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.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted.

pi+ multiplicities from HERMES, Target: H, VM subtracted, Not VM subtracted.

pi- multiplicities from HERMES, Target: H, VM subtracted, Not VM subtracted.

K+ multiplicities from HERMES, Target: H, VM subtracted, Not VM subtracted.

K- multiplicities from HERMES, Target: H, VM subtracted, Not VM subtracted.

pi+ target asymmetries from HERMES, VM subtracted.

pi- target asymmetries from HERMES, VM subtracted.

K+ target asymmetries from HERMES, VM subtracted.

K- target asymmetries from HERMES, VM subtracted.

pi+ target asymmetries from HERMES, pi- target asymmetries from HERMES, VM subtracted, Z in the range 0.2-0.3.

pi+ target asymmetries from HERMES, pi- target asymmetries from HERMES, VM subtracted, Z in the range 0.3-0.4.

pi+ target asymmetries from HERMES, pi- target asymmetries from HERMES, VM subtracted, Z in the range 0.4-0.6.

pi+ target asymmetries from HERMES, pi- target asymmetries from HERMES, VM subtracted, Z in the range 0.6-0.8.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

pi+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

pi- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

K+ multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.2-0.3.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.3-0.4.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.4-0.6.

K- multiplicities from HERMES, Target: H, Target: D, VM subtracted, Z in the range 0.6-0.8.

Correlation matrix for $xg_2$ in 23 $x$-bins.

Multiplicity distributions measured in the current region of the Breit frame for the bin of 2*E(Breit,current region) = 12 to 20.

Multiplicity distributions measured in the current region of the Breit frame for the bin of 2*E(Breit,current region) = 20 to 30.

Multiplicity distributions measured in the current region of the Breit frame for the bin of 2*E(Breit,current region) = 30 to 45.

Multiplicity distributions measured in the current region of the Breit frame for the bin of 2*E(Breit,current region) = 45 to 100.

Multiplicity distributions measured in the current region of the Breit frame for the Meff bin 1.5 to 4.

Multiplicity distributions measured in the current region of the Breit frame for the Meff bin 4 to 8.

Multiplicity distributions measured in the current region of the Breit frame for the Meff bin 8 to 12.

Multiplicity distributions measured in the current region of the Breit frame for the Meff bin 12 to 20.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for W = 70 to 100 GeV.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for W = 100 to 150 GeV.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for W = 150 to 225 GeV.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 1.5 to 4.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 4 to 8.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 8 to 12.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 12 to 20.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 20 to 30.

Mean charged multiplicity measured in the Breit frame as a function of 2*E(Breit current region) with the assumptions of stable or decaying K0 and LAMBDA particles.

Mean charged multiplicity measured to the current fragmentation region of the HCM frame as a function of W with the assumptions of stable or decaying K0 and LAMBDA particles.

Mean charged multiplicity measured in the Breit frame as a function of Meff with the assumptions of stable or decaying K0 and LAMBDA particles.

Mean charged multiplicity measured in the current fragmentation region of the HCM frame as a function of Meff with the assumptions of stable or decaying K0 and LAMBDA particles.

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

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

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

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

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

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

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

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

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

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

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

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

PI+ multiplicty ratio (Helium/Deuterium) as a function of Z.

K+ multiplicty ratio (Helium/Deuterium) as a function of Z.

P multiplicty ratio (Helium/Deuterium) as a function of Z.

PI+ multiplicty ratio (Helium/Deuterium) as a function of Q**2.

K+ multiplicty ratio (Helium/Deuterium) as a function of Q**2.

P multiplicty ratio (Helium/Deuterium) as a function of Q**2.

PI+ multiplicty ratio (Neon/Deuterium) as a function of NU.

K+ multiplicty ratio (Neon/Deuterium) as a function of NU.

P multiplicty ratio (Neon/Deuterium) as a function of NU.

PI+ multiplicty ratio (Neon/Deuterium) as a function of Z.

K+ multiplicty ratio (Neon/Deuterium) as a function of Z.

P multiplicty ratio (Neon/Deuterium) as a function of Z.

PI+ multiplicty ratio (Neon/Deuterium) as a function of Q**2.

K+ multiplicty ratio (Neon/Deuterium) as a function of Q**2.

P multiplicty ratio (Neon/Deuterium) as a function of Q**2.

PI+ multiplicty ratio (Krypton/Deuterium) as a function of NU.

K+ multiplicty ratio (Krypton/Deuterium) as a function of NU.

P multiplicty ratio (Krypton/Deuterium) as a function of NU.

PI+ multiplicty ratio (Krypton/Deuterium) as a function of Z.

K+ multiplicty ratio (Krypton/Deuterium) as a function of Z.

P multiplicty ratio (Krypton/Deuterium) as a function of Z.

PI+ multiplicty ratio (Krypton/Deuterium) as a function of Q**2.

K+ multiplicty ratio (Krypton/Deuterium) as a function of Q**2.

P multiplicty ratio (Krypton/Deuterium) as a function of Q**2.

PI+ multiplicty ratio (Xenon/Deuterium) as a function of NU.

K+ multiplicty ratio (Xenon/Deuterium) as a function of NU.

P multiplicty ratio (Xenon/Deuterium) as a function of NU.

PI+ multiplicty ratio (Xenon/Deuterium) as a function of Z.

K+ multiplicty ratio (Xenon/Deuterium) as a function of Z.

P multiplicty ratio (Xenon/Deuterium) as a function of Z.

PI+ multiplicty ratio (Xenon/Deuterium) as a function of Q**2.

K+ multiplicty ratio (Xenon/Deuterium) as a function of Q**2.

P multiplicty ratio (Xenon/Deuterium) as a function of Q**2.

PI- multiplicity ratio (Helium/Deuterium) as a function of NU.

K- multiplicity ratio (Helium/Deuterium) as a function of NU.

PBAR multiplicity ratio (Helium/Deuterium) as a function of NU.

PI- multiplicity ratio (Helium/Deuterium) as a function of Z.

K- multiplicity ratio (Helium/Deuterium) as a function of Z.

PBAR multiplicity ratio (Helium/Deuterium) as a function of Z.

PI- multiplicity ratio (Helium/Deuterium) as a function of Q**2.

K- multiplicity ratio (Helium/Deuterium) as a function of Q**2.

PBAR multiplicity ratio (Helium/Deuterium) as a function of Q**2.

PI- multiplicity ratio (Neon/Deuterium) as a function of NU.

K- multiplicity ratio (Neon/Deuterium) as a function of NU.

PBAR multiplicity ratio (Neon/Deuterium) as a function of NU.

PI- multiplicity ratio (Neon/Deuterium) as a function of Z.

K- multiplicity ratio (Neon/Deuterium) as a function of Z.

PBAR multiplicity ratio (Neon/Deuterium) as a function of Z.

PI- multiplicity ratio (Neon/Deuterium) as a function of Q**2.

K- multiplicity ratio (Neon/Deuterium) as a function of Q**2.

PBAR multiplicity ratio (Neon/Deuterium) as a function of Q**2.

PI- multiplicity ratio (Krypton/Deuterium) as a function of NU.

K- multiplicity ratio (Krypton/Deuterium) as a function of NU.

PBAR multiplicity ratio (Krypton/Deuterium) as a function of NU.

PI- multiplicity ratio (Krypton/Deuterium) as a function of Z.

K- multiplicity ratio (Krypton/Deuterium) as a function of Z.

PBAR multiplicity ratio (Krypton/Deuterium) as a function of Z.

PI- multiplicity ratio (Krypton/Deuterium) as a function of Q**2.

K- multiplicity ratio (Krypton/Deuterium) as a function of Q**2.

PBAR multiplicity ratio (Krypton/Deuterium) as a function of Q**2.

PI- multiplicity ratio (Xenon/Deuterium) as a function of NU.

K- multiplicity ratio (Xenon/Deuterium) as a function of NU.

PBAR multiplicity ratio (Xenon/Deuterium) as a function of NU.

PI- multiplicity ratio (Xenon/Deuterium) as a function of Z.

K- multiplicity ratio (Xenon/Deuterium) as a function of Z.

PBAR multiplicity ratio (Xenon/Deuterium) as a function of Z.

PI- multiplicity ratio (Xenon/Deuterium) as a function of Q**2.

K- multiplicity ratio (Xenon/Deuterium) as a function of Q**2.

PBAR multiplicity ratio (Xenon/Deuterium) as a function of Q**2.

PI+ multiplicity ratio (Helium/Deuterium) as a function of PT**2.

K+ multiplicity ratio (Helium/Deuterium) as a function of PT**2.

P multiplicity ratio (Helium/Deuterium) as a function of PT**2.

PI- multiplicity ratio (Helium/Deuterium) as a function of PT**2.

K- multiplicity ratio (Helium/Deuterium) as a function of PT**2.

PBAR multiplicity ratio (Helium/Deuterium) as a function of PT**2.

PI+ multiplicity ratio (Neon/Deuterium) as a function of PT**2.

K+ multiplicity ratio (Neon/Deuterium) as a function of PT**2.

P multiplicity ratio (Neon/Deuterium) as a function of PT**2.

PI- multiplicity ratio (Neon/Deuterium) as a function of PT**2.

K- multiplicity ratio (Neon/Deuterium) as a function of PT**2.

PBAR multiplicity ratio (Neon/Deuterium) as a function of PT**2.

PI+ multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

K+ multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

P multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

PI- multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

K- multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

PBAR multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

PI+ multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

K+ multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

P multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

PI- multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

K- multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

PBAR multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

PI0 multiplicity ratio (Helium/Deuterium) as a function of NU.

PI0 multiplicity ratio (Helium/Deuterium) as a function of Z.

PI0 multiplicity ratio (Helium/Deuterium) as a function of Q**2.

PI0 multiplicity ratio (Helium/Deuterium) as a function of PT**2.

PI0 multiplicity ratio (Neon/Deuterium) as a function of NU.

PI0 multiplicity ratio (Neon/Deuterium) as a function of Z.

PI0 multiplicity ratio (Neon/Deuterium) as a function of Q**2.

PI0 multiplicity ratio (Neon/Deuterium) as a function of PT**2.

PI0 multiplicity ratio (Krypton/Deuterium) as a function of NU.

PI0 multiplicity ratio (Krypton/Deuterium) as a function of Z.

PI0 multiplicity ratio (Krypton/Deuterium) as a function of Q**2.

PI0 multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

PI0 multiplicity ratio (Xenon/Deuterium) as a function of NU.

PI0 multiplicity ratio (Xenon/Deuterium) as a function of Z.

PI0 multiplicity ratio (Xenon/Deuterium) as a function of Q**2.

PI0 multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for Z > 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for Z > 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of PT**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of PT**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of PT**2 for Z > 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for Z > 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for Z > 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of PT**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of PT**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of PT**2 for Z > 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for Z > 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for Z > 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of PT**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of PT**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of PT**2 for Z > 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for Z > 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for Z > 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of PT**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of PT**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of PT**2 for Z > 0.7.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Z for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Z for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Z for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Q**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Q**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Q**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of PT**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of PT**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of PT**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Z for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Z for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Z for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Q**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Q**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Q**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of PT**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of PT**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of PT**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Z for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Z for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Z for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Q**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Q**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Q**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of PT**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of PT**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of PT**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Z for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Z for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Z for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Q**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Q**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Q**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of PT**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of PT**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of PT**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Z for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Z for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Z for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Z for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Z for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Z for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Z for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Z for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 20 TO 23.5 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 17 TO 20 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 14 TO 17 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 11 TO 14 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 6 TO 11 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 20 TO 23.5 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 17 TO 20 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 14 TO 17 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 11 TO 14 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 6 TO 11 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 20 TO 23.5 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 17 TO 20 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 14 TO 17 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 11 TO 14 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 6 TO 11 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 20 TO 23.5 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 17 TO 20 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 14 TO 17 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 11 TO 14 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 6 TO 11 GeV.

Beam SSA as a function of Z, X, hadronic PT and Q**2 corrected for the decay of exclusively produced VMs with the DSYS error due to the uncertainty in the VM subtraction.

Beam SSA as a function of Z, X, hadronic PT and Q**2 corrected for the decay of exclusively produced VMs with the DSYS error due to the uncertainty in the VM subtraction.

Beam SSA as a function of Z, X, hadronic PT and Q**2 corrected for the decay of exclusively produced VMs with the DSYS error due to the uncertainty in the VM subtraction.

Integrals of G1 over different X ranges for DEUT target at various Q*2 values. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).. The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2. Axis error includes +- 5.0/5.0 contribution.

Integrals of G1 over different X ranges for N target at various Q*2 values. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).. The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Integral of G1 for the Non-Singet contribution. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).. The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2. Axis error includes +- 5.2/5.2 contribution.

The measured and Born asymmetries for the proton target at the average values of the average values of X, Y,and Q**2 in 45 bins. DSYS includes the 5.2 PCT normalization uncertainty.

The measured and Born asymmetries for the deuterium target at the average values of the average values of X, Y,and Q**2 in 45 bins. DSYS includes the 5 PCT normalization uncertainty.

Virtual photon asymmetries A1 for the proton and deuterium targets at the average values of X,and Q**2 in 45 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).

Structure functions G1 for the proton and deuterium targets at the average values of X,and Q**2 in 45 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).

Virtual photon asymmetries A1 for the proton and deuterium targets at the average values of X,and Q**2 in 19 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Structure functions G1 for the proton and deuterium targets at the average values of X,and Q**2 in 19 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Structure functions G1 for the proton and deuterium targets at the average values of X,and Q**2 in 15 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Virtual photon asymmetries A1 for the proton and deuterium targets at the average values of X,and Q**2 in 15 bins. The first DSYS is the experimental uncertainty and includes the 5.2 (5.0) PCT normalization uncertainty for the proton (deuteron) data. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Structure functions G1(n) and G1(NS)for the proton and deuterium targets at the average values of X,and Q**2 in 45 bins. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD).

Structure functions G1(n) and G1(NS)for the proton and deuterium targets at the average values of X,and Q**2 in 19 bins. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Structure functions G1(n) and G1(NS)for the proton and deuterium targets at the average values of X,and Q**2 in 15 bins. The second DSYS systematic error is due to the uncertainty in the parameterizations (R, F2, A2, Azz, omegaD). The third DSYS systematic error is due to the uncertainty in evolving to a common Q**2.

Correlation matrix for the Asymmetry, A1 and G1 for the P target at the average values of X and Q**2 in 45 bins.

Correlation matrix for the Asymmetry, A1 and G1 for the DEUT target at the average values of X and Q**2 in 45 bins.

Correlation matrix for G1 for the P target in 19 X bins (averaged over Q**2).

Correlation matrix for G1 for the DEUT target in 19 X bins (averaged over Q**2).

Correlation matrix for G1 for the P target in 15 X bins (Q**2 > 1 GeV**2), averaged over Q**2.

Correlation matrix for G1 for the DEUT target in 15 X bins (Q**2 > 1 GeV**2), averaged over Q**2.

The photoabsorption asymmetry A1 for electroproduction of PHI mesons by quasi-real photons.

The photoabsorption asymmetry A1 for exclusive RHO0 production as a function of X.

The photoabsorption asymmetry A1 for exclusive RHO0 production as a function of Q**2.

The photoabsorption asymmetry A1 for exclusive RHO0 production as a function of TP.