Differential cross section for proton production with a negative pion beam and Beryllium target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Beryllium target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Beryllium target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Beryllium target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Beryllium target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Beryllium target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Beryllium target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Beryllium target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Beryllium target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Carbon target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Carbon target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Carbon target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Carbon target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Carbon target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Carbon target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Carbon target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Carbon target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Carbon target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Carbon target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Carbon target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Carbon target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Aluminium target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Aluminium target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Aluminium target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Aluminium target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Aluminium target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Aluminium target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Aluminium target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Aluminium target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Aluminium target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Aluminium target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Aluminium target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Aluminium target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Copper target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Copper target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Copper target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Copper target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Copper target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Copper target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Copper target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Copper target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Copper target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Copper target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Copper target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Copper target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Tin target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Tin target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Tin target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Tin target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Tin target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Tin target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Tin target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Tin target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Tin target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Tin target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Tin target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Tin target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Tantallum target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Tantallum target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Tantallum target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Tantallum target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Tantallum target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Tantallum target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Tantallum target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Tantallum target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Tantallum target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Tantallum target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Tantallum target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Tantallum target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Lead target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Lead target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Lead target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a negative pion beam and Lead target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Lead target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Lead target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Lead target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a positive pion beam and Lead target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Lead target in the angular range 0.050 to 0.100 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Lead target in the angular range 0.100 to 0.150 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Lead target in the angular range 0.150 to 0.200 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

Differential cross section for proton production with a proton beam and Lead target in the angular range 0.200 to 0.250 radians. The errors are the square-root of the diagonal elements of the covariant matrix.

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.

Breakdown of syst. uncertainties (fully bin-by-bin correlated) for differential cross section for $e^+e^-\rightarrow\pi^+\pi^-\gamma$, with $50^o<\theta_\gamma<130^o$

Bare cross section for $e^+e^-\rightarrow\pi^+\pi^-$

Statistical covariance matrix for bare cross section for $e^+e^-\rightarrow\pi^+\pi^-$

Inverse statistical covariance matrix for bare cross section for $e^+e^-\rightarrow\pi^+\pi$

Breakdown of syst. uncertainties (fully bin-by-bin correlated) for the cross section for $e^+e^-\rightarrow\pi^+\pi^-$

Pion form factor $|F_\pi|^2$

Statistical covariance matrix for pion form factor $|F_\pi|^2$

Inverse statistical covariance matrix $|F_\pi|^2$

Breakdown of syst. uncertainties (fully bin-by-bin correlated) for the pion form factor $|F_\pi|^2$

Vacuum polarisation correction $\delta_{VP}(s)=(\frac{\alpha_{em}(s)}{\alpha_{em}(0)})^2$, with $\sigma^{bare} = \sigma^{dressed}/\delta$ - calculated using the routine from F.Jegerlehner: https://web.archive.org/web/20170828074416/http://www-com.physik.hu-berlin.de/~fjeger/alphaQEDn.uu (2003, archived on August 28, 2017)

Final State Radiation correction $(1.+\eta_{FSR}(s))$, evaluated using the formula in Eur. Phys. J. C 24, 51-69 (2002)

The differential radiator function cross section $H(M_{\pi\pi}^2,s)\cdot \frac{\pi \alpha^2 \beta_\pi^3}{3 M_{\pi\pi}^2 s}$, inclusive in $\theta_\gamma$, in bins of 0.01 GeV$^2$ in $M_{\pi\pi}^2$. The value used for $s$ in the Monte Carlo production is $s = 999.85\; GeV^2$, corresponding to the mean value of DA$\Phi$NE energy for data collected in 2006. Obtained with the PHOKHARA5 MC generator, see Eur. Phys. J. C 27, 563 (2003) and https://looptreeduality.csic.es/phokhara/phokhara5.0.tar.gz

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.

The COLLINS asymmetry for negatively charged hadrons as a function of X.

The COLLINS asymmetry for negatively charged hadrons as a function of Z.

The COLLINS asymmetry for negatively charged hadrons as a function of PT.

The SIVERS asymmetry for positively charged hadrons as a function of X.

The SIVERS asymmetry for positively charged hadrons as a function of Z.

The SIVERS asymmetry for positively charged hadrons as a function of PT.

The SIVERS asymmetry for negatively charged hadrons as a function of X.

The SIVERS asymmetry for negatively charged hadrons as a function of Z.

The SIVERS asymmetry for negatively charged hadrons as a function of PT.

The COLLINS asymmetry for positively charged hadrons as a function of Z for X > 0.05.

The COLLINS asymmetry for positively charged hadrons as a function of PT for X > 0.05.

The COLLINS asymmetry for negatively charged hadrons as a function of Z for X > 0.05.

The COLLINS asymmetry for negatively charged hadrons as a function of PT for X > 0.05.

The SIVERS asymmetry for positively charged hadrons as a function of Z for X > 0.032.

The SIVERS asymmetry for positively charged hadrons as a function of PT for X > 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of Z for X > 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of PT for X > 0.032.

The COLLINS asymmetry for positively charged hadrons as a function of W for X > 0.032.

The COLLINS asymmetry for negatively charged hadrons as a function of W for X > 0.032.

The SIVERS asymmetry for positively charged hadrons as a function of W for X > 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of W for X > 0.032.

The COLLINS asymmetry for positively charged hadrons as a function of W for X < 0.032.

The COLLINS asymmetry for negatively charged hadrons as a function of W for X < 0.032.

The SIVERS asymmetry for positively charged hadrons as a function of W for X < 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of W for X < 0.032.

The COLLINS asymmetry for positively charged hadrons as a function of X for W > 7.5 GeV.

The COLLINS asymmetry for negatively charged hadrons as a function of X for W > 7.5 GeV.

The SIVERS asymmetry for positively charged hadrons as a function of X for W > 7.5 GeV.

The SIVERS asymmetry for negatively charged hadrons as a function of X for W > 7.5 GeV.

The COLLINS asymmetry for positively charged hadrons as a function of X for W < 7.5 GeV.

The COLLINS asymmetry for negatively charged hadrons as a function of X for W < 7.5 GeV.

The SIVERS asymmetry for positively charged hadrons as a function of X for W < 7.5 GeV.

The SIVERS asymmetry for negatively charged hadrons as a function of X for W < 7.5 GeV.

Measured differential yield of charged hadrons as a function oftransverse momentum for the pseudorapidity range -2.4 to +2.4 for centre-of-mass energy 7000 GeV. Errors are statistical and systematic added in quadrature.

Reconstructed differential charged hadron yields as a function of pseudorapidity averaged over the three methods methodsat a centre-of-mass energy of 7000 GeV.Errors shown are systematic (4 pct).Systematic errors are less than 0.5 pct of the values.