Distribution of exclusive jet multiplicity.

Distribution of pT (leading jet) [GeV] with at least one jet in the event.

Distribution of pT (leading jet) [GeV] with exactly one jet in the event.

Distribution of pT (leading jet) [GeV] with at least two jets in the event.

Distribution of pT (leading jet) [GeV] with at least three jets in the event.

Distribution of pT (2nd jet) [GeV] with at least two jets in the event.

Distribution of pT (3rd jet) [GeV] with at least three jets in the event.

Distribution of ST [GeV] with at least two jets in the event.

Distribution of ST [GeV] with exactly two jets in the event.

Distribution of ST [GeV] with at least three jets in the event.

Distribution of ST [GeV] with exactly three jets in the event.

Distribution of DR(jj) [GeV] with at least two jets in the event.

Distribution of DPhi(jj) [GeV] with at least two jets in the event.

Distribution of m(jj) [GeV] with at least two jets in the event.

Distribution of leading jet rapidity with at least one jet in the event.

Distribution of 2nd jet rapidity with at least two jets in the event.

Distribution of 3rd jet rapidity with at least three jets in the event.

The nuclear modification factor of charged particles as a function of transverse momentum, measured in minimum-bias (NSD) p-Pb collisions at sqrt(sNN) = 5.02 TeV in two pseudorapidity ranges, |eta(cms)| < 0.3 and -1.3 < eta(cms) < 0.3.

Proton-to-pion ratios as a function of pT measured in Pb-Pb and pp collisions.

Kaon-to-pion ratios as a function of pT measured in Pb-Pb and pp collisions.

The nuclear modification factor RAA as a function of pT for different particle species, for 0-5% collision centralities.

The nuclear modification factor RAA as a function of pT for different particle species, for 60-80% collision centralities.

The inclusive (SPS+DPS) cross-section ratio (times 10^6) as a function of J/psi transverse momentum under the TRANSVERSE-0 spin-alignment hypothesis. The first uncertainty is statistical and the second uncertainty is systematic.

The inclusive (SPS+DPS) cross-section ratio (times 10^6) as a function of J/psi transverse momentum under the TRANSVERSE-P spin-alignment hypothesis. The first uncertainty is statistical and the second uncertainty is systematic.

The inclusive (SPS+DPS) cross-section ratio (times 10^6) as a function of J/psi transverse momentum under the TRANSVERSE-M spin-alignment hypothesis. The first uncertainty is statistical and the second uncertainty is systematic.

Z0 total and fiducial production cross sections times branching fractions.

W+ to W- ratios of total and fiducial production cross sections times branching fractions.

(W+ + W-) to Z0 ratios of total and fiducial production cross sections times branching fractions.

pT-differential cross section of prompt Ds+ mesons measured in p-Pb collisions in the rapidity interval -0.96<y_cms<0.04.

Nuclear modification factor R(pPb) of prompt D0 mesons vs. pT measured in p-Pb collisions in the rapidity interval -0.96<y_cms<0.04.

Nuclear modification factor R(pPb) of D+ mesons vs. pT measured in p-Pb collisions in the rapidity interval -0.96<y_cms<0.04.

Nuclear modification factor R(pPb) of D*+ mesons vs. pT measured in p-Pb collisions in the rapidity interval -0.96<y_cms<0.04.

Nuclear modification factor R(pPb) of Ds+ mesons vs. pT measured in p-Pb collisions in the rapidity interval -0.96<y_cms<0.04.

Average of D0, D+, D*+ nuclear modification factors R(pPb) vs. pT.

$p_{\rm T}$-differential yield of (K$^{*0}$ + $\overline{K^{*0}}$)/2 in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (20-40% multiplicity class).

$p_{\rm T}$-differential yield of (K$^{*0}$ + $\overline{K^{*0}}$)/2 in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (40-60% multiplicity class).

$p_{\rm T}$-differential yield of (K$^{*0}$ + $\overline{K^{*0}}$)/2 in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (60-80% multiplicity class).

$p_{\rm T}$-differential yield of (K$^{*0}$ + $\overline{K^{*0}}$)/2 in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (80-100multiplicity class).

$p_{\rm T}$-differential invariant yield of $phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (NSD). Additional systematic error: +- 3.1% (normalization).

$p_{\rm T}$-differential yield of $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (0-5% multiplicity class).

$p_{\rm T}$-differential yield of $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (5-10% multiplicity class).

$p_{\rm T}$-differential yield of $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (10-20% multiplicity class).

$p_{\rm T}$-differential yield of $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (20-40% multiplicity class).

$p_{\rm T}$-differential yield of $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (40-60% multiplicity class).

$p_{\rm T}$-differential yield of $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (60-80% multiplicity class).

$p_{\rm T}$-differential yield of $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (80-100% multiplicity class).

$p_{\rm T}$-integrated yield d$N$/d$y$ of (K$^{*0}$ + $\overline{K^{*0}}$)/2 in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV. Yields are normalised to the visible cross section for each V0A multiplicity event class and to NSD events for the minimum bias case (additional normalization systematic error: +- 3.1%).

Mean $p_{\rm T}$ of (K$^{*0}$ + $\overline{K^{*0}}$)/2 in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV for each V0A multiplicity event class.

$p_{\rm T}$-integrated yield d$N$/d$y$ of $phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV. Yields are normalised to the visible cross section for each V0A multiplicity event class and to NSD events for the minimum bias case (additional normalization systematic error: +- 3.1%).

Mean $p_{\rm T}$ of $phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV for each V0A multiplicity event class.

Mean $p_{\rm T}$ as function of the mass for particles measured with the ALICE detector in INEL pp collisions at $\sqrt{s}$ = 7 TeV in |y| < 0.5.

Mean $p_{\rm T}$ as function of the mass for particles measured with the ALICE detector in 0-20% p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}$ = 5.02 TeV in -0.5 < y < 0.

Ratio of $p_{\rm T}$-differential yields of (p + $\bar{p}$) and $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (0-5$\%$ multiplicity class).

Ratio of $p_{\rm T}$-differential yields of (p + $\bar{p}$) and $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (5-10% multiplicity class).

Ratio of $p_{\rm T}$-differential yields of (p + $\bar{p}$) and $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (10-20% multiplicity class).

Ratio of $p_{\rm T}$-differential yields of (p + $\bar{p}$) and $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (20-40% multiplicity class).

Ratio of $p_{\rm T}$-differential yields of (p + $\bar{p}$) and $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (40-60% multiplicity class).

Ratio of $p_{\rm T}$-differential yields of (p + $\bar{p}$) and $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (60-80% multiplicity class).

Ratio of $p_{\rm T}$-differential yields of (p + $\bar{p}$) and $\phi$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (80-100% multiplicity class).

Ratio of $p_{\rm T}$-integrated yields of $(K^{*0}+\overline{K^{*0}})$ to long lived hadrons for different V0A multiplicity classes in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV.

Ratio of $p_{\rm T}$-integrated yields of 2$\phi$ to long lived hadrons for different V0A multiplicity classes in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV.

Summary of results for cross-section of non-prompt $J/\psi$ decaying to a muon pair for 8 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of prompt $\psi(2S)$ decaying to a muon pair for 7 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of prompt $\psi(2S)$ decaying to a muon pair for 8 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of non-prompt $\psi(2S)$ decaying to a muon pair for 7 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of non-prompt $\psi(2S)$ decaying to a muon pair for 8 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $J/\psi$ decaying to a muon pair as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $J/\psi$ decaying to a muon pair as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $\psi(2S)$ decaying to a muon pair as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $\psi(2S)$ decaying to a muon pair as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Mean weight correction factor for $J/\psi$ under the "longitudinal" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "transverse zero" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "transverse positive" spin-alignment transverse positive hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "transverse negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "longitudinal" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "transverse zero" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "transverse positive" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "transverse negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "longitudinal" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "transverse zero" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "transverse positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "transverse negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "longitudinal" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "transverse zero" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "transverse positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "transverse negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Ratios of transverse-momentum distributions of charged particles in three intervals of multiplicities to the respective one for inclusive (INEL>0) collisions. The spectra were normalised by the integral prior to division.

Fig. 5: Ratio between the $v_{2}^{\mu}\{\rm{2PC,sub}\}$ coefficients from muon-tracklet correlations in Pb-going direction and in the p-going direction.

Invariant yields of identified pions in Pb-Pb collisions.

Invariant yields of identified kaons in Pb-Pb collisions.

Invariant yields of identified protons in Pb-Pb collisions.

The nuclear modification factor RAA as a function of pT for different particle species in 0-5% Pb-Pb collisions.

The nuclear modification factor RAA as a function of pT for different particle species in 5-10% Pb-Pb collisions.

The nuclear modification factor RAA as a function of pT for different particle species in 10-20% Pb-Pb collisions.

The nuclear modification factor RAA as a function of pT for different particle species in 20-40% Pb-Pb collisions.

The nuclear modification factor RAA as a function of pT for different particle species in 40-60% Pb-Pb collisions.

The nuclear modification factor RAA as a function of pT for different particle species in 60-80% Pb-Pb collisions.

Kaon-to-pion ratios as a function of pT measured in Pb-Pb collisions.

Proton-to-pion ratios as a function of pT measured in Pb-Pb collisions.

Kaon-to-pion ratio integrated for pT > 10 GeV/c measured in Pb-Pb collisions.

Proton-to-pion ratio integrated for pT > 10 GeV/c measured in Pb-Pb collisions.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 0-5%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 5-10%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 5-10%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 5-10%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 5-10%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 10-20%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 10-20%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 10-20%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 10-20%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 20-30%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 20-30%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 20-30%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 20-30%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 30-40%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 30-40%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 30-40%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 30-40%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 40-50%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 40-50%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 40-50%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 40-50%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 50-60%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 50-60%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 50-60%.

Ratio of $\rm v_{2}\{{SP}\}$ in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 50-60%.

Centrality dependence of the average $\rm v_{2}\{{SP}\}$ variation in the $\rm large-q_{2}^{TPC}$.

Centrality dependence of the average $\rm v_{2}\{{SP}\}$ variation in the $\rm small-q_{2}^{TPC}$.

Centrality dependence of the average $\rm v_{2}\{{SP}\}$ variation in the $\rm large-q_{2}^{V0C}$.

Centrality dependence of the average $\rm v_{2}\{{SP}\}$ variation in the $\rm small-q_{2}^{V0C}$.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the absolute values of the $q_{2}^{TPC}$, centrality 5-10%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the absolute values of the $q_{2}^{V0C}$, centrality 5-10%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the self-normalized values of the $q_{2}^{TPC}$, centrality 5-10%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the self-normalized values of the $q_{2}^{V0C}$, centrality 5-10%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the absolute values of the $q_{2}^{TPC}$, centrality 30-40%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the absolute values of the $q_{2}^{V0C}$, centrality 30-40%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the self-normalized values of the $q_{2}^{TPC}$, centrality 30-40%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the self-normalized values of the $q_{2}^{V0C}$, centrality 30-40%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the absolute values of the $q_{2}^{TPC}$, centrality 50-60%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the absolute values of the $q_{2}^{V0C}$, centrality 50-60%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the self-normalized values of the $q_{2}^{TPC}$, centrality 50-60%.

Average $\rm v_{2}\{{SP}\}$ variation as a function of the self-normalized values of the $q_{2}^{V0C}$, centrality 50-60%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 0-5%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 0-5%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 0-5%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 0-5%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 5-10%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 5-10%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 5-10%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 5-10%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 10-20%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 10-20%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 10-20%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 10-20%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 20-30%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 20-30%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 20-30%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 20-30%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 30-40%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 30-40%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 30-40%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 30-40%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 40-50%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 40-50%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 40-50%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 40-50%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{TPC}$ to unbiased sample, centrality 50-60%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{TPC}$ to unbiased sample, centrality 50-60%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm large-q_{2}^{V0C}$ to unbiased sample, centrality 50-60%.

Ratio of the $p_{\rm T}$ distribution of charged hadrons in the $\rm small-q_{2}^{V0C}$ to unbiased sample, centrality 50-60%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 0-5%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 0-5%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 0-5%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 0-5%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 0-5%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 0-5%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 5-10%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 5-10%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 5-10%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 5-10%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 5-10%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 5-10%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 10-20%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 10-20%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 10-20%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 10-20%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 10-20%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 10-20%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 20-30%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 20-30%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 20-30%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 20-30%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 20-30%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 20-30%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 30-40%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 30-40%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 30-40%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 30-40%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 30-40%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 30-40%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 40-50%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 40-50%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 40-50%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 40-50%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 40-50%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 40-50%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 50-60%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 50-60%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{TPC}$ sample to the unbiased sample, centrality 50-60%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 50-60%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 50-60%.

Fig. 10: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm large-q_{2}^{V0C}$ sample to the unbiased sample, centrality 50-60%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 0-5%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 0-5%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 0-5%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 0-5%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 0-5%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 0-5%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 5-10%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 5-10%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 5-10%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 5-10%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 5-10%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 5-10%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 10-20%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 10-20%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 10-20%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 10-20%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 10-20%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 10-20%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 20-30%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 20-30%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 20-30%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 20-30%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 20-30%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 20-30%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 30-40%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 30-40%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 30-40%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 30-40%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 30-40%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 30-40%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 40-50%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 40-50%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 40-50%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 40-50%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 40-50%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 40-50%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 50-60%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 50-60%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{TPC}$ sample to the unbiased sample, centrality 50-60%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified pions in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 50-60%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified kaons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 50-60%.

Fig. 11: Ratio of the $p_{\rm T}$ distribution of identified protons in the $\rm small-q_{2}^{V0C}$ sample to the unbiased sample, centrality 50-60%.

Ratio of the fiducial cross section for $t\bar{t}$ events with two leptons and at least four b-jets to the fiducial cross section for $t\bar{t}$ events with two leptons and at least four jets, at least two of which must be b-jets. The definition of the cross-sections includes $t\bar{t}+Z / H$ events that pass the fiducial requirements.

Measured fiducial cross section for $t\bar{t}$ events with exactly one lepton and at least five jets, of which at least three are b-jets. The definition of the cross-section excludes $t\bar{t}+Z / H$ events that pass the fiducial requirements.

Measured fiducial cross section for $t\bar{t}$ events with two leptons and at least three b-jets. The definition of the cross-section excludes $t\bar{t}+Z / H$ events that pass the fiducial requirements.

Measured fiducial cross section for $t\bar{t}$ events with two leptons and at least four b-jets. The definition of the cross-section excludes $t\bar{t}+Z / H$ events that pass the fiducial requirements.

Ratio of the fiducial cross section for $t\bar{t}$ events with two leptons and at least four b-jets to the fiducial cross section for $t\bar{t}$ events with two leptons and at least four jets, at least two of which must be b-jets. The definition of the cross-sections excludes $t\bar{t}+Z / H$ events that pass the fiducial requirements.

Centrality dependence of the Psi(2S) Q_pPb in the backward rapidity range (-4.46<y_cms<-2.96). The first uncertainty is statistical, the second is a systematic one. The third systematic uncertainty is fully correlated over centrality, while the fourth one is fully correlated over centrality and correlated between the JPsi and the Psi(2S) charmonium states.

Centrality dependence of the Psi(2S) Q_pPb in the forward rapidity range (2.03<y_cms<3.53). The first uncertainty is statistical, the second is the systematic one. The third systematic uncertainty is fully correlated over centrality, while the fourth one is fully correlated over centrality and correlated between the JPsi and the Psi(2S) charmonium states.

Psi(2S)/J/Psi)_pA/(Psi(2S)/J/Psi)_pp double ratio in the backward rapidity range (-4.46<y_cms<-2.96) plotted as a function of the crossing time. The first uncertainty is statistical, the second is the systematic one.

Psi(2S)/J/Psi)_pA/(Psi(2S)/J/Psi)_pp double ratio in the forward rapidity range (2.03<y_cms<3.53) plotted as a function of the crossing time. The first uncertainty is statistical, the second is the systematic one.

Double Ratio RGAMMA in 0-20% central inelastic PbPb collisions at center-of-mass energy per nucleon 2.76 TeV.

Double Ratio RGAMMA in 20-40% central inelastic PbPb collisions at center-of-mass energy per nucleon 2.76 TeV.

Double Ratio RGAMMA in 40-80% central inelastic PbPb collisions at center-of-mass energy per nucleon 2.76 TeV.

Invariant differential yields of inclusive GAMMA produced in 0-20% central inelastic PbPb collisions at center-of-mass energy per nucleon 2.76 TeV.

Invariant differential yields of inclusive GAMMA produced in 20-40% central inelastic PbPb collisions at center-of-mass energy per nucleon 2.76 TeV.

Invariant differential yields of inclusive GAMMA produced in 40-80% central inelastic PbPb collisions at center-of-mass energy per nucleon 2.76 TeV.

Inclusive J/$\psi$ $R_{\rm AA}$ and Pb-Pb yields as a function of centrality, $p_{\rm T}<2$ GeV/$c$ and $2.5<y<4.0$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 15% (12%) affects all the $R_{\rm AA}$ (yields) values.

Inclusive J/$\psi$ $R_{\rm AA}$ and Pb-Pb yields as a function of centrality, $2<p_{\rm T}<5$ GeV/$c$ and $2.5<y<4.0$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 14% (11%) affects all the $R_{\rm AA}$ (yields) values.

Inclusive J/$\psi$ $R_{\rm AA}$ and Pb-Pb yields as a function of centrality, $5<p_{\rm T}<8$ GeV/$c$ and $2.5<y<4.0$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 18% (10%) affects all the $R_{\rm AA}$ (yields) values.

Inclusive J/$\psi$ $R_{\rm AA}$ and Pb-Pb yields as a function of $p_{\rm T}$ for the 0-20% centrality class and $2.5<y<4.0$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 8% (4%) affects all the $R_{\rm AA}$ (yields) values.

Inclusive J/$\psi$ $R_{\rm AA}$ and Pb-Pb yields as a function of $p_{\rm T}$ for the 20-40% centrality class and $2.5<y<4.0$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 8% (4%) affects all the $R_{\rm AA}$ (yields) values.

Inclusive J/$\psi$ $R_{\rm AA}$ and Pb-Pb yields as a function of $p_{\rm T}$ for the 0-40% centrality class and $2.5<y<4.0$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 8% (4%) affects all the $R_{\rm AA}$ (yields) values.

Inclusive J/$\psi$ $R_{\rm AA}$ and Pb-Pb yields as a function of $p_{\rm T}$ for the 40-90% centrality class and $2.5<y<4.0$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 9% (4%) affects all the $R_{\rm AA}$ (yields) values.

Inclusive J/$\psi$ $R_{\rm AA}$ and Pb-Pb yields as a function of $p_{\rm T}$ for the 0-90% centrality class and $2.5<y<4.0$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 8% (4%) affects all the $R_{\rm AA}$ (yields) values.

Inclusive J/$\psi$ $R_{\rm AA}$ and Pb-Pb yields as a function of $y$ for the 0-90% centrality class and $p_{\rm T}<8$ GeV/$c$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 8% (4%) affects all the $R_{\rm AA}$ (yields) values.

Inclusive J/$\psi$ $R_{\rm AA}$ as a function of centrality, $0.3 <p_{\rm T}<8$ GeV/$c$ and $0.3<p_{\rm T}<2$ GeV/$c$ in the rapidity range $2.5<y<4.0$. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 15% affects all the $R_{\rm AA}$ values.

Inclusive J/$\psi$ $R_{\rm AA}$ for $2.5<y<4.0$ in the centrality classes 0-90%, 0-20%, 20-40 and 40-90% for the lowest $p_{\rm T}$ range when the $0.3$ GeV/$c$ $p_{\rm T}$ cut is applied. Statistical and systematic uncertainties are also reported. A global systematic uncertainty of 8%, 8%, 8% and 9% affect the $R_{\rm AA}$ values, respectively.

Inclusive $[\psi\text{(2S)/J/}\psi]_{\rm Pb-Pb}$ and $[\psi\text{(2S)/J/}\psi]_{\rm Pb-Pb}\;/\;[\psi\text{(2S)/J/}\psi]_{\rm pp}$ ratios as a function of centrality for $p_{\rm T}<3$ GeV/$c$. Statistical and systematic uncertainties are reported when the value is not given as an upper limit.

Inclusive $[\psi\text{(2S)/J/}\psi]_{\rm Pb-Pb}$ and $[\psi\text{(2S)/J/}\psi]_{\rm Pb-Pb}\;/\;[\psi\text{(2S)/J/}\psi]_{\rm pp}$ ratios as a function of centrality for $3<p_{\rm T}<8$ GeV/$c$.

$p_{\rm T}$ dependence of the J/$\psi$ nuclear modification factor $R_{\rm pA}$ in the backward rapidity range (-4.46<$y_{\rm cms}$<-2.96). The first uncertainty is statistical, the second one is the $p_{\rm T}$-uncorrelated systematic uncertainty, the third is the partially $p_{\rm T}$-correlated, while the fourth is the $p_{\rm T}$-correlated one.

$p_{\rm T}$ dependence of the J/$\psi$ nuclear modification factor $R_{\rm pA}$ in the mid-rapidity range (-1.37<$y_{\rm cms}$<-0.43). The first uncertainty is statistical, the second one is the $p_{\rm T}$-uncorrelated systematic uncertainty, the third is the $p_{\rm T}$-correlated one.

$p_{\rm T}$ dependence of the J/$\psi$ nuclear modification factor $R_{\rm pA}$ in the forward rapidity range (2.03<$y_{\rm cms}$<3.53). The first uncertainty is statistical, the second one is the $p_{\rm T}$-uncorrelated systematic uncertainty, the third is the partially $p_{\rm T}$-correlated, while the fourth is the $p_{\rm T}$-correlated one.

Estimate of the $p_{\rm T}$-dependence of the Cold Nuclear Matter effects in Pb-Pb collisions calculated as $R^2_{\rm pPb}$. The first uncertainty is statistical, the second one is the $p_{\rm T}$-uncorrelated systematic uncertainty, the third is the $p_{\rm T}$-correlated one.

Estimate of the $p_{\rm T}$-dependence of the Cold Nuclear Matter effects in Pb-Pb collisions calculated as $R_{\rm pPb}$(-4.46 <y< -2.96) $\times$ $R_{\rm pPb}$(2.03 <y< 3.53). The first uncertainty is statistical, the second one is the $p_{\rm T}$-uncorrelated systematic uncertainty, the third is the partially $p_{\rm T}$-correlated, while the fourth is the $p_{\rm T}$ correlated one.

$p_{\rm T}$-dependence of the ratio between the $R_{\rm PbPb}$ and the cold nuclear matter effects evaluated as $R_{\rm pPb}$(-4.46 <y< -2.96) $\times$ $R_{\rm pPb}$(2.03 <y< 3.53). The first uncertainty is statistical, the second one is the quadratic combination of $p_{\rm T}$-uncorrelated and $p_{\rm T}$-partially correlated systematic uncertainties, while the third is the $p_{\rm T}$ correlated one.

Per-trigger yield modification, $I_{\rm AA}$, on the away side with trigger $\pi^{0}$ particle at $8 < p_{T}^{trig} < 16~GeV/c$ for $0$-$10$$\%$ Pb-Pb collisions at $\sqrt{s_{NN}}$= 2.76 TeV.

Efficiency for the calorimetric MET>80 GeV trigger as a function of the metastable R-hadron mass. The R-hadron decays to g/qq plus neutralino of mass = m(gluino) - 100 GeV with a lifetime of 1 ns.

Efficiency for the calorimetric MET>80 GeV trigger as a function of the metastable R-hadron mass. The R-hadron decays to g/qq plus neutralino of mass 100 GeV with a lifetime of 1 ns.

Efficiency for the calorimetric MET>80 GeV trigger as a function of the stable chargino mass.

Total selection efficiency as a function of the stable R-hadron mass.

Total selection efficiency as a function of the metastable R-hadron mass. The R-hadron decays to g/qq plus neutralino of mass 100 GeV with a lifetime of 10 ns.

Total selection efficiency as a function of the metastable R-hadron mass. The R-hadron decays to g/qq plus neutralino of mass = m(gluino) - 100 GeV with a lifetime of 10 ns.

Total selection efficiency as a function of the metastable R-hadron mass. The R-hadron decays to g/qq plus neutralino of mass 100 GeV with a lifetime of 1 ns.

Total selection efficiency as a function of the stable chargino mass.

Ionisation distribution of all the CR2 tracks, and those not matched to a reconstructed muon. The two distributions are normalised to their total number of entries.

Distribution of the mass of selected candidates, derived from the specific ionisation loss, for an example of gluino R-hadron signal, for searches for stable particles. The signal distributions are stacked on the expected background, and a narrower binning is used for them to allow the signal shape to be seen more clearly. The number of signal events is that expected according to the theoretical cross sections.

Distribution of the mass of selected candidates, derived from the specific ionisation loss, for one example of chargino signal, for searches for stable particles. The signal distributions are stacked on the expected background, and a narrower binning is used for them to allow the signal shape to be seen more clearly. The number of signal events is that expected according to the theoretical cross sections.

Distribution of the mass of selected candidates, derived from the specific ionisation loss, for background and data, for searches for stable particles. The expected background is shown with its total uncertainty (sum in quadrature of statistical, normalisation and systematic errors).

Distribution of the mass of selected candidates, derived from the specific ionisation loss, for an example of gluino R-hadron signal, for searches for metastable particles. The signal distributions are stacked on the expected background, and a narrower binning is used for them to allow the signal shape to be seen more clearly. The number of signal events is that expected according to the theoretical cross sections.

Distribution of the mass of selected candidates, derived from the specific ionisation loss, for an example of chargino signal, for searches for metastable particles. The signal distributions are stacked on the expected background, and a narrower binning is used for them to allow the signal shape to be seen more clearly. The number of signal events is that expected according to the theoretical cross sections.

Distribution of the mass of selected candidates, derived from the specific ionisation loss, for background and data. The expected background is shown with its total uncertainty (sum in quadrature of statistical, normalisation and systematic errors).

Theoretical values for the cross section of gluino pairs production with their uncertainty.

Expected upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau =10 ns, decaying into g/qq plus a light neutralino of mass 100 GeV, in the background-only case, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau =10 ns, decaying into g/qq plus a light neutralino of mass 100 GeV.

Expected upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau =10 ns, decaying into g/qq plus a heavy neutralino of mass(gluino) - 100 GeV, in the background-only case, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau =10 ns, decaying into g/qq plus a heavy neutralino of mass(gluino) - 100 GeV.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section, plus 1 experimental sigma.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section, minus 1 experimental sigma.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section minus its uncertainty.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section plus its uncertainty.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section, plus 1 experimental sigma.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section, minus 1 experimental sigma.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section minus its uncertainty.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into g/qq plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section plus its uncertainty.

Expected upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau =10 ns, decaying into tt plus a light neutralino of mass 100 GeV, in the background-only case, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau =10 ns, decaying into tt plus a light neutralino of mass 100 GeV.

Expected upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau =10 ns, decaying into tt plus a heavy neutralino of mass(gluino) - 100 GeV, in the background-only case, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau =10 ns, decaying into tt plus a heavy neutralino of mass(gluino) - 100 GeV.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section, plus 1 experimental sigma.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section, minus 1 experimental sigma.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section minus its uncertainty.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a light neutralino of mass 100 GeV, with respect to the nominal theoretical cross section plus its uncertainty.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section, plus 1 experimental sigma.

The expected excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section, minus 1 experimental sigma.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section minus its uncertainty.

The observed excluded range of lifetimes as a function of gluino mass for gluino R-hadrons decaying into tt plus a heavy neutralino of mass = m(gluino) - 100 GeV, with respect to the nominal theoretical cross section plus its uncertainty.

Theoretical values for the production cross section of charginos or chargino/neutralino pairs, with their uncertainty.

Expected upper limits on the production cross section as a function of mass for metastable charginos, with lifetime tau =1.0 ns, decaying into neutralino + pion, in the background-only case, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable charginos, with lifetime tau =1.0 ns, decaying into neutralino + pion.

The expected excluded range of lifetimes as a function of chargino mass for charginos decaying into neutralino plus pion, with respect to the nominal theoretical cross section.

The expected excluded range of lifetimes as a function of chargino mass for charginos decaying into neutralino plus pion, with respect to the nominal theoretical cross section, plus 1 experimental sigma.

The expected excluded range of lifetimes as a function of chargino mass for charginos decaying into neutralino plus pion, with respect to the nominal theoretical cross section, minus 1 experimental sigma.

The observed excluded range of lifetimes as a function of chargino mass for charginos decaying into neutralino plus pion, with respect to the nominal theoretical cross section.

The observed excluded range of lifetimes as a function of chargino mass for charginos decaying into neutralino plus pion, with respect to the nominal theoretical cross section minus its uncertainty.

The observed excluded range of lifetimes as a function of gluino mass for chargino mass for charginos decaying into neutralino plus pion, with respect to the nominal theoretical cross section plus its uncertainty.

dEdx ionization for data, 1 TeV gluino R-hadrons stable and decaying in 100 GeV neutralinos with a 10 ns lifetime and for charginos of 350 GeV. Tracks that fulfil all the requirements up to including the High-m_T (see Tab.1 in the paper) are considered at this stage and normalised to an integrated luminosity of 18.4 fb^-1.

Expected upper limits on the production cross section as a function of mass for stable gluino R-hadrons, in case of background only, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for stable gluino R-hadrons.

Theoretical values for the cross section of squark pairs production with their uncertainty.

Expected upper limits on the production cross section as a function of mass for stable sbottom R-hadrons, in case of background only, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for stable sbottom $R$-hadrons. Cross section IN PB.

Expected upper limits on the production cross section as a function of mass for stop R-hadrons, in case of background only, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for stop R-hadrons.

Expected upper limits on the production cross section as a function of mass for stable charginos, in case of background only, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for stable charginos.

Expected upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau=1.0 ns, decaying to g/qq plus a light neutralino of mass 100 GeV.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau=1.0 ns, decaying to g/qq plus a light neutralino of mass 100 GeV.

Expected upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau=1.0 ns, decaying to g/qq plus a heavy neutralino of mass = m(gluino) - 100 GeV.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau=1.0 ns, decaying to g/qq plus a heavy neutralino of mass = m(gluino) - 100 GeV.

Expected upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau=1.0 ns, decaying to tt plus a light neutralino of mass 100 GeV.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau=1.0 ns, decaying to tt plus a light neutralino of mass 100 GeV.

Expected upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau=1.0 ns, decaying to tt plus a heavy neutralino of mass = m(gluino) - 100 GeV.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable gluino R-hadrons, with lifetime tau=1.0 ns, decaying to tt plus a heavy neutralino of mass = m(gluino) - 100 GeV.

Expected upper limits on the production cross section as a function of mass for metastable charginos, with lifetime tau =15 ns, decaying to neutralino and pion, in case of background only, with its 1 sigma band.

Observed 95 PCT upper limits on the production cross section as a function of mass for metastable charginos, with lifetime tau =15 ns, decaying to neutralino and pion, in case of background only, with its 1 sigma band.

Double differential cross-section for $J/\psi$-from-$b$ mesons as a function of $p_\perp$ in bins of $y$. The first uncertainties are statistical, the second are the correlated systematic uncertainties shared between bins and the last are the uncorrelated systematic uncertainties.

The fraction of $J/\psi$-from-$b$ mesons (in %) in bins of the $J/\psi$ $p_\perp$ and $y$. The uncertainties are statistical only. The systematic uncertainties are negligible.

The fraction of $J/\psi$-from-$b$ mesons (in %) in bins of the $J/\psi$ $p_\perp$ and $y$. The uncertainties are statistical only. The systematic uncertainties are negligible.

Differential cross-sections as a function of $p_\perp$ integrated over $y$ for prompt $J/\psi$ mesons. The first uncertainties are statistical and the second (third) are uncorrelated (correlated) systematic uncertainties amongst bins.

Differential cross-sections as a function of $p_\perp$ integrated over $y$ for prompt $J/\psi$ mesons. The first uncertainties are statistical and the second (third) are uncorrelated (correlated) systematic uncertainties amongst bins.

Differential cross-sections as a function of $p_\perp$ integrated over $y$ for $J/\psi$-from-$b$ mesons. The first uncertainties are statistical and the second (third) are uncorrelated (correlated) systematic uncertainties amongst bins.

Differential cross-sections as a function of $p_\perp$ integrated over $y$ for $J/\psi$-from-$b$ mesons. The first uncertainties are statistical and the second (third) are uncorrelated (correlated) systematic uncertainties amongst bins.

Differential cross-sections as a function of $y$ integrated over $p_\perp$ for prompt $J/\psi$ mesons. The first uncertainties are statistical and the second (third) are the correlated (uncorrelated) systematic uncertainties.

Differential cross-sections as a function of $y$ integrated over $p_\perp$ for prompt $J/\psi$ mesons. The first uncertainties are statistical and the second (third) are the correlated (uncorrelated) systematic uncertainties.

Differential cross-sections as a function of $y$ integrated over $p_\perp$ for $J/\psi$-from-$b$ mesons. The first uncertainties are statistical and the second (third) are the correlated (uncorrelated) systematic uncertainties.

Differential cross-sections as a function of $y$ integrated over $p_\perp$ for $J/\psi$-from-$b$ mesons. The first uncertainties are statistical and the second (third) are the correlated (uncorrelated) systematic uncertainties.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $p_\perp$ in bins of $y$ for prompt $J/\psi$ mesons. The systematic errors are negligible.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $p_\perp$ in bins of $y$ for prompt $J/\psi$ mesons. The systematic errors are negligible.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $p_\perp$ in bins of $y$ for $J/\psi$-from-$b$ mesons. The systematic errors are negligible.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $p_\perp$ in bins of $y$ for $J/\psi$-from-$b$ mesons. The systematic errors are negligible.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $y$ integrated over $p_\perp$ for prompt $J/\psi$ mesons. The systematic errors are negligible.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $y$ integrated over $p_\perp$ for prompt $J/\psi$ mesons. The systematic errors are negligible.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $y$ integrated over $p_\perp$ for $J/\psi$-from-$b$ mesons. The systematic errors are negligible.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $y$ integrated over $p_\perp$ for $J/\psi$-from-$b$ mesons. The systematic errors are negligible.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $p_\perp$ integrated over $y$ for prompt $J/\psi$ mesons.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $p_\perp$ integrated over $y$ for prompt $J/\psi$ mesons.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $p_\perp$ integrated over $y$ for $J/\psi$-from-$b$ mesons. The systematic errors are negligible.

Ratios of differential cross-sections between measurements at $\sqrt{s} = 13$ TeV and $\sqrt{s} = 8$ TeV as a function of $p_\perp$ integrated over $y$ for $J/\psi$-from-$b$ mesons. The systematic errors are negligible.

$K^{0}_{S}$ transverse momentum spectrum: V0M Class IV (pp at $\sqrt{s}=7$ TeV).

$K^{0}_{S}$ transverse momentum spectrum: V0M Class V (pp at $\sqrt{s}=7$ TeV).

$K^{0}_{S}$ transverse momentum spectrum: V0M Class VI (pp at $\sqrt{s}=7$ TeV).

$K^{0}_{S}$ transverse momentum spectrum: V0M Class VII (pp at $\sqrt{s}=7$ TeV).

$K^{0}_{S}$ transverse momentum spectrum: V0M Class VIII (pp at $\sqrt{s}=7$ TeV).

$K^{0}_{S}$ transverse momentum spectrum: V0M Class IX (pp at $\sqrt{s}=7$ TeV).

$K^{0}_{S}$ transverse momentum spectrum: V0M Class X (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class I (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class II (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class III (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class IV (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class V (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class VI (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class VII (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class VIII (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class IX (pp at $\sqrt{s}=7$ TeV).

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum: V0M Class X (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class I (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class II (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class III (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class IV (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class V (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class VI (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class VII (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class VIII (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class IX (pp at $\sqrt{s}=7$ TeV).

$\Xi^{-}+\bar{\Xi}^{+}$ transverse momentum spectrum: V0M Class X (pp at $\sqrt{s}=7$ TeV).

$\Omega^{-}+\bar{\Omega}^{+}$ transverse momentum spectrum: V0M Class I+II (pp at $\sqrt{s}=7$ TeV).

$\Omega^{-}+\bar{\Omega}^{+}$ transverse momentum spectrum: V0M Class III+IV (pp at $\sqrt{s}=7$ TeV).

$\Omega^{-}+\bar{\Omega}^{+}$ transverse momentum spectrum: V0M Class V+VI (pp at $\sqrt{s}=7$ TeV).

$\Omega^{-}+\bar{\Omega}^{+}$ transverse momentum spectrum: V0M Class VII+VIII (pp at $\sqrt{s}=7$ TeV).

$\Omega^{-}+\bar{\Omega}^{+}$ transverse momentum spectrum: V0M Class IX+X (pp at $\sqrt{s}=7$ TeV).

$2K^{0}_{S}/(\pi^{+}+\pi^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of the average charged particle multiplicity density at midrapidity.

$(\Lambda+\bar{\Lambda})/(\pi^{+}+\pi^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of the average charged particle multiplicity density at midrapidity.

$(\Xi^{-}+\bar{\Xi}^{+})/(\pi^{+}+\pi^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of the average charged particle multiplicity density at midrapidity.

$(\Omega^{-}+\bar{\Omega}^{+})/(\pi^{+}+\pi^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of the average charged particle multiplicity density at midrapidity.

$\pi^{+}+\pi^{-}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$p+\bar{p}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$K^{0}_{S}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$\Lambda+\bar{\Lambda}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$\Xi^{-}+\bar{\Xi}^{+}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$\Omega^{-}+\bar{\Omega}^{+}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$(\Lambda+\bar{\Lambda})/2K^{0}_{S}$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of charged particle multiplicity density at midrapidity.

$(p+\bar{p})/(\pi^{+}+\pi^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of charged particle multiplicity density at midrapidity.

$(2K^{0}_{S})/(\pi^{+}+\pi^{-})$ double-ratio vs multiplicity for pp collisions at $\sqrt{s}=7$ TeV.

$(\Lambda+\bar{\Lambda})/(\pi^{+}+\pi^{-})$ double-ratio vs multiplicity for pp collisions at $\sqrt{s}=7$ TeV.

$(\Xi^{-}+\bar{\Xi}^{+})/(\pi^{+}+\pi^{-})$ double-ratio vs multiplicity for pp collisions at $\sqrt{s}=7$ TeV.

$(\Omega^{-}+\bar{\Omega}^{+})/(\pi^{+}+\pi^{-})$ double-ratio vs multiplicity for pp collisions at $\sqrt{s}=7$ TeV.

Event multiplicity classes, their corresponding fraction of the INEL>0 cross-section and their corresponding average charged particle density at midrapidity ($|\eta|<0.5$). The value of in the inclusive (INEL>0) class is 5.96 $\pm$ 0.23. The uncertainties are the quadratic sum of statistical and systematic contributions.