Distributions of $m_T$ in the $W^{+}$ signal selection for mu final states for the pp collisions at $\sqrt{s}=$ 13TeV after the maximum likelihood fit. The EW backgrounds include the contributions from DY, $W\to\tau\nu$, and diboson processes.

Distributions of $m_T$ in the $W^{-}$ signal selection for e final states for the pp collisions at $\sqrt{s}=$ 5TeV after the maximum likelihood fit. The EW backgrounds include the contributions from DY, $W\to\tau\nu$, and diboson processes.

Distributions of $m_T$ in the $W^{-}$ signal selection for mu final states for the pp collisions at $\sqrt{s}=$ 5TeV after the maximum likelihood fit. The EW backgrounds include the contributions from DY, $W\to\tau\nu$, and diboson processes.

Distributions of $m_T$ in the $W^{-}$ signal selection for e final states for the pp collisions at $\sqrt{s}=$ 13TeV after the maximum likelihood fit. The EW backgrounds include the contributions from DY, $W\to\tau\nu$, and diboson processes.

Distributions of $m_T$ in the $W^{-}$ signal selection for mu final states for the pp collisions at $\sqrt{s}=$ 13TeV after the maximum likelihood fit. The EW backgrounds include the contributions from DY, $W\to\tau\nu$, and diboson processes.

Distributions of $m_{ll}$ in the Z signal selection for ee final states for the pp collisions at $\sqrt{s}=$ 5TeV after the maximum likelihood fit. The EW backgrounds include the contributions from DY, $W\to l\nu$, and diboson processes.

Distributions of $m_{ll}$ in the Z signal selection for mumu final states for the pp collisions at $\sqrt{s}=$ 5TeV after the maximum likelihood fit. The EW backgrounds include the contributions from DY, $W\to l\nu$, and diboson processes.

Distributions of $m_{ll}$ in the Z signal selection for ee final states for the pp collisions at $\sqrt{s}=$ 13TeV after the maximum likelihood fit. The EW backgrounds include the contributions from DY, $W\to l\nu$, and diboson processes.

Distributions of $m_{ll}$ in the Z signal selection for mumu final states for the pp collisions at $\sqrt{s}=$ 13TeV after the maximum likelihood fit. The EW backgrounds include the contributions from DY, $W\to l\nu$, and diboson processes.

Figure 4 Fiducial cross sections and ratios for $W\to\ell\nu$ and $Z\to\ell\ell$ processes at 13TeV

Figure 5 Fiducial cross sections and ratios for $W\to\ell\nu$ and $Z\to\ell\ell$ processes at 5.02TeV

Figure 6 Fiducial cross sections and ratios for $W\to\ell\nu$ and $Z\to\ell\ell$ processes between 13TeV and 5.02TeV

Figure 7 Total cross sections and ratios for $W\to\ell\nu$ and $Z\to\ell\ell$ processes at 13TeV

Figure 8 Total cross sections and ratios for $W\to\ell\nu$ and $Z\to\ell\ell$ processes at 5.02TeV

Figure 9 Total cross sections and ratios for $W\to\ell\nu$ and $Z\to\ell\ell$ processes between 13TeV and 5.02TeV

Summary of theoretical predictions of the total inclusive cross sections for W and Z boson production times leptonic branching fractions at ppbar collisions.

Summary of experimental measurements of the total inclusive cross sections for W and Z boson production times leptonic branching fractions at UA1 and UA2.

Summary of experimental measurements of the total inclusive cross sections for W and Z boson production times leptonic branching fractions at D0.

Summary of experimental measurements of the total inclusive cross sections for W and Z boson production times leptonic branching fractions at CDF.

Summary of theoretical predictions of the total inclusive cross sections for W boson production times leptonic branching fractions at pp collisions.

Summary of experimental measurements of the total inclusive cross sections for Z boson production times leptonic branching fractions at pp collisions.

Summary of experimental measurements of the total inclusive cross sections for W and Z boson production times leptonic branching fractions at CMS.

Single-differential production cross-sections for nonprompt $J/\psi$ mesons as a function of $p_\text{T}$. The first uncertainties are statistical, the second are correlated systematic uncertainties shared between intervals, and the last are uncorrelated systematic uncertainties.

Single-differential production cross-sections for prompt $J/\psi$ mesons as a function of $y$. The first uncertainties are statistical, the second are correlated systematic uncertainties shared between intervals, and the last are uncorrelated systematic uncertainties.

Single-differential production cross-sections for nonprompt $J/\psi$ mesons as a function of $y$. The first uncertainties are statistical, the second are correlated systematic uncertainties shared between intervals, and the last are uncorrelated systematic uncertainties.

Fraction of nonprompt $J/\psi$ mesons (in \%) in ($p_\text{T},y$) intervals. The first uncertainty is statistical and the second is systematic.

Nuclear modification factor $R_{p\text{Pb}}$ for prompt $J/\psi$ mesons as a function of $y$. The first uncertainty is statistical and the second is systematic.

Nuclear modification factor $R_{p\text{Pb}}$ for nonprompt $J/\psi$ mesons as a function of $y$. The first uncertainty is statistical and the second is systematic.

Cross-section ratios between 8 TeV and 5 TeV measurements for prompt $J/\psi$ mesons as a function of $p_\text{T}$. The first uncertainty is statistical and the second is systematic.

Cross-section ratios between 8 TeV and 5 TeV measurements for prompt $J/\psi$ mesons as a function of $y$. The first uncertainty is statistical and the second is systematic.

Cross-section ratios between 13 TeV and 5 TeV measurements for prompt $J/\psi$ mesons as a function of $p_\text{T}$. The first uncertainty is statistical and the second is systematic.

Cross-section ratios between 13 TeV and 5 TeV measurements for prompt $J/\psi$ mesons as a function of $y$. The first uncertainty is statistical and the second is systematic.

Cross-section ratios between 8 TeV and 5 TeV measurements for nonprompt $J/\psi$ mesons as a function of $p_\text{T}$. The first uncertainty is statistical and the second is systematic.

Cross-section ratios between 8 TeV and 5 TeV measurements for nonprompt $J/\psi$ mesons as a function of $y$. The first uncertainty is statistical and the second is systematic.

Cross-section ratios between 13 TeV and 5 TeV measurements for nonprompt $J/\psi$ mesons as a function of $p_\text{T}$. The first uncertainty is statistical and the second is systematic.

Cross-section ratios between 13 TeV and 5 TeV measurements for nonprompt $J/\psi$ mesons as a function of $y$. The first uncertainty is statistical and the second is systematic.

Relative changes of cross-sections (in \%), for a polarisation of $\lambda_{\theta}=-0.2$ rather than zero, in ($p_\text{T},y$) intervals.

Relative changes of cross-sections (in \%), for a polarisation of $\lambda_{\theta}=-1$ rather than zero, in ($p_\text{T},y$) intervals.

Relative changes of cross-sections (in \%), for a polarisation of $\lambda_{\theta}=+1$ rather than zero, in ($p_\text{T},y$) intervals.

<K+>/<PI>+.

Inverse slope parameter T.

Inverse slope parameter T.

Inverse slope parameter T.

Inverse slope parameter T.

K-/PI- at y=0.

K-/PI- at y=0.

<K->/<PI->.

<K->/<PI->.

The second-order Fourier coefficients, $V_{3\Delta}(2, |\Delta\eta| > 2)$, as a function of $N_{offline}^{trk}$ for charged particles, after correcting for back-to-back jet correlations, estimated from the 10 $\leq$ $N_{offline}^{trk}$ < 20 range.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $N_{offline}^{trk}$ for charged particles.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $N_{offline}^{trk}$ for charged particles.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $N_{offline}^{trk}$ for charged particles.

The triangular flow after correcting for back-to-back jet correlations, $v_{3}^{sub}(2, |\Delta\eta| > 2)$, as a function of $N_{offline}^{trk}$ for charged particles.

The triangular flow after correcting for back-to-back jet correlations, $v_{3}^{sub}(2, |\Delta\eta| > 2)$, as a function of $N_{offline}^{trk}$ for charged particles.

The triangular flow after correcting for back-to-back jet correlations, $v_{3}^{sub}(2, |\Delta\eta| > 2)$, as a function of $N_{offline}^{trk}$ for charged particles.

The elliptic flow, $v_{2}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for charged particles.

The elliptic flow, $v_{2}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for charged particles.

The elliptic flow, $v_{2}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for charged particles.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for charged particles.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for charged particles.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for charged particles.

The elliptic flow, $v_{2}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for charged particles.

The elliptic flow, $v_{2}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for $K^{0}_{S}$.

The elliptic flow, $v_{2}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for $\Lambda/\bar{\Lambda}$.

The elliptic flow, $v_{2}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for charged particles.

The elliptic flow, $v_{2}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for $K^{0}_{S}$.

The elliptic flow, $v_{2}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for $\Lambda/\bar{\Lambda}$.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for charged particles.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for $K^{0}_{S}$.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $p_{T}$ for $\Lambda/\bar{\Lambda}$.

The elliptic flow per constituent quark after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)/n_{q}$, as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ for $K^{0}_{S}$.

The elliptic flow per constituent quark after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ for $\Lambda/\bar{\Lambda}$.

The four-particle cumulant, $c_{2}(4)$, as a function of $N_{offline}^{trk}$ for charged particles.

The four-particle cumulant, $c_{2}(4)$, as a function of $N_{offline}^{trk}$ for charged particles.

The four-particle cumulant, $c_{2}(4)$, as a function of $N_{offline}^{trk}$ for charged particles.

The six-particle cumulant, $c_{2}(6)$, as a function of $N_{offline}^{trk}$ for charged particles.

The elliptic flow after correcting for back-to-back jet correlations, $v_{2}^{sub}(2, |\Delta\eta| > 2)$, as a function of $N_{offline}^{trk}$ for charged particles.

The elliptic flow, $v_{2}(4)$, as a function of $N_{offline}^{trk}$ for charged particles.

The elliptic flow, $v_{2}(6)$, as a function of $N_{offline}^{trk}$ for charged particles.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL collisions at a centre-of-mass energy of 2760 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for NSD collisions at a centre-of-mass energy of 2760 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL>0 collisions at a centre-of-mass energy of 2760 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL collisions at a centre-of-mass energy of 7000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for NSD collisions at a centre-of-mass energy of 7000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL collisions at a centre-of-mass energy of 8000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for NSD collisions at a centre-of-mass energy of 8000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Charged particle pseudorapidiy densities in the pseudorapidity region -0.5 to 0.5 for INEL collisions.

Charged particle pseudorapidiy densities in the pseudorapidity region -0.5 to 0.5 for NSD collisions.

Charged particle pseudorapidiy densities in the pseudorapidity region -0.5 to 0.5 for INEL>0 collisions.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Mean charged particle multiplicities in 3 pseudorapidity intervals in P P NSD collisions from 900 to 8000 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -0.5 to 0.5 in P P NSD collisions at centre-of-mass energies from 900 to 8000 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -1.0 to 1.0 in P P NSD collisions at centre-of-mass energies from 900 to 8000 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -1.5 to 1.5 in P P NSD collisions at centre-of-mass energies from 900 to 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 8000 GeV.

Production rate for the $\pi^{0}$ production in the rapidity range $9.2 < y < 9.4$ in $p+p$ collisions and in the rapidity range $-9.2 > y_\rm{lab} > -9.4$ in $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the rapidity range $9.4 < y < 9.6$ in $p+p$ collisions and in the rapidity range $-9.4 > y_\rm{lab} > -9.6$ in $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the rapidity range $9.6 < y < 9.8$ in $p+p$ collisions and in the rapidity range $-9.6 > y_\rm{lab} > -9.8$ in $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the rapidity range $9.8 < y < 10.0$ in $p+p$ collisions and in the rapidity range $-9.8 > y_\rm{lab} > -10.0$ in $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the rapidity range $10.0 < y < 10.2$ in $p+p$ collisions and in the rapidity range $-10.0 > y_\rm{lab} > -10.2$ in $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the rapidity range $10.2 < y < 10.4$ in $p+p$ collisions and in the rapidity range $-10.2 > y_\rm{lab} > -10.4$ in $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the rapidity range $10.4 < y < 10.6$ in $p+p$ collisions and in the rapidity range $-10.4 > y_\rm{lab} > -10.6$ in $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the rapidity range $10.6 < y < 10.8$ in $p+p$ collisions and in the rapidity range $-10.6 > y_\rm{lab} > -10.8$ in $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the $p_\rm{T}$ range $0.0 < p_\rm{T} < 0.2$ GeV in $p+p$ and $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the $p_\rm{T}$ range $0.2 < p_\rm{T} < 0.4$ GeV in $p+p$ and $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the $p_\rm{T}$ range $0.4 < p_\rm{T} < 0.6$ GeV in $p+p$ and $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the $p_\rm{T}$ range $0.6 < p_\rm{T} < 0.8$ GeV in $p+p$ and $p+\rm{Pb}$ collisions.

Production rate for the $\pi^{0}$ production in the $p_\rm{T}$ range $0.8 < p_\rm{T} < 1.0$ GeV in $p+p$ and $p+\rm{Pb}$ collisions.

Nuclear modification factor for the $\pi^{0}$s in the rapidity ranges $-8.8>y_\rm{lab}>-9.0$, $-9.0>y_\rm{lab}>-9.2$, and $-9.2>y_\rm{lab}>-9.4$ in $p+\rm{Pb}$ collisions at $\sqrt{s_\rm{NN}}=5.02$ TeV. The uncertainties include both statistical and systematic uncertainties.

Nuclear modification factor for the $\pi^{0}$s in the rapidity ranges $-9.4>y_\rm{lab}>-9.6$, $-9.6>y_\rm{lab}>-9.8$, and $-9.8>y_\rm{lab}>-10.0$ in $p+\rm{Pb}$ collisions at $\sqrt{s_\rm{NN}}=5.02$ TeV. The uncertainties include both statistical and systematic uncertainties.

Nuclear modification factor for the $\pi^{0}$s in the rapidity ranges $-10.0>y_\rm{lab}>-10.2$, $-10.2>y_\rm{lab}>-10.4$, and $-10.4>y_\rm{lab}>-10.6$ in $p+\rm{Pb}$ collisions at $\sqrt{s_\rm{NN}}=5.02$ TeV. The uncertainties include both statistical and systematic uncertainties.

Nuclear modification factor for the $\pi^{0}$s in the rapidity ranges $-10.6>y_\rm{lab}>-10.8$ in $p+\rm{Pb}$ collisions at $\sqrt{s_\rm{NN}}=5.02$ TeV. The uncertainties include both statistical and systematic uncertainties.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 0.9\ TeV$ events with the unlike-charge reference sample for various multiplicity intervals $n_{ch}$ for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV$ events with the unlike-charge reference sample for various multiplicity intervals $n_{ch}$ for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. The statistical uncertainties at $7\ TeV$ were corrected on the $\sqrt{\chi^{2}/ndf}$ and they more smaller than systematic uncertainties. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV\ HM$ events with the unlike-charge reference sample for various multiplicity intervals $n_{ch}$ for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 0.9\ TeV$ ($n_{ch} \ge 2$) events with the unlike-charge reference sample for various $k_{T}$ intervals for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. The statistical uncertainties were corrected on the $\sqrt{\chi^{2}/ndf}$ when $\chi^{2}/ndf > 1$. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV$ ($n_{ch} \ge 2$) events with the unlike-charge reference sample for various $k_{T}$ intervals for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. Where only one error is shown for parameters $C_{0}$ and $\epsilon$ , this represents the statistical uncertainty only. The statistical uncertainties were corrected on the $\sqrt{\chi^{2}/ndf}$ when $\chi^{2}/ndf > 1$. The statistical uncertainties at $7\ TeV$ more smaller than systematic uncertainties.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV\ HM$ ($n_{ch} \ge 150$) events with the unlike-charge reference sample for various $k_{T}$ intervals for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. The statistical uncertainties were corrected on the $\sqrt{\chi^{2}/ndf}$ when $\chi^{2}/ndf > 1$.Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV$ events with the unlike-charge reference sample for various $k_{T}$ intervals of different multiplicity regions $n_{ch}$ for the exponential parametrization $\Omega^{(E)}$. The statistical uncertainties were corrected on the $\sqrt{\chi^{2}/ndf}$ when $\chi^{2}/ndf > 1$. The statistical uncertainties smaller than systematic uncertainties. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The $Q$ distribution measured at $0.9\ TeV$ for unlike-sign pairs for $p_{T} > 100\ MeV$ and $|\eta|<2.5$, renormalized to the total number of charged-particle pairs. The error bars represents the statistical uncertainties.

The $Q$ distribution measured at $0.9\ TeV$ for like-sign pairs for $p_{T} > 100\ MeV$ and $|\eta|<2.5$, renormalized to the total number of charged-particle pairs. The error bars represents the statistical uncertainties.

The $Q$ distribution measured at $7\ TeV$ for unlike-sign pairs for $p_{T} > 100\ MeV$ and $|\eta|<2.5$, renormalized to the total number of charged-particle pairs. The error bars represents the statistical uncertainties.

The $Q$ distribution measured at $7\ TeV$ for like-sign pairs for $p_{T} > 100\ MeV$ and $|\eta|<2.5$, renormalized to the total number of charged-particle pairs. The error bars represents the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $0.9\ TeV$ using unlike-charge particle reference sample for different $n_{ch}$ intervals $p_{T} > 100\ MeV$ and $|\eta|<2.5$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $0.9\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals with multiplicity $n_{ch} \ge 2$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different multiplicity intervals $n_{ch}$ with $p_{T} > 100\ MeV$ and $|\eta| < 2.5$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals with multiplicity $n_{ch} \ge 2$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV\ HM$ using unlike-charge particle reference sample for different $n_{ch}$ intervals $p_{T} > 100\ MeV$ and $|\eta|<2.5$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured with $7\ TeV\ HM$ data using unlike-charge particle reference sample for different $k_{T}$ intervals with multiplicity $n_{ch} \ge 150$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals within multiplicity interval $n_{ch} = 2-9$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals within multiplicity interval $n_{ch} = 10-24$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals within multiplicity interval $n_{ch} = 25-80$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals within multiplicity interval $n_{ch} = 81-125$. The error bars represents only the statistical uncertainties.

Energy dependence of average photon multiplicity in INEL proton-proton collisions.

Energy dependence of average photon multiplicity in NSD proton-proton collisions.

Photon pseudorapidity distribution in INEL proton-proton collisions at sqrt(s)=0.9 TeV.

Photon pseudorapidity distribution in INEL proton-proton collisions at sqrt(s)=2.76 TeV.

Photon pseudorapidity distribution in INEL proton-proton collisions at sqrt(s)=7 TeV.