The unfolded differential charge asymmetry as a function of the transverse momentum of the top pair system. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NNLO in QCD and NLO in EW theory are listed. The scale uncertainty is obtained by varying renormalisation and factorisation scales independently by a factor of 2 or 0.5 around $\mu_0$ to calculate the maximum and minimum value of the asymmetry, respectively. The nominal value $\mu_0$ is chosen as $H_T/4$. The variations in which one scale is multiplied by 2 while the other scale is divided by 2 are excluded. Finally, the scale and MC integration uncertainties are added in quadrature.

The unfolded differential charge asymmetry as a function of the longitudinal boost of the top pair system. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NNLO in QCD and NLO in EW theory are listed. The scale uncertainty is obtained by varying renormalisation and factorisation scales independently by a factor of 2 or 0.5 around $\mu_0$ to calculate the maximum and minimum value of the asymmetry, respectively. The nominal value $\mu_0$ is chosen as $H_T/4$. The variations in which one scale is multiplied by 2 while the other scale is divided by 2 are excluded. Finally, the scale and MC integration uncertainties are added in quadrature.

The unfolded inclusive leptonic asymmetry. The unfolded $A_C^{\ell\bar{\ell}}$ is obtained in the reduced phase-space defined by the requirement $|\Delta |\eta_{\ell\bar{\ell}}||<2.5$. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NLO in QCD and NLO in EW theory are listed. The theory uncertainty is obtained by varying both scales by a factor of 0.5 or 2.0 to calculate the minimum and maximum value of the asymmetry, respectively.

The unfolded differential leptonic asymmetry as a function of the invariant mass of the di-lepton pair. The unfolded $A_C^{\ell\bar{\ell}}$ is obtained in the reduced phase-space defined by the requirement $|\Delta |\eta_{\ell\bar{\ell}}||<2.5$. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NLO in QCD and NLO in EW theory are listed. The theory uncertainty is obtained by varying both scales by a factor of 0.5 or 2.0 to calculate the minimum and maximum value of the asymmetry, respectively.

The unfolded differential leptonic asymmetry as a function of the transverse momentum of the di-lepton pair. The unfolded $A_C^{\ell\bar{\ell}}$ is obtained in the reduced phase-space defined by the requirement $|\Delta |\eta_{\ell\bar{\ell}}||<2.5$. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NLO in QCD and NLO in EW theory are listed. The theory uncertainty is obtained by varying both scales by a factor of 0.5 or 2.0 to calculate the minimum and maximum value of the asymmetry, respectively.

The unfolded differential leptonic asymmetry as a function of the longitudinal boost of the di-lepton pair. The unfolded $A_C^{\ell\bar{\ell}}$ is obtained in the reduced phase-space defined by the requirement $|\Delta |\eta_{\ell\bar{\ell}}||<2.5$. The measured values are given with statistical and systematic uncertainties. The SM theory predictions calculated at NLO in QCD and NLO in EW theory are listed. The theory uncertainty is obtained by varying both scales by a factor of 0.5 or 2.0 to calculate the minimum and maximum value of the asymmetry, respectively.

Individual 68% and 95% CL bounds on the relevant Wilson coefficients of the SM Effective Field Theory in units of $\text{TeV}^{-2}$. The bounds are derived from the $A_C^{t\bar{t}}$ inclusive measurement. The experimental uncertainties are accounted for, in the form of the complete covariance matrix that keeps track of correlations between bins for the differential measurement. The theory uncertainty from the NNLO QCD + NLO EW calculation is included by explicitly varying the renormalization and factorization scales, or the parton density functions, in the calculation and registering the variations in the intervals.

Individual 68% and 95% CL bounds on the relevant Wilson coefficients of the SM Effective Field Theory in units of $\text{TeV}^{-2}$. The bounds are derived from the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement. The experimental uncertainties are accounted for, in the form of the complete covariance matrix that keeps track of correlations between bins for the differential measurement. The theory uncertainty from the NNLO QCD + NLO EW calculation is included by explicitly varying the renormalization and factorization scales, or the parton density functions, in the calculation and registering the variations in the intervals.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ inclusive measurement. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement for $\beta_{z,t\bar{t}}$ $\in$ [0,0.3]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement for $\beta_{z,t\bar{t}}$ $\in$ [0.3,0.6]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement for $\beta_{z,t\bar{t}}$ $\in$ [0.6,0.8]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement for $\beta_{z,t\bar{t}}$ $\in$ [0.8,1]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ < 500 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ $\in$ [500,750] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ $\in$ [750,1000] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ $\in$ [1000,1500] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement for $m_{t\bar{t}}$ > 1500 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement for $p_{T,t\bar{t}}$ < 30 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement for $p_{T,t\bar{t}}$ $\in$ [30,120] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement for $p_{T,t\bar{t}}$ > 120 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ inclusive measurement. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement for $\beta_{z,\ell\bar{\ell}}$ $\in$[0,0.3]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement for $\beta_{z,\ell\bar{\ell}}$ $\in$[0.3,0.6]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement for $\beta_{z,\ell\bar{\ell}}$ $\in$[0.6,0.8]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement for $\beta_{z,\ell\bar{\ell}}$ $\in$[0.8,1]. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement for $m_{\ell\bar{\ell}}$ < 200 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement for $m_{\ell\bar{\ell}}$ $\in$ [200,300] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement for $m_{\ell\bar{\ell}}$ $\in$ [300,400] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement for $m_{\ell\bar{\ell}}$ > 400 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement for $p_{T,\ell\bar{\ell}}$ < 20 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement for $p_{T,\ell\bar{\ell}}$ $\in$ [20, 70] GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Ranking of the systematic uncertainties with marginalisation for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement for $p_{T,\ell\bar{\ell}}$ > 70 GeV. The effect on unfolded $A_C$ for down and up variation of the systematic uncertainty is shown, respectively. The pulls and constraints of the ranked NPs are obtained from data.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{t\bar{t}}$ inclusive measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{\ell\ell}$ inclusive measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Post-marginalisation correlation coefficients $\rho_{ij}$ of nuisance parameters for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement. Only $|\rho_{ij}| > 0.05$ values are included.

Covariance matrix for the $A_C^{t\bar{t}}$ vs $m_{t\bar{t}}$ measurement.

Covariance matrix for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement.

Covariance matrix for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement.

Covariance matrix for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement.

Covariance matrix for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement.

Covariance matrix for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement.

Light quark ($uds$) Collins asymmetries obtained by fitting the U/L and U/C double ratios as a function of ($z_1$,$z_2$) for $K\pi$ hadron pairs. In the first column, the $z$ bins and their respective mean values for the hadron ($K$ or $\pi$) in one hemisphere are reported; in the following column, the same variables for the second hadron ($K$ or $\pi$) are shown; in the third column the mean value of $\sin^2\theta_{2}/(1+\cos^2\theta_{2})$ is summarized, calculated in the RF0 frame; in the last two columns the asymmetry results are summarized. The mean values of the quantities reported in the table are calculated by summing the corresponding values for each $K\pi$ pair and dividing by the number of $K\pi$ pairs that fall into each ($z_1$,$z_2$) interval. Note that the $A^{UL}$ and $A^{UC}$ results are strongly correlated since they are obtained by using the same data set.

Light quark ($uds$) Collins asymmetries obtained by fitting the U/L and U/C double ratios as a function of ($z_1$,$z_2$) for pion pairs. In the first column, the $z$ bins and their respective mean values for the pion in one hemisphere are reported; in the following column, the same variables for the second pion are shown; in the third column the mean value of $\sin^2\theta_{th}/(1+\cos^2\theta_{th})$ is summarized, calculated in the RF12 frame; in the last two columns the asymmetry results are summarized. The mean values of the quantities reported in the table are calculated by summing the corresponding values for each $\pi\pi$ pair and dividing by the number of $\pi\pi$ pairs that fall into each ($z_1$,$z_2$) interval. Note that the $A^{UL}$ and $A^{UC}$ results are strongly correlated since they are obtained by using the same data set.

Light quark ($uds$) Collins asymmetries obtained by fitting the U/L and U/C double ratios as a function of ($z_1$,$z_2$) for pion pairs. In the first column, the $z$ bins and their respective mean values for the pion in one hemisphere are reported; in the following column, the same variables for the second pion are shown; in the third column the mean value of $\sin^2\theta_{2}/(1+\cos^2\theta_{2})$ is summarized, calculated in the RF0 frame; in the last two columns the asymmetry results are summarized. The mean values of the quantities reported in the table are calculated by summing the corresponding values for each $\pi\pi$ pair and dividing by the number of $\pi\pi$ pairs that fall into each ($z_1$,$z_2$) interval. Note that the $A^{UL}$ and $A^{UC}$ results are strongly correlated since they are obtained by using the same data set.

The fully corrected measurement of ASYM(FB) as a function of the muon-pair invariant mass.

Double-spin azimuthal asymmetries for a transversely (T) polarised target and a longitudinally (L) polarised beam.

Double-spin azimuthal asymmetries for a transversely (T) polarised target and a longitudinally (L) polarised beam.

Double-spin azimuthal asymmetries for a transversely (T) polarised target and a longitudinally (L) polarised beam.

The DVCS cross section DSIG/DT in three different regions of Q**2.

The DVCS cross section DSIG/DT in three regions of W.

Overall value of the SLOPE parameter of the fit to the DSIG/DT distribution.

Overall value of the fit to the W distribution of the form W**POWER.

Value of the power of the fit to the W distribution of the form W**POWER in three Q**2 regions.

Value of the fitted slope parameter in three Q**2 regions.

Value of the fitted slope parameter in three W regions.

The measured beam charge asymmetry defined as the difference in the DSIG/DPHI distributions between E+ P and E- P collisions.

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.

Beam SSA as a function of Z, X, hadronic PT and Q**2 corrected for the decay of exclusively produced VMs with the DSYS error due to the uncertainty in the VM subtraction.

Beam SSA as a function of Z, X, hadronic PT and Q**2 corrected for the decay of exclusively produced VMs with the DSYS error due to the uncertainty in the VM subtraction.

Beam SSA as a function of Z, X, hadronic PT and Q**2 corrected for the decay of exclusively produced VMs with the DSYS error due to the uncertainty in the VM subtraction.

Differential K0S cross section in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.

Differential K0S cross section in DIS events as a function of Bjorken X. for Q**2 from 5 to 25 GeV**2.

Differential K0S cross section in DIS events as a function of Bjorken X. for Q**2 > 25 GeV**2.

Differential K0S cross section in DIS events as a function of Q**2. for Q**2 > 5 GeV**2.

Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of transverse momentum (lab). for Q**2 from 5 to 25 GeV**2.

Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of transverse momentum (lab). for Q**2 > 25 GeV**2.

Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of pseudorapidity (lab). for Q**2 from 5 to 25 GeV**2.

Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.

Differential LAMBDA/LAMBDABAR cross section in DIS eventsas a function of Bjorken X. for Q**2 from 5 to 25 GeV**2.

Differential LAMBDA/LAMBDABAR cross section in DIS eventsas a function of Bjorken X. for Q**2 > 25 GeV**2.

Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of Q**2. for Q**2 > 5 GeV**2.

Differential K0S cross section in photoproduction events as a function of transverse momentum (lab).

Differential K0S cross section in photoproduction events as a function of pseudorapidity (lab).

Differential K0S cross section in photoproduction events as a function of XOBS(C=GAMMA).

Differential LAMBDA/LAMBDABAR cross section in photoproduction events as a function of transverse momentum (lab).

Differential LAMBDA/LAMBDABAR cross section in photoproduction events as a function of pseudorapidity (lab).

Differential LAMBDA/LAMBDABAR cross section in photoproduction events as a function of XOBS(C=GAMMA).

Asymmetry in LAMBDA/LAMBDABAR production in DIS events as a function of transverse momentum (lab). for Q**2 > 25 GeV**2.

Asymmetry in LAMBDA/LAMBDABAR production in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.

Asymmetry in LAMBDA/LAMBDABAR production in DIS events as a function of Bjorken X. for Q**2 > 25 GeV**2.

Asymmetry in LAMBDA/LAMBDABAR production in DIS events as a function of Q**2. for Q**2 > 25 GeV**2.

Asymmetry in LAMBDA/LAMBDABAR production in photoproduction events as a function of transverse momentum (lab).

Asymmetry in LAMBDA/LAMBDABAR production in photoproduction events as a function of pseudorapidity (lab).

Asymmetry in LAMBDA/LAMBDABAR production in photoproduction events as a function of XOBS(C=GAMMA).

LAMBDA/K0S production ratio in DIS events as a function of transverse momentum (lab). for Q**2 from 5 to 25 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of transverse momentum (lab). for Q**2 > 25 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of pseudorapidity (lab). for Q**2 from 5 to 25 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 5 to 25 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 > 25 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Q**2 > 5 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Bjorken X from 2.0E-5 to 3.0E-4.

LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Bjorken X from 3.0E-4 to 6.0E-4.

LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Bjorken X from 6.0E-4 to 1.4E-3.

LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Bjorken X from 1.4E-3 to 2.0E-2.

LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 5.0 to 9.5 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 9.5 to 25.0 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 25 to 100 GeV**2.

LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 100 to 500 GeV**2.

LAMBDA/K0S production ratio in photoproduction events as a function of transverse momentum (lab).

LAMBDA/K0S production ratio in photoproduction events as a function of pseudorapidity (lab).

LAMBDA/K0S production ratio in photoproduction events as a function of XOBS(C=GAMMA).

LAMBDA/K0S production ratio in photoproduction events as a function of transverse momentum (lab). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.

LAMBDA/K0S production ratio in photoproduction events as a function of transverse momentum (lab). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.

LAMBDA/K0S production ratio in photoproduction events as a function of pseudorapidity (lab). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.

LAMBDA/K0S production ratio in photoproduction events as a function of pseudorapidity (lab). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.

LAMBDA/K0S production ratio in photoproduction events as a function of XOBS(C=GAMMA). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.

LAMBDA/K0S production ratio in photoproduction events as a function of XOBS(C=GAMMA). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.

K0S/Charged particle production ratio in DIS events as a function of transverse momentum (lab). for Q**2 > 25 GeV**2.

K0S/Charged particle production ratio in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.

K0S/Charged particle production ratio in photoproduction events as a function of transverse momentum (lab).

K0S/Charged particle production ratio in photoproduction events as a function of pseudorapidity (lab).

K0S/Charged particle production ratio in photoproduction events as a function of transverse momentum (lab). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.

K0S/Charged particle production ratio in photoproduction events as a function of transverse momentum (lab). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.

K0S/Charged particle production ratio in photoproduction events as a function of pseudorapidity (lab). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.

K0S/Charged particle production ratio in photoproduction events as a function of pseudorapidity (lab). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.

Integrals of G1 over different X ranges for DEUT target at various Q*2 values. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).. The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2. Axis error includes +- 5.0/5.0 contribution.

Integrals of G1 over different X ranges for N target at various Q*2 values. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).. The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Integral of G1 for the Non-Singet contribution. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).. The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2. Axis error includes +- 5.2/5.2 contribution.

The measured and Born asymmetries for the proton target at the average values of the average values of X, Y,and Q**2 in 45 bins. DSYS includes the 5.2 PCT normalization uncertainty.

The measured and Born asymmetries for the deuterium target at the average values of the average values of X, Y,and Q**2 in 45 bins. DSYS includes the 5 PCT normalization uncertainty.

Virtual photon asymmetries A1 for the proton and deuterium targets at the average values of X,and Q**2 in 45 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).

Structure functions G1 for the proton and deuterium targets at the average values of X,and Q**2 in 45 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).

Virtual photon asymmetries A1 for the proton and deuterium targets at the average values of X,and Q**2 in 19 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Structure functions G1 for the proton and deuterium targets at the average values of X,and Q**2 in 19 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Structure functions G1 for the proton and deuterium targets at the average values of X,and Q**2 in 15 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Virtual photon asymmetries A1 for the proton and deuterium targets at the average values of X,and Q**2 in 15 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Structure functions G1(n) and G1(NS)for the proton and deuterium targets at the average values of X,and Q**2 in 45 bins. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).

Structure functions G1(n) and G1(NS)for the proton and deuterium targets at the average values of X,and Q**2 in 19 bins. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Structure functions G1(n) and G1(NS)for the proton and deuterium targets at the average values of X,and Q**2 in 15 bins. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Correlation matrix for the Asymmetry, A1 and G1 for the P target at the average values of X and Q**2 in 45 bins.

Correlation matrix for the Asymmetry, A1 and G1 for the DEUT target at the average values of X and Q**2 in 45 bins.

Correlation matrix for G1 for the P target in 19 X bins (averaged over Q**2).

Correlation matrix for G1 for the DEUT target in 19 X bins (averaged over Q**2).

Correlation matrix for G1 for the P target in 15 X bins (Q**2 > 1 GeV**2), averaged over Q**2.

Correlation matrix for G1 for the DEUT target in 15 X bins (Q**2 > 1 GeV**2), averaged over Q**2.

Collins asymmetry against PT for leading negative hadrons.

Collins asymmetry against Bjorken X for leading negative hadrons.

Collins asymmetry against Z for leading negative hadrons.

Collins asymmetry against PT for all positive hadrons.

Collins asymmetry against Bjorken X for all positive hadrons.

Collins asymmetry against Z for all positive hadrons.

Collins asymmetry against PT for leading positive hadrons.

Collins asymmetry against Bjorken X for leading positive hadrons.

Collins asymmetry against Z for leading positive hadrons.

Sivers asymmetry against PT for all negative hadrons.

Sivers asymmetry against Bjorken X for all negative hadrons.

Sivers asymmetry against Z for all negative hadrons.

Sivers asymmetry against PT for leading negative hadrons.

Sivers asymmetry against Bjorken X for leading negative hadrons.

Sivers asymmetry against Z for leading negative hadrons.

Sivers asymmetry against PT for all positive hadrons.

Sivers asymmetry against Bjorken X for all positive hadrons.

Sivers asymmetry against Z for all positive hadrons.

Sivers asymmetry against PT for leading positive hadrons.

Sivers asymmetry against Bjorken X for leading positive hadrons.

Sivers asymmetry against Z for leading positive hadrons.

Differential cross sections for non-radiative E+ E- --> E+ E- events at centre of mass energy 196 GeV.

Differential cross sections for non-radiative E+ E- --> E+ E- events at centre of mass energy 200 GeV.

Differential cross sections for non-radiative E+ E- --> E+ E- events at centre of mass energy 202 GeV.

Differential cross sections for non-radiative E+ E- --> E+ E- events at centre of mass energy 205 GeV.

Differential cross sections for non-radiative E+ E- --> E+ E- events at centre of mass energy 207 GeV.

Measured cross sections and forward-backward asymmetries for inclusive E+ E- --> MU+ MU- events.

Measured cross sections and forward-backward asymmetries for non-radiative E+ E- --> MU+ MU- events.

Differential cross sections for non-radiative E+ E- --> MU+ MU- events at centre of mass energy 183 GeV.

Differential cross sections for non-radiative E+ E- --> MU+ MU- events at centre of mass energy 189 GeV.

Differential cross sections for non-radiative E+ E- --> MU+ MU- events at centre of mass energy 192 GeV.

Differential cross sections for non-radiative E+ E- --> MU+ MU- events at centre of mass energy 196 GeV.

Differential cross sections for non-radiative E+ E- --> MU+ MU- events at centre of mass energy 200 GeV.

Differential cross sections for non-radiative E+ E- --> MU+ MU- events at centre of mass energy 202 GeV.

Differential cross sections for non-radiative E+ E- --> MU+ MU- events at centre of mass energy 205 GeV.

Differential cross sections for non-radiative E+ E- --> MU+ MU- events at centre of mass energy 207 GeV.

Measured cross sections and forward-backward asymmetries for inclusive E+ E- --> TAU+ TAU- events.

Measured cross sections and forward-backward asymmetries for non-radiative E+ E- --> TAU+ TAU- events.

Differential cross sections for non-radiative E+ E- --> TAU+ TAU- events atcentre of mass energy 183 GeV.

Differential cross sections for non-radiative E+ E- --> TAU+ TAU- events atcentre of mass energy 189 GeV.

Differential cross sections for non-radiative E+ E- --> TAU+ TAU- events atcentre of mass energy 192 GeV.

Differential cross sections for non-radiative E+ E- --> TAU+ TAU- events atcentre of mass energy 196 GeV.

Differential cross sections for non-radiative E+ E- --> TAU+ TAU- events atcentre of mass energy 200 GeV.

Differential cross sections for non-radiative E+ E- --> TAU+ TAU- events atcentre of mass energy 202 GeV.

Differential cross sections for non-radiative E+ E- --> TAU+ TAU- events atcentre of mass energy 205 GeV.

Differential cross sections for non-radiative E+ E- --> TAU+ TAU- events atcentre of mass energy 207 GeV.

Measured values of the inclusive and non radiative cross sections for the process E+ E- --> Q QBAR.

Measured MU+ MU- cross section for the high-energy data sample.

Measured TAU+ TAU- cross section for the inclusive data sample.

Measured TAU+ TAU- cross section for the high-energy data sample.

Measured E+ E- --> E+ E- cross section for the inclusive data sample.

Measured E+ E- --> E+ E- cross section for the high-energy data sample.

Measured Forward-Backward asymmetry in MU+ MU- production from the inclusive data sample.

Measured Forward-Backward asymmetry in MU+ MU- production from the high-energy data sample.

Measured Forward-Backward asymmetry in TAU+ TAU- production from the inclusive data sample.

Measured Forward-Backward asymmetry in TAU+ TAU- production from the high-energy data sample.

Measured Forward-Backward asymmetry in E+ E- production for the inclusive data sample.

Measured Forward-Backward asymmetry in E+ E- production for the high-energy data sample.

Differential cross sections for E+ E- production as a function of the scattering angle for the high-energy data sample for centre of mass energy 192 GeV.

Differential cross sections for E+ E- production as a function of the scattering angle for the high-energy data sample for centre of mass energy 196 GeV.

Differential cross sections for E+ E- production as a function of the scattering angle for the high-energy data sample for centre of mass energy 200 GeV.

Differential cross sections for E+ E- production as a function of the scattering angle for the high-energy data sample for centre of mass energy 202 GeV.

Differential cross sections for E+ E- production as a function of the scattering angle for the high-energy data sample for centre of mass energy 205 GeV.

Differential cross sections for E+ E- production as a function of the scattering angle for the high-energy data sample for centre of mass energy 207 GeV.

Differential cross sections for E+ E- production as a function of the scattering angle for the high-energy data sample for centre of mass energy 208 GeV.

Asymmetries as a function of X for ALL hadrons.

Asymmetries as a function of Z for ALL hadrons.

Asymmetries as a function of PT for ALL hadrons.

The cross section for tau+ tau- production corrected to the simple kinematic acceptance region defined by N = M(P=3_4)**2/S > 0.01. Statistical errors onlyare shown. Also given is the cross section value corrected for the beam energy spread to correspond to the physical cross section at the central value of SQRT(S).

The forward-backward charge asymmetry in E+ E- --> MU+ MU- production corrected to the simple kinematic acceptance region ABS(COS(THETA(P=5))) < 0.95 and THETA(C=ACOL) < 15 degrees, and the energy of each fermion required to be greaterthan 6 GeV. Statistical errors only are shown. Also given are the asymmetries a fter correction for the beam energy spread to correspond to the physical asymmetry at the central value of SQRT(S).

The forward-backward charge asymmetry in E+ E- --> TAU+ TAU- production corrected to the simple kinematic acceptance region ABS(COS(THETA(P=5))) < 0.90 andTHETA(C=ACOL) < 15 degrees, and the energy of each fermion required to be great er than 6 GeV. Statistical errors only are shown. Also given are the asymmetriesafter correction for the beam energy spread to correspond to the physical asymm etry at the central value of SQRT(S).

The forward-backward charge asymmetry in E+ E- --> E+ E- production corrected to the simple kinematic acceptance region ABS(COS(THETA(P=5))) < 0.70 and THETA(C=ACOL) < 10 degrees, and the energy of each fermion required to be greater than 6 GeV. Statistical errors only are shown. Also given are the asymmetries after correction for the beam energy spread to correspond to the physical asymmetryat the central value of SQRT(S).

The pole asymmetry for the 1996 data sets.

The combined value of the pole asymmetry and effective electroweak mixing angle using all data sets.

The value of the pole asymmetry and effective electroweak mixing angle obtained by combining the present results with previous SLD measurements.

No description provided.

No description provided.

No description provided.

No description provided.

Cross sections for hadron production from the 1995 data. The first DSYS error is the uncorrelated part of the systematic error. The second DSYS error is from the statistical error on the absolute luminosity. In addition there is a fully correlated multiplicative contribution to the systematic error of 0.039 PCT plus an absolute uncertainty of 3.2pb together with an additional error from the absolute luminosity of 0.091 PCT.

Cross sections for mu+ mu- production from the 1993 data extrapolated to full phase space. The DSYS error is the uncorrelated part of the systematic error.In addition there is a fully correlated multiplicative contribution to the syst ematic error of 0.31 PCT plus an absolute uncertainty of 0.3pb.

Cross sections for mu+ mu- production from the 1994 data extrapolated to full phase space. The DSYS error is the uncorrelated part of the systematic error.In addition there is a fully correlated multiplicative contribution to the syst ematic error of 0.31 PCT plus an absolute uncertainty of 0.3pb.

Cross sections for mu+ mu- production from the 1995 data extrapolated to full phase space. The DSYS error is the uncorrelated part of the systematic error.In addition there is a fully correlated multiplicative contribution to the syst ematic error of 0.36 PCT plus an absolute uncertainty of 0.3pb.

Cross sections for tau+ tau- production from the 1993 data extrapolated to full phase space. The DSYS error is the uncorrelated part of the systematic error. In addition there is a fully correlated multiplicative contribution to the systematic error of 0.57 PCT plus an absolute uncertainty of 1.2pb.

Cross sections for tau+ tau- production from the 1994 data extrapolated to full phase space. The DSYS error is the uncorrelated part of the systematic error. In addition there is a fully correlated multiplicative contribution to the systematic error of 0.57 PCT plus an absolute uncertainty of 1.2pb.

Cross sections for tau+ tau- production from the 1995 data extrapolated to full phase space. The DSYS error is the uncorrelated part of the systematic error. In addition there is a fully correlated multiplicative contribution to the systematic error of 0.57 PCT plus an absolute uncertainty of 1.2pb.

Cross sections for e+ e- production from the 1993 data in the fiducial volume (THETA) 44 to 136 degrees and (PSI) < 25 degrees. The DSYS error is the uncorrelated part of the systematic error. In addition there is a fully correlated multiplicative contribution to the systematic error of 0.14 PCT. The right hand column gives the s-channel contribution to the total cross section in the full solid angle with its statistcal error.

Cross sections for e+ e- production from the 1994 data in the fiducial volume (THETA) 44 to 136 degrees and (PSI) < 25 degrees. The DSYS error is the uncorrelated part of the systematic error. In addition there is a fully correlated multiplicative contribution to the systematic error of 0.14 PCT. The right hand column gives the s-channel contribution to the total cross section in the full solid angle with its statistcal error.

Cross sections for e+ e- production from the 1995 data in the fiducial volume (THETA) 44 to 136 degrees and (PSI) < 25 degrees. The DSYS error is the uncorrelated part of the systematic error. In addition there is a fully correlated multiplicative contribution to the systematic error of 0.23 PCT. The right hand column gives the s-channel contribution to the total cross section in the full solid angle with its statistcal error.

Forward-Backward Asymmetries of mu+ mu- production from the 1993 data including an acollinearity cut of PSI < 15 degrees. The errors are statistical only and there is an additional correlated absolute error of 0.0008 to be added.

Forward-Backward Asymmetries of mu+ mu- production from the 1994 data including an acollinearity cut of PSI < 15 degrees. The errors are statistical only and there is an additional correlated absolute error of 0.0008 to be added.

Forward-Backward Asymmetries of mu+ mu- production from the 1995 data including an acollinearity cut of PSI < 15 degrees. The errors are statistical only and there is an additional correlated absolute error of 0.0015 to be added.

Forward-Backward Asymmetries of tau+ tau- production from the 1993 data including an acollinearity cut of PSI < 10 degrees. The errors are statistical onlyand there is an additional correlated absolute error of 0.0032 to be added.

Forward-Backward Asymmetries of tau+ tau- production from the 1994 data including an acollinearity cut of PSI < 10 degrees. The errors are statistical onlyand there is an additional correlated absolute error of 0.0032 to be added.

Forward-Backward Asymmetries of tau+ tau- production from the 1995 data including an acollinearity cut of PSI < 10 degrees. The errors are statistical onlyand there is an additional correlated absolute error of 0.0032 to be added.

Forward-Backward Asymmetries of e+ e- production from the 1993 data in the fiducial volume THETA from 44 to 136 degrees and including an acollinearity cut of PSI < 25 degrees. The errors are statistical only and there is an additional correlated absolute error of 0.0025 to be added. The right most column is the s-channel contribution in the full solid angle.

Forward-Backward Asymmetries of e+ e- production from the 1994 data in the fiducial volume THETA from 44 to 136 degrees and including an acollinearity cut of PSI < 25 degrees. The errors are statistical only and there is an additional correlated absolute error of 0.0025 to be added. The right most column is the s-channel contribution in the full solid angle.

Forward-Backward Asymmetries of e+ e- production from the 1995 data in the fiducial volume THETA from 44 to 136 degrees and including an acollinearity cut of PSI < 25 degrees. The errors are statistical only and there is an additional correlated absolute error of 0.0025 to be added. The right most column is the s-channel contribution in the full solid angle.

Cross section and forward-backward asymmetry in the E+ E- channel for the 1993 data. The polar angle is 44 to 136 degrees. Additional systematic error for cross section of 0.46 PCT (efficiencies and backgrounds) and 0.29 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0026.

Cross section and forward-backward asymmetry in the E+ E- channel for the 1994 data. The polar angle is 44 to 136 degrees. Additional systematic error for cross section of 0.52 PCT (efficiencies and backgrounds) and 0.14 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0021.

Cross section and forward-backward asymmetry in the E+ E- channel for the 1995 data. The polar angle is 44 to 136 degrees. Additional systematic error for cross section of 0.52 PCT (efficiencies and backgrounds) and 0.14 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0020.

Cross section and forward-backward asymmetry in the MU+ MU- channel for the1993 data. The polar angle is 20 to 160 degrees. Additional systematic error for cross section of 0.28 PCT (efficiencies and backgrounds) and 0.29 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0009.

Cross section and forward-backward asymmetry in the MU+ MU- channel for the1994 data. The polar angle is 20 to 160 degrees. Additional systematic error for cross section of 0.26 PCT (efficiencies and backgrounds) and 0.14 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0005.

Cross section and forward-backward asymmetry in the MU+ MU- channel for the1995 data. The polar angle is 20 to 160 degrees. Additional systematic error for cross section of 0.28 PCT (efficiencies and backgrounds) and 0.14 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0011.

Cross section and forward-backward asymmetry in the TAU+ TAU- channel for the 1993 data. Additional systematic error for cross section of 0.60 PCT (efficiencies and backgrounds) and 0.29 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0020.

Cross section and forward-backward asymmetry in the TAU+ TAU- channel for the 1994 data. Additional systematic error for cross section of 0.60 PCT (efficiencies and backgrounds) and 0.14 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0020.

Cross section and forward-backward asymmetry in the TAU+ TAU- channel for the 1995 data. Additional systematic error for cross section of 0.60 PCT (efficiencies and backgrounds) and 0.14 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0020.

Measurement of the observed Born cross section for the 1992-1995 data from the ISR events. SPRIME is the reduced energy after the ISR.

Measurement of the forward-backward asymmetry for the 1991 to 1995 data from the ISR events.

Measured cross sections for the electron-pair events. For Bhabha scattering events both the leptons have to be inside 44 to 136 degrees.

Forward backward asymmetry for lepton-pair events.

Measured cross sections for the tau-pair events.

Measured cross sections for the electron-pair events. For Bhabha scattering events both the leptons have to be inside 44 to 136 degrees.

Angular distributions for (MU+ MU-) and (TAU+ TAU-) events for the inclusive data sample. Statistical and systematic errors are combined.

Angular distributions for (MU+ MU-) and (TAU+ TAU-) events for the high-energy data sample. Statistical and systematic errors are combined.

Angular distributions for (E+ E-) events for the high energy event sample (ZETA <25 DEGS) Statistical and systematic errors are combined.

No description provided.

The quoted uncertaintis include statistical and systematic components.

No description provided.

No description provided.

No description provided.

No description provided.

No description provided.

No description provided.

The virtual photon deuteron asymmetries in smaller X an Q**2 bins. Errors are statistical only.

The spin-dependent proton structure function G1.

The spin-dependent structure function G1(P) evolved to Q**2=10 GeV**2.. The second systematic (DSYS) error is due to the uncertainty in the QCD evolution.

The spin-dependent deuteron structure function G1.

The spin-dependent structure function G1(D) evolved to Q**2=10 GeV**2. The second systematic (DSYS) error is due to the uncertainty in the QCD evolution.

No description provided.

The nonsinglet spin-dependent structure function G1(NS) calculated from themeasured the G1(P) and G1(D).

The nonsinglet spin-dependent structure function G1(NS) evolved to Q**2=10 GeV**2.. The second systematic (DSYS) error is due to the uncertainty in the QCD evolution.

The first moment integral for the nonsinglet structure function G1(NS).

G1 is evolved to Q2= 10 GEV**2, second DSYS for this value indicates the uncertainty in the QCD evolution. Regge behavior and QCD approach were used to obtaint the values at low X.

Errors include statistical and systematic effects combined, with the formerdominant.

Errors include statistical and systematic effects combined, with the formerdominant. The data are corrected to no interference between initial- and final-stateradiation. See text for explanation.

Errors include statistical and systematic effects combined, with the formerdominant. The data are corrected to no interference between initial- and final-stateradiation. See text for explanation.

Errors include statistical and systematic effects combined, with the formerdominant.

SIG(C=MEAS) and SIG(C=CORR) stand for measured values without (C=MEAS) and with (C=CORR) correction for interference between initial- and final-state radiation.

ASYM(C=MEAS) and ASYM(C=CORR) stand for measured values without (C=MEAS) and with (C=CORR) correction for interference between initial- and final-state radiation.

ASYM(C=MEAS) and ASYM(C=CORR) stand for measured values without (C=MEAS) and with (C=CORR) correction for interference between initial- and final-state radiation.

ASYM(C=MEAS) and ASYM(C=CORR) stand for measured values without (C=MEAS) and with (C=CORR) correction for interference between initial- and final-state radiation.

SIG(C=MEAS) and SIG(C=CORR) stand for measured values without (C=MEAS) and with (C=CORR) correction for interference between initial- and final-state radiation.

No description provided.

No description provided.

No description provided.