$M_{p\eta}$ invariant mass distribution for $E_\gamma$ = 1400-1500 MeV.

$M_{p\eta}$ invariant mass distribution for $E_\gamma$ = 1500-1600 MeV.

$M_{p\eta}$ invariant mass distribution under the conditions: $E_\gamma$ = 1400-1500 MeV; 1120 MeV $\leq M_{p\pi^0} \leq$ 1220 MeV; $\theta_p^{lab} \leq$ 25°; 25° $\leq \theta_\gamma^{lab} \leq$ 155°.

$M_{p\eta}$ invariant mass distribution under the conditions: $E_\gamma$ = 1400-1500 MeV; 1120 MeV $\leq M_{p\pi^0} \leq$ 1220 MeV; $\theta_p^{lab} \leq$ 25°; 1° $\leq \theta_\gamma^{lab} \leq$ 155°.

$M_{p\eta}$ invariant mass distribution for $E_\gamma$ = 1400-1500 MeV and $M_{p\pi^0} \leq$ 1190 MeV, allowing for all proton and photon laboratory angles.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1420-1540 MeV and $M_{p\pi^0} \leq$ 1170 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1420-1540 MeV and $M_{p\pi^0} \leq$ 1180 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1420-1540 MeV and $M_{p\pi^0} \leq$ 1190 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1420-1540 MeV and $M_{p\pi^0} \leq$ 1200 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1420-1540 MeV and $M_{p\pi^0} \leq$ 1210 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1420-1540 MeV and $M_{p\pi^0} \leq$ 1220 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1400-1420 MeV and $M_{p\pi^0} \leq$ 1190 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1420-1460 MeV and $M_{p\pi^0} \leq$ 1190 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1460-1500 MeV and $M_{p\pi^0} \leq$ 1190 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1500-1540 MeV and $M_{p\pi^0} \leq$ 1190 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1540-1600 MeV and $M_{p\pi^0} \leq$ 1190 MeV.

$M_{p\eta}$ invariant mass distribution for the incident photon energy range $E_\gamma$ = 1420-1540 MeV and $M_{p\pi^0} \leq$ 1190 MeV.

Excess yield relative to the PWA distributions in the invariant mass distributions $M^2_{p\eta}$.

Excess yield relative to the PWA distributions in the invariant mass distributions $M^2_{\pi^0\eta}$.

Excess yield relative to the PWA distributions in the invariant mass distributions $M^2_{p\pi^0}$, with a cut on the structure in the $M^2_{p\eta}$ invariant mass distribution.

Excess yield relative to the PWA distributions in the $p-\eta$ opening angle distribution in the $\gamma p$ centre-of-mass system.

Excess yield relative to the PWA distributions in the $p-\eta$ opening angle distribution in the $\gamma p$ centre-of-mass system.

Excess yield relative to the PWA distributions in the $\pi^0-\eta$ opening angle distribution in the $\gamma p$ centre-of-mass system.

Excess yield relative to the PWA distributions in the $\pi^0-\eta$ opening angle distribution in the $\gamma p$ centre-of-mass system.

Differential cross section $d\sigma/dM_{\pi^0\eta}$ for $E_\gamma$ = 1540-1600 MeV.

$M_{p\eta}$ invariant mass distribution, taken as difference to the PWA calculations (s. Fig. 11).

$M_{\pi^0\eta}$ invariant mass distribution, taken as difference to the PWA calculations (s. Fig. 11).

$\theta_{p\eta}$ opening angle distribution, taken as difference to the PWA calculations (s. Fig. 12).

$\theta_{\pi^0\eta}$ opening angle distribution, taken as difference to the PWA calculations (s. Fig. 12).

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.

$W$ dependence of the differential cross section ${\rm d}\sigma/{\rm d}|\cos\theta^*|$ in five $|\cos\theta^*|$ bins for $Q^2$=6.89 GeV$^2$.

$W$ dependence of the differential cross section ${\rm d}\sigma/{\rm d}|\cos\theta^*|$ in five $|\cos\theta^*|$ bins for $Q^2$=8.92 GeV$^2$.

$W$ dependence of the differential cross section ${\rm d}\sigma/{\rm d}|\cos\theta^*|$ in five $|\cos\theta^*|$ bins for $Q^2$=10.93 GeV$^2$.

$W$ dependence of the differential cross section ${\rm d}\sigma/{\rm d}|\cos\theta^*|$ in five $|\cos\theta^*|$ bins for $Q^2$=13.37 GeV$^2$.

$W$ dependence of the differential cross section ${\rm d}\sigma/{\rm d}|\cos\theta^*|$ in five $|\cos\theta^*|$ bins for $Q^2$=17.23 GeV$^2$.

$W$ dependence of the differential cross section ${\rm d}\sigma/{\rm d}|\cos\theta^*|$ in five $|\cos\theta^*|$ bins for $Q^2$=24.25 GeV$^2$.

$W$ dependence of the integrated cross section in nine $Q^2$ bins.

The effective exponential slope, $b_n$, obtained from the fit of double differential photoproduction cross sections ${\rm d^2}\sigma_{\gamma p}/{\rm d}x_L{\rm d}p_{T,n}^2$ to a single exponential function in bins of $x_L$. The first uncertainty represents the fit error from the statistical and uncorrelated systematic uncertainty and the second one is due to the correlated systematic uncertainty.

Energy dependence of the exclusive photoproduction of a $\rho^0$ meson associated with a leading neutron, $\gamma p \to \rho^0 n \pi^+$. The first uncertainty is statistical and the second is systematic. The global normalisation uncertainty of $4.4\%$ is not included. $\Phi_{\gamma}$ is the integral of the photon flux, Eq. (3) of paper, in a given $W_{\gamma p}$ bin.

Differential photoproduction cross section ${\rm d}\sigma_{\gamma p}/{\rm d}\eta$ for the exclusive process $\gamma p \to \rho^0 n \pi^+$ as a function of the $\rho^0$ pseudorapidity in the kinematic range $0.35 < x_L < 0.95$, $\theta_n < 0.75$ mrad and $20 < W_{\gamma p} < 100$ GeV. The statistical, uncorrelated and correlated systematic uncertainties, $\delta_{stat}$, $\delta_{sys}^{unc}$ and $\delta_{sys}^{cor}$ respectively, are given, which does not include the global normalisation error of $4.4\%$.

Differential photoproduction cross section ${\rm d}\sigma_{\gamma p}/{\rm d}t^{\prime}$ for the exclusive process $\gamma p \to \rho^0 n \pi^+$ as a function of the $\rho^0$ four-momentum transfer squared, $t^{\prime}$, in the kinematic range $0.35 < x_L < 0.95$, $\theta_n < 0.75$ mrad and $20 < W_{\gamma p} < 100$ GeV. The statistical, uncorrelated and correlated systematic uncertainties, $\delta_{stat}$, $\delta_{sys}^{unc}$ and $\delta_{sys}^{cor}$ respectively, are given, which does not include the global normalisation error of $4.4\%$.

Exponential slopes, $b_1$ and $b_2$, and the ratio $\sigma_1/\sigma_2$, obtained from the components of fit, Eq. (14) of paper, to the differential cross section ${\rm d}\sigma_{\gamma p}/{\rm d}t^{\prime}$ in bins of $x_L$. The errors represent the statistical and systematic uncertainties added in quadrature.

Exponential slopes, $b_1$ and $b_2$, and the ratio $\sigma_1/\sigma_2$, obtained from the components of fit, Eq. (14) of paper, to the differential cross section ${\rm d}\sigma_{\gamma p}/{\rm d}t^{\prime}$ in bins of $p_{T,n}^2$. The errors represent the statistical and systematic uncertainties added in quadrature.

Energy dependence of elastic $\rho^0$ photoproduction on the pion, $\gamma \pi^+ \to \rho^0 \pi^+$, extracted in the one-pion-exchange approximation using OPE1 sample. The first uncertainty represents the full experimental error and the second is the model error coming from the pion flux uncertainty (see text). $\Gamma_\pi(x_L)$ represents the value of the pion flux, Eqs. (5-6) of paper, integrated over the $p_{T,n}<0.2$ GeV range, at a given $x_L$.

Cross section of elastic $\rho^0$ photoproduction on the pion, $\gamma \pi^+ \to \rho^0 \pi^+$, extracted in the one-pion-exchange approximation using three different samples: full sample, OPE1 and OPE2. The first uncertainty represents the full experimental error and the second is the model error coming from the pion flux uncertainty (see text). $\Gamma_\pi$ represents the value of the pion flux, Eqs. (5-6) of paper, integrated over the corresponding $(x_L,p_{T,n})$ range.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.200-1.250 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.250-1.300 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.300-1.350 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.350-1.400 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.400-1.450 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.450-1.500 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.500-1.550 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.550-1.600 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.600-1.650 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.650-1.700 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.700-1.800 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.800-1.900 GeV.

Differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.900-2.000 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.125-1.150 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.150-1.175 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.175-1.20 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.200-1.250 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.250-1.300 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.300-1.350 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.350-1.400 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.400-1.450 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.450-1.500 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.500-1.550 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.550-1.600 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.600-1.650 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.650-1.700 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.700-1.800 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.800-1.900 GeV.

Inclusive differential cross-sections of $\omega$ mesons produced off the free proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.900-2.000 GeV.

Total cross-section as a function of the incident photon energy for $\omega$ mesons produced off the free proton obtained from exclusive and inclusive analysis$.

Slope parameter and horizontal level from the fits to the differential cross-sections $d\sigma/dt$ for $\omega$ mesons produced off the free proton.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.158-1.208 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.208-1.233 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.233-1.258 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.258-1.308 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.308-1.358 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.358-1.408 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.408-1.508 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.508-1.608 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.608-1.708 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.708-1.808 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.808-1.908 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound proton versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.908-2.008 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.158-1.208 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.208-1.233 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.233-1.258 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.258-1.308 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.308-1.358 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.358-1.408 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.408-1.508 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.508-1.608 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.608-1.708 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.708-1.808 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.808-1.908 GeV.

Differential cross-sections of $\omega$ mesons produced off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.908-2.008 GeV.

Slope parameter and horizontal level from the fits to the differential cross-sections $d\sigma/dt$ for $\omega$ mesons produced off the bound proton.

Slope parameter and horizontal level from the fits to the differential cross-sections $d\sigma/dt$ for $\omega$ mesons produced off the bound neutron.

Inclusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.158-1.208 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.208-1.233 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.233-1.258 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.258-1.308 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.308-1.358 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.358-1.408 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.408-1.508 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.508-1.608 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.608-1.708 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.708-1.808 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.808-1.908 GeV.

Inlusive differential cross-sections of $\omega$ mesons produced off deuterium versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.908-2.008 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.158-1.208 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.208-1.233 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.233-1.258 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.258-1.308 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.308-1.358 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.358-1.408 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.408-1.508 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.508-1.608 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.608-1.708 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.708-1.808 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.808-1.908 GeV.

Sum of the exclusive differential cross-sections of $\omega$ mesons produced off the bound proton and off the bound neutron versus $\cos(\theta^\omega_{\mathrm{c.m.}})$ and versus the momentum transfer to the nucleon, $t$, for incident photon energy $E_\gamma$ = 1.908-2.008 GeV.

Total cross-section as a function of the incident photon energy for $\omega$ mesons produced off the bound proton $\sigma_p^{\mathrm{bound}}$, off the bound neutron $\sigma_n^{\mathrm{bound}}$, the sum of the two exclusive cross-sections $\sigma_p^{\mathrm{bound}}+\sigma_n^{\mathrm{bound}}$, the quasi-free inclusive cross-section $\sigma_{\mathrm{incl}}$ and the cross-section off the neutron calculated by $\sigma_{\mathrm{incl}}-\sigma_p^{\mathrm{bound}}$.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.16-1.17, 1.17-1.18 and 1.18-1.19.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.19-1.20, 1.20-1.21 and 1.21-1.22.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.22-1.23, 1.23-1.24 and 1.24-1.25.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.25-1.26, 1.26-1.27 and 1.27-1.28.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.28-1.29, 1.29-1.30 and 1.30-1.31.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.31-1.32, 1.32-1.33 and 1.33-1.34.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.34-1.35, 1.35-1.36 and 1.36-1.37.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.37-1.38, 1.38-1.39 and 1.39-1.40.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.40-1.41, 1.41-1.42 and 1.42-1.43.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.43-1.44, 1.44-1.45 and 1.45-1.46.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.46-1.47, 1.47-1.48 and 1.48-1.49.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.49-1.50, 1.50-1.51 and 1.51-1.52.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.52-1.53, 1.53-1.54 and 1.54-1.55.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.55-1.56, 1.56-1.57 and 1.57-1.58.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.58-1.59, 1.59-1.60 and 1.60-1.61.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.61-1.62, 1.62-1.63 and 1.63-1.64.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.64-1.65, 1.65-1.66 and 1.66-1.67.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.67-1.68, 1.68-1.69 and 1.69-1.70.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.70-1.71, 1.71-1.72 and 1.72-1.73.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.73-1.74, 1.74-1.75 and 1.75-1.76.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.76-1.77, 1.77-1.78 and 1.78-1.79.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.79-1.80, 1.80-1.81 and 1.81-1.82.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.82-1.83, 1.83-1.84 and 1.84-1.85.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.85-1.86, 1.86-1.87 and 1.87-1.88.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.88-1.89, 1.89-1.90 and 1.90-1.92.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.92-1.94, 1.94-1.96 and 1.96-1.98.

The cos(Theta*) dependence of the differential cross section for the W ranges 1.98-2.00, 2.00-2.02 and 2.02-2.04.

The cos(Theta*) dependence of the differential cross section for the W ranges 2.04-2.06, 2.06-2.08 and 2.08-2.10.

The cos(Theta*) dependence of the differential cross section for the W ranges 2.10-2.12, 2.12-2.14 and 2.14-2.16.

The cos(Theta*) dependence of the differential cross section for the W ranges 2.16-2.18, 2.18-2.20 and 2.20-2.22.

The cos(Theta*) dependence of the differential cross section for the W ranges 2.22-2.24, 2.24-2.26 and 2.26-2.28.

The cos(Theta*) dependence of the differential cross section for the W ranges 2.28-2.30, 2.30-2.32 and 2.32-2.34.

The cos(Theta*) dependence of the differential cross section for the W ranges 2.34-2.36, 2.36-2.38 and 2.38-2.40.

The cos(Theta*) dependence of the differential cross section for the W ranges 2.40-2.44, 2.44-2.48 and 2.48-2.52.

The cos(Theta*) dependence of the differential cross section for the W ranges 2.52-2.56, 2.56-2.60 and 2.60-2.70.

The cos(Theta*) dependence of the differential cross section for the W ranges 2.70-2.80, 2.80-2.90 and 2.90-3.00.

The cos(Theta*) dependence of the differential cross section for the W ranges 3.00-3.10, 3.10-3.20 and 3.20-3.30.

Measured differential photoproduction cross sections as a function of the squared transverse momentum of the J/PSI in 4 bins of elasticity.

Measured differential photoproduction cross sections as a function of the elasticity of the J/PSI in 4 bins of transverse momentum.

Measured differential electroproduction cross section as a function of Q**2.

Measured differential electroproduction cross section as a function of the squared transverse momentum of the J/PSI in the GAMMA* P frame.

Measured differential electroproduction cross section as a function of the elasticity of the J/PSI.

Measured differential electroproduction cross section as a function of the photon-proton centre of mass energy W.

Measured differential electroproduction cross section as a function of the squared transverse momentum of the J/PSI in the GAMMA* P rest frame.

Measured differential electroproduction cross section as a function of the squared transverse momentum of the J/PSI in the GAMMA* P rest frame.

Measured differential electroproduction cross section as a function of the squared transverse momentum of the J/PSI in the GAMMA* P rest frame.

Measured differential electroproduction cross section as a function of the elasticity of the J/PSI.

Measured differential electroproduction cross section as a function of the elasticity of the J/PSI.

Measured differential electroproduction cross section as a function of the elasticity of the J/PSI.

Measured polarization parameter in the Helicity Frame. Here ALPHA is given by DSIG/DCOS(THETA) ~ 1+ ALPHA COS(THETA)**2 and NU is given by DSIG/DPHI ~ 1+ ALPHA/3 + (NU/3)*COS(2THETA).

Measured polarization parameter in the Collins-Soper Frame. Here ALPHA is given by DSIG/DCOS(THETA) ~ 1+ ALPHA COS(THETA)**2 and NU is given by DSIG/DPHI ~ 1+ ALPHA/3 + (NU/3)*COS(2THETA).

Measured polarization parameter in the Helicity Frame. Here ALPHA is given by DSIG/DCOS(THETA) ~ 1+ ALPHA COS(THETA)**2 and NU is given by DSIG/DPHI ~ 1+ ALPHA/3 + (NU/3)*COS(2THETA).

Measured polarization parameter in the Collins-Soper Frame. Here ALPHA is given by DSIG/DCOS(THETA) ~ 1+ ALPHA COS(THETA)**2 and NU is given by DSIG/DPHI ~ 1+ ALPHA/3 + (NU/3)*COS(2THETA).

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.

Differential cross section for ETA production at incident photon energy 1.000 to 1.050 GeV.

Differential cross section for ETA production at incident photon energy 1.050 to 1.100 GeV.

Differential cross section for ETA production at incident photon energy 1.100 to 1.150 GeV.

Differential cross section for ETA production at incident photon energy 1.150 to 1.200 GeV.

Differential cross section for ETA production at incident photon energy 1.200 to 1.250 GeV.

Differential cross section for ETA production at incident photon energy 1.250 to 1.300 GeV.

Differential cross section for ETA production at incident photon energy 1.300 to 1.350 GeV.

Differential cross section for ETA production at incident photon energy 1.350 to 1.400 GeV.

Differential cross section for ETA production at incident photon energy 1.400 to 1.450 GeV.

Differential cross section for ETA production at incident photon energy 1.450 to 1.500 GeV.

Differential cross section for ETA production at incident photon energy 1.500 to 1.550 GeV.

Differential cross section for ETA production at incident photon energy 1.550 to 1.600 GeV.

Differential cross section for ETA production at incident photon energy 1.600 to 1.650 GeV.

Differential cross section for ETA production at incident photon energy 1.650 to 1.700 GeV.

Differential cross section for ETA production at incident photon energy 1.700 to 1.750 GeV.

Differential cross section for ETA production at incident photon energy 1.750 to 1.800 GeV.

Differential cross section for ETA production at incident photon energy 1.800 to 1.850 GeV.

Differential cross section for ETA production at incident photon energy 1.850 to 1.900 GeV.

Differential cross section for ETA production at incident photon energy 1.900 to 1.950 GeV.

Differential cross section for ETA production at incident photon energy 1.950 to 2.000 GeV.

Differential cross section for ETA production at incident photon energy 2.000 to 2.050 GeV.

Differential cross section for ETA production at incident photon energy 2.050 to 2.100 GeV.

Differential cross section for ETA production at incident photon energy 2.100 to 2.150 GeV.

Differential cross section for ETA production at incident photon energy 2.150 to 2.200 GeV.

Differential cross section for ETA production at incident photon energy 2.200 to 2.250 GeV.

Differential cross section for ETA production at incident photon energy 2.250 to 2.300 GeV.

Differential cross section for ETA production at incident photon energy 2.300 to 2.350 GeV.

Differential cross section for ETA production at incident photon energy 2.350 to 2.400 GeV.

Differential cross section for ETA production at incident photon energy 2.400 to 2.450 GeV.

Differential cross section for ETA production at incident photon energy 2.450 to 2.500 GeV.

Differential cross section for ETA production at incident photon energy 2.500 to 2.550 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.500 to 1.550 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.550 to 1.600 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.600 to 1.650 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.650 to 1.700 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.700 to 1.750 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.750 to 1.800 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.800 to 1.850 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.850 to 1.900 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.900 to 1.950 GeV.

Differential cross section for ETAPRIME production at incident photon energy 1.950 to 2.000 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.000 to 2.050 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.050 to 2.100 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.100 to 2.150 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.150 to 2.200 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.200 to 2.250 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.250 to 2.300 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.300 to 2.350 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.350 to 2.400 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.400 to 2.450 GeV.

Differential cross section for ETAPRIME production at incident photon energy 2.450 to 2.500 GeV.

Total P GAMMA --> ETA P cross section.

Total P GAMMA --> ETAPRIME P cross section.