Charged-hadron spectrum in the centrality interval 5-10% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 10-20% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 20-30% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 30-40% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 40-60% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 60-90% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 0-90% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron cross-section in pp collisions. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 0-5% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Charged-hadron spectrum in the centrality interval 5-10% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Charged-hadron spectrum in the centrality interval 10-20% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Charged-hadron spectrum in the centrality interval 20-30% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Charged-hadron spectrum in the centrality interval 30-40% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Charged-hadron spectrum in the centrality interval 40-50% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Charged-hadron spectrum in the centrality interval 50-60% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Charged-hadron spectrum in the centrality interval 60-80% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Charged-hadron cross-section in pp collisions. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 0-5% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 5-10% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 10-20% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 20-30% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 30-40% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 40-50% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 50-60% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-hadron spectrum in the centrality interval 60-80% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.

Nuclear modification factor in centrality interval 0-5% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-50% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 50-60% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-80% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 0-5% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 5-10% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 10-20% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 20-30% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 30-40% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-50% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-50% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 40-50% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 50-60% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 50-60% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 50-60% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-80% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-80% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Nuclear modification factor in centrality interval 60-80% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for pp collisions at 2.76 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 2.76 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 2.76 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for pp collisions at 2.76 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 2.76 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for pp collisions at 2.76 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 2.76 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 2.76 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 2.76 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 2.76 TeV.

Charged-particle multiplicity distribution for pp collisions at 5.02 TeV.

Koba-Nielsen-Olesen scaled charged-particle multiplicity distribution for pp collisions at 5.02 TeV.

Charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 5.02 TeV.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for pp collisions at 5.02 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 5.02 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 5.02 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for pp collisions at 5.02 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 5.02 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for pp collisions at 5.02 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 5.02 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 5.02 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 5.02 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 5.02 TeV.

Charged-particle multiplicity distribution for pp collisions at 7.0 TeV.

Koba-Nielsen-Olesen scaled charged-particle multiplicity distribution for pp collisions at 7.0 TeV.

Charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 7.0 TeV.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for pp collisions at 7.0 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 7.0 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 7.0 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for pp collisions at 7.0 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 7.0 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for pp collisions at 7.0 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 7.0 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 7.0 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 7.0 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 7.0 TeV.

Charged-particle multiplicity distribution for pp collisions at 8.0 TeV.

Koba-Nielsen-Olesen scaled charged-particle multiplicity distribution for pp collisions at 8.0 TeV.

Charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 8.0 TeV.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for pp collisions at 8.0 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 8.0 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 8.0 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for pp collisions at 8.0 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 8.0 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for pp collisions at 8.0 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 8.0 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 8.0 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 8.0 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 8.0 TeV.

Charged-particle multiplicity distribution for pp collisions at 13.0 TeV.

Koba-Nielsen-Olesen scaled charged-particle multiplicity distribution for pp collisions at 13.0 TeV.

Charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 13.0 TeV.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for pp collisions at 13.0 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 13.0 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pp collisions at 13.0 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for pp collisions at 13.0 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 13.0 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for pp collisions at 13.0 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 13.0 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pp collisions at 13.0 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 13.0 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pp collisions at 13.0 TeV.

Charged-particle multiplicity distribution for pPb collisions at 5.02 TeV.

Koba-Nielsen-Olesen scaled charged-particle multiplicity distribution for pPb collisions at 5.02 TeV.

Charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pPb collisions at 5.02 TeV.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for pPb collisions at 5.02 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pPb collisions at 5.02 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pPb collisions at 5.02 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for pPb collisions at 5.02 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pPb collisions at 5.02 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for pPb collisions at 5.02 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pPb collisions at 5.02 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pPb collisions at 5.02 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pPb collisions at 5.02 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pPb collisions at 5.02 TeV.

Charged-particle multiplicity distribution for pPb collisions at 8.16 TeV.

Koba-Nielsen-Olesen scaled charged-particle multiplicity distribution for pPb collisions at 8.16 TeV.

Charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pPb collisions at 8.16 TeV.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for pPb collisions at 8.16 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pPb collisions at 8.16 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for pPb collisions at 8.16 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for pPb collisions at 8.16 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pPb collisions at 8.16 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for pPb collisions at 8.16 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pPb collisions at 8.16 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for pPb collisions at 8.16 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pPb collisions at 8.16 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for pPb collisions at 8.16 TeV.

Charged-particle multiplicity distribution for XeXe collisions at 5.44 TeV.

Koba-Nielsen-Olesen scaled charged-particle multiplicity distribution for XeXe collisions at 5.44 TeV.

Charged-particle transverse momentum spectra as a function of charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for XeXe collisions at 5.44 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for XeXe collisions at 5.44 TeV.

Charged-particle multiplicity distribution for PbPb collisions at 2.76 TeV.

Koba-Nielsen-Olesen scaled charged-particle multiplicity distribution for PbPb collisions at 2.76 TeV.

Charged-particle transverse momentum spectra as a function of charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for PbPb collisions at 2.76 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for PbPb collisions at 2.76 TeV.

Charged-particle multiplicity distribution for PbPb collisions at 5.02 TeV.

Koba-Nielsen-Olesen scaled charged-particle multiplicity distribution for PbPb collisions at 5.02 TeV.

Charged-particle transverse momentum spectra as a function of charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Charged-particle mean transverse momentum as a function of charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Charged-particle transverse momentum spectra integrated over charged-particle multipliciy for PbPb collisions at 5.02 TeV.

Charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Charged-particle mean transverse momentum as a function of relative charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Standard deviation of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Standard deviation over mean of charged-particle transverse momentum spectra as a function of relative charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Charged-particle mean transverse momentum divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Standard deviation of charged-particle transverse momentum spectra divided by its multiplicity-integrated value as a function of relative charged-particle multiplicity for PbPb collisions at 5.02 TeV.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 5-10% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 10-20% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 20-40% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 40-60% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 60-80% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 80-100% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 0-5% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 5-10% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 10-20% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 20-40% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 40-60% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 60-80% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 80-100% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 0-5% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 5-10% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 10-20% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 20-40% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 40-60% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 60-80% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 80-100% centrality class and ZNA estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for CL1 estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for V0A estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for ZNAmult estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for ZNAPb estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions for 5 participant quarks as a function of the number of participants for CL1 estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions for 5 participant quarks as a function of the number of participants for V0A estimator.

trigger particle momentum dependence of observables RMS for wide component in p-p collisions at 7 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables RMS for wide component in p-p collisions at 7 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables RMS for wide component in p-p collisions at 7 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables RMS for narrow component in p-Pb collisions at 5.02 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables RMS for narrow component in p-Pb collisions at 5.02 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables RMS for narrow component in p-Pb collisions at 5.02 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables RMS for wide component in p-Pb collisions at 5.02 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables RMS for wide component in p-Pb collisions at 5.02 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables RMS for wide component in p-Pb collisions at 5.02 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-p collisions at 7 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-p collisions at 7 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-p collisions at 7 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-p collisions at 7 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-p collisions at 7 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-p collisions at 7 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-Pb collisions at 5.02 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-Pb collisions at 5.02 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-Pb collisions at 5.02 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-Pb collisions at 5.02 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-Pb collisions at 5.02 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-Pb collisions at 5.02 TeV with 0.6<xlong<1.0.

Transverse momentum spectra of charged particles in pp collisions.

Ratio Data/MC

Additional systematic error for pp data: +3.0 pct -3.0 pct Additional systematic error for PBPB 0-5 pct data: +0.08 pct -0.08 pct Additional systematic error for PBPB 5-10 pct data: +0.24 pct -0.24 pct Additional systematic error for PBPB 10-20 pct data: +0.46 pct -0.46 pct Additional systematic error for PBPB 20-30 pct data: +0.81 pct -0.81 pct Additional systematic error for PBPB 30-40 pct data: +1.26 pct -1.26 pct Additional systematic error for PBPB 40-50 pct data: +1.86 pct -1.86 pct Additional systematic error for PBPB 50-60 pct data: +2.64 pct -2.64 pct Additional systematic error for PBPB 60-70 pct data: +3.67 pct -3.67 pct Additional systematic error for PBPB 70-80 pct data: +5.01 pct -5.01 pct.

Additional systematic error for PBPB 0-5 pct data: +2.2 pct -2.2 pct Additional systematic error for PBPB 5-10 pct data: +2.2 pct -2.2 pct Additional systematic error for PBPB 10-20 pct data: +2.4 pct -2.4 pct Additional systematic error for PBPB 20-30 pct data: +2.7 pct -2.7 pct Additional systematic error for PBPB 30-40 pct data: +3.4 pct -3.4 pct Additional systematic error for PBPB 40-50 pct data: +3.7 pct -3.7 pct Additional systematic error for PBPB 50-60 pct data: +4.9 pct -4.9 pct Additional systematic error for PBPB 60-70 pct data: +6.7 pct -6.7 pct Additional systematic error for PBPB 70-80 pct data: +7.1 pct -7.1 pct.

Additional systematic error for PBPB 0-5 pct data: +2.7 pct -2.7 pct Additional systematic error for PBPB 5-10 pct data: +3.5 pct -3.5 pct Additional systematic error for PBPB 10-20 pct data: +3.5 pct -3.5 pct Additional systematic error for PBPB 20-30 pct data: +4.1 pct -4.1 pct Additional systematic error for PBPB 30-40 pct data: +3.7 pct -3.7 pct Additional systematic error for PBPB 40-50 pct data: +3.9 pct -3.9 pct Additional systematic error for PBPB 50-60 pct data: +3.6 pct -3.6 pct Additional systematic error for PBPB 60-70 pct data: +4.6 pct -4.6 pct Additional systematic error for PBPB 70-80 pct data: +5.9 pct -5.9 pct.

Additional systematic error for P-PB NSD data: +4.6 pct -4.6 pct.

$p_{\rm{T}}$-differential yield of $\Sigma^{*+}$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (NSD).

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

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

$p_{\rm{T}}$-differential yield of $\Sigma^{*+}$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (20-60% multiplicity class).

$p_{\rm{T}}$-differential yield of $\Sigma^{*+}$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (20-60% multiplicity class).

$p_{\rm{T}}$-differential yield of $\Sigma^{*+}$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (60-100% multiplicity class).

$p_{\rm{T}}$-differential yield of $\Sigma^{*+}$ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (60-100% multiplicity class).

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

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

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

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

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

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

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

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

$p_{\rm{T}}$-differential yield of ($\Xi^{*0}+\overline{\Xi}^{*0}$)/2 in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (60-100\% multiplicity class).

$p_{\rm{T}}$-differential yield of ($\Xi^{*0}+\overline{\Xi}^{*0}$)/2 in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV (60-100\% multiplicity class).

$p_{\rm T}$-integrated yield d$N$/d$y$ of ($\Sigma^{*\pm}+\overline{\Sigma}^{*\mp}$)/4 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.

$p_{\rm T}$-integrated yield d$N$/d$y$ of ($\Sigma^{*\pm}+\overline{\Sigma}^{*\mp}$)/4 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.

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

Mean $p_{\rm T}$ of $\Sigma^{*\pm}$ 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 ($\Xi^{*0}+\overline{\Xi}^{0})$)/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.

$p_{\rm T}$-integrated yield d$N$/d$y$ of ($\Xi^{*0}+\overline{\Xi}^{0})$)/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.

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

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

Integrated yield ratio.

Integrated yield ratio.

Integrated yield ratio.

Integrated yield ratio.

Integrated yield ratio.

Integrated yield ratio.

Integrated yield ratio.

Integrated yield ratio.

Charged-particle per-event yields measured in 5-10% PbPb centrality class.

Charged-particle per-event yields measured in 10-30% PbPb centrality class.

Charged-particle per-event yields measured in 10-30% PbPb centrality class.

Charged-particle per-event yields measured in 30-50% PbPb centrality class.

Charged-particle per-event yields measured in 30-50% PbPb centrality class.

Charged-particle per-event yields measured in 50-70% PbPb centrality class.

Charged-particle per-event yields measured in 50-70% PbPb centrality class.

Charged-particle per-event yields measured in 70-90% PbPb centrality class.

Charged-particle per-event yields measured in 70-90% PbPb centrality class.

Charged-particle per-event yields measured in pp collisions. A factor of 70 mb is used to scale the pp spectrum from a differential cross section to a per-event yield for direct comparison to the PbPb spectra. The lumi uncertainty is a 2.3% fully correlated uncertainty.

Charged-particle per-event yields measured in pp collisions. A factor of 70 mb is used to scale the pp spectrum from a differential cross section to a per-event yield for direct comparison to the PbPb spectra. The lumi uncertainty is a 2.3% fully correlated uncertainty.

PbPb nuclear modification factor measured in 0-5% PbPb centrality class.

PbPb nuclear modification factor measured in 0-5% PbPb centrality class.

PbPb nuclear modification factor measured in 5-10% PbPb centrality class.

PbPb nuclear modification factor measured in 5-10% PbPb centrality class.

PbPb nuclear modification factor measured in 10-30% PbPb centrality class.

PbPb nuclear modification factor measured in 10-30% PbPb centrality class.

PbPb nuclear modification factor measured in 30-50% PbPb centrality class.

PbPb nuclear modification factor measured in 30-50% PbPb centrality class.

PbPb nuclear modification factor measured in 50-70% PbPb centrality class.

PbPb nuclear modification factor measured in 50-70% PbPb centrality class.

PbPb nuclear modification factor measured in 70-90% PbPb centrality class.

PbPb nuclear modification factor measured in 70-90% PbPb centrality class.

PbPb nuclear modification factor measured in 0-10% PbPb centrality class.

PbPb nuclear modification factor measured in 0-10% PbPb centrality class.

PbPb nuclear modification factor measured in 0-100% PbPb centrality class.

PbPb nuclear modification factor measured in 0-100% PbPb centrality class.

pPb nuclear modification factor.

pPb nuclear modification factor.

$R_{pPb}$ as a function of $p_{T}$ integrated over rapidity range $-1.8<y*<1.3$ for the 0--90% centrality interval for the three geometric models: (a) Glauber, (b) Glauber-Gribov with $\omega_{\sigma}=0.11$ and (c) Glauber-Gribov with $\omega_{\sigma}=0.2$.

$R_{pPb}$ values as a function of $p_{T}$ in the 0--90% centrality interval averaged over $|y*|<0.5$.The $\langle T_{Pb} \rangle$ value for the ATLAS centrality correction is calculated with the Glauber model. The total systematic uncertainties, which include the uncertainty in $\langle T_{Pb} \rangle$, are indicated by lines of the same colour. Strict quantitative agreement is not expected as each measurement uses different rapidity intervals for the centrality determination and apply different event selection criteria to reject diffractive collisions.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields integrated over $-1.8<y*<1.3$ for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields integrated over $-1.8<y*<1.3$ for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields integrated over $-1.8<y*<1.3$ for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{CP}$ as a function of $p_{T}$ extracted from the invariant yields integrated over $|\eta|<2.3$ for seven centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{CP}$ as a function of $p_{T}$ extracted from the invariant yields integrated over $|\eta|<2.3$ for seven centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{CP}$ as a function of $p_{T}$ extracted from the invariant yields integrated over $|\eta|<2.3$ for seven centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $p_{T}$ extracted from the invariant yields for six rapidity ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$R_{pPb}$ as a function of $y*$ extracted from the invariant yields for eight $p_{T}$ ranges, for eight centrality intervals, and for different geometrical models used to calculate $\langle T_{Pb} \rangle$.

$p_{\rm T}$-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.

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 80 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 90 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 80 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 90 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 80 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 90 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 80 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 90 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and 80 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and 90 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and 80 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and 90 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and 80 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and 90 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and 80 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and 90 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and $N_{offline}^{trk}>$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and $N_{offline}^{trk}>$ 110 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and $N_{offline}^{trk}>$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and $N_{offline}^{trk}>$ 110 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and $N_{offline}^{trk}>$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and $N_{offline}^{trk}>$ 110 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and $N_{offline}^{trk}>$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and $N_{offline}^{trk}>$ 110 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 and integrated over the region $|\Delta\Phi| < \Delta\Phi_{ZYAM}$ for pp data at $\sqrt{s} =$ 13 $TeV$. The associated yield as a function of $p_{T}$ for events with $N^{offline}_{trk} \geq$ 105. The $p_{T}$ value for each $p_{T}$ bin is the average $p_{T}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 for pp data at $\sqrt{s} =$ 7 $TeV$. The associated yield as a function of $p_{T}$ for events with $N^{offline}_{trk} \geq$ 110. The $p_{T}$ value for each $p_{T}$ bin is the average $p_{T}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 and integrated over the region $|\Delta\Phi| < \Delta\Phi_{ZYAM}$ for pp data at $\sqrt{s} =$ 13 $TeV$. The associated yield as a function of $N_{trk}^{offline}$ for events with 1.0 $< p_{T} <$ 2.0 GeV/c. The $N_{trk}^{offline}$ value for each $N_{trk}^{offline}$ bin is the average $N_{trk}^{offline}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 for pp data at $\sqrt{s} =$ 7 $TeV$. The associated yield as a function of $N_{trk}^{offline}$ for events with 1.0 $< p_{T} <$ 2.0 GeV/c. The $N_{trk}^{offline}$ value for each $N_{trk}^{offline}$ bin is the average $N_{trk}^{offline}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 pPb data at $\sqrt{s} =$ 5.02 $TeV$. The associated yield as a function of $N_{trk}^{offline}$ for events with 1.0 $< p_{T} <$ 2.0 GeV/c. The $N_{trk}^{offline}$ value for each $N_{trk}^{offline}$ bin is the average $N_{trk}^{offline}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 PbPb data at $\sqrt{s} =$ 2.76 $TeV$. The associated yield as a function of $N_{trk}^{offline}$ for events with 1.0 $< p_{T} <$ 2.0 GeV/c. The $N_{trk}^{offline}$ value for each $N_{trk}^{offline}$ bin is the average $N_{trk}^{offline}$ value.