$p_{\mathrm{T}}$-differential $\mathrm{D}^{+}_\mathrm{s}$ production cross section at midrapidity ($|y|<0.5$) in pp collisions at $\sqrt{s}$ = 13 TeV Branching ratio of $\mathrm{D}^{+}_\mathrm{s}\rightarrow\phi\pi^+\rightarrow\mathrm{K}^+\mathrm{K}^-\pi^+$: $(2.22 \pm 0.06)\%$. Global relative uncertainty on BR: $2.7\%$ Global relative uncertainty on luminosity: $1.6\%$

$p_{\mathrm{T}}$-differential $\Lambda_\mathrm{c}^{+}$ production cross section at midrapidity ($|y|<0.5$) in pp collisions at $\sqrt{s}$ = 13 TeV Global relative uncertainty on luminosity: $1.6\%$

$p_{\mathrm{T}}$-differential $\Xi_\mathrm{c}^{+}$ production cross section at midrapidity ($|y|<0.5$) in pp collisions at $\sqrt{s}$ = 13 TeV Global relative uncertainty on luminosity: $1.6\%$

$p_{\mathrm{T}}$-differential $\mathrm{D}^{+}/\mathrm{D}^{0}$ ratio in pp collisions at $\sqrt{s}$ = 13 TeV Global relative uncertainty on BR: $1.9\%$

$p_{\mathrm{T}}$-differential $\mathrm{D}^{*+}/\mathrm{D}^{0}$ ratio in pp collisions at $\sqrt{s}$ = 13 TeV Global relative uncertainty on BR: $0.7\%$

$p_{\mathrm{T}}$-differential $\mathrm{D}^{+}_\mathrm{s}/\mathrm{D}^{0}$ ratio in pp collisions at $\sqrt{s}$ = 13 TeV Global relative uncertainty on BR: $2.8\%$

$p_{\mathrm{T}}$-differential $\mathrm{D}^{+}_\mathrm{s}/\mathrm{D}^{+}$ ratio in pp collisions at $\sqrt{s}$ = 13 TeV Global relative uncertainty on BR: $3.2\%$

$p_{\mathrm{T}}$-differential $\mathrm{D}^{+}_\mathrm{s}/(\mathrm{D}^{0}+\mathrm{D}^{+})$ ratio in pp collisions at $\sqrt{s}$ = 13 TeV Global relative uncertainty on BR: $3.3\%$

$\Lambda_\mathrm{c}^{+}/\mathrm{D}^{0}$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\Xi_\mathrm{c}^{+}/\mathrm{D}^{0}$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\sigma(\mathrm{D}^{0})$ $\sqrt{s}$ = 13 TeV / $\sigma(\mathrm{D}^{0})$ $\sqrt{s}$ = 5.02 TeV

$\sigma(\mathrm{D}^{+})$ $\sqrt{s}$ = 13 TeV $/ \sigma(\mathrm{D}^{+})$ $\sqrt{s}$ = 5.02 TeV

$\sigma(\mathrm{D}^{*+})$ $\sqrt{s}$ = 13 TeV / $\sigma(\mathrm{D}^{*+})$ $\sqrt{s}$ = 5.02 TeV

$\sigma(\mathrm{D}^{+}_\mathrm{s})$ $\sqrt{s}$ = 13 TeV $/ \sigma(\mathrm{D}^{+}_\mathrm{s})$ $\sqrt{s}$ = 5.02 TeV

$\sigma(\Lambda^{+}_\mathrm{c})$ $\sqrt{s}$ = 13 TeV $/ \sigma(\Lambda^{+}_\mathrm{c})$ $\sqrt{s}$ = 5.02 TeV

$\sigma(\Xi^{+}_\mathrm{c})$ $\sqrt{s}$ = 13 TeV $/ \sigma(\Xi^{0}_\mathrm{c})$ $\sqrt{s}$ = 5.02 TeV

$\sigma(\Xi^{0}_\mathrm{c})$ $\sqrt{s}$ = 13 TeV / $\sigma(\Xi^{0}_\mathrm{c})$ $\sqrt{s}$ = 5.02 TeV

$\mathrm{D}^{0}$ ratio |$y$| < 0.5 / $2 < y < 2.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{0}$ ratio |$y$| < 0.5 / $3 < y < 3.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{0}$ ratio |$y$| < 0.5 / $4 < y < 4.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{+}$ ratio |$y$| < 0.5 / $2 < y < 2.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{+}$ ratio |$y$| < 0.5 / $3 < y < 3.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{+}$ ratio |$y$| < 0.5 / $4 < y < 4.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{*+}$ ratio |$y$| < 0.5 / $2 < y < 2.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{*+}$ ratio |$y$| < 0.5 / $3 < y < 3.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{*+}$ ratio |$y$| < 0.5 / $4 < y < 4.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{+}_\mathrm{s}$ ratio |$y$| < 0.5 / $2 < y < 2.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{+}_\mathrm{s}$ ratio |$y$| < 0.5 / $3 < y < 3.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

$\mathrm{D}^{+}_\mathrm{s}$ ratio |$y$| < 0.5 / $4 < y < 4.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

Double ratio $\mathrm{D}^{0}$ 13 TeV / 5.02 TeV |$y$| < 0.5 / $2 < y < 2.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

Double ratio $\mathrm{D}^{0}$ 13 TeV / 5.02 TeV |$y$| < 0.5 / $3 < y < 3.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

Double ratio $\mathrm{D}^{0}$ 13 TeV / 5.02 TeV |$y$| < 0.5 / $4 < y < 4.5$ in pp collisions at $\sqrt{s}$ = 13 TeV

Charm $f_\mathrm{s}/(f_\mathrm{u}+f_\mathrm{d})$ in pp collisions at $\sqrt{s}$ = 13 TeV

$f(\mathrm{c \rightarrow h_c})$ in pp collisions at $\sqrt{s}$ = 13 TeV

$f(\mathrm{c \rightarrow h_c})$ in pp collisions at $\sqrt{s}$ = 5.02 TeV

$\sigma(\mathrm{c\bar{c}})$ at $|y|<0.5$ in pp collisions vs.$\sqrt{s}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 0-10% centrality

$\Delta\phi$ projection of balance function in low $p_{T}$ in 30-40% centrality

1D $\Delta\eta$ projection of balance function in low $p_{T}$ in 70-80% centrality

$\Delta\eta$ projection of balance function in low $p_{T}$ in 0-40 $N_{trk}$

$\Delta\eta$ projection of balance function in low $p_{T}$ in 120-150 $N_{trk}$

$\Delta\eta$ projection of balance function in low $p_{T}$ in 270-300 $N_{trk}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 0-40 $N_{trk}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 120-150 $N_{trk}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 270-300 $N_{trk}$

The width of balance function in $<|\Delta\eta|>$ in low $p_{T}$ for PbPb collisions

Balance function width in low $p_{T}$ PbPb relative $<|\Delta\eta|>/<|\Delta\eta|>_{N_{ch}<65}$

The width of balance function in $<|\Delta\eta|>$ in low $p_{T}$ for pPb collisions

Balance function width in low $p_{T}$ in pPb relative $<|\Delta\eta|>/<|\Delta\eta|>_{N_{ch}<24}$

The width of the balance function in $<|\Delta\phi|>$ in low $p_{T}$ for PbPb collisions

Balance function width in low $p_{T}$ in PbPb for relative $<|\Delta\phi|>/<|\Delta\phi|>_{N_{ch}<65}$

The width of the balance function in $<|\Delta\phi|>$ in low $p_{T}$ for pPb collisions

Balance function width in low $p_{T}$ in pPb for relative $|\Delta\phi|/<|\Delta\phi|>_{N_{ch}<24}$

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in pPb for 0-40 $N_{trk}$

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in pPb for 120-150 $N_{trk}$

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in pPb for 270-300 $N_{trk}$

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in pPb for $N_{trk}$ 0-40

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in pPb for $N_{trk}$ 120-150

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in pPb for $N_{trk}$ 270-300

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in pPb for $N_{trk}$ 0-40

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in pPb for $N_{trk}$ 120-150

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in pPb for $N_{trk}$ 270-300

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for $N_{trk}$ 0-40

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for $N_{trk}$ 120-150

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for $N_{trk}$ 270-300

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for low $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for high $p_{T}$

Average width of the balance function in $\Delta \phi$ with $p_{T}$ for low $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for high $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for low $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for high $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for low $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for high $p_{T}$

The nuclear modification factor $\mathrm{R_{AA}}$ versus $p_{\mathrm{T}}$ for prompt $\Lambda^+_c$ production in centrality regions of 0-90, 0-10, 10-30, 30-50 and 50-90% in PbPb collisions. The global uncertainty includes the uncertainties for the luminosity of pp collisions, number of MB events in PbPb collisions, and tracking efficiency. The global uncertainty for $\mathrm{R_{AA}}$ is 16.5%.

The ratio of the production cross sections of prompt $\Lambda^+_c$ to prompt $\mathrm{D_0}$ versus $p_{\mathrm{T}}$ from pp collisions. The global normalization uncertainty is 6.6%.

The ratio of the $\mathrm{T_{AA}}$-scaled prompt $\Lambda^+_c$ yields to prompt $\mathrm{D_0}$ versus $p_{\mathrm{T}}$ from PbPb collisions for 0-90 and 0-10% centrality classes. The global normalization uncertainty is 7.3%.

$p_{\rm T}$-differential cross section of charged-particle jets from model predictions in p-Pb collisions at $\sqrt{s_{\rm NN}} = 5.02$ TeV.

$p_{\rm T}$-differential cross section ratios of charged-particle jets in pp collisions at $\sqrt{s} = 5.02$ TeV.

$p_{\rm T}$-differential cross section ratios of charged-particle jets in p-Pb collisions at $\sqrt{s_{\rm NN}} = 5.02$ TeV.

$p_{\rm T}$-differential $R_{\rm pPb}$ of charged-particle jets in p-Pb collisions at $\sqrt{s_{\rm NN}} = 5.02$ TeV.

$p_{\rm T}$-differential $R_{\rm pPb}$ of charged-particle jets in p-Pb collisions at $\sqrt{s_{\rm NN}} = 5.02$ TeV.

The Levy scale parameter $R$ versus the transverse mass $m_{\mathrm{T}}$ in different centrality classes for negatively and positively charged hadron pairs.

The $1/R^2$ distribution vs. transverse mass $m_{\mathrm{T}}$ in different centrality classes for negatively and positively charged hadron pairs.

The linear-fit parameter $A$ versus $\langle N_{\text{part}}\rangle$ for positively and negatively charged hadron pairs. The bin range on $\langle N_{\text{part}}\rangle$ represents the 68% confidence interval associated to its uncertainty.

The linear-fit parameter $B$ versus $\langle N_{\text{part}}\rangle$ for positively and negatively charged hadron pairs. The bin range on $\langle N_{\text{part}}\rangle$ represents the 68% confidence interval associated to its uncertainty.

The Levy scale parameter $R$ versus $\langle N_{\text{part}}\rangle^{1/3}$ in different $m_{\mathrm{T}}$ classes for negatively and positively charged hadron pairs. The bin range on $\langle N_{\text{part}}\rangle^{1/3}$ represents the 68% confidence interval associated to its uncertainty.

The Levy stability index $\alpha$ versus the transverse mass $m_{\mathrm{T}}$ in different centrality classes for negatively and positively charged hadron pairs.

The average Levy stability index $\langle \alpha \rangle$ versus $\langle N_{\text{part}}\rangle$ for both positively and negatively charged hadron pairs. The bin range on $\langle N_{\text{part}}\rangle$ represents the 68% confidence interval associated to its uncertainty.

The correlation strength $\lambda$ versus the transverse mass $m_{\mathrm{T}}$ in different centrality classes for negatively and positively charged hadron pairs.

The correlation strength (re-scaled with the square of the pion fraction) $\lambda ^*$ versus the transverse mass $m_{\mathrm{T}}$ in different centrality classes for positively and negatively charged hadron pairs.

Measured coherent J/psi cross section for the XNXN forward class. Note that for each rapidity range the 0n0n uncertainty related to migrations is preceded by a ∓, while the other neutron classes have a ±; this means that these uncertainties are anti-correlated.

Photonuclear cross sections extracted from the UPC measurements.

Nuclear suppression factor extracted from the UPC measurements.

The $v_{3}$ values as a function of centrality for prompt and nonprompt J/$\psi$ mesons.The kinematic range is 6.5 $< p_{\text{T}} <$ 50 GeV/c and $|y| < 2.4$.

The $v_{2}$ values of prompt J/$\psi$ mesons as a function of $p_{\text{T}}$ in the 10–60% centrality range. The results for 3 $< p_{\text{T}} <$ 6.5 and 6.5 $< p_{\text{T}} <$ 50 GeV/c are studied in the rapidity range of 1.6 $< |y| <$ 2.4 and $|y| <$ 2.4, respectively.

The $v_{2}$ values as functions of $p_{\text{T}}$ for prompt J/$\psi$ and prompt $\psi$(2S) mesons in the 10–60% centrality range. The results for $p_{\text{T}}$ < 6.5 and $p_{\text{T}}$ > 6.5 GeV/c are studied in the rapidity range of 1.6 $< |y| <$ 2.4 and $|y| <$ 2.4, respectively.

The $v_{2}$ values as functions of centrality for prompt J/$\psi$ and prompt $\psi$(2S) mesons. The kinematic range is 6.5 $< p_{\text{T}} <$ 50 GeV/c and $|y| <$ 2.4.

The $v_{3}$ values as functions of $p_{\text{T}}$ for prompt J/$\psi$ and prompt $\psi$(2S) mesons in the 10–60% centrality range. The results for $p_{\text{T}}$ < 6.5 and $p_{\text{T}}$ > 6.5 GeV/c are studied in the rapidity range of 1.6 $< |y| <$ 2.4 and $|y| <$ 2.4, respectively.

The $v_{3}$ values as functions of centrality for prompt J/$\psi$ and prompt $\psi$(2S) mesons. The kinematic range is 6.5 $< p_{\text{T}} <$ 50 GeV/c and $|y| <$ 2.4.

Measured $R_\text{AA}$ for the $\Upsilon(3S)$ state as functions of PbPb collision centrality, integrated over the full kinematic range $p_\text{T}$ < 30 GeV/c and |y| < 2.4. The global uncertainty "PP MB" represents the pp luminosity and PbPb $N_\text{MB}$ combined uncertainties, whereas the global uncertainty "PP 3S" corresponds to the uncertainty on the $\Upsilon(3S)$ pp yields.

Measured $R_\text{AA}$ for the$\Upsilon(2S)$ state in the 0–90% centrality interval, integrated over the full kinematic range $p_\text{T}$ < 30 GeV/c and |y| < 2.4. The global uncertainty "PP MB" represents the pp luminosity and PbPb $N_\text{MB}$ combined uncertainties, whereas the global uncertainty "PP 2S" corresponds to the uncertainty on the $\Upsilon(2S)$ pp yields.

Measured $R_\text{AA}$ for the$\Upsilon(2S)$ state in the 0–90% centrality interval, integrated over the full kinematic range $p_\text{T}$ < 30 GeV/c and |y| < 2.4. The global uncertainty "PP MB" represents the pp luminosity and PbPb $N_\text{MB}$ combined uncertainties, whereas the global uncertainty "PP 2S" corresponds to the uncertainty on the $\Upsilon(2S)$ pp yields.

Measured $R_\text{AA}$ for the $\Upsilon(3S)$ state in the 0–90% centrality interval, integrated over the full kinematic range $p_\text{T}$ < 30 GeV/c and |y| < 2.4. The global uncertainty "PP MB" represents the pp luminosity and PbPb $N_\text{MB}$ combined uncertainties, whereas the global uncertainty "PP 3S" corresponds to the uncertainty on the$\Upsilon(3S)$ pp yields.

Measured $R_\text{AA}$ for the $\Upsilon(3S)$ state in the 0–90% centrality interval, integrated over the full kinematic range $p_\text{T}$ < 30 GeV/c and |y| < 2.4. The global uncertainty "PP MB" represents the pp luminosity and PbPb $N_\text{MB}$ combined uncertainties, whereas the global uncertainty "PP 3S" corresponds to the uncertainty on the$\Upsilon(3S)$ pp yields.

Measured $R_\text{AA}$ for the $\Upsilon(2S)$ state as functions of transverse momentum $p_\text{T}$, integrated over the rapidity range of |y| < 2.4 and the 0–90% centrality interval. The global uncertainty combines the uncertainties of $T_\text{AA}$ , pp luminosity, and PbPb $N_\text{MB}$.

Measured $R_\text{AA}$ for the $\Upsilon(2S)$ state as functions of transverse momentum $p_\text{T}$, integrated over the rapidity range of |y| < 2.4 and the 0–90% centrality interval. The global uncertainty combines the uncertainties of $T_\text{AA}$ , pp luminosity, and PbPb $N_\text{MB}$.

Measured $R_\text{AA}$ for the $\Upsilon(3S)$ state as functions of transverse momentum $p_\text{T}$, integrated over the rapidity range of |y| < 2.4 and the 0–90% centrality interval. The global uncertainty combines the uncertainties of $T_\text{AA}$ , pp luminosity, and PbPb $N_\text{MB}$.

Measured $R_\text{AA}$ for the $\Upsilon(3S)$ state as functions of transverse momentum $p_\text{T}$, integrated over the rapidity range of |y| < 2.4 and the 0–90% centrality interval. The global uncertainty combines the uncertainties of $T_\text{AA}$ , pp luminosity, and PbPb $N_\text{MB}$.

The double ratios of $\Upsilon(3S)$ /$\Upsilon(2S)$ as functions of PbPb collision centrality, integrated over the full kinematic range $p_\text{T}$ < 30 GeV/c and |y| < 2.4. The global uncertainty represents the combined systematic and statistical uncertainties from pp data.

The double ratios of $\Upsilon(3S)$ /$\Upsilon(2S)$ as functions of PbPb collision centrality, integrated over the full kinematic range $p_\text{T}$ < 30 GeV/c and |y| < 2.4. The global uncertainty represents the combined systematic and statistical uncertainties from pp data.

The double ratios of $\Upsilon(3S)$ /$\Upsilon(2S)$ in the 0–90% centrality interval, integrated over the full kinematic range $p_\text{T}$ < 30 GeV/c and |y| < 2.4. The global uncertainty represents the combined systematic and statistical uncertainties from pp data.

The double ratios of $\Upsilon(3S)$ /$\Upsilon(2S)$ in the 0–90% centrality interval, integrated over the full kinematic range $p_\text{T}$ < 30 GeV/c and |y| < 2.4. The global uncertainty represents the combined systematic and statistical uncertainties from pp data.

The double ratios of $\Upsilon(3S)$ /$\Upsilon(2S)$ as functions of transverse momentum $p_\text{T}$, integrated over the rapidity range of |y| < 2.4 and the 0–90% centrality interval.

The double ratios of $\Upsilon(3S)$ /$\Upsilon(2S)$ as functions of transverse momentum $p_\text{T}$, integrated over the rapidity range of |y| < 2.4 and the 0–90% centrality interval.

Yields for $\Upsilon(2S)$ mesons in PbPb collisions in centrality $0--90\%$ and $|y| < 2.4$, corrected for acceptance and efficiency, and normalized by the nuclear thickness function $\langle T_{AA} \rangle$ and the number of minimum bias events $N_{MB}$. The numbers are in units of pb$/GeV/c$.

Yields for $\Upsilon(2S)$ mesons in PbPb collisions in $p_\text{T} < 30GeV/c$ and $|y| < 2.4$, corrected for acceptance and efficiency, and normalized by the nuclear thickness function $\langle T_{AA} \rangle$ and the number of minimum bias events $N_{MB}$. The numbers are in units of pb$/GeV/c$.

Yields for $\Upsilon(3S)$ mesons in PbPb collisions in centrality $0--90\%$ and $|y| < 2.4$, corrected for acceptance and efficiency, and normalized by the nuclear thickness function $\langle T_{AA} \rangle$ and the number of minimum bias events $N_{MB}$. The numbers are in units of pb$/GeV/c$.

Yields for $\Upsilon(3S)$ mesons in PbPb collisions in $p_\text{T} < 30GeV/c$ and $|y| < 2.4$, corrected for acceptance and efficiency, and normalized by the nuclear thickness function $\langle T_{AA} \rangle$ and the number of minimum bias events $N_{MB}$. The numbers are in units of pb$/GeV/c$.

Yields for $\Upsilon(1S)$ mesons in PbPb collisions in $p_\text{T} < 30GeV/c$ and $|y| < 2.4$, corrected for acceptance and efficiency, and normalized by the nuclear thickness function $\langle T_{AA} \rangle$ and the number of minimum bias events $N_{MB}$. The numbers are in units of pb$/GeV/c$. The values and global integrated luminosity uncertainty are quoted from data taken from CMS in 2018 LHC PbPb run.

The total coherent $\mathrm{J}/\psi$ photoproduction cross section as a function of photon-nuclear center-of-mass energy per nucleon $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$, measured in PbPb ultra-peripheral collisions at $\sqrt{s_{\mathrm{NN}}}$ = 5.02 TeV. The $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$ values used correspond to the center of each rapidity range. The theoretical uncertainties is due to the uncertainties in the photon flux.

The nuclear gluon suppression factor $R_{\mathrm{g}}^{\mathrm{Pb}}$ as a function of Bjorken $x$ extracted from the CMS measurement of the coherent $\mathrm{J}/\psi$ photoproduction in PbPb ultra-peripheral collisions at $\sqrt{s_{\mathrm{NN}}}$ = 5.02 TeV. The $x$ values are evaluated at the centers of their corresponding rapidity ranges. The theoretical uncertainties are due to the uncertainties in the photon flux and the impulse approximation model.

The nuclear gluon suppression factor $R_{\mathrm{g}}^{\mathrm{Pb}}$ as a function of Bjorken $x$ extracted from the CMS measurement of the coherent $\mathrm{J}/\psi$ photoproduction in PbPb ultra-peripheral collisions at $\sqrt{s_{\mathrm{NN}}}$ = 5.02 TeV. The $x$ values are evaluated at the centers of their corresponding rapidity ranges. The theoretical uncertainties are due to the uncertainties in the photon flux and the impulse approximation model.

The total covariance matrix of the total coherent photoproduction cross section as a function of photon-nuclear center-of-mass energy per nucleon $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$. The covariance matrix includes both the experimental and theoretical (photon flux) uncertainties. The bins are ordered as increasing in $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$.

The photon flux values from STARLight as a function of rapidity, in different neutron multiplicity classes: 0n0n, 0nXn, and XnXn.

The experimental covariance matrix of the total coherent photoproduction cross section as a function of photon-nuclear center-of-mass energy per nucleon $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$. The bins are ordered as increasing in $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$.

The covariance matrix for the flux in the 0n0n neutron multiplicity class.

The theoretical (photon flux) covariance matrix of the total coherent photoproduction cross section as a function of photon-nuclear center-of-mass energy per nucleon $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$. The bins are ordered as increasing in $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$.

The covariance matrix for the flux in the 0nXn neutron multiplicity class.

The covariance matrix for the flux in the XnXn neutron multiplicity class.

The total covariance matrix of the total coherent photoproduction cross section as a function of photon-nuclear center-of-mass energy per nucleon $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$. The covariance matrix includes both the experimental and theoretical (photon flux) uncertainties. The bins are ordered as increasing in $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$.

The experimental covariance matrix of the total coherent photoproduction cross section as a function of photon-nuclear center-of-mass energy per nucleon $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$. The bins are ordered as increasing in $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$.

The theoretical (photon flux) covariance matrix of the total coherent photoproduction cross section as a function of photon-nuclear center-of-mass energy per nucleon $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$. The bins are ordered as increasing in $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$.