Ratio of differential UPC dimuon cross sections from data and STARlight shown as a function of $|y_{\mu\mu}|$ in the interval $10 < |m_{\mu\mu}| < 20$ GeV.

Ratio of differential UPC dimuon cross sections from data and STARlight shown as a function of $|y_{\mu\mu}|$ in the interval $20 < |m_{\mu\mu}| < 40$ GeV.

Ratio of differential UPC dimuon cross sections from data and STARlight 2.0 shown as a function of $|y_{\mu\mu}|$ in the interval $40 < |m_{\mu\mu}| < 80$ GeV.

Differential UPC dimuon cross sections shown as a function of $|m_{\mu\mu}|$ in the interval $0 < |y_{\mu\mu}| < 0.8$.

Differential UPC dimuon cross sections shown as a function of $|m_{\mu\mu}|$ in the interval $0.8 < |y_{\mu\mu}| < 1.6$.

Differential UPC dimuon cross sections shown as a function of $|m_{\mu\mu}|$ in the interval $1.6 < |y_{\mu\mu}| < 2.4$.

Ratio of differential UPC dimuon cross sections from data and STARlight shown as a function of $|m_{\mu\mu}|$ in the interval $0 < |y_{\mu\mu}| < 0.8$.

Ratio of differential UPC dimuon cross sections from data and STARlight shown as a function of $|m_{\mu\mu}|$ in the interval $0.8 < |y_{\mu\mu}| < 1.6$.

Ratio of differential UPC dimuon cross sections from data and STARlight 2.0 shown as a function of $|m_{\mu\mu}|$ in the interval $1.6 < |y_{\mu\mu}| < 2.4$.

Differential UPC dimuon cross sections shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $10 < |m_{\mu\mu}| < 20$ GeV.

Differential UPC dimuon cross sections shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $20 < |m_{\mu\mu}| < 40$ GeV.

Differential UPC dimuon cross sections shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $40 < |m_{\mu\mu}| < 80$ GeV.

Ratio of differential UPC dimuon cross sections from data and STARlight shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $10 < |m_{\mu\mu}| < 20$ GeV.

Ratio of differential UPC dimuon cross sections from data and STARlight shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $20 < |m_{\mu\mu}| < 40$ GeV.

Ratio of differential UPC dimuon cross sections from data and STARlight 2.0 shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $40 < |m_{\mu\mu}| < 80$ GeV.

Differential UPC dimuon cross sections shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $10 < |m_{\mu\mu}| < 20$ GeV and $|y_{\mu\mu}|<0.8$.

Differential UPC dimuon cross sections shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $20 < |m_{\mu\mu}| < 40$ GeV and $|y_{\mu\mu}|<0.8$.

Differential UPC dimuon cross sections shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $40 < |m_{\mu\mu}| < 80$ GeV and $|y_{\mu\mu}|<0.8$.

Ratio of differential UPC dimuon cross sections from data and STARlight shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $10 < |m_{\mu\mu}| < 20$ GeV and $|y_{\mu\mu}|<0.8$.

Ratio of differential UPC dimuon xsects from data and STARlight shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $20 < |m_{\mu\mu}| < 40$ GeV and $|y_{\mu\mu}|<0.8$.

Ratio of differential UPC dimuon cross sections from data and STARlight 2.0 shown as a function of $|\cos\theta^{\star}_{\mu\mu}|$ in the interval $40 < |m_{\mu\mu}| < 80$ GeV and $|y_{\mu\mu}|<0.8$.

Differential cross section as a function of k_max

Ratio of data/STARlight for differential cross sections as a function of k_max

Differential cross section as a function of k_min

Ratio of data/STARlight for differential cross sections as a function of k_min

Differential cross sections in $\alpha$ (acoplanarity) integrated over the full fiducial volume

Fraction of Xn0n events as a function of $m_{\mu\mu}$ for $0<|y_{\mu\mu}|<0.8$

Fraction of Xn0n events as a function of $y_{\mu\mu}$ for $10<|m_{\mu\mu}|<20$ GeV

Fraction of Xn0n events as a function of $m_{\mu\mu}$ for $0.8<|y_{\mu\mu}|<1.6$

Fraction of Xn0n events as a function of $y_{\mu\mu}$ for $20<|m_{\mu\mu}|<40$ GeV

Fraction of Xn0n events as a function of $m_{\mu\mu}$ for $1.6<|y_{\mu\mu}|<2.4$

Fraction of Xn0n events as a function of $y_{\mu\mu}$ for $40<|m_{\mu\mu}|<80$ GeV

Fraction of XnXn events as a function of $m_{\mu\mu}$ for $0<|y_{\mu\mu}|<0.8$

Fraction of XnXn events as a function of $y_{\mu\mu}$ for $10<|m_{\mu\mu}|<20$ GeV

Fraction of XnXn events as a function of $m_{\mu\mu}$ for $0.8<|y_{\mu\mu}|<1.6$

Fraction of XnXn events as a function of $y_{\mu\mu}$ for $20<|m_{\mu\mu}|<40$ GeV

Fraction of XnXn events as a function of $m_{\mu\mu}$ for $1.6<|y_{\mu\mu}|<2.4$

Fraction of XnXn events as a function of $y_{\mu\mu}$ for $40<|m_{\mu\mu}|<80$ GeV

Measured normalised differential fiducial cross sections of $\gamma\gamma \rightarrow \gamma\gamma$ production in Pb+Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV for diphoton $|cos(\theta*)|$ are shown as points with error bars giving the statistical uncertainty and grey bands indicating the size of the total uncertainty. The results are compared with the prediction from the SuperChic v3.0 MC generator (solid line).

Measured normalised differential fiducial cross sections of $\gamma\gamma \rightarrow \gamma\gamma$ production in Pb+Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV for average photon transverse momentum are shown as points with error bars giving the statistical uncertainty and grey bands indicating the size of the total uncertainty. The results are compared with the prediction from the SuperChic v3.0 MC generator (solid line) with bands denoting the theoretical uncertainty.

Measured normalised differential fiducial cross sections of $\gamma\gamma \rightarrow \gamma\gamma$ production in Pb+Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV for average photon transverse momentum are shown as points with error bars giving the statistical uncertainty and grey bands indicating the size of the total uncertainty. The results are compared with the prediction from the SuperChic v3.0 MC generator (solid line).

Measured differential fiducial cross sections of $\gamma\gamma \rightarrow \gamma\gamma$ production in Pb+Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV for diphoton rapidity are shown as points with error bars giving the statistical uncertainty and grey bands indicating the size of the total uncertainty. The results are compared with the prediction from the SuperChic v3.0 MC generator (solid line) with bands denoting the theoretical uncertainty.

Measured normalised differential fiducial cross sections of $\gamma\gamma \rightarrow \gamma\gamma$ production in Pb+Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV for diphoton rapidity are shown as points with error bars giving the statistical uncertainty and grey bands indicating the size of the total uncertainty. The results are compared with the prediction from the SuperChic v3.0 MC generator (solid line).

The 95% CL upper limit on the ALP cross section $\sigma_{\gamma\gamma\rightarrow a \rightarrow\gamma\gamma}$ for the $\gamma\gamma\rightarrow a \rightarrow \gamma\gamma$ process as a function of ALP mass m$_{a}$. The observed upper limit is shown as a solid black line and the expected upper limit is shown by the dashed black line with its $\pm1$ and $\pm2$ standard deviation bands. The discontinuity at $m_{a}=70 GeV$ is caused by the increase of the mass-bin width which brings an increase in signal acceptance.

The 95% CL upper limit on the ALP coupling $1/\Lambda_{a}$ for the $\gamma\gamma\rightarrow a \rightarrow \gamma\gamma$ process as a function of ALP mass m$_{a}$. The observed upper limit is shown as a solid black line and the expected upper limit is shown by the dashed black line with its $\pm1$ and $\pm2$ standard deviation bands. The discontinuity at $m_{a} = 70 GeV$ is caused by the increase of the mass-bin width which brings an increase in signal acceptance.

Ratio of unfolded width of azimuthal angular correlation distributions (P PB/ P P). Different colors correspond to different combinations of p_{T,1} and p_{T,2}

Ratio of unfolded Dijet conditional yields (P PB/ P P). Different colors correspond to different combinations of p_{T,1} and p_{T,2}

Unfolded width of azimuthal angular correlation distributions (Delta p_{T} > 3). Full markers represent p+Pb, open markers p+p

Unfolded Dijet conditional yields (Delta p_{T} > 3). Full markers represent p+Pb, open markers p+p

Ratio of unfolded width of azimuthal angular correlation distributions (P PB/ P P) (Delta p_{T} > 3). Different colors correspond to different combinations of p_{T,1} and p_{T,2}

Ratio of unfolded Dijet conditional yields (P PB/ P P) (Delta p_{T} > 3). Different colors correspond to different combinations of p_{T,1} and p_{T,2}

IRing2 for HT2>=500 GeV, NJets>=5

IRing2 for HT2>=1000 GeV, NJets>=2

IRing2 for HT2>=1000 GeV, NJets>=3

IRing2 for HT2>=1000 GeV, NJets>=4

IRing2 for HT2>=1000 GeV, NJets>=5

IRing2 for HT2>=1500 GeV, NJets>=2

IRing2 for HT2>=1500 GeV, NJets>=3

IRing2 for HT2>=1500 GeV, NJets>=4

IRing2 for HT2>=1500 GeV, NJets>=5

IRing128 for HT2>=500 GeV, NJets>=2

IRing128 for HT2>=500 GeV, NJets>=3

IRing128 for HT2>=500 GeV, NJets>=4

IRing128 for HT2>=500 GeV, NJets>=5

IRing128 for HT2>=1000 GeV, NJets>=2

IRing128 for HT2>=1000 GeV, NJets>=3

IRing128 for HT2>=1000 GeV, NJets>=4

IRing128 for HT2>=1000 GeV, NJets>=5

IRing128 for HT2>=1500 GeV, NJets>=2

IRing128 for HT2>=1500 GeV, NJets>=3

IRing128 for HT2>=1500 GeV, NJets>=4

IRing128 for HT2>=1500 GeV, NJets>=5

ICyl16 for HT2>=500 GeV, NJets>=2

ICyl16 for HT2>=500 GeV, NJets>=3

ICyl16 for HT2>=500 GeV, NJets>=4

ICyl16 for HT2>=500 GeV, NJets>=5

ICyl16 for HT2>=1000 GeV, NJets>=2

ICyl16 for HT2>=1000 GeV, NJets>=3

ICyl16 for HT2>=1000 GeV, NJets>=4

ICyl16 for HT2>=1000 GeV, NJets>=5

ICyl16 for HT2>=1500 GeV, NJets>=2

ICyl16 for HT2>=1500 GeV, NJets>=3

ICyl16 for HT2>=1500 GeV, NJets>=4

ICyl16 for HT2>=1500 GeV, NJets>=5

IRing2 covariance for HT2>=500 GeV, NJets>=2 (Table 1)

IRing2 covariance for HT2>=500 GeV, NJets>=3 (Table 2)

IRing2 covariance for HT2>=500 GeV, NJets>=4 (Table 3)

IRing2 covariance for HT2>=500 GeV, NJets>=5 (Table 4)

IRing2 covariance for HT2>=1000 GeV, NJets>=2 (Table 5)

IRing2 covariance for HT2>=1000 GeV, NJets>=3 (Table 6)

IRing2 covariance for HT2>=1000 GeV, NJets>=4 (Table 7)

IRing2 covariance for HT2>=1000 GeV, NJets>=5 (Table 8)

IRing2 covariance for HT2>=1500 GeV, NJets>=2 (Table 9)

IRing2 covariance for HT2>=1500 GeV, NJets>=3 (Table 10)

IRing2 covariance for HT2>=1500 GeV, NJets>=4 (Table 11)

IRing2 covariance for HT2>=1500 GeV, NJets>=5 (Table 12)

IRing128 covariance for HT2>=500 GeV, NJets>=2 (Table 13)

IRing128 covariance for HT2>=500 GeV, NJets>=3 (Table 14)

IRing128 covariance for HT2>=500 GeV, NJets>=4 (Table 15)

IRing128 covariance for HT2>=500 GeV, NJets>=5 (Table 16)

IRing128 covariance for HT2>=1000 GeV, NJets>=2 (Table 17)

IRing128 covariance for HT2>=1000 GeV, NJets>=3 (Table 18)

IRing128 covariance for HT2>=1000 GeV, NJets>=4 (Table 19)

IRing128 covariance for HT2>=1000 GeV, NJets>=5 (Table 20)

IRing128 covariance for HT2>=1500 GeV, NJets>=2 (Table 21)

IRing128 covariance for HT2>=1500 GeV, NJets>=3 (Table 22)

IRing128 covariance for HT2>=1500 GeV, NJets>=4 (Table 23)

IRing128 covariance for HT2>=1500 GeV, NJets>=5 (Table 24)

ICyl16 covariance for HT2>=500 GeV, NJets>=2 (Table 25)

ICyl16 covariance for HT2>=500 GeV, NJets>=3 (Table 26)

ICyl16 covariance for HT2>=500 GeV, NJets>=4 (Table 27)

ICyl16 covariance for HT2>=500 GeV, NJets>=5 (Table 28)

ICyl16 covariance for HT2>=1000 GeV, NJets>=2 (Table 29)

ICyl16 covariance for HT2>=1000 GeV, NJets>=3 (Table 30)

ICyl16 covariance for HT2>=1000 GeV, NJets>=4 (Table 31)

ICyl16 covariance for HT2>=1000 GeV, NJets>=5 (Table 32)

ICyl16 covariance for HT2>=1500 GeV, NJets>=2 (Table 33)

ICyl16 covariance for HT2>=1500 GeV, NJets>=3 (Table 34)

ICyl16 covariance for HT2>=1500 GeV, NJets>=4 (Table 35)

ICyl16 covariance for HT2>=1500 GeV, NJets>=5 (Table 36)

IRing2 covariance, complete

1-IRing128 covariance, complete

1-ICyl16 covariance, complete

$p_{T, jet}$ resolution for $20 < p_{T, jet}^{GEN} < 40$ GeV/c $R=0.4$ full jets. Jets are measured from all angles relative to the event plane in the 20-50% most central events.

Response matrix showing correlation between GEN and RECO $p_{T, jet}$ for matched GEN-level to RECO-level jets. Jets are measured from all angles relative to the event plane in the 20-50% most central events.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c in-plane jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c mid-plane jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c out-of-plane jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c JEWEL (with recoils) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c JEWEL (no recoils) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c in-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c mid-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c out-of-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c JEWEL (with recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 15-20 GeV/c JEWEL (no recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c in-plane jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c mid-plane jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c out-of-plane jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c JEWEL (with recoils) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c JEWEL (no recoils) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c in-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c mid-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c out-of-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c JEWEL (with recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 15-20 GeV/c JEWEL (no recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c in-plane jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c mid-plane jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c out-of-plane jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c JEWEL (with recoils) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c JEWEL (no recoils) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c in-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c mid-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c out-of-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c JEWEL (with recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of near-side associated charged hadrons for 20-40 GeV/c JEWEL (no recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c in-plane jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c mid-plane jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c out-of-plane jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c JEWEL (with recoils) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c JEWEL (no recoils) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c in-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c mid-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c out-of-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c JEWEL (with recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Yield measurement of away-side associated charged hadrons for 20-40 GeV/c JEWEL (no recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c in-plane jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c mid-plane jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c out-of-plane jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c JEWEL (with recoils) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c JEWEL (no recoils) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c in-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c mid-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c out-of-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c JEWEL (with recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 15-20 GeV/c JEWEL (no recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c in-plane jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c mid-plane jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c out-of-plane jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c JEWEL (with recoils) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c JEWEL (no recoils) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c in-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c mid-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c out-of-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c JEWEL (with recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 15-20 GeV/c JEWEL (no recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c in-plane jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c mid-plane jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c out-of-plane jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c JEWEL (with recoils) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c JEWEL (no recoils) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c in-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c mid-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c out-of-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c JEWEL (with recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of near-side associated charged hadrons for 20-40 GeV/c JEWEL (no recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c in-plane jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c mid-plane jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c out-of-plane jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c JEWEL (with recoils) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c JEWEL (no recoils) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c in-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c mid-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c out-of-plane ($p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c JEWEL (with recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

Width measurement of away-side associated charged hadrons for 20-40 GeV/c JEWEL (no recoils, $p_{T, assoc}$ inclusive) jets from 20-50% centrality collisions.

mid-plane/in-plane ratio of near-side yields associated charged hadrons for 15-20 GeV/c jets from 20-50% centrality collisions.

out-of-plane/in-plane ratio of near-side yields associated charged hadrons for 15-20 GeV/c jets from 20-50% centrality collisions.

mid-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of near-side yields associated charged hadrons for 15-20 GeV/c jets from 20-50% centrality collisions.

out-of-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of near-side yields associated charged hadrons for 15-20 GeV/c jets from 20-50% centrality collisions.

mid-plane/in-plane ratio of away-side yields associated charged hadrons for 15-20 GeV/c jets from 20-50% centrality collisions.

out-of-plane/in-plane ratio of away-side yields associated charged hadrons for 15-20 GeV/c jets from 20-50% centrality collisions.

mid-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of away-side yields associated charged hadrons for 15-20 GeV/c jets from 20-50% centrality collisions.

out-of-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of away-side yields associated charged hadrons for 15-20 GeV/c jets from 20-50% centrality collisions.

mid-plane/in-plane ratio of near-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.

out-of-plane/in-plane ratio of near-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.

mid-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of near-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.

out-of-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of near-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.

mid-plane/in-plane ratio of away-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.

out-of-plane/in-plane ratio of away-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.

mid-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of away-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.

out-of-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of away-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.

Proton cumulants as a function of reference multiplicity (black circles) from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Centrality-binned results with and without centrality bin width corrections are represented by red circles and blue squares, respectively. Vertical dashed lines indicate the centrality classes, from right to left: 0–5%, 5–10%, 10–20%. Data points in this figure are only corrected for detector efficiency but not for the pileup effect, which will be discussed in a later section.

Proton cumulants as a function of reference multiplicity (black circles) from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Centrality-binned results with and without centrality bin width corrections are represented by red circles and blue squares, respectively. Vertical dashed lines indicate the centrality classes, from right to left: 0–5%, 5–10%, 10–20%. Data points in this figure are only corrected for detector efficiency but not for the pileup effect, which will be discussed in a later section.

Proton cumulants as a function of reference multiplicity from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Pileup corrected and uncorrected cumulants as a function of reference multiplicity are represented by black circles and blue open squares, respectively. Red circles and blue-filled squares represent the results of centrality binned data.

Proton cumulants as a function of reference multiplicity from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Pileup corrected and uncorrected cumulants as a function of reference multiplicity are represented by black circles and blue open squares, respectively. Red circles and blue-filled squares represent the results of centrality binned data.

Ratios of proton cumulants as a function of reference multiplicity from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Pileup corrected and uncorrected cumulants are represented by black circles and blue open squares, respectively. Red circles and blue-filled squares represent the results of centrality binned data.

Ratios of proton cumulants as a function of reference multiplicity from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Pileup corrected and uncorrected cumulants are represented by black circles and blue open squares, respectively. Red circles and blue-filled squares represent the results of centrality binned data.

UrQMD results of the proton cumulant ratios up to sixth order in Au+Au collisions at $\sqrt{s_{\rm NN}}$= 3 GeV. The black circles are without VF correction while blue squares and red triangles are results with VFC which used $N_{\rm part}$ distributions from UrQMD and Glauber models, respectively. The blue crosses are calculations using UrQMD events with b $\leq$ 3 fm. The above results are applied CBWC except for the one (blue crosses) using b $\leq$3 fm events.

UrQMD results of the proton cumulant ratios up to sixth order in Au+Au collisions at $\sqrt{s_{\rm NN}}$= 3 GeV. The black circles are without VF correction while blue squares and red triangles are results with VFC which used $N_{\rm part}$ distributions from UrQMD and Glauber models, respectively. The blue crosses are calculations using UrQMD events with b $\leq$ 3 fm. The above results are applied CBWC except for the one (blue crosses) using b $\leq$3 fm events.

Proton cumulants up to sixth order in $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Data without volume fluctuation correction is shown as grey open squares while data with volume fluctuation correction using $N_{\rm part}$ distributions from Glauber and UrQMD models are shown as black circles and black open triangles, respectively. The corresponding centrality binned cumulants are shown in blue squares, red circles, and orange triangles, respectively. Similarly to Fig. 6, the vertical dashed lines indicate the centrality classes.

Proton cumulants up to sixth order in $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Data without volume fluctuation correction is shown as grey open squares while data with volume fluctuation correction using $N_{\rm part}$ distributions from Glauber and UrQMD models are shown as black circles and black open triangles, respectively. The corresponding centrality binned cumulants are shown in blue squares, red circles, and orange triangles, respectively. Similarly to Fig. 6, the vertical dashed lines indicate the centrality classes.

Proton cumulant ratios up to sixth order in $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Data without volume fluctuation correction are shown as grey open squares while data with volume fluctuation correction using $N_{\rm part}$ distributions from Glauber and UrQMD models are shown as black circles and black open triangles, respectively. The corresponding centrality binned cumulants are shown in blue squares, red circles, and orange triangles, respectively. Similarly to Fig. 6, the vertical dashed lines indicate the centrality classes.

Proton cumulant ratios up to sixth order in $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Data without volume fluctuation correction are shown as grey open squares while data with volume fluctuation correction using $N_{\rm part}$ distributions from Glauber and UrQMD models are shown as black circles and black open triangles, respectively. The corresponding centrality binned cumulants are shown in blue squares, red circles, and orange triangles, respectively. Similarly to Fig. 6, the vertical dashed lines indicate the centrality classes.

UrQMD results of proton cumulant ratios up to sixth order in Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. The vertical dashed lines indicate the centrality classes.

Experimental results on centrality dependence of cumulants (left panels) and cumulant ratios (right panels) up to sixth order of the proton multiplicity distributions in Au+Au collisions at $N_{\rm part}$ = 3 GeV. The open squares are data without VF correction while red circles and blue triangles are results with VF correction with $N_{\rm part}$ distributions from Glauber and UrQMD models, respectively.

Experimental results on centrality dependence of cumulants (left panels) and cumulant ratios (right panels) up to sixth order of the proton multiplicity distributions in Au+Au collisions at $N_{\rm part}$ = 3 GeV. The open squares are data without VF correction while red circles and blue triangles are results with VF correction with $N_{\rm part}$ distributions from Glauber and UrQMD models, respectively.

Same as Fig. 14 but for correlation function (left panels) and their normalized ratios (right panels).

Same as Fig. 14 but for correlation function (left panels) and their normalized ratios (right panels).

Cumulants and cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. The transverse momentum window is $p_{\rm T}$ from $0.4<p_{\rm T}<2.0$ GeV/$c$ and the rapidity window is $−0.5<y<0$. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD predictions are depicted by gold bands.

Cumulants and cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. The transverse momentum window is $p_{\rm T}$ from $0.4<p_{\rm T}<2.0$ GeV/$c$ and the rapidity window is $−0.5<y<0$. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD predictions are depicted by gold bands.

Same as Fig. 16 but for correlation functions and correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

Same as Fig. 16 but for correlation functions and correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

The transverse-momentum and rapidity dependence of cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. In the left column, the $p_{\rm T}$ analysis window is $0.4<p_{\rm T}<2.0$ GeV/$c$ while the rapidity window is varied in the range $y_{\rm min}<y<0$. In the right column, the rapidit$y$ analysis window is $−0.5<y<0$ while the $p_{\rm T}$ is varied in the range $0.4<p_{\rm T}<p_{\rm T}^{\rm max}$ GeV/$c$. The most central (0–5%) and peripheral (50–60%) events are depicted by black squares and blue triangles, respectively. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD simulations for the top 0–5% and 50–60% are shown by gold and blue bands, respectively.

The transverse-momentum and rapidity dependence of cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. In the left column, the $p_{\rm T}$ analysis window is $0.4<p_{\rm T}<2.0$ GeV/$c$ while the rapidity window is varied in the range $y_{\rm min}<y<0$. In the right column, the rapidit$y$ analysis window is $−0.5<y<0$ while the $p_{\rm T}$ is varied in the range $0.4<p_{\rm T}<p_{\rm T}^{\rm max}$ GeV/$c$. The most central (0–5%) and peripheral (50–60%) events are depicted by black squares and blue triangles, respectively. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD simulations for the top 0–5% and 50–60% are shown by gold and blue bands, respectively.

The transverse-momentum and rapidity dependence of cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. In the left column, the $p_{\rm T}$ analysis window is $0.4<p_{\rm T}<2.0$ GeV/$c$ while the rapidity window is varied in the range $y_{\rm min}<y<0$. In the right column, the rapidit$y$ analysis window is $−0.5<y<0$ while the $p_{\rm T}$ is varied in the range $0.4<p_{\rm T}<p_{\rm T}^{\rm max}$ GeV/$c$. The most central (0–5%) and peripheral (50–60%) events are depicted by black squares and blue triangles, respectively. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD simulations for the top 0–5% and 50–60% are shown by gold and blue bands, respectively.

The transverse-momentum and rapidity dependence of cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. In the left column, the $p_{\rm T}$ analysis window is $0.4<p_{\rm T}<2.0$ GeV/$c$ while the rapidity window is varied in the range $y_{\rm min}<y<0$. In the right column, the rapidit$y$ analysis window is $−0.5<y<0$ while the $p_{\rm T}$ is varied in the range $0.4<p_{\rm T}<p_{\rm T}^{\rm max}$ GeV/$c$. The most central (0–5%) and peripheral (50–60%) events are depicted by black squares and blue triangles, respectively. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD simulations for the top 0–5% and 50–60% are shown by gold and blue bands, respectively.

As in Fig. 18 but for transverse-momentum and rapidity dependence of correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

As in Fig. 18 but for transverse-momentum and rapidity dependence of correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

As in Fig. 18 but for transverse-momentum and rapidity dependence of correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

As in Fig. 18 but for transverse-momentum and rapidity dependence of correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

This dataset corresponds to Figure 2, the v2 ratio value estimated between epd (\Psi_1) and tpc (\Psi_2) in the paper

This dataset corresponds to Figure 2, the v2 ratio value estimated between epd (\Psi_1) and epd (\Psi_2) in the paper

This dataset corresponds to Figure 3, the \Delta\gamma_{112}multiply N_{part} value estimated by tpc (\Psi_2) in the paper

This dataset corresponds to Figure 3, the \Delta\gamma_{112}multiply N_{part} value estimated by epd (\Psi_2) in the paper

This dataset corresponds to Figure 3, the \Delta\gamma_{1111}multiply N_{part} value estimated by epd (\Psi_1) in the paper

This dataset corresponds to Figure 3, the ratio between \Delta\gamma_{1111} (by epd \Psi_1) and \Delta\gamma(112) (by tpc \Psi_2) in the paper

This dataset corresponds to Figure 3, the ratio between \Delta\gamma_{1111} (by epd \Psi_1) and \Delta\gamma(112) (by epd \Psi_2) in the paper

This dataset corresponds to Figure 4, the \Delta\gamma_{112}multiply N_{part} and scaled by v_2 estimated by tpc (\Psi_2) in the paper

This dataset corresponds to Figure 4, the \Delta\gamma_{112}multiply N_{part} and scaled by v_2 estimated by epd (\Psi_2) in the paper

This dataset corresponds to Figure 4, the \Delta\gamma_{1111}multiply N_{part} and scaled by v_2 estimated by epd (\Psi_1) in the paper

This dataset corresponds to Figure 4, the ratio between \Delta\gamma_{1111} scaled by v_{211} (by epd \Psi_1) and \Delta\gamma(112) scaled by v_2 (by tpc \Psi_2) in the paper

This dataset corresponds to Figure 4, the ratio between \Delta\gamma_{1111} scaled by v_{211} (by epd \Psi_1) and \Delta\gamma(112) scaled by v_2 (by epd \Psi_2) in the paper

Expected and observed $95\%$ CL limits on the absolute value of the up-type quark coupling parameter $|\zeta_\mathrm{u}|$ for masses of the $A$ boson ranging from $20$ to $90\,\mathrm{GeV}$.

Observed $p_0$ values for the fits on the production cross-section for $gg\rightarrow A$ times the branching ratio for $A$ decaying into two $\tau$-leptons for $A$ boson masses from $20$ to $90\,\mathrm{GeV}$. For the fit on the up-type quark coupling parameter the $p_0$ values agree up to a precision of $O(10^{-5})$.

Results for full matrix measurement differential in $m(t\bar{t})$

Results for full matrix measurement differential in $m(t\bar{t})$ for $|cos(\theta)| < 0.4$

Results for full matrix measurement differential in $p_{T}(t)$

Results for $D$ measurement inclusive from $m(t\bar{t})$

Results for $D$ measurement inclusive from $p_{T}(t)$

Results for $\tilde{D}$ measurement inclusive in $m(t\bar{t})$

Results for $\tilde{D}$ measurement inclusive in $p_{T}(t)$

Results for $D$ measurement differential in $m(t\bar{t})$

Results for $\tilde{D}$ measurement differential in $m(t\bar{t})$

Results for $\tilde{D}$ measurement differential in $m(t\bar{t})$ for $|cos(\theta)| < 0.4$

Results for $D$ measurement differential in $p_{T}(t)$

Results for $\tilde{D}$ measurement differential in $p_{T}(t)$