Distributions of MaxMin alternative algorithm $m(h_{\mathrm{cand1}},h_{\mathrm{cand2}})_{\mathrm{avg}}$ after the background-only fit. The backgrounds which contribute only a small amount (diboson, W+jets and ttbar+W/Z/h) are grouped and labelled as `Other'.

Distributions of Leading jet $p_T$ after the background-only fit. The backgrounds which contribute only a small amount (diboson, W+jets and ttbar+W/Z/h) are grouped and labelled as `Other'.

Distributions of MaxMin algorithm $m_{hcand}$ after the background-only fit. The backgrounds which contribute only a small amount (diboson, W+jets and ttbar+W/Z/h) are grouped and labelled as `Other'.

Signal efficiency in SRA_M_m60 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal acceptance in SRC_28 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal acceptance in SRC_26 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal acceptance in SRC_24 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal acceptance in SRA_M_dm130 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal acceptance in SRB for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal acceptance in SRA_L_dm130 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal acceptance in SRC_incl for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal acceptance in SRA_L_m60 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal acceptance in SRA_incl_dm130 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal acceptance in SRA_incl_m60 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal efficiency in SRA_H_m60 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal efficiency in SRA_L_dm130 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal efficiency in SRB for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal acceptance in SRC_22 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal efficiency in SRA_H_dm130 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal efficiency in SRC_24 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal efficiency in SRC_26 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal acceptance in SRA_H_m60 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal efficiency in SRA_incl_m60 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal efficiency in SRC_22 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal acceptance in SRA_M_m60 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal efficiency in SRC_28 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal acceptance in SRA_H_dm130 for simplified models with $\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$ production

Signal efficiency in SRA_incl_dm130 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal efficiency in SRA_L_m60 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal efficiency in SRA_M_dm130 for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Signal efficiency in SRC_incl for simplified models with '$\widetilde{b}\widetilde{b}$ $\rightarrow$ $b\bar{b} \widetilde{\chi}_2^0 \widetilde{\chi}_2^0$ $\rightarrow$ hh$\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$, h $\rightarrow$ $b\bar{b}$' production

Observed 95% CLs exclusion limit for the $\Delta M(\widetilde{\chi}_{2}^{0},\widetilde{\chi}_{1}^{0})$=130GeV signal grid for the best combined signal regions.

Expected 95% CLs exclusion limit for the $\Delta M(\widetilde{\chi}_{2}^{0},\widetilde{\chi}_{1}^{0})$=130GeV signal grid for the best combined signal regions.

Observed 95% CLs exclusion limit for the $M(\widetilde{\chi}_{1}^{0})$=60GeV signal grid for the best combined signal regions.

Expected 95% CLs exclusion limit for the $M(\widetilde{\chi}_{1}^{0})$=60GeV signal grid for the best combined signal regions.

Model dependent upper limit on the best combined signal regions considered in the $\Delta M(\widetilde{\chi}_{2}^{0},\widetilde{\chi}_{1}^{0})$=130GeV signal grid

Model dependet upper limits on the best combined signal regions considered in the $\Delta M(\widetilde{\chi}_{2}^{0},\widetilde{\chi}_{1}^{0})$=130GeV signal grid

Result of background only fit applied to signal regions. Event yields from the signal regions compared with SM MC predictions for the 3 highest contributing backgrounds separately and combined minor backgrounds.

Expected background event yields and dominant systematic uncertainties on background estimates in the A-type (inclusive), B-type and C-type (inclusive) regions.

Background-only fit results for the A- and B-type regions performed using 139$fb^{-1}$ of data. The quoted uncertainties on the fitted SM background include both the statistical and systematic uncertainties.

Background-only fit results for the C-type region performed using 139$fb^{-1}$ of data. The quoted uncertainties on the fitted SM background include both the statistical and systematic uncertainties.

Observed 95% CL upper limits on the visible cross sections σvis, the observed (S95obs) and expected (S95exp) 95% CL upper limits on the number of signal events with ± 1 σ excursions of the expectation, the CL of the background-only hypothesis, CLB, the discovery p-value (p0), truncated at 0.5, and the associated significance.

Cutflow of the MC events scaled to 139 $fb^{-1}$ for the SRA selections, with a scalar bottom signal of m$(\widetilde{b}_{1},\widetilde{\chi}_2^0,\widetilde{\chi}_1^0) = (1100, 330, 200)$ GeV, considered.

Cutflow of the MC events scaled to 139 $fb^{-1}$ for the SRB selections, with a scalar bottom signal of m$(\widetilde{b}_{1},\widetilde{\chi}_2^0,\widetilde{\chi}_1^0) = (700, 680, 550)$ GeV, considered.

Cutflow of the MC events scaled to 139 $fb^{-1}$ for the SRC selections, with a scalar bottom signal of m$(\widetilde{b}_{1},\widetilde{\chi}_2^0,\widetilde{\chi}_1^0) = (1200, 1150, 60)$ GeV, considered.

Measured cross sections for inclusive isolated-photon production as a function of $E_{\rm T}^{\gamma}$ for $1.81<|\eta^{\gamma}|<2.37$.

Predicted cross sections for inclusive isolated-photon production as a function of $E_{\rm T}^{\gamma}$ for $|\eta^{\gamma}|<0.6$.

Predicted cross sections for inclusive isolated-photon production as a function of $E_{\rm T}^{\gamma}$ for $0.6<|\eta^{\gamma}|<1.37$.

Predicted cross sections for inclusive isolated-photon production as a function of $E_{\rm T}^{\gamma}$ for $1.56<|\eta^{\gamma}|<1.81$.

Predicted cross sections for inclusive isolated-photon production as a function of $E_{\rm T}^{\gamma}$ for $1.81<|\eta^{\gamma}|<2.37$.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Measured differential cross section with associated uncertainties as a function of $|\eta^*|$ in the VBF fiducial region. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $\sum\tau_{C,j}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma\gamma}$ in bins of $p_{T}^{\gamma\gamma j}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $\Delta\phi_{jj}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{j1}$ in the VBF fiducial region. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{j1}$ in bins of $\Delta\phi_{jj}$ in the VBF fiducial region. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma1}/m_{\gamma\gamma}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma\gamma} (N_\mathrm{jets}^{p_T>50\ \mathrm{GeV}}=0)$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma2}/m_{\gamma\gamma}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $\Delta\phi_{jj}$ in the VBF fiducial region. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $N_\mathrm{jets}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $N$($b$-jets). Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate. For the meaning of the bins please refer to the figure.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma\gamma jj}$ in the VBF fiducial region. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $H_{T}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $m_{jj}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma\gamma jj}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma\gamma}$ in bins of $\tau_{C,j1}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $|y_{\gamma\gamma}|$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured inclusive cross sections in the five fiducial regions. Each systematic uncertainty source is fully uncorrelated with the other sources.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma\gamma}$ in bins of $|y_{\gamma\gamma}|$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $\tau_{C,j1}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma\gamma}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $(p_{T}^{\gamma1}-p_{T}^{\gamma2})/m_{\gamma\gamma}$ in bins of $(p_{T}^{\gamma1}+p_{T}^{\gamma2})/m_{\gamma\gamma}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{j1}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma\gamma j}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $p_{T}^{\gamma\gamma} (N_\mathrm{jets}^{p_T>60\ \mathrm{GeV}}=0)$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of $m_{\gamma\gamma j}$. Each systematic uncertainty source is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma} (N_\mathrm{jets}^{p_T>60\ \mathrm{GeV}}=0)$.

Post-fit correlation matrix for the differential cross section measured as a function of $N_\mathrm{jets}$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma j}$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma jj}$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma} (N_\mathrm{jets}^{p_T>50\ \mathrm{GeV}}=0)$.

Post-fit correlation matrix for the differential cross section measured as a function of $|\eta^*|$ in the VBF fiducial region.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma}$ in bins of $\tau_{C,j1}$. The bins are the same as in the corresponding plot of the differential cross section.

Post-fit correlation matrix for the differential cross section measured as a function of $|y_{\gamma\gamma}|$.

Post-fit correlation matrix for the differential cross section measured as a function of $\pi - |\Delta\phi_{\gamma\gamma,jj}|$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma jj}$ in the VBF fiducial region.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma}$ in bins of $|y_{\gamma\gamma}|$. The bins are the same as in the corresponding plot of the differential cross section.

Post-fit correlation matrix for the differential cross section measured as a function of $\tau_{C,j1}$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{j1}$ in bins of $\Delta\phi_{jj}$ in the VBF fiducial region. The bins are the same as in the corresponding plot of the differential cross section.

Post-fit correlation matrix for the differential cross section measured as a function of $\Delta\phi_{jj}$ in the VBF fiducial region.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma}$ in bins of $p_{T}^{\gamma\gamma j}$. The bins are the same as in the corresponding plot of the differential cross section.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma2}/m_{\gamma\gamma}$.

Post-fit correlation matrix for the differential cross section measured as a function of $m_{jj}$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{j1}$ in the VBF fiducial region.

Post-fit correlation matrix for the differential cross section measured as a function of $(p_{T}^{\gamma1}-p_{T}^{\gamma2})/m_{\gamma\gamma}$ in bins of $(p_{T}^{\gamma1}+p_{T}^{\gamma2})/m_{\gamma\gamma}$. The bins are the same as in the corresponding plot of the differential cross section.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma} (N_\mathrm{jets}^{p_T>30\ \mathrm{GeV}}=0)$.

Post-fit correlation matrix for the differential cross section measured as a function of $H_{T}$.

Post-fit correlation matrix for the differential cross section measured as a function of $\sum\tau_{C,j}$.

Post-fit correlation matrix for the differential cross section measured as a function of $N$($b$-jets).

Post-fit correlation matrix for the differential cross section measured as a function of $\Delta\phi_{jj}$.

Post-fit correlation matrix for the differential cross section measured as a function of $m_{\gamma\gamma j}$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{j1}$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma} (N_\mathrm{jets}^{p_T>40\ \mathrm{GeV}}=0)$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma1}/m_{\gamma\gamma}$.

Post-fit correlation matrix for the differential cross section measured as a function of $p_{T}^{\gamma\gamma}$.

Observed statistical correlations, evaluated with a bootstrapping technique, between $p_\mathrm{T}^{\gamma\gamma}$, $N_\mathrm{jets}$, $m_{jj}$, $\Delta\phi_{jj}$, and $p_\mathrm{T}^{j1}$

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

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

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

$\langle r \rangle$, forward jet.

$\langle r \rangle$, central jet.

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

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

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

$\langle r \rangle$, both jets.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Limit Plot

Limit Plot

Limit Plot

HVT WW Acceptance times Efficiency

HVT WZ Acceptance times Efficiency

RS Graviton WW Acceptance times Efficiency

RS Graviton ZZ Acceptance times Efficiency

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

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

Observed upper limits at the 95% CL on the cross section for generic $W^\prime$ production and decay to the electron+neutrino channel as a function of the $W^\prime$ pole mass.

Observed upper limits at the 95% CL on the cross section for generic $W^\prime$ production and decay to the muon+neutrino channel as a function of the $W^\prime$ pole mass.

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

Observed upper limits at the 95% CL on the visible cross section in the electron+neutrino channel as a function of the transverse mass threshold.

Observed upper limits at the 95% CL on the visible cross section in the muon+neutrino channel as a function of the transverse mass threshold.

Product of acceptance and efficiency for the electron and muon selections as a function of the $W^\prime$ pole mass.

Expected upper limits at the 95% CL on the cross section for generic $W^\prime$ production and decay to the electron+neutrino channel as a function of the $W^\prime$ pole mass.

Expected upper limits at the 95% CL on the cross section for generic $W^\prime$ production and decay to the muon+neutrino channel as a function of the $W^\prime$ pole mass.

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

Upper limits on $\sigma\times B$ as a function of $m_{e^*}$ in the $e\nu J$ channel. The $\pm 1(2)\sigma$ uncertainty bands around the expected limit represent all sources of systematic and statistical uncertainties.

Lower limits on $\Lambda$ as a function of $m_{e^*}$ for the $eejj$ channel. The $\pm\ 1(2)\sigma$ uncertainty bands around the expected limit represent all sources of systematic and statistical uncertainties. The limits for $m_{e^*}\gt4$ TeV are the result of extrapolation.

Lower limits on $\Lambda$ as a function of $m_{e^*}$ for the $e\nu J$ channel. The $\pm\ 1(2)\sigma$ uncertainty bands around the expected limit represent all sources of systematic and statistical uncertainties.

Lower limits on $\Lambda$ as a function of $m_{e^*}$ combined for the $eejj$ and the $e\nu J$ channels. The $\pm\ 1(2)\sigma$ uncertainty bands around the expected limit represent all sources of systematic and statistical uncertainties. The limits for $m_{e^*}\gt4$ TeV are the result of extrapolation.