Inclusive differential PHI production cross section as a function of PT in the rapidity ranges 3.16-3.34 and 3.34-3.52.

Inclusive differential PHI production cross section as a function of PT in the rapidity ranges 3.52-3.70 and 3.70-3.88.

Inclusive differential PHI production cross section as a function of PT in the rapidity range 3.88-4.06.

Inclusive differential PHI production cross section as a function of PT over the rapidity range 2.44-4.06.

Inclusive differential PHI production cross section as a function of rapidity over the PT range 0.6 to 5.0.

$\bar{\Lambda}$ over $K^{0}_{s}$ production ratio in $pp$ collisions at 900 Gev ($0.25 < p_T < 2.50$ GeV$/c$) in $y$ intervals.

$\bar{\Lambda}$ to $\Lambda$ production ratio in $pp$ collisions at 900 Gev for $2.0 < y < 4.0$ in intervals of $p_T$.

$\bar{\Lambda}$ to $K^{0}_{s}$ production ratio in $pp$ collisions at 900 Gev for $2.0 < y < 4.0$ in intervals of $p_T$.

$\bar{\Lambda}$ to $K^{0}_{s}$ production ratio in $pp$ collisions at 900 Gev ($2.0 < y < 4.0$; $0.25 < p_T < 2.50$ GeV$/c$) in rapidity loss intervals.

$\bar{\Lambda}$ to $K^{0}_{s}$ production ratio in $pp$ collisions at 900 Gev ($2.0 < y < 4.0$; $0.25 < p_T < 2.50$ GeV$/c$) in rapidity loss intervals.

$\bar{\Lambda}$ to $\Lambda$ production ratio in $pp$ collisions at 7 TeV in $y$ intervals for ($0.15 < p_T < 0.65$), ($0.65 < p_T < 1.00$), ($1.00 < p_T < 2.50$) GeV$/c$.

$\bar{\Lambda}$ to $K^{0}_{s}$ production ratio in $pp$ collisions at 7 TeV in $y$ intervals for ($0.15 < p_T < 0.65$), ($0.65 < p_T < 1.00$), ($1.00 < p_T < 2.50$) GeV$/c$.

$\bar{\Lambda}$ to $\Lambda$ production ratio in $pp$ collisions at 7 TeV ($0.15 < p_T < 2.50$ GeV$/c$) in $y$ intervals.

$\bar{\Lambda}$ to $K^{0}_{s}$ production ratio in $pp$ collisions at 7 TeV ($0.15 < p_T < 2.50$ GeV$/c$) in $y$ intervals.

$\bar{\Lambda}$ to $\Lambda$ production ratio in $pp$ collisions at 7 Tev for $2.0 < y < 4.5$ in $p_T$ intervals.

$\bar{\Lambda}$ to $K^{0}_{s}$ production ratio in $pp$ collisions at 7 Tev for $2.0 < y < 4.5$ in $p_T$ intervals.

$\bar{\Lambda}$ to $\Lambda$ production ratio in $pp$ collisions at 7 Tev ($2.0 < y < 4.5$; $0.15 < p_T < 2.50$ GeV$/c$) in rapidity loss intervals.

$\bar{\Lambda}$ to $K^{0}_{s}$ production ratio in $pp$ collisions at 7 Tev ($2.0 < y < 4.5$; $0.15 < p_T < 2.50$ GeV$/c$) in rapidity loss intervals.

$\Omega + \bar{\Omega}$ invariant mass spectra from Cu+Cu $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The uncertainties on the spectra points are statistical and systematic combined.

$K^0_S$ invariant mass spectra from Au+Au $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The uncertainties on the spectra points are statistical and systematic combined.

$\Lambda$ and $\bar{\Lambda}$ invariant mass spectra from Au+Au $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The $\Lambda$ and $\bar{\Lambda}$ yields have not been feed down subtracted from weak decays. The uncertainties on the spectra points are statistical and systematic combined.

$K^0_S$, $\Lambda$, and $\bar{\Lambda}$, spectra divided by $\langle N_{part} \rangle$ for Cu+Cu $0 − 10\%$ ($\langle N_{part} \rangle \sim 99$) and Au+Au $20 − 40\%$ ($\langle N_{part} \rangle \sim 141$) $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The $\Lambda$ and $\bar{\Lambda}$ yields have been feed down subtracted from weak decays. The uncertainties on the spectra points are statistical and systematic; for clarity the uncertainty on $\langle N_{part} \rangle$ has not been included. The curves show the functions described in the text used to extract $dN/dy$.

$\Xi + \bar{\Xi}$ spectra divided by $\langle N_{part} \rangle$ for Cu+Cu $0 − 10\%$ ($\langle N_{part} \rangle \sim 99$) $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The uncertainties on the spectra points are statistical and systematic; for clarity the uncertainty on $\langle N_{part} \rangle$ has not been included. The curves show the functions described in the text used to extract $dN/dy$.

$\Xi + \bar{\Xi}$ spectra divided by $\langle N_{part} \rangle$ for Au+Au $20 − 40\%$ ($\langle N_{part} \rangle \sim 141$) $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The uncertainties on the spectra points are statistical and systematic; for clarity the uncertainty on $\langle N_{part} \rangle$ has not been included. The curves show the functions described in the text used to extract $dN/dy$.

$\Omega + \bar{\Omega}$ spectra divided by $\langle N_{part} \rangle$ for Cu+Cu $0 − 10\%$ ($\langle N_{part} \rangle \sim 99$) $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The uncertainties on the spectra points are statistical and systematic; for clarity the uncertainty on $\langle N_{part} \rangle$ has not been included. The curves show the functions described in the text used to extract $dN/dy$.

$\Omega + \bar{\Omega}$ spectra divided by $\langle N_{part} \rangle$ for Au+Au $20 − 40\%$ ($\langle N_{part} \rangle \sim 141$) $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The uncertainties on the spectra points are statistical and systematic; for clarity the uncertainty on $\langle N_{part} \rangle$ has not been included. The curves show the functions described in the text used to extract $dN/dy$.

The enhancement factor for (multi-) strange particles in Cu+Cu $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The $\Lambda$, and $\bar{\Lambda}$ yields have been feed-down subtracted in all cases. The black bars show the normalization uncertainties, and the uncertainties for the heavy-ion points are the combined statistical and systematic errors. Curves described in the text, where $B_{K} = 2.0$, $B_{\Lambda} = 2.4$, $B_{\Xi} = 5.0$ and $B_{\Omega} = 12.1$.

The enhancement factor for (multi-) strange particles in Au+Au $\sqrt{s_{NN}} = 200$ GeV collisions, where $|y| < 0.5$. The $\Lambda$, and $\bar{\Lambda}$ yields have been feed-down subtracted in all cases. The black bars show the normalization uncertainties, and the uncertainties for the heavy-ion points are the combined statistical and systematic errors. Curves described in the text, where $B_{K} = 2.0$, $B_{\Lambda} = 2.4$, $B_{\Xi} = 5.0$ and $B_{\Omega} = 12.1$.

Ratio of particle yields in central Cu+Cu and midcentral Au+Au collisions when $\langle N_{part} \rangle = 99$ in each case for $|y| < 0.5$. $\pi$ yields are from elsewhere [17]. Boxed uncertainties are from the Glauber calculations and are correlated for every particle. $\langle N_{part>1} \rangle$ refers to the parameterization shown by eq. 1, while the EPOS and AMPT models are described in the text. The default settings are used for each model. The vertical lines show the remaining independent statistical and systematic uncertainties.

Diphoton production cross section as a function of the diphoton rapidity.

Diphoton production cross section differential in the cosine of the polar angle in the Collins-Soper frame.

Diphoton production cross section differential in the sub-leading to leading photon transverse momentum ratio (z).

Cross section measurements for the reaction E+ E- --> PHI F0(980). Statistical errors only.

Cross section measurements for the reaction E+ E- --> PHI F0(600). Statistical errors only.

Cross section measurements for the reaction E+ E- --> K+ K- PI0 PI0. Statistical errors only.

Cross section measurements for the reaction E+ E- --> PHI F0(980). Statistical errors only.

Cross section measurements for the reaction E+ E- --> K+ K- K+ K-. Statistical errors only.

Cross section as a function of DELTA(PHI) for leading jet transverse momentum > 56 GeV. . The (sys) error in the table is due to the limited MC statistics and is uncorrelated bin-to-bin. The other two systematic errors are correlated.

Cross section as a function of DELTA(PHI) for leading jet transverse momentum > 84 GeV. . The (sys) error in the table is due to the limited MC statistics and is uncorrelated bin-to-bin. The other two systematic errors are correlated.

Cross section as a function of DELTA(PHI) for leading jet transverse momentum > 120 GeV. . The (sys) error in the table is due to the limited MC statistics and is uncorrelated bin-to-bin. The other two systematic errors are correlated.

Normalized dijet angular distribution for the dijet mass range 1100 to 1400 GeV.

Normalized dijet angular distribution for the dijet mass range 850 to 1100 GeV.

Normalized dijet angular distribution for the dijet mass range 650 to 850 GeV.

Normalized dijet angular distribution for the dijet mass range 500 to 650 GeV.

Normalized dijet angular distribution for the dijet mass range 350 to 500 GeV.

Normalized dijet angular distribution for the dijet mass range 250 to 350 GeV.

Distribution of the logarithm of the central thrust minor for events with jet transverse momentum > 30 GeV, jet |pseudorapidity| < 1.3 and leading the jet transverse momentum from 125 to 200 GeV/c,.

Distribution of the logarithm of the central transverse thrust for events with jet transverse momentum > 30 GeV, jet |pseudorapidity| < 1.3 and leading the jet transverse momentum from > 200 GeV/c,.

Distribution of the logarithm of the central thrust minor for events with jet transverse momentum > 30 GeV, jet |pseudorapidity| < 1.3 and leading the jet transverse momentum from > 200 GeV/c,.