Data from Fig. 3 lower right panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 13$ TeV as a function of the jet multiplicity with $|\eta_{j}| < 2.4$.

Data from Fig. 4 upper right panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 13$ TeV as a function of the p$_T$-leading jet transverse momentum with $|\eta_{j}| < 4.7$.

Data from Fig. 5 left panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 13$ TeV as a function of the p$_T$-leading jet transverse momentum with $|\eta_{j}| < 4.7$.

Data from Fig. 4 lower right panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 13$ TeV as a function of the p$_T$-leading jet $|\eta_{j}|$ with $|\eta_{j}| < 4.7$.

Data from Fig. 5 right panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 13$ TeV as a function of the p$_T$-subleading jet $|\eta_{j}|$ with $|\eta_{j}| < 4.7$.

Data from Fig. 6 left panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 13$ TeV as a function of the invariant mass of the two p$_T$ leading jets with $|\eta_{j}| < 4.7$.

Data from Fig. 6 right panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 13$ TeV as a function of the invariant of pseudorapidity separation of the two $p$_T$ leading jets with $|\eta_{j}| < 4.7$.

Data from Fig. 2 upper left. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ differential cross section at $\sqrt{s} = 8$ TeV as a function of the jet multiplicity with $|\eta| < 4.7$.

Data from Fig. 3 upper left panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 8$ TeV as a function of the jet multiplicity with $|\eta| < 4.7$.

Data from Fig. 2 lower left panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ differential cross section at $\sqrt{s} = 8$ TeV as a function of the jet multiplicity with $|\eta| < 2.4$.

Data from Fig. 3 lower left panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 8$ TeV as a function of the jet multiplicity with $|\eta| < 2.4$.

Data from Fig. 4 upper left panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 8$ TeV as a function of the p$_T$-leading jet transverse momentum with $|\eta| < 4.7$.

Data from Fig. 4 lower left panel. The $\textrm{pp} \to \textrm{ZZ}\to \ell\ell\ell^{\prime}\ell^{\prime}$ normalized differential cross section at $\sqrt{s} = 8$ TeV as a function of the p$_T$-leading jet transverse $\eta$ with $|\eta| < 4.7$.

Differential cross section times dimuon branching fraction of Y(1S) as a function of $y^{Y}_{CM}$ in pPb collisions. The global uncertainty arises from the integrated luminosity uncertainty in pPb collisions.

Differential cross section times dimuon branching fraction of Y(2S) as a function of $y^{Y}_{CM}$ in pPb collisions. The global uncertainty arises from the integrated luminosity uncertainty in pPb collisions.

Differential cross section times dimuon branching fraction of Y(3S) as a function of $y^{Y}_{CM}$ in pPb collisions. The global uncertainty arises from the integrated luminosity uncertainty in pPb collisions.

Differential cross section times dimuon branching fraction of Y(1S) as a function of pT in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(2S) as a function of pT in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(3S) as a function of pT in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(1S) as a function of $|y^{Y}_{CM}|$ in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(2S) as a function of $|y^{Y}_{CM}|$ in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(3S) as a function of $|y^{Y}_{CM}|$ in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Nuclear modification factor of Y(1S) as a function of pT. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(2S) as a function of pT. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(3S) as a function of pT. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(1S) as a function of $y^{Y}_{CM}$. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(2S) as a function of $y^{Y}_{CM}$. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(3S) as a function of $y^{Y}_{CM}$. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(1S) at forward and backward $y^{Y}_{CM}$ for pT < 6 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(2S) at forward and backward $y^{Y}_{CM}$ for pT < 6 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(3S) at forward and backward $y^{Y}_{CM}$ for pT < 6 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(1S) at forward and backward $y^{Y}_{CM}$ for 6 < pT < 30 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(2S) at forward and backward $y^{Y}_{CM}$ for 6 < pT < 30 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(3S) at forward and backward $y^{Y}_{CM}$ for 6 < pT < 30 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

RFB of Y(1S) versus $N^{|\eta_{lab}|<2.4}_{tracks}$.

RFB of Y(2S) versus $N^{|\eta_{lab}|<2.4}_{tracks}$.

RFB of Y(3S) versus $N^{|\eta_{lab}|<2.4}_{tracks}$.

RFB of Y(1S) versus $E^{|\eta_{lab}|>4}_{T}$.

RFB of Y(2S) versus $E^{|\eta_{lab}|>4}_{T}$.

RFB of Y(3S) versus $E^{|\eta_{lab}|>4}_{T}$.

Nuclear modification factor of Y(1S), Y(2S), and Y(3S) integrated over pT and $y^{Y}_{CM}$. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

The observed $m_{T}$ and $m_{jj}$ distributions in the ejj (upper left), $\mu$~jj (upper right), $\tau_{h}$~jj (lower left), and $0\ell$~jj (lower right) signal regions compared with the post-fit SM background yields from the fit described in the text. The pre-fit background yields and shapes are determined using data-driven methods for the major backgrounds, and based on simulation for the smaller backgrounds. Expected signal distributions are overlaid. The last bin in the $m_{T}$ distributions of the $1\ell$~jj channels include all events with $m_{T} > 210$~GeV. The last bin of the $m_{jj}$ distributions of the $0\ell$~jj channel include all events with $m_{jj} > 3800$~GeV.

The observed $m_{T}$ and $m_{jj}$ distributions in the ejj (upper left), $\mu$~jj (upper right), $\tau_{h}$~jj (lower left), and $0\ell$~jj (lower right) signal regions compared with the post-fit SM background yields from the fit described in the text. The pre-fit background yields and shapes are determined using data-driven methods for the major backgrounds, and based on simulation for the smaller backgrounds. Expected signal distributions are overlaid. The last bin in the $m_{T}$ distributions of the $1\ell$~jj channels include all events with $m_{T} > 210$~GeV. The last bin of the $m_{jj}$ distributions of the $0\ell$~jj channel include all events with $m_{jj} > 3800$~GeV.

Combined 95% CL UL on the cross section as a function of $m(\tilde{\chi}_{2}^{0})=m(\tilde{\chi}_{1}^{\pm})$. The results correspond to $\Delta m=1$ GeV (left) and $\Delta m=50$ GeV (right) mass gaps between the chargino and the lightest neutralino in the light slepton model. The top row shows the expected limits, and the bottom row shows the observed limits.

Combined 95% CL UL on the cross section as a function of $m(\tilde{\chi}_{2}^{0})=m(\tilde{\chi}_{1}^{\pm})$. The results correspond to $\Delta m=1$ GeV (left) and $\Delta m=50$ GeV (right) mass gaps between the chargino and the lightest neutralino in the light slepton model. The top row shows the expected limits, and the bottom row shows the observed limits.

Combined 95% CL UL on the cross section as a function of $m(\tilde{\chi}_{2}^{0})=m(\tilde{\chi}_{1}^{\pm})$. The results correspond to $\Delta m=1$ GeV (left) and $\Delta m=50$ GeV (right) mass gaps between the chargino and the lightest neutralino in the light slepton model. The top row shows the expected limits, and the bottom row shows the observed limits.

Combined 95% CL UL on the cross section as a function of $m(\tilde{\chi}_{2}^{0})=m(\tilde{\chi}_{1}^{\pm})$. The results correspond to $\Delta m=1$ GeV (left) and $\Delta m=50$ GeV (right) mass gaps between the chargino and the lightest neutralino in the light slepton model. The top row shows the expected limits, and the bottom row shows the observed limits.

(Left) Expected and observed 95% confidence level upper limit (UL) on the signal cross section as a function of $m(\tilde{\chi}_{1}^{\pm})$ and $\Delta m$, assuming the light slepton model with slepton mass defined as the average of the \tilde{\chi}_{2}^{0} and \tilde{\chi}_{1}^{\pm} masses, $x_{\widetilde{\ell}}=0.5$. The lower left edge of each bin represents the \{$m(\tilde{\chi}_{1}^{\pm})$,$\Delta m$\} combination used to calculate the UL on the signal cross section. For example, the lowest and leftmost bin corresponds to the UL on the signal cross section for the scenario with $m(\tilde{\chi}_{1}^{\pm}) = 100$ GeV and $\Delta m = 1$ GeV. (Right) Combined 95% CL UL on the cross section as a function of $m_{\tilde{\chi}_{2}^{0}}=m_{\tilde{\chi}_{1}^{\pm}}$, for $\Delta m=1$ GeV and $\Delta m=30$ GeV mass gaps between the chargino and the neutralino, assuming the light slepton model.

(Left) Expected and observed 95% confidence level upper limit (UL) on the signal cross section as a function of $m(\tilde{\chi}_{1}^{\pm})$ and $\Delta m$, assuming the light slepton model with slepton mass defined as the average of the \tilde{\chi}_{2}^{0} and \tilde{\chi}_{1}^{\pm} masses, $x_{\widetilde{\ell}}=0.5$. The lower left edge of each bin represents the \{$m(\tilde{\chi}_{1}^{\pm})$,$\Delta m$\} combination used to calculate the UL on the signal cross section. For example, the lowest and leftmost bin corresponds to the UL on the signal cross section for the scenario with $m(\tilde{\chi}_{1}^{\pm}) = 100$ GeV and $\Delta m = 1$ GeV. (Right) Combined 95% CL UL on the cross section as a function of $m_{\tilde{\chi}_{2}^{0}}=m_{\tilde{\chi}_{1}^{\pm}}$, for $\Delta m=1$ GeV and $\Delta m=30$ GeV mass gaps between the chargino and the neutralino, assuming the light slepton model.

(Left) Expected and observed 95% confidence level upper limit (UL) on the signal cross section as a function of $m(\tilde{\chi}_{1}^{\pm})$ and $\Delta m$, assuming the light slepton model with slepton mass defined as the average of the \tilde{\chi}_{2}^{0} and \tilde{\chi}_{1}^{\pm} masses, $x_{\widetilde{\ell}}=0.5$. The lower left edge of each bin represents the \{$m(\tilde{\chi}_{1}^{\pm})$,$\Delta m$\} combination used to calculate the UL on the signal cross section. For example, the lowest and leftmost bin corresponds to the UL on the signal cross section for the scenario with $m(\tilde{\chi}_{1}^{\pm}) = 100$ GeV and $\Delta m = 1$ GeV. (Right) Combined 95% CL UL on the cross section as a function of $m_{\tilde{\chi}_{2}^{0}}=m_{\tilde{\chi}_{1}^{\pm}}$, for $\Delta m=1$ GeV and $\Delta m=30$ GeV mass gaps between the chargino and the neutralino, assuming the light slepton model.

(Left) Expected and observed 95% confidence level upper limit (UL) on the signal cross section as a function of $m(\tilde{\chi}_{1}^{\pm})$ and $\Delta m$, assuming the \tilde{\chi}_{1}^{\pm} and \tilde{\chi}_{2}^{0} decays proceed via $W^{*}$ and $Z^{*}$. The lower left edge of each bin represents the \{$m(\tilde{\chi}_{1}^{\pm})$,$\Delta m$\} combination used to calculate the UL on the signal cross section. For example, the lowest and leftmost bin corresponds to the UL on the signal cross section for the scenario with $m(\tilde{\chi}_{1}^{\pm}) = 100$ GeV and $\Delta m = 1$ GeV. (Right) The 95% CL UL on the cross section as a function of $m_{\tilde{\chi}_{2}^{0}}=m_{\tilde{\chi}_{1}^{\pm}}$, for $\Delta m=1$ GeV and $\Delta m=30$ GeV mass gaps between the chargino and the neutralino, after combining 0 lepton and 1 lepton channels, assuming the \tilde{\chi}_{1}^{\pm} and \tilde{\chi}_{2}^{0} decays proceed via $W^{*}$ and $Z^{*}$.

(Left) Expected and observed 95% confidence level upper limit (UL) on the signal cross section as a function of $m(\tilde{\chi}_{1}^{\pm})$ and $\Delta m$, assuming the \tilde{\chi}_{1}^{\pm} and \tilde{\chi}_{2}^{0} decays proceed via $W^{*}$ and $Z^{*}$. The lower left edge of each bin represents the \{$m(\tilde{\chi}_{1}^{\pm})$,$\Delta m$\} combination used to calculate the UL on the signal cross section. For example, the lowest and leftmost bin corresponds to the UL on the signal cross section for the scenario with $m(\tilde{\chi}_{1}^{\pm}) = 100$ GeV and $\Delta m = 1$ GeV. (Right) The 95% CL UL on the cross section as a function of $m_{\tilde{\chi}_{2}^{0}}=m_{\tilde{\chi}_{1}^{\pm}}$, for $\Delta m=1$ GeV and $\Delta m=30$ GeV mass gaps between the chargino and the neutralino, after combining 0 lepton and 1 lepton channels, assuming the \tilde{\chi}_{1}^{\pm} and \tilde{\chi}_{2}^{0} decays proceed via $W^{*}$ and $Z^{*}$.

Example description

Combined 95% CL expected upper limit on the signal cross section as a function of $m_{\tilde{\chi}_{2}^{0}}=m_{\tilde{\chi}_{1}^{\pm}}$ for a $\Delta m=1$ GeV mass gap between the chargino and the lightest neutralino in the $W Z$ model.

Combined 95% CL expected upper limit on the signal cross section as a function of $m_{\tilde{\chi}_{2}^{0}}=m_{\tilde{\chi}_{1}^{\pm}}$ for a $\Delta m=50$ GeV mass gap between the chargino and the lightest neutralino in the $W Z$ model.

Combined 95% CL observed upper limit on the signal cross section as a function of $m_{\tilde{\chi}_{2}^{0}}=m_{\tilde{\chi}_{1}^{\pm}}$ for a $\Delta m=1$ GeV mass gap between the chargino and the lightest neutralino in the $W Z$ model.

Combined 95% CL observed upper limit on the signal cross section as a function of $m_{\tilde{\chi}_{2}^{0}}=m_{\tilde{\chi}_{1}^{\pm}}$ for a $\Delta m=50$ GeV mass gap between the chargino and the lightest neutralino in the $W Z$ model.

Covariance matrix from the combined fit of the $m_{ extrm{jj}}$ and $m_{ extrm{T}}$ distributions in the $0\ell extrm{jj}$ and $1\ell extrm{jj}$ search regions.

Summary of typical systematic uncertainties for the signal.

Numbers of observed events for all signal regions, including predicted background contributions and expected signal yields.

Limits on anomalous quartic couplings at 95% CL.

Expected and observed 95% CL upper limits on the cross section times the branching ratio sigma(P P --> W+- a)B(a --> W+- W-+) as a function of ALP mass

Expected and observed 95% CL upper limits on the photophobic ALP model parameter 1/f_a as a function of ALP mass.

Observed signal strength, and observed signal cross section.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $\phi^*$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $\phi^*$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Integrated fiducial cross section for the DY process measured in the muon channel. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of dimuon invariant mass. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of rapidity in the centre-of-mass frame for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of rapidity in the centre-of-mass frame for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $\phi^*$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $\phi^*$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Integrated cross section for the DY process measured in the muon channel. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Forward-backward ratios for $15<m_{\mu\mu}<60$ GeV. Quoted uncertainties are the quadratic sum of the statistical and systematic uncertainties.

Forward-backward ratios for $60<m_{\mu\mu}<120$ GeV. Quoted uncertainties are the quadratic sum of the statistical and systematic uncertainties.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of dimuon invariant mass.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of rapidity in the centre-of-mass frame for $15<m_{\mu\mu}<60$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of rapidity in the centre-of-mass frame for $60<m_{\mu\mu}<120$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $p_{\textrm{T}}$ for $15<m_{\mu\mu}<60$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $p_{\textrm{T}}$ for $60<m_{\mu\mu}<120$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $\phi^*$ for $15<m_{\mu\mu}<60$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $\phi^*$ for $60<m_{\mu\mu}<120$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of rapidity in the centre-of-mass frame, putting together low and high masses. Each bin is labeled lm_i or hm_i, where lm stands for $15<m_{\mu\mu}<60$ GeV, hm stands for $60<m_{\mu\mu}<120$ GeV, and i is the corresponding bin number in rapidity in the centre-of-mass frame. The global normalisation uncertainty of 3.5% is not included. Data from Figure [3, 4, 4].

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $p_{\textrm{T}}$, putting together low and high masses. Each bin is labeled lm_i or hm_i, where lm stands for $15<m_{\mu\mu}<60$ GeV, hm stands for $60<m_{\mu\mu}<120$ GeV, and i is the corresponding bin number in $p_{\textrm{T}}$. The global normalisation uncertainty of 3.5% is not included. Data from Figure [3, 4, 4].

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $\phi^*$, putting together low and high masses. Each bin is labeled lm_i or hm_i, where lm stands for $15<m_{\mu\mu}<60$ GeV, hm stands for $60<m_{\mu\mu}<120$ GeV, and i is the corresponding bin number in $\phi^*$. The global normalisation uncertainty of 3.5% is not included. Data from Figure [3, 4, 4].

The $ {{{\mathrm {B}}}\to {\mathrm {D^0}}} $ nuclear modification factor $ {R_{\mathrm {AA}}} $ for PbPb collisions at ${\sqrt {\smash [b]{s_{_{\mathrm {NN}}}}}} = $ 5.02 TeV.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for bbA prodcution and the branching fraction $\mathrm{A} \rightarrow \tau\tau$, obtained from the combination of the $\mathrm{e}\tau_\mathrm{h}$ and $\mu\tau_\mathrm{h}$ channels in the 1 b tag category, as a function of the A boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for bbA prodcution and the branching fraction $\mathrm{A} \rightarrow \tau\tau$, obtained in the $\mathrm{e}\tau_\mathrm{h}$ channel of the 1 b tag category, as a function of the A boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for bbA prodcution and the branching fraction $\mathrm{A} \rightarrow \tau\tau$, obtained in the $\mu\tau_\mathrm{h}$ channel of the 1 b tag category, as a function of the A boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

The product of acceptance, efficiency, and branching fraction of the qbX signal with $\mathrm{X} \rightarrow \tau\tau$ and $m_{\mathrm{B}}=170~\mathrm{GeV}$ in $\mathrm{e}\tau_\mathrm{h}$ and $\mu\tau_\mathrm{h}$ channels of the 1b1f and 1b1c event categories, as a function of the X boson mass. The selections are as described in the paper. The uncertainty refers to the statistical uncertainty only.

Observed $m_{\tau\tau}$ distribution in the $\mathrm{e}\tau_\mathrm{h}$ channel of the 1b1f category, compared to the expected SM background contributions. The distributions of the qbX signal with $m_{\mathrm{B}}=170~\mathrm{GeV}$, and X boson mass 40 and 60 GeV are overlaid to illustrate the sensitivity. They are normalized to the cross section times branching fraction of 20 pb. The uncertainty band represents the sum in quadrature of statistical and systematic uncertainties obtained from the fit. The lower panel shows the ratio between the observed and expected events in each bin.

Observed $m_{\tau\tau}$ distribution in the $\mathrm{e}\tau_\mathrm{h}$ channel of the 1b1c category, compared to the expected SM background contributions. The distributions of the qbX signal with $m_{\mathrm{B}}=170~\mathrm{GeV}$, and X boson mass 40 and 60 GeV are overlaid to illustrate the sensitivity. They are normalized to the cross section times branching fraction of 20 pb. The uncertainty band represents the sum in quadrature of statistical and systematic uncertainties obtained from the fit. The lower panel shows the ratio between the observed and expected events in each bin.

Observed $m_{\tau\tau}$ distribution in the $\mu\tau_\mathrm{h}$ channel of the 1b1f category, compared to the expected SM background contributions. The distributions of the qbX signal with $m_{\mathrm{B}}=170~\mathrm{GeV}$, and X boson mass 40 and 60 GeV are overlaid to illustrate the sensitivity. They are normalized to the cross section times branching fraction of 20 pb. The uncertainty band represents the sum in quadrature of statistical and systematic uncertainties obtained from the fit. The lower panel shows the ratio between the observed and expected events in each bin.

Observed $m_{\tau\tau}$ distribution in the $\mu\tau_\mathrm{h}$ channel of the 1b1c category, compared to the expected SM background contributions. The distributions of the qbX signal with $m_{\mathrm{B}}=170~\mathrm{GeV}$, and X boson mass 40 and 60 GeV are overlaid to illustrate the sensitivity. They are normalized to the cross section times branching fraction of 20 pb. The uncertainty band represents the sum in quadrature of statistical and systematic uncertainties obtained from the fit. The lower panel shows the ratio between the observed and expected events in each bin.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for the prodcution of the qbX signal with mB = 170 GeV and the branching fraction $\mathrm{X} \rightarrow \tau\tau$, obtained from the combination of the $\mathrm{e}\tau_\mathrm{h}$ and $\mu\tau_\mathrm{h}$ channels, and the 1b1f and 1b1c categories, as a function of the X boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for the prodcution of the qbX signal with mB = 300 GeV and the branching fraction $\mathrm{X} \rightarrow \tau\tau$, obtained from the combination of the $\mathrm{e}\tau_\mathrm{h}$ and $\mu\tau_\mathrm{h}$ channels, and the 1b1f and 1b1c categories, as a function of the X boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for the prodcution of the qbX signal with mB = 450 GeV and the branching fraction $\mathrm{X} \rightarrow \tau\tau$, obtained from the combination of the $\mathrm{e}\tau_\mathrm{h}$ and $\mu\tau_\mathrm{h}$ channels, and the 1b1f and 1b1c categories, as a function of the X boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for the prodcution of the qbX signal with mB = 170 GeV and the branching fraction $\mathrm{X} \rightarrow \tau\tau$, obtained in the $\mathrm{e}\tau_\mathrm{h}$ channel of the 1b1f category, as a function of the X boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for the prodcution of the qbX signal with mB = 170 GeV and the branching fraction $\mathrm{X} \rightarrow \tau\tau$, obtained in the $\mathrm{e}\tau_\mathrm{h}$ channel of the 1b1c category, as a function of the X boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for the prodcution of the qbX signal with mB = 170 GeV and the branching fraction $\mathrm{X} \rightarrow \tau\tau$, obtained in the $\mu\tau_\mathrm{h}$ channel of the 1b1f category, as a function of the X boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

Observed (black solid) and expected (black dotted) limits at 95% confidence level on the product of the the cross section for the prodcution of the qbX signal with mB = 170 GeV and the branching fraction $\mathrm{X} \rightarrow \tau\tau$, obtained in the $\mu\tau_\mathrm{h}$ channel of the 1b1c category, as a function of the X boson mass. The green and yellow bands represent the one and two standard deviation uncertainties in the expected limits.

Gluino - neutralino mass points lying on the observed $+1\sigma_{theory}$ exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the observed $-1\sigma_{theory}$ exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the expected exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the expected $+1\sigma_{exp}$ exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the expected $-1\sigma_{exp}$ exclusion contour of T5qqqqHG model.

Observed $95\%$ CL upper limit on the production cross section of gluinos in T5bbbbZG model.

Expected $95\%$ CL upper limit on the production cross section of gluinos in T5bbbbZG model.

Gluino - neutralino mass points lying on the observed exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the observed $+1\sigma_{theory}$ exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the observed $-1\sigma_{theory}$ exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the expected exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the expected $+1\sigma_{exp}$ exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the expected $-1\sigma_{exp}$ exclusion contour of T5qqqqHG model.

Observed $95\%$ CL upper limit on the production cross section of gluinos in T5ttttZG model.

Expected $95\%$ CL upper limit on the production cross section of gluinos in T5ttttZG model.

Gluino - neutralino mass points lying on the observed exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the observed $+1\sigma_{theory}$ exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the observed $-1\sigma_{theory}$ exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the expected exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the expected $+1\sigma_{exp}$ exclusion contour of T5qqqqHG model.

Gluino - neutralino mass points lying on the expected $-1\sigma_{exp}$ exclusion contour of T5qqqqHG model.

Observed $95\%$ CL upper limit on the production cross section of gluinos in T6ttZG model.

Expected $95\%$ CL upper limit on the production cross section of gluinos in T6ttZG model.

Stop - neutralino mass points lying on the observed exclusion contour of T5qqqqHG model.

Stop - neutralino mass points lying on the observed $+1\sigma_{theory}$ exclusion contour of T5qqqqHG model.

Stop - neutralino mass points lying on the observed $-1\sigma_{theory}$ exclusion contour of T5qqqqHG model.

Stop - neutralino mass points lying on the expected exclusion contour of T5qqqqHG model.

Stop - neutralino mass points lying on the expected $+1\sigma_{exp}$ exclusion contour of T5qqqqHG model.

Stop - neutralino mass points lying on the expected $-1\sigma_{exp}$ exclusion contour of T5qqqqHG model.

The distributions of likelihood discriminant for data, simulated QCD multijet events, and simulated signal events. Data and simulated events are selected with the displaced-jet trigger. The offline $H_{T}$ is required to be larger than 400 GeV, and the jets are required to have $p_{T}>50\ \mathrm{GeV}$ and $|\eta|<2.0$. Three benchmark signal distributions are shown (dashed lines) for the jet-jet model with $m_{X}=300\ \mathrm{GeV}$ and varying lifetimes. For visualization each signal process is given a cross section, $\sigma$, such that $\sigma\ 35.9 \mathrm{fb}^{-1} = 1 \times 10^{6}$.

Numbers of predicted and observed background events for the nominal background method and the three cross-checks in the control region. Shown are the comparisons for likelihood discriminant thresholds of 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, and 0.9. The error bars represent the statistical uncertainties of the predictions and the observations. The data points at different likelihood discriminant thresholds are correlated, since the events passing higher likelihood discriminant thresholds also pass lower likelihood discriminant thresholds.

Numbers of predicted and observed background events for the nominal background method and the three cross-checks in the control region. Shown are the comparisons for likelihood discriminant thresholds of 0.95, 0.96, 0.97, 0.98, 0.99, and 0.9993. The error bars represent the statistical uncertainties of the predictions and the observations. The data points at different likelihood discriminant thresholds are correlated, since the events passing higher likelihood discriminant thresholds also pass lower likelihood discriminant thresholds.

The expected and observed $95\%$ $\text{CL}$ upper limits on the pair production cross section of the long-lived particle X, assuming a $100\%$ branching fraction for X to decay to a quark-antiquark pair, shown at different masses and different proper decay lengths for the jet-jet model.

the expected and observed $95\%$ $\text{CL}$ upper limits on the pair production cross section of the long-lived gluino, assuming a $100\%$ branching fraction for $\widetilde{\mathrm{g}}\to\mathrm{g}\widetilde{\mathrm{G}}$ decays.

the expected and observed $95\%$ $\text{CL}$ limits for the long-lived gluino model in the mass-lifetime plane, assuming a $100\%$ branching fraction for $\widetilde{\mathrm{g}}\to\mathrm{g}\widetilde{\mathrm{G}}$ decays, based on the NLO+NLL calculation of the gluino pair production cross section at $\sqrt{s}=13\ \mathrm{TeV}$.

the expected and observed $95\%$ $\text{CL}$ upper limits on the pair production cross section of the long-lived gluino, assuming a $100\%$ branching fraction for $\widetilde{\mathrm{g}}\to\mathrm{tbs}$ decays.

the expected and observed $95\%$ $\text{CL}$ limits for the long-lived gluino model in the mass-lifetime plane, assuming a $100\%$ branching fraction for $\widetilde{\mathrm{g}}\to\mathrm{tbs}$ decays, based on the NLO+NLL calculation of the gluino pair production cross section at $\sqrt{s}=13\ \mathrm{TeV}$.

the expected and observed $95\%$ $\text{CL}$ upper limits on the pair production cross section of the long-lived top squark, assuming a $100\%$ branching fraction for $\widetilde{\mathrm{t}}\to\mathrm{b}\ell$ decays.

the expected and observed $95\%$ $\text{CL}$ limits for the long-lived top squark model in the mass-lifetime plane, assuming a $100\%$ branching fraction for $\widetilde{\mathrm{t}}\to\mathrm{b}\ell$ decays, based on the NLO+NLL calculation of the top squark pair production cross section at $\sqrt{s}=13\ \mathrm{TeV}$.

the expected and observed $95\%$ $\text{CL}$ upper limits on the the pair production cross section of the long-lived top squark, assuming a $100\%$ branching fraction for $\widetilde{\mathrm{t}}\to\mathrm{\overline{d}\overline{d}}$ decays.

the expected and observed $95\%$ $\text{CL}$ limits for the long-lived top squark model in the mass-lifetime plane, assuming a $100\%$ branching fraction for $\widetilde{\mathrm{t}}\to\mathrm{\overline{d}\overline{d}}$ decays, based on an NLO+NLL calculation of the top squark pair production cross section at $\sqrt{s}=13\ \mathrm{TeV}$.