Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Matrix of statistical correlation coefficients of the unfolded jet cross sections at low $Q^2$.

Matrix of statistical correlation coefficients of the unfolded normalised jet cross sections at low $Q^2$.

Inclusive jet cross sections for $P_T^{\rm jet}$ = 5-7 GeV$^2$ measured as a function of $Q^2$ in the range 150-15000 GeV$^2$. The cross section values and uncertainties have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>). See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections for $P_T^{\rm jet}$ = 5-7 GeV$^2$ measured as a function of $Q^2$ in the range 150-15000 GeV$^2$. The cross section values and uncertainties have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>). See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Matrix of statistical correlation coefficients of the unfolded jet cross sections at high $Q^2$. The statistical correlations have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>).

Matrix of statistical correlation coefficients of the unfolded normalised jet cross sections at high $Q^2$. The statistical correlations have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>).

The strong coupling extracted from the normalised inclusive jet, dijet and trijet data at NLO as a function of the renormalisation scale $\mu_r$. For each $\mu_r$ the values of the strong coupling $\alpha_s(\mu_r)$ and the equivalent values $\alpha_s(M_Z)$ are given with experimental (exp) and theoretical (th) uncertainties.

$\rm dN_{ch}/dy$ versus y distribution derived from the $\rm dN_{ch}/d\eta$ distribution along with pt distributions and particle ratios measured in ALICE. Errors are systematic.

The ratio of the standard deviation of the rapidity distribution of charged particles to that expected from Landau hydrodynamics versus versus $\sqrt{s}$/nucleon-pair. The standard deviation for data for all charged particles is derived from the $\rm dN_{ch}/d\eta$ distributions measured at various energies and converted to $\rm dN_{ch}/dy$ in a consistent manner. The data from the BRAHMS and PHOBOS experiments derived by the present authors from these experiments $dN/d\eta$ distributions.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 32 GeV and jet cone opening angle 0.23.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 38 GeV and jet cone opening angle 0.23.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 19 GeV and jet cone opening angle 0.28.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 23 GeV and jet cone opening angle 0.28.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 28 GeV and jet cone opening angle 0.28.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 32 GeV and jet cone opening angle 0.28.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 38 GeV and jet cone opening angle 0.28.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 19 GeV and jet cone opening angle 0.34.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 23 GeV and jet cone opening angle 0.34.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 28 GeV and jet cone opening angle 0.34.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 32 GeV and jet cone opening angle 0.34.

Distribution of multiplicity of charged particles in a jet as a function of LN(1/X) for mean jet energy 38 GeV and jet cone opening angle 0.34.

Differential cross section DSIG/DX for the two values of longitudinal polarization of the electron beam.

Differential cross section DSIG/DY for the two values of longitudinal polarization of the electron beam.

Values of the differential cross section DSIG/DQ**2 with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DX with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DY with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DQ**2 with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DX with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DY with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 280 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 530 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 950 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 1700 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 3000 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 5300 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 9500 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 17000 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 30000 GeV**2.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

The reduced cross section at Q**2 = 60 GeV**2 for centre-of-mass energy 318.

The reduced cross section at Q**2 = 80 GeV**2 for centre-of-mass energy 318.

The reduced cross section at Q**2 = 110 GeV**2 for centre-of-mass energy 318.

The reduced cross section at Q**2 = 24 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 32 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 45 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 60 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 80 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 110 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 24 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 32 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 45 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 60 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 80 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 110 GeV**2 for centre-of-mass energy 225.

FL and F2 at Q**2 = 24 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 32 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 45 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 60 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 80 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 110 GeV**2 with no constraints on FL or F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and R as a function of Q**2 with no constraints on F2 or FL. The quantites are quoted such that Q**2/X is constant for each value which correspinds to Y = 0.71 at Ecm=225 GeV.

FL and R as a function of Q**2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2. The quantites are quoted such that Q**2/X is constant for each value which correspinds to Y = 0.71 at Ecm=225 GeV.

Percentage contributions of the various sources of systematic error for Q**2 = 24 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 32 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 45 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 60 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 80 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 110 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 24 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 32 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 45 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 60 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 80 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 110 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 24 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 32 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 45 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 60 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 80 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 110 GeV**2 for centrof-mass energy 225.

Measured D+- cross section as a function of X.

Measured D+- cross section as a function of the transverse momentum of the D meson.

Measured D+- cross section as a function of the pseudorapidity of the D meson.

Measured D0/DBAR0 cross section as a function of Q**2.

Measured D0/DBAR0 cross section as a function of X.

Measured D0/DBAR0 cross section as a function of the transverse momentum of the D meson.

Measured D0/DBAR0 cross section as a function of the pseudorapidity of the D meson.

Measured cross section for D+- mesons in Q**2 and Y bins.

Measured cross section for D0/DBAR0 mesons in Q**2 and Y bins.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D+- mesons.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D+- mesons.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D+- mesons.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D0/DBAR0 mesons not coming from D*+- decays.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D0/DBAR0 mesons not coming from D*+- decays.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D0/DBAR0 mesons not coming from D*+- decays.. The second systematic error is from the extrapolation to the full phase space.

The combined F2(NAME=CHARM) structure function from the production cross section of D+- and D0/DBAR0 mesons.. The second systematic error is from the extrapolation to the full phase space.. The additional error from the branching ratio is 3.3 PCT.

The combined F2(NAME=CHARM) structure function from the production cross section of D+- and D0/DBAR0 mesons.. The second systematic error is from the extrapolation to the full phase space.. The additional error from the branching ratio is 3.3 PCT.

The combined F2(NAME=CHARM) structure function from the production cross section of D+- and D0/DBAR0 mesons.. The second systematic error is from the extrapolation to the full phase space.. The additional error from the branching ratio is 3.3 PCT.

Differential cross sections as a function of X(C=GAMMA) from beauty and charm quarks.

Differential cross sections for the most energetic jet as a function of ET from beauty and charm quarks.

Differential cross sections for the most energetic jet as a function of ET from beauty and charm quarks.

Differential cross sections as a function of the electron ET for the jet associated to the electron from beauty or charm decays.

Proton structure function F2 at Q**2 = 55 GeV**2.

Proton structure function F2 at Q**2 = 70 GeV**2.

Proton structure function F2 at Q**2 = 90 GeV**2.

Proton structure function F2 at Q**2 = 120 GeV**2.

Proton structure function F2 at Q**2 = 190 GeV**2.

Proton structure function F2 at Q**2 = 320 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 25 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 35 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 45 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 55 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 70 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 90 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 120 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 190 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 190 GeV**2.

The diffractive cross section multiplied by (Q**2)*(Q**2+M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 1.2 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 3 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 6 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 11 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 20 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 30 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 35 GeV for W = 220 GeV.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9455 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7353 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4098 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1712 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0588 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0270 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9605 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7955 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4930 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.2244 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0805 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0374 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9690 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8333 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.5556 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.2711 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1011 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0476 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9745 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8594 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.6044 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.3125 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1209 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0576 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9798 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8861 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.6604 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.3665 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1489 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0722 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9843 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9091 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7143 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4265 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1837 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0909 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9881 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9302 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7692 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4979 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.2308 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9925 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9548 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8407 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.6109 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.3220 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1743 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9726 and Q**2 = 320 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8989 and Q**2 = 320 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7256 and Q**2 = 320 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4444 and Q**2 = 320 GeV**2.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.00015 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.00015 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0003 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0003 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0003 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0006 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0006 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0006 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0050 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0050 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.005.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.005.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.040.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.060 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Differential polarized inclusive jet cross sections as a function of jet transverse energy.

Differential polarized inclusive jet cross sections as a function of photon virtuality, Q**2.

Differential polarized inclusive jet cross sections as a function of photon virtuality, Q**2.

Differential polarized inclusive jet cross sections as a function of X. Update: contrary to the publication, this is D(SIG)/DLOG10(X) not D(SIG)/DX.

Differential polarized inclusive jet cross sections as a function of X. Update: contrary to the publication, this is D(SIG)/DLOG10(X) not D(SIG)/DX.

Integrated polarized inclusive-jet cross section in the given kinematical range for the E- beam.

Integrated polarized inclusive-jet cross section in the given kinematical range for the E+ beam.

Differential unpolarized cross section for single jet production as a function of the jet pseudorapidity.

Differential unpolarized cross section for two jet production as a function of the mean jet pseudorapidity.

Differential unpolarized cross section for three jet production as a function of the mean jet pseudorapidity.

Differential unpolarized cross section for single jet production as a function of the jet transverse energy.

Differential unpolarized cross section for two jet production as a function of the mean jet transverse energy.

Differential unpolarized cross section for three jet production as a function of the mean jet transverse energy.

Differential unpolarized cross section for single jet production as a function of photon virtuality, Q**2.

Differential unpolarized cross section for two jet production as a function of photon virtuality, Q**2.

Differential unpolarized cross section for three jet production as a function of photon virtuality, Q**2.

Differential unpolarized inclusive-jet cross section as a function of X. Update: contrary to the publication, this is D(SIG)/DLOG10(X) not D(SIG)/DX.

Integrated unpolarized jet cross section in the given kinemetical region.

Differential unpolarized dijet cross section as a function of the dijet mass.

Differential unpolarized three-jet cross section as a function of the three-jet mass.

Differential cross section DSIG/DZ(NAME=POMERON) for diffractive photoproduction of dijets as a function of Z(NAME=POMERON).

Differential cross section for the diffractive photoproduction of dijets as a function of ET of the highest jet.

Differential cross section for the diffractive photoproduction of dijets as a function of pseudorapidity (ETARAP) of the highest ET jet.

Differential cross section for the diffractive photoproduction of dijets as a function of X(C=GAMMA,OBS).

Differential cross section DSIG/DY for diffractive photoproduction of dijets as a function of Y for X(C=GAMMA,OBS) > 0.75.

Differential cross section DSIG/DM(P=5_6_7) for diffractive photoproduction of dijets as a function of M(P=5_6_7) for X(C=GAMMA,OBS) > 0.75.

Differential cross section DSIG/DX(NAME=POMERON) for diffractive photoproduction of dijets as a function of X(NAME=POMERON) for X(C=GAMMA,OBS) > 0.75.

Differential cross section DSIG/DZ(NAME=POMERON) for diffractive photoproduction of dijets as a function of Z(NAME=POMERON) for X(C=GAMMA,OBS) > 0.75.

Differential cross section DSIG/DY for diffractive photoproduction of dijets as a function of Y for X(C=GAMMA,OBS) < 0.75.

Differential cross section DSIG/DM(P=5_6_7) for diffractive photoproduction of dijets as a function of M(P=5_6_7) for X(C=GAMMA,OBS) < 0.75.

Differential cross section DSIG/DX(NAME=POMERON) for diffractive photoproduction of dijets as a function of X(NAME=POMERON) for X(C=GAMMA,OBS) < 0.75.

Differential cross section DSIG/DZ(NAME=POMERON) for diffractive photoproduction of dijets as a function of Z(NAME=POMERON) for X(C=GAMMA,OBS) < 0.75.