Additional information containing number of events which were used to reconstruct the numvers matching to Figure 1 and 2.

Additional information containing number of events which were used to reconstruct the numvers matching to Figure 1 and 2.

Additional information containing number of events which were used to reconstruct the numvers matching to Figure 1 and 2.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 22.5 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 22.5 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV $p$+$p$ collisions.

The mean from the NBD fit as a function of $N_{part}$ for 200 GeV Au+Au collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The mean from the NBD fit as a function of $N_{part}$ for 62.4 GeV Au+Au collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The mean from the NBD fit as a function of $N_{part}$ for 200 GeV Cu+Cu collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The mean from the NBD fit as a function of $N_{part}$ for 62.4 GeV Cu+Cu collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The mean from the NBD fit as a function of $N_{part}$ for 22.5 GeV Cu+Cu collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of centrality for 200 GeV Au+Au collisions in the range 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 200 GeV Au+Au collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 62.4 GeV Au+Au collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 200 GeV Cu+Cu collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 62.4 GeV Cu+Cu collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 22.5 GeV Cu+Cu collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Scaled variance for 200 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 200 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 200 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 200 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 200 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The scaled variance as a funciton of $N_{part}$ for 200 GeV Au+Au collisions in the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

Measured cross section for the process E+ E- --> QUARK QUARKBAR TAU NEUTRINO.

Measured cross section for the process E+ E- --> QUARK QUARKBAR QUARK QUARKBAR.

Measured value of the QUARK QUARKBAR cross section.

Measured values of the cross section for W+ W- production into the fully leptonic decay mode summed over all lepton modes and assuming charged lepton universality.

Measured values of the cross section for W+ W- production into semi leptonic decay mode summed over all lepton flavours and assuming charged lepton universality.

Measured values of the cross section for W+ W- production in the fully hadronic decay mode.

The measured values of the E+ E- --> W+ W- cross section summed over all decay modes.

Angular distributions of the W+ W- cross sections resulting from the sum of the (QUARK QUARKBAR ELECTRON NEUTRINO) and the (QUARK QUARKBAR MUON NEUTRINO) cross sections.

Cross sections as a function of W for the lower Q**2, Z pole, data.

Cross sections as a function of W for the high Q**2 data.

Cross sections for the two photon RHO0 RHO0 and non-resonance data for the lower Q**2, Z pole, data.

Cross sections for the two photon RHO0 RHO0 and non-resonance data for the higher Q**2 data.

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\overline{\mathrm{p}}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{p}\mathrm{p}$ at $\sqrt{s}=62.4\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$

$\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{+}$, $\mathrm{p}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=62.4\,\mathrm{Ge\!V}$

$\overline{\mathrm{p}}/\mathrm{\pi}^{-}$, $\mathrm{p}/\mathrm{\pi}^{+}$ versus $p_{\mathrm{T}}$ for $\mathrm{\pi}^{-}$, $\mathrm{\pi}^{+}$, $\mathrm{p}$, $\overline{\mathrm{p}}$ in $\mathrm{Au}-\mathrm{Au}$ at $\sqrt{s_{\mathrm{NN}}}=200\,\mathrm{Ge\!V}$

Data from Figure 3b on charged pion production. Data correspond to charged particle production, corrected to the contribution from (PI+ + PI-)/2.

Data from Figure 3b on charged pion production. Data correspond to charged particle production, corrected to the contribution from (PI+ + PI-)/2.

Data from Figure 3c on charged pion production. Data correspond to charged particle production, corrected to the contribution from (PI+ + PI-)/2.

Data from Figure 3d on charged pion production. Data correspond to charged particle production, corrected to the contribution from (PI+ + PI-)/2.

Data from Figure 4a on forward jet production differential in x, low PT

Data from Figure 4a on forward jet production differential in x, high PT

Data from Figure 5a on forward jet production differential in delta(phi), low x

Data from Figure 5b on forward jet production differential in delta(phi), high x

The reduced cross section at Q**2 = 60 GeV**2 for centre-of-mass energy 318.

The reduced cross section at Q**2 = 80 GeV**2 for centre-of-mass energy 318.

The reduced cross section at Q**2 = 110 GeV**2 for centre-of-mass energy 318.

The reduced cross section at Q**2 = 24 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 32 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 45 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 60 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 80 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 110 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 24 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 32 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 45 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 60 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 80 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 110 GeV**2 for centre-of-mass energy 225.

FL and F2 at Q**2 = 24 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 32 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 45 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 60 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 80 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 110 GeV**2 with no constraints on FL or F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and R as a function of Q**2 with no constraints on F2 or FL. The quantites are quoted such that Q**2/X is constant for each value which correspinds to Y = 0.71 at Ecm=225 GeV.

FL and R as a function of Q**2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2. The quantites are quoted such that Q**2/X is constant for each value which correspinds to Y = 0.71 at Ecm=225 GeV.

Percentage contributions of the various sources of systematic error for Q**2 = 24 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 32 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 45 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 60 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 80 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 110 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 24 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 32 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 45 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 60 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 80 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 110 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 24 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 32 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 45 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 60 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 80 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 110 GeV**2 for centrof-mass energy 225.

Statistical errors only. Data supplied by S. Belforte.