Data from Figure 3b on charged pion production. Data correspond to charged particle production, corrected to the contribution from (PI+ + PI-)/2.

Data from Figure 3b on charged pion production. Data correspond to charged particle production, corrected to the contribution from (PI+ + PI-)/2.

Data from Figure 3c on charged pion production. Data correspond to charged particle production, corrected to the contribution from (PI+ + PI-)/2.

Data from Figure 3d on charged pion production. Data correspond to charged particle production, corrected to the contribution from (PI+ + PI-)/2.

Data from Figure 4a on forward jet production differential in x, low PT

Data from Figure 4a on forward jet production differential in x, high PT

Data from Figure 5a on forward jet production differential in delta(phi), low x

Data from Figure 5b on forward jet production differential in delta(phi), high x

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

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

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

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

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

The central region charged particle density.

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

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range < 1.5 and the ET range > 8 GeV using the inclusive KT jet finding algorithm.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range 1.5 TO 2.2 and the ET range > 8 GeV using the inclusive KT jet finding algorithm.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range > 2.2 and the ET range > 8 GeV using the inclusive KT jet finding algorithm.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range < 1.5 and the ET range 5 TO 8 GeV using the cone jet finding algorthm with cone radius = 1.0.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range 1.5 TO 2.2 and the ET range 5 TO 8 GeV using the cone jet finding algorthm with cone radius = 1.0.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range > 2.2 and the ET range 5 TO 8 GeV using the cone jet finding algorthm with cone radius = 1.0.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range < 1.5 and the ET range > 8 GeV using the cone jet finding algorthm with cone radius = 1.0.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range 1.5 TO 2.2 and the ET range > 8 GeV using the cone jet finding algorthm with cone radius = 1.0.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range > 2.2 and the ET range > 8 GeV using the cone jet finding algorthm with cone radius = 1.0.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range < 1.5 and the ET range 5 TO 8 GeV using the cone jet finding algorthm with cone radius = 0.7.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range 1.5 TO 2.2 and the ET range 5 TO 8 GeV using the cone jet finding algorthm with cone radius = 0.7.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range > 2.2 and the ET range 5 TO 8 GeV using the cone jet finding algorthm with cone radius = 0.7.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range < 1.5 and the ET range > 8 GeV using the cone jet finding algorthm with cone radius = 0.7.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range 1.5 TO 2.2 and the ET range > 8 GeV using the cone jet finding algorthm with cone radius = 0.7.

The dependence of the jet shapes on the transverse jet energy ET in the pseudorapidity range > 2.2 and the ET range > 8 GeV using the cone jet finding algorthm with cone radius = 0.7.

The average number of subjets as a function of the resolution parameter YCUT using the inclusive KT jet finding algorithm in the pseudorapidity range < 1.5 and the ET range 5 TO 8 GeV YCUT using the inclusive KT jet finding algorithm.

The average number of subjets as a function of the resolution parameter YCUT using the inclusive KT jet finding algorithm in the pseudorapidity range 1.5 TO 2.2 and the ET range 5 TO 8 GeV YCUT using the inclusive KT jet finding algorithm.

The average number of subjets as a function of the resolution parameter YCUT using the inclusive KT jet finding algorithm in the pseudorapidity range > 2.2 and the ET range 5 TO 8 GeV YCUT using the inclusive KT jet finding algorithm.

The average number of subjets as a function of the resolution parameter YCUT using the inclusive KT jet finding algorithm in the pseudorapidity range < 1.5 and the ET range > 8 GeV YCUT using the inclusive KT jet finding algorithm.

The average number of subjets as a function of the resolution parameter YCUT using the inclusive KT jet finding algorithm in the pseudorapidity range 1.5 TO 2.2 and the ET range > 8 GeV YCUT using the inclusive KT jet finding algorithm.

The average number of subjets as a function of the resolution parameter YCUT using the inclusive KT jet finding algorithm in the pseudorapidity range > 2.2 and the ET range > 8 GeV YCUT using the inclusive KT jet finding algorithm.

The inclusive transverse energy flow at a mean X of 0.00057 and mean Q**2 of 4.2 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00016 and mean Q**2 of 6.3 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00027 and mean Q**2 of 7.0 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.0005 and mean Q**2 of 7.0 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00108 and mean Q**2 of 7.3 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00036 and mean Q**2 of 13.1 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00063 and mean Q**2 of 14.1 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00111 and mean Q**2 of 14.1 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00226 and mean Q**2 of 14.9 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00093 and mean Q**2 of 28.8 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00207 and mean Q**2 of 31.2 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00472 and mean Q**2 of 33.2 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00203 and mean Q**2 of 59.4 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.00704 and mean Q**2 of 70.2 GeV**2 for the low Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.0043 and mean Q**2 of 175. GeV**2 for the high Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.01 and mean Q**2 of 253. GeV**2 for the high Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.026 and mean Q**2 of 283. GeV**2 for the high Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.012 and mean Q**2 of 511. GeV**2 for the high Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.026 and mean Q**2 of 617. GeV**2 for the high Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.076 and mean Q**2 of 682. GeV**2 for the high Q**2 sample.

The inclusive transverse energy flow at a mean X of 0.11 and mean Q**2 of 2200. GeV**2 for the high Q**2 sample.

The inclusive transverse energy flow at a mean Q**2 of 3.5 GeV**2 at a mean W of 185 GeV for the low Q**2 sample.

The inclusive transverse energy flow at a mean Q**2 of 7 GeV**2 at a mean W of 185 GeV for the low Q**2 sample.

The inclusive transverse energy flow at a mean Q**2 of 14 GeV**2 at a mean W of 185 GeV for the low Q**2 sample.

The inclusive transverse energy flow at a mean Q**2 of 30 GeV**2 at a mean W of 185 GeV for the low Q**2 sample.

The inclusive transverse energy flow at a mean Q**2 of 61 GeV**2 at a mean W of 185 GeV for the low Q**2 sample.

The inclusive transverse energy flow at a mean Q**2 of 191 GeV**2 at a mean W of 185 GeV for the high Q**2 sample.

The inclusive transverse energy flow at a mean Q**2 of 294 GeV**2 at a mean W of 185 GeV for the high Q**2 sample.

The inclusive transverse energy flow at a mean Q**2 of 1103 GeV**2 at a mean W of 185 GeV for the high Q**2 sample.

Variation of the mean ET with Q**2 in the pseudorapidity bin -0.5 TO 0.5.

Variation of the mean ET with Q**2 in the pseudorapidity bin 2.0 TO 3.0.

Normalised distribution in M(P=4_5) for NC and CC dijet events. M(P=4_5) is the dijet mass.

Normalised distribution in ZP for NC and CC dijet events. ZP corresponds to 0.5*MIN(1-COS(THETA*)) summed over the two jets. THETA* is the polar angle of each parton in the c.m. system of the virtual boson and the incoming parton.

Normalised distribution in XP for NC and CC dijet events. XP is the ratio X/PSI where PSI is the fraction of the protons for momentacarried by the parton entering the hard scattering process.

Normalised distribution in ET(C=FOWARD) for NC and CC dijet events. ET(C=FORWARD) is the transverse energy of the most (non-remnant) forward jet.

Normalised distribution in THETA(C=FORWARD) for NC and CC dijet events. THETA(C=FORWARD) is the polar angle of the most (non-remnant) forward jet.

Normalised distribution in dijet mass for CC and NC events with Q**2 > 5000GeV**2.

Corrected mean values of the Jet Mass (RHO) distribution as a function of Q.

Corrected mean values of the C-Parameter (C-PARAM) distribution as a function of Q.

Corrected mean values of the Y21 distribution (using Factorisable Jade alogrithm) as a function of Q.

Corrected mean values of the Y21 distribution (using Durham kT alogrithm) as a function of Q.

Normalised (1-THRUST) distribution (w.r.t.current hemisphere axis).

Normalised (1-THRUST) distribution (w.r.t.current hemisphere axis).

Normalised (1-THRUST) distribution (w.r.t.current hemisphere axis).

Normalised (1-THRUST) distribution (w.r.t.current hemisphere axis).

Normalised (1-THRUST) distribution (w.r.t.current hemisphere axis).

Normalised (1-THRUST) distribution (w.r.t.current hemisphere axis).

Normalised (1-THRUST) distribution (w.r.t.current hemisphere axis).

Normalised (1-THRUST) distribution (w.r.t.current hemisphere axis).

Normalised Jet Broadening (B) distribution (w.r.t.current hemisphere axis).

Normalised Jet Broadening (B) distribution (w.r.t.current hemisphere axis).

Normalised Jet Broadening (B) distribution (w.r.t.current hemisphere axis).

Normalised Jet Broadening (B) distribution (w.r.t.current hemisphere axis).

Normalised Jet Broadening (B) distribution (w.r.t.current hemisphere axis).

Normalised Jet Broadening (B) distribution (w.r.t.current hemisphere axis).

Normalised Jet Broadening (B) distribution (w.r.t.current hemisphere axis).

Normalised Jet Broadening (B) distribution (w.r.t.current hemisphere axis).

Normalised (1-THRUST) distribution (w.r.t.max long. momentum axis).

Normalised (1-THRUST) distribution (w.r.t.max long. momentum axis).

Normalised (1-THRUST) distribution (w.r.t.max long. momentum axis).

Normalised (1-THRUST) distribution (w.r.t.max long. momentum axis).

Normalised (1-THRUST) distribution (w.r.t.max long. momentum axis).

Normalised (1-THRUST) distribution (w.r.t.max long. momentum axis).

Normalised (1-THRUST) distribution (w.r.t.max long. momentum axis).

Normalised (1-THRUST) distribution (w.r.t.max long. momentum axis).

Normalised Jet Mass (RHO) distribution.

Normalised Jet Mass (RHO) distribution.

Normalised Jet Mass (RHO) distribution.

Normalised Jet Mass (RHO) distribution.

Normalised Jet Mass (RHO) distribution.

Normalised Jet Mass (RHO) distribution.

Normalised Jet Mass (RHO) distribution.

Normalised Jet Mass (RHO) distribution.

Normalised C-Parameter(C-PARAM) distribution.

Normalised C-Parameter(C-PARAM) distribution.

Normalised C-Parameter(C-PARAM) distribution.

Normalised C-Parameter(C-PARAM) distribution.

Normalised C-Parameter(C-PARAM) distribution.

Normalised C-Parameter(C-PARAM) distribution.

Normalised C-Parameter(C-PARAM) distribution.

Normalised C-Parameter(C-PARAM) distribution.

Normalised Y21 distribution (using Factorisable Jade alogrithm).

Normalised Y21 distribution (using Factorisable Jade alogrithm).

Normalised Y21 distribution (using Factorisable Jade alogrithm).

Normalised Y21 distribution (using Factorisable Jade alogrithm).

Normalised Y21 distribution (using Factorisable Jade alogrithm).

Normalised Y21 distribution (using Factorisable Jade alogrithm).

Normalised Y21 distribution (using Factorisable Jade alogrithm).

Normalised Y21 distribution (using Factorisable Jade alogrithm).

Normalised Y21 distribution (using Durham kT alogrithm).

Normalised Y21 distribution (using Durham kT alogrithm).

Normalised Y21 distribution (using Durham kT alogrithm).

Normalised Y21 distribution (using Durham kT alogrithm).

Normalised Y21 distribution (using Durham kT alogrithm).

Normalised Y21 distribution (using Durham kT alogrithm).

Normalised Y21 distribution (using Durham kT alogrithm).

Normalised Y21 distribution (using Durham kT alogrithm).

The slope of the measured T distribution for elastic PHI meson production.

Full set of spin density matrix elements for elastic electroproduction of PHI mesons for W around 75 GeV.

The value of the combination of matrix elements 2*r^5_{11}+r^{5}_{00} for three Q**2 bins.

Ratio of the longitudinal to transverse cross sections for elastic PHI meson electroproduction.