(Anti)proton spectrum in V0M multiplicity class IV - V

(Anti)proton spectrum in V0M multiplicity class VI

(Anti)proton spectrum in V0M multiplicity class VII

(Anti)proton spectrum in V0M multiplicity class VIII

(Anti)proton spectrum in V0M multiplicity class IX

(Anti)proton spectrum in V0M multiplicity class X

(Anti)proton spectrum in V0M multiplicity class INEL > 0

(Anti)deuteron spectrum in V0M multiplicity class I

(Anti)deuteron spectrum in V0M multiplicity class II

(Anti)deuteron spectrum in V0M multiplicity class III

(Anti)deuteron spectrum in V0M multiplicity class IV - V

(Anti)deuteron spectrum in V0M multiplicity class VI

(Anti)deuteron spectrum in V0M multiplicity class VII

(Anti)deuteron spectrum in V0M multiplicity class VIII

(Anti)deuteron spectrum in V0M multiplicity class IX

(Anti)deuteron spectrum in V0M multiplicity class X

(Anti)deuteron spectrum in V0M multiplicity class INEL > 0

(Anti)helion spectrum in V0M multiplicity class I - III

(Anti)helion spectrum in V0M multiplicity class IV - X

(Anti)helion spectrum in V0M multiplicity class INEL > 0

Mean transverse momentum $<p_\mathrm{T}>$ of protons as a function of the charged particle multiplicity density at mid-rapidity

Mean transverse momentum $<p_\mathrm{T}>$ of deuterons as a function of the charged particle multiplicity density at mid-rapidity

Mean transverse momentum $<p_\mathrm{T}>$ of helions as a function of the charged particle multiplicity density at mid-rapidity

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class I

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class II

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class III

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class IV - V

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class VI

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class VII

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class VIII

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class IX

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class X

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class INEL > 0

Coalescence parameter $B_3$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class I - III

Coalescence parameter $B_3$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class IV - X

Coalescence parameter $B_3$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class INEL > 0

Coalescence parameter $B_2$ as a function of the charged particle multiplicity density at mid-rapidity

Coalescence parameter $B_3$ as a function of the charged particle multiplicity density at mid-rapidity

Deuteron over proton ratio as a function of the charged particle multiplicity density at mid-rapidity

Helion over proton ratio as a function of the charged particle multiplicity density at mid-rapidity

The $m_{lJ}$ distribution in the boosted DY control region, muon channel.

The $m_{lljj}$ distribution in the resolved flavor control region.

The $m_{lJ}$ distribution in the boosted flavor control region, with electron jet.

The $m_{lJ}$ distribution in the boosted flavor control region, with muon jet

The $m_{lljj}$ distribution in the resolved signal region, electron channel.

The $m_{lljj}$ distribution in the resolved signal region, muon channel.

The $m_{lJ}$ distribution in the boosted signal region, electron channel.

The $m_{lJ}$ distribution in the boosted signal region, muon channel.

The expected and observed $95\%$ CL upper limits on the production cross section times the branching fraction $\sigma (\mathrm{p}\mathrm{p} \rightarrow W_{R}) \mathcal{B}(W_{R} \rightarrow \mathrm{e}\mathrm{e}\mathrm{q}\overline{\mathrm{q}'})$ for $m_{N} = m_{W_{R}}/2$ GeV in the electron channel. The red solid lines represent the values expected from the theory.

The expected and observed $95\%$ CL upper limits on the production cross section times the branching fraction $\sigma (\mathrm{p}\mathrm{p} \rightarrow W_{R}) \mathcal{B}(W_{R} \rightarrow \mathrm{e}\mathrm{e}\mathrm{q}\overline{\mathrm{q}'})$ for $m_{N} = m_{W_{R}}/2$ GeV in the muon channel. The red solid lines represent the values expected from the theory.

The expected and observed $95\%$ CL upper limits on the production cross section times the branching fraction $\sigma (\mathrm{p}\mathrm{p} \rightarrow W_{R}) \mathcal{B}(W_{R} \rightarrow \mathrm{e}\mathrm{e}\mathrm{q}\overline{\mathrm{q}'})$ for $m_{N} = 200$ GeV in the electron channel. The red solid lines represent the values expected from the theory.

The expected and observed $95\%$ CL upper limits on the production cross section times the branching fraction $\sigma (\mathrm{p}\mathrm{p} \rightarrow W_{R}) \mathcal{B}(W_{R} \rightarrow \mathrm{e}\mathrm{e}\mathrm{q}\overline{\mathrm{q}'})$ for $m_{N} = 200$ GeV in the muon channel. The red solid lines represent the values expected from the theory.

The observed $95\%$ CL upper limits on the production cross section times the branching fraction $\sigma (\mathrm{p}\mathrm{p} \rightarrow W_{R}) \mathcal{B}(W_{R} \rightarrow \mathrm{e}\mathrm{e}\mathrm{q}\overline{\mathrm{q}'})$ divided by the theory cross sections in the electron channel. The observed exclusions are shown for the resolved (solid green), boosted (solid blue), and combined (solid black) channels, along with the expected exclusion for the combined result (dotted black). The dash-dotted lines represent the one standard deviation of the expected exclusion. The observed exclusions from the previous search performed by the CMS Collaboration (arXiv:1803.11116) is also shown in magenta.

The observed $95\%$ CL upper limits on the production cross section times the branching fraction $\sigma (\mathrm{p}\mathrm{p} \rightarrow W_{R}) \mathcal{B}(W_{R} \rightarrow \mathrm{e}\mathrm{e}\mathrm{q}\overline{\mathrm{q}'})$ divided by the theory cross sections in the muon channel. The observed exclusions are shown for the resolved (solid green), boosted (solid blue), and combined (solid black) channels, along with the expected exclusion for the combined result (dotted black). The dash-dotted lines represent the one standard deviation of the expected exclusion. The observed exclusions from the previous search performed by the CMS Collaboration (arXiv:1803.11116) is also shown in magenta.

Relative uncertainties in the total yields of the signal and background predictions.

Covariance matrix for all bins used in the background-only fit of the electron channel of this analysis. There are 243 bins in total, 81 for every data-taking year. For every year, each region has nine bins and the bins are grouped by rergion in the following order: ee boosted DY CR, #mu-jet flavor CR, ee resolved DY CR, resolved flavor CR, ee boosted SR, ee resolved SR, #mu#mu boosted DY CR, e-jet flavor CR, and #mu#mu resolved DY CR.

Covariance matrix for all bins used in the background-only fit of the muon channel of this analysis. There are 243 bins in total, 81 for every data-taking year. For every year, each region has nine bins and the bins are grouped by rergion in the following order: ee boosted DY CR, #mu-jet flavor CR, ee resolved DY CR, #mu#mu boosted DY CR, e-jet flavor CR, $#mu#mu$ resolved DY CR, resolved flavor CR, #mu#mu boosted SR, and the #mu#mu resolved SR.

Predicted signal yields for the 2016 data-taking period, corresponding to $35.9\,\text{fb}^{-1}$, after the application of each search requirement for the $m_{W_{R}} = 0.3$, 0.4, and 0.5 TeV and $m_{N} = 0.2$ TeV signal hypotheses for the boosted , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2016 data-taking period, corresponding to $35.9\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (3.0,1.4)$ TeV signal hypothesis for the resolved , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2016 data-taking period, corresponding to $35.9\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (4.0,2.0)$ TeV signal hypothesis for the resolved , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2016 data-taking period, corresponding to $35.9\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (5.0,3.0)$ TeV signal hypothesis for the resolved , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2016 data-taking period, corresponding to $35.9\,\text{fb}^{-1}$, after the application of each search requirement for the $m_{W_{R}} = 0.3$, 0.4, and 0.5 TeV and $m_{N} = 0.2$ TeV signal hypotheses for the boosted , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2016 data-taking period, corresponding to $35.9\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (3.0,1.4)$ TeV signal hypothesis for the resolved , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2016 data-taking period, corresponding to $35.9\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (4.0,2.0)$ TeV signal hypothesis for the resolved , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2016 data-taking period, corresponding to $35.9\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (5.0,3.0)$ TeV signal hypothesis for the resolved , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2017 data-taking period, corresponding to $41.5\,\text{fb}^{-1}$, after the application of each search requirement for the $m_{W_{R}} = 0.3$, 0.4, and 0.5 TeV and $m_{N} = 0.2$ TeV signal hypotheses for the boosted , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2017 data-taking period, corresponding to $41.5\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (3.0,1.4)$ TeV signal hypothesis for the resolved , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2017 data-taking period, corresponding to $41.5\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (4.0,2.0)$ TeV signal hypothesis for the resolved , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2017 data-taking period, corresponding to $41.5\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (5.0,3.0)$ TeV signal hypothesis for the resolved , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2017 data-taking period, corresponding to $41.5\,\text{fb}^{-1}$, after the application of each search requirement for the $m_{W_{R}} = 0.3$, 0.4, and 0.5 TeV and $m_{N} = 0.2$ TeV signal hypotheses for the boosted , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2017 data-taking period, corresponding to $41.5\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (3.0,1.4)$ TeV signal hypothesis for the resolved , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2017 data-taking period, corresponding to $41.5\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (4.0,2.0)$ TeV signal hypothesis for the resolved , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2017 data-taking period, corresponding to $41.5\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (5.0,3.0)$ TeV signal hypothesis for the resolved , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2018 data-taking period, corresponding to $59.7\,\text{fb}^{-1}$, after the application of each search requirement for the $m_{W_{R}} = 0.3$, 0.4, and 0.5 TeV and $m_{N} = 0.2$ TeV signal hypotheses for the boosted , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2018 data-taking period, corresponding to $59.7\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (3.0,1.4)$ TeV signal hypothesis for the resolved , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2018 data-taking period, corresponding to $59.7\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (4.0,2.0)$ TeV signal hypothesis for the resolved , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2018 data-taking period, corresponding to $59.7\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (5.0,3.0)$ TeV signal hypothesis for the resolved , dielectron channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2018 data-taking period, corresponding to $59.7\,\text{fb}^{-1}$, after the application of each search requirement for the $m_{W_{R}} = 0.3$, 0.4, and 0.5 TeV and $m_{N} = 0.2$ TeV signal hypotheses for the boosted , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2018 data-taking period, corresponding to $59.7\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (3.0,1.4)$ TeV signal hypothesis for the resolved , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2018 data-taking period, corresponding to $59.7\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (4.0,2.0)$ TeV signal hypothesis for the resolved , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Predicted signal yields for the 2018 data-taking period, corresponding to $59.7\,\text{fb}^{-1}$, after the application of each search requirement for the $(m_{W_{R}},m_{N}) = (5.0,3.0)$ TeV signal hypothesis for the resolved , dimuon channel.The requirements listed are cumulative such that only the events and objects passing a given requirement are considered in subsequent requirements.

Cross sections calculated to next-to-leading (NLO) accuracy

The $p_{T}$ dependencies of $v_{1}$ within $-0.4<y<-0.1$ for $t$ in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity and $p_{T}$ dependencies of $v_{1}$ for $^{3}$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The $p_{T}$ dependencies of $v_{1}$ within $-0.1<y<0$ for $^4$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The $p_{T}$ dependencies of $v_{1}$ within $-0.4<y<-0.1$ for $^{4}$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity and $p_{T}$ dependencies of $v_{2}$ for $p$ in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity and $p_{T}$ dependencies of $v_{2}$ for $d$ in 10-40% mid-central Au+Au collisions at 3 GeV.

The $p_{T}$ dependencies of $v_{2}$ within $-0.1<y<0$ for $t$ in 10-40% mid-central Au+Au collisions at 3 GeV.

The $p_{T}$ dependencies of $v_{2}$ within $-0.4<y<-0.1$ for $t$ in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity and $p_{T}$ dependencies of $v_{2}$ for $^{3}$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The $p_{T}$ dependencies of $v_{2}$ within $-0.1<y<0$ for $^4$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The $p_{T}$ dependencies of $v_{2}$ within $-0.4<y<-0.1$ for $^{4}$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity dependencies of $v_{1}$ for $p$, $d$, and $^{3}$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity dependencies of $v_{1}$ for $t$ and $^{4}$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity dependencies of $v_{1}$ from JAM plus coalescence calculations in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity dependencies of $v_{2}$ for $p$, $d$, and $^{3}$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity dependencies of $v_{2}$ for $t$ and $^{4}$He in 10-40% mid-central Au+Au collisions at 3 GeV.

The rapidity dependencies of $v_{2}$ from JAM plus coalescence calculations in 10-40% mid-central Au+Au collisions at 3 GeV.

Light nucleus scaled $v_{1}$ slopes as a function os collision energy in 10-40 mid-cantral Au+Au collisions.

Light nucleus scaled $v_{1}$ slopes from JAM plus coalescence in 10-40 mid-cantral Au+Au collisions at 3 GeV.

Simultaneous EW and QCD WV signal strength fit.

The $\mathrm{\Lambda_c^+ / D^0}$ production yield ratio in central (0--10\%) and mid-central (30--50\%) Pb--Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$ TeV.

The nuclear modification factor of prompt $\mathrm{\Lambda_c^+}$ as a function transverse momentum in central (0--10\%) and mid-central (30--50\%) Pb--Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$ TeV.

The nuclear modification factor of prompt $\mathrm{\Lambda_c^+}$ as a function transverse momentum in central (0--10\%) and mid-central (30--50\%) Pb--Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$ TeV.

The $1\sigma_{\text{exp}}$ variation of the expected exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=1.0$.

The observed exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0.1$.

The expected exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0.1$.

The observed exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0.15$.

The expected exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0.15$.

The observed exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0.2$.

The expected exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0.2$.

The observed exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0.4$.

The expected exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0.4$.

The observed exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0.6$.

The expected exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=0p6$.

The observed exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=1.5$.

The expected exclusion contour at 95% CL as a function of the smuon and neutralino masses, for $\lambda_{231}^{'}=1.5$.

The observed exclusion contour at 95% CL as a function of the leptoquark mass and coupling strength.

The expected exclusion contour at 95% CL as a function of the leptoquark mass and coupling strength.

The minus $1\sigma_{\text{theory}}$ variation of the observed exclusion contour at 95% CL as a function of the leptoquark mass and coupling strength.

The plus $1\sigma_{\text{theory}}$ variation of the observed exclusion contour at 95% CL as a function of the leptoquark mass and coupling strength.

The $1\sigma_{\text{exp}}$ variation of the expected exclusion contour at 95% CL as a function of the leptoquark mass and coupling strength.

Observed yields, and fake lepton background yields in the $e^{+}\mu^{-}$ and $e^{-}\mu^{+}$ channels of SR-MET, along with the results of the $e^{+}\mu^{-}/e^{-}\mu^{+}$ ratio measurement and 1-sided p-value in SR-MET, binned in $M_{T2}$.

Observed yields, and fake lepton background yields in the $e^{+}\mu^{-}$ and $e^{-}\mu^{+}$ channels of SR-JET, along with the results of the $e^{+}\mu^{-}/e^{-}\mu^{+}$ ratio measurement and 1-sided p-value in SR-JET, binned in $H_{\text{P}}$.

Observed and expected 95% CL upper limits on the total number of signal events entering the $e^{+}\mu^{-}$ and $e^{-}\mu^{+}$ channels of each bin of SR-MET. The regions are binned in the same way as the ratio $\rho$ measurement. The limits are shown for a selection of 'z' values, where 'z' is the fraction of the total signal events entering the $e^{+}\mu^{-}$ channel.

Observed and expected 95% CL upper limits on the total number of signal events entering the $e^{+}\mu^{-}$ and $e^{-}\mu^{+}$ channels of each bin of SR-JET. The regions are binned in the same way as the ratio $\rho$ measurement. The limits are shown for a selection of 'z' values, where 'z' is the fraction of the total signal events entering the $e^{+}\mu^{-}$ channel.

Signal yields following each cut in the analysis, for representative $R$-parity-violating supersymmetry and leptoquark signals. All yields are MC generator-weighted and normalised to $139~\text{fb}^{-1}$. The cut labelled `Preselection' includes trigger requirements, and requires exactly one Baseline electron and one Baseline muon. At this point, the muon charge-bias correction weights are also applied. The $R$-parity-violating supersymmetry models were generated by specifying a top-quark in the final state and applying a two-lepton filter, hence the first row also includes events where the top quark decays to an electron.

Jet multiplicity in the selected events. The hatched band correspond to systematic and statistical uncertainties. The lower panels show the data-to-prediction ratio.

Inclusive ttbar cross section in pp collisions as a function of the center-of-mass energy; previous CMS measurements at 7, 8, and 13 TeV in the separate lepton+jets and dilepton channels are displayed, along with the combined measurement at 5.02 TeV presented in this analysis. The NNLO+NNLL theoretical prediction using the NNPDF3.1 PDF set with $alpha_{S}({m}_{Z})$ = 0.118 and ${m}_{t}$ = 172.5 GeV is shown in the main plot. In the inset, the combined measurement is shown together with previous measurements at 5.02 TeV, and additional predictions at 5.02 TeV using the MSHT20 , CT18, and ABMP16 NNLO PDF sets, the latter with $alpha_{S}({m}_{Z})$ = 0.115 and ${m}_{t}$ = 170.4 GeV, are compared, along with the NNPDF3.1 NNLO prediction, to the individual and combined results from this analysis. The vertical bars and bands represent the total uncertainties in the data and in the predictions, respectively. Points corresponding to measurements at the same center-of-mass energy are horizontally shifted for better readability.

Summary of the statistical and systematic uncertainty sources for the ttbar cross section measurement.

Event yields for all the processes at the final level of selection.

Excluded signal cross section at $95\%$ CL for Hut coupling. Each jet category and their combination are shown separately.

Excluded signal cross section at $95\%$ CL for Hut coupling. Each jet category and their combination are shown separately.

Observed upper limits on the branching fractions $\mathcal{B}(\mathrm{t}\to\mathrm{Hu})$ and $\mathcal{B}(\mathrm{t}\to\mathrm{Hc})$ at $95\%$ CL.

Expected upper limits on the branching fractions $\mathcal{B}(\mathrm{t}\to\mathrm{Hu})$ and $\mathcal{B}(\mathrm{t}\to\mathrm{Hc})$ at $95\%$ CL.

Expected +1 standard deviation upper limits on the branching fractions $\mathcal{B}(\mathrm{t}\to\mathrm{Hu})$ and $\mathcal{B}(\mathrm{t}\to\mathrm{Hc})$ at $95\%$ CL.

Expected -1 standard deviation upper limits on the branching fractions $\mathcal{B}(\mathrm{t}\to\mathrm{Hu})$ and $\mathcal{B}(\mathrm{t}\to\mathrm{Hc})$ at $95\%$ CL.

Expected +2 standard deviation upper limits on the branching fractions $\mathcal{B}(\mathrm{t}\to\mathrm{Hu})$ and $\mathcal{B}(\mathrm{t}\to\mathrm{Hc})$ at $95\%$ CL.

Expected -2 standard deviation upper limits on the branching fractions $\mathcal{B}(\mathrm{t}\to\mathrm{Hu})$ and $\mathcal{B}(\mathrm{t}\to\mathrm{Hc})$ at $95\%$ CL.

Observed upper limits on the anomalous couplings $\kappa_{\mathrm{Hut}}$ and $\kappa_{\mathrm{Hut}}$ at $95\%$ CL.

Expected upper limits on the anomalous couplings $\kappa_{\mathrm{Hut}}$ and $\kappa_{\mathrm{Hut}}$ at $95\%$ CL.

Expected +1 standard deviation upper limits on the anomalous couplings $\kappa_{\mathrm{Hut}}$ and $\kappa_{\mathrm{Hut}}$ at $95\%$ CL.

Expected -1 standard deviation upper limits on the anomalous couplings $\kappa_{\mathrm{Hut}}$ and $\kappa_{\mathrm{Hut}}$ at $95\%$ CL.

Expected +2 standard deviation upper limits on the anomalous couplings $\kappa_{\mathrm{Hut}}$ and $\kappa_{\mathrm{Hut}}$ at $95\%$ CL.

Expected -2 standard deviation upper limits on the anomalous couplings $\kappa_{\mathrm{Hut}}$ and $\kappa_{\mathrm{Hut}}$ at $95\%$ CL.