Measured differential cross section with associated uncertainties as a function of COS(THETA*). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of DELTAYRAP(2GAMMA). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of MULT(JET,PT>30 GEV). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of MULT(JET,PT>50 GEV). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of PT(JET1). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of PT(JET2). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of HT. Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of YRAP(JET1). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of YRAP(JET2). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of M(2JET). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of DELTAYRAP(2JET). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of ABSDPHI(2JET). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of DPHI(2JET). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of PT(2GAMMA2JET). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of DPHI(2GAMMA,2JET). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of TAUJET. Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of SUM(TAUJET). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of PT(2GAMMA) [NJET=0,PT>30 GEV]. Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of PT(2GAMMA) [NJET=1,PT>30 GEV]. Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of PT(2GAMMA) [NJET=2,PT>30 GEV]. Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

Measured differential cross section with associated uncertainties as a function of PT(2GAMMA) [NJET>=3,PT>30 GEV]. Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.

The measured cross sections or cross section limits of the diphoton, VBF-enhanced, Nlepton $\geq$ 1, high $E_{T}^{miss}$, and ttH-enhanced fiducial regions are shown.

Measured differential cross section with associated uncertainties as a function of diphoton transverse momentum in bins of ABS(COS(THETA*)). Each systematic uncertainty sources is fully uncorrelated with the other sources and fully correlated across bins, except for the background modelling systematics for which an uncorrelated treatment across bins is more appropriate.Each systematic uncertainty sources is fully uncorrelated with the other sources.

Non-perturbative correction factors in percent accounting for the impact of hadronisation and the underlying event activity for all measured variables and fiducial regions. Regions of phase space where no reliable estimate could be obtained are listed as 100 without uncertainties. Uncertainties are evaluated by deriving these factors using different generators and tunes as described in the text. No factor are given for the Nlepton $\geq$ 1 and High-$E_{T}^{miss}$ fiducial regions as the gluon fusion contamination in both is negligible.

Isolation efficiencies in percent for gluon fusion $H\rightarrow\gamma\gamma$ for each fiducial region/variable bin measured in this analysis. The isolation efficiency is defined as the probability for both photons to fulfil the isolation criteria (as described in Section 9.1) for events that pass the diphoton kinematic criteria. Regions of phase space where no reliable estimate could be obtained are listed as 100 without uncertainties. Uncertainties are assigned in the same way as for the non-perturbative correction factors: by varying the fragmentation and underlying event modelling. These factors can be multiplied by the kinematic acceptance factors (see Table 29) to extrapolate an inclusive gluon fusion Higgs prediction to the fiducial volume used in this analysis. No factors for the Nlepton $\geq$ 1 and High $E_{T}^{miss}$ fiducial regions are provided as the gluon fusion contamination is negligible.

Combined non-perturbative (Table 27) and particle-level isolation correction factors (Table 28) in percent accounting for the impact of hadronisation and the underlying event activity for all measured variables and fiducial regions. Regions of phase space where no reliable estimate could be obtained are listed as 100 without uncertainties. The uncertainties on the combined values properly take into account the correlations between both multiplicative factors.

Diphoton kinematic acceptances in percent for gluon-gluon fusion for the diphoton fiducial region and all differential variable bins studied in this paper, defined as the probability to fulfill the diphoton kinematic criteria: $p_{T}$/$m_{\gamma\gamma}$ < 0.35 (0.25) for the leading (subleading) photon and $|\eta_{\gamma\gamma}|$ < 2.37. The factors are evaluated using the Powheg NNLOPSevent generator. Uncertainties are taken from PDF variations. QCD scale variations have a negligible impact on these factors. The range of each bin is given in Table 26.

observed statistical correlations between pTyy, Njets, mjj, |DeltaPhijj| and pTj1

ggH default MC + XH predictions

XH ( = VBF + VH + ttH + bbH ) MC predictions

Best-fit values and uncertainties of the production-mode cross sections times branching ratio.

Best-fit values and uncertainties of the simplified template cross sections times branching ratio.

Observed correlations between the measured simplified template cross sections, including both the statistical and systematic uncertainties.

Best-fit values and uncertainties of the simplified template cross sections times branching ratio.

Observed correlations between the measured simplified template cross sections, including both the statistical and systematic uncertainties.

Observed correlations between the measured simplified template cross sections, including both the statistical and systematic uncertainties.

Distribution of the missing transverse momentum $E_{\mathrm{T}}^{\mathrm{miss}}$ for the sample satisfying all requirements of the $\mathrm{SR}^{\gamma\gamma}_{W-L}$ selection except the $E_{\mathrm{T}}^{\mathrm{miss}}$ requirement itself. Overlaid are the expected SM backgrounds, separated into the various contributing sources. Also shown are the signal expectations for the ($m_{\tilde{W}}$, $m_{\tilde{\chi}^{0}_{1}}$) = (1000,100) GeV and ($m_{\tilde{W}}$, $m_{\tilde{\chi}^{0}_{1}}$) = (1000,800) GeV models. The vertical dashed lines and right-pointing arrows show the region of the $E_{\mathrm{T}}^{\mathrm{miss}}$ observable selected for inclusion in $\mathrm{SR}^{\gamma\gamma}_{W-L}$ and $\mathrm{SR}^{\gamma\gamma}_{W-H}$. The lower panels show the ratio of observed data to the combined SM expectation. For these plots, the band represents the range of combined statistical and systematic uncertainty in the SM expectation. Events outside the range of the displayed region are included in the highest-value bin.

Distribution of the missing transverse momentum $E_{\mathrm{T}}^{\mathrm{miss}}$ for the sample satisfying all requirements of the $\mathrm{SR}^{\gamma\gamma}_{W-H}$ selection except the $E_{\mathrm{T}}^{\mathrm{miss}}$ requirement itself. Overlaid are the expected SM backgrounds, separated into the various contributing sources. Also shown are the signal expectations for the ($m_{\tilde{W}}$, $m_{\tilde{\chi}^{0}_{1}}$) = (1000,100) GeV and ($m_{\tilde{W}}$, $m_{\tilde{\chi}^{0}_{1}}$) = (1000,800) GeV models. The vertical dashed lines and right-pointing arrows show the region of the $E_{\mathrm{T}}^{\mathrm{miss}}$ observable selected for inclusion in $\mathrm{SR}^{\gamma\gamma}_{W-L}$ and $\mathrm{SR}^{\gamma\gamma}_{W-H}$. The lower panels show the ratio of observed data to the combined SM expectation. For these plots, the band represents the range of combined statistical and systematic uncertainty in the SM expectation. Events outside the range of the displayed region are included in the highest-value bin.

Comparisons between expected and observed content of the validation and signal regions for the photon+jets analysis. The uncertainties in the expected numbers of events are the combined statistical and systematic uncertainties. The lower panel shows the pull (difference between observed and expected event counts normalized by the uncertainty) for each region.

Distribution of the missing transverse momentum $E_{\mathrm{T}}^{\mathrm{miss}}$ for the sample satisfying all requirements of the $\mathrm{SR}^{\gamma j}_{H}$ selection except the $E_{\mathrm{T}}^{\mathrm{miss}}$ requirement itself. Overlaid are the expected SM backgrounds, separated into the various contributing sources. Also shown are the signal expectations for points in the $m_{\tilde{g}}-m_{\tilde{\chi}^{0}_{1}}$ parameter space of the GGM model relevant to the photon+jets analysis (mass values in GeV). The value of the gluino mass arises from the choice $M_{3}$ = 1900 GeV. The $\tilde{\chi}^{0}_{1}$ mass values of 1868, 1920, 442 and 652 GeV arise from the choices $\mu$ = 1810, 1868, 400 and 600 GeV, respectively, combined with the constraint that the branching fraction of $\tilde{\chi}^{0}_{1}$ $\to \gamma \tilde{G}$ be 50%. The vertical dashed lines and right-pointing arrows show the region of the $E_{\mathrm{T}}^{\mathrm{miss}}$ observable selected for inclusion in $\mathrm{SR}^{\gamma j}_{H}$ and $\mathrm{SR}^{\gamma j}_{L}$ for $\mathrm{SR}^{\gamma j}_{L200}$, the $E_{\mathrm{T}}^{\mathrm{miss}}$ requirement is 200 GeV rather than 300 GeV. The lower panels show the ratio of observed data to the combined SM expectation. For these plots, the band represents the range of statistical uncertainty in the SM expectation. Events outside the range of the displayed region are included in the highest-value bin.

Distribution of the missing transverse momentum $E_{\mathrm{T}}^{\mathrm{miss}}$ for the sample satisfying all requirements of the $\mathrm{SR}^{\gamma j}_{L}$ or $\mathrm{SR}^{\gamma j}_{L200}$ selection except the $E_{\mathrm{T}}^{\mathrm{miss}}$ requirement itself. Overlaid are the expected SM backgrounds, separated into the various contributing sources. Also shown are the signal expectations for points in the $m_{\tilde{g}}-m_{\tilde{\chi}^{0}_{1}}$ parameter space of the GGM model relevant to the photon+jets analysis (mass values in GeV). The value of the gluino mass arises from the choice $M_{3}$ = 1900 GeV. The $\tilde{\chi}^{0}_{1}$ mass values of 1868, 1920, 442 and 652 GeV arise from the choices $\mu$ = 1810, 1868, 400 and 600 GeV, respectively, combined with the constraint that the branching fraction of $\tilde{\chi}^{0}_{1} \to \gamma \tilde{G}$ be 50%. The vertical dashed lines and right-pointing arrows show the region of the $E_{\mathrm{T}}^{\mathrm{miss}}$ observable selected for inclusion in $\mathrm{SR}^{\gamma j}_{H}$ and $\mathrm{SR}^{\gamma j}_{L}$ for $\mathrm{SR}^{\gamma j}_{L200}$, the $E_{\mathrm{T}}^{\mathrm{miss}}$ requirement is 200 GeV rather than 300 GeV. The lower panels show the ratio of observed data to the combined SM expectation. For these plots, the band represents the range of statistical uncertainty in the SM expectation. Events outside the range of the displayed region are included in the highest-value bin.

Expected exclusion limits in the gluino-bino mass plane, using the $\mathrm{SR}^{\gamma\gamma}_{S-H}$ analysis for $m_{\tilde{\chi}^{0}_{1}} > 1600$ GeV and the $\mathrm{SR}^{\gamma\gamma}_{S-L}$ analysis for $m_{\tilde{\chi}^{0}_{1}} < 1600$ GeV.

Observed exclusion limits in the gluino--bino mass plane, using the $\mathrm{SR}^{\gamma\gamma}_{S-H}$ analysis for $m_{\tilde{\chi}^{0}_{1}} > 1600$ GeV and the $\mathrm{SR}^{\gamma\gamma}_{S-L}$ analysis for $m_{\tilde{\chi}^{0}_{1}} < 1600$ GeV.

Expected exclusion limit in the squark-bino mass plane, using the $\mathrm{SR}^{\gamma\gamma}_{S-H}$ analysis for $m_{\tilde{\chi}^{0}_{1}} > 900$ GeV and the $\mathrm{SR}^{\gamma\gamma}_{S-L}$ analysis for $m_{\tilde{\chi}^{0}_{1}} < 900$ GeV.

Observed exclusion limit in the squark--bino mass plane, using the $\mathrm{SR}^{\gamma\gamma}_{S-H}$ analysis for $m_{\tilde{\chi}^{0}_{1}} > 900$ GeV and the $\mathrm{SR}^{\gamma\gamma}_{S-L}$ analysis for $m_{\tilde{\chi}^{0}_{1}} < 900$ GeV.

Expected exclusion limit in the wino-bino mass plane, using the $\mathrm{SR}^{\gamma\gamma}_{W-H}$ analysis for $m_{\tilde{\chi}^{0}_{1}} > 400$ GeV and the $\mathrm{SR}^{\gamma\gamma}_{W-L}$ analysis for $m_{\tilde{\chi}^{0}_{1}}$ < 400$ GeV.

Observed exclusion limit in the wino-bino mass plane, using the $\mathrm{SR}^{\gamma\gamma}_{W-H}$ analysis for $m_{\tilde{\chi}^{0}_{1}} > 400$ GeV and the $\mathrm{SR}^{\gamma\gamma}_{W-L}$ analysis for $m_{\tilde{\chi}^{0}_{1}}$ < 400$ GeV.

Expected exclusion limits for the $\mu > 0$ higgsino-bino GGM model explored by the photon+jets analysis.

Observed exclusion limits for the $\mu > 0$ higgsino-bino GGM model explored by the photon+jets analysis.

Distribution of the transverse momentum $p_{\mathrm{T}} (\ell\gamma\gamma)$ of events in the $\ell\gamma\gamma$ control region (except without a cut on $p_{\mathrm{T}} (\ell\gamma\gamma)$). Also shown is the expected contribution from various SM sources, including $W(\to\ell\nu) + \gamma\gamma$ production itself. The displayed uncertainties are a combination of those from all SM sources except $W(\to\ell\nu) + \gamma\gamma$ production, and include statistical and systematic uncertainties.

Distribution of $E_{\mathrm{T}}^{\mathrm{miss}}$ for diphoton events in a validation region defined by a requirement of $H_{\mathrm{T}} > 1750$ GeV. Also shown is the expected contribution from various SM sources, as well as their combined statistical and systematic uncertainties.

Distribution of $H_{\mathrm{T}}$ for diphoton events in a validation region defined by requirement of $E_{\mathrm{T}}^{\mathrm{miss}} > 100$ GeV. Also shown is the expected contribution from various SM sources, as well as their combined statistical and systematic uncertainties.

Distribution of $m_{\mathrm{eff}}$ for events satisfying all requirements $\mathrm{SR}^{\gamma j}_{H}$ save the $m_{\mathrm{eff}}$ requirement itself. Also shown is the expected contribution from various SM sources, and their combined statistical uncertainties.

Distribution of $m_{\mathrm{eff}}$ for events satisfying all requirements $\mathrm{SR}^{\gamma j}_{L}$ save the $m_{\mathrm{eff}}$ requirement itself. Also shown is the expected contribution from various SM sources, and their combined statistical uncertainties.

Derived exclusion limits for the gluino-bino GGM model explored by the diphoton analysis. For each point in the gluino-bino parameter space, the SR ($\mathrm{SR}^{\gamma\gamma}_{S-L}$ or $\mathrm{SR}^{\gamma\gamma}_{S-H}$) that provides the best expected sensitivity is used to estimate the exclusion likelihood. The model dependent upper limits on cross-section (fb) are shown by grey numbers for each signal point.

Derived exclusion limits for the squark-bino GGM model explored by the diphoton analysis. For each point in the squark-bino parameter space, the SR ($\mathrm{SR}^{\gamma\gamma}_{S-L}$ or $\mathrm{SR}^{\gamma\gamma}_{S-H}$) that provides the best expected sensitivity is used to estimate the exclusion likelihood. The model dependent upper limits on cross-section (fb) are shown by grey numbers for each signal point.

Derived exclusion limits for the wino-bino GGM model explored by the diphoton analysis. For each point in the wino-bino parameter space, the SR ($\mathrm{SR}^{\gamma\gamma}_{W-L}$ or $\mathrm{SR}^{\gamma\gamma}_{W-H}$) that provides the best expected sensitivity is used to estimate the exclusion likelihood. The model dependent upper limits on cross-section (fb) are shown by grey numbers for each signal point.

Derived exclusion limits for the $\mu > 0$ higgsino-bino GGM model explored by the photon+jets analysis. For each point in the higgsino-bino parameter space, the SR ($\mathrm{SR}^{\gamma j}_{L}$ or $\mathrm{SR}^{\gamma j}_{H}$) that provides the best expected sensitivity is used to estimate the exclusion likelihood. The model dependent upper limits on cross-section (fb) are shown by grey numbers for each signal point.

Derived exclusion limits for the gluino-bino GGM model explored by the diphoton analysis. For each point in the gluino-bino parameter space, the SR ($\mathrm{SR}^{\gamma\gamma}_{S-L}$ or $\mathrm{SR}^{\gamma\gamma}_{S-H}$) that provides the best expected sensitivity is used to estimate the exclusion likelihood. The labels indicate the best-expected signal region for each point, where SL and SH mean $\mathrm{SR}^{\gamma\gamma}_{S-L}$ and $\mathrm{SR}^{\gamma\gamma}_{S-H}$, respectively.

Derived exclusion limits for the squark-bino GGM model explored by the diphoton analysis. For each point in the squark-bino parameter space, the SR ($\mathrm{SR}^{\gamma\gamma}_{S-L}$ or $\mathrm{SR}^{\gamma\gamma}_{S-H}$) that provides the best expected sensitivity is used to estimate the exclusion likelihood. The labels indicate the best-expected signal region for each point, where SL and SH mean $\mathrm{SR}^{\gamma\gamma}_{S-L}$ and $\mathrm{SR}^{\gamma\gamma}_{S-H}$, respectively.

Derived exclusion limits for the wino--bino GGM model explored by the diphoton analysis. For each point in the wino-bino parameter space, the SR ($\mathrm{SR}^{\gamma\gamma}_{W-L}$ or $\mathrm{SR}^{\gamma\gamma}_{W-H}$) that provides the best expected sensitivity is used to estimate the exclusion likelihood. The labels indicate the best-expected signal region for each point, where WL and WH mean $\mathrm{SR}^{\gamma\gamma}_{W-L}$ and $\mathrm{SR}^{\gamma\gamma}_{W-H}$, respectively.

Derived exclusion limits for the $\mu > 0$ higgsino-bino GGM model explored by the photon+jets analysis. For each point in the higgsino-bino parameter space, the SR ($\mathrm{SR}^{\gamma j}_{L}$ or $\mathrm{SR}^{\gamma j}_{H}$) that provides the best expected sensitivity is used to estimate the exclusion likelihood. The labels indicate the best-expected signal region for each point, where L and H mean $\mathrm{SR}^{\gamma j}_{L}$ and $\mathrm{SR}^{\gamma j}_{H}$, respectively.

Acceptance and efficiency for $\mathrm{SR}^{\gamma\gamma}_{S-L}$ for the signal models of the gluino-bino GGM grid.

Acceptance and efficiency for $\mathrm{SR}^{\gamma\gamma}_{S-H}$ for the signal models of the gluino-bino GGM grid.

Acceptance and efficiency for $\mathrm{SR}^{\gamma\gamma}_{S-L}$ for the signal models of the squark-bino GGM grid.

Acceptance and efficiency for $\mathrm{SR}^{\gamma\gamma}_{S-H}$ for the signal models of the squark-bino GGM grid.

Acceptance and efficiency for $\mathrm{SR}^{\gamma\gamma}_{W-L}$ for the signal models of the wino-bino GGM grid.

Acceptance and efficiency for $\mathrm{SR}^{\gamma\gamma}_{W-H}$ for the signal models of the wino-bino GGM grid.

Acceptance and efficiency for $\mathrm{SR}^{\gamma j}_{L}$ for the signal models of the photon+jets GGM grid.

Acceptance and efficiency for $\mathrm{SR}^{\gamma j}_{H}$ for the signal models of the photon+jets GGM grid.

Cutflow for the $\mathrm{SR}^{\gamma\gamma}_{S-L}$ selection for one relevant signal point in the gluino-bino model, where the gluinos have mass of 1900 GeV and the $\tilde{\chi}^{0}_{1}$ has a mass of 300 GeV (10000 generated events). The numbers are normalized to a luminosity of 36.1 fb$^{-1}$.

Cutflow for the $\mathrm{SR}^{\gamma\gamma}_{S-H}$ selection for one relevant signal point in the gluino-bino model, where the gluinos have mass of 1900 GeV and the $\tilde{\chi}^{0}_{1}$ has a mass of 1700 GeV (10000 generated events). The numbers are normalized to a luminosity of 36.1 fb$^{-1}$.

Cutflow for the $\mathrm{SR}^{\gamma\gamma}_{S-L}$ selection for one relevant signal point in the squark-bino model, where the squarks have mass of 1700 GeV and the $\tilde{\chi}^{0}_{1}$ has a mass of 200 GeV (10000 generated events). The numbers are normalized to a luminosity of 36.1 fb$^{-1}$.

Cutflow for the $\mathrm{SR}^{\gamma\gamma}_{S-H}$ selection for one relevant signal point in the squark-bino model, where the squarks have mass of 1700 GeV and the $\tilde{\chi}^{0}_{1}$ has a mass of 1600 GeV (10000 generated events). The numbers are normalized to a luminosity of 36.1 fb$^{-1}$.

Cutflow for the $\mathrm{SR}^{\gamma\gamma}_{W-L}$ selection for one relevant signal point in the wino-bino model, where the winos have mass of 1000 GeV and the $\tilde{\chi}^{0}_{1}$ has a mass of 200 GeV (10000 generated events). The numbers are normalized to a luminosity of 36.1 fb$^{-1}$.

Cutflow for the $\mathrm{SR}^{\gamma\gamma}_{W-H}$ selection for one relevant signal point in the wino-bino model, where the winos have mass of 1000 GeV and the $\tilde{\chi}^{0}_{1}$ has a mass of 800 GeV (10000 generated events). The numbers are normalized to a luminosity of 36.1 fb$^{-1}$.

Cutflow for the $\mathrm{SR}^{\gamma j}_{L}$ selection, for two relevant signal points in the higgsino-bino model, where the gluinos have mass of 1974 GeV and the $\tilde{\chi}^{0}_{1}$ has a mass of 442 GeV (10000 generated events), and 652 GeV (10000 generated events). The numbers are normalized to a luminosity of 36.1 fb$^{-1}$.

Cutflow for the $\mathrm{SR}^{\gamma j}_{H}$ selection, for two relevant signal points in the higgsino-bino model, where the gluinos have mass of 1974 GeV and the $\tilde{\chi}^{0}_{1}$ has a mass of 1868 GeV (10000 generated events), and 1920 GeV (10000 generated events). The numbers are normalized to a luminosity of 36.1 fb$^{-1}$.

Observed and expected upper limits at 95% CL on the median product of the signal cross section and the branching fraction for the QBH decay to $e\mu$ as a function of threshold mass.

Cross section of QBH as a function of mass. The cross section includes the branching ratio of QBH decaying to $e\mu$.

Observed and expected upper limits at 95% CL on the product of the signal cross section and the branching fraction(B), assuming B=10% for the decay Z' to $e\mu$, as a function of m(Z').

Cross section of Z' as a function of mass. The cross sections include branching ratio $BR(Z' -> e \mu) = 10\%$

x_J distribution of incluisve dijets in pp collisions

x_J distribution of b-quark dijets in pp collisions

x_J distribution of incluisve dijets in PbPb collisions (0-10%)

x_J distribution of b-quark dijets in PbPb collisions (0-10%)

x_J distribution of incluisve dijets in PbPb collisions (10-30%)

x_J distribution of b-quark dijets in PbPb collisions (10-30%)

x_J distribution of incluisve dijets in PbPb collisions (30-100%)

x_J distribution of b-quark dijets in PbPb collisions (30-100%)

Mean x_J of incluisve dijets in pp and PbPb collisions vs. number of participants

Mean x_J of b-quark dijets in pp and PbPb collisions vs. numberof participants

Mean x_J of inclusive jets and b-quark dijets in PbPb collisions minus mean x_J in pp collisions vs. numberof participants

Reconstructed mtb distribution in data and for the background after the fit to the data in the signal region SR2. The statistical uncertainty on data points is calculated using assymetric Poisson confidence intervals.

Reconstructed mtb distribution in data and for the background after the fit to the data in the signal region SR3. The statistical uncertainty on data points is calculated using assymetric Poisson confidence intervals.

Reconstructed mtb distribution in data and for the background after the fit to the data in the validation region VR. The statistical uncertainty on data points is calculated using assymetric Poisson confidence intervals.

Regions of the non-universal G(221) parameter space excluded at 95% CL.

Number of expected $W^{\prime}_{\rm SSM}$, $W^{\prime}_{\rm NU}$, Standard Model background and observed events passing the optimal $m_{\rm T}$ threshold for each considered signal mass hypothesis. The expectations include the total statistical and systematic uncertainty added in quadrature. The yields and uncertainties are calculated before applying the statistical fitting procedure.

Acceptance for $W^{\prime}_{\rm SSM}$ as a function of the $W^{\prime}_{\rm SSM}$ mass, shown after successively applying selection at generator-level. The acceptance times efficiency is calculated with respect to all $W^{\prime}_{\rm SSM} \to \tau\nu$ events with a generated $\tau\nu$ mass above 120 GeV. The "selected tau" criteria include the requirement of a $\tau_{\rm had-vis}$ with $p_{\rm T}$ > 50 GeV and $|\eta|$ < 2.4. The $m_{\rm T}$ threshold for each $W^{\prime}_{\rm SSM}$ mass is defined in Table 5.

Acceptance times efficiency for $W^{\prime}_{\rm SSM}$ as a function of the $W^{\prime}_{\rm SSM}$ mass, shown after successively applying selection at reconstruction-level. The acceptance times efficiency is calculated with respect to all $W^{\prime}_{\rm SSM} \to \tau\nu$ events with a generated $\tau\nu$ mass above 120 GeV. "Preselection" includes all criteria prior to those shown. The $m_{\rm T}$ threshold for each $W^{\prime}_{\rm SSM}$ mass is defined in Table 5.

Reconstruction efficiency as a function of $m_{\rm T}$ (see HepData abstract for parameterization), defined as the ratio of the number of $\tau\nu$ events remaining after applying the full selection at reconstruction-level to those remaining after applying the fiducial selection at generator-level. The efficiency is largely model independent, with an uncertainty of ~10% due to model choice.

$\xi^\mathrm{jet}$ distributions for jets associated with an isolated photon in pp and 0-10% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\mathrm{jet}$ distributions for 50-100% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\mathrm{jet}$ distributions for 30-50% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\mathrm{jet}$ distributions for 10-30% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\mathrm{jet}$ distributions for 0-10% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

$\xi^\gamma_{\mathrm{T}}$ distributions for jets associated with an isolated photon in pp and 50-100% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

$\xi^\gamma_{\mathrm{T}}$ distributions for jets associated with an isolated photon in pp and 30-50% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

$\xi^\gamma_{\mathrm{T}}$ distributions for jets associated with an isolated photon in pp and 10-30% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

$\xi^\gamma_{\mathrm{T}}$ distributions for jets associated with an isolated photon in pp and 0-10% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\gamma_{\mathrm{T}}$ distributions for 50-100% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\gamma_{\mathrm{T}}$ distributions for 30-50% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\gamma_{\mathrm{T}}$ distributions for 10-30% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\gamma_{\mathrm{T}}$ distributions for 0-10% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

$p_{T}^{t,2}$ absolute differential cross-section at particle level

$|{y}^{t,2}|$ absolute differential cross-section at particle level

$m^{t\bar{t}}$ absolute differential cross-section at particle level

$p_{T}^{t\bar{t}}$ absolute differential cross-section at particle level

$|y^{t\bar{t}}|$ absolute differential cross-section at particle level

$\chi^{t\bar{t}}$ absolute differential cross-section at particle level

$|y_{B}^{t\bar{t}}|$ absolute differential cross-section at particle level

$|p_{out}^{t\bar{t}}|$ absolute differential cross-section at particle level

$\Delta \phi(t_{1}, t_{2})$ absolute differential cross-section at particle level

$H_{T}^{t\bar{t}}$ absolute differential cross-section at particle level

$|\cos\theta^{*}|$ absolute differential cross-section at particle level

$p_{T}^{t,1}$ normalized differential cross-section at particle level

$|{y}^{t,1}|$ normalized differential cross-section at particle level

$p_{T}^{t,2}$ normalized differential cross-section at particle level

$|{y}^{t,2}|$ normalized differential cross-section at particle level

$m^{t\bar{t}}$ normalized differential cross-section at particle level

$p_{T}^{t\bar{t}}$ normalized differential cross-section at particle level

$|y^{t\bar{t}}|$ normalized differential cross-section at particle level

$\chi^{t\bar{t}}$ normalized differential cross-section at particle level

$|y_{B}^{t\bar{t}}|$ normalized differential cross-section at particle level

$|p_{out}^{t\bar{t}}|$ normalized differential cross-section at particle level

$\Delta \phi(t_{1}, t_{2})$ normalized differential cross-section at particle level

$H_{T}^{t\bar{t}}$ normalized differential cross-section at particle level

$|\cos\theta^{*}|$ normalized differential cross-section at particle level

$p_{T}^{t,1}$ covariance matrix for the absolute differential cross-section at particle level

$p_{T}^{t,1}$ correlation matrix for the absolute differential cross-section at particle level

$p_{T}^{t,1}$ covariance matrix for the normalized differential cross-section at particle level

$p_{T}^{t,1}$ correlation matrix for the normalized differential cross-section at particle level

$|{y}^{t,1}|$ covariance matrix for the absolute differential cross-section at particle level

$|{y}^{t,1}|$ correlation matrix for the absolute differential cross-section at particle level

$|{y}^{t,1}|$ covariance matrix for the normalized differential cross-section at particle level

$|{y}^{t,1}|$ correlation matrix for the normalized differential cross-section at particle level

$p_{T}^{t,2}$ covariance matrix for the absolute differential cross-section at particle level

$p_{T}^{t,2}$ correlation matrix for the absolute differential cross-section at particle level

$p_{T}^{t,2}$ covariance matrix for the normalized differential cross-section at particle level

$p_{T}^{t,2}$ correlation matrix for the normalized differential cross-section at particle level

$|{y}^{t,2}|$ covariance matrix for the absolute differential cross-section at particle level

$|{y}^{t,2}|$ correlation matrix for the absolute differential cross-section at particle level

$|{y}^{t,2}|$ covariance matrix for the normalized differential cross-section at particle level

$|{y}^{t,2}|$ correlation matrix for the normalized differential cross-section at particle level

$m^{t\bar{t}}$ covariance matrix for the absolute differential cross-section at particle level

$m^{t\bar{t}}$ correlation matrix for the absolute differential cross-section at particle level

$m^{t\bar{t}}$ covariance matrix for the normalized differential cross-section at particle level

$m^{t\bar{t}}$ correlation matrix for the normalized differential cross-section at particle level

$p_{T}^{t\bar{t}}$ covariance matrix for the absolute differential cross-section at particle level

$p_{T}^{t\bar{t}}$ correlation matrix for the absolute differential cross-section at particle level

$p_{T}^{t\bar{t}}$ covariance matrix for the normalized differential cross-section at particle level

$p_{T}^{t\bar{t}}$ correlation matrix for the normalized differential cross-section at particle level

$|y^{t\bar{t}}|$ covariance matrix for the absolute differential cross-section at particle level

$|y^{t\bar{t}}|$ correlation matrix for the absolute differential cross-section at particle level

$|y^{t\bar{t}}|$ covariance matrix for the normalized differential cross-section at particle level

$|y^{t\bar{t}}|$ correlation matrix for the normalized differential cross-section at particle level

$\chi^{t\bar{t}}$ covariance matrix for the absolute differential cross-section at particle level

$\chi^{t\bar{t}}$ correlation matrix for the absolute differential cross-section at particle level

$\chi^{t\bar{t}}$ covariance matrix for the normalized differential cross-section at particle level

$\chi^{t\bar{t}}$ correlation matrix for the normalized differential cross-section at particle level

$|y_{B}^{t\bar{t}}|$ covariance matrix for the absolute differential cross-section at particle level

$|y_{B}^{t\bar{t}}|$ correlation matrix for the absolute differential cross-section at particle level

$|y_{B}^{t\bar{t}}|$ covariance matrix for the normalized differential cross-section at particle level

$|y_{B}^{t\bar{t}}|$ correlation matrix for the normalized differential cross-section at particle level

$|p_{out}^{t\bar{t}}|$ covariance matrix for the absolute differential cross-section at particle level

$|p_{out}^{t\bar{t}}|$ correlation matrix for the absolute differential cross-section at particle level

$|p_{out}^{t\bar{t}}|$ covariance matrix for the normalized differential cross-section at particle level

$|p_{out}^{t\bar{t}}|$ correlation matrix for the normalized differential cross-section at particle level

$\Delta \phi(t_{1}, t_{2})$ covariance matrix for the absolute differential cross-section at particle level

$\Delta \phi(t_{1}, t_{2})$ correlation matrix for the absolute differential cross-section at particle level

$\Delta \phi(t_{1}, t_{2})$ covariance matrix for the normalized differential cross-section at particle level

$\Delta \phi(t_{1}, t_{2})$ correlation matrix for the normalized differential cross-section at particle level

$H_{T}^{t\bar{t}}$ covariance matrix for the absolute differential cross-section at particle level

$H_{T}^{t\bar{t}}$ correlation matrix for the absolute differential cross-section at particle level

$H_{T}^{t\bar{t}}$ covariance matrix for the normalized differential cross-section at particle level

$H_{T}^{t\bar{t}}$ correlation matrix for the normalized differential cross-section at particle level

$|\cos\theta^{*}|$ covariance matrix for the absolute differential cross-section at particle level

$|\cos\theta^{*}|$ correlation matrix for the absolute differential cross-section at particle level

$|\cos\theta^{*}|$ covariance matrix for the normalized differential cross-section at particle level

$|\cos\theta^{*}|$ correlation matrix for the normalized differential cross-section at particle level

Statistical correlation matrix for the absolute differential cross-section of all 13 variables at particle level. The observables are arranged as follows: leading top pT - ${p_{{T}}}^{t,1}$ [bins 1-8], leading top rapidity - $|y^{t,1}|$ [bins 9-14], subleading top pT - ${p_{{T}}}^{t,2}$ [bins 15-21], subleading top rapidity - $|y^{t,2}|$ [bins 22-27], ttbar mass - $m^{t\bar{t}}$ [bins 28-37], ttbar pT - ${p_{{T}}}^{t\bar{t}}$ [bins 38-43], ttbar rapidity - $|y^{t\bar{t}}|$ [bins 44-49], chi ttbar - ${\chi}^{t\bar{t}}$ [bins 50-56], delta phi ttbar - ${\Delta\phi}(t_1,t_2)$ [bins 57-60], ttbar out of plane momentum - $|p_{out}^{t\bar{t}}|$ [bins 61-67], yboost ttbar - $|y_{B}^{t\bar{t}}|$ [68-74], cos theta star - $|{\cos{\theta}^{\star}}|$ [bins 75-80], HT ttbar - $H_{T}^{t\bar{t}}$ [bins 81-87].

Statistical correlation matrix for the normalized differential cross-section of all 13 variables at particle level. The observables are arranged as follows: leading top pT - ${p_{{T}}}^{t,1}$ [bins 1-8], leading top rapidity - $|y^{t,1}|$ [bins 9-14], subleading top pT - ${p_{{T}}}^{t,2}$ [bins 15-21], subleading top rapidity - $|y^{t,2}|$ [bins 22-27], ttbar mass - $m^{t\bar{t}}$ [bins 28-37], ttbar pT - ${p_{{T}}}^{t\bar{t}}$ [bins 38-43], ttbar rapidity - $|y^{t\bar{t}}|$ [bins 44-49], chi ttbar - ${\chi}^{t\bar{t}}$ [bins 50-56], delta phi ttbar - ${\Delta\phi}(t_1,t_2)$ [bins 57-60], ttbar out of plane momentum - $|p_{out}^{t\bar{t}}|$ [bins 61-67], yboost ttbar - $|y_{B}^{t\bar{t}}|$ [68-74], cos theta star - $|{\cos{\theta}^{\star}}|$ [bins 75-80], HT ttbar - $H_{T}^{t\bar{t}}$ [bins 81-87].

${p_{{T}}}^{t}$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|y^{t}|$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${p_{{T}}}^{t,1}$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|y^{t,1}|$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${p_{{T}}}^{t,2}$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{y}^{t,2}|$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$m^{t\bar{t}}$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${p_{{T}}}^{t\bar{t}}$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{y}^{t\bar{t}}|$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${\chi}^{t\bar{t}}$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{y_{B}}^{t\bar{t}}|$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{p_{out}}^{t\bar{t}}|$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${\Delta\phi}(t_1,t_2)$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${H_{T}}^{t\bar{t}}$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{\cos{\theta}^{\star}}|$ absolute differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${p_{{T}}}^{t}$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|y^{t}|$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${p_{{T}}}^{t,1}$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|y^{t,1}|$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${p_{{T}}}^{t,2}$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{y}^{t,2}|$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$m^{t\bar{t}}$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${p_{{T}}}^{t\bar{t}}$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{y}^{t\bar{t}}|$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${\chi}^{t\bar{t}}$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{y_{B}}^{t\bar{t}}|$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{p_{out}}^{t\bar{t}}|$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${\Delta\phi}(t_1,t_2)$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$H_{T}^{t\bar{t}}$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

$|{\cos{\theta}^{\star}}|$ normalized differential cross-section at parton level. The parton level phase-space is limited to the region $p_T^{t,1} > 500~$GeV, $p_T^{t,2} > 350~$GeV.

${p_{{T}}}^{t}$ covariance matrix for the absolute differential cross-section at parton level

${p_{{T}}}^{t}$ correlation matrix for the absolute differential cross-section at parton level

${p_{{T}}}^{t}$ covariance matrix for the normalized differential cross-section at parton level

${p_{{T}}}^{t}$ correlation matrix for the normalized differential cross-section at parton level

$|y^{t}|$ covariance matrix for the absolute differential cross-section in parton level

$|y^{t}|$ correlation matrix for the absolute differential cross-section at parton level

$|y^{t}|$ covariance matrix for the normalized differential cross-section in parton level

$|y^{t}|$ correlation matrix for the normalized differential cross-section at parton level

${p_{{T}}}^{t,1}$ covariance matrix for the absolute differential cross-section at parton level

${p_{{T}}}^{t,1}$ correlation matrix for the absolute differential cross-section at parton level

${p_{{T}}}^{t,1}$ covariance matrix for the normalized differential cross-section at parton level

${p_{{T}}}^{t,1}$ correlation matrix for the normalized differential cross-section at parton level

$|y^{t,1}|$ covariance matrix for the absolute differential cross-section at parton level

$|y^{t,1}|$ correlation matrix for the absolute differential cross-section at parton level

$|y^{t,1}|$ covariance matrix for the normalized differential cross-section at parton level

$|y^{t,1}|$ correlation matrix for the normalized differential cross-section at parton level

${p_{{T}}}^{t,2}$ covariance matrix for the absolute differential cross-section at parton level

${p_{{T}}}^{t,2}$ correlation matrix for the absolute differential cross-section at parton level

${p_{{T}}}^{t,2}$ covariance matrix for the normalized differential cross-section at parton level

${p_{{T}}}^{t,2}$ correlation matrix for the normalized differential cross-section at parton level

$|{y}^{t,2}|$ covariance matrix for the absolute differential cross-section at parton level

$|{y}^{t,2}|$ correlation matrix for the absolute differential cross-section at parton level

$|{y}^{t,2}|$ covariance matrix for the normalized differential cross-section at parton level

$|{y}^{t,2}|$ correlation matrix for the normalized differential cross-section at parton level

$m^{t\bar{t}}$ covariance matrix for the absolute differential cross-section at parton level

$m^{t\bar{t}}$ correlation matrix for the absolute differential cross-section at parton level

$m^{t\bar{t}}$ covariance matrix for the normalized differential cross-section at parton level

$m^{t\bar{t}}$ correlation matrix for the normalized differential cross-section at parton level

${p_{{T}}}^{t\bar{t}}$ covariance matrix for the absolute differential cross-section at parton level

${p_{{T}}}^{t\bar{t}}$ correlation matrix for the absolute differential cross-section at parton level

${p_{{T}}}^{t\bar{t}}$ covariance matrix for the normalized differential cross-section at parton level

${p_{{T}}}^{t\bar{t}}$ correlation matrix for the normalized differential cross-section at parton level

$|{y}^{t\bar{t}}|$ covariance matrix for the absolute differential cross-section at parton level

$|{y}^{t\bar{t}}|$ correlation matrix for the absolute differential cross-section at parton level

$|{y}^{t\bar{t}}|$ covariance matrix for the normalized differential cross-section at parton level

$|{y}^{t\bar{t}}|$ correlation matrix for the normalized differential cross-section at parton level

${\chi}^{t\bar{t}}$ covariance matrix for the absolute differential cross-section at parton level

${\chi}^{t\bar{t}}$ correlation matrix for the absolute differential cross-section at parton level

${\chi}^{t\bar{t}}$ covariance matrix for the normalized differential cross-section at parton level

${\chi}^{t\bar{t}}$ correlation matrix for the normalized differential cross-section at parton level

$|{y_{B}}^{t\bar{t}}|$ covariance matrix for the absolute differential cross-section at parton level

$|{y_{B}}^{t\bar{t}}|$ correlation matrix for the absolute differential cross-section at parton level

$|{y_{B}}^{t\bar{t}}|$ covariance matrix for the normalized differential cross-section at parton level

$|{y_{B}}^{t\bar{t}}|$ correlation matrix for the normalized differential cross-section at parton level

$|{p_{out}}^{t\bar{t}}|$ covariance matrix for the absolute differential cross-section at parton level

$|{p_{out}}^{t\bar{t}}|$ correlation matrix for the absolute differential cross-section at parton level

$|{p_{out}}^{t\bar{t}}|$ covariance matrix for the normalized differential cross-section at parton level

$|{p_{out}}^{t\bar{t}}|$ correlation matrix for the normalized differential cross-section at parton level

${\Delta\phi}(t_1,t_2)$ covariance matrix for the absolute differential cross-section at parton level

${\Delta\phi}(t_1,t_2)$ correlation matrix for the absolute differential cross-section at parton level

${\Delta\phi}(t_1,t_2)$ covariance matrix for the normalized differential cross-section at parton level

${\Delta\phi}(t_1,t_2)$ correlation matrix for the normalized differential cross-section at parton level

$H_{T}^{t\bar{t}}$ covariance matrix for the absolute differential cross-section at parton level

$H_{T}^{t\bar{t}}$ correlation matrix for the absolute differential cross-section at parton level

$H_{T}^{t\bar{t}}$ covariance matrix for the normalized differential cross-section at parton level

$H_{T}^{t\bar{t}}$ correlation matrix for the normalized differential cross-section at parton level

$|{\cos{\theta}^{\star}}|$ covariance matrix for the absolute differential cross-section at parton level

$|{\cos{\theta}^{\star}}|$ correlation matrix for the absolute differential cross-section at parton level

$|{\cos{\theta}^{\star}}|$ covariance matrix for the normalized differential cross-section at parton level

$|{\cos{\theta}^{\star}}|$ correlation matrix for the normalized differential cross-section at parton level

Statistical correlation matrix for the absolute differential cross-section of all 15 variables at parton level. The observables are arranged as follows: random top pT - ${p_{{T}}}^{t}$ [bins 1-8], random top rapidity - $|y^{t}|$ [bins 9-16], leading top pT - ${p_{{T}}}^{t,1}$ [bins 17-24], leading top rapidity - $|y^{t,1}|$ [bins 25-32], subleading top pT - ${p_{{T}}}^{t,2}$ [bins 33-39], subleading top rapidity - $|y^{t,2}|$ [bins 40-46], ttbar mass - $m^{t\bar{t}}$ [bins 48-57], ttbar pT - ${p_{{T}}}^{t\bar{t}}$ [bins 58-63], ttbar rapidity - $|y^{t\bar{t}}|$ [bins 66-71], chi ttbar ${\chi}^{t\bar{t}}$ - [bins 74-80], delta phi ttbar - ${\Delta\phi}(t_1,t_2)$ [bins 81-84], ttbar out of plane momentum - $|p_{out}^{t\bar{t}}|$ [bins 85-91], yboost ttbar - $|y_{B}^{t\bar{t}}|$ [92-98], cos theta star - $|{\cos{\theta}^{\star}}|$ [bins 99-104], HT ttbar $H_{T}^{t\bar{t}}$ [bins 105-114].

Statistical correlation matrix for the normalized differential cross-section of all 15 variables at parton level. The observables are arranged as follows: random top pT - ${p_{{T}}}^{t}$ [bins 1-8], random top rapidity - $|y^{t}|$ [bins 9-16], leading top pT - ${p_{{T}}}^{t,1}$ [bins 17-24], leading top rapidity - $|y^{t,1}|$ [bins 25-32], subleading top pT - ${p_{{T}}}^{t,2}$ [bins 33-39], subleading top rapidity - $|y^{t,2}|$ [bins 40-46], ttbar mass - $m^{t\bar{t}}$ [bins 48-57], ttbar pT - ${p_{{T}}}^{t\bar{t}}$ [bins 58-63], ttbar rapidity - $|y^{t\bar{t}}|$ [bins 66-71], chi ttbar ${\chi}^{t\bar{t}}$ - [bins 74-80], delta phi ttbar - ${\Delta\phi}(t_1,t_2)$ [bins 81-84], ttbar out of plane momentum - $|p_{out}^{t\bar{t}}|$ [bins 85-91],yboost ttbar - $|y_{B}^{t\bar{t}}|$ [92-98], cos theta star - $|{\cos{\theta}^{\star}}|$ [bins 99-104], HT ttbar $H_{T}^{t\bar{t}}$ [bins 105-114].