$\lambda_{{\rm \overline{p}}{\rm \overline{p}}}+\lambda_{{\rm \overline{p}} \overline{\Lambda}}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$\lambda_{{\rm \overline{p}}{\rm \overline{p}}}+\lambda_{{\rm \overline{p}} \overline{\Lambda}}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$\lambda_{{\rm \overline{p}}{\rm \overline{p}}}+\lambda_{{\rm \overline{p}} \overline{\Lambda}}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$\lambda_{{\rm p}{\rm {p}}}+\lambda_{{\rm {p}}\Lambda}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm {p}}{\rm {p}}$.

$\lambda_{{\rm p}{\rm {p}}}+\lambda_{{\rm {p}}\Lambda}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm {p}}{\rm {p}}$.

$\lambda_{{\rm p}{\rm {p}}}+\lambda_{{\rm {p}}\Lambda}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm {p}}{\rm {p}}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $0-10\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $10-30\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $30-50\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm {p}}{\rm {p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm {p}}{\rm {p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm {p}}{\rm {p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

C2 versus qinv for mixed-charge pions in six kT intervals. 45-50% centrality.

Fit parameters from two-pion correlations. 0-5% and 45-50% centrality. EW = Edgeworth, Gauss=Gaussian.

C3 versus Q3 for same-charge pions in six centrality intervals. Low KT3.

Cummulant c3 versus Q3 for same-charge pions in six centrality intervals. Low KT3.

C3 versus Q3 for same-charge pions in six centrality intervals. High KT3.

Cummulant c3 versus Q3 for same-charge pions in six centrality intervals. High KT3.

C3 versus Q3 for mixed-charge pions in six centrality intervals. Low KT3.

Cummulant c3 versus Q3 for mixed-charge pions in six centrality intervals. Low KT3.

C3 versus Q3 for mixed-charge pions in six centrality intervals. High KT3.

Cummulant c3 versus Q3 for mixed-charge pions in six centrality intervals. High KT3.

r3 for 0-5% centrality.

r3 for 5-10% centrality.

r3 for 10-20% centrality.

r3 for 20-30% centrality.

r3 for 30-40% centrality.

r3 for 40-50% centrality.

Projections of the correlation function C.

Projections of the correlation function C.

Projections of the correlation function C.

Projections of the correlation function C.

Pion HBT radii for the 5% most central collisions.

Pion HBT radii for the 5% most central collisions from the STAR experiment at 200 GeV taken from Adams et al. PR C71(2005)044906.

Ratio of Pion HBT radii for the OUT projection to that for the SIDE projection for the 5% most central collisions.

Ratio of Pion HBT radii for the OUT projection to that for the SIDE projection for the 5% most central collisions from the STAR experiment at 200 GeV taken from Adams et al. PR C71(2005)044906.;.

Pion HBT radii at KT=0.3 for the 5% most central collisions as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

Product of the three HBT radii at KT=0.3 for the 5% most central collisions as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

The decoupling time extracted from R_long(KT) as a function of the central charged multiplicity. Data from other experiments is shown for comparison.