Reference multiplicity distributions obtained from Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV data (black markers), Glauber model (red histogram), and unfolding approach to separate single and pileup contributions. Vertical lines represent statistical uncertainties. Single, pileup, and single+pileup collisions are shown in solid blue markers, dashed green, and dashed pink lines, respectively. The 0–5% central events and 5–60% mid-central to peripheral events are indicated by black arrows. The ratio of the single+pileup to the measured multiplicity distribution is shown in the lower panel.

Reference multiplicity distributions obtained from Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV data (black markers), Glauber model (red histogram), and unfolding approach to separate single and pileup contributions. Vertical lines represent statistical uncertainties. Single, pileup, and single+pileup collisions are shown in solid blue markers, dashed green, and dashed pink lines, respectively. The 0–5% central events and 5–60% mid-central to peripheral events are indicated by black arrows. The ratio of the single+pileup to the measured multiplicity distribution is shown in the lower panel.

Proton cumulants as a function of reference multiplicity (black circles) from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Centrality-binned results with and without centrality bin width corrections are represented by red circles and blue squares, respectively. Vertical dashed lines indicate the centrality classes, from right to left: 0–5%, 5–10%, 10–20%. Data points in this figure are only corrected for detector efficiency but not for the pileup effect, which will be discussed in a later section.

Proton cumulants as a function of reference multiplicity (black circles) from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Centrality-binned results with and without centrality bin width corrections are represented by red circles and blue squares, respectively. Vertical dashed lines indicate the centrality classes, from right to left: 0–5%, 5–10%, 10–20%. Data points in this figure are only corrected for detector efficiency but not for the pileup effect, which will be discussed in a later section.

Proton cumulants as a function of reference multiplicity (black circles) from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Centrality-binned results with and without centrality bin width corrections are represented by red circles and blue squares, respectively. Vertical dashed lines indicate the centrality classes, from right to left: 0–5%, 5–10%, 10–20%. Data points in this figure are only corrected for detector efficiency but not for the pileup effect, which will be discussed in a later section.

Proton cumulants as a function of reference multiplicity from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Pileup corrected and uncorrected cumulants as a function of reference multiplicity are represented by black circles and blue open squares, respectively. Red circles and blue-filled squares represent the results of centrality binned data.

Proton cumulants as a function of reference multiplicity from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Pileup corrected and uncorrected cumulants as a function of reference multiplicity are represented by black circles and blue open squares, respectively. Red circles and blue-filled squares represent the results of centrality binned data.

Ratios of proton cumulants as a function of reference multiplicity from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Pileup corrected and uncorrected cumulants are represented by black circles and blue open squares, respectively. Red circles and blue-filled squares represent the results of centrality binned data.

Ratios of proton cumulants as a function of reference multiplicity from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Pileup corrected and uncorrected cumulants are represented by black circles and blue open squares, respectively. Red circles and blue-filled squares represent the results of centrality binned data.

UrQMD results of the proton cumulant ratios up to sixth order in Au+Au collisions at $\sqrt{s_{\rm NN}}$= 3 GeV. The black circles are without VF correction while blue squares and red triangles are results with VFC which used $N_{\rm part}$ distributions from UrQMD and Glauber models, respectively. The blue crosses are calculations using UrQMD events with b $\leq$ 3 fm. The above results are applied CBWC except for the one (blue crosses) using b $\leq$3 fm events.

UrQMD results of the proton cumulant ratios up to sixth order in Au+Au collisions at $\sqrt{s_{\rm NN}}$= 3 GeV. The black circles are without VF correction while blue squares and red triangles are results with VFC which used $N_{\rm part}$ distributions from UrQMD and Glauber models, respectively. The blue crosses are calculations using UrQMD events with b $\leq$ 3 fm. The above results are applied CBWC except for the one (blue crosses) using b $\leq$3 fm events.

Proton cumulants up to sixth order in $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Data without volume fluctuation correction is shown as grey open squares while data with volume fluctuation correction using $N_{\rm part}$ distributions from Glauber and UrQMD models are shown as black circles and black open triangles, respectively. The corresponding centrality binned cumulants are shown in blue squares, red circles, and orange triangles, respectively. Similarly to Fig. 6, the vertical dashed lines indicate the centrality classes.

Proton cumulants up to sixth order in $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Data without volume fluctuation correction is shown as grey open squares while data with volume fluctuation correction using $N_{\rm part}$ distributions from Glauber and UrQMD models are shown as black circles and black open triangles, respectively. The corresponding centrality binned cumulants are shown in blue squares, red circles, and orange triangles, respectively. Similarly to Fig. 6, the vertical dashed lines indicate the centrality classes.

Proton cumulant ratios up to sixth order in $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Data without volume fluctuation correction are shown as grey open squares while data with volume fluctuation correction using $N_{\rm part}$ distributions from Glauber and UrQMD models are shown as black circles and black open triangles, respectively. The corresponding centrality binned cumulants are shown in blue squares, red circles, and orange triangles, respectively. Similarly to Fig. 6, the vertical dashed lines indicate the centrality classes.

Proton cumulant ratios up to sixth order in $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions. Data without volume fluctuation correction are shown as grey open squares while data with volume fluctuation correction using $N_{\rm part}$ distributions from Glauber and UrQMD models are shown as black circles and black open triangles, respectively. The corresponding centrality binned cumulants are shown in blue squares, red circles, and orange triangles, respectively. Similarly to Fig. 6, the vertical dashed lines indicate the centrality classes.

UrQMD results of proton cumulant ratios up to sixth order in Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. The vertical dashed lines indicate the centrality classes.

Experimental results on centrality dependence of cumulants (left panels) and cumulant ratios (right panels) up to sixth order of the proton multiplicity distributions in Au+Au collisions at $N_{\rm part}$ = 3 GeV. The open squares are data without VF correction while red circles and blue triangles are results with VF correction with $N_{\rm part}$ distributions from Glauber and UrQMD models, respectively.

Experimental results on centrality dependence of cumulants (left panels) and cumulant ratios (right panels) up to sixth order of the proton multiplicity distributions in Au+Au collisions at $N_{\rm part}$ = 3 GeV. The open squares are data without VF correction while red circles and blue triangles are results with VF correction with $N_{\rm part}$ distributions from Glauber and UrQMD models, respectively.

Same as Fig. 14 but for correlation function (left panels) and their normalized ratios (right panels).

Same as Fig. 14 but for correlation function (left panels) and their normalized ratios (right panels).

Cumulants and cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. The transverse momentum window is $p_{\rm T}$ from $0.4<p_{\rm T}<2.0$ GeV/$c$ and the rapidity window is $−0.5<y<0$. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD predictions are depicted by gold bands.

Cumulants and cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. The transverse momentum window is $p_{\rm T}$ from $0.4<p_{\rm T}<2.0$ GeV/$c$ and the rapidity window is $−0.5<y<0$. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD predictions are depicted by gold bands.

Same as Fig. 16 but for correlation functions and correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

Same as Fig. 16 but for correlation functions and correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

The transverse-momentum and rapidity dependence of cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. In the left column, the $p_{\rm T}$ analysis window is $0.4<p_{\rm T}<2.0$ GeV/$c$ while the rapidity window is varied in the range $y_{\rm min}<y<0$. In the right column, the rapidit$y$ analysis window is $−0.5<y<0$ while the $p_{\rm T}$ is varied in the range $0.4<p_{\rm T}<p_{\rm T}^{\rm max}$ GeV/$c$. The most central (0–5%) and peripheral (50–60%) events are depicted by black squares and blue triangles, respectively. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD simulations for the top 0–5% and 50–60% are shown by gold and blue bands, respectively.

The transverse-momentum and rapidity dependence of cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. In the left column, the $p_{\rm T}$ analysis window is $0.4<p_{\rm T}<2.0$ GeV/$c$ while the rapidity window is varied in the range $y_{\rm min}<y<0$. In the right column, the rapidit$y$ analysis window is $−0.5<y<0$ while the $p_{\rm T}$ is varied in the range $0.4<p_{\rm T}<p_{\rm T}^{\rm max}$ GeV/$c$. The most central (0–5%) and peripheral (50–60%) events are depicted by black squares and blue triangles, respectively. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD simulations for the top 0–5% and 50–60% are shown by gold and blue bands, respectively.

The transverse-momentum and rapidity dependence of cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. In the left column, the $p_{\rm T}$ analysis window is $0.4<p_{\rm T}<2.0$ GeV/$c$ while the rapidity window is varied in the range $y_{\rm min}<y<0$. In the right column, the rapidit$y$ analysis window is $−0.5<y<0$ while the $p_{\rm T}$ is varied in the range $0.4<p_{\rm T}<p_{\rm T}^{\rm max}$ GeV/$c$. The most central (0–5%) and peripheral (50–60%) events are depicted by black squares and blue triangles, respectively. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD simulations for the top 0–5% and 50–60% are shown by gold and blue bands, respectively.

The transverse-momentum and rapidity dependence of cumulant ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV. In the left column, the $p_{\rm T}$ analysis window is $0.4<p_{\rm T}<2.0$ GeV/$c$ while the rapidity window is varied in the range $y_{\rm min}<y<0$. In the right column, the rapidit$y$ analysis window is $−0.5<y<0$ while the $p_{\rm T}$ is varied in the range $0.4<p_{\rm T}<p_{\rm T}^{\rm max}$ GeV/$c$. The most central (0–5%) and peripheral (50–60%) events are depicted by black squares and blue triangles, respectively. Statistical and systematic uncertainties are represented by black and gray bars, respectively. UrQMD simulations for the top 0–5% and 50–60% are shown by gold and blue bands, respectively.

As in Fig. 18 but for transverse-momentum and rapidity dependence of correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

As in Fig. 18 but for transverse-momentum and rapidity dependence of correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

As in Fig. 18 but for transverse-momentum and rapidity dependence of correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

As in Fig. 18 but for transverse-momentum and rapidity dependence of correlation function ratios of proton multiplicity distributions for Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 3 GeV.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

Collision energy dependence of the cumulant ratios: $C_2/C_1=\sigma/M$, $C_3/C_2=S\sigma$, and $C_4/C_2=\kappa\sigma^2$, for protons (open squares) and net protons (red circles) from top 0–5% (top panels) and 50–60% (bottom panels) Au+Au collisions at RHIC. The points for protons are shifted horizontally for clarity. The new result for protons from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au collisions is shown as a filled square. UrQMD results with $|y|<0.5$ for protons are shown as gold bands while those for net protons are shown as green dashed lines or green bands. At 3GeV, the model results for protons (−0.5) are shown as blue crosses. UrQMD results of proton and net-proton $C_4/C_2$, see right panels, are almost totally overlapped. The open cross is the result of the model with a fixed impact parameter $b < 3$ fm. The hydrodynamic calculations, for 5% central Au+Au collisions, for protons from $|y|<0.5$ are shown as dashed red linea and the result of the 3 GeV protons from $−0.5<y<0$ is shown as an open red star.

$K^-$ (a), invariant yields as a function of $m_T-m_0$ for various rapidity regions in 10--40\% central Au+Au collisions at ${\sqrt{s_{\mathrm{NN}}} = \mathrm{3\,GeV}}$. Statistics and systematic uncertainties are added quadratic here for plotting. Solid and dashed black lines depict $m_T$ exponential function fits to the measured data points with arbitrate scaling factors in each rapidity windows.

$\phi$ meson (b) invariant yields as a function of $m_T-m_0$ for various rapidity regions in 10--40\% central Au+Au collisions at ${\sqrt{s_{\mathrm{NN}}} = \mathrm{3\,GeV}}$. Statistics and systematic uncertainties are added quadratic here for plotting. Solid and dashed black lines depict $m_T$ exponential function fits to the measured data points with arbitrate scaling factors in each rapidity windows.

$\Xi^-$ (c) invariant yields as a function of $m_T-m_0$ for various rapidity regions in 10--40\% central Au+Au collisions at ${\sqrt{s_{\mathrm{NN}}} = \mathrm{3\,GeV}}$. Statistics and systematic uncertainties are added quadratic here for plotting. Solid and dashed black lines depict $m_T$ exponential function fits to the measured data points with arbitrate scaling factors in each rapidity windows.

$K^-$ (a), invariant yields as a function of $m_T-m_0$ for various rapidity regions in 40--60\% central Au+Au collisions at ${\sqrt{s_{\mathrm{NN}}} = \mathrm{3\,GeV}}$. Statistics and systematic uncertainties are added quadratic here for plotting. Solid and dashed black lines depict $m_T$ exponential function fits to the measured data points with arbitrate scaling factors in each rapidity windows.

$\phi$ meson (b) invariant yields as a function of $m_T-m_0$ for various rapidity regions in 40--60\% central Au+Au collisions at ${\sqrt{s_{\mathrm{NN}}} = \mathrm{3\,GeV}}$. Statistics and systematic uncertainties are added quadratic here for plotting. Solid and dashed black lines depict $m_T$ exponential function fits to the measured data points with arbitrate scaling factors in each rapidity windows.

Rapidity density distributions of $K^-$ (squares), $p_T$-integrated yields $dN/dy$ in 0--10\% (a), 10--40\% (b) and 40--60\% central (c) Au+Au collisions at ${\sqrt{s_{\mathrm{NN}}} = \mathrm{3\,GeV}}$. %The full symbols show the measured data, while the open ones are data reflected with respect to $y=0$ in the center-of-mass frame. Solid lines depict Gaussian function fits to the data points.

Rapidity density distributions of $\phi$ meson (circles) $p_T$-integrated yields $dN/dy$ in 0--10\% (a), 10--40\% (b) and 40--60\% central (c) Au+Au collisions at ${\sqrt{s_{\mathrm{NN}}} = \mathrm{3\,GeV}}$. %The full symbols show the measured data, while the open ones are data reflected with respect to $y=0$ in the center-of-mass frame. Solid lines depict Gaussian function fits to the data points.

Rapidity density distributions of $\Xi^-$ (diamonds) $p_T$-integrated yields $dN/dy$ in 0--10\% (a), 10--40\% (b) and 40--60\% central (c) Au+Au collisions at ${\sqrt{s_{\mathrm{NN}}} = \mathrm{3\,GeV}}$. %The full symbols show the measured data, while the open ones are data reflected with respect to $y=0$ in the center-of-mass frame. Solid lines depict Gaussian function fits to the data points.

$\phi/K^-$ (a) and $\phi/\Xi^-$ (b) ratio as a function of collision energy, $\sqrt{s_{\mathrm{NN}}}$. The solid black circles show the measurements presented here in 0-10\% centrality bin, while empty markers in black or grey are used for data from various other energies and/or collision systems. The grey solid line represents a THERMUS calculation based on the Grand Canonical Ensemble (GCE) while the dotted lines depict calculations based on the Canonical Ensemble (CE) with different parameters of strangeness correlation radius ($r_c$). The green dashed line, green shaded band and the solid red line show transport model calculations from the public versions $\mathrm{UrQMD}^{1}$, modified $\mathrm{UrQMD}^{2}$ and SMASH, respectively.

Rapidity($y$) dependence of $v_1$ (top panels) and $v_2$ (bottom panels) of proton and $\Lambda$ baryons (left panels), pions (middle panels) and kaons (right panels) in 10-40% centrality for the $\sqrt{s_{NN}}$ = 3GeV Au+Au collisions. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The UrQMD and JAM results are shown as bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. The value of the incompressibility $\kappa$ = 380 MeV is used in the mean-field option. More detailed model descriptions and data comparisons can be found in Supplemental Material.

Rapidity($y$) dependence of $v_1$ (top panels) and $v_2$ (bottom panels) of proton and $\Lambda$ baryons (left panels), pions (middle panels) and kaons (right panels) in 10-40% centrality for the $\sqrt{s_{NN}}$ = 3GeV Au+Au collisions. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The UrQMD and JAM results are shown as bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. The value of the incompressibility $\kappa$ = 380 MeV is used in the mean-field option. More detailed model descriptions and data comparisons can be found in Supplemental Material.

Rapidity($y$) dependence of $v_1$ (top panels) and $v_2$ (bottom panels) of proton and $\Lambda$ baryons (left panels), pions (middle panels) and kaons (right panels) in 10-40% centrality for the $\sqrt{s_{NN}}$ = 3GeV Au+Au collisions. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The UrQMD and JAM results are shown as bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. The value of the incompressibility $\kappa$ = 380 MeV is used in the mean-field option. More detailed model descriptions and data comparisons can be found in Supplemental Material.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

$v_2$ scaled by the number of constituent quarks, $v_2/n_q$ , as a function of scaled transverse kinetic energy ($(m_T − m_0)/n_q$) for pions, kaons and protons from Au+Au collisions in 10-40% centrality at $\sqrt{s_{NN}}$ = 3, 27, and 54.4 GeV for positive charged particles (left panel) and negative charged particles (right panel). Colored dashed lines represent the scaling fit to data in 7.7, 14.5, 27, 54.4, and 200 GeV Au+Au collisions from STAR experiment at RHIC [43–45]. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points.

Collision energy dependence of (top panel) directed flow slope $dv_1/dy|_{y=0}$ for p, $\Lambda, \pi$(combined from $\pi^{\pm}$), K(combined from $K^{\pm}$ and $K_S^0$), $\phi$ and $\Xi^−$, and (bottom panel) elliptic flow $v_2$ for p, $\pi$(combined from $\pi^{\pm}$) in heavy- ion collisions. Collision centrality for all data from RHIC is 10-40%, except for 4.5 GeV where 10-30% is for $dv_1/dy|_{y=0}$ and 0-30% is for $v_2$. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The JAM and UrQMD results are shown as colored bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. For clarity the x-axis value of the data points have been shifted.

Collision energy dependence of (top panel) directed flow slope $dv_1/dy|_{y=0}$ for p, $\Lambda, \pi$(combined from $\pi^{\pm}$), K(combined from $K^{\pm}$ and $K_S^0$), $\phi$ and $\Xi^−$, and (bottom panel) elliptic flow $v_2$ for p, $\pi$(combined from $\pi^{\pm}$) in heavy- ion collisions. Collision centrality for all data from RHIC is 10-40%, except for 4.5 GeV where 10-30% is for $dv_1/dy|_{y=0}$ and 0-30% is for $v_2$. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The JAM and UrQMD results are shown as colored bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. For clarity the x-axis value of the data points have been shifted.

Collision energy dependence of (top panel) directed flow slope $dv_1/dy|_{y=0}$ for p, $\Lambda, \pi$(combined from $\pi^{\pm}$), K(combined from $K^{\pm}$ and $K_S^0$), $\phi$ and $\Xi^−$, and (bottom panel) elliptic flow $v_2$ for p, $\pi$(combined from $\pi^{\pm}$) in heavy- ion collisions. Collision centrality for all data from RHIC is 10-40%, except for 4.5 GeV where 10-30% is for $dv_1/dy|_{y=0}$ and 0-30% is for $v_2$. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The JAM and UrQMD results are shown as colored bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. For clarity the x-axis value of the data points have been shifted.

Collision energy dependence of (top panel) directed flow slope $dv_1/dy|_{y=0}$ for p, $\Lambda, \pi$(combined from $\pi^{\pm}$), K(combined from $K^{\pm}$ and $K_S^0$), $\phi$ and $\Xi^−$, and (bottom panel) elliptic flow $v_2$ for p, $\pi$(combined from $\pi^{\pm}$) in heavy- ion collisions. Collision centrality for all data from RHIC is 10-40%, except for 4.5 GeV where 10-30% is for $dv_1/dy|_{y=0}$ and 0-30% is for $v_2$. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The JAM and UrQMD results are shown as colored bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. For clarity the x-axis value of the data points have been shifted.

Collision energy dependence of (top panel) directed flow slope $dv_1/dy|_{y=0}$ for p, $\Lambda, \pi$(combined from $\pi^{\pm}$), K(combined from $K^{\pm}$ and $K_S^0$), $\phi$ and $\Xi^−$, and (bottom panel) elliptic flow $v_2$ for p, $\pi$(combined from $\pi^{\pm}$) in heavy- ion collisions. Collision centrality for all data from RHIC is 10-40%, except for 4.5 GeV where 10-30% is for $dv_1/dy|_{y=0}$ and 0-30% is for $v_2$. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The JAM and UrQMD results are shown as colored bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. For clarity the x-axis value of the data points have been shifted.

Collision energy dependence of (top panel) directed flow slope $dv_1/dy|_{y=0}$ for p, $\Lambda, \pi$(combined from $\pi^{\pm}$), K(combined from $K^{\pm}$ and $K_S^0$), $\phi$ and $\Xi^−$, and (bottom panel) elliptic flow $v_2$ for p, $\pi$(combined from $\pi^{\pm}$) in heavy- ion collisions. Collision centrality for all data from RHIC is 10-40%, except for 4.5 GeV where 10-30% is for $dv_1/dy|_{y=0}$ and 0-30% is for $v_2$. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The JAM and UrQMD results are shown as colored bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. For clarity the x-axis value of the data points have been shifted.

Collision energy dependence of (top panel) directed flow slope $dv_1/dy|_{y=0}$ for p, $\Lambda, \pi$(combined from $\pi^{\pm}$), K(combined from $K^{\pm}$ and $K_S^0$), $\phi$ and $\Xi^−$, and (bottom panel) elliptic flow $v_2$ for p, $\pi$(combined from $\pi^{\pm}$) in heavy- ion collisions. Collision centrality for all data from RHIC is 10-40%, except for 4.5 GeV where 10-30% is for $dv_1/dy|_{y=0}$ and 0-30% is for $v_2$. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The JAM and UrQMD results are shown as colored bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. For clarity the x-axis value of the data points have been shifted.

Collision energy dependence of (top panel) directed flow slope $dv_1/dy|_{y=0}$ for p, $\Lambda, \pi$(combined from $\pi^{\pm}$), K(combined from $K^{\pm}$ and $K_S^0$), $\phi$ and $\Xi^−$, and (bottom panel) elliptic flow $v_2$ for p, $\pi$(combined from $\pi^{\pm}$) in heavy- ion collisions. Collision centrality for all data from RHIC is 10-40%, except for 4.5 GeV where 10-30% is for $dv_1/dy|_{y=0}$ and 0-30% is for $v_2$. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The JAM and UrQMD results are shown as colored bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. For clarity the x-axis value of the data points have been shifted.

Collision energy dependence of (top panel) directed flow slope $dv_1/dy|_{y=0}$ for p, $\Lambda, \pi$(combined from $\pi^{\pm}$), K(combined from $K^{\pm}$ and $K_S^0$), $\phi$ and $\Xi^−$, and (bottom panel) elliptic flow $v_2$ for p, $\pi$(combined from $\pi^{\pm}$) in heavy- ion collisions. Collision centrality for all data from RHIC is 10-40%, except for 4.5 GeV where 10-30% is for $dv_1/dy|_{y=0}$ and 0-30% is for $v_2$. Statistical and systematic uncertainties are shown as bars and gray bands, respectively. Some uncertainties are smaller than the data points. The JAM and UrQMD results are shown as colored bands:golden, red and blue bands stand for JAM mean-field, UrQMD mean-field and UrQMD cascade mode, respectively. For clarity the x-axis value of the data points have been shifted.

Mixed higher-order flow harmonic $v_6\{\Psi_{33}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_7\{\Psi_{223}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_4\{\Psi_{22}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_5\{\Psi_{23}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{222}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{33}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_7\{\Psi_{223}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_4\{\Psi_{22}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_5\{\Psi_{23}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{222}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{33}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_7\{\Psi_{223}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_4\{\Psi_{22}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_5\{\Psi_{23}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{222}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{33}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_7\{\Psi_{223}\}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

The overall flow harmonic $v_4\{\Psi_{4}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

The overall flow harmonic $v_5\{\Psi_{5}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

The overall flow harmonic $v_6\{\Psi_{6}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

The overall flow harmonic $v_6\{\Psi_{6}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

The overall flow harmonic $v_7\{\Psi_{7}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

The overall flow harmonic $v_4\{\Psi_{4}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

The overall flow harmonic $v_5\{\Psi_{5}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

The overall flow harmonic $v_6\{\Psi_{6}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

The overall flow harmonic $v_6\{\Psi_{6}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

The overall flow harmonic $v_7\{\Psi_{7}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_4\{\Psi_{22}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_5\{\Psi_{23}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{222}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{33}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_7\{\Psi_{223}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Mixed higher-order flow harmonic $v_4\{\Psi_{22}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_5\{\Psi_{23}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{222}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_6\{\Psi_{33}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_7\{\Psi_{223}\}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{422}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{523}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{6222}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{633}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{7223}$ from the scalar-product method at 5.02 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{422}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{523}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{6222}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{633}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{7223}$ from the scalar-product method at 5.02 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{422}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{523}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{6222}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{633}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{7223}$ from the scalar-product method at 2.76 TeV as a function of PT in the 0-20% centrality range.

Nonlinear response coefficient $\chi_{422}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{523}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{6222}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{633}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

Nonlinear response coefficient $\chi_{7223}$ from the scalar-product method at 2.76 TeV as a function of PT in the 20-60% centrality range.

Mixed higher-order flow harmonic $v_4\{\Psi_{22}\}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Mixed higher-order flow harmonic $v_5\{\Psi_{23}\}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Mixed higher-order flow harmonic $v_6\{\Psi_{222}\}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Mixed higher-order flow harmonic $v_6\{\Psi_{33}\}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Mixed higher-order flow harmonic $v_7\{\Psi_{223}\}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Mixed higher-order flow harmonic $v_4\{\Psi_{22}\}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Mixed higher-order flow harmonic $v_5\{\Psi_{23}\}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Mixed higher-order flow harmonic $v_6\{\Psi_{222}\}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Mixed higher-order flow harmonic $v_6\{\Psi_{33}\}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Mixed higher-order flow harmonic $v_7\{\Psi_{223}\}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{422}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{523}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{6222}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{633}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{7223}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{422}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{523}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{6222}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{633}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{7223}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{422}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{523}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{6222}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{633}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{7223}$ from the scalar-product method at 5.02 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{422}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{523}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{6222}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{633}$ from the scalar-product method at 2.76 TeV as a function of centrality.

Nonlinear response coefficient $\chi_{7223}$ from the scalar-product method at 2.76 TeV as a function of centrality.

The cumulant $c_2\{8\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in pPb collisions.

The elliptic flow $v_2\{6\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in PbPb collisions.

The elliptic flow $v_2\{8\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in PbPb collisions.

The elliptic flow $v_2\{\text{LYZ}\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in PbPb collisions.

The elliptic flow $v_2\{6\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in pPb collisions.

The elliptic flow $v_2\{8\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in pPb collisions.

The elliptic flow $v_2\{\text{LYZ}\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in pPb collisions.

The cumulant ratio $c_2\{6\}/v_2\{4\}$ as a function of $c_2\{4\}/v_2\{2\}$ in pPb collisions.

The cumulant ratio $c_2\{8\}/v_2\{6\}$ as a function of $c_2\{4\}/v_2\{2\}$ in pPb collisions.

The cumulant ratio $c_2\{6\}/v_2\{4\}$ as a function of $c_2\{4\}/v_2\{2\}$ in PbPb collisions.

The cumulant ratio $c_2\{8\}/v_2\{6\}$ as a function of $c_2\{4\}/v_2\{2\}$ in PbPb collisions.

The product of the electronic width of the PHI(1020) and its branching fraction to KS KL.

Cross section measurement for PHI(1680).

Mass measurement for PHI(1680).

Measurement of the PHI(1680) width.

The product of the electronic width of the PHI(1680) and its branching fraction to KS KL.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> KS KL PI+ PI-) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> KS KS PI+ PI-) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> KS KS K+ K-) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> K*(892) KS PI) * BR(K*(892) --> KS PI) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> K2*(1430) KS PI) * BR(K2*(1430) --> KS PI) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> K*(892)+ K*(892)-) * (BR(K*(892) --> KS PI))**2 and the 90% C.L. J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> K2*(1430) K*(892)) * BR(K2*(1430) --> KS PI) * BR(K*(892) --> KS PI) and the 90% C.L. J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> KS KS PHI(1020)) * BR(PHI --> K+ K-) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> F2PRIME(1525) PHI(1020)) * BR(PHI --> K+ K-} * BR(F2PRIME(1525) --> KS KS) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> F2PRIME(1525) K+ K-) * BR(F2PRIME(1525) --> KS KS) and the J/PSI branching fraction.

Cross section measurements for the reaction E+ E- --> PHI F0(980). Statistical errors only.

Cross section measurements for the reaction E+ E- --> PHI F0(600). Statistical errors only.

Cross section measurements for the reaction E+ E- --> K+ K- PI0 PI0. Statistical errors only.

Cross section measurements for the reaction E+ E- --> PHI F0(980). Statistical errors only.

Cross section measurements for the reaction E+ E- --> K+ K- K+ K-. Statistical errors only.

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The differential cross section as a function of PHI, the angle between the positron scattering plane and the proton scattering plane for the LRG and the LPS data samples.

The azimuthal asymmetries ALT and ATT as a function of X(NAME=POMERON).

The azimuthal asymmetries ALT and ATT as a function of BETA.

The azimuthal asymmetries ALT and ATT as a function of ABS(T).

The azimuthal asymmetries ALT and ATT as a function of Q**2.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 2.5 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 3.9 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 7.1 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 14 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 40 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 2.5 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 3.9 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 7.1 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 14 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 40 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 2.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 3.9 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 7.1 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 14 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 40 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 2.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 3.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 4.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 5.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 6.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 8.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 12 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 16 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 22 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 30 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 40 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 50 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 65 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 85 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 110 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 140 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 185 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 255 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the Rosenbluth separation technique fit method.. E99M29 E99M30 E99M31.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the Rosenbluth separation technique fit method.. E99M29 E99M30 E99M31.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the Rosenbluth separation technique fit method.. E99M29 E99M30 E99M31.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.8 to -0.4.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.4 to -0.1.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.2 to 0.5.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.5 to 0.8.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.

Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5, and.

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.

Measurement of the E+ E- --> PHI F(980)0 cross section.

Measurement of the E+ E- --> K+ K- PI0 PI0 cross section. Statistical errors only.

Measurement of the E+ E- --> PHI F0 cross section for the F0 --> PI0 PI0 final state. Statistical errors only.

Measurement of the E+ E- --> K+ K- K+ K- cross section. Statistical errors only.

Differential cross section for indicent photon energy 825 MeV.

Differential cross section for indicent photon energy 875 MeV.

Differential cross section for indicent photon energy 925 MeV.

Differential cross section for indicent photon energy 975 MeV.

Differential cross section for indicent photon energy 1025 MeV.

Differential cross section for indicent photon energy 1075 MeV.

Differential cross section for indicent photon energy 1125 MeV.

Differential cross section for indicent photon energy 1175 MeV.

Differential cross section for indicent photon energy 1225 MeV.

Differential cross section for indicent photon energy 1275 MeV.

Differential cross section for indicent photon energy 1325 MeV.

Differential cross section for indicent photon energy 1375 MeV.

Differential cross section for indicent photon energy 1425 MeV.

Differential cross section for indicent photon energy 1475 MeV.

Differential cross section for indicent photon energy 1525 MeV.

Differential cross section for indicent photon energy 1575 MeV.

Differential cross section for indicent photon energy 1625 MeV.

Differential cross section for indicent photon energy 1675 MeV.

Differential cross section for indicent photon energy 1725 MeV.

Differential cross section for indicent photon energy 1775 MeV.

Differential cross section for indicent photon energy 1825 MeV.

Differential cross section for indicent photon energy 1875 MeV.

Differential cross section for indicent photon energy 1925 MeV.

Differential cross section for indicent photon energy 1975 MeV.

Differential cross section for indicent photon energy 2025 MeV.

Differential cross section for indicent photon energy 2075 MeV.

Differential cross section for indicent photon energy 2125 MeV.

Differential cross section for indicent photon energy 2175 MeV.

Differential cross section for indicent photon energy 2225 MeV.

Differential cross section for indicent photon energy 2275 MeV.

Differential cross section for indicent photon energy 2325 MeV.

Differential cross section for indicent photon energy 2375 MeV.

Differential cross section for indicent photon energy 2425 MeV.

Differential cross section for indicent photon energy 2475 MeV.

Differential cross section for indicent photon energy 2525 MeV.

Differential cross section for indicent photon energy 2575 MeV.

Differential cross section for indicent photon energy 2625 MeV.

Differential cross section for indicent photon energy 2675 MeV.

Differential cross section for indicent photon energy 2725 MeV.

Differential cross section for indicent photon energy 2775 MeV.

Measured cross section for E+ E- --> OMEGA F0(975) with statistical errors only.

Measured cross section for E+ E- --> 2(PI+ PI-) ETA with statistical errorsonly.

Measured cross section for E+ E- --> ETAPRIME PI+ PI- with statistical errors only.

Measured cross section for E+ E- --> F1(1285) PI+ PI- with statistical errors only.

Measured cross section for E+ E- --> K+ K- PI+ PI- PI0 with statistical errors only.

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

Measured cross section for E+ E- --> OMEGA K+ K- with statistical errors only.

Measured cross section for E+ E- --> K+ K- PI+ PI- ETA with statistical errors only.

Spin parity analysis fits for RHO+ RHO-.

Differential cross sections for ETAPRIME photoproduction on the proton at photon energies 1.980, 2.029 and 2.079 GeV. The errors shown are combined statistical and systematic.

Differential cross sections for ETAPRIME photoproduction on the proton at photon energies 2.129, 2.178 and 2.227 GeV. The errors shown are combined statistical and systematic.

Differential cross sections DSIG/DT for Q**2 = 2.042 GeV**2 and W = 2.63 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.320 GeV**2 and W = 2.70 GeV.

Differential cross sections DSIG/DT for Q**2 = 1.785 GeV**2 and W = 2.21 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.050 GeV**2 and W = 2.33 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.350 GeV**2 and W = 2.47 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.639 GeV**2 and W = 2.58 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.914 GeV**2 and W = 2.62 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.050 GeV**2 and W = 2.09 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.350 GeV**2 and W = 2.21 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.650 GeV**2 and W = 2.32 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.950 GeV**2 and W = 2.43 GeV.

Differential cross sections DSIG/DT for Q**2 = 3.295 GeV**2 and W = 2.51 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.055 GeV**2 and W = 1.90 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.350 GeV**2 and W = 2.00 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.650 GeV**2 and W = 2.10 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.950 GeV**2 and W = 2.19 GeV.

Differential cross sections DSIG/DT for Q**2 = 3.350 GeV**2 and W = 2.31 GeV.

Differential cross sections DSIG/DT for Q**2 = 3.807 GeV**2 and W = 2.41 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.371 GeV**2 and W = 1.85 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.651 GeV**2 and W = 1.91 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.950 GeV**2 and W = 1.99 GeV.

Differential cross sections DSIG/DT for Q**2 = 3.350 GeV**2 and W = 2.09 GeV.

Differential cross sections DSIG/DT for Q**2 = 3.850 GeV**2 and W = 2.21 GeV.

Differential cross sections DSIG/DT for Q**2 = 4.307 GeV**2 and W = 2.30 GeV.

Differential cross sections DSIG/DT for Q**2 = 2.968 GeV**2 and W = 1.85 GeV.

Differential cross sections DSIG/DT for Q**2 = 3.357 GeV**2 and W = 1.91 GeV.

Differential cross sections DSIG/DT for Q**2 = 3.850 GeV**2 and W = 2.01 GeV.

Differential cross sections DSIG/DT for Q**2 = 4.350 GeV**2 and W = 2.11 GeV.

Differential cross sections DSIG/DT for Q**2 = 4.765 GeV**2 and W = 2.16 GeV.

Differential cross sections DSIG/DT for Q**2 = 3.882 GeV**2 and W = 1.86 GeV.

Differential cross sections DSIG/DT for Q**2 = 4.352 GeV**2 and W = 1.91 GeV.

Differential cross sections DSIG/DT for Q**2 = 4.850 GeV**2 and W = 2.00 GeV.

Spin density matrix elements R^04_0 and R^04_1-1 from the 1D projection method.

Spin density matrix element R^04_00 using the moments method.

Spin density matrix element RE(R^04_10) using the moments method.

Spin density matrix element R^04_1-1 using the moments method.

Spin density matrix element R^01_00 using the moments method.

Spin density matrix element R^01_11 using the moments method.

Spin density matrix element RE(R^01_10) using the moments method.

Spin density matrix element R^01_1-1 using the moments method.

Spin density matrix element IM(R^02_10) using the moments method.

Spin density matrix element IM(R^02_1-1) using the moments method.

Spin density matrix element R^05_00 using the moments method.

Spin density matrix element R^05_11 using the moments method.

Spin density matrix element RE(R^05_10) using the moments method.

Spin density matrix element R^05_1-1 using the moments method.

Spin density matrix element IM(R^06_10) using the moments method.

Spin density matrix element IM(R^06_1-1) using the moments method.

Measured production cross section for the E+ E- process as a function of W for Q**2 from 1.2 to 8.5 GeV**2 for the Z-pole data.

Measured production cross section for the E+ E- process as a function of W for Q**2 from 8.8 to 30 GeV**2 for the high energy data.

Measured production cross section cross section for the two photon process as a function of W for Q**2 from 1.2 to 8.5 GeV**2 for the Z-pole data.

Measured production cross section cross section for the two photon process as a function of W for Q**2 from 8.8 to 30 GeV**2 for the high energy data.

Measured production cross section for the two-photon process as a function of W for Q**2 from 1.2 to 8.5 GeV**2 for the Z-pole data.

Measured production cross section for the two-photon process as a function of W for Q**2 from 8.8 to 30 GeV**2 for the high energy data.

Measured cross section DSIG/DM(PI+PI-) for the W range 1475 to 1500GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1500 to 1525GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1525 to 1550GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1550 to 1575GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1575 to 1600GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1600 to 1625GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1625 to 1650GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1650 to 1675GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1675 to 1700GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1700 to 1725GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1725 to 1750GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1750 to 1775GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1775 to 1800GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1800 to 1825GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1825 to 1850GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1850 to 1875GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1875 to 1900GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1900 to 1925GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1925 to 1950GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1950 to 1975GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 1975 to 2000GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 2000 to 2025GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 2025 to 2050GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 2050 to 2075GeV.

Measured cross section DSIG/DM(PI+PI-) for the W range 2075 to 2100GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1400 to 1425GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1425 to 1450GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1450 to 1475GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1475 to 1500GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1500 to 1525GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1525 to 1550GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1550 to 1575GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1575 to 1600GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1600 to 1625GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1625 to 1650GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1650 to 1675GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1675 to 1700GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1700 to 1725GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1725 to 1750GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1750 to 1775GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1775 to 1800GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1800 to 1825GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1825 to 1850GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1850 to 1875GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1875 to 1900GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1900 to 1925GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1925 to 1950GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1950 to 1975GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 1975 to 2000GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 2000 to 2025GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 2025 to 2050GeV.

Measured cross section DSIG/DM(PI+Proton) for the W range 2050 to 2075GeV.