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 $W_{\gamma \mathrm{N}}^{\mathrm{Pb}}$.

The measured Z boson production cross section in pp collisions as a function of the Z boson rapidity for the dielectron decay channel.

Event centrality dependence of the $\mbox{Z}\rightarrow\mu^{+}\mu^{-}$ yields per MB event in PbPb collisions, divided by the expected average nuclear overlap function, $T_{\rm AA}$. On the horizontal axis, event centrality is depicted as the average number of participating nucleons, $N_{\rm part}$.

Event centrality dependence of the $\mbox{Z}\rightarrow e^{+}e^{-}$ yields per MB event in PbPb collisions, divided by the expected average nuclear overlap function, $T_{\rm AA}$. On the horizontal axis, event centrality is depicted as the average number of participating nucleons, $N_{\rm part}$.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson $p_{\rm T}$ for the dimuon decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson $p_{\rm T}$ for the dielectron decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson rapidity for the dimuon decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson rapidity for the dielectron decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson rapidity for the combined leptonic decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson $p_{\rm T}$ for the combined leptonic decay channel.

Event centrality dependence of the $\mbox{Z}\rightarrow l^{+}l^{-}$ yields per MB event in PbPb collisions, divided by the expected average nuclear overlap function, $T_{\rm AA}$. On the horizontal axis, event centrality is depicted as the average number of participating nucleons, $N_{\rm part}$.

The measured Z boson production cross section in pp collisions as a function of the Z boson rapidity for the combined leptonic decay channel.

The measured Z boson production cross section in pp collisions as a function of the Z boson pT for the combined leptonic decay channel in |y|<1.44.

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