The fraction of the direct photon component as a function of $p_T$.

The fraction of the direct photon component as a function of $p_T$.

Invariant yield (Au+Au) of direct photons as a function of $p_T$.

Invariant yield (Au+Au) of direct photons as a function of $p_T$.

Invariant yield (Au+Au) of direct photons as a function of $p_T$.

Invariant cross section ($p$+$p$) of direct photons as a function of $p_T$.

Per-trigger yield versus $\Delta\phi$ for various trigger and partner $p_T$ ($p^a_T \otimes p^b_T$), arranged by increasing pair proxy energy (sum of $p^a_T$ and $p^b_T$), in Au + Au collisions for 5-10 $\otimes$ 2-3, 4-5 $\otimes$ 4-5, 5-10 $\otimes$ 3-5, and 5-10 $\otimes$ 5-10 GeV/c.

RHS versus $p^b_T$ for p + p collisions for four trigger selections.

RHS versus $p^b_T$ for Au + Au collisions for four trigger selections.

RHS versus $N_{part}$ for 2-3 $\otimes$ 2-3 GeV/$c$. Shaded bars (brackets) represent $p_T$ -correlated uncertainties due to elliptic flow (ZYAM procedure). The most left point is from p+p.

Per-trigger yield $\Delta\phi$ distribution and corresponding fits for 2-3 $\otimes$ 2-3 GeV/c in 0-5% Au+Au collisions.

a) D versus centrality from FIT 1 and FIT2 for 2 - 3 GeV/$c$ bin. The error bars are the statistical errors; The shaded bars and brackets are the systematic errors due to $v_2$. b) The fraction of the shoulder Gaussian yield relative to the total away-side yield as function of centrality determined from FIT2.

Values of D determined from FIT1 as function of partner $p_T$ for 2-3 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT1 as function of partner $p_T$ for 3-4 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT1 as function of partner $p_T$ for 4-5 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT2 as function of partner $p_T$ for 2-3 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT2 as function of partner $p_T$ for 3-4 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT2 as function of partner $p_T$ for 4-5 GeV/c $p_T$ range in 0-20% Au+Au.

Per-trigger yield as function of partner $p_T$ for the HR region for the 0-20% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the HR region for the 20-40% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the HR region for the 40-60% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the HR region for the 60-92% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the HR region for the p + p collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the 0-20% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the 20-40% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the 40-60% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the 60-92% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the p + p collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Near-side Gaussian widths versus partner $p_T$ for four trigger $p_T$ ranges for 0-20 % Au + Au.

Near-side Gaussian widths versus partner $p_T$ for four trigger $p_T$ ranges for 0-20 % p + p.

Near-side Gaussian widths versus $N_{part}$ for five successively increasing $p^a_T$ $\otimes$ $p^b_T$. The most left point in each panel represents the value from p + p.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% p + p.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% Au + Au.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% Au + Au.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% Au + Au.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% Au + Au.

Per-trigger yield versus $\Delta\eta$ for 0-20% central Au + Au collisions. Results are shown for four $p^a_T \otimes p^b_T$ selections as indicated.

Per-trigger yield versus $\Delta\eta$ for 0-20% central p + p collisions. Results are shown for four $p^a_T \otimes p^b_T$ selections as indicated.

The projection of 2-D per-trigger yield in $\lvert \Delta\eta \rvert$ < 0.7 $\otimes$ $\lvert \Delta\phi \rvert$ < 0.7 and 0-20% central Au+Au collisions onto $\Delta\eta$ for four $p^a_T \otimes p^b_T$ selections.

The projection of 2-D per-trigger yield in $\lvert \Delta\eta \rvert$ < 0.7 $\otimes$ $\lvert \Delta\phi \rvert$ < 0.7 and 0-20% central Au+Au collisions onto $\Delta\phi$ for four $p^a_T \otimes p^b_T$ selections.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the head region for Au + Au for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the away-side shoulder region for Au + Au for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the near-side region for Au + Au for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the head region for p + p for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the away-side shoulder region for p + p for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the near-side region for p + p for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, calculated for five partner pT ranges in the HR. Results for triggers in 3-4 GeV/c.

Truncated mean $p_T$, $\langle p_T \rangle$, calculated for five partner pT ranges in the HR. Results for triggers in 4-5 GeV/c.

Truncated mean $p_T$, $\langle p_T \rangle$, calculated for five partner pT ranges in the HR. Results for triggers in 3-4 GeV/c.

Truncated mean $p_T$, $\langle p_T \rangle$, calculated for five partner pT ranges in the HR. Results for triggers in 4-5 GeV/c.

The near-side pair suppression factor $J_{AA}$ in 0-20% Au + Au collisions as function of $p^b_T$ for various ranges of $p^a_T$.

The near-side $J_{AA}$ as function of $p^b_T$ and $p^{sum}_T$ for four $p^a_T$ bins and three centrality bins. Data for 20-40%.

The near-side $J_{AA}$ as function of $p^b_T$ and $p^{sum}_T$ for four $p^a_T$ bins and three centrality bins. Data for 40-60%.

The near-side $J_{AA}$ as function of $p^b_T$ and $p^{sum}_T$ for four $p^a_T$ bins and three centrality bins. Data for 60-92%.

The pair suppression factor $J_{AA}$ for the away-side HR in 0-20% Au + Au collisions as function of $p_b^T$ for various ranges of $p_a^T$.

The pair suppression factor $J_{AA}$ for the away-side HR in 20-40% Au + Au collisions as function of $p_b^T$ for various ranges of $p_a^T$.

The pair suppression factor $J_{AA}$ for the away-side HR in 40-60% Au + Au collisions as function of $p_b^T$ for various ranges of $p_a^T$.

The pair suppression factor $J_{AA}$ for the away-side HR in 60-92% Au + Au collisions as function of $p_b^T$ for various ranges of $p_a^T$.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in 0-20 % Au + Au collisions.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in 20-40 % Au + Au collisions.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in 40-60 % Au + Au collisions.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in 60-92 % Au + Au collisions.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in p + p collisions.

$\pi^0$ invariant yields for different centralities. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

$\pi^0$ invariant yields for different centralities. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

$\pi^0$ $R_{AA}$ for the most central (0-5%) Au+Au collisions and PQM model calculations for different values of $<\bar{q}>$. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Integrated nuclear modification factor ($R_{AA}$) for $\pi^0$ as a function of collision centrality.

Experimental correlation moments $R^2_{x2}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^2_{x2}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^2_{y2}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^2_{y2}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x6}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x6}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{y6}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{y6}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{x2y2}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{x2y2}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{x4}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{x}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{y4}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{y4}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x2y4}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x2y4}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x4y2}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x4y2}(q)$ Fit. Systematic errors are less than the statistical errors.

Source function profile $S(r_x)$ Image in the PCMS.

Source function profile $S(r_x)$ Fit in the PCMS. The blue line represents the Hump fit.

Source function profile $S(r_y)$ Image in the PCMS.

Source function profile $S(r_y)$ Fit in the PCMS. The blue line represents the Hump fit.

Source function profile $S(r_z)$ Image in the PCMS.

Source function profile $S(r_z)$ Fit in the PCMS. The blue line represents the Hump fit.

Associated correlation profile $C(q_x)$ Image in the PCMS.

Associated correlation profile $C(q_x)$ Fit in the PCMS.

Associated correlation profile $C(q_y)$ Image in the PCMS.

Associated correlation profile $C(q_y)$ Fit in the PCMS.

Associated correlation profile $C(q_z)$ Image in the PCMS.

Associated correlation profile $C(q_z)$ Fit in the PCMS.

Source function comparison between Therminator calculation and image for $S(r_x)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_x)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_y)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_y)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_z)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_z)$ in PCMS.

$\Delta$$t_{LCM}$ from Therminator events compared with various assumptions for $\Delta\tau$ and resonance emissions.

$\Delta$$t_{LCM}$ from Therminator events compared with various assumptions for $\Delta\tau$ and resonance emissions.

<p>Jet-pair distributions for associated baryons for $1 < p_{T,assoc} < 1.3\ \mathrm{GeV}/c$ and $1.6 < p_{T,assoc} < 2.0\ \mathrm{GeV}/c$. Results are for a hadron trigger $2.5 < p_T < 4.0\ \mathrm{GeV}/c$ and centrality selections of 0-20% and 20-40%.</p> <p><i>Note that only statistical uncertainties are available.</i></p>

<p>Conditional jet yeilds for associated mesons for near-side jets.</p> <p><i>Note that only statistical uncertainties are available.</i></p>

<p>Conditional jet yeilds for associated mesons for away-side jets.</p> <p><i>Note that only statistical uncertainties are available.</i></p>

<p>Conditional jet yeilds for associated baryons for near-side jets.</p> <p><i>Note that only statistical uncertainties are available.</i></p>

<p>Conditional jet yeilds for associated baryons for away-side jets.</p> <p><i>Note that only statistical uncertainties are available.</i></p>

<p>Ratio of jet-associated baryons to jet-associated mesons for near-side jets.</p> <p><i>Note that only statistical uncertainties are available.</i></p>

<p>Ratio of jet-associated baryons to jet-associated mesons for away-side jets.</p> <p><i>Note that only statistical uncertainties are available.</i></p>

J/PSI invariant (1/(2PI*PT))*D2(N)/DPT/DYRAP versus PT at mid rapidity (-0.35<y<0.35) in D+AU collisions.

J/PSI invariant (1/(2PI*PT))*D2(N)/DPT/DYRAP versus PT at forward rapidity (1.2<y<2.2) in D+AU collisions.

J/PSI invariant (1/(2PI*PT))*D2(N)/DPT/DYRAP versus centrality at backward rapidity (-2.2<y<-1.2) in D+AU collisions.

J/PSI invariant (1/(2PI*PT))*D2(N)/DPT/DYRAP versus centrality at mid rapidity (-0.35<y<0.35) in D+AU collisions.

J/PSI invariant (1/(2PI*PT))*D2(N)/DPT/DYRAP versus centrality at forward rapidity (1.2<y<2.2) in D+AU collisions.

Nuclear modification factor versus rapidity in D+AU collisions, over 3 bins of rapidity.

Nuclear modification factor versus rapidity in D+AU collisions, over 5 bins of rapidity.

Nuclear modification factor versus PT at backward rapidity (-2.2<y<-1.2) in D+AU collisions.

Nuclear modification factor versus PT at mid rapidity (-0.35<y<0.35) in D+AU collisions.

Nuclear modification factor versus PT at forward rapidity (1.2<y<2.2) in D+AU collisions.

Nuclear modification factor versus centrality at backward rapidity (-2.2<y<-1.2) in D+AU collisions.

Nuclear modification factor versus centrality at mid rapidity (-0.35<y<0.35) in D+AU collisions.

Nuclear modification factor versus centrality at forward rapidity (1.2<y<2.2) in D+AU collisions.

Mean PT^2 versus rapidity, extracted from a fit to the data, for DEUT + Au reactions. The mean value of PT^2 is calculated from the data for PT < 5 Gev/c.

Mean PT^2 versus rapidity, extracted from a fit to the data, for P + P reactions. The mean value of PT^2 is calculated from the data for PT < 5 Gev/c.

Breakup cross section of c-c_bar pairs inside cold nuclear matter,integrated over the whole domain of rapidity.The breakup cross section is calculated with two models of shadowing for nuclear PDFs ; the EKS model and the NDSG model. The uncertainties given, containing statistical and systematical error, are corresponding to one standard deviation.

Breakup cross section of c-c_bar pairs inside cold nuclear matter for different ranges of rapidity.The breakup cross section is calculated with two models of shadowing for nuclear PDFs ; the EKS model and the NDSG model. The uncertainties given, containing statistical and systematical error, are corresponding to one standard deviation.

Breakup cross section of c-c_bar pairs inside cold nuclear matter, integrated over the whole domain of rapidity.The breakup cross section is calculated with two models of shadowing for nuclear PDFs ; the EKS model and the NDSG model. The uncertainties given, containing statistical and systematical error, are corresponding to one standard deviation.

Breakup cross section of c-c_bar pairs inside cold nuclear matter for different ranges of rapidity.The breakup cross section is calculated with two models of shadowing for nuclear PDFs ; the EKS model and the NDSG model. The uncertainties given, containing statistical and systematical error, are corresponding to one standard deviation.

The cross section for E+ E- --> ETA K+ K- excluding the contribution from PHI --> K+ K- with statistical errors only.

The cross section for E+ E- --> PHI ETA with statistical errors only.

Isoscalar (I=0) component of the cross section for E+ E- --> K*(892) K with statistical errors only.

Isovector (I=1) component of the cross section for E+ E- --> K*(892) K with statistical errors only.

Isoscalar (I=0) component of the cross section for E+ E- --> K2*(1430) K with statistical errors only.

Isovector (I=1) component of the cross section for E+ E- --> K2*(1430) K with statistical errors only.