Slices of 2D distributions of observed events and the post-fit templates in the TT pass region, projected onto the plane of leading jet mass mJ1, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the TT pass region, projected onto the plane of leading jet mass mJ1, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the TT pass region, projected onto the plane of leading jet mass mJ1, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the LL pass region, projected onto the plane of corrected HH mass (mHH) mHH, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the LL pass region, projected onto the plane of corrected HH mass (mHH) mHH, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the LL pass region, projected onto the plane of corrected HH mass (mHH) mHH, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the TT pass region, projected onto the plane of corrected HH mass (mHH) mHH, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the TT pass region, projected onto the plane of corrected HH mass (mHH) mHH, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the TT pass region, projected onto the plane of corrected HH mass (mHH) mHH, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the semi-resolved pass region, projected onto the plane of corrected HH mass (mHH) mHH, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the semi-resolved pass region, projected onto the plane of corrected HH mass (mHH) mHH, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the semi-resolved pass region, projected onto the plane of corrected HH mass (mHH) mHH, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the semi-resolved pass region, projected onto the plane of leading jet mass mJ1, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the semi-resolved pass region, projected onto the plane of leading jet mass mJ1, including expected radion signal at 1.5 TeV.

Slices of 2D distributions of observed events and the post-fit templates in the semi-resolved pass region, projected onto the plane of leading jet mass mJ1, including expected radion signal at 1.5 TeV.

The observed (solid black line) and expected (dashed black line) upper limits at 95% CL on $\sigma$(pp->X)B(X->HH->4b) for the narrow spin-0 radion model. The green (yellow) bands represent one (two) standard deviations from the expected limit. The predicted theoretical cross sections are also shown.

The observed (solid black line) and expected (dashed black line) upper limits at 95% CL on $\sigma$(pp->X)B(X->HH->4b) for the narrow width spin-2 bulk graviton model. The green (yellow) bands represent one (two) standard deviations from the expected limit. The predicted theoretical cross sections are also shown.

The observed (solid black line) and expected (dashed black line) upper limits at 95% CL on $\sigma$(pp->X)B(X->HH->4b) for the 10%-width spin-0 radion model. The green (yellow) bands represent one (two) standard deviations from the expected limit. The predicted theoretical cross sections are also shown.

The observed (solid black line) and expected (dashed black line) upper limits at 95% CL on $\sigma$(pp->X)B(X->HH->4b) for the 10%-width spin-2 bulk graviton model. The green (yellow) bands represent one (two) standard deviations from the expected limit. The predicted theoretical cross sections are also shown.

Correlations of the ttH signal-strength modifiers in the different Higgs pT bins of the STXS measurement.

Observed and expected upper 95% CL limit on the tH signal strength modifier $\mu_{tH}$ with $\mu_{ttH}=1$ for different channels and years, where the uncertainties are uncorrelated between the channels and years, and in their combination. The one and two standard deviation confidence intervals on the expected limit are also listed (sigma).

Likelihood-ratio test statistic as a function of the ttH and tH signal strength modifiers $\mu_{ttH}$ and $\mu_{tH}$. The observed best fit point is $(\mu_{tH}, \mu_{ttH}) = (-3.83, +0.35)$.

Observed and expected likelihood ratio test statistic as a function of $\kappa_{t}$ and $\kappa_{V}$. The observed best fit point is $(\kappa_{t}, \kappa_{V}) = (+0.59, +1.40)$.

Observed and expected likelihood ratio test statistic as a function of $\kappa_{t}$ for $\kappa_{V}=1$. The observed best fit point is $\kappa_{t} = +0.54$.

Observed and expected likelihood ratio test statistic as a function of $\kappa_{t}$ and $\tilde{\kappa}_{t}$ with $\kappa_{V}=1$. The observed best fit point is $(\kappa_{t}, \tilde{\kappa}_{t}) = (+0.53, 0.00)$.

Observed and expected likelihood ratio test statistic as a function of $f_{CP}$. The overall modifier of the top-Higgs coupling strength is profiled such that the likelihood attains its minimum at each point in the plane, and $\kappa_{V}$ is set to 1. The observed best fit point is $f_{CP} = 0.00$.

Observed and expected likelihood ratio test statistic as a function of $\cos(\alpha)$. The overall modifier of the top-Higgs coupling strength is profiled such that the likelihood attains its minimum at each point in the plane, and $\kappa_{V}$ is set to 1. The observed best fit point is $\cos(\alpha) = +1.00$.

Observed and expected likelihood ratio test statistic as a function of $\kappa_{t}$ and $\tilde{\kappa}_{t}$ with $\kappa_{V}=1$, in the $H \rightarrow bb$, $H\rightarrow\gamma\gamma$, $H\rightarrow ZZ$, $H\rightarrow WW$, and $H\rightarrow\tau\tau$ decay channels and in their combination.

Observed and expected likelihood ratio test statistic as a function of $f_{CP}$, in the $H \rightarrow bb$, $H\rightarrow\gamma\gamma$, $H\rightarrow ZZ$, $H\rightarrow WW$, and $H\rightarrow\tau\tau$ decay channel and in their combination. The overall modifier of the top-Higgs coupling strength is profiled such that the likelihood attains its minimum at each point in the plane, and $\kappa_{V}$ is set to 1.

Observed and expected likelihood ratio test statistic as a function of $\cos(\alpha)$, in the $H \rightarrow bb$, $H\rightarrow\gamma\gamma$, $H\rightarrow ZZ$, $H\rightarrow WW$, and $H\rightarrow\tau\tau$ decay channels and in their combination. The overall modifier of the top-Higgs coupling strength is profiled such that the likelihood attains its minimum at each point in the plane, and $\kappa_{V}$ is set to 1.

non prompt $\psi(2S)$ $\lambda_\theta$

The product of detector acceptance and analysis selection efficiency in the muon channel as functions of the particle X mass. Three analysis requirements are applied consecutively: event reconstruction, HLT, and final signal selection. The product of detector acceptance and analysis selection efficiencies are shown at each stage in red, blue, and orange, respectively.

Background-only fit to data. The lower panel contains the pull distribution, defined as the difference between the data yield and the background prediction divided by their combined uncertainty (electron channel).

Background-only fit to data. The lower panel contains the pull distribution, defined as the difference between the data yield and the background prediction divided by their combined uncertainty (muon channel).

The systematic uncertainties affecting signal normalization (electron channel).

The systematic uncertainties affecting signal normalization (muon channel).

The 95% CL expected and observed limits on P P --> X --> W gamma as a function of the resonant mass with leptonic decays of W bosons (narrow width).

The 95% CL expected and observed limits on P P --> X --> W gamma as a function of the resonant mass with leptonic decays of W bosons (broad width).

The 95% CL expected and observed limits on P P --> X --> W gamma as a function of the resonant mass with both leptonic and hadronic decays of W bosons (narrow width).

The 95% CL expected and observed limits on P P --> X --> W gamma as a function of the resonant mass with both leptonic and hadronic decays of W bosons (broad width).

The observed local p-values for narrow resonance width hypotheses.

The observed local p-values for broad resonance width hypotheses.

Expected and observed exclusion limits at 95% CL in the asymptotic approximation, on the product of the production cross section and branching fraction into two photons for an additional SM-like Higgs boson, for the VBF plus VH processes, from the analysis of the combined data from 2016, 2017, and 2018.

Expected and observed exclusion limits at 95% CL in the asymptotic approximation, on the product of the production cross section and branching fraction into two photons for an additional SM-like Higgs boson, assuming 100% production via the VBF processes, from the analysis of the combined data from 2016, 2017, and 2018.

Expected and observed exclusion limits at 95% CL in the asymptotic approximation, on the product of the production cross section and branching fraction into two photons for an additional SM-like Higgs boson, assuming 100% production via the VH processes, from the analysis of the combined data from 2016, 2017, and 2018.

Histogram of the Hbb AK8 jet softdrop mass for data, simulated signal and background events, and the background yields estimated from data in region A.

Histogram of the Hbb AK8 jet softdrop mass for data and simulated signal and background events.

Histogram of $p_{T}(H) + p_{T}(W)$ at the LHE level.

The signal yield estimated by simulation, background yield predicted from data, and observed yield in the signal region.

Observed and expected BDT output in the signal region used for the extraction of the SM-like signal strength. The yields and uncertainties of the expected contributions are shown after the fit to the data. The rightmost bin includes the overflow.

Limits on the signal strength of SM VBS WH production

Observed and expected significance of the measurement of SM VBS WH production

95% confidence limits on the signal strength in the SM analysis

A scan of $-2\Delta\ln L$, where $L$ is the likelihood, for the SM analysis plotted as a function of the signal strength $\mu$ for the expected (red) and the observed (black) data.

The data, fitted signal, and background distributions for the VBS dijet mass in the $t\overline{t}$ control region of the SM analysis.

The data, fitted signal, and background distributions for the W+jets BDT score in the W+jets control region of the SM analysis.

Fitted SME coefficients and their uncertainties at 1$\sigma$ and 2$sigma$, measured in fits of single coefficients while the coefficients corresponding to the three other directions are left floating, within the $c_L$, $c_R$, $c$, and $d$ families. The error bar includes statistical and systematic uncertainties.

Uncertainty breakdown for SME fits of single coefficients while the coefficients corresponding to the three other directions are left floating, by splitting according to the treatment of time dependence:\ flat across sidereal time (flat luminosity component, background normalization, theory), correlated in sidereal time bins (trigger, luminosity stability and linearity, pileup, MC statistical uncertainty, single top quark decay in the SME), systematics uncorrelated in sidereal time bins (other experimental uncertainties), and statistical uncertainty.

Figure 3 top left. Expected and observed 95% CL upper limits on the product of the production cross section and branching fraction as a function of the RS graviton mass $m_{G}$ for the full Run 2 data set are shown. Expected $1\sigma$ and $2\sigma$ limit bands are shown in green and yellow, respectively

Figure 3 top right. Expected and observed 95% CL upper limits on the product of the production cross section and branching fraction as a function of the heavy higgs mass $m_{S}$ for the full Run 2 data set are shown. Expected $1\sigma$ and $2\sigma$ limit bands are shown in green and yellow, respectively

Figure 3 mid left. Expected and observed 95% CL upper limits on the product of the production cross section and branching fraction as a function of the RS graviton mass $m_{G}$ for the full Run 2 data set are shown. Expected $1\sigma$ and $2\sigma$ limit bands are shown in green and yellow, respectively

Figure 3 mid right. Expected and observed 95% CL upper limits on the product of the production cross section and branching fraction as a function of the heavy higgs mass $m_{S}$ for the full Run 2 data set are shown. Expected $1\sigma$ and $2\sigma$ limit bands are shown in green and yellow, respectively

Figure 3 bottom left. Expected and observed 95% CL upper limits on the product of the production cross section and branching fraction as a function of the RS graviton mass $m_{G}$ for the full Run 2 data set are shown. Expected $1\sigma$ and $2\sigma$ limit bands are shown in green and yellow, respectively

Figure 3 bottom right. Expected and observed 95% CL upper limits on the product of the production cross section and branching fraction as a function of the heavy higgs mass $m_{S}$ for the full Run 2 data set are shown. Expected $1\sigma$ and $2\sigma$ limit bands are shown in green and yellow, respectively

Figure 4 top left. Expected 95% CL upper limits on the product of the cross section and branching fraction as a function of the $m_{G}$ versus the resonance width for the full Run 2 data set.

Figure 4 top right. Observed 95% CL upper limits on the product of the cross section and branching fraction as a function of the $m_{G}$ versus the resonance width for the full Run 2 data set.

Figure 4 bottom left. Expected 95% CL upper limits on the product of the cross section and branching fraction as a function of the $m_{S}$ versus the resonance width for the full Run 2 data set.

Figure 4 bottom right. Observed 95% CL upper limits on the product of the cross section and branching fraction as a function of the $m_{S}$ versus the resonance width for the full Run 2 data set.

Figure 6. The $m_{\gamma\gamma}$ spectra and background prediction after nuisance paramter marginalization (post-fit) due to SM diphoton production ($\gamma\gamma$) and fake photon production (j$\gamma$, jj) for the EBEB, combining the 2016, 2017, and 2018 data sets. The prediction with a large extra dimensions signal (GRW convention with $M_{S}$ = 9 TeV) is also shown. The pull distributions, normalized to the statistical uncertainty only, are shown underneath the spectra. The last bin contains the overflow of events beyond $m_{\gamma\gamma}$ > 3.5 TeV.

Figure 6. The $m_{\gamma\gamma}$ spectra and background prediction after nuisance paramter marginalization (post-fit) due to SM diphoton production ($\gamma\gamma$) and fake photon production (j$\gamma$, jj) for the EBEE, combining the 2016, 2017, and 2018 data sets. The prediction with a large extra dimensions signal (GRW convention with $M_{S}$ = 9 TeV) is also shown. The pull distributions, normalized to the statistical uncertainty only, are shown underneath the spectra. The last bin contains the overflow of events beyond $m_{\gamma\gamma}$ > 3.5 TeV.

Figure 7. The exclusion limit for the clockwork framework over the k--M5 parameter space. The shaded region denotes where the theory becomes nonperturbative. The region below and to the left of the solid line constitutes the excluded region. Expected 1std and 2std limit bands are shown in green and yellow, respectively.