<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $p_{T,jet}^{lead}$ region of $2.5 \;\mathrm{GeV} < p_{T,jet}^{lead} < 7 \;\mathrm{GeV}$ for $N_{jet} \geq 3$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $p_{T,jet}^{lead}$ region of $7 \;\mathrm{GeV} < p_{T,jet}^{lead} < 12 \;\mathrm{GeV}$ for $N_{jet} \geq 1$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $p_{T,jet}^{lead}$ region of $7 \;\mathrm{GeV} < p_{T,jet}^{lead} < 12 \;\mathrm{GeV}$ for $N_{jet} \geq 2$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $p_{T,jet}^{lead}$ region of $7 \;\mathrm{GeV} < p_{T,jet}^{lead} < 12 \;\mathrm{GeV}$ for $N_{jet} \geq 3$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $p_{T,jet}^{lead}$ region of $12 \;\mathrm{GeV} < p_{T,jet}^{lead} < 30 \;\mathrm{GeV}$ for $N_{jet} \geq 1$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $p_{T,jet}^{lead}$ region of $12 \;\mathrm{GeV} < p_{T,jet}^{lead} < 30 \;\mathrm{GeV}$ for $N_{jet} \geq 2$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $p_{T,jet}^{lead}$ region of $12 \;\mathrm{GeV} < p_{T,jet}^{lead} < 30 \;\mathrm{GeV}$ for $N_{jet} \geq 3$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $Q^{2}$ region of $10 \;\mathrm{GeV}^{2} < Q^{2} < 50 \;\mathrm{GeV}^{2}$ for $N_{jet} \geq 1$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $Q^{2}$ region of $10 \;\mathrm{GeV}^{2} < Q^{2} < 50 \;\mathrm{GeV}^{2}$ for $N_{jet} \geq 2$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $Q^{2}$ region of $10 \;\mathrm{GeV}^{2} < Q^{2} < 50 \;\mathrm{GeV}^{2}$ for $N_{jet} \geq 3$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $Q^{2}$ region of $50 \;\mathrm{GeV}^{2} < Q^{2} < 100 \;\mathrm{GeV}^{2}$ for $N_{jet} \geq 1$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $Q^{2}$ region of $50 \;\mathrm{GeV}^{2} < Q^{2} < 100 \;\mathrm{GeV}^{2}$ for $N_{jet} \geq 2$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $Q^{2}$ region of $50 \;\mathrm{GeV}^{2} < Q^{2} < 100 \;\mathrm{GeV}^{2}$ for $N_{jet} \geq 3$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $Q^{2}$ region of $100 \;\mathrm{GeV}^{2} < Q^{2} < 350 \;\mathrm{GeV}^{2}$ for $N_{jet} \geq 1$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $Q^{2}$ region of $100 \;\mathrm{GeV}^{2} < Q^{2} < 350 \;\mathrm{GeV}^{2}$ for $N_{jet} \geq 2$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

<b>Note: in the paper, uncertainties are given in relative terms. The HEPData table contains absolute numbers. The original data file, containing relative uncertainties as in the paper, is available via the 'Resources' button above.</b> Differential cross sections, $d\sigma/d\Delta\phi$, in the $Q^{2}$ region of $100 \;\mathrm{GeV}^{2} < Q^{2} < 350 \;\mathrm{GeV}^{2}$ for $N_{jet} \geq 3$, as obtained from the data, ARIADNE MC simulations, and perturbative calculations at $\mathcal{O}(\alpha_{s})$ and $\mathcal{O}(\alpha_{s}^{2})$ accuracy. Other details are as in the caption to Table 1.

QED correction factors for inclusive measurement, as estimated with RAPGAP.

QED correction factors for $2.5 \;\mathrm{GeV} < p_{T,jet}^{lead} < 7 \;\mathrm{GeV}$ and $N_{jet} \geq 1$, as estimated with RAPGAP.

QED correction factors for $2.5 \;\mathrm{GeV} < p_{T,jet}^{lead} < 7 \;\mathrm{GeV}$ and $N_{jet} \geq 2$, as estimated with RAPGAP.

QED correction factors for $2.5 \;\mathrm{GeV} < p_{T,jet}^{lead} < 7 \;\mathrm{GeV}$ and $N_{jet} \geq 3$, as estimated with RAPGAP.

QED correction factors for $7 \;\mathrm{GeV} < p_{T,jet}^{lead} < 12 \;\mathrm{GeV}$ and $N_{jet} \geq 1$, as estimated with RAPGAP.

QED correction factors for $7 \;\mathrm{GeV} < p_{T,jet}^{lead} < 12 \;\mathrm{GeV}$ and $N_{jet} \geq 2$, as estimated with RAPGAP.

QED correction factors for $7 \;\mathrm{GeV} < p_{T,jet}^{lead} < 12 \;\mathrm{GeV}$ and $N_{jet} \geq 3$, as estimated with RAPGAP.

QED correction factors for $12 \;\mathrm{GeV} < p_{T,jet}^{lead} < 30 \;\mathrm{GeV}$ and $N_{jet} \geq 1$, as estimated with RAPGAP.

QED correction factors for $12 \;\mathrm{GeV} < p_{T,jet}^{lead} < 30 \;\mathrm{GeV}$ and $N_{jet} \geq 2$, as estimated with RAPGAP.

QED correction factors for $12 \;\mathrm{GeV} < p_{T,jet}^{lead} < 30 \;\mathrm{GeV}$ and $N_{jet} \geq 3$, as estimated with RAPGAP.

QED correction factors for $10 \;\mathrm{GeV}^{2} < Q^{2} < 50 \;\mathrm{GeV}^{2}$ and $N_{jet} \geq 1$, as estimated with RAPGAP.

QED correction factors for $10 \;\mathrm{GeV}^{2} < Q^{2} < 50 \;\mathrm{GeV}^{2}$ and $N_{jet} \geq 2$, as estimated with RAPGAP.

QED correction factors for $10 \;\mathrm{GeV}^{2} < Q^{2} < 50 \;\mathrm{GeV}^{2}$ and $N_{jet} \geq 3$, as estimated with RAPGAP.

QED correction factors for $50 \;\mathrm{GeV}^{2} < Q^{2} < 100 \;\mathrm{GeV}^{2}$ and $N_{jet} \geq 1$, as estimated with RAPGAP.

QED correction factors for $50 \;\mathrm{GeV}^{2} < Q^{2} < 100 \;\mathrm{GeV}^{2}$ and $N_{jet} \geq 2$, as estimated with RAPGAP.

QED correction factors for $50 \;\mathrm{GeV}^{2} < Q^{2} < 100 \;\mathrm{GeV}^{2}$ and $N_{jet} \geq 3$, as estimated with RAPGAP.

QED correction factors for $100 \;\mathrm{GeV}^{2} < Q^{2} < 350 \;\mathrm{GeV}^{2}$ and $N_{jet} \geq 1$, as estimated with RAPGAP.

QED correction factors for $100 \;\mathrm{GeV}^{2} < Q^{2} < 350 \;\mathrm{GeV}^{2}$ and $N_{jet} \geq 2$, as estimated with RAPGAP.

QED correction factors for $100 \;\mathrm{GeV}^{2} < Q^{2} < 350 \;\mathrm{GeV}^{2}$ and $N_{jet} \geq 3$, as estimated with RAPGAP.

The correlation matrix for the inclusive measurement. The azimuthal correlation angle $\Delta\phi$ of each lepton--leading-jet pair was assigned a bin ID between 0 to 59 segmented uniformly from 0 to $\pi$. This bin ID was offset by multiples of 60 based on the jet multiplicity so that the pair from a single jet event, as suggested by the MC simulation, was assigned a value between 0 to 59, dijet events were given 60 to 119, trijet 120 to 179, and four or more jets 180 to 239.

The correlation matrix for $2.5 \;\mathrm{GeV} < p_{T,jet}^{lead} < 7 \;\mathrm{GeV}$. Other details are as in the caption to Fig. 13.

The correlation matrix for $7 \;\mathrm{GeV} < p_{T,jet}^{lead} < 12 \;\mathrm{GeV}$. Other details are as in the caption to Fig. 13.

The correlation matrix for $12 \;\mathrm{GeV} < p_{T,jet}^{lead} < 30 \;\mathrm{GeV}$. Other details are as in the caption to Fig. 13.

The correlation matrix for $10 \;\mathrm{GeV}^{2} < Q^{2} < 50 \;\mathrm{GeV}^{2}$. Other details are as in the caption to Fig. 13.

The correlation matrix for $50 \;\mathrm{GeV}^{2} < Q^{2} < 100 \;\mathrm{GeV}^{2}$. Other details are as in the caption to Fig. 13.

The correlation matrix for $100 \;\mathrm{GeV}^{2} < Q^{2} < 350 \;\mathrm{GeV}^{2}$. Other details are as in the caption to Fig. 13.

Numerical data for $(K^+ + K^-)/2$ from Figure 1.

Numerical data for $K^0_S$ from Figure 2.

Numerical data for $K^0_S$ from Figure 2.

Numerical data for $(K^+ + K^-)/2$ from Figure 2.

Numerical data for $(K^+ + K^-)/2$ from Figure 2.

Numerical data for $K^0_S$ lifetime from Figure 6.

Numerical data for $K^0_S$ lifetime from Figure 6.

Numerical data for $K^0_S$ $y$-$p_T$ spectrum from Figure 7.

Correlation matrix of the unfolding uncertainty between the inclusive-jet measurement and the previous dijet measurement. Correlations are given in percent.

Summary of different determinations of $\alpha_s(M_Z^2)$ at NNLO or higher order, adapted from PDG, see references therein. The red points are included in the PDG world average. The averages from each sub-field are shown as yellow bands and the world average as a blue band. A recent measurement from CMS using jet cross sections and the latest determination from HERAPDF, which are not yet included in the world average, are shown in green. The current determination, assuming half-correlated and half-uncorrelated scale uncertainties, is shown in black.

Value of the strong coupling $\alpha_s(\mu^2)$ as a function of the scale $\mu$. The data points indicate determinations from measurements that were performed close to the indicated scale. The uncertainties represent the full uncertainty of each determination. All depicted results were obtained at least at NNLO. They are based on data from $e^+e^-$, $ep$ and $pp$ collisions, as well as from $\tau$ lepton decays and quarkonium states. The solid blue line shows the PDG world average. Also shown are the $\alpha_s(M_Z^2)$ values corresponding to each data point.

Double-differential inclusive-jet cross sections using the alternative treatment of QED radiation, as explained in <a href="https://inspirehep.net/literature/2714089">the accompanying thesis</a> (section 9.5.3 and table C.7) and <a href="https://arxiv.org/abs/2405.18136">arXiv:2405.18136</a>. The alternative treatment affects the central value of the cross sections, $\sigma$, the QED correction factors $c_\text{QED}$ and their uncertainty and the sum of all uncorrelated uncertainties $\delta_\text{uncor}$. All other uncertainties and corrections are identical to Tables 1 and 2 and should be taken from there.

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^+$ at 13$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^-$ at 13$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $p$ at 19$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^+$ at 19$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^-$ at 19$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^+$ at 19$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^-$ at 19$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $p$ at 30$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\bar{p}$ at 30$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^+$ at 30$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^-$ at 30$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^+$ at 30$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^-$ at 30$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $p$ at 40$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\bar{p}$ at 40$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^+$ at 40$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^-$ at 40$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^+$ at 40$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^-$ at 40$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $p$ at 75$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\bar{p}$ at 75$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^+$ at 75$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^-$ at 75$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^+$ at 75$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^-$ at 75$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $p$ at 150$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\bar{p}$ at 150$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^+$ at 150$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $\pi^-$ at 150$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^+$ at 150$A$ GeV/c

Two-dimensional distributions ($y$ vs. $p_T$ ) of double differential yields of $K^-$ at 150$A$ GeV/c

Rapidity ($y$) spectra of $\pi^+$ at 13$A$ GeV/c

Rapidity ($y$) spectra of $\pi^-$ at 13$A$ GeV/c

Rapidity ($y$) spectra of $\pi^+$ at 19$A$ GeV/c

Rapidity ($y$) spectra of $\pi^-$ at 19$A$ GeV/c

Rapidity ($y$) spectra of $\pi^+$ at 30$A$ GeV/c

Rapidity ($y$) spectra of $\pi^-$ at 30$A$ GeV/c

Rapidity ($y$) spectra of $\pi^+$ at 40$A$ GeV/c

Rapidity ($y$) spectra of $\pi^-$ at 40$A$ GeV/c

Rapidity ($y$) spectra of $\pi^+$ at 75$A$ GeV/c

Rapidity ($y$) spectra of $\pi^-$ at 75$A$ GeV/c

Rapidity ($y$) spectra of $\pi^+$ at 150$A$ GeV/c

Rapidity ($y$) spectra of $\pi^-$ at 150$A$ GeV/c

The parameters of double-Gaussian fit to $\pi^+$ rapidity spectra

The parameters of double-Gaussian fit to $\pi^-$ rapidity spectra

Rapidity spectrum of negatively charged pions obtained with $h^-$ method in central Ar+Sc collisions at 30$A$ GeV/$c$ The results of $h^-$ analysis of Ar+Sc collisions used for comparison are published in reference [17]

Rapidity spectrum of negatively charged pions obtained with $h^-$ method in central Ar+Sc collisions at 150$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^+$ at 13$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^+$ at 19$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^+$ at 30$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^+$ at 40$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^+$ at 75$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^+$ at 150$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^-$ at 13$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^-$ at 19$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^-$ at 30$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^-$ at 40$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^-$ at 75$A$ GeV/$c$

Rapidity dependence of the inverse slope parameter $T$ fitted to $p_T$ spectrum of $K^-$ at 150$A$ GeV/$c$

Rapidity ($y$) spectra of $K^+$ at 13$A$ GeV/c

Rapidity ($y$) spectra of $K^-$ at 13$A$ GeV/c

Rapidity ($y$) spectra of $K^+$ at 19$A$ GeV/c

Rapidity ($y$) spectra of $K^-$ at 19$A$ GeV/c

Rapidity ($y$) spectra of $K^+$ at 30$A$ GeV/c

Rapidity ($y$) spectra of $K^-$ at 30$A$ GeV/c

Rapidity ($y$) spectra of $K^+$ at 40$A$ GeV/c

Rapidity ($y$) spectra of $K^-$ at 40$A$ GeV/c

Rapidity ($y$) spectra of $K^+$ at 75$A$ GeV/c

Rapidity ($y$) spectra of $K^-$ at 75$A$ GeV/c

Rapidity ($y$) spectra of $K^+$ at 150$A$ GeV/c

Rapidity ($y$) spectra of $K^-$ at 150$A$ GeV/c

The parameters of double-Gaussian fit to $K^+$ rapidity spectra

The parameters of double-Gaussian fit to $K^-$ rapidity spectra

Rapidity ($y$) spectra of $p$ at 13$A$ GeV/c

Rapidity ($y$) spectra of $p$ at 19$A$ GeV/c

Rapidity ($y$) spectra of $p$ at 30$A$ GeV/c

Rapidity ($y$) spectra of $\bar{p}$ at 30$A$ GeV/c

Rapidity ($y$) spectra of $p$ at 40$A$ GeV/c

Rapidity ($y$) spectra of $\bar{p}$ at 40$A$ GeV/c

Rapidity ($y$) spectra of $p$ at 75$A$ GeV/c

Rapidity ($y$) spectra of $\bar{p}$ at 75$A$ GeV/c

Rapidity ($y$) spectra of $p$ at 150$A$ GeV/c

Rapidity ($y$) spectra of $\bar{p}$ at 150$A$ GeV/c

The parameters of double-Gaussian fit to $\bar{p}$ rapidity spectra

The energy dependence of the inverse slope parameter $T(K^+)$ of $p_T$ spectra at mid-rapidity of positively charged $K$ mesons for ArSc. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^+)$ of $p_T$ spectra at mid-rapidity of positively charged $K$ mesons for BeBe. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^+)$ of $p_T$ spectra at mid-rapidity of positively charged $K$ mesons for ppWorld. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^+)$ of $p_T$ spectra at mid-rapidity of positively charged $K$ mesons for pp. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^+)$ of $p_T$ spectra at mid-rapidity of positively charged $K$ mesons for AuAu. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^+)$ of $p_T$ spectra at mid-rapidity of positively charged $K$ mesons for PbPb. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^-)$ of $p_T$ spectra at mid-rapidity of negatively charged $K$ mesons for ArSc. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^-)$ of $p_T$ spectra at mid-rapidity of negatively charged $K$ mesons for BeBe. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^-)$ of $p_T$ spectra at mid-rapidity of negatively charged $K$ mesons for ppWorld. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^-)$ of $p_T$ spectra at mid-rapidity of negatively charged $K$ mesons for pp. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^-)$ of $p_T$ spectra at mid-rapidity of negatively charged $K$ mesons for AuAu. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the inverse slope parameter $T(K^-)$ of $p_T$ spectra at mid-rapidity of negatively charged $K$ mesons for PbPb. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^+/\pi^+$ ratio at mid-rapidity for ArSc. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^+/\pi^+$ ratio at mid-rapidity for BeBe. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^+/\pi^+$ ratio at mid-rapidity for ppWorld. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^+/\pi^+$ ratio at mid-rapidity for pp. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^+/\pi^+$ ratio at mid-rapidity for AuAu. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^+/\pi^+$ ratio at mid-rapidity for PbPb. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^-/\pi^-$ ratio at mid-rapidity for ArSc. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^-/\pi^-$ ratio at mid-rapidity for BeBe. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^-/\pi^-$ ratio at mid-rapidity for ppWorld. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^-/\pi^-$ ratio at mid-rapidity for pp. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^-/\pi^-$ ratio at mid-rapidity for AuAu. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $K^-/\pi^-$ ratio at mid-rapidity for PbPb. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^+\rangle/\langle\pi^+\rangle$ mean multiplicity ratio for ArSc. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^+\rangle/\langle\pi^+\rangle$ mean multiplicity ratio for BeBe. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^+\rangle/\langle\pi^+\rangle$ mean multiplicity ratio for ppWorld. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^+\rangle/\langle\pi^+\rangle$ mean multiplicity ratio for pp. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^+\rangle/\langle\pi^+\rangle$ mean multiplicity ratio for AuAu. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^+\rangle/\langle\pi^+\rangle$ mean multiplicity ratio for PbPb. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^-\rangle/\langle\pi^-\rangle$ mean multiplicity ratio for ArSc. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^-\rangle/\langle\pi^-\rangle$ mean multiplicity ratio for BeBe. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^-\rangle/\langle\pi^-\rangle$ mean multiplicity ratio for ppWorld. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^-\rangle/\langle\pi^-\rangle$ mean multiplicity ratio for pp. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^-\rangle/\langle\pi^-\rangle$ mean multiplicity ratio for AuAu. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

The energy dependence of the $\langle K^-\rangle/\langle\pi^-\rangle$ mean multiplicity ratio for PbPb. The data used for comparison, other than Ar+Sc, are published in references [2-4,13,17,53-64]

Proton rapidity spectra in central Be+Be collisions at $19A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in central Be+Be collisions at $30A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in central Be+Be collisions at $40A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in central Be+Be collisions at $75A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in central Be+Be collisions at $150A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in inelastic p+p collisions at $20$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in inelastic p+p collisions at $30$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in inelastic p+p collisions at $40$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in inelastic p+p collisions at $75$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in inelastic p+p collisions at $150$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in central Pb+Pb collisions at $20A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in central Pb+Pb collisions at $30A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in central Pb+Pb collisions at $40A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in central Pb+Pb collisions at $80A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

Proton rapidity spectra in central Pb+Pb collisions at $150A$ GeV/$c$ beam momentum. The data used for comparison, other than Ar+Sc, are published in references [2,13,17]

System size dependence of the $K^+/\pi^+$ ratio at mid-rapidity in $central$ nucleus-nucleus and inelastic $p$+$p$ interactions obtained at beam momenta of $\approx 150A$ GeV/$c$. The data used for comparison, other than Ar+Sc, are published in references [2,13,17,53].

The performance of jet energy resolution (JER) for jets with |y| < 2.1 evaluated as a function of pT_truth in different centrality bins. Simulated hard scatter events were overlaid onto events from a dedicated sample of minimum-bias Xe+Xe data. The fit parameters are listed in a sperate table (Extras 1)

The relative magnitude of systematic uncertainties for per-pair normalized xJ distributions in 0-10% Xe+Xe centrality

The relative magnitude of systematic uncertainties for absolutely normalized xJ distributions in 0-10% Xe+Xe centrality

The relative magnitude of systematic uncertainties for rho distributions for leading jets in 0-10% Xe+Xe centrality

Per-pair normalized xJ distribution evaluated in four centrality intervals and given pT1 interval.

Per-pair normalized xJ distribution evaluated in four centrality intervals and given pT1 interval.

Per-pair normalized xJ distribution evaluated in four centrality intervals and given pT1 interval.

Absolutely normalized xJ distribution evaluated in four centrality intervals and given pT1 interval.

Absolutely normalized xJ distribution evaluated in four centrality intervals and given pT1 interval.

Absolutely normalized xJ distribution evaluated in four centrality intervals and given pT1 interval.

Per-pair normalized xJ distribution in Xe+Xe collisions.

Per-pair normalized xJ distribution in Pb+Pb collisions.

Per-pair normalized xJ distribution in Xe+Xe collisions.

Per-pair normalized xJ distribution in Pb+Pb collisions.

Per-pair normalized xJ distribution in Xe+Xe collisions.

Per-pair normalized xJ distribution in Pb+Pb collisions.

Absolutely normalized xJ distribution in Xe+Xe collisions.

Absolutely normalized xJ distribution in Xe+Xe collisions.

Absolutely normalized xJ distribution in Xe+Xe collisions.

Absolutely normalized xJ distribution in Xe+Xe collisions.

Absolutely normalized xJ distribution in Xe+Xe collisions.

Absolutely normalized xJ distribution in Xe+Xe collisions.

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of leading jet pT in the same centrality intervals.

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of leading jet pT in the same centrality intervals.

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of leading jet pT in the same centrality intervals.

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of subleading jet pT in the same centrality intervals.

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of subleading jet pT in the same centrality intervals.

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of subleading jet pT in the same centrality intervals.

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of leading jet pT in the same SUM ETFCal intervals (selecting equivalent event activity)

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of leading jet pT in the same SUM ETFCal intervals (selecting equivalent event activity)

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of leading jet pT in the same SUM ETFCal intervals (selecting equivalent event activity)

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of subleading jet pT in the same SUM ETFCal intervals (selecting equivalent event activity)

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of subleading jet pT in the same SUM ETFCal intervals (selecting equivalent event activity)

The ratios of Xe+Xe and Pb+Pb pair nuclear-modification factors, rho, evaluated as a function of subleading jet pT in the same SUM ETFCal intervals (selecting equivalent event activity)

Parameter a,b, and c from JER fits in Figure 1b.

Per-pair normalized xJ distribution in Xe+Xe collisions for selected Pb+Pb centrality and pT1 bin.

Per-pair normalized xJ distribution in Xe+Xe collisions for selected Pb+Pb centrality and pT1 bin.

Per-pair normalized xJ distribution in Xe+Xe collisions for selected Pb+Pb centrality and pT1 bin.

Per-pair normalized xJ distribution in Xe+Xe collisions for selected Pb+Pb centrality and pT1 bin.

Per-pair normalized xJ distribution in Xe+Xe collisions for selected Pb+Pb centrality and pT1 bin.

Per-pair normalized xJ distribution in Xe+Xe collisions for selected Pb+Pb centrality and pT1 bin.

Per-pair normalized xJ distribution in Xe+Xe collisions for selected Pb+Pb centrality and pT1 bin.

Per-pair normalized xJ distribution in Xe+Xe collisions for selected Pb+Pb centrality and pT1 bin.

Per-pair normalized xJ distribution in Xe+Xe collisions for selected Pb+Pb centrality and pT1 bin.

The unfolded differential charge asymmetry as a function of the transverse momentum of the top pair system. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NNLO in QCD and NLO in EW theory are listed. The scale uncertainty is obtained by varying renormalisation and factorisation scales independently by a factor of 2 or 0.5 around $\mu_0$ to calculate the maximum and minimum value of the asymmetry, respectively. The nominal value $\mu_0$ is chosen as $H_T/4$. The variations in which one scale is multiplied by 2 while the other scale is divided by 2 are excluded. Finally, the scale and MC integration uncertainties are added in quadrature.

The unfolded differential charge asymmetry as a function of the longitudinal boost of the top pair system. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NNLO in QCD and NLO in EW theory are listed. The scale uncertainty is obtained by varying renormalisation and factorisation scales independently by a factor of 2 or 0.5 around $\mu_0$ to calculate the maximum and minimum value of the asymmetry, respectively. The nominal value $\mu_0$ is chosen as $H_T/4$. The variations in which one scale is multiplied by 2 while the other scale is divided by 2 are excluded. Finally, the scale and MC integration uncertainties are added in quadrature.

The unfolded inclusive leptonic asymmetry. The unfolded $A_C^{\ell\bar{\ell}}$ is obtained in the reduced phase-space defined by the requirement $|\Delta |\eta_{\ell\bar{\ell}}||<2.5$. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NLO in QCD and NLO in EW theory are listed. The theory uncertainty is obtained by varying both scales by a factor of 0.5 or 2.0 to calculate the minimum and maximum value of the asymmetry, respectively.

The unfolded differential leptonic asymmetry as a function of the invariant mass of the di-lepton pair. The unfolded $A_C^{\ell\bar{\ell}}$ is obtained in the reduced phase-space defined by the requirement $|\Delta |\eta_{\ell\bar{\ell}}||<2.5$. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NLO in QCD and NLO in EW theory are listed. The theory uncertainty is obtained by varying both scales by a factor of 0.5 or 2.0 to calculate the minimum and maximum value of the asymmetry, respectively.

The unfolded differential leptonic asymmetry as a function of the transverse momentum of the di-lepton pair. The unfolded $A_C^{\ell\bar{\ell}}$ is obtained in the reduced phase-space defined by the requirement $|\Delta |\eta_{\ell\bar{\ell}}||<2.5$. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NLO in QCD and NLO in EW theory are listed. The theory uncertainty is obtained by varying both scales by a factor of 0.5 or 2.0 to calculate the minimum and maximum value of the asymmetry, respectively.

The unfolded differential leptonic asymmetry as a function of the longitudinal boost of the di-lepton pair. The unfolded $A_C^{\ell\bar{\ell}}$ is obtained in the reduced phase-space defined by the requirement $|\Delta |\eta_{\ell\bar{\ell}}||<2.5$. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NLO in QCD and NLO in EW theory are listed. The theory uncertainty is obtained by varying both scales by a factor of 0.5 or 2.0 to calculate the minimum and maximum value of the asymmetry, respectively.

Individual 68% and 95% CL bounds on the relevant Wilson coefficients of the SM Effective Field Theory in units of $\text{TeV}^{-2}$. The bounds are derived from the $A_C^{t\bar{t}}$ inclusive measurement. The experimental uncertainties are accounted for, in the form of the complete covariance matrix that keeps track of correlations between bins for the differential measurement. The theory uncertainty from the NNLO QCD + NLO EW calculation is included by explicitly varying the renormalization and factorization scales, or the parton density functions, in the calculation and registering the variations in the intervals.

Individual 68% and 95% CL bounds on the relevant Wilson coefficients of the SM Effective Field Theory in units of $\text{TeV}^{-2}$. The bounds are derived from the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement. The experimental uncertainties are accounted for, in the form of the complete covariance matrix that keeps track of correlations between bins for the differential measurement. The theory uncertainty from the NNLO QCD + NLO EW calculation is included by explicitly varying the renormalization and factorization scales, or the parton density functions, in the calculation and registering the variations in the intervals.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ inclusive measurement. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement for $\beta_{z,t\bar{t}}$ $\in$ [0,0.3]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement for $\beta_{z,t\bar{t}}$ $\in$ [0.3,0.6]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement for $\beta_{z,t\bar{t}}$ $\in$ [0.6,0.8]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement for $\beta_{z,t\bar{t}}$ $\in$ [0.8,1]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ < 500 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ $\in$ [500,750] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ $\in$ [750,1000] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ $\in$ [1000,1500] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ > 1500 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement for $p_{T,t\bar{t}}$ < 30 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement for $p_{T,t\bar{t}}$ $\in$ [30,120] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement for $p_{T,t\bar{t}}$ > 120 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ inclusive measurement. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement for $\beta_{z,\ell\bar{\ell}}$ $\in$[0,0.3]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement for $\beta_{z,\ell\bar{\ell}}$ $\in$[0.3,0.6]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement for $\beta_{z,\ell\bar{\ell}}$ $\in$[0.6,0.8]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement for $\beta_{z,\ell\bar{\ell}}$ $\in$[0.8,1]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement for $m_{\ell\bar{\ell}}$ < 200 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement for $m_{\ell\bar{\ell}}$ $\in$ [200,300] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement for $m_{\ell\bar{\ell}}$ $\in$ [300,400] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement for $m_{\ell\bar{\ell}}$ > 400 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement for $p_{T,\ell\bar{\ell}}$ < 20 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement for $p_{T,\ell\bar{\ell}}$ $\in$ [20, 70] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement for $p_{T,\ell\bar{\ell}}$ > 70 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{t\bar{t}}$ inclusive measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{\ell\ell}$ inclusive measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Covariance matrix for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Double-differential cross-sections for prompt $D^0$ mesons in intervals of $p_\mathrm{T}$ and $y^\ast$ in backward rapidity regions.

Nuclear modification factor $R_{p\mathrm{Pb}}$ for prompt $D^0$ mesons in intervals of $p_\mathrm{T}$ and $y^\ast$ for $p_\mathrm{T} < 10\,\mathrm{GeV}/c$ in forward rapidity regions.

Nuclear modification factor $R_{p\mathrm{Pb}}$ for prompt $D^0$ mesons in intervals of $p_\mathrm{T}$ and $y^\ast$ for $p_\mathrm{T} < 10\,\mathrm{GeV}/c$ in forward rapidity regions.

Nuclear modification factor $R_{p\mathrm{Pb}}$ for prompt $D^0$ mesons in intervals of $p_\mathrm{T}$ and $y^\ast$ for $p_\mathrm{T} < 10\,\mathrm{GeV}/c$ in backward rapidity regions.

Nuclear modification factor $R_{p\mathrm{Pb}}$ for prompt $D^0$ mesons in intervals of $p_\mathrm{T}$ and $y^\ast$ for $p_\mathrm{T} < 10\,\mathrm{GeV}/c$ in backward rapidity regions.

Forward-backward production ratio $R_\mathrm{FB}$ for prompt $D^0$ mesons as a function of $p_\mathrm{T}$, integrated over $2.5 < |y^\ast| < 4.0$.

Forward-backward production ratio $R_\mathrm{FB}$ for prompt $D^0$ mesons as a function of $p_\mathrm{T}$, integrated over $2.5 < |y^\ast| < 4.0$.