The Bose-Einstein correlation (BEC) parameter R as a function of n_ch for HMT events using different MC generators in the calculation of R₂(Q). The uncertainties shown are statistical. The lower panel of each plot shows the ratio of the BEC parameters obtained using EPOS LHC (red circles), Pythia 8 Monash (blue squares) and Herwig++ UE-EE-5 (green triangles) compared with the parameters obtained using Pythia 8 A2. The gray band in the lower panels is the MC systematic uncertainty, obtained as explained in the text.

The Bose-Einstein correlation (BEC) parameter R as a function of k_T for MB events using different MC generators in the calculation of R₂(Q). The uncertainties shown are statistical. The lower panel of each plot shows the ratio of the BEC parameters obtained using EPOS LHC (red circles), Pythia 8 Monash (blue squares) and Herwig++ UE-EE-5 (green triangles) compared with the parameters obtained using Pythia 8 A2. The gray band in the lower panels is the MC systematic uncertainty, obtained as explained in the text.

The Bose-Einstein correlation (BEC) parameter λ as a function of k_T for MB events using different MC generators in the calculation of R₂(Q). The uncertainties shown are statistical. The lower panel of each plot shows the ratio of the BEC parameters obtained using EPOS LHC (red circles), Pythia 8 Monash (blue squares) and Herwig++ UE-EE-5 (green triangles) compared with the parameters obtained using Pythia 8 A2. The gray band in the lower panels is the MC systematic uncertainty, obtained as explained in the text.

The two-particle double-ratio correlation function, R₂(Q), for pp collisions for track p_T >100 MeV at √s=13 TeV in the multiplicity interval 71 ≤ n_ch < 80 for the minimum-bias (MB) events. The blue dashed and red solid lines show the results of the exponential and Gaussian fits, respectively. The region excluded from the fits is shown. The statistical uncertainty and the systematic uncertainty for imperfections in the data reconstruction procedure are added in quadrature.

The two-particle double-ratio correlation function, R₂(Q), for pp collisions for track p_T >100 MeV at √s=13 TeV in the multiplicity interval 231 ≤ n_ch < 300 for the high-multiplicity track (HMT) events. The blue dashed and red solid lines show the results of the exponential and Gaussian fits, respectively. The region excluded from the fits is shown. The statistical uncertainty and the systematic uncertainty for imperfections in the data reconstruction procedure are added in quadrature.

The dependence of the correlation strength, λ(m_ch), on rescaled multiplicity, m_ch, obtained from the exponential fit of the R₂(Q) correlation functions for tracks with p_T > 100  MeV and p_T > 500 MeV at √s = 13  TeV for the minimum-bias (MB) and high multiplicity track (HMT) data. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the exponential fit of λ(m_ch) for p_T >100 MeV and p_T >500 MeV, respectively.

The dependence of the correlation strength, λ(m_ch), on rescaled multiplicity, m_ch, obtained from the exponential fit of the R₂(Q) correlation functions for tracks with p_T > 100  MeV and p_T > 500 MeV at √s = 13  TeV for the minimum-bias (MB) and high multiplicity track (HMT) data. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the exponential fit of λ(m_ch) for p_T >100 MeV and p_T >500 MeV, respectively.

The dependence of the correlation strength, λ(m_ch), on rescaled multiplicity, m_ch, obtained from the exponential fit of the R₂(Q) correlation functions for tracks with p_T > 100  MeV and p_T > 500 MeV at √s = 13  TeV for the minimum-bias (MB) and high multiplicity track (HMT) data. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the exponential fit of λ(m_ch) for p_T >100 MeV and p_T >500 MeV, respectively.

The dependence of the correlation strength, λ(m_ch), on rescaled multiplicity, m_ch, obtained from the exponential fit of the R₂(Q) correlation functions for tracks with p_T > 100  MeV and p_T > 500 MeV at √s = 13  TeV for the minimum-bias (MB) and high multiplicity track (HMT) data. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the exponential fit of λ(m_ch) for p_T >100 MeV and p_T >500 MeV, respectively.

The dependence of the source radius, R(m_ch), on m_ch. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the fit of R(m_ch) for ∛m_ch < 1.2 for p_T >100 MeV and p_T >500 MeV, respectively. The black and blue dotted curves are extensions of the black and blue solid curves beyond ∛m_ch > 1.2, respectively. The black and brown dashed curves represent the saturation value of R(m_ch) for ∛m_ch > 1.45 with p_T >100 MeV and for ∛m_ch > 1.6 with p_T >500 MeV, respectively.

The dependence of the source radius, R(m_ch), on m_ch. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the fit of R(m_ch) for ∛m_ch < 1.2 for p_T >100 MeV and p_T >500 MeV, respectively. The black and blue dotted curves are extensions of the black and blue solid curves beyond ∛m_ch > 1.2, respectively. The black and brown dashed curves represent the saturation value of R(m_ch) for ∛m_ch > 1.45 with p_T >100 MeV and for ∛m_ch > 1.6 with p_T >500 MeV, respectively.

The dependence of the source radius, R(m_ch), on m_ch. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the fit of R(m_ch) for ∛m_ch < 1.2 for p_T >100 MeV and p_T >500 MeV, respectively. The black and blue dotted curves are extensions of the black and blue solid curves beyond ∛m_ch > 1.2, respectively. The black and brown dashed curves represent the saturation value of R(m_ch) for ∛m_ch > 1.45 with p_T >100 MeV and for ∛m_ch > 1.6 with p_T >500 MeV, respectively.

The dependence of the source radius, R(m_ch), on m_ch. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the fit of R(m_ch) for ∛m_ch < 1.2 for p_T >100 MeV and p_T >500 MeV, respectively. The black and blue dotted curves are extensions of the black and blue solid curves beyond ∛m_ch > 1.2, respectively. The black and brown dashed curves represent the saturation value of R(m_ch) for ∛m_ch > 1.45 with p_T >100 MeV and for ∛m_ch > 1.6 with p_T >500 MeV, respectively.

The dependence of the R(m_ch) on ∛m_ch. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the fit of R(m_ch) for ∛m_ch < 1.2 for p_T >100 MeV and p_T >500 MeV, respectively. The black and blue dotted curves are extensions of the black and blue solid curves beyond ∛m_ch > 1.2, respectively. The black and brown dashed curves represent the saturation value of R(m_ch) for ∛m_ch > 1.45 with p_T >100 MeV and for ∛m_ch > 1.6 with p_T >500 MeV, respectively

The dependence of the R(m_ch) on ∛m_ch. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the fit of R(m_ch) for ∛m_ch < 1.2 for p_T >100 MeV and p_T >500 MeV, respectively. The black and blue dotted curves are extensions of the black and blue solid curves beyond ∛m_ch > 1.2, respectively. The black and brown dashed curves represent the saturation value of R(m_ch) for ∛m_ch > 1.45 with p_T >100 MeV and for ∛m_ch > 1.6 with p_T >500 MeV, respectively

The dependence of the R(m_ch) on ∛m_ch. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the fit of R(m_ch) for ∛m_ch < 1.2 for p_T >100 MeV and p_T >500 MeV, respectively. The black and blue dotted curves are extensions of the black and blue solid curves beyond ∛m_ch > 1.2, respectively. The black and brown dashed curves represent the saturation value of R(m_ch) for ∛m_ch > 1.45 with p_T >100 MeV and for ∛m_ch > 1.6 with p_T >500 MeV, respectively

The dependence of the R(m_ch) on ∛m_ch. The uncertainties represent the sum in quadrature of the statistical and asymmetric systematic contributions. The black and blue solid curves represent the fit of R(m_ch) for ∛m_ch < 1.2 for p_T >100 MeV and p_T >500 MeV, respectively. The black and blue dotted curves are extensions of the black and blue solid curves beyond ∛m_ch > 1.2, respectively. The black and brown dashed curves represent the saturation value of R(m_ch) for ∛m_ch > 1.45 with p_T >100 MeV and for ∛m_ch > 1.6 with p_T >500 MeV, respectively

Comparison of single-ratio two-particle correlation functions, using the unlike-charge particle (UCP) pair reference sample, for minimum-bias (MB) events, showing C₂^data(Q) (top panel) at 13 TeV (black circles) and 7 TeV (open blue circles), and the ratio of C₂^7 TeV (Q) to C₂^13 TeV (Q) (bottom panel). Comparison of C₂^data (Q) for representative multiplicity region 3.09 < m_ch ≤ 3.86. The statistical and systematic uncertainties, combined in quadrature, are presented. The systematic uncertainties include track efficiency, Coulomb correction, non-closure and multiplicity-unfolding uncertainties.

Comparison of single-ratio two-particle correlation functions, using the unlike-charge particle (UCP) pair reference sample, for minimum-bias (MB) events, showing C₂^data(Q) (top panel) at 13  TeV (black circles) and 7  TeV (open blue circles), and the ratio of C₂^7 TeV (Q) to C₂^13 TeV (Q) (bottom panel). Comparison of C₂^data (Q) for representative k_T region 400 < k_T ≤500  MeV. The statistical and systematic uncertainties, combined in quadrature, are presented. The systematic uncertainties include track efficiency, Coulomb correction, non-closure and multiplicity-unfolding uncertainties.

The k_T dependence of the correlation strength, λ(k_T), obtained from the exponential fit to the R₂(Q) correlation functions for events with multiplicity n_ch ≥ 2 and transfer momentum of tracks with p_T >100 MeV and p_T >500 MeV at √s=13 TeV for the minimum-bias (MB) and high-multiplicity track (HMT) events. The uncertainties represent the sum in quadrature of the statistical and systematic contributions. The curves represent the exponential fits to λ(k_T).

The k_T dependence of the correlation strength, λ(k_T), obtained from the exponential fit to the R₂(Q) correlation functions for events with multiplicity n_ch ≥ 2 and transfer momentum of tracks with p_T >100 MeV and p_T >500 MeV at √s=13 TeV for the minimum-bias (MB) and high-multiplicity track (HMT) events. The uncertainties represent the sum in quadrature of the statistical and systematic contributions. The curves represent the exponential fits to λ(k_T).

The k_T dependence of the correlation strength, λ(k_T), obtained from the exponential fit to the R₂(Q) correlation functions for events with multiplicity n_ch ≥ 2 and transfer momentum of tracks with p_T >100 MeV and p_T >500 MeV at √s=13 TeV for the minimum-bias (MB) and high-multiplicity track (HMT) events. The uncertainties represent the sum in quadrature of the statistical and systematic contributions. The curves represent the exponential fits to λ(k_T).

The k_T dependence of the correlation strength, λ(k_T), obtained from the exponential fit to the R₂(Q) correlation functions for events with multiplicity n_ch ≥ 2 and transfer momentum of tracks with p_T >100 MeV and p_T >500 MeV at √s=13 TeV for the minimum-bias (MB) and high-multiplicity track (HMT) events. The uncertainties represent the sum in quadrature of the statistical and systematic contributions. The curves represent the exponential fits to λ(k_T).

The k_T dependence of the source radius, R(k_T), obtained from the exponential fit to the R₂(Q) correlation functions for events with multiplicity n_ch ≥ 2 and transfer momentum of tracks with p_T >100 MeV and p_T >500 MeV at √s=13 TeV for the minimum-bias (MB) and high-multiplicity track (HMT) events. The uncertainties represent the sum in quadrature of the statistical and systematic contributions. The curves represent the exponential fits to R(k_T).

The k_T dependence of the source radius, R(k_T), obtained from the exponential fit to the R₂(Q) correlation functions for events with multiplicity n_ch ≥ 2 and transfer momentum of tracks with p_T >100 MeV and p_T >500 MeV at √s=13 TeV for the minimum-bias (MB) and high-multiplicity track (HMT) events. The uncertainties represent the sum in quadrature of the statistical and systematic contributions. The curves represent the exponential fits to R(k_T).

The k_T dependence of the source radius, R(k_T), obtained from the exponential fit to the R₂(Q) correlation functions for events with multiplicity n_ch ≥ 2 and transfer momentum of tracks with p_T >100 MeV and p_T >500 MeV at √s=13 TeV for the minimum-bias (MB) and high-multiplicity track (HMT) events. The uncertainties represent the sum in quadrature of the statistical and systematic contributions. The curves represent the exponential fits to R(k_T).

The k_T dependence of the source radius, R(k_T), obtained from the exponential fit to the R₂(Q) correlation functions for events with multiplicity n_ch ≥ 2 and transfer momentum of tracks with p_T >100 MeV and p_T >500 MeV at √s=13 TeV for the minimum-bias (MB) and high-multiplicity track (HMT) events. The uncertainties represent the sum in quadrature of the statistical and systematic contributions. The curves represent the exponential fits to R(k_T).

The two-dimensional dependence on m_ch and k_T for p_T > 100 MeV for the correlation strength, λ, obtained from the exponential fit to the R₂(Q) correlation functions using the MB sample for m_ch ≤ 3.08 and the HMT sample for m_ch > 3.08.

The two-dimensional dependence on m_ch and k_T for p_T > 100 MeV for the source radius, R, obtained from the exponential fit to the R₂(Q) correlation functions using the MB sample for m_ch ≤ 3.08 and the HMT sample for m_ch > 3.08.

The parameter λ for p_T > 100 MeV as a function of k_T in selected low m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 100 MeV as a function of k_T in selected low m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 100 MeV as a function of k_T in selected high m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 100 MeV as a function of k_T in selected high m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 100 MeV as a function of m_ch in k_T intervals between 0.1 and 0.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 100 MeV as a function of m_ch in k_T intervals between 0.1 and 0.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 100 MeV as a function of m_ch in k_T intervals between 0.5 and 1.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 100 MeV as a function of m_ch in k_T intervals between 0.5 and 1.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 100 MeV as a function of k_T in selected low m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 100 MeV as a function of k_T in selected low m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 100 MeV as a function of k_T in selected high m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 100 MeV as a function of k_T in selected high m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 100 MeV as a function of m_ch in k_T intervals between 0.1 and 0.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 100 MeV as a function of m_ch in k_T intervals between 0.1 and 0.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 100 MeV as a function of m_ch in k_T intervals between 0.5 and 1.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 100 MeV as a function of m_ch in k_T intervals between 0.5 and 1.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The fit parameter μ describing the dependence of the correlation strength, λ, on charged-particle scaled multiplicity, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid (blue dashed) curve represents the exponential fit of the dependence of parameter μ on m_ch for tracks with p_T >100 MeV (p_T >500 MeV).

The fit parameter μ describing the dependence of the correlation strength, λ, on charged-particle scaled multiplicity, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid (blue dashed) curve represents the exponential fit of the dependence of parameter μ on m_ch for tracks with p_T >100 MeV (p_T >500 MeV).

The fit parameter μ describing the dependence of the correlation strength, λ, on charged-particle scaled multiplicity, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid (blue dashed) curve represents the exponential fit of the dependence of parameter μ on m_ch for tracks with p_T >100 MeV (p_T >500 MeV).

The fit parameter μ describing the dependence of the correlation strength, λ, on charged-particle scaled multiplicity, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid (blue dashed) curve represents the exponential fit of the dependence of parameter μ on m_ch for tracks with p_T >100 MeV (p_T >500 MeV).

The fit parameter ν describing the dependence of the correlation strength, λ, on charged-particle scaled multiplicity, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid (blue dashed) curve represents the exponential fit of the dependence of parameter ν on m_ch for tracks with p_T >100 MeV (p_T >500 MeV).

The fit parameter ν describing the dependence of the correlation strength, λ, on charged-particle scaled multiplicity, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid (blue dashed) curve represents the exponential fit of the dependence of parameter ν on m_ch for tracks with p_T >100 MeV (p_T >500 MeV).

The fit parameter ν describing the dependence of the correlation strength, λ, on charged-particle scaled multiplicity, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid (blue dashed) curve represents the exponential fit of the dependence of parameter ν on m_ch for tracks with p_T >100 MeV (p_T >500 MeV).

The fit parameter ν describing the dependence of the correlation strength, λ, on charged-particle scaled multiplicity, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid (blue dashed) curve represents the exponential fit of the dependence of parameter ν on m_ch for tracks with p_T >100 MeV (p_T >500 MeV).

The parameter ξ describing the dependence of the source radius, R, on charged-particle scaled multiplicity, m_ch, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid and blue dashed curves represent the saturated value of the parameter ξ for m_ch > 3.0 for tracks with p_T >100 MeV and for m_ch > 2.8 for tracks with p_T >500 MeV, respectively.

The parameter ξ describing the dependence of the source radius, R, on charged-particle scaled multiplicity, m_ch, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid and blue dashed curves represent the saturated value of the parameter ξ for m_ch > 3.0 for tracks with p_T >100 MeV and for m_ch > 2.8 for tracks with p_T >500 MeV, respectively.

The parameter ξ describing the dependence of the source radius, R, on charged-particle scaled multiplicity, m_ch, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid and blue dashed curves represent the saturated value of the parameter ξ for m_ch > 3.0 for tracks with p_T >100 MeV and for m_ch > 2.8 for tracks with p_T >500 MeV, respectively.

The parameter ξ describing the dependence of the source radius, R, on charged-particle scaled multiplicity, m_ch, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid and blue dashed curves represent the saturated value of the parameter ξ for m_ch > 3.0 for tracks with p_T >100 MeV and for m_ch > 2.8 for tracks with p_T >500 MeV, respectively.

The parameter κ describing the dependence of the source radius, R, on charged-particle scaled multiplicity, m_ch, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid and blue dashed curves represent the exponential fit to the parameter κ for tracks with p_T >100 MeV and for tracks with p_T >500 MeV, respectively.

The parameter κ describing the dependence of the source radius, R, on charged-particle scaled multiplicity, m_ch, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid and blue dashed curves represent the exponential fit to the parameter κ for tracks with p_T >100 MeV and for tracks with p_T >500 MeV, respectively.

The parameter κ describing the dependence of the source radius, R, on charged-particle scaled multiplicity, m_ch, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid and blue dashed curves represent the exponential fit to the parameter κ for tracks with p_T >100 MeV and for tracks with p_T >500 MeV, respectively.

The parameter κ describing the dependence of the source radius, R, on charged-particle scaled multiplicity, m_ch, for track p_T>100 MeV and track p_T>500 MeV in the minimum-bias (MB) and high-multiplicity track (HMT) samples at √s = 13 TeV. The error bars and boxes represent the statistical and systematic contributions, respectively. The black solid and blue dashed curves represent the exponential fit to the parameter κ for tracks with p_T >100 MeV and for tracks with p_T >500 MeV, respectively.

The two-dimensional dependence on m_ch and k_T for p_T > 500 MeV for the correlation strength, λ, obtained from the exponential fit to the R₂(Q) correlation functions using the MB sample for m_ch ≤ 3.08 and the HMT sample for m_ch > 3.08.

The two-dimensional dependence on m_ch and k_T for p_T > 500 MeV for the source radius, R, obtained from the exponential fit to the R₂(Q) correlation functions using the MB sample for m_ch ≤ 3.08 and the HMT sample for m_ch > 3.08.

The parameter λ for p_T > 500 MeV as a function of k_T in selected low m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 500 MeV as a function of k_T in selected low m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 500 MeV as a function of k_T in selected high m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 500 MeV as a function of k_T in selected high m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 500 MeV as a function of m_ch in k_T intervals between 0.5 and 1.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter λ for p_T > 500 MeV as a function of m_ch in k_T intervals between 0.5 and 1.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 500 MeV as a function of k_T in selected low m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 500 MeV as a function of k_T in selected low m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 500 MeV as a function of k_T in selected high m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 500 MeV as a function of k_T in selected high m_ch intervals. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 500 MeV as a function of m_ch in k_T intervals between 0.5 and 1.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

The parameter R for p_T > 500 MeV as a function of m_ch in k_T intervals between 0.5 and 1.5 GeV. The error bars and boxes represent the statistical and systematic contributions, respectively.

ATLAS and CMS results for the source radius R as a function of n_ch in pp interactions at 13 TeV. The CMS results (open circles) have been adjusted (by the CMS collaboration) to the ATLAS kinematic region∶ p_T > 100 MeV and |η|<2.5. The ATLAS uncertainties are the sum in quadrature of the statistical and asymmetric systematic uncertainties. For CMS, only the systematic uncertainties are shown since the statistical uncertainties are smaller than the marker size. The dashed blue (ATLAS) and black (CMS) lines represent the fit to ∛n_ch at low multiplicity, continued as dotted lines beyond the fit range. The solid green (ATLAS) and broken black (CMS) lines indicate the plateau level at high multiplicity.

ATLAS and CMS results for the source radius R as a function of n_ch in pp interactions at 13 TeV. The CMS results (open circles) have been adjusted (by the CMS collaboration) to the ATLAS kinematic region∶ p_T > 100 MeV and |η|<2.5. The ATLAS uncertainties are the sum in quadrature of the statistical and asymmetric systematic uncertainties. For CMS, only the systematic uncertainties are shown since the statistical uncertainties are smaller than the marker size. The dashed blue (ATLAS) and black (CMS) lines represent the fit to ∛n_ch at low multiplicity, continued as dotted lines beyond the fit range. The solid green (ATLAS) and broken black (CMS) lines indicate the plateau level at high multiplicity.

ATLAS and CMS results for the source radius R as a function of n_ch in pp interactions at 13 TeV. The CMS results (open circles) have been adjusted (by the CMS collaboration) to the ATLAS kinematic region∶ p_T > 100 MeV and |η|<2.5. The ATLAS uncertainties are the sum in quadrature of the statistical and asymmetric systematic uncertainties. For CMS, only the systematic uncertainties are shown since the statistical uncertainties are smaller than the marker size. The dashed blue (ATLAS) and black (CMS) lines represent the fit to ∛n_ch at low multiplicity, continued as dotted lines beyond the fit range. The solid green (ATLAS) and broken black (CMS) lines indicate the plateau level at high multiplicity.

ATLAS and CMS results for the source radius R as a function of ∛n_ch in pp interactions at 13 TeV. The CMS results (open circles) have been adjusted (by the CMS collaboration) to the ATLAS kinematic region∶ p_T > 100 MeV and |η|<2.5. The ATLAS uncertainties are the sum in quadrature of the statistical and asymmetric systematic uncertainties. For CMS, only the systematic uncertainties are shown since the statistical uncertainties are smaller than the marker size. The dashed blue (ATLAS) and black (CMS) lines represent the fit to ∛n_ch at low multiplicity, continued as dotted lines beyond the fit range. The solid green (ATLAS) and broken black (CMS) lines indicate the plateau level at high multiplicity.

ATLAS and CMS results for the source radius R as a function of ∛n_ch in pp interactions at 13 TeV. The CMS results (open circles) have been adjusted (by the CMS collaboration) to the ATLAS kinematic region∶ p_T > 100 MeV and |η|<2.5. The ATLAS uncertainties are the sum in quadrature of the statistical and asymmetric systematic uncertainties. For CMS, only the systematic uncertainties are shown since the statistical uncertainties are smaller than the marker size. The dashed blue (ATLAS) and black (CMS) lines represent the fit to ∛n_ch at low multiplicity, continued as dotted lines beyond the fit range. The solid green (ATLAS) and broken black (CMS) lines indicate the plateau level at high multiplicity.

ATLAS and CMS results for the source radius R as a function of ∛n_ch in pp interactions at 13 TeV. The CMS results (open circles) have been adjusted (by the CMS collaboration) to the ATLAS kinematic region∶ p_T > 100 MeV and |η|<2.5. The ATLAS uncertainties are the sum in quadrature of the statistical and asymmetric systematic uncertainties. For CMS, only the systematic uncertainties are shown since the statistical uncertainties are smaller than the marker size. The dashed blue (ATLAS) and black (CMS) lines represent the fit to ∛n_ch at low multiplicity, continued as dotted lines beyond the fit range. The solid green (ATLAS) and broken black (CMS) lines indicate the plateau level at high multiplicity.

Systematic uncertainties (in percent) in the correlation strength, λ, and source radius, R, for the exponential fit of the two-particle double-ratio correlation functions, R₂(Q), for p_T > 100 MeV at √s= 13 TeV for the MB and HMT events. The choice of MC generator gives rise to asymmetric uncertainties, denoted by uparrow and downarrow. This asymmetry propagates through to the cumulative uncertainty. The columns under ‘Uncertainty range’ show the range of systematic uncertainty from the fits in the various n_ch intervals.

The results of the fits to the dependencies of the correlation strength, λ, and source radius, R, on the average rescaled charged-particle multiplicity, m_ch, for |η| < 2.5 and both p_T > 100 MeV and p_T > 500 MeV at √s = 13 TeV for the minimum-bias (MB) and the high-multiplicity track (HMT) events. The parameters γ and δ resulting from a joint fit to the MB and HMT data are presented. The total uncertainties are shown.

The results of the fits to the dependencies of the correlation strength, λ, and source radius, R, on the pair average transverse momentum, k_T, for various functional forms and for minimum-bias (MB) and high-multiplicity track (HMT) events for p_T > 100 MeV and p_T > 500 MeV at √s = 13 TeV. The total uncertainties are shown.

The Bose-Einstein correlation (BEC) parameters λ and R as a function of n_ch and k_T using different MC generators in the calculation of R₂(Q). (a) λ versus n_ch for MB events, (b) λ versus n_ch for HMT events, (c) λ versus k_T and (d) R versus k_T for MB events. The uncertainties shown are statistical. The lower panel of each plot shows the ratio of the BEC parameters obtained using EPOS LHC (red circles), Pythia 8 Monash (blue squares) and Herwig++ UE-EE-5 (green triangles) compared with the parameters obtained using Pythia 8 A2. The gray band in the lower panels is the MC systematic uncertainty, obtained as explained in the text.

The Bose-Einstein correlation (BEC) parameters λ and R as a function of n_ch and k_T using different MC generators in the calculation of R₂(Q). (a) λ versus n_ch for MB events, (b) λ versus n_ch for HMT events, (c) λ versus k_T and (d) R versus k_T for MB events. The uncertainties shown are statistical. The lower panel of each plot shows the ratio of the BEC parameters obtained using EPOS LHC (red circles), Pythia 8 Monash (blue squares) and Herwig++ UE-EE-5 (green triangles) compared with the parameters obtained using Pythia 8 A2. The gray band in the lower panels is the MC systematic uncertainty, obtained as explained in the text.

The Bose-Einstein correlation (BEC) parameters λ and R as a function of n_ch and k_T using different MC generators in the calculation of R₂(Q). (a) λ versus n_ch for MB events, (b) λ versus n_ch for HMT events, (c) λ versus k_T and (d) R versus k_T for MB events. The uncertainties shown are statistical. The lower panel of each plot shows the ratio of the BEC parameters obtained using EPOS LHC (red circles), Pythia 8 Monash (blue squares) and Herwig++ UE-EE-5 (green triangles) compared with the parameters obtained using Pythia 8 A2. The gray band in the lower panels is the MC systematic uncertainty, obtained as explained in the text.

The Bose-Einstein correlation (BEC) parameters λ and R as a function of n_ch and k_T using different MC generators in the calculation of R₂(Q). (a) λ versus n_ch for MB events, (b) λ versus n_ch for HMT events, (c) λ versus k_T and (d) R versus k_T for MB events. The uncertainties shown are statistical. The lower panel of each plot shows the ratio of the BEC parameters obtained using EPOS LHC (red circles), Pythia 8 Monash (blue squares) and Herwig++ UE-EE-5 (green triangles) compared with the parameters obtained using Pythia 8 A2. The gray band in the lower panels is the MC systematic uncertainty, obtained as explained in the text.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 10, (b) 11 < n_ch ≤ 20, (c) 21 < n_ch ≤ 30, (d) 31 < n_ch ≤ 40, (e) 41 < n_ch ≤ 50, (f) 51 < n_ch ≤ 60, (g) 61 < n_ch ≤ 70, (h) 71 < n_ch ≤ 80 and (i) 81 < n_ch ≤ 90. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 10, (b) 11 < n_ch ≤ 20, (c) 21 < n_ch ≤ 30, (d) 31 < n_ch ≤ 40, (e) 41 < n_ch ≤ 50, (f) 51 < n_ch ≤ 60, (g) 61 < n_ch ≤ 70, (h) 71 < n_ch ≤ 80 and (i) 81 < n_ch ≤ 90. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 10, (b) 11 < n_ch ≤ 20, (c) 21 < n_ch ≤ 30, (d) 31 < n_ch ≤ 40, (e) 41 < n_ch ≤ 50, (f) 51 < n_ch ≤ 60, (g) 61 < n_ch ≤ 70, (h) 71 < n_ch ≤ 80 and (i) 81 < n_ch ≤ 90. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 10, (b) 11 < n_ch ≤ 20, (c) 21 < n_ch ≤ 30, (d) 31 < n_ch ≤ 40, (e) 41 < n_ch ≤ 50, (f) 51 < n_ch ≤ 60, (g) 61 < n_ch ≤ 70, (h) 71 < n_ch ≤ 80 and (i) 81 < n_ch ≤ 90. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 10, (b) 11 < n_ch ≤ 20, (c) 21 < n_ch ≤ 30, (d) 31 < n_ch ≤ 40, (e) 41 < n_ch ≤ 50, (f) 51 < n_ch ≤ 60, (g) 61 < n_ch ≤ 70, (h) 71 < n_ch ≤ 80 and (i) 81 < n_ch ≤ 90. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 10, (b) 11 < n_ch ≤ 20, (c) 21 < n_ch ≤ 30, (d) 31 < n_ch ≤ 40, (e) 41 < n_ch ≤ 50, (f) 51 < n_ch ≤ 60, (g) 61 < n_ch ≤ 70, (h) 71 < n_ch ≤ 80 and (i) 81 < n_ch ≤ 90. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 10, (b) 11 < n_ch ≤ 20, (c) 21 < n_ch ≤ 30, (d) 31 < n_ch ≤ 40, (e) 41 < n_ch ≤ 50, (f) 51 < n_ch ≤ 60, (g) 61 < n_ch ≤ 70, (h) 71 < n_ch ≤ 80 and (i) 81 < n_ch ≤ 90. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 10, (b) 11 < n_ch ≤ 20, (c) 21 < n_ch ≤ 30, (d) 31 < n_ch ≤ 40, (e) 41 < n_ch ≤ 50, (f) 51 < n_ch ≤ 60, (g) 61 < n_ch ≤ 70, (h) 71 < n_ch ≤ 80 and (i) 81 < n_ch ≤ 90. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 10, (b) 11 < n_ch ≤ 20, (c) 21 < n_ch ≤ 30, (d) 31 < n_ch ≤ 40, (e) 41 < n_ch ≤ 50, (f) 51 < n_ch ≤ 60, (g) 61 < n_ch ≤ 70, (h) 71 < n_ch ≤ 80 and (i) 81 < n_ch ≤ 90. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 91 < n_ch ≤ 100, (b) 101 < n_ch ≤ 125, (c) 126 < n_ch ≤ 150, (d) 151 < n_ch ≤ 200, (e) 201 < n_ch ≤ 250. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 91 < n_ch ≤ 100, (b) 101 < n_ch ≤ 125, (c) 126 < n_ch ≤ 150, (d) 151 < n_ch ≤ 200, (e) 201 < n_ch ≤ 250. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 91 < n_ch ≤ 100, (b) 101 < n_ch ≤ 125, (c) 126 < n_ch ≤ 150, (d) 151 < n_ch ≤ 200, (e) 201 < n_ch ≤ 250. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 91 < n_ch ≤ 100, (b) 101 < n_ch ≤ 125, (c) 126 < n_ch ≤ 150, (d) 151 < n_ch ≤ 200, (e) 201 < n_ch ≤ 250. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 91 < n_ch ≤ 100, (b) 101 < n_ch ≤ 125, (c) 126 < n_ch ≤ 150, (d) 151 < n_ch ≤ 200, (e) 201 < n_ch ≤ 250. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 101 < n_ch ≤ 110, (b) 111 < n_ch ≤ 120, (c) 121 < n_ch ≤ 130, (d) 131 < n_ch ≤ 140, (e) 141 < n_ch ≤ 155, (f) 156 < n_ch ≤ 175, (g) 176 < n_ch ≤ 200, (h) 201 < n_ch ≤ 230 and (i) 231 < n_ch ≤ 300. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 101 < n_ch ≤ 110, (b) 111 < n_ch ≤ 120, (c) 121 < n_ch ≤ 130, (d) 131 < n_ch ≤ 140, (e) 141 < n_ch ≤ 155, (f) 156 < n_ch ≤ 175, (g) 176 < n_ch ≤ 200, (h) 201 < n_ch ≤ 230 and (i) 231 < n_ch ≤ 300. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 101 < n_ch ≤ 110, (b) 111 < n_ch ≤ 120, (c) 121 < n_ch ≤ 130, (d) 131 < n_ch ≤ 140, (e) 141 < n_ch ≤ 155, (f) 156 < n_ch ≤ 175, (g) 176 < n_ch ≤ 200, (h) 201 < n_ch ≤ 230 and (i) 231 < n_ch ≤ 300. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 101 < n_ch ≤ 110, (b) 111 < n_ch ≤ 120, (c) 121 < n_ch ≤ 130, (d) 131 < n_ch ≤ 140, (e) 141 < n_ch ≤ 155, (f) 156 < n_ch ≤ 175, (g) 176 < n_ch ≤ 200, (h) 201 < n_ch ≤ 230 and (i) 231 < n_ch ≤ 300. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 101 < n_ch ≤ 110, (b) 111 < n_ch ≤ 120, (c) 121 < n_ch ≤ 130, (d) 131 < n_ch ≤ 140, (e) 141 < n_ch ≤ 155, (f) 156 < n_ch ≤ 175, (g) 176 < n_ch ≤ 200, (h) 201 < n_ch ≤ 230 and (i) 231 < n_ch ≤ 300. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 101 < n_ch ≤ 110, (b) 111 < n_ch ≤ 120, (c) 121 < n_ch ≤ 130, (d) 131 < n_ch ≤ 140, (e) 141 < n_ch ≤ 155, (f) 156 < n_ch ≤ 175, (g) 176 < n_ch ≤ 200, (h) 201 < n_ch ≤ 230 and (i) 231 < n_ch ≤ 300. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 101 < n_ch ≤ 110, (b) 111 < n_ch ≤ 120, (c) 121 < n_ch ≤ 130, (d) 131 < n_ch ≤ 140, (e) 141 < n_ch ≤ 155, (f) 156 < n_ch ≤ 175, (g) 176 < n_ch ≤ 200, (h) 201 < n_ch ≤ 230 and (i) 231 < n_ch ≤ 300. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 101 < n_ch ≤ 110, (b) 111 < n_ch ≤ 120, (c) 121 < n_ch ≤ 130, (d) 131 < n_ch ≤ 140, (e) 141 < n_ch ≤ 155, (f) 156 < n_ch ≤ 175, (g) 176 < n_ch ≤ 200, (h) 201 < n_ch ≤ 230 and (i) 231 < n_ch ≤ 300. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 101 < n_ch ≤ 110, (b) 111 < n_ch ≤ 120, (c) 121 < n_ch ≤ 130, (d) 131 < n_ch ≤ 140, (e) 141 < n_ch ≤ 155, (f) 156 < n_ch ≤ 175, (g) 176 < n_ch ≤ 200, (h) 201 < n_ch ≤ 230 and (i) 231 < n_ch ≤ 300. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), for the high-multiplicity track (HMT) events using the unlike-charge particle (UCP) pairs reference sample for k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample for n_ch - intervals∶ (a) 2 < n_ch ≤ 9, (b) 10 < n_ch ≤ 18, (c) 19 < n_ch ≤ 27, (d) 28 < n_ch ≤ 36, (e) 37 < n_ch ≤ 45, (f) 46 < n_ch ≤ 54, (g) 55 < n_ch ≤ 63, (h) 64 < n_ch ≤ 72, (i) 73 < n_ch ≤ 81, (j) 82 < n_ch ≤ 90, (k) 91 < n_ch ≤ 113, and (l) 114 < n_ch ≤ 136. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The single-ratio two-particle correlation functions, C₂^data(Q), at 7 TeV for the minimum-bias (MB) events using the unlike-charge particle (UCP) pairs reference sample k_T - intervals∶ (a) 100 < k_T ≤ 200 MeV, (b) 200 < k_T ≤ 300 MeV, (c) 300 < k_T ≤ 400 MeV, (d) 400 < k_T ≤ 500 MeV, (e) 500 < k_T ≤ 600 MeV, (f) 600 < k_T ≤ 700 MeV, (g) 700 < k_T ≤ 1000 MeV, and (h) 1000 < k_T ≤ 1500 MeV. The error bars represent the statistical uncertainties. The boxes represent the systematic uncertainties, which are the sum in quadrature of a variation of the Coulomb correction, the track reconstruction efficiency and the unfolding matrix.

The correlation strength, λ, and source radius, R, of the exponential fits to the two-particle double-ratio correlation functions, R₂(Q), in dependence on the multiplicity, m_ch, intervals for the minimum-bias (MB) and the high-multiplicity track (HMT) events for p_T > 100 MeV at √s = 13 TeV. Statistical uncertainties for √χ²/ndf>1 are corrected by the √χ²/ndf. The total uncertainties are shown.

The correlation strength, λ, and source radius, R, of the exponential fits to the two-particle double-ratio correlation functions, R₂(Q), in dependence on the multiplicity, m_ch, intervals for the minimum-bias (MB) and the high-multiplicity track (HMT) events for p_T > 500 MeV at √s = 13 TeV. Statistical uncertainties for √χ²/ndf>1 are corrected by the √χ²/ndf. The total uncertainties are shown.

The correlation strength, λ, and source radius, R, of the exponential fits to the two-particle double-ratio correlation functions, R₂(Q), in dependence on the pair transverse momentum, k_T, intervals for the minimum-bias (MB) and the high-multiplicity track (HMT) events for p_T > 100 MeV at √s = 13 TeV. Statistical uncertainties for √χ²/ndf>1 are corrected by the √χ²/ndf. The total uncertainties are shown.

The correlation strength, λ, and source radius, R, of the exponential fits to the two-particle double-ratio correlation functions, R₂(Q), in dependence on the pair transverse momentum, k_T, intervals for the minimum-bias (MB) and the high-multiplicity track (HMT) events for p_T > 500 MeV at √s = 13 TeV. Statistical uncertainties for √χ²/ndf>1 are corrected by the √χ²/ndf. The total uncertainties are shown.

Final state radiation correction used in the $\phi_{\eta}^{*}$ cross-section measurement. The first uncertainty is statistical and the second is systematic.

Final state radiation correction used in the $y^{Z}-p_{T}^{Z}$ cross-section measurement. The first uncertainty is statistical and the second is systematic.

Final state radiation correction used in the $y^{Z}-\phi_{\eta}^{*}$ cross-section measurement. The first uncertainty is statistical and the second is systematic.

Correlation matrix of statistical uncertainty for one-dimensional $y^Z$ measurement.

Correlation matrix of statistical uncertainty for one-dimensional $p_{T}^{Z}$ measurement.

Correlation matrix of statistical uncertainty for one-dimensional $\phi_{\eta}^{*}$ measurement.

Correlation matrix of statistical uncertainty for two-dimensional $y^Z-p_{T}^{Z}$ measurement.

Correlation matrix of statistical uncertainty for two-dimensional $y^Z-\phi_{\eta}^{*}$ measurement.

Correlation matrix of efficiency uncertainty for one-dimensional $y^Z$ measurement.

Correlation matrix of efficiency uncertainty for one-dimensional $p_{T}^{Z}$ measurement.

Correlation matrix of efficiency uncertainty for one-dimensional $\phi_{\eta}^{*}$ measurement.

Correlation matrix of efficiency uncertainty for two-dimensional $y^Z-p_{T}^{Z}$ measurement.

Correlation matrix of efficiency uncertainty for two-dimensional $y^Z-\phi_{\eta}^{*}$ measurement.

Measured total $Z$-boson cross-section for different datasets. The first uncertainty is statistical, the second systematic, and the third is due to the luminosity.

Measured single differential cross-sections in interval regions of $y^{Z}$. The first uncertainty is statistical, the second systematic, and the third is due to the luminosity.

Measured single differential cross-sections in interval regions of $p_{T}^{Z}$. The first uncertainty is statistical, the second systematic, and the third is due to the luminosity.

Measured single differential cross-sections in interval regions of $\phi_{\eta}^{*}$. The first uncertainty is statistical, the second systematic, and the third is due to the luminosity.

Measured double differential cross-sections in interval regions of $y^{Z}$ and $p_{T}^{Z}$. The first uncertainty is statistical, the second systematic, and the third is due to the luminosity.

Measured double differential cross-sections in interval regions of $y^{Z}$ and $\phi_{\eta}^{*}$. The first uncertainty is statistical, the second systematic, and the third is due to the luminosity.

Systematic uncertainties in the single differential cross-sections in interval regions of $y^{Z}$, presented in percentage. The contributions from efficiency (Eff), background (BKG), final state radiation (FSR), closure test (Closure), and alignment and calibration (Alignment) are shown.

Systematic uncertainties in the single differential cross-sections in interval regions of $p_{T}^{Z}$, presented in percentage. The contributions from efficiency (Eff), background (BKG), final state radiation (FSR), closure test (Closure), and alignment and calibration (Alignment) are shown.

Systematic uncertainties in the single differential cross-sections in interval regions of $\phi_{\eta}^{*}$, presented in percentage. The contributions from efficiency (Eff), background (BKG), final state radiation (FSR), closure test (Closure), and alignment and calibration (Alignment) are shown.

Systematic uncertainties in the double differential cross-sections in interval regions of $y^{Z}$ and $p_{T}^{Z}$, presented in percentage. The contributions from efficiency (Eff), background (BKG), final state radiation (FSR), closure test (Closure), and alignment and calibration (Alignment) are shown.

Systematic uncertainties in the double differential cross-sections in interval regions of $y^{Z}$ and $\phi_{\eta}^{*}$, presented in percentage. The contributions from efficiency (Eff), background (BKG), final state radiation (FSR), closure test (Closure), and alignment and calibration (Alignment) are shown.

The contribution from different systematic uncertainties to the measured $t\bar{t}t\bar{t}$ production cross section, grouped in categories.

The results of the fitted signal strength $\mu$ in the 1L/2LOS and 2LSS/3L combined channel.

The results of fitted inclusive ${t\bar{t}t\bar{t}}$ cross-section in the 1L/2LOS and 2LSS/3L combined channel.

Comparison between data and prediction for the distribution of the sum of the pseudo-continuous b-tagging score over the six jets with the highest score in the 1L,$\geq$9j,$\geq$3b region before the fit.

Comparison between data and prediction for the distribution of the sum of the pseudo-continuous b-tagging score over the six jets with the highest score in the 1L,$\geq$9j,$\geq$3b region after the fit.

Comparison between data and prediction for the distribution of the sum of the pseudo-continuous b-tagging score over the six jets with the highest score in the 2LOS,$\geq$7j,$\geq$3b region before the fit.

Comparison between data and prediction for the distribution of the sum of the pseudo-continuous b-tagging score over the six jets with the highest score in the 2LOS,$\geq$7j,$\geq$3b region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,$\geq$8j,$\geq$3b region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,$\geq$8j,$\geq$3b region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,$\geq$6j,$\geq$3b region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,$\geq$6j,$\geq$3b region after the fit.

Comparison between data and prediction for the distribution of number of jets in the 1L,$\geq$8j,$\geq$3b region before the fit.

Comparison between data and prediction for the distribution of number of jets in the 1L,$\geq$8j,$\geq$3b region after the fit.

Comparison between data and prediction for the distribution of number of jets in the 2LOS,$\geq$6j,$\geq$3b region before the fit.

Comparison between data and prediction for the distribution of number of jets in the 2LOS,$\geq$6j,$\geq$3b region after the fit.

Comparison between data and prediction for the distribution of b-jets multiplicity in the 1L,$\geq$8j,$\geq$3b region before the fit.

Comparison between data and prediction for the distribution of b-jets multiplicity in the 1L,$\geq$8j,$\geq$3b region after the fit.

Comparison between data and prediction for the distribution of b-jets multiplicity in the 2LOS,$\geq$6j,$\geq$3b region before the fit.

Comparison between data and prediction for the distribution of b-jets multiplicity in the 2LOS,$\geq$6j,$\geq$3b region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,9j,4b signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,9j,4b signal region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,9j,$\geq$5b signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,9j,$\geq$5b signal region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,3bL signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,3bL signal region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,3bH signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,3bH signal region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,4b signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,4b signal region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,$\geq$5b signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,$\geq$5b signal region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,7j,$\geq$4b signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,7j,$\geq$4b signal region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,$\geq$8j,3bL signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,$\geq$8j,3bL signal region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,$\geq$8j,3bH signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,$\geq$8j,3bH signal region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,$\geq$8j,$\geq$4b signal region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,$\geq$8j,$\geq$4b signal region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,3bV validation region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,3bV validation region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,9j,3bV validation region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,9j,3bV validation region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,3bV validation region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 1L,$\geq$10j,3bV validation region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,6j,3bV validation region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,6j,3bV validation region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,7j,3bV validation region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,7j,3bV validation region after the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,$\geq$8j,3bV validation region before the fit.

Comparison between data and prediction for the distribution of the BDT score in the 2LOS,$\geq$8j,3bV validation region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,3bL control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,3bL control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,3bH control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,3bH control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,9j,3bL control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,9j,3bL control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,9j,3bH control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,9j,3bH control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,4b control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,4b control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,$\geq$5b control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 1L,8j,$\geq$5b control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,6j,3bL control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,6j,3bL control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,6j,3bH control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,6j,3bH control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,7j,3bL control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,7j,3bL control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,7j,3bH control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,7j,3bH control region after the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,6j,$\geq$4b control region before the fit.

Comparison between data and prediction for the distribution of the scalar sum of all jet and lepton pT in the event in the 2LOS,6j,$\geq$4b control region after the fit.

Measured fiducial cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> e+e- final state.

Measured fiducial cross section times leptonic branching ratio for W+ production in the W+ -> mu+ nu final state.

Measured fiducial cross section times leptonic branching ratio for W- production in the W- -> mu- nubar final state.

Measured fiducial cross section times leptonic branching ratio for W+/- production in the combined W+ -> mu+ nu and W- -> mu- nubar final state.

Measured fiducial cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> mu+ mu- final state.

Measured total cross section times leptonic branching ratio for W+ production in the W+ -> e+ nu final state.

Measured total cross section times leptonic branching ratio for W- production in the W- -> e- nubar final state.

Measured total cross section times leptonic branching ratio for W+/- production in the combined W+ -> e+ nu and W- -> e- nubar final state.

Measured total cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> e+ e- final state.

Measured total cross section times leptonic branching ratio for W+ production in the W+ -> mu+ nu final state.

Measured total cross section times leptonic branching ratio for W- production in the W- -> mu- nubar final state.

Measured total cross section times leptonic branching ratio for W+/- production in the combined W+ -> mu+ nu and W- -> mu- nubar final state.

Measured total cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> mu+ mu- final state.

Measured total cross section times leptonic branching ratio for W+ production in the W+ -> l+ nu (l = e, mu) final states.

Measured total cross section times leptonic branching ratio for W- production in the W- -> l- nubar (l = e, mu) final states.

Measured total cross section times leptonic branching ratio for W+/- production in the combined W+ -> l+ nu and W- -> l- nubar (l = e, mu) final states.

Measured total cross section times leptonic branching ratio for Z/gamma* production in the combined Z/gamma* -> l+ l- (l = e, mu) final states.

Measured total cross-section ratio R_{W+/Z} = sigma (W+ -> e+ nu) / sigma (Z/gamma^* -> e+ e-).

Measured total cross-section ratio R_{W-/Z} = sigma (W- -> e- nubar) / sigma (Z/gamma^* -> e+ e-).

Measured total cross-section ratio R_{W+-/Z} = sigma (W+/- -> e+/- nu/nubar) / sigma (Z/gamma^* -> e+ e-).

Measured total cross-section ratio R_{W+/Z} = sigma (W+ -> mu+ nu) / sigma (Z/gamma^* -> mu+ mu-).

Measured total cross-section ratio R_{W-/Z} = sigma (W- -> mu- nubar) / sigma (Z/gamma^* -> mu+ mu-).

Measured total cross-section ratio R_{W+-/Z} = sigma (W+/- -> mu+/- nu/nubar) / sigma (Z/gamma^* -> mu+ mu-).

Measured total cross-section ratio R_{W+/Z} = sigma (W+ -> l+ nu) / sigma (Z/gamma^* -> l+ l-) where (l = e, mu).

Measured total cross-section ratio R_{W-/Z} = sigma (W- -> l- nubar) / sigma (Z/gamma^* -> l+ l-) where (l = e, mu).

Measured total cross-section ratio R_{W+-/Z} = sigma (W+/- -> l+/- nu/nubar) / sigma (Z/gamma^* -> l+ l-) where (l = e, mu).

Measured lepton asymmetry from W+ -> e+ nu and W- -> e- nubar, binned as a function pseudorapidity.

Measured lepton asymmetry from W+ -> e+ nu and W- -> e- nubar.

Measured lepton asymmetry from W+ -> mu+ nu and W- -> mu- nubar, binned as a function pseudorapidity.

Measured lepton asymmetry from W+ -> mu+ nu and W- -> mu- nubar.

Measured lepton asymmetry from W+ -> l+ nu and W- -> l- nubar (l = e, mu), binned as a function pseudorapidity.

Measured lepton asymmetry from W+ -> l+ nu and W- -> l- nubar (l = e, mu).

Measured value of TT and LT polarized cross sections extracted from the data.

Values of r_04_00 and r_1_1-1 extracted from the angular distributions.

Differential cross section for XI- production as a function of the invariant mass of the XI- with either of the K+ mesons for incident photon energy 3.09 Gev.

Differential cross section for XI- production as a function of the invariant mass of the XI- with either of the K+ mesons for incident photon energy 3.19 Gev.

Differential cross section for XI- production as a function of the invariant mass of the XI- with either of the K+ mesons for incident photon energy 3.29 Gev.

Differential cross section for XI- production as a function of the invariant mass of the XI- with either of the K+ mesons for incident photon energy 3.39 Gev.

Differential cross section for XI- production as a function of the invariant mass of the XI- with either of the K+ mesons for incident photon energy 3.49 Gev.

Differential cross section for XI- production as a function of the invariant mass of the XI- with either of the K+ mesons for incident photon energy 3.59 Gev.

Differential cross section for XI- production as a function of the invariant mass of the XI- with either of the K+ mesons for incident photon energy 3.69 Gev.

Differential cross section for XI- production as a function of the invariant mass of the XI- with either of the K+ mesons for incident photon energy 3.79 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 2.79 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 2.89 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 2.99 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 3.09 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 3.19 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 3.29 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 3.39 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 3.49 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 3.59 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 3.69 Gev.

Differential cross section for XI- production as a function of the invariant mass of the K+ meson pair for incident photon energy 3.79 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 2.79 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 2.89 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 2.99 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 3.09 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 3.19 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 3.29 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 3.39 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 3.49 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 3.59 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 3.69 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of the XI- in the photon-proton cm frame for incident photon energy 3.79 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 2.79 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 2.89 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 2.99 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 3.09 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 3.19 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 3.29 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 3.39 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 3.49 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 3.59 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 3.69 Gev.

Differential cross section for XI- production as a function of the cosine of the polar angle of each K+ in the photon-proton cm frame for incident photon energy 3.79 Gev.

Total cross section fo XI- production.

Differential cross section for XI(1530)- production as a function of the cosine of the polar angle of the XI(1530)- in the photon-proton cm frame for incident photon energy 3.35 to 4.75 GeV.

Total cross section for XI(1530)- production.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

The inclusive charged particle differential cross section.

The K0 + K0BAR inclusive differential cross section. The last line in the table is the integral over the full X range of the measurement.. There is an additional 3.4 PCT normalization error (included in the integral).

The LAMBDA + LAMBDABAR inclusive differential cross section. The last line in the table is the integral over the full X range of the measurement.. There is an additional 3.4 PCT normalization error (included in the integral).

No description provided.

The K*0 + K*BAR0 inclusive differential cross section. The last line in the table is the integral over the full X range of the measurement.. There is an additional 3.4 PCT normalization error (included in the integral).

The PHI meson inclusive differential cross section. The last line in the table is the integral over the full X range of the measurement.. There is an additional 3.4 PCT normalization error (included in the integral).

Measured differential cross section for the production of charged pions perZ0 decay into light, charm and bottom quarks separately. The errors given are t he sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

The ratios of light to heavy quark production of charged pions. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

Measured differential cross section for the production of charged kaons perZ0 decay into light, charm and bottom quarks separately. The errors given are t he sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

The ratios of light to heavy quark production of charged kaons. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

Measured differential cross section for the production of neutral K* mesonsper Z0 decay into light, charm and bottom quarks separately. The errors given a re the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

The ratios of light to heavy quark production of neutral K* mesons. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

Measured differential cross section for proton/antiproton production per Z0decay into light, charm and bottom quarks separately. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours arenot included.

The ratios of light to heavy quark production of proton/antiprotons. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to thethree flavours are not included.

Measured differential cross section for lambda/antilambda production per Z0decay into light, charm and bottom quarks separately. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours arenot included.

The ratios of light to heavy quark lambda/lambdabar production. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

Measured differential cross section for the production of neutral kaons perZ0 decay into light, charm and bottom quarks separately. The errors given are t he sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

The ratios of light to heavy quark for neutral kaon production. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

Measured differential cross section for phi meson production per Z0 decay into light, charm and bottom quarks separately. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from theunfolding procedure. Systematic errors common to the three flavours are not inc luded.

The ratios of light to heavy quark for phi meson production. The errors given are the sum in quadrature of the statistical errors and those systematic errors arising from the unfolding procedure. Systematic errors common to the three flavours are not included.

Corrected total cross sections per hadronic Z decay, and per decay into light, CQ or BQ primary flavour separately. The errors given are the sum in quadrature of experimental and extrapolation uncertainties.

Differences of total cross sections per hadronic Z decay, between CQ (and BQ) and light quarks decays. The errors given are the sum in quadrature of experimental and extrapolation uncertainties.

The differential cross sections for the production of positive and negativepions in light (u,d,s) quark jets from hadronic Z0 decays. The errors given are the sum in quadrature of statistical errors and those systematic errors arising from the light quark tagging and unfolding procedure.. Here QUARK (QUARKBAR) means any light quark (antiquark).

The normalized difference between the differential cross sections for the production of positive and negative pions in light (u,d,s) quark jets from hadronic Z0 decays. The errors given are the sum in quadrature of statistical errors and those systematic errors arising from the light quark tagging and unfolding procedure.. Here QUARK (QUARKBAR) means any light quark (antiquark).

The differential cross sections for the production of neutral K* and K*BAR mesons in light (u,d,s) quark jets from hadronic Z0 decays. The errors given arethe sum in quadrature of statistical errors and those systematic errors arising from the light quark tagging and unfolding procedure.. Here QUARK (QUARKBAR) means any light quark (antiquark).

The normalized difference between the differential cross sections for the production of neutral K* and K*BAR mesons in light (u,d,s) quark jets from hadronic Z0 decays. The errors given are the sum in quadrature of statistical errors and those systematic errors arising from the light quark tagging and unfolding procedure.. Here QUARK (QUARKBAR) means any light quark (antiquark).

The differential cross sections for the production of positive and negativeK mesons in light (u,d,s) quark jets from hadronic Z0 decays. The errors given are the sum in quadrature of statistical errors and those systematic errors arising from the light quark tagging and unfolding procedure.. Here QUARK (QUARKBAR) means any light quark (antiquark).

The normalized difference between the differential cross sections for the production of positive and negative kaons in light (u,d,s) quark jets from hadronic Z0 decays. The errors given are the sum in quadrature of statistical errors and those systematic errors arising from the light quark tagging and unfolding procedure.. Here QUARK (QUARKBAR) means any light quark (antiquark).

The differential cross sections for the production of proton and antiprotons in light (u,d,s) quark jets from hadronic Z0 decays. The errors given are the sum in quadrature of statistical errors and those systematic errors arising fromthe light quark tagging and unfolding procedure.. Here QUARK (QUARKBAR) means any light quark (antiquark).

The normalized difference between the differential cross sections for the production of protons and antiprotons in light (u,d,s) quark jets from hadronic Z0 decays. The errors given are the sum in quadrature of statistical errors and those systematic errors arising from the light quark tagging and unfolding procedure.. CCT. = Here QUARK (QUARKBAR) means any light quark (antiquark).

The differential cross sections for the production of lambdas and antilambdas in light (u,d,s) quark jets from hadronic Z0 decays. The errors given are thesum in quadrature of statistical errors and those systematic errors arising fro m the light quark tagging and unfolding procedure.. Here QUARK (QUARKBAR) means any light quark (antiquark).

The normalized difference between the differential cross sections for the production of protons and antiprotons in light (u,d,s) quark jets from hadronic Z0 decays. The errors given are the sum in quadrature of statistical errors and those systematic errors arising from the light quark tagging and unfolding procedure.. Here QUARK (QUARKBAR) means any light quark (antiquark).