\chi}_1^0 \to e^+e^-\nu$ decays.

Numbers of events satisfying each selection criterion in turn for the dilepton $e^{\pm}\mu^{\mp}$ channel, using the model listed in http://hepdata.cedar.ac.uk/view/ins1362183/d44. The ''Trigger'' line includes the event-level cosmic-muon veto and the requirements placed on the primary vertex, but not the offline filter selection. This is included in the ''Lepton reconstruction and DV match'' line, along with all other requirements placed on offline-reconstructed leptons. The sample contains about 50% $\tilde{\chi}_1^0 \to e^{\pm}\mu^{\mp}\nu$ decays, 25% $\tilde{\chi}_1^0 \to e^+e^-\nu$ and 25% $\tilde{\chi}_1^0 \to \mu^+\mu^-\nu$ decays.

Numbers of events satisfying each selection criterion in turn for the dilepton $\mu^+\mu^-$ channel, using the model listed in http://hepdata.cedar.ac.uk/view/ins1362183/d44. The ''Trigger'' line includes the event-level cosmic-muon veto and the requirements placed on the primary vertex, but not the offline filter selection. This is included in the ''Lepton reconstruction and DV match'' line, along with all other requirements placed on offline-reconstructed leptons. About 20,000 events of the full sample are analyzed, which contain an equal mixture of $\tilde{\chi}_1^0 \to e^{\pm}\mu^{\mp}\nu$ and $\tilde{\chi}_1^0 \to \mu^+\mu^-\nu$ decays.

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.

The $\gamma$ differential transverse momentum cross-section in an inclusive $\gamma+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ selection for central rapidities $\vert y_{\gamma} \vert > 1.4$.

The Z boson differential transverse momentum cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ over $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq1$ selection.

The $\gamma$ boson differential transverse momentum cross-section in an inclusive $\gamma+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ over $Z+\mathrm{jets}$, $N_{\mathrm{jets}} \geq1$ selection for central rapidities $\vert y_{\gamma} \vert < 1.4$.

The Z boson differential transverse momentum over $H_{\mathrm{T}}$ cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ selection.

The Z boson differential transverse momentum over $H_{\mathrm{T}}$ cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq3$ selection.

The log (base 10) of the Z boson differential transverse momentum over the leading jet transverse momentum cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq2$ selection.

The log (base 10) of the Z boson differential transverse momentum over the leading jet transverse momentum cross-section in an inclusive $Z/\gamma^{*}+\mathrm{jets}$, $N_{\mathrm{jets}} \geq3$ selection.

Differential cross-section ratio of Z over $\gamma$ as a function of the total transverse momentum cross-section and for central bosons ($\vert y_{\mathrm{V}}\vert < 1.4$) in an inclusive $ N_{\mathrm{jets}}\geq 1 $ selection.

Differential cross-section ratio of Z over $\gamma$ as a function of the total transverse momentum cross-section and for central bosons ($\vert y_{\mathrm{V}}\vert < 1.4$) in a $ H_{\mathrm{T}}$% > 300 GeV, N_{\mathrm{jets}}\geq 1 $ selection.

Differential cross-section ratio of Z over $\gamma$ as a function of the total transverse momentum cross-section and for central bosons ($\vert y_{\mathrm{V}}\vert < 1.4$) in an inclusive $ N_{\mathrm{jets}}\geq 2 $ selection.

Differential cross-section ratio of Z over $\gamma$ as a function of the total transverse momentum cross-section and for central bosons ($\vert y_{\mathrm{V}}\vert < 1.4$) in an inclusive $ N_{\mathrm{jets}}\geq 3 $ selection.