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. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{t\bar{t}}$ vs $p_{T,t\bar{t}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{t\bar{t}}$ vs $\beta_{z,t\bar{t}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{\ell\ell}$ vs $m_{\ell\bar{\ell}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{\ell\ell}$ vs $p_{T,\ell\bar{\ell}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Covariance matrix for the $A_C^{\ell\ell}$ vs $\beta_{z,\ell\bar{\ell}}$ measurement. The total (stat. + syst.) uncertainties are considered.

Photon beam asymmetry Sigma at W= 1.3147 GeV

Photon beam asymmetry Sigma at W= 1.3289 GeV

Photon beam asymmetry Sigma at W= 1.3430 GeV

Photon beam asymmetry Sigma at W= 1.3569 GeV

Photon beam asymmetry Sigma at W= 1.3707 GeV

Photon beam asymmetry Sigma at W= 1.3843 GeV

Photon beam asymmetry Sigma at W= 1.3978 GeV

Photon beam asymmetry Sigma at W= 1.4112 GeV

Photon beam asymmetry Sigma at W= 1.4244 GeV

Photon beam asymmetry Sigma at W=1.2254987 GeV

Photon beam asymmetry Sigma at W=1.2290003 GeV

Photon beam asymmetry Sigma at W=1.2324995 GeV

Photon beam asymmetry Sigma at W=1.2355029 GeV

Photon beam asymmetry Sigma at W=1.2389989 GeV

Photon beam asymmetry Sigma at W=1.2425001 GeV

Photon beam asymmetry Sigma at W=1.2455020 GeV

Photon beam asymmetry Sigma at W=1.2484967 GeV

Photon beam asymmetry Sigma at W=1.2514991 GeV

Photon beam asymmetry Sigma at W=1.2550029 GeV

Photon beam asymmetry Sigma at W=1.2584969 GeV

Photon beam asymmetry Sigma at W=1.2614979 GeV

Photon beam asymmetry Sigma at W=1.2644992 GeV

Photon beam asymmetry Sigma at W=1.2675008 GeV

Photon beam asymmetry Sigma at W=1.2705027 GeV

Photon beam asymmetry Sigma at W=1.2739984 GeV

Photon beam asymmetry Sigma at W=1.2774992 GeV

Photon beam asymmetry Sigma at W=1.2804996 GeV

Photon beam asymmetry Sigma at W=1.2835003 GeV

Photon beam asymmetry Sigma at W=1.2864940 GeV

Photon beam asymmetry Sigma at W=1.2895026 GeV

Photon beam asymmetry Sigma at W=1.2924970 GeV

Photon beam asymmetry Sigma at W=1.2954989 GeV

Photon beam asymmetry Sigma at W=1.2989995 GeV

Photon beam asymmetry Sigma at W=1.3024980 GeV

Photon beam asymmetry Sigma at W=1.3054984 GeV

Photon beam asymmetry Sigma at W=1.3084992 GeV

Photon beam asymmetry Sigma at W=1.3115002 GeV

Photon beam asymmetry Sigma at W=1.3145016 GeV

Photon beam asymmetry Sigma at W=1.3175032 GeV

Photon beam asymmetry Sigma at W=1.3204980 GeV

Photon beam asymmetry Sigma at W=1.3235001 GeV

Photon beam asymmetry Sigma at W=1.3265026 GeV

Photon beam asymmetry Sigma at W=1.3294983 GeV

Photon beam asymmetry Sigma at W=1.3325013 GeV

Photon beam asymmetry Sigma at W=1.3354976 GeV

Photon beam asymmetry Sigma at W=1.3385012 GeV

Photon beam asymmetry Sigma at W=1.3414981 GeV

Photon beam asymmetry Sigma at W=1.3445022 GeV

Photon beam asymmetry Sigma at W=1.3474997 GeV

Photon beam asymmetry Sigma at W=1.3504974 GeV

Photon beam asymmetry Sigma at W=1.3535024 GeV

Photon beam asymmetry Sigma at W=1.3565007 GeV

Photon beam asymmetry Sigma at W=1.3594993 GeV

Photon beam asymmetry Sigma at W=1.3624982 GeV

Photon beam asymmetry Sigma at W=1.3654974 GeV

Photon beam asymmetry Sigma at W=1.3684968 GeV

Photon beam asymmetry Sigma at W=1.3714966 GeV

Photon beam asymmetry Sigma at W=1.3744966 GeV

Photon beam asymmetry Sigma at W=1.3774969 GeV

Photon beam asymmetry Sigma at W=1.3804974 GeV

Photon beam asymmetry Sigma at W=1.3834983 GeV

Photon beam asymmetry Sigma at W=1.3864994 GeV

Photon beam asymmetry Sigma at W=1.3890010 GeV

Photon beam asymmetry Sigma at W=1.3914981 GeV

Photon beam asymmetry Sigma at W=1.3945022 GeV

Photon beam asymmetry Sigma at W=1.3974998 GeV

Photon beam asymmetry Sigma at W=1.4004978 GeV

Photon beam asymmetry Sigma at W=1.4035026 GeV

Photon beam asymmetry Sigma at W=1.4065011 GeV

Photon beam asymmetry Sigma at W=1.4094998 GeV

Photon beam asymmetry Sigma at W=1.4119939 GeV

Photon beam asymmetry Sigma at W=1.4144969 GeV

Photon beam asymmetry Sigma at W=1.4174985 GeV

Photon beam asymmetry Sigma at W=1.4205005 GeV

Photon beam asymmetry Sigma at W=1.4235027 GeV

Photon beam asymmetry Sigma at W=1.4259986 GeV

Photon beam asymmetry Sigma at W=1.4284967 GeV

Photon beam asymmetry Sigma at W=1.4315018 GeV

Photon beam asymmetry Sigma at W=1.4345006 GeV

Photon beam asymmetry Sigma at W=1.4374997 GeV

Photon beam asymmetry Sigma at W=1.4399974 GeV

Photon beam asymmetry Sigma at W=1.4424973 GeV

Photon beam asymmetry Sigma at W=1.4454993 GeV

Photon beam asymmetry Sigma at W=1.4485015 GeV

Target asymmetry T for c.m. energy W= 1.3693 GeV

Target asymmetry T for c.m. energy W= 1.3897 GeV

Target asymmetry T for c.m. energy W= 1.4098 GeV

Target asymmetry T for c.m. energy W= 1.4296 GeV

Target asymmetry T for c.m. energy W= 1.4492 GeV

Target asymmetry T for c.m. energy W= 1.4685 GeV

Target asymmetry T for c.m. energy W= 1.4875 GeV

Target asymmetry T for c.m. energy W= 1.5063 GeV

Target asymmetry T for c.m. energy W= 1.5249 GeV

Target asymmetry T for c.m. energy W= 1.5432 GeV

Target asymmetry T for c.m. energy W= 1.5614 GeV

Target asymmetry T for c.m. energy W= 1.5793 GeV

Target asymmetry T for c.m. energy W= 1.5970 GeV

Target asymmetry T for c.m. energy W= 1.6146 GeV

Target asymmetry T for c.m. energy W= 1.6319 GeV

Target asymmetry T for c.m. energy W= 1.6491 GeV

Target asymmetry T for c.m. energy W= 1.6660 GeV

Target asymmetry T for c.m. energy W= 1.6828 GeV

Target asymmetry T for c.m. energy W= 1.6995 GeV

Target asymmetry T for c.m. energy W= 1.7160 GeV

Target asymmetry T for c.m. energy W= 1.7323 GeV

Target asymmetry T for c.m. energy W= 1.7485 GeV

Target asymmetry T for c.m. energy W= 1.7645 GeV

Target asymmetry T for c.m. energy W= 1.7804 GeV

Target asymmetry T for c.m. energy W= 1.7961 GeV

Target asymmetry T for c.m. energy W= 1.8117 GeV

Target asymmetry T for c.m. energy W= 1.8272 GeV

Target asymmetry T for c.m. energy W= 1.8425 GeV

Target asymmetry T for c.m. energy W= 1.8577 GeV

Target asymmetry T for c.m. energy W= 1.8728 GeV

Target asymmetry T for c.m. energy W= 1.8878 GeV

Beam-target asymmetry F for c.m. energy W= 1.3062 GeV

Beam-target asymmetry F for c.m. energy W= 1.3275 GeV

Beam-target asymmetry F for c.m. energy W= 1.3486 GeV

Beam-target asymmetry F for c.m. energy W= 1.3693 GeV

Beam-target asymmetry F for c.m. energy W= 1.3897 GeV

Beam-target asymmetry F for c.m. energy W= 1.4098 GeV

Beam-target asymmetry F for c.m. energy W= 1.4296 GeV

Beam-target asymmetry F for c.m. energy W= 1.4492 GeV

Beam-target asymmetry F for c.m. energy W= 1.4685 GeV

Beam-target asymmetry F for c.m. energy W= 1.4875 GeV

Beam-target asymmetry F for c.m. energy W= 1.5063 GeV

Beam-target asymmetry F for c.m. energy W= 1.5249 GeV

Beam-target asymmetry F for c.m. energy W= 1.5432 GeV

Beam-target asymmetry F for c.m. energy W= 1.5614 GeV

Beam-target asymmetry F for c.m. energy W= 1.5793 GeV

Beam-target asymmetry F for c.m. energy W= 1.5970 GeV

Beam-target asymmetry F for c.m. energy W= 1.6146 GeV

Beam-target asymmetry F for c.m. energy W= 1.6319 GeV

Beam-target asymmetry F for c.m. energy W= 1.6491 GeV

Beam-target asymmetry F for c.m. energy W= 1.6660 GeV

Beam-target asymmetry F for c.m. energy W= 1.6828 GeV

Beam-target asymmetry F for c.m. energy W= 1.6995 GeV

Beam-target asymmetry F for c.m. energy W= 1.7160 GeV

Beam-target asymmetry F for c.m. energy W= 1.7323 GeV

Beam-target asymmetry F for c.m. energy W= 1.7485 GeV

Beam-target asymmetry F for c.m. energy W= 1.7645 GeV

Beam-target asymmetry F for c.m. energy W= 1.7804 GeV

Beam-target asymmetry F for c.m. energy W= 1.7961 GeV

Beam-target asymmetry F for c.m. energy W= 1.8117 GeV

Beam-target asymmetry F for c.m. energy W= 1.8272 GeV

Beam-target asymmetry F for c.m. energy W= 1.8425 GeV

Beam-target asymmetry F for c.m. energy W= 1.8577 GeV

Beam-target asymmetry F for c.m. energy W= 1.8728 GeV

Beam-target asymmetry F for c.m. energy W= 1.8878 GeV

Target asymmetry T for c.m. cos(Theta_pi0)= 0.819

Target asymmetry T for c.m. cos(Theta_pi0)= 0.707

Target asymmetry T for c.m. cos(Theta_pi0)= 0.574

Target asymmetry T for c.m. cos(Theta_pi0)= 0.423

Target asymmetry T for c.m. cos(Theta_pi0)= 0.259

Target asymmetry T for c.m. cos(Theta_pi0)= 0.087

Target asymmetry T for c.m. cos(Theta_pi0)= -0.087

Target asymmetry T for c.m. cos(Theta_pi0)= -0.259

Target asymmetry T for c.m. cos(Theta_pi0)= -0.423

Target asymmetry T for c.m. cos(Theta_pi0)= -0.574

Target asymmetry T for c.m. cos(Theta_pi0)= -0.707

Target asymmetry T for c.m. cos(Theta_pi0)= -0.819

Target asymmetry T for c.m. cos(Theta_pi0)= -0.906

Target asymmetry T for c.m. cos(Theta_pi0)= -0.966

Target asymmetry T for c.m. cos(Theta_pi0)= -0.996

Target asymmetry T for c.m. energy W= 1.5584 GeV

Target asymmetry T for c.m. energy W= 1.5882 GeV

Target asymmetry T for c.m. energy W= 1.6175 GeV

Target asymmetry T for c.m. energy W= 1.6462 GeV

Target asymmetry T for c.m. energy W= 1.6745 GeV

Target asymmetry T for c.m. energy W= 1.7022 GeV

Target asymmetry T for c.m. energy W= 1.7431 GeV

Target asymmetry T for c.m. energy W= 1.7961 GeV

Target asymmetry T for c.m. energy W= 1.8476 GeV

Beam-target asymmetry F for c.m. energy W= 1.4969 GeV

Beam-target asymmetry F for c.m. energy W= 1.5156 GeV

Beam-target asymmetry F for c.m. energy W= 1.5341 GeV

Beam-target asymmetry F for c.m. energy W= 1.5584 GeV

Beam-target asymmetry F for c.m. energy W= 1.5882 GeV

Beam-target asymmetry F for c.m. energy W= 1.6175 GeV

Beam-target asymmetry F for c.m. energy W= 1.6462 GeV

Beam-target asymmetry F for c.m. energy W= 1.6745 GeV

Beam-target asymmetry F for c.m. energy W= 1.7022 GeV

Beam-target asymmetry F for c.m. energy W= 1.7431 GeV

Beam-target asymmetry F for c.m. energy W= 1.7961 GeV

Beam-target asymmetry F for c.m. energy W= 1.8476 GeV

Differential cross section at W=1.0813873 GeV

Differential cross section at W=1.0834244 GeV

Differential cross section at W=1.0854490 GeV

Differential cross section at W=1.0874871 GeV

Differential cross section at W=1.0895214 GeV

Differential cross section at W=1.0915347 GeV

Differential cross section at W=1.0935786 GeV

Differential cross section at W=1.0956101 GeV

Differential cross section at W=1.0976464 GeV

Differential cross section at W=1.0996192 GeV

Differential cross section at W=1.1016993 GeV

Differential cross section at W=1.1037073 GeV

Differential cross section at W=1.1057288 GeV

Differential cross section at W=1.1077549 GeV

Differential cross section at W=1.1097605 GeV

Differential cross section at W=1.1117962 GeV

Differential cross section at W=1.1137946 GeV

Differential cross section at W=1.1158229 GeV

Differential cross section at W=1.1178392 GeV

Differential cross section at W=1.1198602 GeV

Differential cross section at W=1.1218776 GeV

Differential cross section at W=1.1238330 GeV

Differential cross section at W=1.1258932 GeV

Differential cross section at W=1.1278915 GeV

Differential cross section at W=1.1299029 GeV

Differential cross section at W=1.1339149 GeV

Differential cross section at W=1.1359156 GeV

Photon beam asymmetry Sigma at W=1.0752268 GeV

Photon beam asymmetry Sigma at W=1.0773190 GeV

Photon beam asymmetry Sigma at W=1.0793464 GeV

Photon beam asymmetry Sigma at W=1.0813873 GeV

Photon beam asymmetry Sigma at W=1.0834244 GeV

Photon beam asymmetry Sigma at W=1.0854490 GeV

Photon beam asymmetry Sigma at W=1.0874871 GeV

Photon beam asymmetry Sigma at W=1.0895214 GeV

Photon beam asymmetry Sigma at W=1.0915347 GeV

Photon beam asymmetry Sigma at W=1.0935786 GeV

Photon beam asymmetry Sigma at W=1.0956101 GeV

Photon beam asymmetry Sigma at W=1.0976464 GeV

Photon beam asymmetry Sigma at W=1.0996192 GeV

Photon beam asymmetry Sigma at W=1.1016993 GeV

Photon beam asymmetry Sigma at W=1.1037073 GeV

Photon beam asymmetry Sigma at W=1.1057288 GeV

Photon beam asymmetry Sigma at W=1.1077549 GeV

Photon beam asymmetry Sigma at W=1.1097605 GeV

Photon beam asymmetry Sigma at W=1.1117962 GeV

Photon beam asymmetry Sigma at W=1.1137946 GeV

Photon beam asymmetry Sigma at W=1.1158229 GeV

Photon beam asymmetry Sigma at W=1.1178392 GeV

Photon beam asymmetry Sigma at W=1.1198602 GeV

Photon beam asymmetry Sigma at W=1.1218776 GeV

Photon beam asymmetry Sigma at W=1.1238330 GeV

Photon beam asymmetry Sigma at W=1.1258932 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.