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.

Measured cross sections for Z0 production.

Ratios of W to Z cross sections.

Ratios of W+ to W- cross sections.

Measured cross sections in the restricted fiducial and kinematic acceptance for W and Z production in the electron decay channel.

Measured cross sections in the restricted fiducial and kinematic acceptance for W production in the muon decay channel.

Measured cross sections in the restricted fiducial and kinematic acceptance for Z production in the muon decay channel.

$\bar{\Lambda}$ to $K^{0}_{s}$ production ratio in $pp$ collisions at 900 GeV in $y$ intervals for ($0.25 < p_T < 0.65$), ($0.65 < p_T < 1.00$), ($1.00 < p_T < 2.50$) GeV$/c$.

Lambdabar over Lambda @ 900 GeV (0.25 < pT < 2.5) GeV/c in y intervals.

$\bar{\Lambda}$ to $\Lambda$ production ratio in $pp$ collisions at 900 GeV ($0.25 < p_T < 2.50$ GeV$/c$) in $y$ intervals.

Lambdabar over K0s @ 900 Gev (0.25 < pT < 2.5 GeV/c) in y intervals.

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

Lambdabar over Lambda @ 900 Gev for (2.0 < y < 4.0) in intervals of pT.

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

Lambdabar over K0s @ 900 Gev for (2.0 < y < 4.0) in intervals of pT.

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

Lambdabar over K0s @ 900 Gev for (2.0 < y < 4.0) in intervals of pT.

$\bar{\Lambda}$ 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.

Lambdabar over K0s @ 900 Gev for (2.0 < y < 4.0) in intervals of pT.

$\bar{\Lambda}$ 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.

Lambdabar over Lambda @ 7TeV in y interals for (0.15<PT<0.65),(0.65<PT<1.00),(1.00<PT<2.50) GeV/c.

$\bar{\Lambda}$ 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$/c$.

Lambdabar over K0s @ 7TeV in y interals for (0.15<PT<0.65),(0.65<PT<1.00),(1.00<PT<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$/c$.

Lambdabar over Lambda @ 7 TeV (0.15 < pT < 2.5) GeV/c in y intervals.

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

Lambdabar over K0s @ 7 TeV (0.15 < pT < 2.5) 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.

Lambdabar over Lambda @ 7 Tev for (2.0 < y < 4.5) in pT intervals.

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

Lambdabar over K0s @ 7 Tev for (2.0 < y < 4.5) in pT 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.

Lambdabar over K0s @ 7 Tev for (2.0 < y < 4.5) in pT 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.

Lambdabar over K0s @ 7 Tev for (2.0 < y < 4.5) in pT 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.

$\rho^0$ production cross section determined with the data set collected with trigger B, as a function of momentum transfer $t$, fitted with a double exponential fit function in the range $t < 0.1$. The statistical errors are shown. The ratio of incoherent to coherent cross sections is measured to be $0.20 \pm 0.8$. The fit parameters are shown in Table I.

Comparison of theoretical predictions to the measured total cross section for coherent $\rho^0$ production as a functionof $\sqrt{s_{NN}}$ . The measured cross section is based on the dataset collected with trigger B. The error bars show the sum of the statistical and systematic uncertainties. See text for details.

Fully corrected average charged particle scalar PT Sum per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 0.9 TeV.

Fully corrected average charged particle scalar PT Sum per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 7 TeV.

Ratio of the fully corrected average charged particle scalar PT Sum at 7 TeV to that at 0.9 TeV.

Normalized multiplicity distribution of charged particles produced in proton-proton collisions at a center-of-mass energy of 0.9 TeV with the leading track-jet transverse momentum > 3 GeV.

Normalized multiplicity distribution of charged particles produced in proton-proton collisions at a center-of-mass energy of 7 TeV with the leading track-jet transverse momentum > 3 GeV.

Normalized multiplicity distribution of charged particles produced in proton-proton collisions at a center-of-mass energy of 7 TeV with the leading track-jet transverse momentum > 20 GeV.

Normalized scalar PT Sum distribution of charged particles produced in proton-proton collisions at a center-of-mass energy of 0.9 TeV with the leading track-jet transverse momentum > 3 GeV.

Normalized scalar PT Sum distribution of charged particles produced in proton-proton collisions at a center-of-mass energy of 7 TeV with the leading track-jet transverse momentum > 3 GeV.

Normalized scalar PT Sum distribution of charged particles produced in proton-proton collisions at a center-of-mass energy of 7 TeV with the leading track-jet transverse momentum > 20 GeV.

PT distribution of charged particles produced in proton-proton collisions at a center-of-mass energy of 0.9 TeV with the leading track-jet transverse momentum > 3 GeV.

PT distribution of charged particles produced in proton-proton collisions at a center-of-mass energy of 7 TeV with the leading track-jet transverse momentum > 3 GeV.

PT distribution of charged particles produced in proton-proton collisions at a center-of-mass energy of 7 TeV with the leading track-jet transverse momentum > 20 GeV.

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).