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.

The combined differential $D^{*\pm}$-production cross section as a function of $Q^2$, with its uncorrelated and correlated uncertainties.

The combined differential $D^{*\pm}$-production cross section as a function of $y$, with its uncorrelated and correlated uncertainties.

The combined double-differential $D^{*\pm}$-production cross section as a function of $Q^2$ and $y$, with its uncorrelated and correlated uncertainties.

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.

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 $Q^2$.

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.

The neutral current reduced cross section at Q^2=90 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=120 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=150 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=200 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=250 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=300 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=400 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=500 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=650 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=800 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=35 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=45 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=60 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=90 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=120 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=150 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=200 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=250 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=300 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=400 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=500 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=650 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=800 GeV^2 for a proton energy of 575 GeV.

The proton structure functions FL and F2 measured at Q^2=1.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=2.0 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=2.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=3.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=5.0 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=6.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=8.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=12 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=15 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=20 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=25 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=35 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=45 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=60 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=90 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=120 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=150 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=200 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=250 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=300 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=400 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=500 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=650 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=800 GeV^2 as a function of X without model assumptions.

The proton structure function FL obtained by averaging the FL data from the previous tables.

The proton-dissociative photoproduction cross section derived from the low-energy data set as a function of the photon-proton centre-of-mass energy W. PHI_T is the transeverse polarised photon flux.

The elastic photoproduction differential cross section derived from the high-energy data set as a function of the negative squared momentum transfer at the proton vertex T.

The proton-dissociative photoproduction differential cross section derived from the high-energy data set as a function of the negative squared momentum transfer at the proton vertex T.

The elastic photoproduction differential cross section derived from the low-energy data set as a function of the negative squared momentum transfer at the proton vertex T.

The proton-dissociative photoproduction differential cross section derived from the low-energy data set as a function of the negative squared momentum transfer at the proton vertex T.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity PT interval 0-1.5 in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity PT interval 1.5-5 in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of -25.8 % for Q^2 values of 8000, 12000, 20000, 30000 and 50000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 8000, 12000, 20000, 30000 and GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 8000, 12000, 20000, and GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 8000, 12000, 20000, 30000 and GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of -25.8 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of -25.8 % for Q^2 values of 5000, 8000, 15000, 30000 and GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 5000, 8000, 15000, and GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 5000, 8000, 15000, and GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 5000, 8000, 15000, and GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 90, 120, 150, 200 and 250 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 300, 400, 500, 650 and 800 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 90, 120, 150, 200 and 250 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 300, 400, 500, 650 and 800 GeV^2.

The Neutral Current Reduced Cross Section for E+- P interactions with a beam polarisation of 0 % as a function of Q^2 at Y=0.75.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 8000, 12000, 20000, 30000 and 50000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 8000, 12000, 20000, 30000 and GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 5000, 8000, 15000, 30000 and GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 5000, 8000, 15000, and GeV^2.

The combined HERA I+II Neutral Current Reduced Cross Section and F2 for E- P interactions with a beam polarisation of 0 %.

The combined HERA I+II Neutral Current Reduced Cross Section and F2 for E+ P interactions with a beam polarisation of 0 %.

The combined HERA I+II Charged Current Double Differential Cross Section and Reduced Cross Section for E- P interactions with a beam polarisation of 0 %.

The combined HERA I+II Charged Current Double Differential Cross Section and Reduced Cross Section for E+ P interactions with a beam polarisation of 0 %.

The Neutral Current DSIG/DQ**2 for E- P interactions with a beam polarisation of -25.8% and +36.0% as a function of Q^2 at Y<0.9.

The Neutral Current DSIG/DQ**2 for E+ P interactions with a beam polarisation of -37.0% and +32.5% as a function of Q^2 at Y<0.9.

The Charged Current DSIG/DQ**2 for E- P interactions with a beam polarisation of -25.8% and +36.0% as a function of Q^2 at Y<0.9.

The Charged Current DSIG/DQ**2 for E+ P interactions with a beam polarisation of -37.0% and +32.5% as a function of Q^2 at Y<0.9.

The Neutral Current DSIG/DQ**2 for E+- P interactions with a beam polarisation of 0% as a function of Q^2 at Y<0.9.

The Charged Current DSIG/DQ**2 for E+- P interactions with a beam polarisation of 0% as a function of Q^2 at Y<0.9.

The Combined HERA I+ II Neutral Current DSIG/DQ**2 for E+- P interactions with a beam polarisation of 0% as a function of Q^2 at Y<0.9.

The Combined HERA I+ II Neutral Current DSIG/DQ**2 for E+- P interactions with a beam polarisation of 0% as a function of Q^2 at Y<0.9.

The measured structure function F2(gZ) determined using the polarised HERA II data set for Q^2 values of 200, 250, 300 and 400 GeV^2.

The measured structure function F2(gZ) determined using the polarised HERA II data set for Q^2 values of 500, 650, 800 and 1000 GeV^2.

The measured structure function F2(gZ) determined using the polarised HERA II data set for Q^2 values of 1200, 1500, 2000 and 3000 GeV^2.

The measured structure function F2(gZ) determined using the polarised HERA II data set for Q^2 values of 5000, 8000, 12000 and 20000 GeV^2.

Averaged structure function F2(gz) for a Q^2 value of 1500 GeV^2 determined using the polarised HERA II data set.

The measured structure function xF3(gZ) determined using the polarised HERA II data set for Q^2 values of 5000, 8000, 12000, 20000 and 30000 GeV^2.

The measured structure function xF3(gZ) determined using the polarised HERA II data set for Q^2 values of 1200, 1500, 2000, 3000 and GeV^2.

Averaged structure function xF3(gz) for a Q^2 value of 1500 GeV^2 determined using the polarised HERA II data set.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0003 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0003 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=3.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=5.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=6.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=15.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=20.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=25.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=35.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=45.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=3.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=5.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=6.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=15.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=20.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=25.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=35.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=45.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=60.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=90.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=3.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=5.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=6.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=15.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=20.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=25.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=35.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=45.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=60.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=90.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=200.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=400.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=3.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=5.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=6.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=15.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=20.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=25.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=35.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=45.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=60.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=90.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=200.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=400.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=800.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=1600.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.