PI0_PI0 invariant mass distribution at an incident kinetic energy of 1200 MeV.

PI0_PI0 invariant mass distribution at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the PI0_PI0 opening angle (DELTA) at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the PI0_PI0 opening angle (DELTA) at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the PI0_PI0 opening angle (DELTA) at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the PI0_PI0 opening angle (DELTA) at an incident kinetic energy of 1300 MeV.

P_PI0 invariant mass distribution at an incident kinetic energy of 1000 MeV.

P_PI0 invariant mass distribution at an incident kinetic energy of 1100 MeV.

P_PI0 invariant mass distribution at an incident kinetic energy of 1200 MeV.

P_PI0 invariant mass distribution at an incident kinetic energy of 1300 MeV.

P_PI0_PI0 invariant mass distribution at an incident kinetic energy of 1000 MeV.

P_PI0_PI0 invariant mass distribution at an incident kinetic energy of 1100 MeV.

P_PI0_PI0 invariant mass distribution at an incident kinetic energy of 1200 MeV.

P_PI0_PI0 invariant mass distribution at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the Proton centre-of-mass angle at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the Proton centre-of-mass angle at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the Proton centre-of-mass angle at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the Proton centre-of-mass angle at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the PI0 centre-of-mass angle at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the PI0 centre-of-mass angle at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the PI0 centre-of-mass angle at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the PI0 centre-of-mass angle at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the PI0_PI0 centre-of-mass angle at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the PI0_PI0 centre-of-mass angle at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the PI0_PI0 centre-of-mass angle at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the PI0_PI0 centre-of-mass angle at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the PI0 angle in the PI0_PI0 subsystem at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the PI0 angle in the PI0_PI0 subsystem at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the PI0 angle in the PI0_PI0 subsystem at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the PI0 angle in the PI0_PI0 subsystem at an incident kinetic energy of 1300 MeV.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 718.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 723.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 727.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 731.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 735.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 739.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 743.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 748.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 752.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 756.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 760.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 768.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 772.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 777.1 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 781.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 785.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 789.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 793.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 797.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 801.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 805.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 809.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 814.1 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 818.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 822.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 826.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 830.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 834.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 838.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 842.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 846.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 850.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 854.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 858.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 862.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 866.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 870.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 874.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 878.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 882.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 886.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 890.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 894.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 898.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 902.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 906.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 910.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.3 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 914.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 918.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 922.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 926.1 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 930.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 933.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 937.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 941.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 945.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 949.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 953.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 957.1 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 960.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 964.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 968.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 972.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 976.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 980.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 983.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 987.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 991.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 995.1 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 998.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1002.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.4 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1006.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1011.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1019.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1026.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1034.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1041.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1048.6 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1055.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1063.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1070.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1077.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1084.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1091.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1098.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1105.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1112.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1119.1 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1125.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1132.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.5 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1139.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1146.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1152.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1159.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1165.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1172.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1178.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1185.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1191.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1198.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1204.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1210.5 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1216.7 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1222.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1229.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.6 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1235.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1242.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1251.3 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1260.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.8 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1268.9 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1277.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1287.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.7 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1300.0 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.9 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1315.1 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.8 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1335.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.8 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1355.4 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.8 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1376.2 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 4.9 PCT.

Differential cross section for the reaction GAMMA P --> ETA P at a photon energy of 1394.8 MeV. The errors in the table are statistical only and there is an overall systematic uncertainty of 5.0 PCT.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.72 to 1.73 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.73 to 1.74 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.74 to 1.75 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.75 to 1.76 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.76 to 1.77 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.77 to 1.78 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.78 to 1.79 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.79 to 1.8 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.8 to 1.81 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.81 to 1.82 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.82 to 1.83 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.83 to 1.84 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.84 to 1.85 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.85 to 1.86 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.86 to 1.87 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.87 to 1.88 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.88 to 1.89 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.89 to 1.9 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.9 to 1.91 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.91 to 1.92 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.92 to 1.93 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.93 to 1.94 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.94 to 1.95 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.96 to 1.97 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.97 to 1.98 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.98 to 1.99 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 1.99 to 2 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2 to 2.01 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.01 to 2.02 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.02 to 2.03 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.03 to 2.04 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.04 to 2.05 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.05 to 2.06 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.06 to 2.07 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.07 to 2.08 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.08 to 2.09 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.09 to 2.1 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.1 to 2.11 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.11 to 2.12 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.12 to 2.13 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.13 to 2.14 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.14 to 2.15 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.15 to 2.16 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.16 to 2.17 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.17 to 2.18 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.18 to 2.19 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.19 to 2.2 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.2 to 2.21 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.21 to 2.22 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.22 to 2.23 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.23 to 2.24 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.24 to 2.25 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.25 to 2.26 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.26 to 2.27 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.27 to 2.28 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.28 to 2.29 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.29 to 2.3 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.3 to 2.31 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.31 to 2.32 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.32 to 2.33 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.33 to 2.34 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.34 to 2.35 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.35 to 2.36 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.36 to 2.37 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.37 to 2.38 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.38 to 2.39 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.39 to 2.4 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.4 to 2.41 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.41 to 2.42 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.42 to 2.43 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.43 to 2.44 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.44 to 2.45 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.45 to 2.46 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.46 to 2.47 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.47 to 2.48 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.48 to 2.49 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.49 to 2.5 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.5 to 2.51 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.51 to 2.52 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.52 to 2.53 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.53 to 2.54 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.54 to 2.55 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.55 to 2.56 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.56 to 2.57 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.57 to 2.58 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.58 to 2.59 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.59 to 2.6 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.6 to 2.61 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.61 to 2.62 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.62 to 2.63 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.63 to 2.64 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.64 to 2.65 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.65 to 2.66 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.66 to 2.67 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.67 to 2.68 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.68 to 2.69 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.69 to 2.7 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.7 to 2.71 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.71 to 2.72 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.72 to 2.73 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.75 to 2.76 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.76 to 2.77 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.77 to 2.78 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.78 to 2.79 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.79 to 2.8 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.8 to 2.81 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.81 to 2.82 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.82 to 2.83 GeV.

Differential cross section as a function of COS(THETA(K+,CM)) for the centre-of mass range 2.83 to 2.84 GeV.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.95 to -0.85.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.85 to -0.75.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.75 to -0.65.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.65 to -0.55.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.55 to -0.45.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.45 to -0.35.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.35 to -0.25.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.25 to -0.15.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.15 to -0.05.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.05 to 0.05.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.05 to 0.15.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.15 to 0.25.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.25 to 0.35.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.35 to 0.45.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.45 to 0.55.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.55 to 0.65.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.65 to 0.75.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.75 to 0.85.

Differential cross section as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.85 to 0.95.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.85 to -0.75.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.75 to -0.65.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.65 to -0.55.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.55 to -0.45.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.45 to -0.35.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.35 to -0.25.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.25 to -0.15.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.15 to -0.05.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from -0.05 to 0.05.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.05 to 0.15.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.15 to 0.25.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.25 to 0.35.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.35 to 0.45.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.45 to 0.55.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.55 to 0.65.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.65 to 0.75.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.75 to 0.85.

Recoil polarization as a function of the centre-of-mass energy for the angular range COS(THETA(K+,CM) from 0.85 to 0.95.

The K$\pi$ pair invariant mass distribution integrated over the $K^{*0}$ $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ =62.4 GeV after mixed-event background subtraction.

The Kπ pair invariant mass distribution for various pT bins (top left) pT = 0.4–0.6 GeV/c in Au+Au collisions at √sNN = 200 GeV after the mixed-event background subtraction.

The Kπ pair invariant mass distribution for various pT bins (top right) pT = 0.6–0.8 GeV/c in Au+Au collisions at √sNN = 62.4 GeV after the mixed-event background subtraction.

The Kπ pair invariant mass distribution for various pT bins (bottom left) pT = 0.8–1.0 GeV/c in Au+Au collisions at √sNN = 200 GeV after the mixed-event background subtraction.

The Kπ pair invariant mass distribution for various pT bins (bottom right) pT = 1.0–1.2 GeV/c in Au+Au collisions at √sNN = 62.4 GeV after the mixed-event background subtraction.

The signal-to-background ratio for $K^{*0}$ measurements as a function of $p_T$ for different collision centrality bins (0-10%, 10-40%, 40-60%, 60-80%) in Au+Au collisions at 200 GeV.

$K^{*0}$ mass as a function of $p_T$ for minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

$K^{*0}$ mass as a function of $p_T$ for minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

$K^{*0}$ mass as a function of $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

$K^{*0}$ mass as a function of $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

$K^{*0}$ width as a function of $p_T$ for minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

$K^{*0}$ width as a function of $p_T$ for minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

$K^{*0}$ width as a function of $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

$K^{*0}$ width as a function of $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

The $K^{*0}$ reconstruction efficiency multiplied by the detector acceptance as a function of $p_T$ in Au+Au (|$\eta$| < 0.8) collisions at 200 GeV for different collision centrality bins (0-20% ,20-40% , 40-60%)

The $K^{*0}$ reconstruction efficiency multiplied by the detector acceptance as a function of $p_T$ in Cu+Cu (|$\eta$| < 1.0) collisions at 200 GeV for different collision centrality bins (0-20% ,20-40% , 40-60%)

Mid-rapidity $K^{*0}$ $p_T$ spectra for various collision centrality bins (0-20%, 20-40%, 40-60%, 60-80%) in Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

Mid-rapidity $K^{*0}$ $p_T$ spectra for various collision centrality bins (0-20%, 20-40%, 40-60%) in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

Mid-rapidity $K^{*0}$ $p_T$ spectra for various collision centrality bins (0-20%, 20-40%, 40-60%, 60-80%) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

Mid-rapidity $K^{*0}$ $p_T$ spectra for various collision centrality bins (0-20%, 20-40%, 40-60%) in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity yields dN/dy of $K^{*0}$ as a function of the average number of participating nucleons, $⟨N_{part}⟩$, for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

The mid-rapidity yields dN/dy of $K^{*0}$ as a function of the average number of participating nucleons, $⟨N_{part}⟩$, for Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

The mid-rapidity yields dN/dy of $K^{*0}$ as a function of the average number of participating nucleons, $⟨N_{part}⟩$, for Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity yields dN/dy of $K^{*0}$ as a function of the average number of participating nucleons, $⟨N_{part}⟩$, for Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity $K^{*0}$ $⟨p_T⟩$ as a function $⟨N_{part}⟩$ for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

The mid-rapidity $K^{*0}$ $⟨p_T⟩$ as a function $⟨N_{part}⟩$ for Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

The mid-rapidity $K^{*0}$ $⟨p_T⟩$ as a function $⟨N_{part}⟩$ for Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity $K^{*0}$ $⟨p_T⟩$ as a function $⟨N_{part}⟩$ for Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity $⟨p_T⟩$ of $\pi$, K, p and $K^{*0}$ as a function of $⟨N_{part}⟩$ for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio for Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio for Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio for Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})N(K^-)$ in Au+Au collisions divided by $N(K^{*0})N(K^-)$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$.

Mid-rapidity $N(K^{*0})N(K^-)$ in Cu+Cu collisions divided by $N(K^{*0})N(K^-)$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})N(K^-)$ in d+Au collisions divided by $N(K^{*0})N(K^-)$ ratio in d+Au collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias Au+Au collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias Cu+Cu collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias p+p collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias Au+Au collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias Cu+Cu collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias p+p collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio for Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio for Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio for Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $[N(\phi)/N(K^{*0})]$ in Au+Au collisions divided by $[N(\phi)/N(K^{*0})]$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $[N(\phi)/N(K^{*0})]$ in Cu+Cu collisions divided by $[N(\phi)/N(K^{*0})]$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $[N(\phi)/N(K^{*0})]$ in d+Au collisions divided by $[N(\phi)/N(K^{*0})]$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias Au+Au collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias Cu+Cu collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias p+p collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias Au+Au collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias Cu+Cu collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias p+p collisions as a function of $\sqrt{s_{NN}}$.

The $K^{*0}$ $v_2$ (Run IV) as a function of $p_T$ in minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $K^{*0}$ $v_2$ (Run II) as a function of $p_T$ in minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $K^{*0}$ $R_{CP}$ as a function of $p_T$ in Au+Au collisions at 62.4 and 200 GeV compared to the $R_{CP}$ of $K^0_S$ and $\Lambda$ at 200 GeV.

The $K^{*0}$ $R_{CP}$ as a function of $p_T$ in Au+Au collisions at 62.4 and 200 GeV compared to the $R_{CP}$ of $K^0_S$ and $\Lambda$ at 200 GeV.

The $K^{*0}$ $R_{CP}$ as a function of $p_T$ in Au+Au collisions at 62.4 and 200 GeV compared to the $R_{CP}$ of $K^0_S$ and $\Lambda$ at 200 GeV.

The $K^{*0}$ ~$R_{CP}$~ as a function of $p_T$ in Au+Au collisions at 62.4 and 200 GeV compared to the $R_{CP}$ of $K^0_S$ and $\Lambda$ at 200 GeV.

Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1 & Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1 & Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1 & Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

$v_2$ vs $N_{part}$ in two $p_T$ ranges and $R_{AA}$ vs $N_{part}$ in the same $p_T$ ranges.

$v_2$ vs $N_{part}$ in two $p_T$ ranges and $R_{AA}$ vs $N_{part}$ in the same $p_T$ ranges.

$v_2$ vs $N_{part}$ and $R_{AA}$ vs $N_{part}$ in two $p_T$ ranges compared with WHDG model.

$v_2$ vs $N_{part}$ in two $p_T$ ranges compared with various models.

$R_{AA}$ vs $N_{part}$ in two $p_T$ ranges compared with various models.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 0% to 20% centrality $Au+Au$. 90% Limit on 18-20 and 20-22 GeV/c bins.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 20% to 40% centrality $Au+Au$. 90% Limit for 20-22 GeV/c bin.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 40% to 60% centrality $Au+Au$. 90% Limit for 18-20 GeV/c bin.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 20% to 60% centrality $Au+Au$. 90% Limit for 18-20 GeV/c bin.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 60% to 92% centrality $Au+Au$. 90% Limit for 18-20 GeV/c bin.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 0% to 92% centrality $Au+Au$.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, $p+p$.

${\eta}$ $R_{AA}$, 0% to 5% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 0% to 10% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 10% to 20% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 0% to 20% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 20% to 40% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 40% to 60% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 20% to 60% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 60% to 92% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 0% to 92% centrality $Au+Au$.

${\pi^{0}}$ $R_{AA}$, 0% to 92% centrality $Au+Au$.

${\eta}$ ${R_{AA}}$, 0% to 92% centrality $Au+Au$.

${\eta}$ $R_{AA}$ vs centrality ($p_T>$20 GeV/c).

${\eta}$ $R_{AA}$ vs centrality ($p_T>$5 GeV/c).

Slope ${\eta}$ $R_{AA}$ ($5<p_T<$ 18 GeV/c) vs centrality.

$\chi^{2}/{NDF}$, Prob%, ${\eta}$ $R_{AA}$ ($5<p_T<$ 18 GeV/c) Prob, $R_{AA}$ ($p_T>$ 5 GeV/c) Prob vs centrality

The balance function in terms of $\Delta y$ for identified charged pion pairs from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for nine centrality bins.

The balance function in terms of $\Delta y$ for identified charged kaon pairs from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for nine centrality bins.

The balance function for p+p collisions at $\sqrt{s_{NN}}$ = 200 GeV. The top panel shows the balance function for all charged particles in terms of $\Delta \eta$. The bottom panel gives the balance function for charged pion pairs and charged kaon pairs in terms of $\Delta y$.

The balance function for p+p collisions at $\sqrt{s_{NN}}$ = 200 GeV. The top panel shows the balance function for all charged particles in terms of $\Delta \eta$. The bottom panel gives the balance function for charged pion pairs and charged kaon pairs in terms of $\Delta y$.

The balance function in terms of $\Delta \eta$ for all charged particles from d+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for three centrality bins.

The balance function in terms of $q_{inv}$ for charged pion pairs from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV in nine centrality bins. Curves correspond to a thermal distribution (Eq. 3) plus $K^{0}_{S}$ decay.

The balance function in terms of $q_{inv}$ for charged-pion pairs in two centrality bins over the range 0 < $q_{inv}$ < 0.2 GeV/c.

The balance function in terms of $q_{inv}$ for charged kaon pairs from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV in nine centrality bins. Curves correspond to a thermal (Eq. 3) distribution plus $\phi$ decay.

The balance function in terms of $q_{inv}$ for charged pion pairs [part a)] and charged kaon pairs [part b)] from p+p collisions at $\sqrt{s_{NN}}$ = 200 GeV integrated over all multiplicities. Solid curves correspond to a thermal distribution (Eq. 3) plus $K^{0}_{S}$ and $\rho^{0}$ decay for pions and φ decay for kaons. The dashed curve for pions represents a fit to a thermal distribution (Eq. 3) plus $K^{0}_{S}$ decay and $\rho^{0}$ decay, with the $\rho^{0}$ mass shifted down by 0.04 $GeV/c^{2}$.

The balance function in terms of $q_{long}$ for charged pion pairs from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV in nine centrality bins.

The balance function in terms of $q_{out}$ for charged pion pairs from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV in nine centrality bins.

(Color online) The balance function in terms of $q_{side}$ for charged pion pairs from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for nine centrality bins.

(Color online) The balance function in terms of $\Delta\phi$ for all charged particles with 0.2< pt<2.0 GeV/c from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV in nine centrality bins.The closed circles represent the real data minus the mixed events.

(Color online) The balance function in terms of $\Delta\phi$ for all charged particles with 1.0< pt<10.0 GeV/c from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV in nine centrality bins.The closed circles represent the real data minus the mixed events.

(Color online) The balance function in terms of $\Delta y$ for charged pions from central collisions of Au+Au at $\sqrt{s_{NN}}$ = 200 GeV compared with predictions from the blast-wave model from Ref.[30] and filtered HIJING calculations taking into account acceptance and efficiency.

(Color online) The balance function in terms of $\Delta y$ for charged pions from central collisions of Au+Au at $\sqrt{s_{NN}}$ = 200 GeV compared with predictions from the blast-wave model from Ref.[30] and filtered HIJING calculations taking into account acceptance and efficiency.

(Color online) The balance function in terms of $q_{inv}$ for charged pions from central collisions of Au+Au at $\sqrt{s_{NN}}$ = 200 GeV compared with predictions from the blast-wave model from Ref.[30] and predictions from filtered HIJING calculations including acceptance and efficiency. For the blast-wave calculations, HBT is not included and the decays of the $K^0_S$ and $\rho^0$ are not shown.

(Color online) The balance function in terms of $q_{inv}$ for charged pions from central collisions of Au+Au at $\sqrt{s_{NN}}$ = 200 GeV compared with predictions from the blast-wave model from Ref.[30] and predictions from filtered HIJING calculations including acceptance and efficiency. For the blast-wave calculations, HBT is not included and the decays of the $K^0_S$ and $\rho^0$ are not shown.

(Color online) The balance function width $<\Delta\eta>$ for all charged particles from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV compared with the widths of balance functions calculated using shuffled events. Also shown are the balance function widths for p+p and d+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.Filtered HIJING calculations are also shown for the widths of the balance function from p+p and Au+Au collisions. Filtered UrQMD calculations are shown for the widths of the balance function from Au+Au collisions.

(Color online) The balance function width $<\Delta\eta>$ for all charged particles from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV compared with the widths of balance functions calculated using shuffled events. Also shown are the balance function widths for p+p and d+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.Filtered HIJING calculations are also shown for the widths of the balance function from p+p and Au+Au collisions. Filtered UrQMD calculations are shown for the widths of the balance function from Au+Au collisions.

(Color online) The balance function widths for identified charged pions and charged kaons from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV and p+p collisions at $\sqrt{s}$ = 200 GeV. Filtered HIJING calculations are shown for the same systems. Filtered UrQMD calculations are shown for Au+Au. Also shown is the width of the balance function for pions predicted by the blast-wave model of Ref.[30].

(Color online) The balance function width $\sigma$ extracted from $B(q_{inv})$ for identified charged pions and kaons from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV and p+p collisions at $\sqrt{s}$ = 200 GeV using a thermal fit (Eq. 3) where $\sigma$ is the width. Filtered HIJING and UrQMD calculations are shown for pions and kaons from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. Values are shown for $\sqrt{2mT_{kin}}$ from Au+Au collisions, where m is the mass of a pion or a kaon, and $T_{kin}$ is calculated from identified particle spectra [45]. The width predicted by the blast-wave model of Ref. [30] is also shown for pions.

(Color online) The balance function width $\sigma$ extracted from $B(q_{inv})$ for identified charged pions and kaons from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV and p+p collisions at $\sqrt{s}$ = 200 GeV using a thermal fit (Eq. 3) where $\sigma$ is the width. Filtered HIJING and UrQMD calculations are shown for pions and kaons from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. Values are shown for $\sqrt{2mT_{kin}}$ from Au+Au collisions, where m is the mass of a pion or a kaon, and $T_{kin}$ is calculated from identified particle spectra [45]. The width predicted by the blast-wave model of Ref. [30] is also shown for pions.

(Color online) The widths for the balance functions for pions in terms of $q_{long}$, $q_{out}$, and $q_{side}$ compared with UrQMD calculations.

(Color online) The weighted average cosine of the relative azimuthal angle,$<\cos(\Delta\phi)$, extracted from $B(\Delta\phi)$ for all charged particles with $0.2< p_t <2.0$ from Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV and from all charged particleswith $1.0< p_t <10.0$ GeV/c, compared with predictions using filtered UrQMD calculations.

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=1$ for $0-20$% central

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\mathrm{d}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=1$ for $0-20$% central

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=2$ for $0-20$% central

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\mathrm{d}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=2$ for $0-20$% central

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=3$ for $0-20$% central

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\mathrm{d}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=3$ for $0-20$% central

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=0$ for $0-20$% central

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\overline{\mathrm{d}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=0$ for $0-20$% central

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=1$ for $0-20$% central

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\overline{\mathrm{d}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=1$ for $0-20$% central

$B_{2}$ versus $p_{\mathrm{T}}/A$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=0$ for $0-20$% central

$B_{2}$ versus $p_{\mathrm{T}}/A$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=1$ for $0-20$% central

$B_{2}$ versus $p_{\mathrm{T}}/A$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=2$ for $0-20$% central

$B_{2}$ versus $p_{\mathrm{T}}/A$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=3$ for $0-20$% central

$B_{2}$ versus $p_{\mathrm{T}}/A$ for $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=0$ for $0-20$% central

$B_{2}$ versus $p_{\mathrm{T}}/A$ for $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=1$ for $0-20$% central

$\langle f\rangle$ versus $m_{\mathrm{T}}/A$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=0$ for $0-20$% central

$\langle f\rangle$ versus $m_{\mathrm{T}}/A$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=1$ for $0-20$% central

$\langle f\rangle$ versus $m_{\mathrm{T}}/A$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=2$ for $0-20$% central

$\langle f\rangle$ versus $m_{\mathrm{T}}/A$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=3$ for $0-20$% central

$\langle f\rangle$ versus $m_{\mathrm{T}}/A$ for $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=0$ for $0-20$% central

$\langle f\rangle$ versus $m_{\mathrm{T}}/A$ for $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ near $y=1$ for $0-20$% central