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.

Acceptance * reconstruction efficiency for the P P --> Zprime --> Zh --> llbb/cc signals in the 2-lepton channel.

Acceptance * reconstruction efficiency for the P P --> bbA --> Zh --> vvbb signals in the 0-lepton channel.

Acceptance * reconstruction efficiency for the P P --> bbA --> Zh --> vvbb signals in the 0-lepton channel.

Acceptance * reconstruction efficiency for the P P --> bbA --> Zh --> llbb signals in the 2-lepton channel.

Acceptance * reconstruction efficiency for the P P --> bbA --> Zh --> llbb signals in the 2-lepton channel.

Acceptance * reconstruction efficiency for the P P --> Wprime --> Zh --> lvbb/cc signals in the 0-lepton channel.

Acceptance * reconstruction efficiency for the P P --> Wprime --> Zh --> lvbb/cc signals in the 0-lepton channel.

Acceptance * reconstruction efficiency for the P P --> Wprime --> Zh --> lvbb/cc signals in the 1-lepton channel.

Acceptance * reconstruction efficiency for the P P --> Wprime --> Zh --> lvbb/cc signals in the 1-lepton channel.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the resolved 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the resolved 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the resolved 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the resolved 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the merged 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the merged 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the merged 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the merged 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the resolved 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the resolved 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the resolved 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the resolved 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the merged 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the merged 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the merged 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the merged 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 3+ b-tag signal region. The background prediction is shown after a background-only maximum-likelihood bbA fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 3+ b-tag signal region. The background prediction is shown after a background-only maximum-likelihood bbA fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the resolved 3+ b-tag signal region. The background prediction is shown after a background-only maximum-likelihood bbA fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the resolved 3+ b-tag signal region. The background prediction is shown after a background-only maximum-likelihood bbA fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag signal region with additional b-tagged track jets not associated with the large-R jet. The background prediction is shown after a background-only maximum-likelihood bbA fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag signal region with additional b-tagged track jets not associated with the large-R jet. The background prediction is shown after a background-only maximum-likelihood bbA fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the merged 1+2 b-tag signal region with additional b-tagged track jets not associated with the large-R jet. The background prediction is shown after a background-only maximum-likelihood bbA fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the merged 1+2 b-tag signal region with additional b-tagged track jets not associated with the large-R jet. The background prediction is shown after a background-only maximum-likelihood bbA fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the resolved 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the resolved 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the resolved 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the resolved 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the merged 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the merged 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the merged 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 1-lepton channel in the merged 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the resolved top control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{Vh}$ for the 2-lepton channel in the resolved top control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 1 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag sideband control region. The background prediction is shown after a background-only maximum-likelihood Z' fit to the data. In the plot, the last bin contains the overflow.

Upper limits on Zprime to Z h production cross section times branching fraction in pb.

Upper limits on Zprime to Z h production cross section times branching fraction in pb.

Upper limits on Wprime to W h production cross section times branching fraction in pb.

Upper limits on Wprime to W h production cross section times branching fraction in pb.

Upper limits on ggA to Z h production cross section times branching fraction in pb.

Upper limits on ggA to Z h production cross section times branching fraction in pb.

Upper limits on bbA to Z h production cross section times branching fraction in pb.

Upper limits on bbA to Z h production cross section times branching fraction in pb.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 220 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 220 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 260 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 260 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 300 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 300 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 340 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 340 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 380 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 380 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 400 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 400 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 420 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 420 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 440 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 440 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 460 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 460 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 500 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 500 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 600 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 600 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 700 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 700 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 800 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 800 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 900 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 900 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 1000 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 1000 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 1200 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 1200 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 1400 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 1400 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 1600 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 1600 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 2000 GeV.

Expected and observed two-dimensional likelihood scans of the b-associated production cross section times branching fraction vs the gluon-fusion production cross section times branching fraction at $m_{A}$ = 2000 GeV.

Acceptance * reconstruction efficiency for the P P --> A --> Zh --> vvbb signal in the 0-lepton channel.

Acceptance * reconstruction efficiency for the P P --> A --> Zh --> vvbb signal in the 0-lepton channel.

Acceptance * reconstruction efficiency for the P P --> A --> Zh --> llbb signal in the 2-lepton channel.

Acceptance * reconstruction efficiency for the P P --> A --> Zh --> llbb signal in the 2-lepton channel.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the resolved 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 1 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Event distributions of $m_{T,Vh}$ for the 0-lepton channel in the merged 2 b-tag signal region. The background prediction is shown after a background-only maximum-likelihood W' fit to the data. In the plot, the last bin contains the overflow.

Distributions of expected upper limits at 95% confidence level on the cross section of P P --> A --> Zh as a function of bbA fraction an signal mass.

Distributions of expected upper limits at 95% confidence level on the cross section of P P --> A --> Zh as a function of bbA fraction an signal mass.

Distributions of observed upper limits at 95% confidence level on the cross section of P P --> A --> Zh as a function of bbA fraction an signal mass.

Distributions of observed upper limits at 95% confidence level on the cross section of P P --> A --> Zh as a function of bbA fraction an signal mass.

K$^+$p (K$^+$p $\oplus$ K$^-\overline{\mathrm p}$) correlation function in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (40-100%).

K$^+$p (K$^+$p $\oplus$ K$^-\overline{\mathrm p}$) correlation function in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (60-70%).

K$^+$p (K$^+$p $\oplus$ K$^-\overline{\mathrm p}$) correlation function in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (70-80%).

K$^+$p (K$^+$p $\oplus$ K$^-\overline{\mathrm p}$) correlation function in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (80-90%).

K$^-$p (K$^-$p $\oplus$ K$^+\overline{\mathrm p}$) correlation function in pp collisions at $\sqrt{s}=13$ TeV.

K$^-$p (K$^-$p $\oplus$ K$^+\overline{\mathrm p}$) correlation function in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (0-20%).

K$^-$p (K$^-$p $\oplus$ K$^+\overline{\mathrm p}$) correlation function in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (20-40%).

K$^-$p (K$^-$p $\oplus$ K$^+\overline{\mathrm p}$) correlation function in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (40-100%).

K$^-$p (K$^-$p $\oplus$ K$^+\overline{\mathrm p}$) correlation function in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (60-70%).

K$^-$p (K$^-$p $\oplus$ K$^+\overline{\mathrm p}$) correlation function in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (70-80%).

K$^-$p (K$^-$p $\oplus$ K$^+\overline{\mathrm p}$) correlation function in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}} = 5.02$ TeV (80-90%).

Scaling factor ($\alpha_j $) for $\mathrm{\overline{K}^0 n}$ extracted from the different fits of the K$^-$ p correlation function as a function of the core radius $r_{\mathrm{core}}$.

Scaling factor ($\alpha_j $) for $\pi \Sigma$ extracted from the different fits of the K$^-$ p correlation function as a function of the core radius $r_{\mathrm{core}}$.

This table shows the correlation coefficient between the $\alpha_{\mathrm{\overline{K}^0 n}}$ and $\alpha_{\pi \Sigma}$ parameters extracted from the different fits to the K$^-$ p correlation function with free weights. The results are shown as a function of the core radius $r_{\mathrm{core}}$ shown in Table 7. The error on the correlation coefficient, shown as statistical errors in the table, are obteined by using the Pearson's formula to evaluate the probable error of correlation coefficient.

Differential excess $e^+e^-$ yield in 70--90\% Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV as a function of $m_{\rm ee}$ for $p_{\rm T,ee} < 0.1$ GeV/$c$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$.

Differential $e^+e^-$ yield in 70--90\% Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV as a function of $p_{\rm T,ee}$ for 0.4 $< m_{\rm ee} < 0.7$ GeV/$c^{\rm 2}$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$.

Differential $e^+e^-$ yield in 70--90\% Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV as a function of $p_{\rm T,ee}$ for 0.7 $< m_{\rm ee} < 1.1$ GeV/$c^{\rm 2}$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$. The quoted upper limits correspond to a 90% confidence level.

Differential $e^+e^-$ yield in 70--90\% Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV as a function of $p_{\rm T,ee}$ for 1.1 $< m_{\rm ee} < 2.7$ GeV/$c^{\rm 2}$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$. The quoted upper limits correspond to a 90% confidence level.

Differential excess $e^+e^-$ yield in 70--90\% Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV as a function of $p^{2}_{\rm T,ee}$ for 0.4 $< m_{\rm ee} < 0.7$ GeV/$c^{\rm 2}$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$. The quoted upper limits correspond to a 90% confidence level.

Differential excess $e^+e^-$ yield in 70--90\% Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV as a function of $p^{2}_{\rm T,ee}$ for 0.7 $< m_{\rm ee} < 1.1$ GeV/$c^{\rm 2}$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$. The quoted upper limits correspond to a 90% confidence level.

Differential excess $e^+e^-$ yield in 70--90\% Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV as a function of $p^{2}_{\rm T,ee}$ for 1.1 $< m_{\rm ee} < 2.7$ GeV/$c^{\rm 2}$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$.

Dependence of $\overline{p}$-$\overline{d}$ correlation on pseudorapidity acceptance of $\overline{p}$ and $\overline{d}$ selection in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}$ = 5.02 TeV. Results are for 20.0--30.0$\%$ collision centrality.

Dependence of $\overline{p}$-$\overline{d}$ correlation on pseudorapidity acceptance of $\overline{p}$ and $\overline{d}$ selection in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}$ = 5.02 TeV. Results are for 50.0--60.0$\%$ collision centrality.

Fig. 6b: Number density $N_{\rm ch}$ (left) and $\Sigma p_{\rm T}$ (right) distributions as a function of $p_{\rm T}^{\rm trig}$ in Away and Toward regions after the subtraction of Number density $N_{\rm ch}$ and $\Sigma p_{\rm T}$ distributions in the transverse region for p-Pb collisions for $p_{\rm T} >$ 0.5 GeV/$c$. The shaded areas and the error bars around the data points represent the systematic and statistical uncertainties, respectively.

Fig. 7a: $<p_{\rm T}>$ as a function of $p_{\rm T}^{\rm trig}$ in Toward (left) and Away (right) regions after the subtraction of transverse region for pp collisions for $p_{\rm T} >$ 0.5 GeV/$c$. The shaded areas and the error bars around the data points represent the systematic and statistical uncertainties, respectively.

Fig. 7b: $<p_{\rm T}>$ as a function of $p_{\rm T}^{\rm trig}$ in Toward (left) and Away (right) regions after the subtraction of transverse region for p-Pb collisions for $p_{\rm T} >$ 0.5 GeV/$c$. The shaded areas and the error bars around the data points represent the systematic and statistical uncertainties, respectively.

Fig. A1: Number density $N_{\rm ch}$ (left) and $\Sigma p_{\rm T}$ (right) distributions as a function of $p_{\rm T}^{\rm trig}$ in Transverse, Away, and Toward regions for $p_{\rm T} >$ 0.15 GeV/$c$. The shaded areas and the error bars around the data points represent the systematic and statistical uncertainties, respectively.

Fig. A2: Number density $N_{\rm ch}$ (left) and $\Sigma p_{\rm T}$ (right) distributions as a function of $p_{\rm T}^{\rm trig}$ in Transverse, Away, and Toward regions for $p_{\rm T} >$ 1.0 GeV/$c$. The shaded areas and the error bars around the data points represent the systematic and statistical uncertainties, respectively.

Fig. A3: Number density $N_{\rm ch}$ (left) and $\Sigma p_{\rm T}$ (right) distributions as a function of $p_{\rm T}^{\rm trig}$ in Transverse, Away, and Toward regions for $p_{\rm T} >$ 0.15 GeV/$c$. The shaded areas and the error bars around the data points represent the systematic and statistical uncertainties, respectively.

Fig. A4: Number density $N_{\rm ch}$ (left) and $\Sigma p_{\rm T}$ (right) distributions as a function of $p_{\rm T}^{\rm trig}$ in Transverse, Away, and Toward regions for $p_{\rm T} >$ 1.0 GeV/$c$. The shaded areas and the error bars around the data points represent the systematic and statistical uncertainties, respectively.

$p_{\mathrm T}$-differential yield of $\frac{\mathrm{K^{*0}} + \overline{\mathrm{K^{*0}}}}{2}$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV ($-0.9 < y < -0.6$).

$p_{\mathrm T}$-differential yield of $\frac{\mathrm{K^{*0}} + \overline{\mathrm{K^{*0}}}}{2}$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV ($-1.2 < y < -0.9$).

$p_{\mathrm T}$-differential yield of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV ($0.0 < y < 0.3$).

$p_{\mathrm T}$-differential yield of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV ($-0.3 < y < 0.0$).

$p_{\mathrm T}$-differential yield of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV ($-0.6 < y < -0.3$).

$p_{\mathrm T}$-differential yield of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV ($-0.9 < y < -0.6$).

$p_{\mathrm T}$-differential yield of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV ($-1.2 < y < -0.9$).

d$N$/d$y$ of $\frac{\mathrm{K^{*0}} + \overline{\mathrm{K^{*0}}}}{2}$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (V0A multiplicity classes).

d$N$/d$y$ of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (V0A multiplicity classes).

$\langle p_\mathrm{T}\rangle$ of $\frac{\mathrm{K^{*0}} + \overline{\mathrm{K^{*0}}}}{2}$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (V0A multiplicity classes).

$\langle p_\mathrm{T}\rangle$ of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (V0A multiplicity classes).

(d$N$/$\mathrm{d}y$)/(d$N$/$\mathrm{d}y)_{y=0}$ of $\frac{\mathrm{K^{*0}} + \overline{\mathrm{K^{*0}}}}{2}$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (0-100 %).

(d$N$/$\mathrm{d}y$)/(d$N$/$\mathrm{d}y)_{y=0}$ of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (0-100 %).

$\langle p_\mathrm{T}\rangle_\mathrm{y}$/$\langle p_\mathrm{T}\rangle_\mathrm{y=0}$ of $\frac{\mathrm{K^{*0}} + \overline{\mathrm{K^{*0}}}}{2}$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (0-100 %).

$\langle p_\mathrm{T}\rangle_\mathrm{y}$/$\langle p_\mathrm{T}\rangle_\mathrm{y=0}$ of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (0-100%).

$y_{asym}$ of $\frac{\mathrm{K^{*0}} + \overline{\mathrm{K^{*0}}}}{2}$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (V0A multiplicity classes).

$y_{asym}$ of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (V0A multiplicity classes).

$Q_{CP}$ of $\frac{\mathrm{K^{*0}} + \overline{\mathrm{K^{*0}}}}{2}$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (0-10 %/40-100 %).

$Q_{CP}$ of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (0-10 %/40-100%).

$Q_{CP}$ of $\frac{\mathrm{K^{*0}} + \overline{\mathrm{K^{*0}}}}{2}$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (10-40 %/40-100 %).

$Q_{CP}$ of $\phi$ in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}}~=~$5.02 TeV (10-40 %/40-100%).

Direct photon spectra for minimum bias (0-86%) Au+Au collision at $\sqrt{s_{NN}} = 62.4$ GeV (a) and $39$ GeV (b). For $62.4$ GeV also centrality bins of 0-20% (c) and 20-40% (d) are shown. Data points are shown with statistical and systematic uncertainties, unless the central value is negative (arrows) or is consistent with zero within the statistical uncertainties (arrows with data point). In these cases upper limit with CL = 95$%$ are given.

Inverse slopes, $T_{eff}$ , obtained from fitting the combined data from central collisions shown in Fig. 11 is compared to the fit results of the individual data sets at $\sqrt{s_{NN}} = 62.4$ GeV, $200$ GeV, and $2760$ GeV. Also included is the value for $\sqrt{s_{NN}} = 39$ GeV obtained from fitting the min. bias data set in the lower $p_T$ range.

Integrated invariant direct-photon yields vs. charged particle multiplicity for $p_{T}$ integrated from (a) 0.4 GeV/c, (b) 1.0 GeV/c, (c) 1.5 GeV/c, and (d) 2.0 to 5.0 GeV/c for all available A+A datasets.

Integrated invariant direct-photon yields vs. charged particle multiplicity for $p_{T}$ integrated from (a) 0.4 GeV/c, (b) 1.0 GeV/c, (c) 1.5 GeV/c, and (d) 2.0 to 5.0 GeV/c for all available A+A datasets.

Integrated invariant direct-photon yields vs. charged particle multiplicity for $p_{T}$ integrated from (a) 0.4 GeV/c, (b) 1.0 GeV/c, (c) 1.5 GeV/c, and (d) 2.0 to 5.0 GeV/c for all available A+A datasets.

Integrated invariant direct-photon yields vs. charged particle multiplicity for $p_{T}$ integrated from (a) 0.4 GeV/c, (b) 1.0 GeV/c, (c) 1.5 GeV/c, and (d) 2.0 to 5.0 GeV/c for all available A+A datasets.

Integrated direct-photon yields from A+A collisions for $p_{T,min}$ of $5$ GeV/c (a) and $8$ GeV/c. The representation is the same as in Fig. 13. Also shown are the results from pQCD calculations scaled by $N_{coll}$

Integrated direct-photon yields from A+A collisions for $p_{T,min}$ of $5$ GeV/c (a) and $8$ GeV/c. The representation is the same as in Fig. 13. Also shown are the results from pQCD calculations scaled by $N_{coll}$

The $\alpha$ values extracted using fits to integrated direct photon yields. The dashed line gives the average $\alpha$ value for the 4 lower $p_{T,min}$ points. Also shown is a model calculation for $\alpha$ discussed in the text.

Raw primary antihelium3-to-helium3 ratio from Geant4-based MC simulations as a function of the momentum p_primary with sigma_inel(3Hebar)x1.5.

Raw primary antihelium3-to-helium3 ratio as a function of the momentum p_primary.

Raw primary antihelium3-to-helium3 ratio from Geant4-based MC simulations as a function of the momentum p_primary with default sigma_inel(3Hebar).

Raw primary antihelium3-to-helium3 ratio from Geant4-based MC simulations as a function of the momentum p_primary with sigma_inel(3Hebar)x0.5.

Raw primary antihelium3-to-helium3 ratio from Geant4-based MC simulations as a function of the momentum p_primary with sigma_inel(3Hebar)x1.5.

Inelastic interaction cross section of antihelium-3 on an averaged material element of the ALICE detector (ITS+TPC analysis).

Inelastic interaction cross section of antihelium-3 on an averaged material element of the ALICE detector (ITS+TPC+TOF analysis).

Inelastic interaction cross section of antihelium-3 on an averaged material element of the ALICE detector (ITS+TPC+TOF analysis).

Antihelium-3 cosmic-ray flux from background before the solar modulation

Antihelium-3 cosmic-ray flux from dark matter before the solar modulation

Transparency of the galaxy to antihelium-3 nuclei from background before the solar modulation

Transparency of the galaxy to antihelium-3 nuclei from dark matter before the solar modulation

Antihelium-3 cosmic-ray flux from background after the solar modulation

Antihelium-3 cosmic-ray flux from dark matter after the solar modulation

Transparency of the galaxy to antihelium-3 nuclei from background after the solar modulation

Transparency of the galaxy to antihelium-3 nuclei from dark matter after the solar modulation

Inelastic interaction cross section of antihelium-3 on proton from the fit to the ALICE data.

Inelastic interaction cross section of antihelium-3 on helium-4 from the fit to the ALICE data.

(Anti)proton spectrum in V0M multiplicity class IV - V

(Anti)proton spectrum in V0M multiplicity class VI

(Anti)proton spectrum in V0M multiplicity class VII

(Anti)proton spectrum in V0M multiplicity class VIII

(Anti)proton spectrum in V0M multiplicity class IX

(Anti)proton spectrum in V0M multiplicity class X

(Anti)proton spectrum in V0M multiplicity class INEL > 0

(Anti)deuteron spectrum in V0M multiplicity class I

(Anti)deuteron spectrum in V0M multiplicity class II

(Anti)deuteron spectrum in V0M multiplicity class III

(Anti)deuteron spectrum in V0M multiplicity class IV - V

(Anti)deuteron spectrum in V0M multiplicity class VI

(Anti)deuteron spectrum in V0M multiplicity class VII

(Anti)deuteron spectrum in V0M multiplicity class VIII

(Anti)deuteron spectrum in V0M multiplicity class IX

(Anti)deuteron spectrum in V0M multiplicity class X

(Anti)deuteron spectrum in V0M multiplicity class INEL > 0

(Anti)helion spectrum in V0M multiplicity class I - III

(Anti)helion spectrum in V0M multiplicity class IV - X

(Anti)helion spectrum in V0M multiplicity class INEL > 0

Mean transverse momentum $<p_\mathrm{T}>$ of protons as a function of the charged particle multiplicity density at mid-rapidity

Mean transverse momentum $<p_\mathrm{T}>$ of deuterons as a function of the charged particle multiplicity density at mid-rapidity

Mean transverse momentum $<p_\mathrm{T}>$ of helions as a function of the charged particle multiplicity density at mid-rapidity

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class I

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class II

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class III

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class IV - V

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class VI

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class VII

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class VIII

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class IX

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class X

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class INEL > 0

Coalescence parameter $B_3$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class I - III

Coalescence parameter $B_3$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class IV - X

Coalescence parameter $B_3$ as a function of $p_{\mathrm{T}}$ in V0M multiplicity class INEL > 0

Coalescence parameter $B_2$ as a function of the charged particle multiplicity density at mid-rapidity

Coalescence parameter $B_3$ as a function of the charged particle multiplicity density at mid-rapidity

Deuteron over proton ratio as a function of the charged particle multiplicity density at mid-rapidity

Helion over proton ratio as a function of the charged particle multiplicity density at mid-rapidity

$p_\mathrm{T}$-differential production yield of prompt $\mathrm{D_s^+}$ mesons in the 30-50% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$ in the rapidity interval $|y|<0.5$. Branching ratio of $\mathrm{D_s^+\to \phi\pi^+\to K^-K^+\pi^+}$: 0.0224

$p_\mathrm{T}$-differential nuclear modification factor $R_\mathrm{AA}$ of prompt $\mathrm{D_s^+}$ mesons in the 0-10% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$ in the rapidity interval $|y|<0.5$.

$p_\mathrm{T}$-differential nuclear modification factor $R_\mathrm{AA}$ of prompt $\mathrm{D_s^+}$ mesons in the 0-10% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$ in the rapidity interval $|y|<0.5$.

$p_\mathrm{T}$-differential nuclear modification factor $R_\mathrm{AA}$ of prompt $\mathrm{D_s^+}$ mesons in the 30-50% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$ in the rapidity interval $|y|<0.5$.

$p_\mathrm{T}$-differential nuclear modification factor $R_\mathrm{AA}$ of prompt $\mathrm{D_s^+}$ mesons in the 30-50% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$ in the rapidity interval $|y|<0.5$.

$p_\mathrm{{T}}$-differential production ratios of prompt $\mathrm{D}_s^+/\mathrm{D}^0$ mesons in the 0-10% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$ in the rapidity interval $|y|<0.5$. Branching ratio of $\mathrm{D_s^+\to \phi\pi^+\to K^-K^+\pi^+}$: 0.0224 Branching ratio of $\mathrm{D^0 \to K^-\pi^+}$: 0.0395

$p_\mathrm{{T}}$-differential production ratios of prompt $\mathrm{D}_s^+/\mathrm{D}^0$ mesons in the 0-10% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$ in the rapidity interval $|y|<0.5$. Branching ratio of $\mathrm{D_s^+\to \phi\pi^+\to K^-K^+\pi^+}$: 0.0224 Branching ratio of $\mathrm{D^0 \to K^-\pi^+}$: 0.0395

$p_\mathrm{{T}}$-differential production ratios of prompt $\mathrm{D}_s^+/\mathrm{D}^0$ mesons in the 30-50% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$ in the rapidity interval $|y|<0.5$. Branching ratio of $\mathrm{D_s^+\to \phi\pi^+\to K^-K^+\pi^+}$: 0.0224 Branching ratio of $\mathrm{D^0 \to K^-\pi^+}$: 0.0395

$p_\mathrm{{T}}$-differential production ratios of prompt $\mathrm{D}_s^+/\mathrm{D}^0$ mesons in the 30-50% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$ in the rapidity interval $|y|<0.5$. Branching ratio of $\mathrm{D_s^+\to \phi\pi^+\to K^-K^+\pi^+}$: 0.0224 Branching ratio of $\mathrm{D^0 \to K^-\pi^+}$: 0.0395

$p_\mathrm{{T}}$-differential prompt $\mathrm{D}_s^+/\mathrm{D}^0$ ratios in Pb-Pb collisions in the 0-10% centrality class at $\sqrt{s_\mathrm{NN}}=5.02~\mathrm{TeV}$ divided by those in pp collisions at the same energy.

$p_\mathrm{{T}}$-differential prompt $\mathrm{D}_s^+/\mathrm{D}^0$ ratios in Pb-Pb collisions in the 0-10% centrality class at $\sqrt{s_\mathrm{NN}}=5.02~\mathrm{TeV}$ divided by those in pp collisions at the same energy.

$p_\mathrm{{T}}$-differential prompt $\mathrm{D}_s^+/\mathrm{D}^0$ ratios in Pb-Pb collisions in the 30-50% centrality class at $\sqrt{s_\mathrm{NN}}=5.02~\mathrm{TeV}$ divided by those in pp collisions at the same energy.

$p_\mathrm{{T}}$-differential prompt $\mathrm{D}_s^+/\mathrm{D}^0$ ratios in Pb-Pb collisions in the 30-50% centrality class at $\sqrt{s_\mathrm{NN}}=5.02~\mathrm{TeV}$ divided by those in pp collisions at the same energy.

$p_\mathrm{T}$-differential elliptic flow coefficient $v_2$ of prompt $\mathrm{D_s^+}$ mesons in the 30-50% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$.

$p_\mathrm{T}$-differential elliptic flow coefficient $v_2$ of prompt $\mathrm{D_s^+}$ mesons in the 30-50% centrality class in Pb-Pb collisions at $\sqrt{{s_\mathrm{NN}}}=5.02~\mathrm{{TeV}}$.

Comparison of the azimuthal-correlation distributions of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) with $3 < p_{\rm T} < 5$ GeV/$c$ and charged particles with $1 < p_{\rm T} < 2$ GeV/$c$, in pp collisions at $\sqrt{s} =$ 5 TeV and 13 TeV, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) with $8 < p_{\rm T} < 16$ GeV/$c$ and charged particles with $1 < p_{\rm T} < 2$ GeV/$c$, in pp collisions at $\sqrt{s} =$ 5 TeV and 13 TeV, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) with $16 < p_{\rm T} < 24$ GeV/$c$ and charged particles with $1 < p_{\rm T} < 2$ GeV/$c$, in pp collisions at $\sqrt{s} =$ 5 TeV and 13 TeV, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the near-side associated peak yields measured in pp collisions at $\sqrt{s} = $5, 7, and 13 TeV, for correlations of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak yields measured in pp collisions at $\sqrt{s}=$ 5 TeV and 13 TeV, for correlations of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak width measured in pp collisions at $\sqrt{s} = $5, 7, and 13 TeV, for correlations of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak width measured in pp collisions at $\sqrt{s}=$ 5 TeV and 13 TeV, for correlations of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the away-side associated peak yields measured in pp collisions at $\sqrt{s}=$ 5 TeV and 13 TeV, for correlations of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the away-side associated peak yields measured in pp collisions at $\sqrt{s}=$ 5 TeV and 13 TeV, for correlations of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the away-side associated peak width measured in pp collisions at $\sqrt{s}=$ 5 TeV and 13 TeV, for correlations of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the away-side associated peak width measured in pp collisions at $\sqrt{s}=$ 5 TeV and 13 TeV, for correlations of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the azimuthal-correlation distributions of of D$^{0}$ mesons with $3 < p_{\rm T} < 5$ GeV/$c$ and charged particles with $p_{\rm T} > 0.3$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $5 < p_{\rm T} < 8$ GeV/$c$ and charged particles with $p_{\rm T} > 0.3$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $8 < p_{\rm T} < 16$ GeV/$c$ and charged particles with $p_{\rm T} > 0.3$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $16 < p_{\rm T} < 24$ GeV/$c$ and charged particles with $p_{\rm T} > 0.3$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $3 < p_{\rm T} < 5$ GeV/$c$ and charged particles with $0.3 < p_{\rm T} < 1$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $5 < p_{\rm T} < 8$ GeV/$c$ and charged particles with $0.3 < p_{\rm T} < 1$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $8 < p_{\rm T} < 16$ GeV/$c$ and charged particles with $0.3 < p_{\rm T} < 1$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $16 < p_{\rm T} < 24$ GeV/$c$ and charged particles with $0.3 < p_{\rm T} < 1$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $3 < p_{\rm T} < 5$ GeV/$c$ and charged particles with $1 < p_{\rm T} < 2$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $5 < p_{\rm T} < 8$ GeV/$c$ and charged particles with $1 < p_{\rm T} < 2$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $8 < p_{\rm T} < 16$ GeV/$c$ and charged particles with $1 < p_{\rm T} < 2$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $16 < p_{\rm T} < 24$ GeV/$c$ and charged particles with $1 < p_{\rm T} < 2$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $3 < p_{\rm T} < 5$ GeV/$c$ and charged particles with $2 < p_{\rm T} < 3$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $5 < p_{\rm T} < 8$ GeV/$c$ and charged particles with $2 < p_{\rm T} < 3$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $8 < p_{\rm T} < 16$ GeV/$c$ and charged particles with $2 < p_{\rm T} < 3$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the azimuthal-correlation distributions of D$^{0}$ mesons with $16 < p_{\rm T} < 24$ GeV/$c$ and charged particles with $2 < p_{\rm T} < 3$ GeV/$c$, in pp collisions at $\sqrt{s} = $13 TeV in four different V0 multiplicity classes, after baseline subtraction. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$. The azimuthal-correlation distributions are reported in the range $0 < \Delta\varphi < \pi$.

Comparison of the near-side associated peak yields among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $p_{\rm T} > 0.3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak yields among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak yields among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak yields among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $2 < p_{\rm T} < 3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak width among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $ p_{\rm T} > 0.3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak width among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak width among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the near-side associated peak width among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $2 < p_{\rm T} < 3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the away-side associated peak yields among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $ p_{\rm T} > 0.3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Comparison of the away-side associated peak width among four different V0 multiplicity classes measured in pp collisions at $\sqrt{s} = $13 TeV, for correlations of D$^{0}$ mesons and charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $ p_{\rm T} > 0.3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Near-side associated peak yield of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $ p_{\rm T} > 0.3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Near-side associated peak yield of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Near-side associated peak yield of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Near-side associated peak yield of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $2 < p_{\rm T} < 3$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Near-side associated peak width of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $ p_{\rm T} > 0.3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Near-side associated peak width of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Near-side associated peak width of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Near-side associated peak width of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $2 < p_{\rm T} < 3$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Away-side associated peak yield of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $ p_{\rm T} > 0.3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Away-side associated peak yield of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Away-side associated peak yield of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Away-side associated peak yield of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $2 < p_{\rm T} < 3$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Away-side associated peak width of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $ p_{\rm T} > 0.3 $ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Away-side associated peak width of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $0.3 < p_{\rm T} < 1$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Away-side associated peak width of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $1 < p_{\rm T} < 2$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Away-side associated peak width of D mesons (average of D$^{0}$, D$^{+}$, and D$^{*+}$) correlated with charged particles, as a function of the D-meson $p_{\rm T}$, for associated particle $2 < p_{\rm T} < 3$ GeV/$c$. Rapidity range for the D mesons is $|y^{\rm D}_{\rm cms}| < 0.5$. Correlations are integrated for $|\Delta\eta|=|\eta_{\rm ch}-\eta_{\rm D}| < 1$.

Transverse momentum distributions d$N$/(d$y$d$p_{\mathrm{T}}$) of prompt D$^{+}$ (middle) meson in the 30-50% (diamonds) centrality classes in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV in |y|<0.5. The uncertainties on the BRs are quoted separately and the horizontal bars represent bin widths. The points in the figure of the paper are scaled for visibility by a factor 10$^{-1}$. Branching ratio of D$^+$ --> K$\pi\pi$ = 0.0938

Transverse momentum distributions d$N$/(d$y$d$p_{\mathrm{T}}$) of prompt D*$^{+}$ (right) meson in the 0-10% (crosses) centrality classes in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV in |y|<0.5. The uncertainties on the BRs are quoted separately and the horizontal bars represent bin widths. Branching ratio of D*$^+$ --> D$^0\pi$ = 0.677

Transverse momentum distributions d$N$/(d$y$d$p_{\mathrm{T}}$) of prompt D*$^{+}$ (right) meson in the 30-50% (diamonds) centrality classes in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV in |y|<0.5. The uncertainties on the BRs are quoted separately and the horizontal bars represent bin widths. The points in the figure of the paper are scaled for visibility by a factor 10$^{-1}$. Branching ratio of D*$^+$ --> D$^0\pi$ = 0.677

Ratio D$^{+}$/D$^{0}$ in central Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in |y|<0.5 and as a function of $p_\mathrm{T}$. Statistical (bars) and systematic (boxes) uncertainties are shown. Branching ratio of D$^0$ --> K$\pi$ = 0.0395 Branching ratio of D$^+$ --> K$\pi\pi$ = 0.0938

Ratio D$^{+}$/D$^{0}$ in semicentral Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in |y|<0.5 and as a function of $p_\mathrm{T}$. Statistical (bars) and systematic (boxes) uncertainties are shown. Branching ratio of D$^0$ --> K$\pi$ = 0.0395 Branching ratio of D$^+$ --> K$\pi\pi$ = 0.0938

Ratio D*$^{+}$/D$^{0}$ in central Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in |y|<0.5 and as a function of $p_\mathrm{T}$. Statistical (bars) and systematic (boxes) uncertainties are shown. Branching ratio of D$^0$ --> K$\pi$ = 0.0395 Branching ratio of D*$^+$ --> D$^0\pi$ = 0.677

Ratio D*$^{+}$/D$^{0}$ in semicentral Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in |y|<0.5 and as a function of $p_\mathrm{T}$. Statistical (bars) and systematic (boxes) uncertainties are shown. Branching ratio of D$^0$ --> K$\pi$ = 0.0395 Branching ratio of D*$^+$ --> D$^0\pi$ = 0.677

Nuclear modification factor of D$^{0}$ meson in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in the 0-10% centrality class, in |y|<0.5 and as a function of $p_\mathrm{T}$.

Nuclear modification factor of D$^{+}$ meson in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in the 0-10% centrality class, in |y|<0.5 and as a function of $p_\mathrm{T}$.

Nuclear modification factor of D*$^{+}$ meson in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in the 0-10% centrality class, in |y|<0.5 and as a function of $p_\mathrm{T}$.

Nuclear modification factor of D$^{0}$ meson in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in the 30-50% centrality class, in |y|<0.5 and as a function of $p_\mathrm{T}$.

Nuclear modification factor of D$^{+}$ meson in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in the 30-50% centrality class, in |y|<0.5 and as a function of $p_\mathrm{T}$.

Nuclear modification factor of D*$^{+}$ meson in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in the 30-50% centrality class, in |y|<0.5 and as a function of $p_\mathrm{T}$.

Average nuclear modification factor of D$^{0}$, D$^{+}$ and D*$^{+}$ meson in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in the 0-10% centrality class, in |y|<0.5 and as a function of $p_\mathrm{T}$.

Average nuclear modification factor of D$^{0}$, D$^{+}$ and D*$^{+}$ meson in Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in the 30-50% centrality class, in |y|<0.5 and as a function of $p_\mathrm{T}$.

$p_\mathrm{T}$-integrated nuclear modification factor of D$^{0}$ meson in central (0-10%) and semicentral (30-50%) Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV, in |y|<0.5.

Fig. 11 right: The $p_\mathrm{T}$ differential production cross section of charged-particle anti-$k_{T}$ $R=0.4$ b jets in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}~=~5.02$ TeV using the IP method.

Fig. 12 left: The combined differential production cross section of charged-particle anti-$k_{T}$ $R=0.4$ b jets in pp collisions at $\sqrt{s}~=~5.02$ TeV.

Fig. 12 right: The combined differential production cross section of charged-particle anti-$k_{T}$ $R=0.4$ b jets in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}~=~5.02$ TeV.

Fig. 13 left: The b-jet fraction in pp collisions at $\sqrt{s}~=~5.02$ TeV.

Fig. 13 right: The b-jet fraction in p-Pb collisions at $\sqrt{s_{\mathrm{NN}}~=~5.02$ TeV.

Fig. 14 left: The nuclear modification factor $R_{\mathrm{pPb}}$ of b jets as a function of $P_T$ from the SV method.

Fig. 14 left: The nuclear modification factor $R_{\mathrm{pPb}}$ of b jets as a function of $P_T$ from the IP method.

Fig. 14 right: The combined nuclear modification factor $R_{\mathrm{pPb}}$ of b jets as a function of $P_T$.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Non-prompt J/$\psi$ cross section as a function of transverse momentum in pp at 5.02 TeV

Prompt J/$\psi$ cross section as a function of transverse momentum in pp at 13 TeV

Prompt J/$\psi$ cross section as a function of transverse momentum in pp at 5.02 TeV

Prompt J/$\psi$ cross section as a function of rapidity in pp at 13 TeV

$p_{\rm T}$-differential yields of $\Lambda$(1520) (sum of particle and anti-particle states) in p--Pb collisions at $\sqrt{s_{\mathrm{NN}}}$ $\mathrm{=}$ 5.02 TeV in multiplicity interval 20--40\%. The uncertainty 'sys,$p_{\rm T}$-correlated' indicates the systematic uncertainty after removing the contributions of $p_{\rm T}$-uncorrelated uncertainty.

$p_{\rm T}$-differential yields of $\Lambda$(1520) (sum of particle and anti-particle states) in p--Pb collisions at $\sqrt{s_{\mathrm{NN}}}$ $\mathrm{=}$ 5.02 TeV in multiplicity interval 40--60\%. The uncertainty 'sys,$p_{\rm T}$-correlated' indicates the systematic uncertainty after removing the contributions of $p_{\rm T}$-uncorrelated uncertainty.

$p_{\rm T}$-differential yields of $\Lambda$(1520) (sum of particle and anti-particle states) in p--Pb collisions at $\sqrt{s_{\mathrm{NN}}}$ $\mathrm{=}$ 5.02 TeV in multiplicity interval 60--100\%. The uncertainty 'sys,$p_{\rm T}$-correlated' indicates the systematic uncertainty after removing the contributions of $p_{\rm T}$-uncorrelated uncertainty.

Ratio of $p_{\rm T}$-integrated yields of $\Lambda$(1520) (sum of particle and anti-particle states) to charged $\pi$ ($\pi^{+} + \pi^{-}$) at midrapidity as a function of $\langle {\rm d}N_{\rm ch}/{\rm d} \eta_{\rm lab} \rangle$ in inelastic pp collisions at $\sqrt{s}$ $\mathrm{=}$ 7 TeV.

Ratio of $p_{\rm T}$-integrated yields of $\Lambda$(1520) (sum of particle and anti-particle states) to charged $\pi$ ($\pi^{+} + \pi^{-}$) as a function of $\langle {\rm d}N_{\rm ch}/{\rm d} \eta_{\rm lab} \rangle$ in p--Pb collisions at $\sqrt{s}$ $\mathrm{=}$ 5.02 TeV. The uncertainty 'sys,uncorrelated' indicates the multiplicity uncorrelated systematic uncertainty.

Ratio of $p_{\rm T}$-integrated yields of $\Lambda$(1520) (sum of particle and anti-particle states) to K$^{-}$ at midrapidity as a function of $\langle {\rm d}N_{\rm ch}/{\rm d} \eta_{\rm lab} \rangle$ in inelastic pp collisions at $\sqrt{s}$ $\mathrm{=}$ 7 TeV.

Ratio of $p_{\rm T}$-integrated yields of $\Lambda$(1520) (sum of particle and anti-particle states) to K$^{-}$ as a function of $\langle {\rm d}N_{\rm ch}/{\rm d} \eta_{\rm lab} \rangle$ in p--Pb collisions at $\sqrt{s}$ $\mathrm{=}$ 5.02 TeV. The uncertainty 'sys,uncorrelated' indicates the multiplicity uncorrelated systematic uncertainty.

Ratio of $p_{\rm T}$-integrated yields of $\Lambda$(1520) (sum of particle and anti-particle states) to its ground state particle $\Lambda$ ($\Lambda + \bar{\Lambda}$) at midrapidity as a function of $\langle {\rm d}N_{\rm ch}/{\rm d} \eta_{\rm lab} \rangle$ in inelastic pp collisions at $\sqrt{s}$ $\mathrm{=}$ 7 TeV.

Ratio of $p_{\rm T}$-integrated yields of $\Lambda$(1520) (sum of particle and anti-particle states) to its ground state particle $\Lambda$ ($\Lambda + \bar{\Lambda}$) as a function of $\langle {\rm d}N_{\rm ch}/{\rm d} \eta_{\rm lab} \rangle$ in p--Pb collisions at $\sqrt{s}$ $\mathrm{=}$ 5.02 TeV. The uncertainty 'sys,uncorrelated' indicates the multiplicity uncorrelated systematic uncertainty.

Direct photon spectra(Nucl. Part. Phys. 23, A1 (1997)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in p+p at $\sqrt{s_{NN}}$= 63 GeV.

Direct photon spectra(Sov. J. Nucl. Phys. 51, 836 (1990)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in p+p at $\sqrt{s_{NN}}$= 63 GeV.

Direct photon spectra normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 62.4 GeV.

Direct photon spectra normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 39.0 GeV.

Direct photon spectra(Physical Review C91, 064904 (2015)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physical Review Letters 104, 132301 (2010)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physical Review Letters 109, 152302 (2012)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physical Review C98, 054902 (2018)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Cu+Cu at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physics Letters B754 235 (2016)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Pb+Pb at $\sqrt{s_{NN}}$= 2760 GeV.

Number of binary collisions N_{coll} vs. Charged particle multiplicity in Au+Au at various cm energies.

Charged particle multiplicity vs. centrality in Au+Au at various cm energies.

Number of binary collisions N_{coll} vs. centrality in Au+Au at various cm energies.

Integrated direct photon yield vs. Charged particle multiplicity in various systems at various cm energies.

Charged particle multiplicity vs. centrality in various systems at various cm energies.

Integrated direct photon yield vs. centrality in various systems at various cm energies.

Integrated direct photon yield vs. Charged particle multiplicity in various systems at various cm energies.

Charged particle multiplicity vs. centrality in various systems at various cm energies.

Integrated direct photon yield vs. centrality in various systems at various cm energies.

Global variables for Pb+Pb collisions at the LHC from ALICE.

$p^{pp}_T$ dependence of $S_{loss}$ for $\pi^0$ in 200 GeV Au+Au collisions from 2007 data from the PHENIX experiment at RHIC.

$p^{pp}_T$ dependence of $S_{loss}$ for $\pi^0$ in 200 GeV Au+Au collisions from 2004 data from the PHENIX experiment at RHIC for $p_T$ <10 GeV/$c$.

$p^{pp}_T$ dependence of $S_{loss}$ for $\pi^0$ in 200 GeV Cu+Cu collisions using the spectra measured by PHENIX at RHIC in 2005.

$p^{pp}_T$ dependence of $S_{loss}$ for $\pi^0$ in 62 GeV Au+Au collisions using the spectra measured by PHENIX in 2010.

$p^{pp}_T$ dependence of $S_{loss}$ for $\pi^0$ in 62.4 GeV Cu+Cu collisions using the spectra measured by PHENIX in 2005.

$p^{pp}_T$ dependence of $S_{loss}$ for $\pi^0$ in 2.76 TeV Pb+Pb collisions using the result from the ALICE experiment.

Parameters from fitting the indicated power-law functions for $\delta p_T/p_T$ to the data as a function of $p^{pp}_T$ for Au+Au collisions from 2004 data at $\sqrt{s_{NN}}$ = 200 GeV.

Parameters from fitting the indicated power-law functions for $\delta p_T/p_T$ to the data as a function of $p^{pp}_T$ for Au+Au collisions from 2007 data at $\sqrt{s_{NN}}$ = 200 GeV.

Parameters from fitting the indicated power-law functions for $\delta p_T/p_T$ to the data as a function of $p^{pp}_T$ for Cu+Cu collisions from 2005 data at $\sqrt{s_{NN}}$ = 200 GeV.

Parameters from fitting the indicated power-law functions for $\delta p_T/p_T$ to the data as a function of $p^{pp}_T$ for Pb+Pb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).

Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).

Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).

Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).

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$v_{2,2}^{unsub}$ and $v_{2,2}$ as a function of $\Delta\eta$ calculated from the 2-D per-trigger yields in figure 4(a) and 4(b), respectively.

$v_{3,3}^{unsub}$ and $v_{3,3}$ as a function of $\Delta\eta$ calculated from the 2-D per-trigger yields in figure 4(a) and 4(b), respectively.

$v_{4,4}^{unsub}$ and $v_{4,4}$ as a function of $\Delta\eta$ calculated from the 2-D per-trigger yields in figure 4(a) and 4(b), respectively.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

The integrated per-trigger yield, Y_{int}, on the near-side, the away-side and their difference and Y_{int} from the recoil as a function of event activity. Errors are statistical.

The integrated per-trigger yield, Y_{int}, on the near-side, the away-side and their difference and Y_{int} from the recoil as a function of event activity. Errors are statistical.

The Fourier coefficients $v_{n}$ as a function of $p_{T}^{a}$ extracted from the correlation functions, before and after the subtraction of the recoil component.

The Fourier coefficients $v_{n}$ as a function of $p_{T}^{a}$ extracted from the correlation functions, before and after the subtraction of the recoil component.

The Fourier coefficients $v_{n}$ as a function of $p_{T}^{a}$ extracted from the correlation functions, before and after the subtraction of the recoil component.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The centrality dependence of $v_{2}$ as a function of $N_{ch}^{rec}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{3}$ as a function of $N_{ch}^{rec}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{4}$ as a function of $N_{ch}^{rec}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{2}$ as a function of $E_{T}^{Pb}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{3}$ as a function of $E_{T}^{Pb}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{4}$ as a function of $E_{T}^{Pb}$. Values from before and after the recoil subtraction are included.

The $v_{2}$ as a function of $E_{T}^{Pb}$ obtained indirectly by mapping from the $N_{ch}^{rec}-dependence of $v_{2}$ using the correlation data shown in Fig. 2(b).

The $v_{3}$ as a function of $E_{T}^{Pb}$ obtained indirectly by mapping from the $N_{ch}^{rec}-dependence of $v_{3}$ using the correlation data shown in Fig. 2(b).

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic $v_1$ obtained using factorization from $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic $v_1$ obtained using factorization from $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic $v_1$ obtained using factorization from $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

$v_{2}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method.

$v_{2}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method, after the scaling.

$v_{3}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method.

$v_{3}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method, after the scaling.

$v_{4}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method.

$v_{4}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method, after the scaling.

Correlation between $E_{T}^{FCal}$ and $N_{ch}^{rec}$ for MB events (without weighting) and MB+HMT events (with weighting), errors are statistical.

Differential production yield per binary collision for $W^{-}$ bosons as a function of $|\eta_\ell|$.

The lepton charge asymmetry $A_{\ell}$ from $W^\pm$ bosons as a function of absolute pseudorapidity.