| (Color online) Particle ratios \kskm (a,b) and \phikm (c,d) in pp, \dau, and \ada collisions~\cite{ALICE_strange_900GeV,ALICE_kstar_phi_7TeV,STAR_Kstar_200GeV_2005,STAR_Kstar_2011,STAR_phi_200GeV_2005,STAR_phi_2009,ALICE_piKp_7TeV,NA49_phi_2000,NA49_phi_2008,NA49_piK_2002,STAR_phi_130GeV,PHENIX_mesons_pp_2011,PHENIX_piKp_pp_2011,PHENIX_phi_AuAu_2005,ALICE_piKp_900GeV}. In panels (a) and (c) these ratios are presented for different centrality intervals as a function of \dncr~\cite{ALICE_multiplicity,STAR_centrality_2009,ALICE_multiplicity_pp7TeV,STAR_piKp_CuCu}. In panels (b) and (d), these ratios are presented for pp, central \dau, and central \ada collisions as a function of \rsnno. For quantities marked ``*", boxes represent the total uncertainty (separate uncertainties are not reported). Otherwise, bars represent statistical uncertainties and boxes represent systematic uncertainties. In panel (c), the two most central \phikm points for \au collisions are for overlapping centrality intervals (0-5\% and 0-10\%). In panel (d) the \phikm points for pp and \dau collisions at \rsnn[200~GeV] have been shifted horizontally for visibility. The values given by a grand-canonical thermal model with a chemical freeze-out temperature of 156~MeV are also shown~\cite{Stachel_SQM2013}. |