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

The covariance matrix for the kinematic bins matrix of the $D_s^+$ production asymmetry measured using the combined $\sqrt{s} =7$ and 8 TeV data sets (corresponding to Table 1). The statistical and systematic uncertainties are combined. The kinematic bins are indexed as follows: the three rapidity bins, y, in the range from 2.0 to 4.5 are indexed with $i_y$ ranging from 0 to 2 with the following bin edges: 2.0, 3.0, 3.5, 4.5. The four $p_{\rm T}$ bins in the range from 2.5 to 25.0 GeV/c are indexed with $i_{p_T}$ from 0 to 3 with the following bin edges: 2.5, 4.7, 6.5, 8.5, 25.0 GeV/c. The index of a kinematic bins is then given by: $i_{\rm bin} = 4 \times i_y + i_{p_T}$.

The covariance matrix for the kinematic bins matrix of the $D_s^+$ production asymmetry measured using the $\sqrt{s} =7$ TeV data set (corresponding to Table 2). The statistical and systematic uncertainties are combined. The kinematic bins are indexed as follows: the three rapidity bins, y, in the range from 2.0 to 4.5 are indexed with $i_y$ ranging from 0 to 2 with the following bin edges: 2.0, 3.0, 3.5, 4.5. The four $p_{\rm T}$ bins in the range from 2.5 to 25.0 GeV/c are indexed with $i_{p_T}$ from 0 to 3 with the following bin edges: 2.5, 4.7, 6.5, 8.5, 25.0 GeV/c. The index of a kinematic bins is then given by: $i_{\rm bin} = 4 \times i_y + i_{p_T}$.

The covariance matrix for the kinematic bins matrix of the $D_s^+$ production asymmetry measured using the $\sqrt{s} =8$ TeV data set (corresponding to Table 3). The statistical and systematic uncertainties are combined. The kinematic bins are indexed as follows: the three rapidity bins, y, in the range from 2.0 to 4.5 are indexed with $i_y$ ranging from 0 to 2 with the following bin edges: 2.0, 3.0, 3.5, 4.5. The four $p_{\rm T}$ bins in the range from 2.5 to 25.0 GeV/c are indexed with $i_{p_T}$ from 0 to 3 with the following bin edges: 2.5, 4.7, 6.5, 8.5, 25.0 GeV/c. The index of a kinematic bins is then given by: $i_{\rm bin} = 4 \times i_y + i_{p_T}$.

The particle-level di-jet differential cross section. The systematic uncertainty on the data contains contributions from track finding efficiency, track transverse momentum resolution, calorimeter energy resolution, and unfolding uncertainties. For the theory, values are given for the underlying event and hadronization (UEH) correction uncertainty and the quadrature sum of the UEH and theoretical uncertainties. Both the UEH and theoretical uncertainties include contributions from factorization and renormalization scale uncertainties and PDF uncertainties. An 8.8% uncertainty common to all points due to the integrated luminosity determination is also present, but not included in the systematic values quoted below.

Values of gluon X1 and X2 obtained from the PYTHIA detector-level simulation for the same-sign di-jet topology compared to the gluon X distribution for inclusive jets. The inclusive distribution has been scaled down by a factor of 20 compared to the di-jet distributions.

Values of gluon X1 and X2 obtained from the PYTHIA detector-level simulation for the opposite-sign di-jet topology compared to the gluon X distribution for inclusive jets. The inclusive distribution has been scaled down by a factor of 20 compared to the di-jet distributions.

Di-jet A_LL asymmetry vs parton-level invariant mass for the same-sign di-jet topology. The systematic uncertainty on the mass includes contributions from jet energy scale, the correction to parton-level, and the difference between NLO and PYTHIA cross sections. The systematic uncertainty on the asymmetry includes contributions from trigger and reconstruction bias and residual transverse beam polarization components. A 6.5% uncertainty common to all points due to uncertainty on the measured beam polarizations is also present, but not included in the uncertainties quoted below.

Theoretical predictions for the di-jet A_LL asymmetry for the same-sign topology using the DSSV14 and NNPDFpol1.1 polarized PDF sets. The DSSV14 prediction is presented without uncertainty while the systematic uncertainty on the NNPDFpol1.1 prediction contains contributions from factorization and renormalization scale uncertainties and PDF uncertainties.

Di-jet A_LL asymmetry vs parton-level invariant mass for the opposite-sign di-jet topology. The systematic uncertainty on the mass includes contributions from jet energy scale, the correction to parton-level, and the difference between NLO and PYTHIA cross sections. The systematic uncertainty on the asymmetry includes contributions from trigger and reconstruction bias and residual transverse beam polarization components. A 6.5% uncertainty common to all points due to uncertainty on the measured beam polarizations is also present, but not included in the uncertainties quoted below.

Theoretical predictions for the di-jet A_LL asymmetry for the opposite-sign topology using the DSSV14 and NNPDFpol1.1 polarized PDF sets. The DSSV14 prediction is presented without uncertainty while the systematic uncertainty on the NNPDFpol1.1 prediction contains contributions from factorization and renormalization scale uncertainties and PDF uncertainties.

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