Upper limits on the fiducial cross section times branching ratio to two photons at centre-of-mass energy of 13 TeV of a narrow-width (Γ_X = 4 MeV) spin-0 resonance as a function of its mass m_X.

Upper limits on the production cross section times branching ratio to two photons at centre-of-mass energy of 13 TeV of the lightest KK graviton as a function of its mass m_G* for k/MPl=0.01.

Upper limits on the production cross section times branching ratio to two photons at centre-of-mass energy of 13 TeV of the lightest KK graviton as a function of its mass m_G* for k/MPl=0.10. Only the limits derived with the asymptotic formulae are quoted here.

Upper limits on the production cross section times branching ratio to two photons at centre-of-mass energy of 13 TeV of the lightest KK graviton as a function of its mass m_G* for k/MPl=0.20.

Upper limits on the production cross section times branching ratio to two photons at centre-of-mass energy of 13 TeV of the lightest KK graviton as a function of its mass m_G* for k/MPl=0.30.

Distribution of the diphoton invariant mass for data events passing the spin-0 selection. The data points are plotted at the centre of each bin. The error bars indicate statistical uncertainties. The distribution consists of not only genuine diphoton events, but also events where at least one photon is faked by a jet. There is no data event above 2700 GeV.

Distribution of the diphoton invariant mass for data events passing the spin-2 selection. The data points are plotted at the centre of each bin. The error bars indicate statistical uncertainties. The distribution consists of not only genuine diphoton events, but also events where at least one photon is faked by a jet. There is no data event above 2700 GeV.

Fiducial acceptance and product of the fiducial acceptance times the combined reconstruction and identification efficiency as a function of the mass for a spin-0 resonant signal with narrow width under the spin-0 selection. Only MC statistical uncertainties are included.

Fiducial acceptance and product of the fiducial acceptance times the combined reconstruction and identification efficiency as a function of the mass for a spin-2 resonant signal with k/MPl=0.1 under the spin-2 selection. The definition of fiducial region is provided in JHEP 09 (2016) 001. Only MC statistical uncertainties are included.

Fiducial acceptance and product of the fiducial acceptance times the combined reconstruction and identification efficiency as a function of the mass for an ADD excess (GRW formalism), calculated as the difference between the sum of ADD and SM contributions (including their interference) and the SM contribution, under the spin-2 selection in the signal region M(gamma gamma)>2240 GeV. The definition of fiducial region is provided in JHEP 09 (2016) 001, and M(gamma gamma)>2240 GeV is required in addition. Only MC statistical uncertainties are included.

Expected and observed upper limits at the 95% CL on the BB cross section as a function of B quark mass under the assumption of BR(B->Wt)=1.

Expected and observed upper limits at the 95% CL on the BB cross section as a function of B quark mass for an SU(2) singlet B.

Expected and observed 95% CL lower limits on the mass of the T quark in the branching ratio plane of BR(T->Wb) versus BR(T->Ht).

Expected and observed 95% CL lower limits on the mass of the B quark in the branching ratio plane of BR(T->Wb) versus BR(T->Ht).

Measured and expected $R^\text{miss}$ as a function of $\Delta\phi_\text{jj}$ in the VBF phase space. The fiducial SM predictions for the numerator and the denominator are also given.

Statistical-only correlation matrix for all four measured distributions. <br> <br> Bins labelled 1-7 correspond to the $p_\text{T}^\text{miss}$ distribution in the $\geq 1$ jet phase space. <br> Bins labelled 8-13 correspond to the $p_\text{T}^\text{miss}$ distribution in the VBF phase space. <br> Bins labelled 14-18 correspond to the $M_\text{jj}$ distribution in the VBF phase space. <br> Bins labelled 19-24 correspond to the $\Delta\phi_\text{jj}$ distribution in the VBF phase space.

Statistical-only covariance matrix for all four measured distributions. <br> <br> Bins labelled 1-7 correspond to the $p_\text{T}^\text{miss}$ distribution in the $\geq 1$ jet phase space. <br> Bins labelled 8-13 correspond to the $p_\text{T}^\text{miss}$ distribution in the VBF phase space. <br> Bins labelled 14-18 correspond to the $M_\text{jj}$ distribution in the VBF phase space. <br> Bins labelled 19-24 correspond to the $\Delta\phi_\text{jj}$ distribution in the VBF phase space.

Systematic covariance matrix for all four measured distributions. <br> <br> Bins labelled 1-7 correspond to the $p_\text{T}^\text{miss}$ distribution in the $\geq 1$ jet phase space. <br> Bins labelled 8-13 correspond to the $p_\text{T}^\text{miss}$ distribution in the VBF phase space. <br> Bins labelled 14-18 correspond to the $M_\text{jj}$ distribution in the VBF phase space. <br> Bins labelled 19-24 correspond to the $\Delta\phi_\text{jj}$ distribution in the VBF phase space.

Distributions of the invariant mass of the Higgs boson candidates mh=m_jj with two b-tags in the SR for the third MET category that is used as input to the fit.

Distributions of the invariant mass of the Higgs boson candidates mh=m_J with two b-tags in the SR for the fourth MET category that is used as input to the fit.

Distributions of the invariant mass of the Higgs boson candidates mh=m_jj with one b-tag in the SR for the first MET category which is used as input to the fit.

Distributions of the invariant mass of the Higgs boson candidates mh=m_jj with one b-tag in the SR for the second MET category which is used as input to the fit.

Distributions of the invariant mass of the Higgs boson candidates mh=m_jj with one b-tag in the SR for the third MET category which is used as input to the fit.

Upper limits at the 95% CL on the cross section for SSM W' production and decay to the muon+neutrino channel as a function of the W' pole mass.

Combined (electron and muon channels) upper limits at the 95% CL on the cross section for SSM W' production and decay to a single lepton generation as a function of the W' pole mass.

Product of acceptance and efficiency for the electron and muon selections as a function of the W' pole mass.

Expected 95% CL lower limit on the VLQ $T$ mass as a function of the decay branching ratios into $W b$ and $Ht$.

Observed 95% CL lower limit on the VLQ $T$ mass as a function of the decay branching ratios into $W b$ and $Ht$.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for PbPb collisions at $\sqrt{ s_{NN} }$=2.76 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_3\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_3\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$ v_2\{4\} $ harmonics for reference particles with 0.2 $ < p_{T} < $ 3.0 GeV as a function of $ < N_{ch}(|\eta|<1) > $ for p+Pb collisions at $ \sqrt{ s_{NN} } $= 5.02 TeV.

$ v_2\{4\} $ harmonics for reference particles with 0.2 $ < p_{T}< $ 3.0 GeV as a function of $ < N_{ch}(|\eta|<1) > $ for Pb+Pb collisions at $ \sqrt{ s_{NN} } $= 2.76 TeV.

The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with ten jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with eleven jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with twelve-or-more jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with five jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with six jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with ten-or-more jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with five jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with six jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

The expected background and observed data with ten-or-more jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.

Observed exclusion contours on the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.

Expected exclusion contours on the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.

Observed exclusion contours on the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.

Expected exclusion contours on the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.

Observed exclusion contours on the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.

Expected exclusion contours on the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.

Observed exclusion contours on the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.

Expected exclusion contours on the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.

Observed exclusion contours on the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.

Expected exclusion contours on the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.

Observed upper limits on the model cross-section in units of pb as a function of the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.

Observed upper limits on the model cross-section in units of pb as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.

Observed upper limits on the model cross-section in units of pb as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.

Observed upper limits on the model cross-section in units of pb as a function of the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.

Observed upper limits on the model cross-section in units of pb as a function of the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.

Acceptance as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.

Efficiency as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.

Acceptance as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.

Efficiency as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.

Cut flow for a model of gluino pair production where the gluino decays to two (u, d, s, c) quarks and the neutralino, which then decays to two (u, d, s, c) quarks and a lepton via a lambda' RPV coupling, where each RPV decay can produce any of the four first and second generation leptons (e, mu, nu_e, nu_mu) with equal probability (m_gluino = 1800 GeV, m_neutralino = 900 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.

Cut flow for a model of gluino pair production where each gluino decays to a top quark and a top squark, with the top squark decaying to an s- and a b- quark via a non-zero lambda''_323 RPV coupling (m_gluino = 1600 GeV, m_stop = 1000 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.

Cut flow for a model of gluino pair production where each gluino decays via an off-shell top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino -> uds) via the RPV coupling lambda''_112 (m_gluino = 2000 GeV, m_neutralino = 941 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.

Cut flow for a model of right-handed top squark pair production with the top squark decaying to the lightest supersymmetric particle (LSP) which is considered to be purely higgsino. The higgsino-like LSP decays through the non-zero RPV coupling lambda''_323 (m_stop = 975 GeV, m_neutralino = 600 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.