Observed upper limits at 90% CL on the square of the kinetic mixing coefficient $\epsilon$ in the minimal model of a dark photon

Observed upper limits at 90% CL on the mixing angle $\theta_H$ for the type IV 2HDM+S scenario with fixed $tan\beta=0.5$

The combined efficiency of the dimuon scouting trigger and the MVA muon selection, averaged between 2017 and 2018, weighted by the integrated luminosity of each year. The trigger and selection efficiencies are also included in the table.

Theory cross-section times branching fraction to muons times acceptance for the dark photon and 2HDM+S models.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{1})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}^{\mathrm{add.}}_{2})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{2})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{add.}})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\Delta\mathrm{R}_{\mathrm{b}\mathrm{b}}^{\mathrm{avg}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}_{3})|$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}_{3})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}_{3})$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}_{3})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}_{4})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}_{4})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $H^{\mathrm{b}}_{\mathrm{T}}$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $H^{\mathrm{b}}_{\mathrm{T}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $|\eta(\mathrm{b}^{\mathrm{extra}}_{1})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{1})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}^{\mathrm{extra}}_{2})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{2})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{extra}})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $H^{\mathrm{j}}_{\mathrm{T}}$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $H^{\mathrm{j}}_{\mathrm{T}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\mathrm{m}_{\mathrm{b}\mathrm{b}}^{\mathrm{max}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $H^{\mathrm{light}}_{\mathrm{T}}$ in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $H^{\mathrm{light}}_{\mathrm{T}}$ in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $N_{\mathrm{jets}}$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $N_{\mathrm{jets}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $N_{\mathrm{b}}$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}^{\mathrm{add.}}_{1})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{1})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}^{\mathrm{add.}}_{2})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{2})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{add.}})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\Delta\mathrm{R}_{\mathrm{b}\mathrm{b}}^{\mathrm{avg}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}_{3})|$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}_{3})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}_{3})$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}_{3})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}_{4})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}_{4})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $H^{\mathrm{b}}_{\mathrm{T}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $H^{\mathrm{b}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}^{\mathrm{extra}}_{1})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{1})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}^{\mathrm{extra}}_{2})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{2})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{extra}})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $H^{\mathrm{j}}_{\mathrm{T}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $H^{\mathrm{j}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\mathrm{m}_{\mathrm{b}\mathrm{b}}^{\mathrm{max}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $H^{\mathrm{light}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $H^{\mathrm{light}}_{\mathrm{T}}$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $N_{\mathrm{jets}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $N_{\mathrm{jets}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $N_{\mathrm{b}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}^{\mathrm{add.}}_{1})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{1})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}^{\mathrm{add.}}_{2})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{2})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{add.}})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\Delta\mathrm{R}_{\mathrm{b}\mathrm{b}}^{\mathrm{avg}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}_{3})|$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}_{3})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}_{3})$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}_{3})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}_{4})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}_{4})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{b}}_{\mathrm{T}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{b}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}^{\mathrm{extra}}_{1})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{1})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}^{\mathrm{extra}}_{2})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{2})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{extra}})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{j}}_{\mathrm{T}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{j}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\mathrm{m}_{\mathrm{b}\mathrm{b}}^{\mathrm{max}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{light}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{light}}_{\mathrm{T}}$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $N_{\mathrm{jets}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $N_{\mathrm{jets}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $N_{\mathrm{b}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Fiducial cross sections from the measurements of all observables, compared to predictions from different ttbb simulation approaches. For each of the normalized differential measurements the fiducial cross section in the respective phase space is also determined. In the paper only one representative observable is quoted for each fiducial phase space, while here the measured cross section with the uncertainties from the fit to the respective observable is summarized.

'$\overline{\Lambda}$ $D_{LL}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'$\Lambda$ $D_{LL}$ as a function of $p_{T}$ at $-1.2 < \eta_{\Lambda(\overline{\Lambda})} < 0$'

'$\overline{\Lambda}$ $D_{LL}$ as a function of $p_{T}$ at $-1.2 < \eta_{\Lambda(\overline{\Lambda})} < 0$'

'$\Lambda$ $D_{LL}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'$\overline{\Lambda}$ $D_{LL}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'Two-year-combined $\Lambda$ $D_{LL}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'Two-year-combined $\overline{\Lambda}$ $D_{LL}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'Two-year-combined $\Lambda+\overline{\Lambda}$ $D_{LL}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'Two-year-combined $\Lambda$ $D_{LL}$ as a function of $p_{T}$ at $-1.2 < \eta_{\Lambda(\overline{\Lambda})} < 0$'

'Two-year-combined $\overline{\Lambda}$ $D_{LL}$ as a function of $p_{T}$ at $-1.2 < \eta_{\Lambda(\overline{\Lambda})} < 0$'

'$\Lambda$ $D_{LL}$ as a function of z at $0 < \eta_{jet} < 1.0$'

'$\overline{\Lambda}$ $D_{LL}$ as a function of z at $0 < \eta_{jet} < 1.0$'

'$\Lambda$ $D_{LL}$ as a function of z at $-1.0 < \eta_{jet} < 0$'

'$\overline{\Lambda}$ $D_{LL}$ as a function of z at $-1.0 < \eta_{jet} < 0$'

'particle jet pt as a function of $\Lambda$ z'

'particle jet pt as a function of $\overline{\Lambda}$ z'

'$\Lambda$ $D_{TT}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'$\overline{\Lambda}$ $D_{TT}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'$\Lambda$ $D_{TT}$ as a function of $p_{T}$ at $-1.2 < \eta_{\Lambda(\overline{\Lambda})} < 0$'

'$\overline{\Lambda}$ $D_{TT}$ as a function of $p_{T}$ at $-1.2 < \eta_{\Lambda(\overline{\Lambda})} < 0$'

'$\Lambda$ $D_{TT}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'$\overline{\Lambda}$ $D_{TT}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'Two-year-combined $\Lambda$ $D_{TT}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'Two-year-combined $\overline{\Lambda}$ $D_{TT}$ as a function of $p_{T}$ at $0 < \eta_{\Lambda(\overline{\Lambda})} < 1.2$'

'Two-year-combined $\Lambda$ $D_{TT}$ as a function of $p_{T}$ at $-1.2 < \eta_{\Lambda(\overline{\Lambda})} < 0$'

'Two-year-combined $\overline{\Lambda}$ $D_{TT}$ as a function of $p_{T}$ at $-1.2 < \eta_{\Lambda(\overline{\Lambda})} < 0$'

'$\Lambda$ $D_{TT}$ as a function of z at $0 < \eta_{jet} < 1.0$'

'$\overline{\Lambda}$ $D_{TT}$ as a function of z at $0 < \eta_{jet} < 1.0$'

'$\Lambda$ $D_{TT}$ as a function of z at $-1.0 < \eta_{jet} < 0$'

'$\overline{\Lambda}$ $D_{TT}$ as a function of z at $-1.0 < \eta_{jet} < 0$'

'particle jet pt as a function of $\Lambda$ z'

'particle jet pt as a function of $\overline{\Lambda}$ z'

$v_3\{\Psi_1\}$ vs. rapidity for protons in three large centrality bins from a symmetric acceptance across midrapidity in $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au collisions at STAR. Protons exhibit an increasingly negative slope as the centrality increases.

$v_3\{\Psi_1\}$ vs. rapidity for protons in three large centrality bins from only the backward region in $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au collisions at STAR. Note that the $p_{\mathrm{T}}$ acceptance extends to a lower limit than in Fig. 6.

$v_3\{\Psi_1\}$ vs. $p_{\mathrm{T}}$ for protons in three large centrality bins in $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au collisions at STAR. $v_3\{\Psi_1\}$ becomes increasingly negative as $p_{\mathrm{T}}$ and centrality increase.

Figure 2a, full-event

Figure 2b, subevent

Figure 3

Figure 4

I_{AA} of Au+Au 0%-15% collisions at sqrt{s_{NN}} = 200 GeV for R = 0.5 of pi^{0}+jet with E_{T,trig}= 11-15 GeV.

Yield Ratio R=0.2/R=0.5 of Au+Au 0%-15% collisions at sqrt{s_{NN}} = 200 GeV of gamma_{dir}+jet with E_{T,trig}= 15-20 GeV.

Yield Ratio R=0.2/R=0.5 of Au+Au 0%-15% collisions at sqrt{s_{NN}} = 200 GeV of pi^{0}+jet with E_{T,trig}= 11-15 GeV.

Yield Ratio R=0.2/R=0.5 of p+p collisions at sqrt{s_{NN}} = 200 GeV of gamma_{dir}+jet with E_{T,trig}= 15-20 GeV.

Yield Ratio R=0.2/R=0.5 of p+p collisions at sqrt{s_{NN}} = 200 GeV of pi^{0}+jet with E_{T,trig}= 11-15 GeV.

Rho distribution of ME+30MeV recoil jet R=0.5 for AuAu 0-15% at sqrt{s_{NN}}=200 GeV from MB event sample.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 11-15 GeV.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 11-15 GeV.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and gamma_{rich} E_{T,trig}= 9-11 GeV.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and gamma_{rich} E_{T,trig}= 11-15 GeV.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and gamma_{rich} E_{T,trig}= 15-20 GeV.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and gamma_{rich} E_{T,trig}= 9-11 GeV.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and gamma_{rich} E_{T,trig}= 11-15 GeV.

Per trigger recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and gamma_{rich} E_{T,trig}= 15-20 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma_{rich} E_{T,trig}= 9-11 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma_{rich} E_{T,trig}= 11-15 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma_{rich} E_{T,trig}= 15-20 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma_{rich} E_{T,trig}= 9-11 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma_{rich} E_{T,trig}= 11-15 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma_{rich} E_{T,trig}= 15-20 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma_{rich} E_{T,trig}= 9-11 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma_{rich} E_{T,trig}= 11-15 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma_{rich} E_{T,trig}= 15-20 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma_{rich} E_{T,trig}= 9-11 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma_{rich} E_{T,trig}= 11-15 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma_{rich} E_{T,trig}= 15-20 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 9-11 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 11-15 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 11-15 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 9-11 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger SE recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 11-15 GeV.

Ratio of SE and ME recoil jet distributions for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 11-15 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 9-11 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 11-15 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 15-20 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 9-11 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 11-15 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 15-20 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 11-15 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger ME-subtracted uncorrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 11-15 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 9-11 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 11-15 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 15-20 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 9-11 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 11-15 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 15-20 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 11-15 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger corrected recoil jet distribution for pp at sqrt{s}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 11-15 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 9-11 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 11-15 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 15-20 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 9-11 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 11-15 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 15-20 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 11-15 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 9-11 GeV.

Per trigger corrected recoil jet distribution for AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 11-15 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 9-11 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 11-15 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and gamma E_{T,trig}= 15-20 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 9-11 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 11-15 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and gamma E_{T,trig}= 15-20 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 9-11 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.5 and pi0 E_{T,trig}= 11-15 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 9-11 GeV.

I_AA AuAu 0-15% at sqrt{s_{NN}}=200 GeV with jet R=0.2 and pi0 E_{T,trig}= 11-15 GeV.

Yield Ratio R=0.2/R=0.5 pp at sqrt{s}=200 GeV pi0 E_{T,trig}= 9-11 GeV.

Yield Ratio R=0.2/R=0.5 pp at sqrt{s}=200 GeV pi0 E_{T,trig}= 11-15 GeV.

Yield Ratio R=0.2/R=0.5 pp at sqrt{s}=200 GeV gamma E_{T,trig}= 15-20 GeV.

Yield Ratio R=0.2/R=0.5 AuAu at sqrt{s_{NN}}=200 GeV pi0 E_{T,trig}= 9-11 GeV.

Yield Ratio R=0.2/R=0.5 AuAu at sqrt{s_{NN}}=200 GeV pi0 E_{T,trig}= 11-15 GeV.

Yield Ratio R=0.2/R=0.5 AuAu at sqrt{s_{NN}}=200 GeV gamma E_{T,trig}= 15-20 GeV.

Postfit distributions of $S_\mathrm{T}^\mathrm{MET}$ in the $\mathrm{e}\mu$ channel of the $\geq$1b category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width. The last bin includes the overflow.

Postfit distributions of $S_\mathrm{T}^\mathrm{MET}$ in the $\ell\tau_\mathrm{h}$ channel of the 0b category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width. The last bin includes the overflow.

Postfit distributions of $S_\mathrm{T}^\mathrm{MET}$ in the $\ell\tau_\mathrm{h}$ channel of the $\geq$1b category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width. The last bin includes the overflow.

Postfit distributions of $S_\mathrm{T}^\mathrm{MET}$ in the $\tau_\mathrm{h}\tau_\mathrm{h}$ channel of the 0b category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width. The last bin includes the overflow.

Postfit distributions of $S_\mathrm{T}^\mathrm{MET}$ in the $\tau_\mathrm{h}\tau_\mathrm{h}$ channel of the $\geq$1b category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width. The last bin includes the overflow.

Postfit distributions of $\chi$ in the $\mathrm{e}\mu$ channel of the 0j, $400 < m_\mathrm{vis} < 600\,\mathrm{GeV}$ category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width.

Postfit distributions of $\chi$ in the $\mathrm{e}\mu$ channel of the 0j, $m_\mathrm{vis} > 600\,\mathrm{GeV}$ category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width.

Postfit distributions of $\chi$ in the $\ell\tau_\mathrm{h}$ channel of the 0j, $400 < m_\mathrm{vis} < 600\,\mathrm{GeV}$ category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width.

Postfit distributions of $\chi$ in the $\ell\tau_\mathrm{h}$ channel of the 0j, $m_\mathrm{vis} > 600\,\mathrm{GeV}$ category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width.

Postfit distributions of $\chi$ in the $\tau_\mathrm{h}\tau_\mathrm{h}$ channel of the 0j, $400 < m_\mathrm{vis} < 600\,\mathrm{GeV}$ category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width.

Postfit distributions of $\chi$ in the $\tau_\mathrm{h}\tau_\mathrm{h}$ channel of the 0j, $m_\mathrm{vis} > 600\,\mathrm{GeV}$ category for the combined 2016-2018 data set after a simultaneous fit of the background and vector LQ signal to the data. The number of events in each bin are divided by the respective bin width.

Exclusion limits on the total cross section of a scalar LQ as a function of LQ mass under the assumption of exclusive LQ couplings to b quarks and $\tau$ leptons.

Exclusion limits on the total cross section of a vector LQ as a function of LQ mass under the assumption of exclusive LQ couplings to b quarks and $\tau$ leptons.

Exclusion limits on the mass of a scalar LQ as a function of the coupling strength $\lambda$ under the assumption of exclusive LQ couplings to b quarks and $\tau$ leptons.

Exclusion limits on the mass of a vector LQ as a function of the coupling strength $\lambda$ under the assumption of exclusive LQ couplings to b quarks and $\tau$ leptons.

Exclusion limits on the coupling strength $\lambda$ of a scalar LQ as a function of the LQ mass under the assumption of exclusive LQ couplings to b quarks and $\tau$ leptons.

Exclusion limits on the coupling strength $\lambda$ of a vector LQ as a function of the LQ mass under the assumption of exclusive LQ couplings to b quarks and $\tau$ leptons.