$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=0.9-1.1$ for $0-10$% 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 $\mathrm{\pi}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.05-3.15$ for $0-10$% 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 $\mathrm{\pi}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.15-3.25$ for $0-10$% 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 $\mathrm{\pi}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.4-3.6$ for $0-10$% 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 $\mathrm{\pi}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=-0.2-0.0$ for $0-10$% 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 $\mathrm{\pi}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=0.0-0.2$ for $0-10$% 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 $\mathrm{\pi}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=0.7-0.9$ for $0-10$% 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 $\mathrm{\pi}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=0.9-1.1$ for $0-10$% 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 $\mathrm{\pi}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.05-3.15$ for $0-10$% 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 $\mathrm{\pi}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.15-3.25$ for $0-10$% 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 $\mathrm{\pi}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.4-3.6$ for $0-10$% 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 $\mathrm{K}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=-0.15-0.15$ for $0-10$% 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 $\mathrm{K}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=0.6-0.8$ for $0-10$% 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 $\mathrm{K}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=0.8-1.0$ for $0-10$% 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 $\mathrm{K}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=2.55-2.65$ for $0-10$% 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 $\mathrm{K}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=2.65-2.75$ for $0-10$% 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 $\mathrm{K}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.15-3.25$ for $0-10$% 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 $\mathrm{K}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.25-3.35$ for $0-10$% 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 $\mathrm{K}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=-0.15-0.15$ for $0-10$% 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 $\mathrm{K}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=0.6-0.8$ for $0-10$% 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 $\mathrm{K}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=0.8-1.0$ for $0-10$% 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 $\mathrm{K}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=2.55-2.65$ for $0-10$% 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 $\mathrm{K}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=2.65-2.75$ for $0-10$% 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 $\mathrm{K}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.15-3.25$ for $0-10$% 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 $\mathrm{K}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=3.25-3.35$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}y}$ versus $y$ for $\mathrm{\pi}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}y}$ versus $y$ for $\mathrm{\pi}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}y}$ versus $y$ for $\mathrm{K}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}y}$ versus $y$ for $\mathrm{K}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\mathrm{\pi}^{-}/\mathrm{\pi}^{+}$ versus $y$ for $\mathrm{\pi}^{-}$,$\mathrm{\pi}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\mathrm{K}^{-}/\mathrm{K}^{+}$ versus $y$ for $\mathrm{K}^{-}$,$\mathrm{K}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\overline{\mathrm{p}}/\mathrm{p}$ versus $y$ for $\overline{\mathrm{p}}$,$\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\mathrm{K}^{+}/\mathrm{\pi}^{+}$ versus $y$ for $\mathrm{K}^{+}$,$\mathrm{\pi}^{+}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\mathrm{K}^{-}/\mathrm{\pi}^{-}$ versus $y$ for $\mathrm{K}^{-}$,$\mathrm{\pi}^{-}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\mathrm{K}^{+}/\mathrm{K}^{-}$ versus $\overline{\mathrm{p}}/\mathrm{p}$ for $\mathrm{K}^{+}$,$\mathrm{K}^{-}$,$\overline{\mathrm{p}}$,$\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\mathrm{K}^{+}/\mathrm{\pi}^{+}$,$\mathrm{K}^{-}/\mathrm{\pi}^{-}$ versus $\overline{\mathrm{p}}/\mathrm{p}$ for $\mathrm{K}^{+}$,$\mathrm{K}^{-}$,$\mathrm{\pi}^{+}$,$\mathrm{\pi}^{-}$,$\overline{\mathrm{p}}$,$\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$T_{\mathrm{K^{+}}}$,$T_{\mathrm{K^{-}}}$ versus $\overline{\mathrm{p}}/\mathrm{p}$ for $\mathrm{K}^{+}$,$\mathrm{K}^{-}$,$\mathrm{p}$,$\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=62.4\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$, $\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\mathrm{\pi}^{+}$, $\mathrm{p}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=0.4-0.9$

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=2.2-2.5$

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=2.2-2.5$

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=2.94-3.1$

$\frac{1}{2\pi p_{\mathrm{T}}}\frac{\mathrm{d}^2N}{\mathrm{d}p_{\mathrm{T}}\mathrm{d}y}$ versus $p_{\mathrm{T}}$ for $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ near $y=2.94-3.1$

$\frac{\mathrm{d}N}{\mathrm{d}y}$ versus $y$ for $\mathrm{p}$,$\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$

$\delta y$,$\delta E$ versus for $\mathrm{p}$,$\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}(y-y_{\mathrm{beam}})}\frac{2}{N_{\mathrm{part}}}$ versus $\mathrm{y}-\mathrm{y}_{\mathrm{beam}}$ for BARYON-ANTIBARYON in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}(y-y_{\mathrm{beam}})}\frac{2}{N_{\mathrm{part}}}$ versus $\mathrm{y}-\mathrm{y}_{\mathrm{beam}}$ for BARYON-ANTIBARYON in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}(y-y_{\mathrm{beam}})}\frac{2}{N_{\mathrm{part}}}$ versus $\mathrm{y}-\mathrm{y}_{\mathrm{beam}}$ for BARYON-ANTIBARYON in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}(y-y_{\mathrm{beam}})}\frac{2}{N_{\mathrm{part}}}$ versus $\mathrm{y}-\mathrm{y}_{\mathrm{beam}}$ for BARYON-ANTIBARYON in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}(y-y_{\mathrm{beam}})}\frac{2}{N_{\mathrm{part}}}$ versus $\mathrm{y}-\mathrm{y}_{\mathrm{beam}}$ for BARYON-ANTIBARYON in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200.0\,\mathrm{Ge\!V}$ for $0-10$% central

$\frac{\mathrm{d}N}{\mathrm{d}(y-y_{\mathrm{beam}})}\frac{2}{N_{\mathrm{part}}}$ versus $\mathrm{y}-\mathrm{y}_{\mathrm{beam}}$ for BARYON-ANTIBARYON in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$ for $0-10$% central

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

The intercepts and slope for the exponential parameterisation of the differential cross section of the form A exp(-B*PT**2). Errors do not contain additional 2.1 PCT uncertainty on the intercepts.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

The intercepts and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the photoproduction sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

The intercept and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the low-Q**2 DIS sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

The intercept and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the mid-Q**2 DIS sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

The intercept and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the high-Q**2 DIS sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

Differential inclusive charged hadron production cross section as a function of PT.

Differential inclusive charged hadron production cross section as a function of pseudorapidity.

Differential inclusive charged hadron production cross section as a function of pseudorapidity.

Differential inclusive charged hadron production cross section as a function of pseudorapidity.

Differential inclusive charged hadron production cross section as a function of pseudorapidity.

Differential inclusive charged hadron production cross section as a function of PT.

Differential inclusive charged hadron production cross section as a function of PT.

Differential inclusive charged hadron production cross section as a function of PT.

Differential inclusive charged hadron production cross section as a function of PT.

SPHERICITY distribution.

PLANARITY distribution.

OBLATENESS distribution.

HEAVY JET Mass distribution in the standard scheme definition.

HEAVY JET Mass distribution in the E scheme definition.

LIGHT JET Mass distribution in the standard scheme definition.

JET MASS DIFFERENCE distribution in the standard scheme definition.

TOTAL JET MASS distribution in the standard scheme definition.

TOTAL JET MASS distribution in the E scheme definition.

Wide Jet Broadening (BMAX) distribution.

Narrow Jet Broadening (BMIN) distribution.

Total Jet Broadening (BTOT) distribution.

Jet Broadening Difference (BDIFF) distribution.

C-PARAMETER distribution.

Integrated 2 Jet rates for YCUT=0.04 (Durham, angle ordered Durham and Cambridge alogrithms) and YCUT = 0.8 (JADE alogrithm).

Integrated 3 Jet rates for YCUT=0.04 (Durham, angle ordered Durham and Cambridge alogrithms) and YCUT = 0.8 (JADE alogrithm).

Integrated Jet Cone Energy Fractions (JCEF) for different anglular intervals.

Integrated values of the Energy Energy Correlations (EEC) for different angular intervals.

Integrated values of the Energy Energy Correlations Asymmetry (AEEC) for different angular intervals.

Mean values of Y23.

Mean values of Thrust related observables.

Mean values of the Jet Broadenings.

Mean values of jet masses in the standard definition scheme.

Mean values of jet masses in the E definition scheme.

Mean values of jet masses in the p definition scheme.

Mean values of the C- and D- Parameter variables.

Rapidity distributions (relative to the thrust axis) for c.m. energies from183 to 196 GeV.

Rapidity distributions (relative to the thrust axis) for c.m. energies from200 to 207 GeV.

LN(1/XP) distributions for c.m. energies from 183 to 196 GeV.

LN(1/XP) distributions for c.m. energies from 200 to 207 GeV.

PTIN distributions for c.m. energies from 183 to 196 GeV.

PTIN distributions for c.m. energies from 200 to 207 GeV.

PTOUT distributions for c.m. energies from 183 to 196 GeV.

PTOUT distributions for c.m. energies from 200 to 207 GeV.

1-THRUST distributions for c.m. energies from 183 to 196 GeV.

1-THRUST distributions for c.m. energies from 200 to 207 GeV.

THRUST-MAJOR distributions for c.m. energies from 183 to 196 GeV.

THRUST-MAJOR distributions for c.m. energies from 200 to 207 GeV.

THRUST-MINOR) distributions for c.m. energies from 183 to 196 GeV.

THRUST-MINOR distributions for c.m. energies from 200 to 207 GeV.

Oblateness distributions for c.m. energies from 183 to 196 GeV.

Oblateness distributions for c.m. energies from 200 to 207 GeV.

Wide Jet Broadening (BMAX) distributions for c.m. energies from 183 to 196 GeV.

Wide Jet Broadening (BMAX) distributions for c.m. energies from 200 to 207 GeV.

Total Jet Broadening (BTOT) distributions for c.m. energies from 183 to 196GeV.

Total Jet Broadening (BTOT) distributions for c.m. energies from 200 to 207GeV.

Jet Broadening Difference (BDIFF) distributions for c.m. energies from 183 to 196 GeV.

Jet Broadening Difference (BDIFF) distributions for c.m. energies from 200 to 207 GeV.

C-PARAMETER distributions for c.m. energies from 183 to 196 GeV.

C-PARAMETER distributions for c.m. energies from 200 to 207 GeV.

D-PARAMETER distributions for c.m. energies from 183 to 196 GeV.

D-PARAMETER distributions for c.m. energies from 200 to 207 GeV.

Heavy Jet Mass distributions in the standard scheme definition for c.m. energies from 183 to 196 GeV.

Heavy Jet Mass distributions in the standard scheme definition for c.m. energies from 200 to 207 GeV.

Heavy Jet Mass distributions in the p scheme definition for c.m. energies from 183 to 196 GeV.

Heavy Jet Mass distributions in the p scheme definition for c.m. energies from 200 to 207 GeV.

Heavy Jet Mass distributions in the E scheme definition for c.m. energies from 183 to 196 GeV.

Heavy Jet Mass distributions in the E scheme definition for c.m. energies from 200 to 207 GeV.

Light Jet Mass distributions in the standard definition for c.m. energies from 183 to 196 GeV.

Light Jet Mass distributions in the standard definition for c.m. energies from 200 to 207 GeV.

Jet Mass Difference distributions from c.m.energies from 183 to 196 GeV.

Jet Mass Difference distributions from c.m.energies from 200 to 207 GeV.

Sphericity distributions for c.m.energies from 183 to 196 GeV.

Sphericity distributions for c.m.energies from 200 to 207 GeV.

Planarity distributions for c.m.energies from 183 to 196 GeV.

Planarity distributions for c.m.energies from 200 to 207 GeV.

Aplanarity distributions for c.m.energies from 183 to 196 GeV.

Aplanarity distributions for c.m.energies from 200 to 207 GeV.

Ratio of cross section for PSI(2S) to J/PSI production. as a function of Z. Statistical errors only.

The measured J/PSI differential cross section DSIG/DZ for different PT cuts.

The measured J/PSI differential cross section DSIG/DPT**2.

The J/PSI cross section versus W.

The measured J/PSI differential cross section DSIG/DYRAP.

J/PSI helicity parameter 'ALPHA', defined as DN/DCOS(THETA) ~ 1 + ALPHA*COS(THETA)**2, as a function of PT in the target frame.The uncertainties are due to the total experimental uncertainties.

J/PSI helicity parameter 'ALPHA', defined as DN/DCOS(THETA) ~ 1 + ALPHA*COS(THETA)**2, as a function of PT in the helicity basis.The uncertainties are due to the total experimental uncertainties.

J/PSI leptoproduction differential cross section as a function of the laboratory frame PT**2.

J/PSI leptoproduction differential cross section as a function of the centre-of-mass frame rapidity Y*.

J/PSI leptoproduction differential cross section as a function of the centre-of-mass frame PT**2.

J/PSI leptoproduction differential cross section as a function of the laboratory frame rapidity Y.

J/PSI leptoproduction differential cross section as a function of Q**2 for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of Z for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of W for laboratort PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of the laboratory frame PT**2 for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of the centre-of-mass frame rapidity Y* for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of the centre-of-mass frame PT**2 for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction double differential cross section as a function of the centre-of-mass frame PT**2 and Z for the Z range 0.3 to 0.6.

J/PSI leptoproduction double differential cross section as a function of the centre-of-mass frame PT**2 and Z for the Z range 0.6 to 0.75.

J/PSI leptoproduction double differential cross section as a function of the centre-of-mass frame PT**2 and Z for Z range 0.75 to 0.9.

J/PSI leptoproduction double differential cross section as a function of Q**2 and Z for the Z range 0.3 to 0.6.

J/PSI leptoproduction double differential cross section as a function of Q**2 and Z for the Z range 0.6 to 0.75.

J/PSI leptoproduction double differential cross section as a function of Q**2 and Z for the Z range 0.75 to 0.9.

J/PSI photoproduction cross section at a mean Q**2 of 10.6 GeV**2.

J/PSI leptoproduction differential cross section as a function of COS(THETA*). for the Z range 0.75 to 0.9.

J/PSI leptoproduction differential cross section as a function of COS(THETA*) in the Q**2 range 2 to 6.5 GeV**2.

J/PSI leptoproduction differential cross section as a function of COS(THETA*) in the Q**2 range 6.5 to 100 GeV**2.

The inelastic J/PSI production cross section as a function of PT**2.

Low Z inelastic J/PSI cross section as a function of W.

Low Z inelastic J/PSI cross section as a function of PT**2.

Inelastic J/PSI cross section for the full Z range. The data come from two different data sets with the points at Z = 0.38 being statistically correlated.