Nuclear modicifation factor vs. N_coll $J\psi$ with|y|<1 and pT < 3 GeV/c in d Au collisions.

The invariant cross section versus transverse momentum for J/$\psi$ with $|y|\lt 1$ in $p+p$ collisions.

The invariant yield versus transverse momentum for $J/\Psi$ with |y| < 1 in 0 - 100 percent central d+Au collisions.

The $V_2${2} and difference between the pairs at ($\eta_{\alpha}$, $\eta_{\beta}$) and ($\eta_{\alpha}$, -$\eta_{\beta}$). The data are from 20-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $V_2${2} and difference between the pairs at ($\eta_{\alpha}$, $\eta_{\beta}$) and ($\eta_{\alpha}$, -$\eta_{\beta}$). The data are from 20-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $V_2${2} and difference between the pairs at ($\eta_{\alpha}$, $\eta_{\beta}$) and ($\eta_{\alpha}$, -$\eta_{\beta}$). The data are from 20-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $V_2${2} and difference between the pairs at ($\eta_{\alpha}$, $\eta_{\beta}$) and ($\eta_{\alpha}$, -$\eta_{\beta}$). The data are from 20-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $V_3${2} and difference between the pairs at ($\eta_{\alpha}$, $\eta_{\beta}$) and ($\eta_{\alpha}$, -$\eta_{\beta}$). The data are from 20-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $V_3${2} and difference between the pairs at ($\eta_{\alpha}$, $\eta_{\beta}$) and ($\eta_{\alpha}$, -$\eta_{\beta}$). The data are from 20-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $V_3${2} and difference between the pairs at ($\eta_{\alpha}$, $\eta_{\beta}$) and ($\eta_{\alpha}$, -$\eta_{\beta}$). The data are from 20-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $V_3${2} and difference between the pairs at ($\eta_{\alpha}$, $\eta_{\beta}$) and ($\eta_{\alpha}$, -$\eta_{\beta}$). The data are from 20-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $V_2^{1/2}$ difference between quadruplets at ($\eta_{\alpha}$, $\eta_{\alpha}$, $\eta_{\beta}$, $\eta_{\beta}$) and ($\eta_{\alpha}$, $\eta_{\alpha}$, -$\eta_{\beta}$, -$\eta_{\beta}$).

The two-particle cumulants, V2{2} as a function of $\eta$ for one particle while averaged over $\eta$ of the partner particle.

The two-particle cumulants, V2{2} as a function of $\eta$.

The two-particle cumulants, V2{2} as a function of $\eta$ for one particle while averaged over $\eta$ of the partner particle.

The difference in two-particle cumulants, V2{2} as a function of $\eta$ for one particle while averaged over $\eta$ of the partner particle.

No description provided.

V3{2} as a function of $\eta$.

<$V_3^2$> as a function of $\eta$.

The $\Delta\eta$-dependent component of the two-particle cumulant with $\Delta\eta$-gap, $D^-$ in Eq. (11), of the second harmonic is shown as a function of ??-gap |$\Delta\eta$| > x.

The $\Delta\eta$-dependent component of the two-particle cumulant with $\Delta\eta$-gap, $D^-$ in Eq. (11), of the third harmonic is shown as a function of ??-gap |$\Delta\eta$| > x.

The nonflow, $\sqrt{\bar{D}_2}$, $\sqrt{\delta_2}$, $\sqrt{\bar{D}_3}$ and flow, $\sqrt{v_2^2/2}$, $\sqrt{<v_2^2>}$ results are shown as a function of centrality percentile for the second harmonic.

The nonflow, $\sqrt{\bar{D}_2}$, $\sqrt{\delta_2}$, $\sqrt{\bar{D}_3}$ and flow, $\sqrt{v_2^2/2}$, $\sqrt{<v_2^2>}$ results are shown as a function of centrality percentile for the second harmonic.

The nonflow, $\sqrt{\bar{D}_2}$, $\sqrt{\delta_2}$, $sqrt{\bar{D}_3}$ and flow, $\sqrt{v_2^2/2}$, $\sqrt{<v_2^2>}$ results are shown as a function of centrality percentile for the second harmonic.

The nonflow, $\sqrt{\bar{D}_2}$, $\sqrt{\delta_2}$, $sqrt{\bar{D}_3}$ and flow, $\sqrt{v_2^2/2}$, $\sqrt{<v_2^2>}$ results are shown as a function of centrality percentile for the third harmonic.

The nonflow, $\sqrt{\bar{D}_2}$, $sqrt{\delta_2}$, $\sqrt{\bar{D}_3}$ and flow, $\sqrt{v_2^2/2}$, $\sqrt{<v_2^2>}$ results are shown as a function of centrality percentile for the third harmonic.

The relative elliptic flow fluctuation $\sigma_2/<v_2>$ centrality dependence in $\sqrt{s_{NN}}$ = 200 GeV Au+Au collisions.

Inclusive J/psi production cross-section as a function of J/psi pT in the J/psi rapidity (|y|) bin 1.5<|y|<2. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Inclusive J/psi production cross-section as a function of J/psi pT in the J/psi rapidity (|y|) bin 0.75<|y|<1.5. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Inclusive J/psi production cross-section as a function of J/psi pT in the J/psi rapidity (|y|) bin |y|<0.75. The first uncertainty is statistical, the second is systematic and the third encapsulates any possible variation due to spin-alignment from the unpolarised central value.

Non-prompt to inclusive production cross-section fraction fB as a function of J/psi pT for J/psi rapidity |y|<0.75 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0). The spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses, plus the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic, the third number is the uncertainty due to spin-alignment.}.

Non-prompt to inclusive production cross-section fraction fB as a function of J/psi pT for J/psi rapidity 0.75<|y|<1.5 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0). The spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses, plus the range of non-prompt cross-sections within lambda_theta = +/-0.1. The first uncertainty is statistical, the second uncertainty is systematic, the third number is the uncertainty due to spin-alignment.

Non-prompt to inclusive production cross-section fraction fB as a function of J/psi pT for J/psi rapidity 1.5<|y|<2 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0). The spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses, plus the range of non-prompt cross-sections within lambda_theta = +/-0.1. The first uncertainty is statistical, the second uncertainty is systematic, the third number is the uncertainty due to spin-alignment.

Non-prompt to inclusive production cross-section fraction fB as a function of J/psi pT for J/psi rapidity 2<|y|<2.4 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0). The spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses, plus the range of non-prompt cross-sections within lambda_theta =+/-0.1. The first uncertainty is statistical, the second uncertainty is systematic, the third number is the uncertainty due to spin-alignment.

Non-prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity |y|<0.75 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0), and the spin-alignment envelope spans the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic. Comparison is made to FONLL predictions.

Non-prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 0.75<|y|<1.5 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0), and the spin-alignment envelope spans the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic. Comparison is made to FONLL predictions.

Non-prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 1.5<|y|<2 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0), and the spin-alignment envelope spans the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic. Comparison is made to FONLL predictions.

Non-prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 2<|y|<2.4 under the assumption that prompt and non-prompt J/psi production is unpolarised (lambda_theta = 0), and the spin-alignment envelope spans the range of non-prompt cross-sections within lambda_theta = +/- 0.1. The first uncertainty is statistical, the second uncertainty is systematic. Comparison is made to FONLL predictions.

Prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity |y|<0.75. The central value assumes unpolarised (lambda_theta = 0) prompt and non-prompt production, and the spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses. The first quoted uncertainty is statistical, the second uncertainty is systematic. Comparison is made to the Colour Evaporation Model prediction.

Prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 0.75<|y|<1.5. The central value assumes unpolarised (lambda_theta = 0) prompt and non-prompt production, and the spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses. The first quoted uncertainty is statistical, the second uncertainty is systematic. Comparison is made to the Colour Evaporation Model prediction.

Prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 1.5<|y|<2. The central value assumes unpolarised (lambda_theta = 0) prompt and non-prompt production, and the spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses. The first quoted uncertainty is statistical, the second uncertainty is systematic. Comparison is made to the Colour Evaporation Model prediction.

Prompt J/psi production cross-sections as a function of J/psi pT for J/psi rapidity 2<|y|<2.4. The central value assumes unpolarised (lambda_theta = 0) prompt and non-prompt production, and the spin-alignment envelope spans the range of possible prompt cross-sections under various polarisation hypotheses. The first quoted uncertainty is statistical, the second uncertainty is systematic. Comparison is made to the Colour Evaporation Model prediction.

Unweighted J/psi candidate yields in bins of $J/psi transverse momentum and rapidity. Uncertainties are statistical only.

Summary table of all sources of considered systematic uncertainty and statistical uncertainty (as a percentage) on the corrected inclusive J/psi production cross-section, for absolute J/psi rapidities within 2<|y|<2.4. The sources of systematic error shown are, in order, Acceptance, Muon recognition, Trigger, Fitting and the Total systematics. Also shown in the last error is the possible envelope of variation the central result due to uncertainty on spin-alignment of the J\psi.

Summary table of all sources of considered systematic uncertainty and statistical uncertainty (as a percentage) on the corrected inclusive J/psi production cross-section, for absolute J/psi rapidities within 1.5<|y|<2. The sources of systematic error shown are, in order, Acceptance, Muon recognition, Trigger, Fitting and the Total systematics. Also shown in the last error is the possible envelope of variation the central result due to uncertainty on spin-alignment of the J/psi.

Summary table of all sources of considered systematic uncertainty and statistical uncertainty (as a percentage) on the corrected inclusive J/psi production cross-section, for absolute J/psi rapidities within 0.75<|y|<1.5. The sources of systematic error shown are, in order, Acceptance, Muon recognition, Trigger, Fitting and the Total systematics. Also shown in the last error is the possible envelope of variation the central result due to uncertainty on spin-alignment of the J/psi.

Summary table of all sources of considered systematic uncertainty and statistical uncertainty (as a percentage) on the corrected inclusive J/psi production cross-section, for absolute rapidities within |y|<0.75. The sources of systematic error shown are, in order, Acceptance, Muon recognition, Trigger, Fitting and the Total systematics. Also shown in the last error is the possible envelope of variation the central result due to uncertainty on spin-alignment of the J/psi.

Breakdown of sources of systematic uncertainty on the non-prompt J/psi fraction measurements, for the bin |y|<0.75, as a function of the J/psi pT.

Breakdown of sources of systematic uncertainty on the non-prompt J/psi fraction measurements, for the bin 0.75<|y|<1.5, as a function of the J/psi pT.

Breakdown of sources of systematic uncertainty on the non-prompt J/psi fraction measurements, for the bin 1.75<|y|<2.0, as a function of the J/psi pT.

Breakdown of sources of systematic uncertainty on the non-prompt J/psi fraction measurements, for the bin 2.0<|y|<2.4, as a function of the J/psi pT.

The observed 95% CL upper limits on the cross section for p p --> zprime x BR(zprime -> e-mu) as a function of the zprime mass.

The measured cross section ratio for W+jets in the muon channel as a function of corrected jet multiplicity.

The cross section times branching ratio for W+jets in the electron channel as a function of the leading jet PT.

The cross section times branching ratio for W+jets in the muon channel as a function of the leading jet PT.

The cross section times branching ratio for W+jets in the electron channel as a function of the next-to-leading jet PT.

The cross section times branching ratio for W+jets in the muon channel as a function of the next-to-leading jet PT.

Nuclear modification factor $R_{dA}$ for $\pi^0$, d + Au, compared to the STAR $\pi^{+-}$ [23,24] and PHENIX $\pi^0$ measurements [27,28]. Nucleon-nucleon inelastic cross section $\sigma^{NN}$ = 42 mb and expected number of collisions $<N_{coll}>$ = 7.5 +- 0.4 from Glauber model. Shaded bands in plot are $p_T$-correlated systematic uncertainties and the error bars are statistical uncertainties. Normalization uncertainty of 14.0% indicated by a shaded band around unity.

Nuclear modification factor $R_{dA}$ for eta, d + Au, compared to PHENIX $\eta$ measurements [27,28]. Nucleon-nucleon inelastic cross section $\sigma^{NN}$ = 42 mb and expected number of collisions $<N_{coll}>$ = 7.5 +- 0.4 from Glauber model. Shaded bands in plot are $p_T$-correlated systematic uncertainties and the error bars are statistical uncertainties. Normalization uncertainty of 14.0% indicated by a shaded band around unity.

Nuclear modification factor $R_{CP}$ for $\pi^0$ measured in d + Au collisions, compared to STAR $\pi^{+-}$ measurements [24]. Peripheral d + Au collisions were used where $R_{CP}$ = ratio of particle production in 40-100% centrality (P) events and 0-20% centrality (C) events. Shaded bands in plot are $p_T$-correlated systematic uncertainties and the error bars are statistical uncertainties. Normalization uncertainty of 11.0% indicated by a shaded band around unity.

Direct photon yield in p + p collisions at $\sqrt{s_{NN}}$ = 200 GeV in terms of the double ration $R_{\gamma}$. Shaded bands in plot are $p_T$-correlated systematic uncertainties and the error bars are statistical uncertainties. The curves correspond to NLO pQCD calculations of the differential cross sections for direct photon [68] and $\pi^0$ [52] production in p + p collisions for different factorization scales $\mu$ (the upper pQCD curve corresponds to $\mu$ = $p_T$/2). The upper limit of the fractional neutral hadron contamination $C_0$ is shown as the shaded band at $R_{\gamma}$ = 0.

Direct photon yield in d + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV in terms of the double ration $R_{\gamma}$. Shaded bands in plot are $p_T$-correlated systematic uncertainties and the error bars are statistical uncertainties. The curves correspond to NLO pQCD calculations of the differential cross sections for direct photon [68] and $\pi^0$ [52] production in p + p collisions for different factorization scales $\mu$ (the upper pQCD curve corresponds to $\mu$ = $p_T$/2). The upper limit of the fractional neutral hadron contamination $C_0$ is shown as the shaded band at $R_{\gamma}$ = 0.

Cross sections for direct photon production at midrapidity in p + p and d + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV, compared to the PHENIX measurement [29] and to the NLO pQCD calculation [68], which was scaled with $<T_{dA}>$ [Eq. (23)] in case of d + Au collisions. The error bars are statistical the shaded bands are $p_T$-correlated systematic uncertainties. The arrows correspond to the 95% confidence limits, as defined in the text. Normalization uncertainties of 11.7% for p+p and 5.3% for d+Au are not shown. Separate columns in the table show upper 95% confidence limits. The 95% confidence limits for the cross section are used when $R_{\gamma}$ did not correspond to a significant direct photon signal, assuming that the statistical and systematic errors both followed a Gaussian distribution, and using the fact that $R_{\gamma}\geq 1$ by definition.