Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction off protons with a Soeding-inspired analytic function --- statistical correlations only. Only one half of the (symmetric) matrix is stored.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction off protons, differential in the dipion mass and in bins of $W$. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction off protons, differential in the dipion mass and in bins of $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons, in bins of the photon-proton energy $W$. The cross section is defined as the integral of the relativistic Breit Wigner resonance in the dipion mass over the range $2m_\pi<m_{\pi\pi}<1.53$ GeV. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons in bins of the photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction cross sections off protons as a function of energy. Parameters with subscript "el" and "pd" correspond to elastic and proton-dissociative cross sections, respectively.

Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction cross sections off protons as a function of energy --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of elastic $\rho^0(770)$ photoproduction cross section off protons as a function of energy (various experiments)

Fit of elastic $\rho^0(770)$ photoproduction cross sections off protons as a function of energy (various experiments) --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction cross section off protons, double-differential in the dipion mass and the momentum transfer $\vert t\vert$. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction cross section off protons, double-differential in the dipion mass and the momentum transfer $\vert t\vert$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons, single-differential in the momentum transfer $\vert t\vert$. The cross section is defined as the integral of the relativistic Breit Wigner resonance in the dipion mass over the range $2m_\pi<m_{\pi\pi}<1.53$ GeV. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons, single differential in the momentum transfer $\vert t\vert$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$. Parameters with subscript "el" and "pd" correspond to elastic and proton-dissociative cross sections, respectively.

Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction double-differenial cross section off protons, as a function of the dipion mass and the momentum transfer $\vert t\vert$, in bins of the photon-proton energy $W$ The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction double-differenial cross section off protons, as a function of the dipion mass and the momentum transfer $\vert t\vert$, in bins of the photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons, single-differential in the momentum transfer $\vert t\vert$, in bins of the photon-proton energy $W$. The cross section is defined as the integral of the relativistic Breit Wigner resonance in the dipion mass over the range $2m_\pi<m_{\pi\pi}<1.53$ GeV. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction cross section off protons, single differential in the momentum transfer $\vert t\vert$ and in bins of the photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Regge fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ and photon-proton energy $W$. Parameters with subscript "el" and "pd" correspond to elastic and proton-dissociative cross sections, respectively.

Regge fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ and photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of $b$-slopes in elastic ($m_Y=m_p$) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ in bins of photon-proton energy $W$.

Fit of $b$-slopes in elastic ($m_Y=m_p$) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ in bins of photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of Pomeron trajectories in elastic ($m_Y=m_p$) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ in bins of photon-proton energy $W$.

Fit of Pomeron trajectories in elastic ($m_Y=m_p$) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ in bins of photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Q**2 dependence of the GAMMA* P cross section for proton dissociative PHI meson production at mean W There is an additional overall normalization uncertainty of 5.3 PCT.

Q**2 dependence of the ratio pf the PHI to RHO0 elastic cross section for mean W There is an additional overall normalization uncertainty of 4.0 PCT.

Q**2 + MASS(V)**2 dependence of the ratio pf the PHI to RHO0 elastic cross section for mean W There is an additional overall normalization uncertainty of 4.0 PCT.

Q**2 dependence of the longitudinal and transverse GAMMA* P cross sections for elastic RHO0 production at mean W There is an additional overall normalization uncertainty of 3.9 PCT.

Q**2 dependence of the longitudinal and transverse GAMMA* P cross sections for elastic PHI production at mean W There is an additional overall normalization uncertainty of 4.7 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for dissociative RHO0 production for Q**2 There is an additional overall normalization uncertainty of 4.6 PCT.

W dependence of the GAMMA* P cross section for dissociative RHO0 production for Q**2 There is an additional overall normalization uncertainty of 4.6 PCT.

W dependence of the GAMMA* P cross section for dissociative RHO0 production for Q**2 There is an additional overall normalization uncertainty of 4.6 PCT.

W dependence of the GAMMA* P cross section for elastic PHI production for Q**2 There is an additional overall normalization uncertainty of 4.7 PCT.

W dependence of the GAMMA* P cross section for elastic PHI production for Q**2 There is an additional overall normalization uncertainty of 4.7 PCT.

W dependence of the GAMMA* P cross section for elastic PHI production for Q**2 There is an additional overall normalization uncertainty of 4.7 PCT.

W dependence of the GAMMA* P cross section for dissociative PHI production for Q**2 There is an additional overall normalization uncertainty of 5.3 PCT.

T dependence of the GAMMA* P cross section for elastic RHO0 production for several values. There is an additional overall normalization uncertainty of 3.9 PCT.

T dependence of the GAMMA* P cross section for dissociative RHO0 production for several values. There is an additional overall normalization uncertainty of 4.6 PCT.

T dependence of the GAMMA* P cross section for elastic PHI production for several values. There is an additional overall normalization uncertainty of 4.7 PCT.

T dependence of the GAMMA* P cross section for dissociative PHI production for several values. There is an additional overall normalization uncertainty of 5.3 PCT.

Q**2 dependence of the slope of the T distribution in elastic RHO0 production.

Q**2 dependence of the slope of the T distribution in elastic PHI production.

Q**2 dependence of the slope of the T distribution in dissociative RHO0 production.

Q**2 dependence of the slope of the T distribution in dissociative PHI production.

W dependence of the GAMMA* P cross section for dissociative RHO0 production in four ABS(T) bins at Q**2 There is an additional normalization uncertainty of 4 PCT.

W dependence of the GAMMA* P cross section for dissociative RHO0 production in four ABS(T) bins at Q**2 There is an additional normalization uncertainty of 4 PCT.

Q**2 dependence of the ratio of proton dissociative to elastic RHO0 meson total cross section. There is an additional overall normalization uncertainty of 2.4 PCT.

Q**2 dependence of the ratio of proton dissociative to elastic PHI meson total cross section. There is an additional overall normalization uncertainty of 2.4 PCT.

Q**2 dependence of the ratio of proton dissociative to elastic RHO0 meson differential cross section at T=0. There is an additional overall normalization uncertainty of 2.4 PCT.

Q**2 dependence of the ratio of proton dissociative to elastic PHI mesondifferential cross section at T=0. There is an additional overall normalization uncertainty of 2.4 PCT.

Slope differences between elastic and proton dissociative scattering for RHO0 meson production.

Slope differences between elastic and proton dissociative scattering for PHI meson production.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Q**2 dependence of the matrix element combination RHO(JJ=5,MM=00) + 2*RHO(JJ=5,MM=11).

Q**2 dependence of the matrix element combination RHO(JJ=1,MM=00) + 2*RHO(JJ=1,MM=11).

T dependence of the matrix element combination RHO(JJ=5,MM=00) + 2*RHO(JJ=5,MM=11).

T dependence of the matrix element combination RHO(JJ=1,MM=00) + 2*RHO(JJ=1,MM=11).

Q**2 dependence of the ratio R.

Q**2 dependence of the ratio R.

W dependence of the ratio R.

W dependence of the ratio R.

W dependence of the ratio R.

T dependence of the ratio R.

T dependence of the ratio R.

Di-pion mass dependence of the ratio R.

Di-pion mass dependence of the ratio R.

Dependence of the exponential slope of the T distribution as a function of the di-pion mass for the Q**2 range 2.5 to 5 GeV**2.

Dependence of the exponential slope of the T distribution as a function of the di-pion mass for the Q**2 range 5 to 60 GeV**2.

Q**2 dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production.

Q**2 dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for PHI production.

T dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production in the Q**2 range 2.5 to 5 GeV**2.

T dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production in the Q**2 range 5 to 60 GeV**2.

T dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for PHI production in the Q**2 range 2.5 to 60 GeV**2.

Di-pion mass dependence of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production in the Q**2 range 2.5 to 5 GeV**2.

Di-pion mass dependence of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production in the Q**2 range 5 to 60 GeV**2.

The multiplicity of charged hadrons for three intervals of mass of the charged hadron system in the forward region.

The multiplicity of charged hadrons for three intervals of mass of the charged hadron system in the backward region.

The multiplicity of positively charged hadrons for three intervals of mass of the charged hadron system in the full phase space region.

The multiplicity of negatively charged hadrons for three intervals of mass of the charged hadron system in the full phase space region.

Charged particle rapidity spectra for three intervals of the mass of the charged haron system.

The central region charged particle density.

The parameter RHO which relects the correlation between the number of particles in the forward and backward hemisphere.

Normalised distribution of (1-THRUST) where THRUST is w.r.t the axis which maximises the sum of the longitudinal momenta in the current hemisphere, for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the axis which maximises the sum of the longitudinal momenta in the current hemisphere, for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the axis which maximises the sum of the longitudinal momenta in the current hemisphere, for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the axis which maximises the sum of the longitudinal momenta in the current hemisphere, for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the vitrual photon axis, for Q = 14.0 to 16.0 GeV and X = 0.00841 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the vitrual photon axis, for Q = 16.0 to 20.0 GeV and X = 0.01180 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the vitrual photon axis, for Q = 20.0 to 30.0 GeV and X = 0.02090 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the vitrual photon axis, for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the vitrual photon axis, for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the vitrual photon axis, for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Normalised distribution of (1-THRUST) where THRUST is w.r.t the vitrual photon axis, for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Normalised distribution of Jet Broadening (B), for Q = 14.0 to 16.0 GeV and X = 0.00841 .

Normalised distribution of Jet Broadening (B), for Q = 16.0 to 20.0 GeV and X = 0.01180 .

Normalised distribution of Jet Broadening (B), for Q = 20.0 to 30.0 GeV and X = 0.02090 .

Normalised distribution of Jet Broadening (B), for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Normalised distribution of Jet Broadening (B), for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Normalised distribution of Jet Broadening (B), for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Normalised distribution of Jet Broadening (B), for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Normalised distribution of the squared Jet Mass (RHO), for Q = 14.0 to 16.0 GeV and X = 0.00841 .

Normalised distribution of the squared Jet Mass (RHO), for Q = 16.0 to 20.0 GeV and X = 0.01180 .

Normalised distribution of the squared Jet Mass (RHO), for Q = 20.0 to 30.0 GeV and X = 0.02090 .

Normalised distribution of the squared Jet Mass (RHO), for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Normalised distribution of the squared Jet Mass (RHO), for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Normalised distribution of the squared Jet Mass (RHO), for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Normalised distribution of the squared Jet Mass (RHO), for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Normalised distribution of the C-Parameter, for Q = 14.0 to 16.0 GeV and X = 0.00841 .

Normalised distribution of the C-Parameter, for Q = 16.0 to 20.0 GeV and X = 0.01180 .

Normalised distribution of the C-Parameter, for Q = 20.0 to 30.0 GeV and X = 0.02090 .

Normalised distribution of the C-Parameter, for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Normalised distribution of the C-Parameter, for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Normalised distribution of the C-Parameter, for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Normalised distribution of the C-Parameter, for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Mean values of the event shape variables.

Covariance matrix for (1-THRUST(C)), for Q = 14.0 to 16.0 GeV and X = 0.00841 .

Covariance matrix for (1-THRUST(C)), for Q = 16.0 to 20.0 GeV and X = 0.01180 .

Covariance matrix for (1-THRUST(C)), for Q = 20.0 to 30.0 GeV and X = 0.02090 .

Covariance matrix for (1-THRUST(C)), for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Covariance matrix for (1-THRUST(C)), for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Covariance matrix for (1-THRUST(C)), for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Covariance matrix for (1-THRUST(C)), for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Covariance matrix for (1-THRUST), for Q = 14.0 to 16.0 GeV and X = 0.00841 .

Covariance matrix for (1-THRUST), for Q = 16.0 to 20.0 GeV and X = 0.01180 .

Covariance matrix for (1-THRUST), for Q = 20.0 to 30.0 GeV and X = 0.02090 .

Covariance matrix for (1-THRUST), for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Covariance matrix for (1-THRUST), for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Covariance matrix for (1-THRUST), for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Covariance matrix for (1-THRUST), for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Covariance matrix for the Jet Broadening (B), for Q = 14.0 to 16.0 GeV and X = 0.00841 .

Covariance matrix for the Jet Broadening (B), for Q = 16.0 to 20.0 GeV and X = 0.01180 .

Covariance matrix for the Jet Broadening (B), for Q = 20.0 to 30.0 GeV and X = 0.02090 .

Covariance matrix for the Jet Broadening (B), for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Covariance matrix for the Jet Broadening (B), for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Covariance matrix for the Jet Broadening (B), for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Covariance matrix for the Jet Broadening (B), for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Covariance matrix for the squared Jet Mass (RHO), for Q = 14.0 to 16.0 GeV and X = 0.00841 .

Covariance matrix for the squared Jet Mass (RHO), for Q = 16.0 to 20.0 GeV and X = 0.01180 .

Covariance matrix for the squared Jet Mass (RHO), for Q = 20.0 to 30.0 GeV and X = 0.02090 .

Covariance matrix for the squared Jet Mass (RHO), for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Covariance matrix for the squared Jet Mass (RHO), for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Covariance matrix for the squared Jet Mass (RHO), for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Covariance matrix for the squared Jet Mass (RHO), for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Covariance matrix for the C-Parameter, for Q = 14.0 to 16.0 GeV and X = 0.00841 .

Covariance matrix for the C-Parameter, for Q = 16.0 to 20.0 GeV and X = 0.01180 .

Covariance matrix for the C-Parameter, for Q = 20.0 to 30.0 GeV and X = 0.02090 .

Covariance matrix for the C-Parameter, for Q = 30.0 to 50.0 GeV and X = 0.04910 .

Covariance matrix for the C-Parameter, for Q = 50.0 to 70.0 GeV and X = 0.11600 .

Covariance matrix for the C-Parameter, for Q = 70.0 to 100.0 GeV and X = 0.19900 .

Covariance matrix for the C-Parameter, for Q = 100.0 to 200.0 GeV and X = 0.32300 .

Normalised decay angular distribution w.r.t. the azimuthal anlge PHI.

Spin density matrix elements from fot to the decay angular distributions.