Normalised cross sections of forward neutron production in DIS as a function of XF. For each measurement, the statistical, the uncorrelated systematic uncertainties and the bin-to-bin correlated systematic uncertainties due to the FNC absolute energy scale (EFNC), the measurement of the particle impact position in the FNC (XYFNC) and the model dependence of the data correction (model) are given.

Diffractive DIS dijet cross section measured differentially as a function of $\log x_P$. The global normalisation uncertainty of $7.8\%$ is not listed explicitly but is included in the total systematic uncertainty. The last two column show the correction factors for hadronisation and QED radiation, respectively. (Note: assume typo in Table 2 that $x_P$ really means $\log x_P$.).

Diffractive DIS dijet cross section measured differentially as a function of $z_P$. The global normalisation uncertainty of $7.8\%$ is not listed explicitly but is included in the total systematic uncertainty. The last two column show the correction factors for hadronisation and QED radiation, respectively.

Diffractive DIS dijet cross section measured differentially as a function of $p^{\ast}_{T,1}$.

Diffractive DIS dijet cross section measured differentially as a function of $p^{\ast}_{T,2}$.

Diffractive DIS dijet cross section measured differentially as a function of $\langle p^{\ast}_{T}\rangle$.

Diffractive DIS dijet cross section measured differentially as a function of $\Delta\eta^{\ast}$.

Diffractive DIS dijet cross section measured differentially as a function of $z_P$ and $Q^2$.

Diffractive DIS dijet cross section measured differentially as a function of $p^{\ast}_{\rm T,1}$ and $Q^2$.

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.

Bin averaged hadron level differential cross sections as a function of the variable $z_{I\!\!P}$ for diffractive dijet DIS. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections as a function of the variable $x_{I\!\!P}$ for diffractive dijet DIS. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections as a function of the variable $y$ for diffractive dijet DIS. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections as a function of the variable $Q^2$ for diffractive dijet DIS. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections for diffractive dijet DIS as a function of the variable $E_T^{*\text{jet1}}$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections for diffractive dijet DIS as a function of the variable $M_X$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections for diffractive dijet DIS as a function of the variable $\vert\Delta\eta^{\text{jets}}\vert$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections for diffractive dijet DIS as a function of the variable $\langle\eta^{\text{jets}}\rangle$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections as a function of the variable $z_{I\!\!P}$ for the dijet photoproduction kinematic range. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections as a function of the variable $x_{I\!\!P}$ for the dijet photoproduction kinematic range. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections as a function of the variable $y$ for the dijet photoproduction kinematic range. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections as a function of the variable $x_\gamma$ for the dijet photoproduction kinematic range. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections in the photoproduction kinematic range as a function of the variable $E_T^{*\text{jet1}}$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections in the photoproduction kinematic range as a function of the variable $M_X$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections in the photoproduction kinematic range as a function of the variable $\vert\Delta\eta^{\text{jets}}\vert$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections in the photoproduction kinematic range as a function of the variable $\langle\eta^{\text{jets}}\rangle$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Ratios of differential diffractive dijet $ep$ cross sections, measured in photoproduction, to measurements in DIS as a function of the variable $\vert\Delta\eta^{\text{jets}}\vert$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given.

Ratios of differential diffractive dijet $ep$ cross sections, measured in photoproduction, to measurements in DIS as a function of the variable $y$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given.

Ratios of differential diffractive dijet $ep$ cross sections, measured in photoproduction, to measurements in DIS as a function of the variable $z_{I\!\!P}$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given.

Ratios of differential diffractive dijet $ep$ cross sections, measured in photoproduction, to measurements in DIS as a function of the variable $E_T^{*\text{jet1}}$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given.

Normalised and absolute PT distributions. In the absolute cross section the first error includes the independent systematic errors. The first systematic error is the overall systematic error and the second is the overall model dependent error.

Normalised and absolute XD distributions. In the absolute cross section the first error includes the independent systematic errors. The first systematic error is the overall systematic error and the second is the overall model dependent error.

Normalised and absolute PT distributions. In the absolute cross section the first error includes the independent systematic errors. The first systematic error is the overall systematic error and the second is the overall model dependent error.

Normalised and absolute XD distributions. In the absolute cross section the first error includes the independent systematic errors. The first systematic error is the overall systematic error and the second is the overall model dependent error.

Charm contribution to F2.

Charm contribution to F2.

Charm contribution to F2.

Charm contribution to F2.

Differential x(name=gamma) photoproduction data (one entry per event).

Differential Z(NAME=POMERON) distribution for photoproduction data (one entry per event).

Differential Z(NAME=POMERON) distribution for DIS data (one entry per event).

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of the invariant mass of the diffractive system (X).

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of W.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of X(NAME=POMERON).

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of BETA=X/X(NAME=POMERON).

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), the fraction of the hadronic final state energy of the DD system which is contained in the two jets.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of X(NAME=GAMMA,C=JETS), the fraction ofthe photon momentum which enters the hard scattering.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of E(NAME=REM,C=GAMMA), the energy sum of all final state hadrons in the photon hemisphere (ETARAP<0) which lie outside the two hightest PT(RF=CM) jet cones.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), for the LOG10(X(NAME=POMERON)) range -1.5 TO -1.3.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), for the LOG10(X(NAME=POMERON)) range -1.75 TO -1.5.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), for the LOG10(X(NAME=POMERON)) range -2.0 TO -1.75.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), for the LOG10(X(NAME=POMERON)) range < -2.0.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), for the Q**2 + PT**2 range 20 TO 35 GEV**2.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), for the Q**2 + PT**2 range 35 TO 45 GEV**2.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), for the Q**2 + PT**2 range 45 TO 60 GEV**2.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), for the Q**2 + PT**2 range > 60 GEV**2.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Q**2 for the restricted interval X(NAME=POMERON) < 0.01.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of the average transverse momentum of the two jets in the c.m.frame for the restricted interval X(NAME=POMERON) < 0.01.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of Z(NAME=POMERON,C=JETS), the fraction of the hadronic final state energy of the DD system which is contained in the two jets for the restricted interval X(NAME=POMERON) < 0.01.

Average values, over the specified interval, of the differential hadron level dijet cross section as a function of PT(NAME=REM,C=POMERON), the PT sum of all final state hadrons in the pomeron hemisphere (ETARAP>0) which lie outside the two hightest PT(RF=CM) jet cones.

Average values, over the specified interval, of the differential hadron level three-jet cross section as a function of the invariant mass of the 3 jet system.

Average values, over the specified interval, of the differential hadron level three-jet cross section as a function of Z(NAME=POMERON,C=3-JETS).

Cross section as a function of Z(NAME=POMERON,C=OBSERVED).

Cross section as a function of LOG10(Q**2).

Cross section as a function of PT(P=4,RF=CM).

Cross section as a function of ETARAP(P=4).

The inclusive 3-JET cross section as a function of Bjorken scaling variableX for the Q**2 range 150 to 5000 GeV**2.

The inclusive 3-JET cross section as a function of the invariant 3-JET massfor the Q**2 range 5 to 100 GeV**2.

The inclusive 3-JET cross section as a function of the invariant 3-JET massfor the Q**2 range 150 to 5000 GeV**2.

Distribution of jet energy fraction X3 = 2E(P=4)/M(P=4_5_6) in the 3 JET centre-of-mass frame for Q**2 from 5 to 100 GeV**2.

Distribution of jet energy fraction X3 = 2E(P=4)/M(P=4_5_6) in the 3 JET centre-of-mass frame for Q**2 from 150 to 5000 GeV**2.

Distribution of jet energy fraction X4 = 2E(P=5)/M(P=4_5_6) in the 3 JET centre-of-mass frame for Q**2 from 5 to 100 GeV**2.

Distribution of jet energy fraction X4 = 2E(P=5)/M(P=4_5_6) in the 3 JET centre-of-mass frame for Q**2 from 150 to 5000 GeV**2.

Distribution of COS(THETA(C=3)) in the 3 JET centre-of-mass frame at Q**2 from 5 to 100 GeV**2. THETA(C=3) is the angle of the most energetic jet with respect to the proton beam direction.

Distribution of COS(THETA(C=3)) in the 3 JET centre-of-mass frame at Q**2 from 150 to 5000 GeV**2. THETA(C=3) is the angle of the most energetic jet with respect to the proton beam direction.

Distribution of PSI(C=3)) in the 3 JET centre-of-mass frame at Q**2 from 5 to 100 GeV**2. PSI(C=3) is the angle between the plane spanned by the highest energy jet and the proton beam and the plane containing the 3 jets.

Distribution of COS(THETA(C=3)) in the 3 JET centre-of-mass frame at Q**2 from 150 to 5000 GeV**2. PSI(C=3) is the angle between the plane spanned by the highest energy jet and the proton beam and the plane containing the 3 jets.

The NC single differential cross section, as a function of Q**2 in the range from 200 to 30000 Gev**2, for Y < 0.9 after correction (KCOR) according to theStandard Model expectation from the measured kinematic cuts y < 0.63 for Q**2 < 890 GeV**2. The first DSYS error is the uncorrelated systematic error and the second is the correlated systematic error.

No description provided.

The structure function, F2, and the reduced cross section, in NC DIS scattering at Q**2 from 150 to 30000 GeV**2 as a function if x and y. The individual corrections used to calculate F2 from the cross sections are given in the following table.

The various corrections to the cross sections used to calcuate the F2 values given in the previous table. See the text of the paper for more details.

The CC double differential cross section and the structure function term PHI(C=CC) - see text of the paper for details - at Q**2 from 150 to 1 5000 GeV**2 as a function of both x and y. Also tabulated are the QED corrections to the data, which have already been applied.

CT = The various sources of error (in percent) to the individual NC reduced cross section given in table 6 - see text of paper for more details;DTOT - TOTAL error. DSTA - STATISTICAL error. DUNC - UNCORRELATED SYSTEMATIC error. DUNC(E) - UNCORRELATED SYSTEMATIC error from the positron energy. DUNC(H) - UNCORRELATED SYSTEMATIC error from the hadronic energy. DCOR - CORRELATED SYSTEMATIC error. DCOR(E+) - CORRELATED SYSTEMATIC from one sig variation in the positron energy. DCOR(T+) - CORRELATED SYSTEMATIC from one sig variation in the positron polar angle. DCOR(H+) - CORRELATED SYSTEMATIC from one sig variation in the hadron energy. DCOR(N+) - CORRELATED SYSTEMATIC from one sig variation in the noise subtraction. DCOR(B+) - CORRELATED SYSTEMATIC from one sig variation in the background subtraction.

The various sources of error (in percent) to the individual CC double differential cross sections given in table 7 - see text of paper for more details. DTOT - TOTAL error. DSTA - STATISTICAL error. DUNC - UNCORRELATED SYSTEMATIC error. DUNC(H) - UNCORRELATED SYSTEMATIC error from the hadronic energy. DCOR - CORRELATED SYSTEMATIC error. DCOR(V+) - CORRELATED SYSTEMATIC from one sig variationin the cut on the Vap/Vp ratio. DCOR(H+) - CORRELATED SYSTEMATIC from one sig variation in the hadron energy. DCOR(N+) - CORRELATED SYSTEMATIC from one sig variation in the noise subtraction. DCOR(B+) - CORRELATED SYSTEMATIC from one sig variation in the background subtraction.

The structure function xF3 dtermined by combining the present NC E- data with previously measured E+ data at a proton enetrgy of 820 GeV. (Adloff et al. EPJ C13 (609) 2000.). The luminosity uncertainties of the E+ P and E- P data sets are included in the systematic error.

The total CC cross section in the region Q**2 > 1000 GeV**2 and Y > 0.9 after applying a small correction factor from the measured Y range from 0.03 0.85.