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.

ASYMUU(COS(PHI(HADRON))) asymmetries for positive and negative hadrons as a function of XB. The errors are statistical and systematic.

ASYMUU(COS(PHI(HADRON))) asymmetries for positive and negative hadrons as a function of Z. The errors are statistical and systematic.

ASYMUU(COS(PHI(HADRON))) asymmetries for positive and negative hadrons as a function of PT(HADRON). The errors are statistical and systematic.

ASYMUU(COS(2*PHI(HADRON))) asymmetries for positive and negative hadrons as a function of XB. The errors are statistical and systematic.

ASYMUU(COS(2*PHI(HADRON))) asymmetries for positive and negative hadrons as a function of Z. The errors are statistical and systematic.

ASYMUU(COS(2*PHI(HADRON))) asymmetries for positive and negative hadrons as a function of PT(HADRON). The errors are statistical and systematic.

ASYMUU(COS(PHI(HADRON))) 3d asymmetries for positive and negative hadrons in the first XB bin. The errors are statistical and systematic.

ASYMUU(COS(PHI(HADRON))) 3d asymmetries for positive and negative hadrons in the second XB bin. The errors are statistical and systematic.

ASYMUU(COS(PHI(HADRON))) 3d asymmetries for positive and negative hadrons in the third XB bin. The errors are statistical and systematic.

ASYMUU(COS(PHI(HADRON))) 3d asymmetries for positive and negative hadrons in the last XB bin. The errors are statistical and systematic.

ASYMUU(COS(2*PHI(HADRON))) 3d asymmetries for positive and negative hadrons in the first XB bin. The errors are statistical and systematic.

ASYMUU(COS(2*PHI(HADRON))) 3d asymmetries for positive and negative hadrons in the second XB bin. The errors are statistical and systematic.

ASYMUU(COS(2*PHI(HADRON))) 3d asymmetries for positive and negative hadrons in the third XB bin. The errors are statistical and systematic.

ASYMUU(COS(2*PHI(HADRON))) 3d asymmetries for positive and negative hadrons in the last XB bin. The errors are statistical and systematic.

PT dependences of the differential multiplicities for 0.0080 < x_Bjorken < 0.0120 and 1.00 < Q^2 < 1.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0080 < x_Bjorken < 0.0120 and 1.50 < Q^2 < 2.10 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 1.00 < Q^2 < 1.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 1.50 < Q^2 < 2.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 2.50 < Q^2 < 3.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 1.00 < Q^2 < 1.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 1.50 < Q^2 < 2.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 2.50 < Q^2 < 3.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 3.50 < Q^2 < 5.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0350 and 1.00 < Q^2 < 1.20 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 1.20 < Q^2 < 1.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 1.50 < Q^2 < 2.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 2.50 < Q^2 < 3.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 3.50 < Q^2 < 6.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0500 and 1.50 < Q^2 < 2.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 2.50 < Q^2 < 3.50 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 3.50 < Q^2 < 6.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 6.00 < Q^2 < 10.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0700 < x_Bjorken < 0.1200 and 3.50 < Q^2 < 6.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0700 < x_Bjorken < 0.1200 and 6.00 < Q^2 < 10.00 GeV^2 for Positive hadrons.

PT dependences of the differential multiplicities for 0.0045 < x_Bjorken < 0.0060 and 1.00 < Q^2 < 1.25 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0060 < x_Bjorken < 0.0080 and 1.00 < Q^2 < 1.30 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0060 < x_Bjorken < 0.0080 and 1.30 < Q^2 < 1.70 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0080 < x_Bjorken < 0.0120 and 1.00 < Q^2 < 1.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0080 < x_Bjorken < 0.0120 and 1.50 < Q^2 < 2.10 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 1.00 < Q^2 < 1.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 1.50 < Q^2 < 2.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0120 < x_Bjorken < 0.0180 and 2.50 < Q^2 < 3.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 1.00 < Q^2 < 1.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 1.50 < Q^2 < 2.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 2.50 < Q^2 < 3.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0180 < x_Bjorken < 0.0250 and 3.50 < Q^2 < 5.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0350 and 1.00 < Q^2 < 1.20 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 1.20 < Q^2 < 1.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 1.50 < Q^2 < 2.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 2.50 < Q^2 < 3.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0250 < x_Bjorken < 0.0400 and 3.50 < Q^2 < 6.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0500 and 1.50 < Q^2 < 2.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 2.50 < Q^2 < 3.50 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 3.50 < Q^2 < 6.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0400 < x_Bjorken < 0.0700 and 6.00 < Q^2 < 10.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0700 < x_Bjorken < 0.1200 and 3.50 < Q^2 < 6.00 GeV^2 for Negative hadrons.

PT dependences of the differential multiplicities for 0.0700 < x_Bjorken < 0.1200 and 6.00 < Q^2 < 10.00 GeV^2 for Negative hadrons.

Fitted average PTs for positive hadrons.

Fitted average PTs for negative hadrons.

The measured transverse asymmetry from the deuteron target as a function of the variable X. Mean values are also given for the variables Q**2[GeV^2], Y, Z, M[GeV], M**2[GeV^2], SIN(THETA), COS(THETA), COS(THETA)**2 and the transverse spin transfer coefficient DNN.

The measured transverse asymmetry from the deuteron target as a function of the variable Z. Mean values are also given for the variables Q**2[GeV^2], Y, X, M[GeV], M**2[GeV^2], SIN(THETA), COS(THETA), COS(THETA)**2 and the transverse spin transfer coefficient DNN.

The measured transverse asymmetry from the deuteron target as a function of the variable M. Mean values are also given for the variables Q**2[GeV^2], Y, Z, X, M**2[GeV^2], SIN(THETA), COS(THETA), COS(THETA)**2 and the transverse spin transfer coefficient DNN Note that the data in the last bin (>1.5) does not contribute to the X and Z distributions.

The COLLINS asymmetry for negatively charged hadrons as a function of X.

The COLLINS asymmetry for negatively charged hadrons as a function of Z.

The COLLINS asymmetry for negatively charged hadrons as a function of PT.

The SIVERS asymmetry for positively charged hadrons as a function of X.

The SIVERS asymmetry for positively charged hadrons as a function of Z.

The SIVERS asymmetry for positively charged hadrons as a function of PT.

The SIVERS asymmetry for negatively charged hadrons as a function of X.

The SIVERS asymmetry for negatively charged hadrons as a function of Z.

The SIVERS asymmetry for negatively charged hadrons as a function of PT.

The COLLINS asymmetry for positively charged hadrons as a function of Z for X > 0.05.

The COLLINS asymmetry for positively charged hadrons as a function of PT for X > 0.05.

The COLLINS asymmetry for negatively charged hadrons as a function of Z for X > 0.05.

The COLLINS asymmetry for negatively charged hadrons as a function of PT for X > 0.05.

The SIVERS asymmetry for positively charged hadrons as a function of Z for X > 0.032.

The SIVERS asymmetry for positively charged hadrons as a function of PT for X > 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of Z for X > 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of PT for X > 0.032.

The COLLINS asymmetry for positively charged hadrons as a function of W for X > 0.032.

The COLLINS asymmetry for negatively charged hadrons as a function of W for X > 0.032.

The SIVERS asymmetry for positively charged hadrons as a function of W for X > 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of W for X > 0.032.

The COLLINS asymmetry for positively charged hadrons as a function of W for X < 0.032.

The COLLINS asymmetry for negatively charged hadrons as a function of W for X < 0.032.

The SIVERS asymmetry for positively charged hadrons as a function of W for X < 0.032.

The SIVERS asymmetry for negatively charged hadrons as a function of W for X < 0.032.

The COLLINS asymmetry for positively charged hadrons as a function of X for W > 7.5 GeV.

The COLLINS asymmetry for negatively charged hadrons as a function of X for W > 7.5 GeV.

The SIVERS asymmetry for positively charged hadrons as a function of X for W > 7.5 GeV.

The SIVERS asymmetry for negatively charged hadrons as a function of X for W > 7.5 GeV.

The COLLINS asymmetry for positively charged hadrons as a function of X for W < 7.5 GeV.

The COLLINS asymmetry for negatively charged hadrons as a function of X for W < 7.5 GeV.

The SIVERS asymmetry for positively charged hadrons as a function of X for W < 7.5 GeV.

The SIVERS asymmetry for negatively charged hadrons as a function of X for W < 7.5 GeV.

The measured strange quark helicity distribution as a funxtion of X.

The Collins and Sivers asymmetry as a function of X for 'ALL' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'ALL' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'ALL' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'ALL' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'ALL' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'ALL' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'ALL' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'ALL' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'ALL' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'ALL' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'ALL' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'ALL' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' positive pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' positivepions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' positive pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' negativepions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' negative pions from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' positivekaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' positive kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' negativekaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' negative kaons from the 2003-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of X for 'LEADING' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of PT for 'LEADING' neutral kaons from the 2002-2004 data.. Errors are statistical only.

The Collins and Sivers asymmetry as a function of Z for 'LEADING' neutral kaons from the 2002-2004 data.. Errors are statistical only.

Bin averaged differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON).

Bin averaged differential cross sections of diffractive di-jet production as a function centre of mass PT of the leading jet.

Bin averaged differential cross sections of diffractive di-jet production as a function of the pseudorapidity difference.

Bin averaged double differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON) in the (Q**2 + PT(LEADING JET)**2) range 29 to 50 GeV.

Bin averaged double differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON) in the (Q**2 + PT(LEADING JET)**2) range 50 to 70 GeV.

Bin averaged double differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON) in the (Q**2 + PT(LEADING JET)**2) range 70 to 100 GeV.

Bin averaged double differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON) in the (Q**2 + PT(LEADING JET)**2) range 100 to 200 GeV.