Detector response matrix (PROB) for the acoplanarity variable (ACO) for mu+ mu- channel (empty bins are not reported).

Acoplanarity (ACO) distributions unfolded for detector resolution, and lepton pair trigger, reconstruction and identification efficiencies for e+ e- channel (empty bins are not reported).

Acoplanarity (ACO) distributions unfolded for detector resolution, and lepton pair trigger, reconstruction and identification efficiencies for mu+ mu- channel (empty bins are not reported).

The lepton pair exclusive selection efficiency in the fiducial region for signal MC events as a function of M and Y for e+ e- channel.

The lepton pair exclusive selection efficiency in the fiducial region for signal MC events as a function of M and Y for mu+ mu- channel.

The lepton pair exclusive selection efficiency in the fiducial region for single-dissociative MC events as a function of M and Y for e+ e- channel.

The lepton pair exclusive selection efficiency in the fiducial region for single-dissociative MC events as a function of M and Y for mu+ mu- channel.

The expected invariant mass distribution of signal Z'@0.75TeV and $\tilde{\nu}_{\tau}$@1TeV. The arbitrary choice of couplings are: $\lambda_{311}^{'}=0.11$ and $\lambda_{i3k}=0.07$ for $\tilde{\nu}_{\tau}$, $Q_{ll^{'}}=1$ for Z' .

Observed and predicted $\mu\tau$ invariant mass distributions.

The expected invariant mass distribution of signal Z'@0.75TeV and $\tilde{\nu}_{\tau}$@1TeV. The arbitrary choice of couplings are: $\lambda_{311}^{'}=0.11$ and $\lambda_{i3k}=0.07$ for $\tilde{\nu}_{\tau}$, $Q_{ll^{'}}=1$ for Z' .

Expected cross section times branching ratio as a function of $\tilde{\nu}_{\tau}$ mass in the $e\mu$ channel for the arbitrary choice of couplings $\lambda_{311}^{'}=0.11$ and $\lambda_{i3k}=0.07$.

The 95% CL limits on cross section times branching ratio as a function of $\tilde{\nu}_{\tau}$ mass in the $e\mu$ channel.

Expected cross section times branching ratio as a function of Z' mass in the $e\mu$ channel for the arbitrary choice of couplings $Q_{ll^{'}}=1$.

The 95% CL limits on cross section times branching ratio as a function of Z' mass in the $e\mu$ channel.

The 95% CL limits on cross section times branching ratio as a function of $\tilde{\nu}_{\tau}$ mass in the $e\tau$ channel.

The 95% CL limits on cross section times branching ratio as a function of Z' mass in the $e\tau$ channel.

The 95% CL limits on cross section times branching ratio as a function of $\tilde{\nu}_{\tau}$ mass in the $\mu\tau$ channel.

The 95% CL limits on cross section times branching ratio as a function of Z' mass in the $\mu\tau$ channel.

The 95% CL limits on lambda'_311 as a function of sneutrino mass for assumed value of lambda_i3k=0.07 for $e\mu$, $e\tau$ and $\mu\tau$ modes.

Estimated SM backgrounds and observed event yields for the validation and search region.

Cut flow for signal $\tilde{\nu}_{\tau}$ and Z' at 1TeV mass point.

Gaussian standard deviation of M(ll') distributions at various signal mass.

Inputs used for the Z'-->$e\mu$ channel limit setting.

Inputs used for the $\tilde{\nu}_{\tau}$-->$e\mu$ channel limit setting.

Inputs used for the Z'-->$e\tau$ channel limit setting.

Inputs used for the $\tilde{\nu}_{\tau}$ -->$e\tau$ channel limit setting.

Inputs used for the Z'-->$\mu\tau$ channel limit setting.

Inputs used for the $\tilde{\nu}_{\tau}$-->$\mu\tau$ channel limit setting.

Measured jet multiplicity distribution in the $W\mu\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured dilepton invariant mass distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured $E_{T}^{miss}$ distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured leading jet $p_{T}$ distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured jet multiplicity distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured transverse mass distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured $E_{T}^{miss}$ distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured leading jet $p_{T}$ distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured jet multiplicity distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured dilepton invariant mass distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured $E_{T}^{miss}$ distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured leading jet $p_{T}$ distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured jet multiplicity distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured distribution of the jet multiplicity for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of $E_{T}^{miss}$ for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of leading jet $p_{T}$ for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_{T}$ to $E_{T}^{miss}$ ratio for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the jet multiplicity for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the jet multiplicity for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ for SR9 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ to $E_{T}^{miss}$ ratio for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ to $E_{T}^{miss}$ ratio for SR9 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Observed and expected 95$\%$ CL limit on the fundamental Planck scale in $4+n$ dimensions, $M_D$, as a function of the number of extra dimensions. In the figure the two results overlap. The shaded areas around the expected limit indicate the expected $\pm 1\sigma$ and $\pm 2\sigma$ ranges of limits in the absence of a signal. The 95$\%$ CL observed limits after the suppression of the events with $\hat{s} > M_D^2$ is applied (truncated) are also given.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the scalar operator D1. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the vector operator D5. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the axial vector operator D8. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the tensor operator D9. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the gluon operator D11. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the gluon operator C5. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Observed 95% CL limits on the suppression scale M* as a function of the mediator mass Mmed, assuming a Z'-like boson in a simplified model and a DM mass of 50 GeV and 400 GeV. The width of the mediator is varied between Mmed/3 and Mmed/8pi.

Observed 95% CL upper limits on the product of couplings of the simplified model vertex in the plane of mediator and WIMP mass (Mmed versus m_chi).

Upper limits at 90% C.L. on the WIMP-nucleon scattering cross section as a function of m_chi for spin-independent interactions, for a coupling strength of unity or the maximum value that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

Upper limits at 90% C.L. on the WIMP-nucleon scattering cross section as a function of m_chi for spin-dependent interactions, for a coupling strength of unity or the maximum value that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

Upper limits at 90% C.L. on the WIMP-nucleon annihilation cross section as a function of m_chi, for a coupling strength of unity or the maximum value that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for degenerate squark/gluino masses.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 1/2 \times m_{\tilde{q}}$.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 1/4 \times m_{\tilde{q}}$.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 2 \times m_{\tilde{q}}$.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 4 \times m_{\tilde{q}}$.

Observed and expected 95$\%$ CL upper limit on $\sigma \times {\rm{BR}}(H \to {\rm{invisible}})$ as a function of the Higgs boson mass.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the scalar operator C1. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Lower limits at 95% CL on the mass of $H_{\mathrm{L}}^{\pm \pm}$ and $H_{\mathrm{R}}^{\pm \pm}$ bosons, assuming a 100% branching ratio to $e^{\pm}e^{\pm}$, $e^{\pm}/\mu^{\pm}$ and $\mu^{\pm}\mu^{\pm}$ pairs. The $1\sigma$ variations are also shown for the expected limits.

The fiducial efficiency for electrons and taus in different $\eta$ ranges ($\epsilon_{\mathrm{fid}}(\eta)$). For electrons from tau decays, the $\eta$ is that of the electron, not the tau. The uncertainties shown reflect the statistical uncertainties of the simulated samples only. UPDATE (18 MAY 2015): Updated fiducial lepton efficiencies.

Expected and observed event yields for the $H_{\mathrm{T}}^{\mathrm{leptons}}$ signal regions.

Expected and observed event yields for the minimum $p_{\mathrm{T}}^{\ell}$ signal regions.

Expected and observed event yields for the $b$-tag signal regions.

Expected and observed event yields for the inclusive $m_{\mathrm{eff}}$ signal regions.

Expected and observed event yields for the high-$E_{\mathrm{T}}^{\mathrm{miss}}$, $m_{\mathrm{eff}}$ signal regions.

Expected and observed event yields for the high-$m_{\mathrm{T}}^{W}$, $m_{\mathrm{eff}}$ signal regions.

Expected and observed event yields for the high-$H_{\mathrm{T}}^{\mathrm{jets}}$, $E_{\mathrm{T}}^{\mathrm{miss}}$ signal regions.

Expected and observed event yields for the low-$H_{\mathrm{T}}^{\mathrm{jets}}$, $E_{\mathrm{T}}^{\mathrm{miss}}$ signal regions.

Expected and observed limits, and corresponding $p$-values and significances (in standard deviations), for signal regions based on cuts on $H_{\mathrm{T}}^{\mathrm{leptons}}$.

Expected and observed limits, and corresponding $p$-values and significances (in standard deviations), for signal regions based on cuts on $p_{\mathrm{T}}^{\ell\mathrm{,min}}$.

Expected and observed limits, and corresponding $p$-values and significances (in standard deviations), for signal regions based on cuts on the number of $b$-tagged jets.

Expected and observed limits, and corresponding $p$-values and significances (in standard deviations), for signal regions based on cuts on $m_{\mathrm{eff}}$.

Expected and observed limits, and corresponding $p$-values and significances (in standard deviations), for signal regions based on cuts on $m_{\mathrm{eff}}$ [GeV]. All these signal regions have an additional requirement of $E_{\mathrm{T}}^{\mathrm{miss}}\geq 100$ GeV.

Expected and observed limits, and corresponding $p$-values and significances (in standard deviations), for signal regions based on cuts on $m_{\mathrm{eff}}$ [GeV]. All these signal regions have an additional requirement of $m_{\mathrm{T}}^{W}\geq 100$ GeV.

Expected and observed limits, and corresponding $p$-values and significances (in standard deviations), for signal regions based on cuts on $E_{\mathrm{T}}^{\mathrm{miss}}$. All these signal regions have an additional requirement of $H_{\mathrm{T}}^{\mathrm{jets}}\geq 150$ GeV.

Expected and observed limits, and corresponding $p$-values and significances (in standard deviations), for signal regions based on cuts on $E_{\mathrm{T}}^{\mathrm{miss}}$. All these signal regions have an additional requirement of $H_{\mathrm{T}}^{\mathrm{jets}} < 150$ GeV.

Trans.min. scalar pT sum density vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum density vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity density vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity density vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Away charged multiplicity density vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity density vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 0 - 5 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 5 - 10 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 10 - 20 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 20 - 50 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 50 - 110 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 110 - 500 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity density vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 0 - 5 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 5 - 10 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 10 - 20 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 20 - 50 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 50 - 110 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 110 - 500 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 0 - 5 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 5 - 10 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 10 - 20 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 20 - 50 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 50 - 110 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 110 - 500 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 0 - 5 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 5 - 10 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 10 - 20 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 20 - 50 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 50 - 110 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 110 - 500 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 0 - 5 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 5 - 10 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 10 - 20 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 20 - 50 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 50 - 110 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 110 - 500 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 0 - 5 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 5 - 10 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 10 - 20 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 20 - 50 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 50 - 110 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 110 - 500 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards <mean pT(charged)> vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse <mean pT(charged)> vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Away <mean pT(charged)> vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Towards <mean pT(charged)> vs charged multiplicity, Born leptons : Statistical and systematic errors are added in quadrature.

Transverse <mean pT(charged)> vs charged multiplicity, Born leptons : Statistical and systematic errors are added in quadrature.

Away <mean pT(charged)> vs charged multiplicity, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 0 - 5 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 5 - 10 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 10 - 20 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 20 - 50 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 50 - 110 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 110 - 500 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.diff. scalar pT sum density vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.diff. charged multiplicity density vs Z-boson pT, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 0 - 5 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 5 - 10 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 10 - 20 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 20 - 50 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 50 - 110 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 110 - 500 GeV, Born leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Away scalar pT sum density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Away charged multiplicity density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 0 - 5 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 5 - 10 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 10 - 20 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 20 - 50 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 50 - 110 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards scalar pT sum distribution, Z-boson pT = 110 - 500 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 0 - 5 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 5 - 10 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 10 - 20 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 20 - 50 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 50 - 110 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards charged multiplicity distribution, Z-boson pT = 110 - 500 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 0 - 5 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 5 - 10 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 10 - 20 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 20 - 50 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 50 - 110 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse charged multiplicity distribution, Z-boson pT = 110 - 500 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 0 - 5 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 5 - 10 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 10 - 20 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 20 - 50 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 50 - 110 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. charged multiplicity distribution, Z-boson pT = 110 - 500 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 0 - 5 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 5 - 10 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 10 - 20 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 20 - 50 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 50 - 110 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. charged multiplicity distribution, Z-boson pT = 110 - 500 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 0 - 5 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 5 - 10 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 10 - 20 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 20 - 50 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 50 - 110 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse scalar pT sum distribution, Z-boson pT = 110 - 500 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards <mean pT(charged)> vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse <mean pT(charged)> vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Away <mean pT(charged)> vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Towards <mean pT(charged)> vs charged multiplicity, dressed leptons : Statistical and systematic errors are added in quadrature.

Transverse <mean pT(charged)> vs charged multiplicity, dressed leptons : Statistical and systematic errors are added in quadrature.

Away <mean pT(charged)> vs charged multiplicity, dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 0 - 5 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 5 - 10 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 10 - 20 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 20 - 50 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 50 - 110 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.min. scalar pT sum distribution, Z-boson pT = 110 - 500 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.diff. scalar pT sum density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.diff. charged multiplicity density vs Z-boson pT, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 0 - 5 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 5 - 10 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 10 - 20 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 20 - 50 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 50 - 110 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Trans.max. scalar pT sum distribution, Z-boson pT = 110 - 500 GeV, Dressed leptons : Statistical and systematic errors are added in quadrature.

Reconstructed $\cos\theta^*$ distributions for data and the SM background estimate in the dimuon channel.

Reconstructed $A_{\rm FB}$ distributions for data and the SM background estimate as a function of dielectron mass.

Reconstructed $A_{\rm FB}$ distributions for data and the SM background estimate as a function of dimuon mass.

Summary of 95% C.L. lower exclusion limits on $\Lambda$ for the combined dilepton contact interaction search, using a uniform positive prior in 1/$\Lambda^2$.

Summary of 95% C.L. lower exclusion limits on $M_{\rm S}$ for the combined dilepton ADD large extra dimensions search, using a uniform positive prior in 1/$M_{\rm S}^8$.

Reconstructed $\cos\theta^*$ distributions for data and the SM background estimate in the electron channel.

Reconstructed $\cos\theta^*$ distributions for data and the SM background estimate in the muon channel.

Distribution of HT after the MTtau requirement for the 1-tau ''Tight'' SR. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in the CRs corresponding to MTtau below 130 GeV. Also shown is the expected signal from typical mSUGRA, GMSB and bRPV samples. The last bin in the expected background distribution is an overflow bin.

Distribution of MTtau1 + MTtau2 in the 2tau channel after all analysis requirements but the final SR requirements on MTtau1 + MTtau2 and HT2j. To reduce the contributions from events with Z bosons decaying into tau leptons, the requirement MTtau1 + MTtau2 > 150 GeV is applied to all distributions. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in the CRs corresponding to HT2j below 550 GeV.

Distribution of HT2j in the 2tau channel after all analysis requirements but the final SR requirements on MTtau1 + MTtau2 and HT2j. To reduce the contributions from events with Z bosons decaying into tau leptons, the requirement MTtau1 + MTtau2 > 150 GeV is applied to all distributions. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in the CRs corresponding to HT2j below 550 GeV.

Distribution of the jet multiplicity in the 2tau channel after all analysis requirements but the final SR requirements on MTtau1 + MTtau2 and HT2j. To reduce the contributions from events with Z bosons decaying into tau leptons, the requirement MTtau1 + MTtau2 > 150 GeV is applied to all distributions. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in the CRs corresponding to HT2j below 550 GeV.

Distribution of the final kinematic variables in the tau+e channel after all analysis requirements but the final SR selections on Meff for the bRPV model. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in specific CRs. The last bin in the expected background distribution is an overflow bin. There are no data events in the overflow bin after all analysis requirements are applied.

Distribution of the final kinematic variables in the tau+e channel after all analysis requirements but the final SR selections on MEFF for the GMSB model. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in specific CRs. The last bin in the expected background distribution is an overflow bin. There are no data events in the overflow bin after all analysis requirements are applied.

Distribution of the final kinematic variables in the tau+e channel after all analysis requirements but the final SR selections on MET for the mSUGRA model. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in specific CRs. The last bin in the expected background distribution is an overflow bin. There are no data events in the overflow bin after all analysis requirements are applied.

Distribution of the final kinematic variables in the tau+e channel after all analysis requirements but the final SR selections on MET for the nGM model. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in specific CRs. The last bin in the expected background distribution is an overflow bin. There are no data events in the overflow bin after all analysis requirements are applied.

Distribution of the final kinematic variables in the tau+mu channel after all analysis requirements but the final SR selections on MEFF for the bRPV model. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in specific CRs. The last bin in the expected background distribution is an overflow bin. There are no data events in the overflow bin after all analysis requirements are applied.

Distribution of the final kinematic variables in the tau+mu channel after all analysis requirements but the final SR selections on MEFF for the GMSB model. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in specific CRs. The last bin in the expected background distribution is an overflow bin. There are no data events in the overflow bin after all analysis requirements are applied.

Distribution of the final kinematic variables in the tau+mu channel after all analysis requirements but the final SR selections on MET for the mSUGRA model. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in specific CRs. The last bin in the expected background distribution is an overflow bin. There are no data events in the overflow bin after all analysis requirements are applied.

Distribution of the final kinematic variables in the tau+mu channel after all analysis requirements but the final SR selections on MET for the nGM model. The SM prediction includes the data-driven corrections discussed in the paper. MC events are normalized to data in specific CRs. The last bin in the expected background distribution is an overflow bin. There are no data events in the overflow bin after all analysis requirements are applied.

Observed 95% CL lower limits on the minimal GMSB model parameters Lambda and tan(beta) using a combination of all channels. The result is obtained using 20.3 fb-1 of sqrt(s) = 8 TeV ATLAS data. Additional model parameters are M(mess) = 250 TeV, N5 = 3, mu>0 and Cgrav =1.

Expected 95% CL lower limits on the minimal GMSB model parameters Lambda and tan(beta) using a combination of all channels. The result is obtained using 20.3 fb-1 of sqrt(s) = 8 TeV ATLAS data. Additional model parameters are M(mess) = 250 TeV, N5 = 3, mu>0 and Cgrav =1.

Observed 95% CL lower limits on the mSUGRA/CMSSM model parameters m0 and m1/2 for the combination of the 1tau, tau+e and tau+mu channels. Additional model parameters are A0 = -2m0, tan(beta) = 30 and sign(mu) = +1.

Expected 95% CL lower limits on the mSUGRA/CMSSM model parameters m0 and m1/2 for the combination of the 1tau, tau+e and tau+mu channels. Additional model parameters are A0 = -2m0, tan(beta) = 30 and sign(mu) = +1.

Observed 95% CL lower limits on the simplified nGM model parameters m(stau) and m(gluino) for the combination of the 2tau, tau+e and tau+mu channels. Additional squark and slepton mass parameters are set to 2.5 TeV, M1 = M2 = 2.5 TeV, and all trilinear coupling terms are set to zero. Also, the parameter mu is fixed to mu = 400 GeV.

Expected 95% CL lower limits on the simplified nGM model parameters m(stau) and m(gluino) for the combination of the 2tau, tau+e and tau+mu channels. Additional squark and slepton mass parameters are set to 2.5 TeV, M1 = M2 = 2.5 TeV, and all trilinear coupling terms are set to zero. Also, the parameter mu is fixed to mu = 400 GeV.

Observed 95% CL lower limits on the bRPV model parameters m0 and m1/2 for the combination of all channels. Additional model parameters are A0 = -2m0 , tan(beta) = 30 and sign(mu) = +1.

Expected 95% CL lower limits on the bRPV model parameters m0 and m1/2 for the combination of all channels. Additional model parameters are A0 = -2m0 , tan(beta) = 30 and sign(mu) = +1.

Cross section predictions for the nGM grid. For each signal point 25000 MC events have been generated.

Observed upper cross section limits for the nGM grid. For each signal point 25000 MC events have been generated. The limit is derived for the combination of the 2tau and the tau+lepton channels.

Systematic uncertainty for the GMSB grid in the 1-tau analysis.

Acceptance for the GMSB grid in the 1-tau analysis.

Efficiency for the GMSB grid in the 1-tau analysis.

The product of acceptance and efficiency for the GMSB grid in the 1-tau analysis.

Expected CLs values for the GMSB grid in the 1tau analysis.

Observed CLs values for the GMSB grid in the 1tau analysis.

Systematic uncertainty for the mSUGRA grid in the 1-tau analysis.

Acceptance for the mSUGRA grid in the 1-tau analysis.

Efficiency for the mSUGRA grid in the 1-tau analysis.

Product of acceptance and efficiency for the mSUGRA grid in the 1-tau analysis.

Expected CLs values for the mSUGRA grid in the 1tau analysis.

Observed CLs values for the mSUGRA grid in the 1tau analysis.

Systematic uncertainty for the bRPV grid in the 1-tau analysis.

Acceptance for the bRPV grid in the 1-tau analysis.

Efficiency for the bRPV grid in the 1-tau analysis.

Product of acceptance and efficiency for the bRPV grid in the 1-tau analysis.

Expected CLs values for the bRPV grid in the 1tau analysis.

Observed CLs values for the bRPV grid in the 1tau analysis.

Systematic uncertainty for the GMSB grid in the 2tau analysis.

Acceptance for the GMSB grid in the 2tau analysis.

Efficiency for the GMSB grid in the 2tau analysis.

Product of acceptance and efficiency for the GMSB grid in the 2tau analysis.

Expected CLs values for the GMSB grid in the 2tau analysis.

Observed CLs values for the GMSB grid in the 2tau analysis.

Systematic uncertainty for the nGM grid in the 2tau analysis.

Acceptance for the nGM grid in the 2tau analysis.

Efficiency for the nGM grid in the 2tau analysis.

Product of acceptance and efficiency for the nGM grid in the 2tau analysis.

Expected CLs values for the nGM grid in the 2tau analysis.

Observed CLs values for the nGM grid in the 2tau analysis.

Systematic uncertainty for the bRPV grid in the 2tau analysis.

Acceptance for the bRPV grid in the 2tau analysis.

Efficiency for the bRPV grid in the 2tau analysis.

Product of acceptance and efficiency for the bRPV grid in the 2tau analysis.

Expected CLs values for the bRPV grid in the 2tau analysis.

Observed CLs values for the bRPV grid in the 2tau analysis.

Systematic Uncertainty for the GMSB grid in the tau+e analysis.

Acceptance for the GMSB grid in the tau+e analysis.

Efficiency for the GMSB grid in the tau+e analysis.

Product of acceptance and efficiency for the GMSB grid in the tau+e analysis.

Expected CLs values for the GMSB grid in the tau+e analysis.

Observed CLs values for the GMSB grid in the tau+e analysis.

Systematic Uncertainty for the nGM grid in the tau+e analysis.

Acceptance for the nGM grid in the tau+e analysis.

Efficiency for the nGM grid in the tau+e analysis.

Product of acceptance and efficiency for the nGM grid in the tau+e analysis.

Expected CLs values for the nGM grid in the tau+e analysis.

Observed CLs values for the nGM grid in the tau+e analysis.

Systematic Uncertainty for the bRPV grid in the tau+e analysis.

Acceptance for the bRPV grid in the tau+e analysis.

Efficiency for the bRPV grid in the tau+e analysis.

Product of acceptance and efficiency for the bRPV grid in the tau+e analysis.

Expected CLs values for the bRPV grid in the tau+e analysis.

Observed CLs values for the bRPV grid in the tau+e analysis.

Systematic Uncertainty for the mSUGRA grid in the tau+e analysis.

Acceptance for the mSUGRA grid in the tau+e analysis.

Efficiency for the mSUGRA grid in the tau+e analysis.

Product of acceptance and efficiency for the mSUGRA grid in the tau+e analysis.

Expected CLs values for the mSUGRA grid in the tau+e analysis.

Observed CLs values for the mSUGRA grid in the tau+e analysis.

Systematic Uncertainty for the GMSB grid in the tau+mu analysis.

Acceptance for the GMSB grid in the tau+mu analysis.

Efficiency for the GMSB grid in the tau+mu analysis.

Product of acceptance and efficiency for the GMSB grid in the tau+mu analysis.

Expected CLs values for the GMSB grid in the tau+mu analysis.

Observed CLs values for the GMSB grid in the tau+mu analysis.

Systematic Uncertainty for the nGM grid in the tau+mu analysis.

Acceptance for the nGM grid in the tau+mu analysis.

Efficiency for the nGM grid in the tau+mu analysis.

Product of acceptance and efficiency for the nGM grid in the tau+mu analysis.

Expected CLs values for the nGM grid in the tau+mu analysis.

Observed CLs values for the nGM grid in the tau+mu analysis.

Systematic Uncertainty for the bRPV grid in the tau+mu analysis.

Acceptance for the bRPV grid in the tau+mu analysis.

Efficiency for the bRPV grid in the tau+mu analysis.

Product of acceptance and efficiency for the bRPV grid in the tau+mu analysis.

Expected CLs values for the bRPV grid in the tau+mu analysis.

Observed CLs values for the bRPV grid in the tau+mu analysis.

Systematic Uncertainty for the mSUGRA grid in the tau+mu analysis.

Acceptance for the mSUGRA grid in the tau+mu analysis.

Efficiency for the mSUGRA grid in the tau+mu analysis.

Product of acceptance and efficiency for the mSUGRA grid in the tau+mu analysis.

Expected CLs values for the mSUGRA grid in the tau+mu analysis.

Observed CLs values for the mSUGRA grid in the tau+mu analysis.

Example cutflow for three benchmark signal points in the 1-tau channel. For the GMSB point 50000 events have been generated, 20000 for nGM and 20000 for mSUGRA respectively. These event numbers are then normalised to 21 fb^{-1} luminosity.

Example cutflow for three benchmark signal points in the 2tau analysis. Specific SRs are indicated at the respective cut. Event numbers are normalised to 21 fb^{-1} luminosity. For the GMSB point 50000 events have been generated, 20000 for nGM and 25000 for bRPV respectively.

Example cutflow for four benchmark signal points in the tau+e analysis. Event numbers are normalised to 21 fb^{-1} luminosity. For the GMSB point 50000 events have been generated, 20000 for nGM, 20000 for mSUGRA and 25000 for bRPV respectively.

Example cutflow for four benchmark signal points in the tau+mu analysis. Event numbers are normalised to 21 fb^{-1} luminosity. For the GMSB point 50000 events have been generated, 20000 for nGM, 20000 for mSUGRA and 25000 for bRPV respectively.

The effective mass distribution in 3-jet signal region.

The effective mass distribution in 4-jet (W) signal region.

The effective mass distribution in 4-jet very-loose and loose signal regions.

The effective mass distribution in 4-jet medium signal region.

The effective mass distribution in 4-jet tight signal region.

The effective mass distribution in 5-jet signal region.

The effective mass distribution in 6-jet loose and medium signal regions.

The effective mass distribution in 6-jet tight signal region.

The effective mass distribution in 6-jet very-tight signal region.

Observed limit 95% CL.

Expected limit 95% CL.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Expected limit 95% CL -1 sigma.

Observed limit 95% CL.

Expected limit 95% CL.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Expected limit 95% CL -1 sigma.

Observed limit 95% CL (m_chi^0_1=0GeV).

Expected limit 95% CL (m_chi^0_1=0GeV).

Observed limit 95% CL +1 sigma (m_chi^0_1=0GeV).

Observed limit 95% CL -1 sigma (m_chi^0_1=0GeV).

Expected limit 95% CL +1 sigma (m_chi^0_1=0GeV).

Expected limit 95% CL -1 sigma (m_chi^0_1=0GeV).

Observed limit 95% CL (m_chi^0_1=395GeV).

Expected limit 95% CL (m_chi^0_1=395GeV).

Observed limit 95% CL (m_chi^0_1=695GeV).

Expected limit 95% CL (m_chi^0_1=695GeV).

Expected limit 95% CL.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Expected limit 95% CL.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Expected limit 95% CL.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Observed CLs contour for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour with plus 1-sigma signal cross-section uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour with minus 1-sigma signal cross-section uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour with plus 1-sigma experimental uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour with minus 1-sigma experimental uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour with plus 1-sigma signal cross-section uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour with minus 1-sigma signal cross-section uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour with plus 1-sigma experimental uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour with minus 1-sigma experimental uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour with plus 1-sigma signal cross-section uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour with minus 1-sigma signal cross-section uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour with plus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

First of two expected CLs contours with minus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Second of two expected CLs contours with minus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour with plus 1-sigma signal cross-section uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour with minus 1-sigma signal cross-section uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour with plus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour with minus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Expected limit 95% CL.

Expected limit 95% CL.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Signal region for points.

Signal region for points.

Signal region for points (m_chi^0_1=0GeV).

Signal region for points (m_chi^0_1=395GeV).

Signal region for points (m_chi^0_1=695GeV).

Observed 95% CL cross-section upper limit for pair-produced gluinos decaying directly.

Observed 95% CL cross-section upper limit for associated gluino-squark production.

Observed 95% CL cross-section upper limit for pair-produced squarks decaying directly.

Observed 95% CL cross-section upper limit for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed 95% CL cross-section upper limit for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed 95% CL cross-section upper limit for the pair-produced squarks each decaying via an intermediate chargino1 to quark, a W boson and a neutralino1.

Observed 95% CL cross-section upper limit for the pair-produced squarks each decaying via an intermediate chargino1 to quark, a W boson and a neutralino1.

Signal region for points.

Observed 95% CL cross-section upper limit for pair-produced gluinos decaying via stops into top+charm+neutralino1.

Production cross-section in PB.

Signal acceptance in PCT for SR2jl.

Signal acceptance times reconstruction efficiency in PCT for SR2jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jl.

Signal acceptance in PCT for SR2jm.

Signal acceptance times reconstruction efficiency in PCT for SR2jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jm.

Signal acceptance in PCT for SR2jt.

Signal acceptance times reconstruction efficiency in PCT for SR2jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jt.

Signal acceptance in PCT for SR2jW.

Signal acceptance times reconstruction efficiency in PCT for SR2jW.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jW.

Signal acceptance in PCT for SR3j.

Signal acceptance times reconstruction efficiency in PCT for SR3j.

Uncertainty on signal acceptance times reconstruction efficiency for SR3j.

Signal acceptance in PCT for SR4jW.

Signal acceptance times reconstruction efficiency in PCT for SR4jW.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jW.

Signal acceptance in PCT for SR4jl-.

Signal acceptance times reconstruction efficiency in PCT for SR4jl-.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jl-.

Signal acceptance in PCT for SR4jl.

Signal acceptance times reconstruction efficiency in PCT for SR4jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jl.

Signal acceptance in PCT for SR4jm.

Signal acceptance times reconstruction efficiency in PCT for SR4jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jm.

Signal acceptance in PCT for SR4jt.

Signal acceptance times reconstruction efficiency in PCT for SR4jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jt.

Signal acceptance in PCT for SR5j.

Signal acceptance times reconstruction efficiency in PCT for SR5j.

Uncertainty on signal acceptance times reconstruction efficiency for SR5j.

Signal acceptance in PCT for SR6jl.

Signal acceptance times reconstruction efficiency in PCT for SR6jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jl.

Signal acceptance in PCT for SR6jm.

Signal acceptance times reconstruction efficiency in PCT for SR6jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jm.

Signal acceptance in PCT for SR6jt.

Signal acceptance times reconstruction efficiency in PCT for SR6jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jt.

Signal acceptance in PCT for SR6jt+.

Signal acceptance times reconstruction efficiency in PCT for SR6jt+.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jt+.

Production cross-section in PB.

Signal acceptance in PCT for SR2jl.

Signal acceptance times reconstruction efficiency in PCT for SR2jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jl.

Signal acceptance in PCT for SR2jm.

Signal acceptance times reconstruction efficiency in PCT for SR2jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jm.

Signal acceptance in PCT for SR2jt.

Signal acceptance times reconstruction efficiency in PCT for SR2jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jt.

Signal acceptance in PCT for SR2jW.

Signal acceptance times reconstruction efficiency in PCT for SR2jW.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jW.

Signal acceptance in PCT for SR3j.

Signal acceptance times reconstruction efficiency in PCT for SR3j.

Uncertainty on signal acceptance times reconstruction efficiency for SR3j.

Signal acceptance in PCT for SR4jW.

Signal acceptance times reconstruction efficiency in PCT for SR4jW.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jW.

Signal acceptance in PCT for SR4jl-.

Signal acceptance times reconstruction efficiency in PCT for SR4jl-.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jl-.

Signal acceptance in PCT for SR4jl.

Signal acceptance times reconstruction efficiency in PCT for SR4jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jl.

Signal acceptance in PCT for SR4jm.

Signal acceptance times reconstruction efficiency in PCT for SR4jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jm.

Signal acceptance in PCT for SR4jt.

Signal acceptance times reconstruction efficiency in PCT for SR4jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jt.

Signal acceptance in PCT for SR5j.

Signal acceptance times reconstruction efficiency in PCT for SR5j.

Uncertainty on signal acceptance times reconstruction efficiency for SR5j.

Signal acceptance in PCT for SR6jl.

Signal acceptance times reconstruction efficiency in PCT for SR6jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jl.

Signal acceptance in PCT for SR6jm.

Signal acceptance times reconstruction efficiency in PCT for SR6jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jm.

Signal acceptance in PCT for SR6jt.

Signal acceptance times reconstruction efficiency in PCT for SR6jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jt.

Signal acceptance in PCT for SR6jt+.

Signal acceptance times reconstruction efficiency in PCT for SR6jt+.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jt+.

The structure functions for Q**2 = 1.74 - 1.75 GeV**2 and XB = 0.223 - 0.224 as functions of t.

The structure functions for Q**2 = 1.87 GeV**2 and XB = 0.270 - 0.272 as functions of t.

The structure functions for Q**2 = 1.95 - 1.96 GeV**2 and XB = 0.313 as functions of t.

The structure functions for Q**2 = 2.10 GeV**2 and XB = 0.238 - 0.239 as functions of t.

The structure functions for Q**2 = 2.21 GeV**2 and XB = 0.275 - 0.277 as functions of t.

The structure functions for Q**2 = 2.24 - 2.25 GeV**2 and XB = 0.332 - 0.339 as functions of t.

The structure functions for Q**2 = 2.34 - 2.35 GeV**2 and XB = 0.403 - 0.404 as functions of t.

The structure functions for Q**2 = 2.71 - 2.72 GeV**2 and XB = 0.336 - 0.344 as functions of t.

The structure functions for Q**2 = 2.75 GeV**2 and XB = 0.423 - 0.424 as functions of t.

The structure functions for Q**2 = 3.12 GeV**2 and XB = 0.362 as functions of t.

The structure functions for Q**2 = 3.22 - 3.23 GeV**2 and XB = 0.431 - 0.432 as functions of t.

The structure functions for Q**2 = 3.29 GeV**2 and XB = 0.496 as functions of t.

The structure functions for Q**2 = 3.67 - 3.68 GeV**2 and XB = 0.451 as functions of t.

The structure functions for Q**2 = 3.76 GeV**2 and XB = 0.513 - 0.514 as functions of t.

The structure functions for Q**2 = 4.23 GeV**2 and XB = 0.539 as functions of t.

Results for G1(DEUT)/F1(DEUT) for the deuteron in bins of (W;Q**2), along with average kinematic values and correction factors for each bin. All values are averaged over the event distribution.

The systematic uncertainties for the nominal muon-channel cross-section measurement. Some sources of uncertainty have both correlated and uncorrelated components. Correlated uncertainties arise from the uncertainty in the electroweak background contributions delta(e.w.)_cor, from corrections to the Monte Carlo modelling of the Z/gamma* pT spectra, and from the reconstruction, trigger and isolation efficiency corrections, given by delta(reco)_cor, delta(trig)_cor and delta(iso)_cor respectively. The uncertainty on the multijet and electroweak background cross sections, given by delta(multijet and delta(e.w.), respectively and muon momentum scale uncertainty, delta(pT_scale) are also correlated. Uncorrelated uncertainties are due to corrections for the trigger and isolation efficiencies, given by delta(trig)_unc and delta(iso)_unc respectively. The uncertainty from the muon resolution correction, delta(res), from the size of the signal Monte Carlo sample, delta(MC), and the uncertaintities due to corrections for the reconstruction, delta(reco)_unc, are also uncorrelated. The luminosity uncertainty 1.8% is not included.

The combined Born-level fiducial differential cross section dsigma/dm_ll, statistical delta(stat), total correlated delta(cor), uncorrelated delta(unc), and total delta(total) uncertainties, as well as individual correlated sources delta(cor)_i. The correlated uncertainties are a linear combination of the 13 correlated uncertainties in the nominal muon and electron channels. As the uncertainties on the combined result no longer originate from individual error sources they are numbered 1-13. Also shown is the correction factor used to derive the dressed cross section (D), and the NNLO extrapolation factor (A) used to derive the cross section for the full phase space, along with the uncertainties associated to variations in scale choice delta(A)_scale, and PDF uncertainty delta(A)_pdf_alpha_s. The luminosity uncertainty 1.8% is not included.

The extended muon channel Born-level fiducial differential cross section dsigma/dm_ll, with the statistical delta(stat), systematic delta(syst), and total delta(tot) uncertainties for each invariant mass bin. Also shown is the correction factor used to derive the dressed cross section (D), and the extrapolation factor (A) used to derive the cross section for the full phase space, along with the uncertainties associated to variations in scale delta(A)_scale, and PDF uncertainty delta(A)_pdf_alpha_s. The luminosity uncertainty 3.5% is not included.

The systematic uncertainties for the extended muon channel cross-section measurement in each invariant mass bin. Correlated uncertainties come from the reconstruction, trigger and isolation efficiency corrections, given by delta(reco), delta(trig) and delta(iso) respectively. The uncertainty on the multijet background cross section, delta(multijet) and the uncertainty on the muon momentum scale, delta(pT_scale), are also correlated across bins. Uncorrelated uncertainties are due to the uncertainty from the muon resolution correction, delta(res), and the sample size of the signal Monte Carlo sample, delta(MC). The luminosity uncertainty 3.5% is not included.

Theory predictions for NLO+LLPS and for fixed-order calculations at NLO and NNLO including higher-order electroweak corrections, for the nominal analysis of the differential cross section dsigma/dm_ll as a function of the invariant mass m_ll. The scale uncertainty is defined as the envelope of variations for 0.5< mu_R,mu_F<2.0 for Powheg. For Fewz the scale uncertainty is defined by the variation 0.5<mu_R=mu_F<2.0. The uncertainty labelled as "stat" in the table corresponds to the pdf+alpha_s uncertainty for Fewz or just the pdf uncertainty for Powheg.

Theory predictions for NLO+LLPS and for fixed-order calculations at NLO and NNLO including higher-order electroweak corrections, for the extended analysis of the differential cross section dsigma/dm_ll as a function of the invariant mass m_ll. The scale uncertainty is defined as the envelope of variations for 0.5<mu_R,mu_F<2.0 for Powheg. For Fewz the scale uncertainty is defined by the variation 0.5<mu_R=mu_F<2.0. The uncertainty labelled as "stat" in the table corresponds to the pdf+alpha_s uncertainty for Fewz or just the pdf uncertainty for Powheg.

Higher-order electroweak corrections in nominal analysis, Delta(HOEW), and the correction for the Photon Induced process, Delta(PI), together with its uncertainty derived from the uncertainty of the photon PDF as a function of the dilepton invariant mass m_ll. Also shown is the difference arising from the non-convergence of calculations derived with different electroweak schema, delta(scheme).

Higher-order electroweak corrections in extended analysis, Delta(HOEW), and the correction for the Photon Induced process, Delta(PI), together with its uncertainty derived from the uncertainty of the photon PDF as a function of the dilepton invariant mass m_ll. Also shown is the difference arising from the non-convergence of calculations derived with different electroweak schema, delta(scheme).

Values of chi^2 for the nominal and extended DY cross-section measurements for predictions based from Fewz at NLO and NNLO and Powheg using MSTW2008 PDFs accounting for the experimental correlated systematic uncertainties. The _pdf_scale columns show the chi^2 when the PDF and scale uncertainties on the theoretical predictions are taken into account.

The chi^2 values from NLO and NNLO QCD fits made using the ATLAS nominal and extended Drell--Yan cross-section measurements and the HERA-I dataset accounting for the experimental correlated systematic uncertainties.

The measured individual cross sections in the fiducial region and the combined cross sections for 4-muon and 4-electron final states at a centre-of-collision energy of 8 TeV.

The measured individual cross sections in the fiducial region and the combined cross sections for for 2-muon-2-electron final states at a centre-of-collision energy of 8 TeV.

The measured cross section for four-lepton final states at a centre-of-collision energy of 8 TeV.

The branching fraction for Z0 --> 4 LEPTON, summed over all final states, measured using both the 7 and 8 TeV datasets.

Inclusive muon cross section from W+->mu+nu simulated with MC with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from W-->mu-nu simulated with MC with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from Z->mu+mu- simulated with MC with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV (the Z is defined as Z/gamma* with m_ll > 60 GeV): the error shown is due to the MC statistics.

Inclusive muon cross section from backgrounds: Z->tau tau, ttbar, Drell-Yan->mu+mu- (Drell-Yan is defined as Z/gamma* with m_ll < 60 GeV) simulated with Pythia with MRSTLO* pdf set for |eta| < 2.5 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from bbar+ccbar production and decays simulated with FONLL with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV: the error shown is the uncertainty due to scale variation, alpha_s+pdf using CTEQ6.6 error set and the heavy quark masses.

Inclusive muon cross section from bbar+ccbar simulated with FONLL removing the resummation term with CTEQ6.6 pdf set for |eta| < 2.5 and pT > 4 GeV?.

Inclusive muon cross section for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: (stat) statistical error, (sys) systematic error. The first systematic error is the intrinsic error of the measurement, the second is the error due to the luminosity.

Inclusive muon cross section after subtraction of W,Z, Drell-Yan and top background for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: (stat): statistical error, (sys): systematic error. The first systematic error is the intrinsic error of the measurement, the second the error due to the luminosity, the third is due to the subtraction of the background and is dominated by the error on the W, Z inclusive cross sections.

Inclusive muon cross section from W+->mu+nu simulated with MC with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from W-->mu-nu simulated with MC with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from Z->mu+mu- simulated with MC with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV (the Z is defined as Z/gamma* with m_ll > 60 GeV): the error shown is due to the MC statistics.

Inclusive muon cross section from backgrounds: Z->tau tau, ttbar, Drell-Yan->mu+mu- (Drell-Yan is defined as Z/gamma* with m_ll < 60 GeV) simulated with Pythia with MRSTLO* pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: the error shown is due to the MC statistics.

Inclusive muon cross section from bbar+ccbar production and decays simulated with FONLL with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV: the error shown is the uncertainty due to scale variation, alpha_s+pdf using CTEQ6.6 error set and the heavy quark masses.

Inclusive muon cross section from bbar+ccbar simulated with FONLL removing the resummation term with CTEQ6.6 pdf set for |eta| < 2.0 excluding 1.37 < |eta| < 1.52 and pT > 4 GeV.

The observed 95% CL upper limits on the cross section for p p --> zprime x BR(zprime -> e-mu) as a function of the zprime mass.

Measured fiducial cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> e+e- final state.

Measured fiducial cross section times leptonic branching ratio for W+ production in the W+ -> mu+ nu final state.

Measured fiducial cross section times leptonic branching ratio for W- production in the W- -> mu- nubar final state.

Measured fiducial cross section times leptonic branching ratio for W+/- production in the combined W+ -> mu+ nu and W- -> mu- nubar final state.

Measured fiducial cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> mu+ mu- final state.

Measured total cross section times leptonic branching ratio for W+ production in the W+ -> e+ nu final state.

Measured total cross section times leptonic branching ratio for W- production in the W- -> e- nubar final state.

Measured total cross section times leptonic branching ratio for W+/- production in the combined W+ -> e+ nu and W- -> e- nubar final state.

Measured total cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> e+ e- final state.

Measured total cross section times leptonic branching ratio for W+ production in the W+ -> mu+ nu final state.

Measured total cross section times leptonic branching ratio for W- production in the W- -> mu- nubar final state.

Measured total cross section times leptonic branching ratio for W+/- production in the combined W+ -> mu+ nu and W- -> mu- nubar final state.

Measured total cross section times leptonic branching ratio for Z/gamma* production in the Z/gamma* -> mu+ mu- final state.

Measured total cross section times leptonic branching ratio for W+ production in the W+ -> l+ nu (l = e, mu) final states.

Measured total cross section times leptonic branching ratio for W- production in the W- -> l- nubar (l = e, mu) final states.

Measured total cross section times leptonic branching ratio for W+/- production in the combined W+ -> l+ nu and W- -> l- nubar (l = e, mu) final states.

Measured total cross section times leptonic branching ratio for Z/gamma* production in the combined Z/gamma* -> l+ l- (l = e, mu) final states.

Measured total cross-section ratio R_{W+/Z} = sigma (W+ -> e+ nu) / sigma (Z/gamma^* -> e+ e-).

Measured total cross-section ratio R_{W-/Z} = sigma (W- -> e- nubar) / sigma (Z/gamma^* -> e+ e-).

Measured total cross-section ratio R_{W+-/Z} = sigma (W+/- -> e+/- nu/nubar) / sigma (Z/gamma^* -> e+ e-).

Measured total cross-section ratio R_{W+/Z} = sigma (W+ -> mu+ nu) / sigma (Z/gamma^* -> mu+ mu-).

Measured total cross-section ratio R_{W-/Z} = sigma (W- -> mu- nubar) / sigma (Z/gamma^* -> mu+ mu-).

Measured total cross-section ratio R_{W+-/Z} = sigma (W+/- -> mu+/- nu/nubar) / sigma (Z/gamma^* -> mu+ mu-).

Measured total cross-section ratio R_{W+/Z} = sigma (W+ -> l+ nu) / sigma (Z/gamma^* -> l+ l-) where (l = e, mu).

Measured total cross-section ratio R_{W-/Z} = sigma (W- -> l- nubar) / sigma (Z/gamma^* -> l+ l-) where (l = e, mu).

Measured total cross-section ratio R_{W+-/Z} = sigma (W+/- -> l+/- nu/nubar) / sigma (Z/gamma^* -> l+ l-) where (l = e, mu).

Measured lepton asymmetry from W+ -> e+ nu and W- -> e- nubar, binned as a function pseudorapidity.

Measured lepton asymmetry from W+ -> e+ nu and W- -> e- nubar.

Measured lepton asymmetry from W+ -> mu+ nu and W- -> mu- nubar, binned as a function pseudorapidity.

Measured lepton asymmetry from W+ -> mu+ nu and W- -> mu- nubar.

Measured lepton asymmetry from W+ -> l+ nu and W- -> l- nubar (l = e, mu), binned as a function pseudorapidity.

Measured lepton asymmetry from W+ -> l+ nu and W- -> l- nubar (l = e, mu).

Differential cross section for the W range 1.71 to 1.72 GeV.

Differential cross section for the W range 1.72 to 1.73 GeV.

Differential cross section for the W range 1.73 to 1.74 GeV.

Differential cross section for the W range 1.74 to 1.75 GeV.

Differential cross section for the W range 1.75 to 1.76 GeV.

Differential cross section for the W range 1.76 to 1.77 GeV.

Differential cross section for the W range 1.77 to 1.78 GeV.

Differential cross section for the W range 1.78 to 1.79 GeV.

Differential cross section for the W range 1.79 to 1.80 GeV.

Differential cross section for the W range 1.80 to 1.81 GeV.

Differential cross section for the W range 1.81 to 1.82 GeV.

Differential cross section for the W range 1.82 to 1.83 GeV.

Differential cross section for the W range 1.83 to 1.84 GeV.

Differential cross section for the W range 1.84 to 1.85 GeV.

Differential cross section for the W range 1.85 to 1.86 GeV.

Differential cross section for the W range 1.86 to 1.87 GeV.

Differential cross section for the W range 1.87 to 1.88 GeV.

Differential cross section for the W range 1.88 to 1.89 GeV.

Differential cross section for the W range 1.89 to 1.90 GeV.

Differential cross section for the W range 1.90 to 1.91 GeV.

Differential cross section for the W range 1.91 to 1.92 GeV.

Differential cross section for the W range 1.92 to 1.93 GeV.

Differential cross section for the W range 1.93 to 1.94 GeV.

Differential cross section for the W range 1.94 to 1.95 GeV.

Differential cross section for the W range 1.96 to 1.97 GeV.

Differential cross section for the W range 1.97 to 1.98 GeV.

Differential cross section for the W range 1.98 to 1.99 GeV.

Differential cross section for the W range 1.99 to 2.00 GeV.

Differential cross section for the W range 2.00 to 2.01 GeV.

Differential cross section for the W range 2.01 to 2.02 GeV.

Differential cross section for the W range 2.02 to 2.03 GeV.

Differential cross section for the W range 2.03 to 2.04 GeV.

Differential cross section for the W range 2.04 to 2.05 GeV.

Differential cross section for the W range 2.05 to 2.06 GeV.

Differential cross section for the W range 2.06 to 2.07 GeV.

Differential cross section for the W range 2.07 to 2.08 GeV.

Differential cross section for the W range 2.08 to 2.09 GeV.

Differential cross section for the W range 2.09 to 2.10 GeV.

Differential cross section for the W range 2.10 to 2.12 GeV.

Differential cross section for the W range 2.12 to 2.14 GeV.

Differential cross section for the W range 2.14 to 2.16 GeV.

Differential cross section for the W range 2.16 to 2.18 GeV.

Differential cross section for the W range 2.18 to 2.20 GeV.

Differential cross section for the W range 2.20 to 2.22 GeV.

Differential cross section for the W range 2.22 to 2.24 GeV.

Differential cross section for the W range 2.24 to 2.26 GeV.

Differential cross section for the W range 2.26 to 2.28 GeV.

Differential cross section for the W range 2.28 to 2.30 GeV.

Differential cross section for the W range 2.30 to 2.32 GeV.

Differential cross section for the W range 2.32 to 2.34 GeV.

Differential cross section for the W range 2.34 to 2.36 GeV.

Differential cross section for the W range 2.36 to 2.40 GeV.

Differential cross section for the W range 2.40 to 2.44 GeV.

Differential cross section for the W range 2.44 to 2.48 GeV.

Differential cross section for the W range 2.48 to 2.52 GeV.

Differential cross section for the W range 2.52 to 2.56 GeV.

Differential cross section for the W range 2.56 to 2.60 GeV.

Differential cross section for the W range 2.60 to 2.64 GeV.

Differential cross section for the W range 2.64 to 2.68 GeV.

Differential cross section for the W range 2.68 to 2.73 GeV.

Differential cross section for the W range 2.75 to 2.84 GeV.

Differential cross section for the W range 1.92 to 1.93 GeV.

Differential cross section for the W range 1.93 to 1.94 GeV.

Differential cross section for the W range 1.94 to 1.95 GeV.

Differential cross section for the W range 1.96 to 1.97 GeV.

Differential cross section for the W range 1.97 to 1.98 GeV.

Differential cross section for the W range 1.98 to 1.99 GeV.

Differential cross section for the W range 1.99 to 2.00 GeV.

Differential cross section for the W range 2.00 to 2.01 GeV.

Differential cross section for the W range 2.01 to 2.02 GeV.

Differential cross section for the W range 2.02 to 2.03 GeV.

Differential cross section for the W range 2.03 to 2.04 GeV.

Differential cross section for the W range 2.04 to 2.05 GeV.

Differential cross section for the W range 2.05 to 2.06 GeV.

Differential cross section for the W range 2.06 to 2.07 GeV.

Differential cross section for the W range 2.07 to 2.08 GeV.

Differential cross section for the W range 2.08 to 2.09 GeV.

Differential cross section for the W range 2.09 to 2.10 GeV.

Differential cross section for the W range 2.10 to 2.12 GeV.

Differential cross section for the W range 2.12 to 2.14 GeV.

Differential cross section for the W range 2.14 to 2.16 GeV.

Differential cross section for the W range 2.16 to 2.18 GeV.

Differential cross section for the W range 2.18 to 2.20 GeV.

Differential cross section for the W range 2.20 to 2.22 GeV.

Differential cross section for the W range 2.22 to 2.24 GeV.

Differential cross section for the W range 2.24 to 2.26 GeV.

Differential cross section for the W range 2.26 to 2.28 GeV.

Differential cross section for the W range 2.28 to 2.30 GeV.

Differential cross section for the W range 2.30 to 2.32 GeV.

Differential cross section for the W range 2.32 to 2.34 GeV.

Differential cross section for the W range 2.34 to 2.36 GeV.

Differential cross section for the W range 2.36 to 2.40 GeV.

Differential cross section for the W range 2.40 to 2.44 GeV.

Differential cross section for the W range 2.44 to 2.48 GeV.

Differential cross section for the W range 2.48 to 2.52 GeV.

Differential cross section for the W range 2.52 to 2.56 GeV.

Differential cross section for the W range 2.56 to 2.60 GeV.

Differential cross section for the W range 2.60 to 2.64 GeV.

Differential cross section for the W range 2.64 to 2.68 GeV.

Differential cross section for the W range 2.68 to 2.73 GeV.

Differential cross section for the W range 2.75 to 2.84 GeV.

Measured value of TT and LT polarized cross sections extracted from the data.

Values of r_04_00 and r_1_1-1 extracted from the angular distributions.

Recoil neutron angular distributions for neutron momenta less than 100 MeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.

Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.

Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the simultaneous EPSILON-PHI fit method.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the Rosenbluth separation technique fit method.. E99M29 E99M30 E99M31.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the Rosenbluth separation technique fit method.. E99M29 E99M30 E99M31.

Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the Rosenbluth separation technique fit method.. E99M29 E99M30 E99M31.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.

Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.