Combined search for electroweak production of winos, binos, higgsinos, and sleptons in proton-proton collisions at $\sqrt{s}$ = 13 TeV

The CMS collaboration Hayrapetyan, Aram ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
CMS-SUS-21-008, 2024.
Inspire Record 2755433 DOI 10.17182/hepdata.145859

A combination of the results of several searches for the electroweak production of the supersymmetric partners of standard model bosons, and of charged leptons, is presented. All searches use proton-proton collision data at $\sqrt{s}$ = 13 TeV recorded with the CMS detector at the LHC in 2016-2018. The analyzed data correspond to an integrated luminosity of up to 137 fb$^{-1}$. The results are interpreted in terms of simplified models of supersymmetry. Two new interpretations are added with this combination: a model spectrum with the bino as the lightest supersymmetric particle together with mass-degenerate higgsinos decaying to the bino and a standard model boson, and the compressed-spectrum region of a previously studied model of slepton pair production. Improved analysis techniques are employed to optimize sensitivity for the compressed spectra in the wino and slepton pair production models. The results are consistent with expectations from the standard model. The combination provides a more comprehensive coverage of the model parameter space than the individual searches, extending the exclusion by up to 125 GeV, and also targets some of the intermediate gaps in the mass coverage.

0 data tables

Version 2
Search for long-lived particles using out-of-time trackless jets in proton-proton collisions at $\sqrt{s}$ = 13 TeV

The CMS collaboration Tumasyan, Armen ; Adam, Wolfgang ; Andrejkovic, Janik Walter ; et al.
JHEP 07 (2023) 210, 2023.
Inspire Record 2613855 DOI 10.17182/hepdata.135827

A search for long-lived particles decaying in the outer regions of the CMS silicon tracker or in the calorimeters is presented. The search is based on a data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the CMS detector at the LHC in 2016-2018, corresponding to an integrated luminosity of 138 fb$^{-1}$. A novel technique, using trackless and out-of-time jet information combined in a deep neural network discriminator, is employed to identify decays of long-lived particles. The results are interpreted in a simplified model of chargino-neutralino production, where the neutralino is the next-to-lightest supersymmetric particle, is long-lived, and decays to a gravitino and either a Higgs or Z boson. This search is most sensitive to neutralino proper decay lengths of approximately 0.5 m, for which masses up to 1.18 TeV are excluded at 95% confidence level. The current search is the best result to date in the mass range from the kinematic limit imposed by the Higgs mass up to 1.8 TeV.

20 data tables

Summary of combined statistical and systematic uncertainties, the size of their effect, and whether it applies to the signal or background yield predictions. Ranges for signal systematic uncertainties reflect their impact on different signal parameter space points.

Feynman diagrams of the effective neutralino pair production in the GMSB simplified model in which the two neutralinos decay into two gravitinos ($\tilde{G}$) and two $Z$ bosons (left), a $Z$ and a Higgs boson ($H$) (center), or two Higgs bosons (right).

Feynman diagrams of the effective neutralino pair production in the GMSB simplified model in which the two neutralinos decay into two gravitinos ($\tilde{G}$) and two $Z$ bosons (left), a $Z$ and a Higgs boson ($H$) (center), or two Higgs bosons (right).

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Version 2
Search for electroweak production of charginos and neutralinos at $\sqrt{s}$ =13 TeV in final states containing hadronic decays of WW, WZ, or WH and missing transverse momentum

The CMS collaboration Tumasyan, Armen ; Adam, Wolfgang ; Andrejkovic, Janik Walter ; et al.
Phys.Lett.B 842 (2023) 137460, 2023.
Inspire Record 2085373 DOI 10.17182/hepdata.127766

This Letter presents a search for direct production of charginos and neutralinos via electroweak interactions. The results are based on data from proton-proton collisions at a center-of-mass energy of 13 TeV collected with the CMS detector at the LHC, corresponding to an integrated luminosity of 137 fb$^{-1}$. The search considers final states with large missing transverse momentum and pairs of hadronically decaying bosons WW, WZ, and WH, where H is the Higgs boson. These bosons are identified using novel algorithms. No significant excess of events is observed relative to the expectations from the standard model. Limits at the 95% confidence level are placed on the cross section for production of mass-degenerate wino-like supersymmetric particles $\tilde{\chi}_1^\pm$ and $\tilde{\chi}_2^0$, and mass-degenerate higgsino-like supersymmetric particles $\tilde{\chi}_1^\pm$, $\tilde{\chi}_2^0$, and $\tilde{\chi}_3^0$. In the limit of a nearly-massless lightest supersymmetric particle $\tilde{\chi}_1^0$, wino-like particles with masses up to 870 and 960 GeV are excluded in the cases of $\tilde{\chi}_2^0$ $\to$ Z$\tilde{\chi}_1^0$ and $\tilde{\chi}_2^0$ $\to$ H$\tilde{\chi}_1^0$, respectively, and higgsino-like particles are excluded between 300 and 650 GeV.

0 data tables

Version 3
Search for higgsinos decaying to two Higgs bosons and missing transverse momentum in proton-proton collisions at $\sqrt{s}$ = 13 TeV

The CMS collaboration Tumasyan, Armen ; Adam, Wolfgang ; Andrejkovic, Janik Walter ; et al.
JHEP 05 (2022) 014, 2022.
Inspire Record 2009652 DOI 10.17182/hepdata.114414

Results are presented from a search for physics beyond the standard model in proton-proton collisions at $\sqrt{s} =$ 13 TeV in channels with two Higgs bosons, each decaying via the process H $\to$$\mathrm{b\bar{b}}$, and large missing transverse momentum. The search uses a data sample corresponding to an integrated luminosity of 137 fb$^{-1}$ collected by the CMS experiment at the CERN LHC. The search is motivated by models of supersymmetry that predict the production of neutralinos, the neutral partners of the electroweak gauge and Higgs bosons. The observed event yields in the signal regions are found to be consistent with the standard model background expectations. The results are interpreted using simplified models of supersymmetry. For the electroweak production of nearly mass-degenerate higgsinos, each of whose decay chains yields a neutralino ($\tilde{\chi}^0_1$) that in turn decays to a massless goldstino and a Higgs boson, $\tilde{\chi}^0_1$ masses in the range 175 to 1025 GeV are excluded at 95% confidence level. For the strong production of gluino pairs decaying via a slightly lighter $\tilde{\chi}^0_2$ to H and a light $\tilde{\chi}^0_1$, gluino masses below 2330 GeV are excluded.

0 data tables

Search for supersymmetry in final states with two or three soft leptons and missing transverse momentum in proton-proton collisions at $\sqrt{s} =$ 13 TeV

The CMS collaboration Tumasyan, Armen ; Adam, Wolfgang ; Andrejkovic, Janik Walter ; et al.
JHEP 04 (2022) 091, 2022.
Inspire Record 1966342 DOI 10.17182/hepdata.114415

A search for supersymmetry in events with two or three low-momentum leptons and missing transverse momentum is performed. The search uses proton-proton collisions at $\sqrt{s} =$ 13 TeV collected in the three-year period 2016-2018 by the CMS experiment at the LHC and corresponding to an integrated luminosity of up to 137 fb$^{-1}$. The data are found to be in agreement with expectations from standard model processes. The results are interpreted in terms of electroweakino and top squark pair production with a small mass difference between the produced supersymmetric particles and the lightest neutralino. For the electroweakino interpretation, two simplified models are used, a wino-bino model and a higgsino model. Exclusion limits at 95% confidence level are set on $\widetilde{\chi}^0_2 / \widetilde{\chi}^\pm_1$ masses up to 275 GeV for a mass difference of 10 GeV in the wino-bino case, and up to 205 (150) GeV for a mass difference of 7.5 (3) GeV in the higgsino case. The results for the higgsino are further interpreted using a phenomenological minimal supersymmetric standard model, excluding the higgsino mass parameter $\mu$ up to 180 GeV with the bino mass parameter $M_1$ at 800 GeV. In the top squark interpretation, exclusion limits are set at top squark masses up to 540 GeV for four-body top squark decays and up to 480 GeV for chargino-mediated decays with a mass difference of 30 GeV.

23 data tables

The post-fit distribution of the $M(\ell\ell)$ variable is shown for the low-MET bin for the DY CR. Uncertainties include both the statistical and systematic components.

The post-fit distribution of the $M(\ell\ell)$ variable is shown for the high-MET bin for the DY CR. Uncertainties include both the statistical and systematic components.

The post-fit distribution of the $M(\ell\ell)$ variable is shown for the low-MET bin for the $\text{t}\bar{\text{t}}$ CR. Uncertainties include both the statistical and systematic components.

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Search for supersymmetry in events with four or more charged leptons in $139\,\textrm{fb}^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collisions with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Braden Keim ; Abbott, Dale ; et al.
JHEP 07 (2021) 167, 2021.
Inspire Record 1852821 DOI 10.17182/hepdata.103062

A search for supersymmetry in events with four or more charged leptons (electrons, muons and $\tau$-leptons) is presented. The analysis uses a data sample corresponding to $139\,\mbox{fb\(^{-1}\)}$ of proton-proton collisions delivered by the Large Hadron Collider at $\sqrt{s}=13$ TeV and recorded by the ATLAS detector. Four-lepton signal regions with up to two hadronically decaying $\tau$-leptons are designed to target several supersymmetric models, while a general five-lepton signal region targets any new physics phenomena leading to a final state with five charged leptons. Data yields are consistent with Standard Model expectations and results are used to set upper limits on contributions from processes beyond the Standard Model. Exclusion limits are set at the 95% confidence level in simplified models of general gauge-mediated supersymmetry, excluding higgsino masses up to $540$ GeV. In $R$-parity-violating simplified models with decays of the lightest supersymmetric particle to charged leptons, lower limits of $1.6$ TeV, $1.2$ TeV, and $2.5$ TeV are placed on wino, slepton and gluino masses, respectively.

83 data tables

The $E_{\mathrm{T}}^{\mathrm{miss}}$ distribution in SR0-ZZ$^{\mathrm{loose}}$ and SR0-ZZ$^{\mathrm{tight}}$ for events passing the signal region requirements except the $E_{\mathrm{T}}^{\mathrm{miss}}$ requirement. Distributions for data, the estimated SM backgrounds after the background-only fit, and an example SUSY scenario are shown. "Other" is the sum of the $tWZ$, $t\bar{t}WW$, $t\bar{t} ZZ$, $t\bar{t} WH$, $t\bar{t} HH$, $t\bar{t} tW$, and $t\bar{t}t\bar{t}$ backgrounds. The last bin captures the overflow events. The lower panel shows the ratio of the observed data to the expected SM background yield in each bin. Both the statistical and systematic uncertainties in the SM background are included in the shaded band. The red arrows indicate the $E_{\mathrm{T}}^{\mathrm{miss}}$ selections in the signal regions.

The $E_{\mathrm{T}}^{\mathrm{miss}}$ distribution in SR0-ZZ$_{\mathrm{bveto}}^{\mathrm{loose}}$ and SR0-ZZ$_{\mathrm{bveto}}^{\mathrm{tight}}$ for events passing the signal region requirements except the $E_{\mathrm{T}}^{\mathrm{miss}}$ requirement. Distributions for data, the estimated SM backgrounds after the background-only fit, and an example SUSY scenario are shown. "Other" is the sum of the $tWZ$, $t\bar{t}WW$, $t\bar{t} ZZ$, $t\bar{t} WH$, $t\bar{t} HH$, $t\bar{t} tW$, and $t\bar{t}t\bar{t}$ backgrounds. The last bin captures the overflow events. The lower panel shows the ratio of the observed data to the expected SM background yield in each bin. Both the statistical and systematic uncertainties in the SM background are included in the shaded band. The red arrows indicate the $E_{\mathrm{T}}^{\mathrm{miss}}$ selections in the signal regions.

The $E_{\mathrm{T}}^{\mathrm{miss}}$ distribution in SR5L. Distributions for data, the estimated SM backgrounds after the background-only fit, and an example SUSY scenario are shown. "Other" is the sum of the $tWZ$, $t\bar{t}WW$, $t\bar{t} ZZ$, $t\bar{t} WH$, $t\bar{t} HH$, $t\bar{t} tW$, and $t\bar{t}t\bar{t}$ backgrounds. The last bin captures the overflow events. The lower panel shows the ratio of the observed data to the expected SM background yield in each bin. Both the statistical and systematic uncertainties in the SM background are included in the shaded band.

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Search for bottom-squark pair production in $pp$ collision events at $\sqrt{s} = 13$ TeV with hadronically decaying $\tau$-leptons, $b$-jets and missing transverse momentum using the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Braden Keim ; Abbott, Brad ; et al.
Phys.Rev.D 104 (2021) 032014, 2021.
Inspire Record 1851675 DOI 10.17182/hepdata.99788

A search for pair production of bottom squarks in events with hadronically decaying $\tau$-leptons, $b$-tagged jets and large missing transverse momentum is presented. The analyzed dataset is based on proton-proton collisions at $\sqrt{s}$ = 13 TeV delivered by the Large Hadron Collider and recorded by the ATLAS detector from 2015 to 2018, and corresponds to an integrated luminosity of 139 fb$^{-1}$. The observed data are compatible with the expected Standard Model background. Results are interpreted in a simplified model where each bottom squark is assumed to decay into the second-lightest neutralino $\tilde \chi_2^0$ and a bottom quark, with $\tilde \chi_2^0$ decaying into a Higgs boson and the lightest neutralino $\tilde \chi_1^0$. The search focuses on final states where at least one Higgs boson decays into a pair of hadronically decaying $\tau$-leptons. This allows the acceptance and thus the sensitivity to be significantly improved relative to the previous results at low masses of the $\tilde \chi_2^0$, where bottom-squark masses up to 850 GeV are excluded at the 95% confidence level, assuming a mass difference of 130 GeV between $\tilde \chi_2^0$ and $\tilde \chi_1^0$. Model-independent upper limits are also set on the cross section of processes beyond the Standard Model.

15 data tables

The expected exclusion contour at $95\%$ CL as a function of the M(Sbottom) vs. M(N2) with the $\Delta M$(N2,N1) = 130 GeV. Masses within the contour are excluded.

The observed exclusion contour at $95\%$ CL as a function of the M(Sbottom) vs. M(N2) with the $\Delta M$(N2,N1) = 130 GeV. Masses within the contour are excluded.

Acceptance in the Single-bin SR as a function of the M(Sbottom) vs. M(N2) with the $\Delta M$(N2,N1) = 130 GeV. Keep in mind that the acceptance is given in units of $10^{-4}$.

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Search for top squark production in fully-hadronic final states in proton-proton collisions at $\sqrt{s} =$ 13 TeV

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
Phys.Rev.D 104 (2021) 052001, 2021.
Inspire Record 1849522 DOI 10.17182/hepdata.103065

A search for production of the supersymmetric partners of the top quark, top squarks, is presented. The search is based on proton-proton collision events containing multiple jets, no leptons, and large transverse momentum imbalance. The data were collected with the CMS detector at the CERN LHC at a center-of-mass energy of 13 TeV, and correspond to an integrated luminosity of 137 fb$^{-1}$. The targeted signal production scenarios are direct and gluino-mediated top squark production, including scenarios in which the top squark and neutralino masses are nearly degenerate. The search utilizes novel algorithms based on deep neural networks that identify hadronically decaying top quarks and W bosons, which are expected in many of the targeted signal models. No statistically significant excess of events is observed relative to the expectation from the standard model, and limits on the top squark production cross section are obtained in the context of simplified supersymmetric models for various production and decay modes. Exclusion limits as high as 1310 GeV are established at the 95% confidence level on the mass of the top squark for direct top squark production models, and as high as 2260 GeV on the mass of the gluino for gluino-mediated top squark production models. These results represent a significant improvement over the results of previous searches for supersymmetry by CMS in the same final state.

51 data tables

Top quark tagging efficiencies are shown as a function of the generator-level top quark $p_T$ for the merged tagging algorithm and resolved tagging algorithm described in the paper. This plot shows the efficiencies as calculated in a sample of simulated $t\bar{t}$ events in which one top quark decays leptonically, while the other decays hadronically. In addition to the individual algorithms shown as orange squares (boosted top quarks) and green inverted triangles (resolved top quarks), the total top quark tagging efficiency (blue dots) is also shown.

W boson tagging efficiencies are shown as a function of the generator-level W boson $p_T$ for the merged tagging algorithm described in the paper. This plot shows the W boson tagging efficiency when calculated in a sample of simulated WW events.

Comparison between data and simulation in the high $\Delta$m portion of the $\ell+\text{jets}$ control region as a function of $p_T^{miss}$ after scaling the simulation to match the total yield in data. The hatched region indicates the total shape uncertainty in the simulation.

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Search for new phenomena in events with two opposite-charge leptons, jets and missing transverse momentum in $pp$ collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
JHEP 04 (2021) 165, 2021.
Inspire Record 1844425 DOI 10.17182/hepdata.98627

The results of a search for direct pair production of top squarks and for dark matter in events with two opposite-charge leptons (electrons or muons), jets and missing transverse momentum are reported, using 139 fb$^{-1}$ of integrated luminosity from proton-proton collisions at $\sqrt{s} = 13$ TeV, collected by the ATLAS detector at the Large Hadron Collider during Run 2 (2015-2018). This search considers the pair production of top squarks and is sensitive across a wide range of mass differences between the top squark and the lightest neutralino. Additionally, spin-0 mediator dark-matter models are considered, in which the mediator is produced in association with a pair of top quarks. The mediator subsequently decays to a pair of dark-matter particles. No significant excess of events is observed above the Standard Model background, and limits are set at 95% confidence level. The results exclude top squark masses up to about 1 TeV, and masses of the lightest neutralino up to about 500 GeV. Limits on dark-matter production are set for scalar (pseudoscalar) mediator masses up to about 250 (300) GeV.

196 data tables

Two-body selection. Distributions of $m_{T2}$ in $SR^{2-body}_{110,\infty}$ for (a) different-flavour and (b) same-flavour events satisfying the selection criteria of the given SR, except the one for the presented variable, after the background fit. The contributions from all SM backgrounds are shown as a histogram stack. ''Others'' includes contributions from $VVV$, $t\bar{t} t$, $t\bar{t}$, $t\bar{t} W$, $t\bar{t} WW$, $t\bar{t} WZ$, $t\bar{t} H$, and $tZ$ processes. The hatched bands represent the total statistical and systematic uncertainty. The rightmost bin of each plot includes overflow events. Reference dark-matter signal models are overlayed for comparison. Red arrows in the upper panels indicate the signal region selection criteria. The bottom panels show the ratio of the observed data to the total SM background prediction, with hatched bands representing the total uncertainty in the background prediction.

Two-body selection. Distributions of $m_{T2}$ in $SR^{2-body}_{110,\infty}$ for (a) different-flavour and (b) same-flavour events satisfying the selection criteria of the given SR, except the one for the presented variable, after the background fit. The contributions from all SM backgrounds are shown as a histogram stack. ''Others'' includes contributions from $VVV$, $t\bar{t} t$, $t\bar{t}$, $t\bar{t} W$, $t\bar{t} WW$, $t\bar{t} WZ$, $t\bar{t} H$, and $tZ$ processes. The hatched bands represent the total statistical and systematic uncertainty. The rightmost bin of each plot includes overflow events. Reference dark-matter signal models are overlayed for comparison. Red arrows in the upper panels indicate the signal region selection criteria. The bottom panels show the ratio of the observed data to the total SM background prediction, with hatched bands representing the total uncertainty in the background prediction.

Three-body selection. Distributions of $M_{\Delta}^R$ in (a,b) $SR_{W}^{3-body}$ and (c,d) $SR_{T}^{3-body}$ for (left) same-flavour and (right) different-flavour events satisfying the selection criteria of the given SR, except the one for the presented variable, after the background fit. The contributions from all SM backgrounds are shown as a histogram stack. ''Others'' includes contributions from $VVV$, $t\bar{t} t$, $t\bar{t}t\bar{t}$, $t\bar{t} W$, $t\bar{t} WW$, $t\bar{t} WZ$, $t\bar{t} H$, and $tZ$ processes. The hatched bands represent the total statistical and systematic uncertainty. The rightmost bin of each plot includes overflow events. Reference top squark pair production signal models are overlayed for comparison. Red arrows in the upper panels indicate the signal region selection criteria. The bottom panels show the ratio of the observed data to the total SM background prediction, with hatched bands representing the total uncertainty in the background prediction; red arrows show data outside the vertical-axis range.

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Version 2
Search for squarks and gluinos in final states with one isolated lepton, jets, and missing transverse momentum at $\sqrt{s}=13$ TeV with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
Eur.Phys.J.C 81 (2021) 600, 2021.
Inspire Record 1839446 DOI 10.17182/hepdata.97041

The results of a search for gluino and squark pair production with the pairs decaying via the lightest charginos into a final state consisting of two $W$ bosons, the lightest neutralinos ($\tilde\chi^0_1$), and quarks, are presented. The signal is characterised by the presence of a single charged lepton ($e^{\pm}$ or $\mu^{\pm}$) from a $W$ boson decay, jets, and missing transverse momentum. The analysis is performed using 139 fb$^{-1}$ of proton-proton collision data taken at a centre-of-mass energy $\sqrt{s}=13$ TeV delivered by the Large Hadron Collider and recorded by the ATLAS experiment. No statistically significant excess of events above the Standard Model expectation is found. Limits are set on the direct production of squarks and gluinos in simplified models. Masses of gluino (squark) up to 2.2 TeV (1.4 TeV) are excluded at 95% confidence level for a light $\tilde\chi^0_1$.

608 data tables

Post-fit $m_{T}$ distribution in the SR 2J b-veto N-1 region. N-1 refers to all cuts except for the requirement on $m_T$ being applied. Uncertainties include statistical and systematic uncertainties. The value 9999 is used as a placeholder for infinity.

Post-fit $m_{T}$ distribution in the SR 2J b-veto N-1 region. N-1 refers to all cuts except for the requirement on $m_T$ being applied. Uncertainties include statistical and systematic uncertainties. The value 9999 is used as a placeholder for infinity.

Post-fit $m_{T}$ distribution in the SR 2J b-tag N-1 region. N-1 refers to all cuts except for the requirement on $m_T$ being applied. Uncertainties include statistical and systematic uncertainties. The value 9999 is used as a placeholder for infinity.

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Version 2
Search for trilepton resonances from chargino and neutralino pair production in $\sqrt{s}$ = 13 TeV $pp$ collisions with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Braden Keim ; Abbott, Brad ; et al.
Phys.Rev.D 103 (2021) 112003, 2021.
Inspire Record 1831992 DOI 10.17182/hepdata.99806

A search is performed for the electroweak pair production of charginos and associated production of a chargino and neutralino, each of which decays through an $R$-parity-violating coupling into a lepton and a $W$, $Z$, or Higgs boson. The trilepton invariant-mass spectrum is constructed from events with three or more leptons, targeting chargino decays that include an electron or muon and a leptonically decaying $Z$ boson. The analyzed dataset corresponds to an integrated luminosity of 139 fb$^{-1}$ of proton-proton collision data produced by the Large Hadron Collider at a center-of-mass energy of $\sqrt{s}$ = 13 TeV and collected by the ATLAS experiment between 2015 and 2018. The data are found to be consistent with predictions from the Standard Model. The results are interpreted as limits at 95% confidence level on model-independent cross sections for processes beyond the Standard Model. Limits are also set on the production of charginos and neutralinos for a Minimal Supersymmetric Standard Model with an approximate $B$-$L$ symmetry. Charginos and neutralinos with masses between 100 GeV and 1100 GeV are excluded depending on the assumed decay branching fractions into a lepton (electron, muon, or $\tau$-lepton) plus a boson ($W$, $Z$, or Higgs).

566 data tables

This is the HEPData space for the trilepton resonance wino search, the full resolution figures can be found here https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/SUSY-2018-36/. The full statistical likelihoods have been provided for this analysis. They can be downloaded by clicking on the purple 'Resources' buttun above where they can then be found in the 'Common Resources' area. A detailed README for how to use the likelihoods is also included in this download. <b>Exclusion contours:</b> <ul display="inline-block"> <li><a href="?table=Obs.%20data%20vs%20SM%20bkg.%20exp.%20in%20CRs%20and%20VRs">Obs. data vs SM bkg. exp. in CRs and VRs</a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Obs_0%20">$\ell=(e, \mu, \tau)$, Obs_0 </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up%20">$\ell=(e, \mu, \tau)$, Obs_0_Up </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down%20">$\ell=(e, \mu, \tau)$, Obs_0_Down </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Exp_0%20">$\ell=(e, \mu, \tau)$, Exp_0 </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up%20">$\ell=(e, \mu, \tau)$, Exp_0_Up </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down%20">$\ell=(e, \mu, \tau)$, Exp_0_Down </a> <li><a href="?table=$\ell=e$,%20Obs_0%20">$\ell=e$, Obs_0 </a> <li><a href="?table=$\ell=e$,%20Obs_0_Up%20">$\ell=e$, Obs_0_Up </a> <li><a href="?table=$\ell=e$,%20Obs_0_Down%20">$\ell=e$, Obs_0_Down </a> <li><a href="?table=$\ell=e$,%20Exp_0%20">$\ell=e$, Exp_0 </a> <li><a href="?table=$\ell=e$,%20Exp_0_Up%20">$\ell=e$, Exp_0_Up </a> <li><a href="?table=$\ell=e$,%20Exp_0_Down%20">$\ell=e$, Exp_0_Down </a> <li><a href="?table=$\ell=\mu$,%20Obs_0%20">$\ell=\mu$, Obs_0 </a> <li><a href="?table=$\ell=\mu$,%20Obs_0_Up%20">$\ell=\mu$, Obs_0_Up </a> <li><a href="?table=$\ell=\mu$,%20Obs_0_Down%20">$\ell=\mu$, Obs_0_Down </a> <li><a href="?table=$\ell=\mu$,%20Exp_0%20">$\ell=\mu$, Exp_0 </a> <li><a href="?table=$\ell=\mu$,%20Exp_0_Up%20">$\ell=\mu$, Exp_0_Up </a> <li><a href="?table=$\ell=\mu$,%20Exp_0_Down%20">$\ell=\mu$, Exp_0_Down </a> <li><a href="?table=$\ell=\tau$,%20Obs_0%20">$\ell=\tau$, Obs_0 </a> <li><a href="?table=$\ell=\tau$,%20Obs_0_Up%20">$\ell=\tau$, Obs_0_Up </a> <li><a href="?table=$\ell=\tau$,%20Obs_0_Down%20">$\ell=\tau$, Obs_0_Down </a> <li><a href="?table=$\ell=\tau$,%20Exp_0%20">$\ell=\tau$, Exp_0 </a> <li><a href="?table=$\ell=\tau$,%20Exp_0_Up%20">$\ell=\tau$, Exp_0_Up </a> <li><a href="?table=$\ell=\tau$,%20Exp_0_Down%20">$\ell=\tau$, Exp_0_Down </a> </ul> <b>Triangle Exclusion contours:</b> <ul display="inline-block"> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs%20Lim">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Obs Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp%20Lim">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Exp Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs%20Lim">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Obs Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp%20Lim">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Exp Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs%20Lim">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Obs Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp%20Lim">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Exp Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs%20Lim">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Obs Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp%20Lim">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Exp Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Obs_0">Triangle, 600 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, 600 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, 600 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Exp_0">Triangle, 600 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, 600 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, 600 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Obs%20Lim">Triangle, 600 GeV, $\ell=e$, Obs Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Exp%20Lim">Triangle, 600 GeV, $\ell=e$, Exp Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Obs_0">Triangle, 700 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, 700 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, 700 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Exp_0">Triangle, 700 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, 700 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, 700 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Obs%20Lim">Triangle, 700 GeV, $\ell=e$, Obs Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Exp%20Lim">Triangle, 700 GeV, $\ell=e$, Exp Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Obs_0">Triangle, 800 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, 800 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, 800 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Exp_0">Triangle, 800 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, 800 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, 800 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Obs%20Lim">Triangle, 800 GeV, $\ell=e$, Obs Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Exp%20Lim">Triangle, 800 GeV, $\ell=e$, Exp Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Obs_0">Triangle, 900 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, 900 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, 900 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Exp_0">Triangle, 900 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, 900 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, 900 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Obs%20Lim">Triangle, 900 GeV, $\ell=e$, Obs Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Exp%20Lim">Triangle, 900 GeV, $\ell=e$, Exp Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, 600 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, 600 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, 600 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, 600 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, 600 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, 600 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Obs%20Lim">Triangle, 600 GeV, $\ell=\mu$, Obs Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Exp%20Lim">Triangle, 600 GeV, $\ell=\mu$, Exp Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, 700 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, 700 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, 700 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, 700 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, 700 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, 700 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Obs%20Lim">Triangle, 700 GeV, $\ell=\mu$, Obs Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Exp%20Lim">Triangle, 700 GeV, $\ell=\mu$, Exp Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, 800 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, 800 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, 800 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, 800 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, 800 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, 800 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Obs%20Lim">Triangle, 800 GeV, $\ell=\mu$, Obs Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Exp%20Lim">Triangle, 800 GeV, $\ell=\mu$, Exp Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, 900 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, 900 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, 900 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, 900 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, 900 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, 900 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Obs%20Lim">Triangle, 900 GeV, $\ell=\mu$, Obs Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Exp%20Lim">Triangle, 900 GeV, $\ell=\mu$, Exp Lim</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Obs_0">Triangle, 200 GeV, $\ell=\tau$, Obs_0</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Obs_0_Up">Triangle, 200 GeV, $\ell=\tau$, Obs_0_Up</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Obs_0_Down">Triangle, 200 GeV, $\ell=\tau$, Obs_0_Down</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Exp_0">Triangle, 200 GeV, $\ell=\tau$, Exp_0</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Exp_0_Up">Triangle, 200 GeV, $\ell=\tau$, Exp_0_Up</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Exp_0_Down">Triangle, 200 GeV, $\ell=\tau$, Exp_0_Down</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Obs%20Lim">Triangle, 200 GeV, $\ell=\tau$, Obs Lim</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Exp%20Lim">Triangle, 200 GeV, $\ell=\tau$, Exp Lim</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Obs_0">Triangle, 300 GeV, $\ell=\tau$, Obs_0</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Obs_0_Up">Triangle, 300 GeV, $\ell=\tau$, Obs_0_Up</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Obs_0_Down">Triangle, 300 GeV, $\ell=\tau$, Obs_0_Down</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Exp_0">Triangle, 300 GeV, $\ell=\tau$, Exp_0</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Exp_0_Up">Triangle, 300 GeV, $\ell=\tau$, Exp_0_Up</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Exp_0_Down">Triangle, 300 GeV, $\ell=\tau$, Exp_0_Down</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Obs%20Lim">Triangle, 300 GeV, $\ell=\tau$, Obs Lim</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Exp%20Lim">Triangle, 300 GeV, $\ell=\tau$, Exp Lim</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Obs_0">Triangle, 400 GeV, $\ell=\tau$, Obs_0</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Obs_0_Up">Triangle, 400 GeV, $\ell=\tau$, Obs_0_Up</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Obs_0_Down">Triangle, 400 GeV, $\ell=\tau$, Obs_0_Down</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Exp_0">Triangle, 400 GeV, $\ell=\tau$, Exp_0</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Exp_0_Up">Triangle, 400 GeV, $\ell=\tau$, Exp_0_Up</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Exp_0_Down">Triangle, 400 GeV, $\ell=\tau$, Exp_0_Down</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Obs%20Lim">Triangle, 400 GeV, $\ell=\tau$, Obs Lim</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Exp%20Lim">Triangle, 400 GeV, $\ell=\tau$, Exp Lim</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Obs_0">Triangle, 500 GeV, $\ell=\tau$, Obs_0</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Obs_0_Up">Triangle, 500 GeV, $\ell=\tau$, Obs_0_Up</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Obs_0_Down">Triangle, 500 GeV, $\ell=\tau$, Obs_0_Down</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Exp_0">Triangle, 500 GeV, $\ell=\tau$, Exp_0</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Exp_0_Up">Triangle, 500 GeV, $\ell=\tau$, Exp_0_Up</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Exp_0_Down">Triangle, 500 GeV, $\ell=\tau$, Exp_0_Down</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Obs%20Lim">Triangle, 500 GeV, $\ell=\tau$, Obs Lim</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Exp%20Lim">Triangle, 500 GeV, $\ell=\tau$, Exp Lim</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ObsLimVal">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, ObsLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ExpLimVal">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ObsLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ExpLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ObsLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ExpLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, ExpLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Obs_0">Triangle, SRFR, 700 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, SRFR, 700 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, SRFR, 700 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Exp_0">Triangle, SRFR, 700 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, SRFR, 700 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, SRFR, 700 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20ObsLimVal">Triangle, SRFR, 700 GeV, $\ell=e$, ObsLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20ExpLimVal">Triangle, SRFR, 700 GeV, $\ell=e$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20ObsLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20ExpLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20ObsLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20ExpLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, ExpLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, SRFR, 700 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, SRFR, 700 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, SRFR, 700 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, SRFR, 700 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, SRFR, 700 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, SRFR, 700 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20ObsLimVal">Triangle, SRFR, 700 GeV, $\ell=\mu$, ObsLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20ExpLimVal">Triangle, SRFR, 700 GeV, $\ell=\mu$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20ObsLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20ExpLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20ObsLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20ExpLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, ExpLimVal</a> </ul> <b>Upper limits:</b> <ul display="inline-block"> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20upperLimit_XS_gr%20">$\ell=(e, \mu, \tau)$, upperLimit_XS_gr </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20expectedUpperLimit_XS_gr%20">$\ell=(e, \mu, \tau)$, expectedUpperLimit_XS_gr </a> <li><a href="?table=$\ell=e$,%20upperLimit_XS_gr%20">$\ell=e$, upperLimit_XS_gr </a> <li><a href="?table=$\ell=e$,%20expectedUpperLimit_XS_gr%20">$\ell=e$, expectedUpperLimit_XS_gr </a> <li><a href="?table=$\ell=\mu$,%20upperLimit_XS_gr%20">$\ell=\mu$, upperLimit_XS_gr </a> <li><a href="?table=$\ell=\mu$,%20expectedUpperLimit_XS_gr%20">$\ell=\mu$, expectedUpperLimit_XS_gr </a> <li><a href="?table=$\ell=\tau$,%20upperLimit_XS_gr%20">$\ell=\tau$, upperLimit_XS_gr </a> <li><a href="?table=$\ell=\tau$,%20expectedUpperLimit_XS_gr%20">$\ell=\tau$, expectedUpperLimit_XS_gr </a> </ul> <b>Kinematic distributions:</b> <ul display="inline-block"> <li><a href="?table=Variable%20bin%20$m_{Z\ell}$%20for%20SRFR%20">Variable bin $m_{Z\ell}$ for SRFR </a> <li><a href="?table=Variable%20bin%20$m_{Z\ell}$%20for%20SR4$\ell$%20">Variable bin $m_{Z\ell}$ for SR4$\ell$ </a> <li><a href="?table=Variable%20bin%20$m_{Z\ell}$%20for%20SR3$\ell$%20">Variable bin $m_{Z\ell}$ for SR3$\ell$ </a> <li><a href="?table=N-1%20for%20SR3$\ell$,%20$E^{miss}_{T}$%20">N-1 for SR3$\ell$, $E^{miss}_{T}$ </a> <li><a href="?table=N-1%20for%20SR3$\ell$,%20$m^{min}_{T}$%20">N-1 for SR3$\ell$, $m^{min}_{T}$ </a> <li><a href="?table=N-1%20for%20SR4$\ell$,%20$E^{miss,SF}_{T}$%20">N-1 for SR4$\ell$, $E^{miss,SF}_{T}$ </a> <li><a href="?table=N-1%20for%20SRFR,%20$m^{asym}_{Z\ell}$%20">N-1 for SRFR, $m^{asym}_{Z\ell}$ </a> <li><a href="?table=$m_{Z\ell}$%20for%20SRFR%20">$m_{Z\ell}$ for SRFR </a> <li><a href="?table=$m_{Z\ell}$%20for%20SR4$\ell$%20">$m_{Z\ell}$ for SR4$\ell$ </a> <li><a href="?table=$m_{Z\ell}$%20for%20SR3$\ell$%20">$m_{Z\ell}$ for SR3$\ell$ </a> <li><a href="?table=$L_{T}$%20for%20SR4$\ell$%20">$L_{T}$ for SR4$\ell$ </a> </ul> <b>Cut flows:</b> <ul display="inline-block"> <li><a href="?table=Yields%20Table">Yields Table</a> <li><a href="?table=Model-Independent%20Results%20Table,%20SRFR">Model-Independent Results Table, SRFR</a> <li><a href="?table=Model-Independent%20Results%20Table,%20SR4$\ell$">Model-Independent Results Table, SR4$\ell$</a> <li><a href="?table=Model-Independent%20Results%20Table,%20SR3$\ell$">Model-Independent Results Table, SR3$\ell$</a> <li><a href="?table=Cutflow%20Table">Cutflow Table</a> </ul> <b>Acceptances and Efficiencies:</b> <ul display="inline-block"> <li><a href="?table=Acceptance%20in%20the%20SRFR%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Acceptance in the SRFR region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Acceptance%20in%20the%20SRFR%20region%20with%20$\ell=$$e$">Acceptance in the SRFR region with $\ell=$$e$</a> <li><a href="?table=Acceptance%20in%20the%20SRFR%20region%20with%20$\ell=$$\mu$">Acceptance in the SRFR region with $\ell=$$\mu$</a> <li><a href="?table=Acceptance%20in%20the%20SRFR%20region%20with%20$\ell=$$\tau$">Acceptance in the SRFR region with $\ell=$$\tau$</a> <li><a href="?table=Acceptance%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Acceptance in the SR4$\ell$ region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Acceptance%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$e$">Acceptance in the SR4$\ell$ region with $\ell=$$e$</a> <li><a href="?table=Acceptance%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$\mu$">Acceptance in the SR4$\ell$ region with $\ell=$$\mu$</a> <li><a href="?table=Acceptance%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$\tau$">Acceptance in the SR4$\ell$ region with $\ell=$$\tau$</a> <li><a href="?table=Acceptance%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Acceptance in the SR3$\ell$ region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Acceptance%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$e$">Acceptance in the SR3$\ell$ region with $\ell=$$e$</a> <li><a href="?table=Acceptance%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$\mu$">Acceptance in the SR3$\ell$ region with $\ell=$$\mu$</a> <li><a href="?table=Acceptance%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$\tau$">Acceptance in the SR3$\ell$ region with $\ell=$$\tau$</a> <li><a href="?table=Efficiency%20in%20the%20SRFR%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Efficiency in the SRFR region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Efficiency%20in%20the%20SRFR%20region%20with%20$\ell=$$e$">Efficiency in the SRFR region with $\ell=$$e$</a> <li><a href="?table=Efficiency%20in%20the%20SRFR%20region%20with%20$\ell=$$\mu$">Efficiency in the SRFR region with $\ell=$$\mu$</a> <li><a href="?table=Efficiency%20in%20the%20SRFR%20region%20with%20$\ell=$$\tau$">Efficiency in the SRFR region with $\ell=$$\tau$</a> <li><a href="?table=Efficiency%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Efficiency in the SR4$\ell$ region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Efficiency%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$e$">Efficiency in the SR4$\ell$ region with $\ell=$$e$</a> <li><a href="?table=Efficiency%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$\mu$">Efficiency in the SR4$\ell$ region with $\ell=$$\mu$</a> <li><a href="?table=Efficiency%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$\tau$">Efficiency in the SR4$\ell$ region with $\ell=$$\tau$</a> <li><a href="?table=Efficiency%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Efficiency in the SR3$\ell$ region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Efficiency%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$e$">Efficiency in the SR3$\ell$ region with $\ell=$$e$</a> <li><a href="?table=Efficiency%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$\mu$">Efficiency in the SR3$\ell$ region with $\ell=$$\mu$</a> <li><a href="?table=Efficiency%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$\tau$">Efficiency in the SR3$\ell$ region with $\ell=$$\tau$</a> <li><a href="?table=Triangle,%20Acceptance%20in%20SRFR,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Acceptance in SRFR, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Acceptance%20in%20SR4$\ell$,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Acceptance in SR4$\ell$, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Acceptance%20in%20SR3$\ell$,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Acceptance in SR3$\ell$, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Efficiency%20in%20SRFR,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Efficiency in SRFR, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Efficiency%20in%20SR4$\ell$,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Efficiency in SR4$\ell$, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Efficiency%20in%20SR3$\ell$,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Efficiency in SR3$\ell$, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Acceptance%20by%20Final%20State%20in%20SRFR">Acceptance by Final State in SRFR</a> <li><a href="?table=Acceptance%20by%20Final%20State%20in%20SR4$\ell$">Acceptance by Final State in SR4$\ell$</a> <li><a href="?table=Acceptance%20by%20Final%20State%20in%20SR3$\ell$">Acceptance by Final State in SR3$\ell$</a> </ul>

This is the HEPData space for the trilepton resonance wino search, the full resolution figures can be found here https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/SUSY-2018-36/. The full statistical likelihoods have been provided for this analysis. They can be downloaded by clicking on the purple 'Resources' buttun above where they can then be found in the 'Common Resources' area. A detailed README for how to use the likelihoods is also included in this download. <b>Exclusion contours:</b> <ul display="inline-block"> <li><a href="?table=Obs.%20data%20vs%20SM%20bkg.%20exp.%20in%20CRs%20and%20VRs">Obs. data vs SM bkg. exp. in CRs and VRs</a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Obs_0%20">$\ell=(e, \mu, \tau)$, Obs_0 </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up%20">$\ell=(e, \mu, \tau)$, Obs_0_Up </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down%20">$\ell=(e, \mu, \tau)$, Obs_0_Down </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Exp_0%20">$\ell=(e, \mu, \tau)$, Exp_0 </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up%20">$\ell=(e, \mu, \tau)$, Exp_0_Up </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down%20">$\ell=(e, \mu, \tau)$, Exp_0_Down </a> <li><a href="?table=$\ell=e$,%20Obs_0%20">$\ell=e$, Obs_0 </a> <li><a href="?table=$\ell=e$,%20Obs_0_Up%20">$\ell=e$, Obs_0_Up </a> <li><a href="?table=$\ell=e$,%20Obs_0_Down%20">$\ell=e$, Obs_0_Down </a> <li><a href="?table=$\ell=e$,%20Exp_0%20">$\ell=e$, Exp_0 </a> <li><a href="?table=$\ell=e$,%20Exp_0_Up%20">$\ell=e$, Exp_0_Up </a> <li><a href="?table=$\ell=e$,%20Exp_0_Down%20">$\ell=e$, Exp_0_Down </a> <li><a href="?table=$\ell=\mu$,%20Obs_0%20">$\ell=\mu$, Obs_0 </a> <li><a href="?table=$\ell=\mu$,%20Obs_0_Up%20">$\ell=\mu$, Obs_0_Up </a> <li><a href="?table=$\ell=\mu$,%20Obs_0_Down%20">$\ell=\mu$, Obs_0_Down </a> <li><a href="?table=$\ell=\mu$,%20Exp_0%20">$\ell=\mu$, Exp_0 </a> <li><a href="?table=$\ell=\mu$,%20Exp_0_Up%20">$\ell=\mu$, Exp_0_Up </a> <li><a href="?table=$\ell=\mu$,%20Exp_0_Down%20">$\ell=\mu$, Exp_0_Down </a> <li><a href="?table=$\ell=\tau$,%20Obs_0%20">$\ell=\tau$, Obs_0 </a> <li><a href="?table=$\ell=\tau$,%20Obs_0_Up%20">$\ell=\tau$, Obs_0_Up </a> <li><a href="?table=$\ell=\tau$,%20Obs_0_Down%20">$\ell=\tau$, Obs_0_Down </a> <li><a href="?table=$\ell=\tau$,%20Exp_0%20">$\ell=\tau$, Exp_0 </a> <li><a href="?table=$\ell=\tau$,%20Exp_0_Up%20">$\ell=\tau$, Exp_0_Up </a> <li><a href="?table=$\ell=\tau$,%20Exp_0_Down%20">$\ell=\tau$, Exp_0_Down </a> </ul> <b>Triangle Exclusion contours:</b> <ul display="inline-block"> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs%20Lim">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Obs Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp%20Lim">Triangle, 600 GeV, $\ell=(e, \mu, \tau)$, Exp Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs%20Lim">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Obs Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp%20Lim">Triangle, 700 GeV, $\ell=(e, \mu, \tau)$, Exp Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs%20Lim">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Obs Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp%20Lim">Triangle, 800 GeV, $\ell=(e, \mu, \tau)$, Exp Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs%20Lim">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Obs Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp%20Lim">Triangle, 900 GeV, $\ell=(e, \mu, \tau)$, Exp Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Obs_0">Triangle, 600 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, 600 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, 600 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Exp_0">Triangle, 600 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, 600 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, 600 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Obs%20Lim">Triangle, 600 GeV, $\ell=e$, Obs Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=e$,%20Exp%20Lim">Triangle, 600 GeV, $\ell=e$, Exp Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Obs_0">Triangle, 700 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, 700 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, 700 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Exp_0">Triangle, 700 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, 700 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, 700 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Obs%20Lim">Triangle, 700 GeV, $\ell=e$, Obs Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=e$,%20Exp%20Lim">Triangle, 700 GeV, $\ell=e$, Exp Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Obs_0">Triangle, 800 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, 800 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, 800 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Exp_0">Triangle, 800 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, 800 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, 800 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Obs%20Lim">Triangle, 800 GeV, $\ell=e$, Obs Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=e$,%20Exp%20Lim">Triangle, 800 GeV, $\ell=e$, Exp Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Obs_0">Triangle, 900 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, 900 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, 900 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Exp_0">Triangle, 900 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, 900 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, 900 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Obs%20Lim">Triangle, 900 GeV, $\ell=e$, Obs Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=e$,%20Exp%20Lim">Triangle, 900 GeV, $\ell=e$, Exp Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, 600 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, 600 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, 600 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, 600 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, 600 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, 600 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Obs%20Lim">Triangle, 600 GeV, $\ell=\mu$, Obs Lim</a> <li><a href="?table=Triangle,%20600%20GeV,%20$\ell=\mu$,%20Exp%20Lim">Triangle, 600 GeV, $\ell=\mu$, Exp Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, 700 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, 700 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, 700 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, 700 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, 700 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, 700 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Obs%20Lim">Triangle, 700 GeV, $\ell=\mu$, Obs Lim</a> <li><a href="?table=Triangle,%20700%20GeV,%20$\ell=\mu$,%20Exp%20Lim">Triangle, 700 GeV, $\ell=\mu$, Exp Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, 800 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, 800 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, 800 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, 800 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, 800 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, 800 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Obs%20Lim">Triangle, 800 GeV, $\ell=\mu$, Obs Lim</a> <li><a href="?table=Triangle,%20800%20GeV,%20$\ell=\mu$,%20Exp%20Lim">Triangle, 800 GeV, $\ell=\mu$, Exp Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, 900 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, 900 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, 900 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, 900 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, 900 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, 900 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Obs%20Lim">Triangle, 900 GeV, $\ell=\mu$, Obs Lim</a> <li><a href="?table=Triangle,%20900%20GeV,%20$\ell=\mu$,%20Exp%20Lim">Triangle, 900 GeV, $\ell=\mu$, Exp Lim</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Obs_0">Triangle, 200 GeV, $\ell=\tau$, Obs_0</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Obs_0_Up">Triangle, 200 GeV, $\ell=\tau$, Obs_0_Up</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Obs_0_Down">Triangle, 200 GeV, $\ell=\tau$, Obs_0_Down</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Exp_0">Triangle, 200 GeV, $\ell=\tau$, Exp_0</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Exp_0_Up">Triangle, 200 GeV, $\ell=\tau$, Exp_0_Up</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Exp_0_Down">Triangle, 200 GeV, $\ell=\tau$, Exp_0_Down</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Obs%20Lim">Triangle, 200 GeV, $\ell=\tau$, Obs Lim</a> <li><a href="?table=Triangle,%20200%20GeV,%20$\ell=\tau$,%20Exp%20Lim">Triangle, 200 GeV, $\ell=\tau$, Exp Lim</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Obs_0">Triangle, 300 GeV, $\ell=\tau$, Obs_0</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Obs_0_Up">Triangle, 300 GeV, $\ell=\tau$, Obs_0_Up</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Obs_0_Down">Triangle, 300 GeV, $\ell=\tau$, Obs_0_Down</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Exp_0">Triangle, 300 GeV, $\ell=\tau$, Exp_0</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Exp_0_Up">Triangle, 300 GeV, $\ell=\tau$, Exp_0_Up</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Exp_0_Down">Triangle, 300 GeV, $\ell=\tau$, Exp_0_Down</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Obs%20Lim">Triangle, 300 GeV, $\ell=\tau$, Obs Lim</a> <li><a href="?table=Triangle,%20300%20GeV,%20$\ell=\tau$,%20Exp%20Lim">Triangle, 300 GeV, $\ell=\tau$, Exp Lim</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Obs_0">Triangle, 400 GeV, $\ell=\tau$, Obs_0</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Obs_0_Up">Triangle, 400 GeV, $\ell=\tau$, Obs_0_Up</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Obs_0_Down">Triangle, 400 GeV, $\ell=\tau$, Obs_0_Down</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Exp_0">Triangle, 400 GeV, $\ell=\tau$, Exp_0</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Exp_0_Up">Triangle, 400 GeV, $\ell=\tau$, Exp_0_Up</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Exp_0_Down">Triangle, 400 GeV, $\ell=\tau$, Exp_0_Down</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Obs%20Lim">Triangle, 400 GeV, $\ell=\tau$, Obs Lim</a> <li><a href="?table=Triangle,%20400%20GeV,%20$\ell=\tau$,%20Exp%20Lim">Triangle, 400 GeV, $\ell=\tau$, Exp Lim</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Obs_0">Triangle, 500 GeV, $\ell=\tau$, Obs_0</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Obs_0_Up">Triangle, 500 GeV, $\ell=\tau$, Obs_0_Up</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Obs_0_Down">Triangle, 500 GeV, $\ell=\tau$, Obs_0_Down</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Exp_0">Triangle, 500 GeV, $\ell=\tau$, Exp_0</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Exp_0_Up">Triangle, 500 GeV, $\ell=\tau$, Exp_0_Up</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Exp_0_Down">Triangle, 500 GeV, $\ell=\tau$, Exp_0_Down</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Obs%20Lim">Triangle, 500 GeV, $\ell=\tau$, Obs Lim</a> <li><a href="?table=Triangle,%20500%20GeV,%20$\ell=\tau$,%20Exp%20Lim">Triangle, 500 GeV, $\ell=\tau$, Exp Lim</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ObsLimVal">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, ObsLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ExpLimVal">Triangle, SRFR, 700 GeV, $\ell=(e, \mu, \tau)$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ObsLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ExpLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Obs_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20Exp_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ObsLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=(e,%20\mu,%20\tau)$,%20ExpLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=(e, \mu, \tau)$, ExpLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Obs_0">Triangle, SRFR, 700 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, SRFR, 700 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, SRFR, 700 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Exp_0">Triangle, SRFR, 700 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, SRFR, 700 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, SRFR, 700 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20ObsLimVal">Triangle, SRFR, 700 GeV, $\ell=e$, ObsLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=e$,%20ExpLimVal">Triangle, SRFR, 700 GeV, $\ell=e$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20ObsLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=e$,%20ExpLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=e$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Obs_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Obs_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Exp_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20Exp_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20ObsLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=e$,%20ExpLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=e$, ExpLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, SRFR, 700 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, SRFR, 700 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, SRFR, 700 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, SRFR, 700 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, SRFR, 700 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, SRFR, 700 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20ObsLimVal">Triangle, SRFR, 700 GeV, $\ell=\mu$, ObsLimVal</a> <li><a href="?table=Triangle,%20SRFR,%20700%20GeV,%20$\ell=\mu$,%20ExpLimVal">Triangle, SRFR, 700 GeV, $\ell=\mu$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20ObsLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR4$\ell$,%20700%20GeV,%20$\ell=\mu$,%20ExpLimVal">Triangle, SR4$\ell$, 700 GeV, $\ell=\mu$, ExpLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Obs_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Obs_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Obs_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Obs_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Exp_0</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Up">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Exp_0_Up</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20Exp_0_Down">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, Exp_0_Down</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20ObsLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, ObsLimVal</a> <li><a href="?table=Triangle,%20SR3$\ell$,%20700%20GeV,%20$\ell=\mu$,%20ExpLimVal">Triangle, SR3$\ell$, 700 GeV, $\ell=\mu$, ExpLimVal</a> </ul> <b>Upper limits:</b> <ul display="inline-block"> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20upperLimit_XS_gr%20">$\ell=(e, \mu, \tau)$, upperLimit_XS_gr </a> <li><a href="?table=$\ell=(e,%20\mu,%20\tau)$,%20expectedUpperLimit_XS_gr%20">$\ell=(e, \mu, \tau)$, expectedUpperLimit_XS_gr </a> <li><a href="?table=$\ell=e$,%20upperLimit_XS_gr%20">$\ell=e$, upperLimit_XS_gr </a> <li><a href="?table=$\ell=e$,%20expectedUpperLimit_XS_gr%20">$\ell=e$, expectedUpperLimit_XS_gr </a> <li><a href="?table=$\ell=\mu$,%20upperLimit_XS_gr%20">$\ell=\mu$, upperLimit_XS_gr </a> <li><a href="?table=$\ell=\mu$,%20expectedUpperLimit_XS_gr%20">$\ell=\mu$, expectedUpperLimit_XS_gr </a> <li><a href="?table=$\ell=\tau$,%20upperLimit_XS_gr%20">$\ell=\tau$, upperLimit_XS_gr </a> <li><a href="?table=$\ell=\tau$,%20expectedUpperLimit_XS_gr%20">$\ell=\tau$, expectedUpperLimit_XS_gr </a> </ul> <b>Kinematic distributions:</b> <ul display="inline-block"> <li><a href="?table=Variable%20bin%20$m_{Z\ell}$%20for%20SRFR%20">Variable bin $m_{Z\ell}$ for SRFR </a> <li><a href="?table=Variable%20bin%20$m_{Z\ell}$%20for%20SR4$\ell$%20">Variable bin $m_{Z\ell}$ for SR4$\ell$ </a> <li><a href="?table=Variable%20bin%20$m_{Z\ell}$%20for%20SR3$\ell$%20">Variable bin $m_{Z\ell}$ for SR3$\ell$ </a> <li><a href="?table=N-1%20for%20SR3$\ell$,%20$E^{miss}_{T}$%20">N-1 for SR3$\ell$, $E^{miss}_{T}$ </a> <li><a href="?table=N-1%20for%20SR3$\ell$,%20$m^{min}_{T}$%20">N-1 for SR3$\ell$, $m^{min}_{T}$ </a> <li><a href="?table=N-1%20for%20SR4$\ell$,%20$E^{miss,SF}_{T}$%20">N-1 for SR4$\ell$, $E^{miss,SF}_{T}$ </a> <li><a href="?table=N-1%20for%20SRFR,%20$m^{asym}_{Z\ell}$%20">N-1 for SRFR, $m^{asym}_{Z\ell}$ </a> <li><a href="?table=$m_{Z\ell}$%20for%20SRFR%20">$m_{Z\ell}$ for SRFR </a> <li><a href="?table=$m_{Z\ell}$%20for%20SR4$\ell$%20">$m_{Z\ell}$ for SR4$\ell$ </a> <li><a href="?table=$m_{Z\ell}$%20for%20SR3$\ell$%20">$m_{Z\ell}$ for SR3$\ell$ </a> <li><a href="?table=$L_{T}$%20for%20SR4$\ell$%20">$L_{T}$ for SR4$\ell$ </a> </ul> <b>Cut flows:</b> <ul display="inline-block"> <li><a href="?table=Yields%20Table">Yields Table</a> <li><a href="?table=Model-Independent%20Results%20Table,%20SRFR">Model-Independent Results Table, SRFR</a> <li><a href="?table=Model-Independent%20Results%20Table,%20SR4$\ell$">Model-Independent Results Table, SR4$\ell$</a> <li><a href="?table=Model-Independent%20Results%20Table,%20SR3$\ell$">Model-Independent Results Table, SR3$\ell$</a> <li><a href="?table=Cutflow%20Table">Cutflow Table</a> </ul> <b>Acceptances and Efficiencies:</b> <ul display="inline-block"> <li><a href="?table=Acceptance%20in%20the%20SRFR%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Acceptance in the SRFR region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Acceptance%20in%20the%20SRFR%20region%20with%20$\ell=$$e$">Acceptance in the SRFR region with $\ell=$$e$</a> <li><a href="?table=Acceptance%20in%20the%20SRFR%20region%20with%20$\ell=$$\mu$">Acceptance in the SRFR region with $\ell=$$\mu$</a> <li><a href="?table=Acceptance%20in%20the%20SRFR%20region%20with%20$\ell=$$\tau$">Acceptance in the SRFR region with $\ell=$$\tau$</a> <li><a href="?table=Acceptance%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Acceptance in the SR4$\ell$ region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Acceptance%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$e$">Acceptance in the SR4$\ell$ region with $\ell=$$e$</a> <li><a href="?table=Acceptance%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$\mu$">Acceptance in the SR4$\ell$ region with $\ell=$$\mu$</a> <li><a href="?table=Acceptance%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$\tau$">Acceptance in the SR4$\ell$ region with $\ell=$$\tau$</a> <li><a href="?table=Acceptance%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Acceptance in the SR3$\ell$ region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Acceptance%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$e$">Acceptance in the SR3$\ell$ region with $\ell=$$e$</a> <li><a href="?table=Acceptance%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$\mu$">Acceptance in the SR3$\ell$ region with $\ell=$$\mu$</a> <li><a href="?table=Acceptance%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$\tau$">Acceptance in the SR3$\ell$ region with $\ell=$$\tau$</a> <li><a href="?table=Efficiency%20in%20the%20SRFR%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Efficiency in the SRFR region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Efficiency%20in%20the%20SRFR%20region%20with%20$\ell=$$e$">Efficiency in the SRFR region with $\ell=$$e$</a> <li><a href="?table=Efficiency%20in%20the%20SRFR%20region%20with%20$\ell=$$\mu$">Efficiency in the SRFR region with $\ell=$$\mu$</a> <li><a href="?table=Efficiency%20in%20the%20SRFR%20region%20with%20$\ell=$$\tau$">Efficiency in the SRFR region with $\ell=$$\tau$</a> <li><a href="?table=Efficiency%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Efficiency in the SR4$\ell$ region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Efficiency%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$e$">Efficiency in the SR4$\ell$ region with $\ell=$$e$</a> <li><a href="?table=Efficiency%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$\mu$">Efficiency in the SR4$\ell$ region with $\ell=$$\mu$</a> <li><a href="?table=Efficiency%20in%20the%20SR4$\ell$%20region%20with%20$\ell=$$\tau$">Efficiency in the SR4$\ell$ region with $\ell=$$\tau$</a> <li><a href="?table=Efficiency%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$(e,%20\mu,%20\tau)$">Efficiency in the SR3$\ell$ region with $\ell=$$(e, \mu, \tau)$</a> <li><a href="?table=Efficiency%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$e$">Efficiency in the SR3$\ell$ region with $\ell=$$e$</a> <li><a href="?table=Efficiency%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$\mu$">Efficiency in the SR3$\ell$ region with $\ell=$$\mu$</a> <li><a href="?table=Efficiency%20in%20the%20SR3$\ell$%20region%20with%20$\ell=$$\tau$">Efficiency in the SR3$\ell$ region with $\ell=$$\tau$</a> <li><a href="?table=Triangle,%20Acceptance%20in%20SRFR,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Acceptance in SRFR, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Acceptance%20in%20SR4$\ell$,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Acceptance in SR4$\ell$, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Acceptance%20in%20SR3$\ell$,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Acceptance in SR3$\ell$, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Efficiency%20in%20SRFR,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Efficiency in SRFR, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Efficiency%20in%20SR4$\ell$,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Efficiency in SR4$\ell$, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Triangle,%20Efficiency%20in%20SR3$\ell$,%20$\ell=(e,%20\mu,%20\tau)$">Triangle, Efficiency in SR3$\ell$, $\ell=(e, \mu, \tau)$</a> <li><a href="?table=Acceptance%20by%20Final%20State%20in%20SRFR">Acceptance by Final State in SRFR</a> <li><a href="?table=Acceptance%20by%20Final%20State%20in%20SR4$\ell$">Acceptance by Final State in SR4$\ell$</a> <li><a href="?table=Acceptance%20by%20Final%20State%20in%20SR3$\ell$">Acceptance by Final State in SR3$\ell$</a> </ul>

The observed data and the SM background expectation in the CRs (pre-fit) and VRs (post-fit). The ''Other'' category mostly consists of tW Z, ttW, and tZ processes. The hatched bands indicate the combined theoretical, experimental, and MC statistical uncertainties. The bottom panel shows the fractional difference between the observed data and expected yields for the CRs and the significance of the difference for the VRs, computed following the profile likelihood method described in Ref. [arXiv: physics/0702156].

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Version 2
Search for squarks and gluinos in final states with jets and missing transverse momentum using 139 fb$^{-1}$ of $\sqrt{s}$ =13 TeV $pp$ collision data with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
JHEP 02 (2021) 143, 2021.
Inspire Record 1827025 DOI 10.17182/hepdata.95664

A search for the supersymmetric partners of quarks and gluons (squarks and gluinos) in final states containing jets and missing transverse momentum, but no electrons or muons, is presented. The data used in this search were recorded by the ATLAS experiment in proton-proton collisions at a centre-of-mass energy of $\sqrt{s}$ = 13 TeV during Run 2 of the Large Hadron Collider, corresponding to an integrated luminosity of 139 fb$^{-1}$. The results are interpreted in the context of various $R$-parity-conserving models where squarks and gluinos are produced in pairs or in association and a neutralino is the lightest supersymmetric particle. An exclusion limit at the 95% confidence level on the mass of the gluino is set at 2.30 TeV for a simplified model containing only a gluino and the lightest neutralino, assuming the latter is massless. For a simplified model involving the strong production of mass-degenerate first- and second-generation squarks, squark masses below 1.85 TeV are excluded if the lightest neutralino is massless. These limits extend substantially beyond the region of supersymmetric parameter space excluded previously by similar searches with the ATLAS detector.

150 data tables

Observed $m_{\mathrm{eff}}$ distributions in signal regions MB-SSd. The histograms show the MC background predictions normalised by the background-only fit. The hatched (red) error bands indicate experimental and MC statistical uncertainties. Expected distributions for benchmark signal model points, normalised using the approximate NNLO+NNLL cross-section times integrated luminosity, are also shown for comparison (masses in GeV).

Observed $m_{\mathrm{eff}}$ distributions in signal regions MB-SSd. The histograms show the MC background predictions normalised by the background-only fit. The hatched (red) error bands indicate experimental and MC statistical uncertainties. Expected distributions for benchmark signal model points, normalised using the approximate NNLO+NNLL cross-section times integrated luminosity, are also shown for comparison (masses in GeV).

Observed metSig distributions in signal regions MB-SSd. The histograms show the MC background predictions normalised by the background-only fit. The hatched (red) error bands indicate experimental and MC statistical uncertainties. Expected distributions for benchmark signal model points, normalised using the approximate NNLO+NNLL cross-section times integrated luminosity, are also shown for comparison (masses in GeV).

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Search for phenomena beyond the Standard Model in events with large $b$-jet multiplicity using the ATLAS detector at the LHC

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
Eur.Phys.J.C 81 (2021) 11, 2021.
Inspire Record 1821239 DOI 10.17182/hepdata.95683

A search is presented for new phenomena in events characterised by high jet multiplicity, no leptons (electrons or muons), and four or more jets originating from the fragmentation of $b$-quarks ($b$-jets). The search uses 139 fb$^{-1}$ of $\sqrt{s}$ = 13 TeV proton-proton collision data collected by the ATLAS experiment at the Large Hadron Collider during Run 2. The dominant Standard Model background originates from multijet production and is estimated using a data-driven technique based on an extrapolation from events with low $b$-jet multiplicity to the high $b$-jet multiplicities used in the search. No significant excess over the Standard Model expectation is observed and 95% confidence-level limits that constrain simplified models of R-parity-violating supersymmetry are determined. The exclusion limits reach 950 GeV in top-squark mass in the models considered.

49 data tables

<b>- - - - - - - - Overview of HEPData Record - - - - - - - -</b> <br><br> <b>Exclusion contours:</b> <ul> <li><a href="?table=stbchionly_obs">Stop to bottom quark and chargino exclusion contour (Obs.)</a> <li><a href="?table=stbchionly_exp">Stop to bottom quark and chargino exclusion contour (Exp.)</a> <li><a href="?table=stbchi_obs">Stop to higgsino LSP exclusion contour (Obs.)</a> <li><a href="?table=stbchi_exp">Stop to higgsino LSP exclusion contour (Exp.)</a> <li><a href="?table=sttN_obs">Stop to top quark and neutralino exclusion contour (Obs.)</a> <li><a href="?table=sttN_exp">Stop to top quark and neutralino exclusion contour (Exp.)</a> </ul> <b>Upper limits:</b> <ul> <li><a href="?table=stbchionly_xSecUL_obs">Obs Xsection upper limit in stop to bottom quark and chargino</a> <li><a href="?table=stop_xSecUL_obs">Obs Xsection upper limit in higgsino LSP</a> <li><a href="?table=stbchionly_xSecUL_exp">Exp Xsection upper limit in stop to bottom quark and chargino</a> <li><a href="?table=stop_xSecUL_exp">Exp Xsection upper limit in higgsino LSP</a> </ul> <b>Kinematic distributions:</b> <ul> <li><a href="?table=SR_yields">SR_yields</a> </ul> <b>Cut flows:</b> <ul> <li><a href="?table=cutflow">cutflow</a> </ul> <b>Acceptance and efficiencies:</b> As explained in <a href="https://twiki.cern.ch/twiki/bin/view/AtlasPublic/SupersymmetryPublicResults#summary_of_auxiliary_material">the twiki</a>. <ul> <li> <b>stbchi_6je4be:</b> <a href="?table=stbchi_Acc_6je4be">stbchi_Acc_6je4be</a> <a href="?table=stbchi_Eff_6je4be">stbchi_Eff_6je4be</a> <li> <b>stbchi_7je4be:</b> <a href="?table=stbchi_Acc_7je4be">stbchi_Acc_7je4be</a> <a href="?table=stbchi_Eff_7je4be">stbchi_Eff_7je4be</a> <li> <b>stbchi_8je4be:</b> <a href="?table=stbchi_Acc_8je4be">stbchi_Acc_8je4be</a> <a href="?table=stbchi_Eff_8je4be">stbchi_Eff_8je4be</a> <li> <b>stbchi_9ji4be:</b> <a href="?table=stbchi_Acc_9ji4be">stbchi_Acc_9ji4be</a> <a href="?table=stbchi_Eff_9ji4be">stbchi_Eff_9ji4be</a> <li> <b>stbchi_6je5bi:</b> <a href="?table=stbchi_Acc_6je5bi">stbchi_Acc_6je5bi</a> <a href="?table=stbchi_Eff_6je5bi">stbchi_Eff_6je5bi</a> <li> <b>stbchi_7je5bi:</b> <a href="?table=stbchi_Acc_7je5bi">stbchi_Acc_7je5bi</a> <a href="?table=stbchi_Eff_7je5bi">stbchi_Eff_7je5bi</a> <li> <b>stbchi_8je5bi:</b> <a href="?table=stbchi_Acc_8je5bi">stbchi_Acc_8je5bi</a> <a href="?table=stbchi_Eff_8je5bi">stbchi_Eff_8je5bi</a> <li> <b>stbchi_9ji5bi:</b> <a href="?table=stbchi_Acc_9ji5bi">stbchi_Acc_9ji5bi</a> <a href="?table=stbchi_Eff_9ji5bi">stbchi_Eff_9ji5bi</a> <li> <b>stbchi_8ji5bi:</b> <a href="?table=stbchi_Acc_8ji5bi">stbchi_Acc_8ji5bi</a> <a href="?table=stbchi_Eff_8ji5bi">stbchi_Eff_8ji5bi</a> <li> <b>sttN_6je4be:</b> <a href="?table=sttN_Acc_6je4be">sttN_Acc_6je4be</a> <a href="?table=sttN_Eff_6je4be">sttN_Eff_6je4be</a> <li> <b>sttN_7je4be:</b> <a href="?table=sttN_Acc_7je4be">sttN_Acc_7je4be</a> <a href="?table=sttN_Eff_7je4be">sttN_Eff_7je4be</a> <li> <b>sttN_8je4be:</b> <a href="?table=sttN_Acc_8je4be">sttN_Acc_8je4be</a> <a href="?table=sttN_Eff_8je4be">sttN_Eff_8je4be</a> <li> <b>sttN_9ji4be:</b> <a href="?table=sttN_Acc_9ji4be">sttN_Acc_9ji4be</a> <a href="?table=sttN_Eff_9ji4be">sttN_Eff_9ji4be</a> <li> <b>sttN_6je5bi:</b> <a href="?table=sttN_Acc_6je5bi">sttN_Acc_6je5bi</a> <a href="?table=sttN_Eff_6je5bi">sttN_Eff_6je5bi</a> <li> <b>sttN_7je5bi:</b> <a href="?table=sttN_Acc_7je5bi">sttN_Acc_7je5bi</a> <a href="?table=sttN_Eff_7je5bi">sttN_Eff_7je5bi</a> <li> <b>sttN_8je5bi:</b> <a href="?table=sttN_Acc_8je5bi">sttN_Acc_8je5bi</a> <a href="?table=sttN_Eff_8je5bi">sttN_Eff_8je5bi</a> <li> <b>sttN_9ji5bi:</b> <a href="?table=sttN_Acc_9ji5bi">sttN_Acc_9ji5bi</a> <a href="?table=sttN_Eff_9ji5bi">sttN_Eff_9ji5bi</a> <li> <b>sttN_8ji5bi:</b> <a href="?table=sttN_Acc_8ji5bi">sttN_Acc_8ji5bi</a> <a href="?table=sttN_Eff_8ji5bi">sttN_Eff_8ji5bi</a> </ul> <b>Truth Code snippets</b> and <b>SLHA</a> files are available under "Resources" (purple button on the left)

The observed exclusion contour at 95% CL as a function of the $\it{m}_{\tilde{\chi}^{\pm}_{1}}$ vs. $\it{m}_{\tilde{t}}$. Masses that are within the contours are excluded. Limits are shown for $B(\tilde{t} \rightarrow b \chi^{+}_{1})$ equal to unity.

The expected exclusion contour at 95% CL as a function of the $\it{m}_{\tilde{\chi}^{\pm}_{1}}$ vs. $\it{m}_{\tilde{t}}$. Masses that are within the contour are excluded. Limits are shown for $B(\tilde{t} \rightarrow b \chi^{+}_{1})$ equal to unity.

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Search for new phenomena in final states with large jet multiplicities and missing transverse momentum using $\sqrt(s) = 13$ TeV proton$-$proton collisions recorded by ATLAS in Run 2 of the LHC

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
JHEP 10 (2020) 062, 2020.
Inspire Record 1811596 DOI 10.17182/hepdata.93733

Results of a search for new particles decaying into eight or more jets and moderate missing transverse momentum are presented. The analysis uses 139 fb$^{-1}$ of proton$-$proton collision data at $\sqrt{s} = 13$ TeV collected by the ATLAS experiment at the Large Hadron Collider between 2015 and 2018. The selection rejects events containing isolated electrons or muons, and makes requirements according to the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. The search extends previous analyses both in using a larger dataset and by employing improved jet and missing transverse momentum reconstruction methods which more cleanly separate signal from background processes. No evidence for physics beyond the Standard Model is found. The results are interpreted in the context of supersymmetry-inspired simplified models, significantly extending the limits on the gluino mass in those models. In particular, limits on the gluino mass are set at 2 TeV when the lightest neutralino is nearly massless in a model assuming a two-step cascade decay via the lightest chargino and second-lightest neutralino.

67 data tables

Post-fit yields for data and prediction in each of the multi-bin signal regions for the 8 jet regions.

Post-fit yields for data and prediction in each of the multi-bin signal regions for the 9 jet regions.

Post-fit yields for data and prediction in each of the multi-bin signal regions for the 10 jet regions.

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Search for supersymmetry in proton-proton collisions at $\sqrt{s} =$ 13 TeV in events with high-momentum Z bosons and missing transverse momentum

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
JHEP 09 (2020) 149, 2020.
Inspire Record 1811111 DOI 10.17182/hepdata.96235

A search for new physics in events with two highly Lorentz-boosted Z bosons and large missing transverse momentum is presented. The analyzed proton-proton collision data, corresponding to an integrated luminosity of 137 fb$^{-1}$, were recorded at $\sqrt{s} =$ 13 TeV by the CMS experiment at the CERN LHC. The search utilizes the substructure of jets with large radius to identify quark pairs from Z boson decays. Backgrounds from standard model processes are suppressed by requirements on the jet mass and the missing transverse momentum. No significant excess in the event yield is observed beyond the number of background events expected from the standard model. For a simplified supersymmetric model in which the Z bosons arise from the decay of gluinos, an exclusion limit of 1920 GeV on the gluino mass is set at 95% confidence level. This is the first search for beyond-standard-model production of pairs of boosted Z bosons plus large missing transverse momentum.

14 data tables

Cross section upper limit vs m(GLUINO) for SMS model T5ZZ.

Cross section upper limit vs m(GLUINO) for SMS model T5ZZ.

Cross section upper limit vs m(GLUINO) for SMS model T5ZZ.

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Version 2
Search for a scalar partner of the top quark in the all-hadronic $t\bar{t}$ plus missing transverse momentum final state at $\sqrt{s}=13$ TeV with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
Eur.Phys.J.C 80 (2020) 737, 2020.
Inspire Record 1793461 DOI 10.17182/hepdata.93906

A search for direct pair production of scalar partners of the top quark (top squarks or scalar third-generation up-type leptoquarks) in the all-hadronic $t\bar{t}$ plus missing transverse momentum final state is presented. The analysis of 139 fb$^{-1}$ of ${\sqrt{s}=13}$ TeV proton-proton collision data collected using the ATLAS detector at the LHC yields no significant excess over the Standard Model background expectation. To interpret the results, a supersymmetric model is used where the top squark decays via $\tilde{t} \to t^{(*)} \tilde{\chi}^0_1$, with $t^{(*)}$ denoting an on-shell (off-shell) top quark and $\tilde{\chi}^0_1$ the lightest neutralino. Three specific event selections are optimised for the following scenarios. In the scenario where $m_{\tilde{t}}> m_t+m_{\tilde{\chi}^0_1}$, top squark masses are excluded in the range 400-1250 GeV for $\tilde{\chi}^0_1$ masses below $200$ GeV at 95 % confidence level. In the situation where $m_{\tilde{t}}\sim m_t+m_{\tilde{\chi}^0_1}$, top squark masses in the range 300-630 GeV are excluded, while in the case where $m_{\tilde{t}}< m_W+m_b+m_{\tilde{\chi}^0_1}$ (with $m_{\tilde{t}}-m_{\tilde{\chi}^0_1}\ge 5$ GeV), considered for the first time in an ATLAS all-hadronic search, top squark masses in the range 300-660 GeV are excluded. Limits are also set for scalar third-generation up-type leptoquarks, excluding leptoquarks with masses below $1240$ GeV when considering only leptoquark decays into a top quark and a neutrino.

118 data tables

<b>- - - - - - - - Overview of HEPData Record - - - - - - - -</b> <br><br> <b>Exclusion contours:</b> <ul> <li><a href="?table=stop_obs">Stop exclusion contour (Obs.)</a> <li><a href="?table=stop_obs_down">Stop exclusion contour (Obs. Down)</a> <li><a href="?table=stop_obs_up">Stop exclusion contour (Obs. Up)</a> <li><a href="?table=stop_exp">Stop exclusion contour (Exp.)</a> <li><a href="?table=stop_exp_down">Stop exclusion contour (Exp. Down)</a> <li><a href="?table=stop_exp_up">Stop exclusion contour (Exp. Up)</a> <li><a href="?table=LQ3u_obs">LQ3u exclusion contour (Obs.)</a> <li><a href="?table=LQ3u_obs_down">LQ3u exclusion contour (Obs. Down)</a> <li><a href="?table=LQ3u_obs_up">LQ3u exclusion contour (Obs. Up)</a> <li><a href="?table=LQ3u_exp">LQ3u exclusion contour (Exp.)</a> <li><a href="?table=LQ3u_exp_down">LQ3u exclusion contour (Exp. Down)</a> <li><a href="?table=LQ3u_exp_up">LQ3u exclusion contour (Exp. Up)</a> </ul> <b>Upper limits:</b> <ul> <li><a href="?table=stop_xSecUpperLimit_obs">stop_xSecUpperLimit_obs</a> <li><a href="?table=stop_xSecUpperLimit_exp">stop_xSecUpperLimit_exp</a> <li><a href="?table=LQ3u_xSecUpperLimit_obs">LQ3u_xSecUpperLimit_obs</a> <li><a href="?table=LQ3u_xSecUpperLimit_exp">LQ3u_xSecUpperLimit_exp</a> </ul> <b>Kinematic distributions:</b> <ul> <li><a href="?table=SRATW_metsigST">SRATW_metsigST</a> <li><a href="?table=SRBTT_m_1fatjet_kt12">SRBTT_m_1fatjet_kt12</a> <li><a href="?table=SRC_RISR">SRC_RISR</a> <li><a href="?table=SRD0_htSig">SRD0_htSig</a> <li><a href="?table=SRD1_htSig">SRD1_htSig</a> <li><a href="?table=SRD2_htSig">SRD2_htSig</a> </ul> <b>Cut flows:</b> <ul> <li><a href="?table=cutflow_SRATT">cutflow_SRATT</a> <li><a href="?table=cutflow_SRATW">cutflow_SRATW</a> <li><a href="?table=cutflow_SRAT0">cutflow_SRAT0</a> <li><a href="?table=cutflow_SRB">cutflow_SRB</a> <li><a href="?table=cutflow_SRC">cutflow_SRC</a> <li><a href="?table=cutflow_SRD0">cutflow_SRD0</a> <li><a href="?table=cutflow_SRD1">cutflow_SRD1</a> <li><a href="?table=cutflow_SRD2">cutflow_SRD2</a> </ul> <b>Acceptance and efficiencies:</b> As explained in <a href="https://twiki.cern.ch/twiki/bin/view/AtlasPublic/SupersymmetryPublicResults#summary_of_auxiliary_material">the twiki</a>. <ul> <li> <b>SRATT:</b> <a href="?table=Acc_SRATT">Acc_SRATT</a> <a href="?table=Eff_SRATT">Eff_SRATT</a> <li> <b>SRATW:</b> <a href="?table=Acc_SRATW">Acc_SRATW</a> <a href="?table=Eff_SRATW">Eff_SRATW</a> <li> <b>SRAT0:</b> <a href="?table=Acc_SRAT0">Acc_SRAT0</a> <a href="?table=Eff_SRAT0">Eff_SRAT0</a> <li> <b>SRBTT:</b> <a href="?table=Acc_SRBTT">Acc_SRBTT</a> <a href="?table=Eff_SRBTT">Eff_SRBTT</a> <li> <b>SRBTW:</b> <a href="?table=Acc_SRBTW">Acc_SRBTW</a> <a href="?table=Eff_SRBTW">Eff_SRBTW</a> <li> <b>SRBT0:</b> <a href="?table=Acc_SRBT0">Acc_SRBT0</a> <a href="?table=Eff_SRBT0">Eff_SRBT0</a> <li> <b>SRC1:</b> <a href="?table=Acc_SRC1">Acc_SRC1</a> <a href="?table=Eff_SRC1">Eff_SRC1</a> <li> <b>SRC2:</b> <a href="?table=Acc_SRC2">Acc_SRC2</a> <a href="?table=Eff_SRC2">Eff_SRC2</a> <li> <b>SRC3:</b> <a href="?table=Acc_SRC3">Acc_SRC3</a> <a href="?table=Eff_SRC3">Eff_SRC3</a> <li> <b>SRC4:</b> <a href="?table=Acc_SRC4">Acc_SRC4</a> <a href="?table=Eff_SRC4">Eff_SRC4</a> <li> <b>SRC5:</b> <a href="?table=Acc_SRC5">Acc_SRC5</a> <a href="?table=Eff_SRC5">Eff_SRC5</a> <li> <b>SRD0:</b> <a href="?table=Acc_SRD0">Acc_SRD0</a> <a href="?table=Eff_SRD0">Eff_SRD0</a> <li> <b>SRD1:</b> <a href="?table=Acc_SRD1">Acc_SRD1</a> <a href="?table=Eff_SRD1">Eff_SRD1</a> <li> <b>SRD2:</b> <a href="?table=Acc_SRD2">Acc_SRD2</a> <a href="?table=Eff_SRD2">Eff_SRD2</a> </ul> <b>Truth Code snippets</b> and <b>SLHA</a> files are available under "Resources" (purple button on the left)

<b>- - - - - - - - Overview of HEPData Record - - - - - - - -</b> <br><br> <b>Exclusion contours:</b> <ul> <li><a href="?table=stop_obs">Stop exclusion contour (Obs.)</a> <li><a href="?table=stop_obs_down">Stop exclusion contour (Obs. Down)</a> <li><a href="?table=stop_obs_up">Stop exclusion contour (Obs. Up)</a> <li><a href="?table=stop_exp">Stop exclusion contour (Exp.)</a> <li><a href="?table=stop_exp_down">Stop exclusion contour (Exp. Down)</a> <li><a href="?table=stop_exp_up">Stop exclusion contour (Exp. Up)</a> <li><a href="?table=LQ3u_obs">LQ3u exclusion contour (Obs.)</a> <li><a href="?table=LQ3u_obs_down">LQ3u exclusion contour (Obs. Down)</a> <li><a href="?table=LQ3u_obs_up">LQ3u exclusion contour (Obs. Up)</a> <li><a href="?table=LQ3u_exp">LQ3u exclusion contour (Exp.)</a> <li><a href="?table=LQ3u_exp_down">LQ3u exclusion contour (Exp. Down)</a> <li><a href="?table=LQ3u_exp_up">LQ3u exclusion contour (Exp. Up)</a> </ul> <b>Upper limits:</b> <ul> <li><a href="?table=stop_xSecUpperLimit_obs">stop_xSecUpperLimit_obs</a> <li><a href="?table=stop_xSecUpperLimit_exp">stop_xSecUpperLimit_exp</a> <li><a href="?table=LQ3u_xSecUpperLimit_obs">LQ3u_xSecUpperLimit_obs</a> <li><a href="?table=LQ3u_xSecUpperLimit_exp">LQ3u_xSecUpperLimit_exp</a> </ul> <b>Kinematic distributions:</b> <ul> <li><a href="?table=SRATW_metsigST">SRATW_metsigST</a> <li><a href="?table=SRBTT_m_1fatjet_kt12">SRBTT_m_1fatjet_kt12</a> <li><a href="?table=SRC_RISR">SRC_RISR</a> <li><a href="?table=SRD0_htSig">SRD0_htSig</a> <li><a href="?table=SRD1_htSig">SRD1_htSig</a> <li><a href="?table=SRD2_htSig">SRD2_htSig</a> </ul> <b>Cut flows:</b> <ul> <li><a href="?table=cutflow_SRATT">cutflow_SRATT</a> <li><a href="?table=cutflow_SRATW">cutflow_SRATW</a> <li><a href="?table=cutflow_SRAT0">cutflow_SRAT0</a> <li><a href="?table=cutflow_SRB">cutflow_SRB</a> <li><a href="?table=cutflow_SRC">cutflow_SRC</a> <li><a href="?table=cutflow_SRD0">cutflow_SRD0</a> <li><a href="?table=cutflow_SRD1">cutflow_SRD1</a> <li><a href="?table=cutflow_SRD2">cutflow_SRD2</a> </ul> <b>Acceptance and efficiencies:</b> As explained in <a href="https://twiki.cern.ch/twiki/bin/view/AtlasPublic/SupersymmetryPublicResults#summary_of_auxiliary_material">the twiki</a>. <ul> <li> <b>SRATT:</b> <a href="?table=Acc_SRATT">Acc_SRATT</a> <a href="?table=Eff_SRATT">Eff_SRATT</a> <li> <b>SRATW:</b> <a href="?table=Acc_SRATW">Acc_SRATW</a> <a href="?table=Eff_SRATW">Eff_SRATW</a> <li> <b>SRAT0:</b> <a href="?table=Acc_SRAT0">Acc_SRAT0</a> <a href="?table=Eff_SRAT0">Eff_SRAT0</a> <li> <b>SRBTT:</b> <a href="?table=Acc_SRBTT">Acc_SRBTT</a> <a href="?table=Eff_SRBTT">Eff_SRBTT</a> <li> <b>SRBTW:</b> <a href="?table=Acc_SRBTW">Acc_SRBTW</a> <a href="?table=Eff_SRBTW">Eff_SRBTW</a> <li> <b>SRBT0:</b> <a href="?table=Acc_SRBT0">Acc_SRBT0</a> <a href="?table=Eff_SRBT0">Eff_SRBT0</a> <li> <b>SRC1:</b> <a href="?table=Acc_SRC1">Acc_SRC1</a> <a href="?table=Eff_SRC1">Eff_SRC1</a> <li> <b>SRC2:</b> <a href="?table=Acc_SRC2">Acc_SRC2</a> <a href="?table=Eff_SRC2">Eff_SRC2</a> <li> <b>SRC3:</b> <a href="?table=Acc_SRC3">Acc_SRC3</a> <a href="?table=Eff_SRC3">Eff_SRC3</a> <li> <b>SRC4:</b> <a href="?table=Acc_SRC4">Acc_SRC4</a> <a href="?table=Eff_SRC4">Eff_SRC4</a> <li> <b>SRC5:</b> <a href="?table=Acc_SRC5">Acc_SRC5</a> <a href="?table=Eff_SRC5">Eff_SRC5</a> <li> <b>SRD0:</b> <a href="?table=Acc_SRD0">Acc_SRD0</a> <a href="?table=Eff_SRD0">Eff_SRD0</a> <li> <b>SRD1:</b> <a href="?table=Acc_SRD1">Acc_SRD1</a> <a href="?table=Eff_SRD1">Eff_SRD1</a> <li> <b>SRD2:</b> <a href="?table=Acc_SRD2">Acc_SRD2</a> <a href="?table=Eff_SRD2">Eff_SRD2</a> </ul> <b>Truth Code snippets</b> and <b>SLHA</a> files are available under "Resources" (purple button on the left)

The observed exclusion contour at 95% CL as a function of the $\it{m}_{\tilde{\chi}^{0}_{1}}$ vs. $\it{m}_{\tilde{t}}$. Masses that are within the contours are excluded.

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Version 2
Search for long-lived, massive particles in events with a displaced vertex and a muon with large impact parameter in $pp$ collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
Phys.Rev.D 102 (2020) 032006, 2020.
Inspire Record 1788448 DOI 10.17182/hepdata.91760

A search for long-lived particles decaying into hadrons and at least one muon is presented. The analysis selects events that pass a muon or missing-transverse-momentum trigger and contain a displaced muon track and a displaced vertex. The analyzed dataset of proton-proton collisions at $\sqrt{s} = 13$ TeV was collected with the ATLAS detector and corresponds to 136 fb$^{-1}$. The search employs dedicated reconstruction techniques that significantly increase the sensitivity to long-lived particle decays that occur in the ATLAS inner detector. Background estimates for Standard Model processes and instrumental effects are extracted from data. The observed event yields are compatible with those expected from background processes. The results are presented as limits at 95% confidence level on model-independent cross sections for processes beyond the Standard Model, and interpreted as exclusion limits in scenarios with pair-production of long-lived top squarks that decay via a small $R$-parity-violating coupling into a quark and a muon. Top squarks with masses up to 1.7 TeV are excluded for a lifetime of 0.1 ns, and masses below 1.3 TeV are excluded for lifetimes between 0.01 ns and 30 ns.

22 data tables

Vertex selection acceptance for the $\tilde{t}$ $R$-hadron benchmark model as a function of the transverse decay distance $r_{DV}$.

Vertex selection efficiency for the $\tilde{t}$ $R$-hadron benchmark model as a function of the transverse decay distance $r_{DV}$.

Track multiplicity $n_{Tracks}$ for preselected DVs in MET-triggered events with at least one muon passing the full selection. Along with the data shown with black markers, the stacked filled histograms represent the background estimates, and predictions for signal scenarios are overlaid with dashed lines. The errors include statistical and systematic uncertainties and are indicated by hatched bands. The DV full selection requirements, $n_{Tracks} \geq 3$ and $m_{DV} > 20$ GeV are visualized with a black arrow.

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Version 2
Search for chargino-neutralino production with mass splittings near the electroweak scale in three-lepton final states in $\sqrt{s}$ = 13 TeV $pp$ collisions with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
Phys.Rev.D 101 (2020) 072001, 2020.
Inspire Record 1771533 DOI 10.17182/hepdata.91127

A search for supersymmetry through the pair production of electroweakinos with mass splittings near the electroweak scale and decaying via on-shell $W$ and $Z$ bosons is presented for a three-lepton final state. The analyzed proton-proton collision data taken at a center-of-mass energy of $\sqrt{s}$ = 13 TeV were collected between 2015 and 2018 by the ATLAS experiment at the Large Hadron Collider, corresponding to an integrated luminosity of 139 fb$^{-1}$. A search, emulating the recursive jigsaw reconstruction technique with easily reproducible laboratory-frame variables, is performed. The two excesses observed in the 2015-2016 data recursive jigsaw analysis in the low-mass three-lepton phase space are reproduced. Results with the full dataset are in agreement with the Standard Model expectations. They are interpreted to set exclusion limits at 95% confidence level on simplified models of chargino-neutralino pair production for masses up to 345 GeV.

58 data tables

Distributions in SR-low of the data and post-fit background prediction for m<sub>T</sub>. The SR-low event selections are applied for each distribution except for the variable shown, where the selection is indicated by a red arrow. The normalization factor for the WZ background is derived from the background-only estimation described in Section 7. The expected distribution for a benchmark signal model is included for comparison. The first (last) bin includes underflow (overflow). The "Top-quark like" category contains the tt&#772;, Wt, and WW processes while the "Others" category contains backgrounds from triboson production and processes that include a Higgs boson, 3 or more tops, and tops produced in association with W or Z bosons. The bottom panel shows the ratio of the data to the post-fit background prediction. The hatched bands indicate the combined theoretical, experimental, and MC statistical uncertainties.

Distributions in SR-low of the data and post-fit background prediction for m<sub>T</sub>. The SR-low event selections are applied for each distribution except for the variable shown, where the selection is indicated by a red arrow. The normalization factor for the WZ background is derived from the background-only estimation described in Section 7. The expected distribution for a benchmark signal model is included for comparison. The first (last) bin includes underflow (overflow). The "Top-quark like" category contains the tt&#772;, Wt, and WW processes while the "Others" category contains backgrounds from triboson production and processes that include a Higgs boson, 3 or more tops, and tops produced in association with W or Z bosons. The bottom panel shows the ratio of the data to the post-fit background prediction. The hatched bands indicate the combined theoretical, experimental, and MC statistical uncertainties.

Distributions in SR-low of the data and post-fit background prediction for H<sup>boost</sup>. The SR-low event selections are applied for each distribution except for the variable shown, where the selection is indicated by a red arrow. The normalization factor for the WZ background is derived from the background-only estimation described in Section 7. The expected distribution for a benchmark signal model is included for comparison. The first (last) bin includes underflow (overflow). The "Top-quark like" category contains the tt&#772;, Wt, and WW processes while the "Others" category contains backgrounds from triboson production and processes that include a Higgs boson, 3 or more tops, and tops produced in association with W or Z bosons. The bottom panel shows the ratio of the data to the post-fit background prediction. The hatched bands indicate the combined theoretical, experimental, and MC statistical uncertainties.

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Version 2
Search for direct stau production in events with two hadronic $\tau$-leptons in $\sqrt{s} = 13$ TeV $pp$ collisions with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
Phys.Rev.D 101 (2020) 032009, 2020.
Inspire Record 1765529 DOI 10.17182/hepdata.92006

A search for the direct production of the supersymmetric partners of $\tau$-leptons (staus) in final states with two hadronically decaying $\tau$-leptons is presented. The analysis uses a dataset of $pp$ collisions corresponding to an integrated luminosity of $139$ fb$^{-1}$, recorded with the ATLAS detector at the Large Hadron Collider at a center-of-mass energy of 13 TeV. No significant deviation from the expected Standard Model background is observed. Limits are derived in scenarios of direct production of stau pairs with each stau decaying into the stable lightest neutralino and one $\tau$-lepton in simplified models where the two stau mass eigenstates are degenerate. Stau masses from 120 GeV to 390 GeV are excluded at 95% confidence level for a massless lightest neutralino.

52 data tables

The observed upper limits on the model cross-section in units of pb for simplified models with combined ${\tilde{\tau}}^{+}_{R,L} {\tilde{\tau}}^{-}_{R,L}$ production. Three points at ${M({\tilde{\chi}}^{0}_{1})}=200GeV$ were removed from the plot but kept in the table because they overlapped with the plot's legend and are far from the exclusion contour.

The observed upper limits on the model cross-section in units of pb for simplified models with combined ${\tilde{\tau}}^{+}_{R,L} {\tilde{\tau}}^{-}_{R,L}$ production. Three points at ${M({\tilde{\chi}}^{0}_{1})}=200GeV$ were removed from the plot but kept in the table because they overlapped with the plot's legend and are far from the exclusion contour.

The observed upper limits on the model cross-section in units of pb for simplified models with ${\tilde{\tau}}_L {\tilde{\tau}}_L$ only production. Three points at $M({\tilde{\chi}}^{0}_{1})=200GeV$ were removed from the plot but kept in the table because they overlapped with the plot's legend and are far from the exclusion contour.

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Version 4
Search for direct production of electroweakinos in final states with one lepton, missing transverse momentum and a Higgs boson decaying into two $b$-jets in (pp) collisions at $\sqrt{s}=13$ TeV with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
Eur.Phys.J.C 80 (2020) 691, 2020.
Inspire Record 1755298 DOI 10.17182/hepdata.90607

The results of a search for electroweakino pair production $pp \rightarrow \tilde\chi^\pm_1 \tilde\chi^0_2$ in which the chargino ($\tilde\chi^\pm_1$) decays into a $W$ boson and the lightest neutralino ($\tilde\chi^0_1$), while the heavier neutralino ($\tilde\chi^0_2$) decays into the Standard Model 125 GeV Higgs boson and a second $\tilde\chi^0_1$ are presented. The signal selection requires a pair of $b$-tagged jets consistent with those from a Higgs boson decay, and either an electron or a muon from the $W$ boson decay, together with missing transverse momentum from the corresponding neutrino and the stable neutralinos. The analysis is based on data corresponding to 139 $\mathrm{fb}^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collisions provided by the Large Hadron Collider and recorded by the ATLAS detector. No statistically significant evidence of an excess of events above the Standard Model expectation is found. Limits are set on the direct production of the electroweakinos in simplified models, assuming pure wino cross-sections. Masses of $\tilde{\chi}^{\pm}_{1}/\tilde{\chi}^{0}_{2}$ up to 740 GeV are excluded at 95% confidence level for a massless $\tilde{\chi}^{0}_{1}$.

212 data tables

The post-fit $m_{CT}$ distribution is shown in the validation region VR-onLM after all the selection requirements are applied other than the $m_{CT}$ cut. The stacked histograms show the expected SM backgrounds. The hatched bands represent the sum in quadrature of systematic and statistical uncertainties of the total SM background. The red line with arrow indicates the $m_{CT}$ cut used in SR selection. The first and the last bin include the underflow and overflow events (where present), respectively.

The post-fit $m_{CT}$ distribution is shown in the validation region VR-onLM after all the selection requirements are applied other than the $m_{CT}$ cut. The stacked histograms show the expected SM backgrounds. The hatched bands represent the sum in quadrature of systematic and statistical uncertainties of the total SM background. The red line with arrow indicates the $m_{CT}$ cut used in SR selection. The first and the last bin include the underflow and overflow events (where present), respectively.

The post-fit $m_{CT}$ distribution is shown in the validation region VR-onLM after all the selection requirements are applied other than the $m_{CT}$ cut. The stacked histograms show the expected SM backgrounds. The hatched bands represent the sum in quadrature of systematic and statistical uncertainties of the total SM background. The red line with arrow indicates the $m_{CT}$ cut used in SR selection. The first and the last bin include the underflow and overflow events (where present), respectively.

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Version 4
Search for squarks and gluinos in final states with same-sign leptons and jets using 139 fb$^{-1}$ of data collected with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
JHEP 06 (2020) 046, 2020.
Inspire Record 1754675 DOI 10.17182/hepdata.91214

A search for supersymmetric partners of gluons and quarks is presented, involving signatures with jets and either two isolated leptons (electrons or muons) with the same electric charge, or at least three isolated leptons. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider between 2015 and 2018, corresponding to a total integrated luminosity of 139 fb$^{-1}$, is used for the search. No significant excess over the Standard Model expectation is observed. The results are interpreted in simplified supersymmetric models featuring both R-parity conservation and R-parity violation, raising the exclusion limits beyond those of previous ATLAS searches to 1600 GeV for gluino masses and 750 GeV for bottom and top squark masses in these scenarios.

120 data tables

Observed 95% CL exclusion contours in signal region Rpc2L0b on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g \to q \bar{q}^{'} \tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm \to W^\pm \tilde{\chi}_2^0$ and $ \tilde{\chi}_2^0 \to Z \tilde{\chi}_1^0$.

Observed 95% CL exclusion contours in signal region Rpc2L0b on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g \to q \bar{q}^{'} \tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm \to W^\pm \tilde{\chi}_2^0$ and $ \tilde{\chi}_2^0 \to Z \tilde{\chi}_1^0$.

Observed 95% CL exclusion contours in signal region Rpc2L0b on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g \to q \bar{q}^{'} \tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm \to W^\pm \tilde{\chi}_2^0$ and $ \tilde{\chi}_2^0 \to Z \tilde{\chi}_1^0$.

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Version 4
Search for electroweak production of charginos and sleptons decaying into final states with two leptons and missing transverse momentum in $\sqrt{s}=13$ TeV $pp$ collisions using the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
Eur.Phys.J.C 80 (2020) 123, 2020.
Inspire Record 1750597 DOI 10.17182/hepdata.89413

A search for the electroweak production of charginos and sleptons decaying into final states with two electrons or muons is presented. The analysis is based on 139 fb$^{-1}$ of proton-proton collisions recorded by the ATLAS detector at the Large Hadron Collider at $\sqrt{s}=13$ TeV. Three $R$-parity-conserving scenarios where the lightest neutralino is the lightest supersymmetric particle are considered: the production of chargino pairs with decays via either $W$ bosons or sleptons, and the direct production of slepton pairs. The analysis is optimised for the first of these scenarios, but the results are also interpreted in the others. No significant deviations from the Standard Model expectations are observed and limits at 95 % confidence level are set on the masses of relevant supersymmetric particles in each of the scenarios. For a massless lightest neutralino, masses up to 420 GeV are excluded for the production of the lightest-chargino pairs assuming $W$-boson-mediated decays and up to 1 TeV for slepton-mediated decays, whereas for slepton-pair production masses up to 700 GeV are excluded assuming three generations of mass-degenerate sleptons.

462 data tables

- - - - - - - - Overview of HEPData Record - - - - - - - - <br/><br/> <b>Background Fit results:</b> <ul> <li><a href="89413?version=1&table=Backgroundfit1">CRs</a> <li><a href="89413?version=1&table=Backgroundfit2">VRs</a> <li><a href="89413?version=1&table=Backgroundfit5">inclusive DF-0J SRs</a> <li><a href="89413?version=1&table=Backgroundfit6">inclusive DF-1J SRs</a> <li><a href="89413?version=1&table=Backgroundfit3">inclusive SF-0J SRs</a> <li><a href="89413?version=1&table=Backgroundfit4">inclusive SF-1J SRs</a> </ul> <b>Kinematic distributions in VRs:</b> <ul> <li><a href="89413?version=1&table=VRkinematics1">$m_{T2}$ in VR-top-low</a> <li><a href="89413?version=1&table=VRkinematics2">$m_{T2}$ in VR-top-high</a> <li><a href="89413?version=1&table=VRkinematics3">$E_T^{miss}$ in VR-WW-0J</a> <li><a href="89413?version=1&table=VRkinematics4">$E_T^{miss}$ in VR-WW-1J</a> <li><a href="89413?version=1&table=VRkinematics5">$E_T^{miss}$ sig in VR-VZ</a> <li><a href="89413?version=1&table=VRkinematics6">$E_T^{miss}$ sig in VR-top-WW</a> </ul> <b>Kinematic distributions in SRs:</b> <ul> <li><a href="89413?version=1&table=SRkinematics1">$m_{T2}$ in SR-SF-0J</a> <li><a href="89413?version=1&table=SRkinematics2">$m_{T2}$ in SR-SF-1J</a> <li><a href="89413?version=1&table=SRkinematics3">$m_{T2}$ in SR-DF-0J</a> <li><a href="89413?version=1&table=SRkinematics4">$m_{T2}$ in SR-DF-1J</a> </ul> <b>Systematic uncertaities:</b> <ul> <li><a href="89413?version=1&table=Systematic uncertainties">dominant systematic uncertainties in the inclusive SRs</a> </ul> <b>Exclusion contours:</b> <ul> <li><a href="89413?version=1&table=Exclusioncontour(obs)1">expected exclusion contour direct chargino-pair production via W decay grid</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)1">observed exclusion contour direct chargino-pair production via W decay grid</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)2">expected exclusion contour direct chargino-pair production via slepton decay grid</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)2">observed exclusion contour direct chargino-pair production via slepton decay grid</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)3">expected exclusion contour direct slepton-pair production grid</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)3">observed exclusion contour direct slepton-pair production grid</a> </ul> <br/><br/><b>AUXILIARY MATERIAL</b><br/> <b>Background Fit in binned SRs:</b> <ul> <li><a href="89413?version=1&table=Backgroundfit7">binned DF-0J SRs</a> <li><a href="89413?version=1&table=Backgroundfit8">binned DF-1J SRs</a> <li><a href="89413?version=1&table=Backgroundfit9">binned SF-0J SRs</a> <li><a href="89413?version=1&table=Backgroundfit10">binned SF-1J SRs</a> </ul> <b>Exclusion contours:</b> <ul> <li><a href="89413?version=1&table=Exclusioncontour(obs)4">expected exclusion contour left-handed slepton-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)4">observed exclusion contour left-handed slepton-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)5">expected exclusion contour right-handed slepton-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)5">observed exclusion contour right-handed slepton-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)6">expected exclusion contour selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)6">observed exclusion contour selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)7">expected exclusion contour left-handed selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)7">observed exclusion contour left-handed selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)8">expected exclusion contour right-handed selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)8">observed exclusion contour right-handed selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)9">expected exclusion contour smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)9">observed exclusion contour smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)10">expected exclusion contour left-handed smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)10">observed exclusion contour left-handed smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)11">expected exclusion contour right-handed smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)11">observed exclusion contour right-handed smuon-pair production</a> </ul> <b>Cross section upper limits:</b> <ul> <li><a href="89413?version=1&table=xsecupperlimits1">upper limits on signal cross section for direct chargino-pair production via W decay</a> <li><a href="89413?version=1&table=xsecupperlimits2">upper limits on signal cross section for direct chargino-pair production via slepton decay</a> <li><a href="89413?version=1&table=xsecupperlimits3">upper limits on signal cross section for direct slepton-pair production</a> </ul> <b>Acceptances and Efficiencies for direct chargino-pair production via W decay grid </b> <ul> <li> <b>Acceptance</b> <br/> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[100,inf)forC1C1WWgrid">SR-DF-0J-[100,inf) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[160,inf)forC1C1WWgrid">SR-DF-0J-[160,inf) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[100,120)forC1C1WWgrid">SR-DF-0J-[100,120) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[120,160)forC1C1WWgrid">SR-DF-0J-[120,160) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[100,105)forC1C1WWgrid">SR-DF-0J-[100,105) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[105,110)forC1C1WWgrid">SR-DF-0J-[105,110) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[110,120)forC1C1WWgrid">SR-DF-0J-[110,120) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[120,140)forC1C1WWgrid">SR-DF-0J-[120,140) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[140,160)forC1C1WWgrid">SR-DF-0J-[140,160) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[160,180)forC1C1WWgrid">SR-DF-0J-[160,180) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[180,220)forC1C1WWgrid">SR-DF-0J-[180,220) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[220,260)forC1C1WWgrid">SR-DF-0J-[220,260) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[260,inf)forC1C1WWgrid">SR-DF-0J-[260,inf) </a><br/> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[100,inf)forC1C1WWgrid">SR-DF-1J-[100,inf) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[160,inf)forC1C1WWgrid">SR-DF-1J-[160,inf) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[100,120)forC1C1WWgrid">SR-DF-1J-[100,120) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[120,160)forC1C1WWgrid">SR-DF-1J-[120,160) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[100,105)forC1C1WWgrid">SR-DF-1J-[100,105) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[105,110)forC1C1WWgrid">SR-DF-1J-[105,110) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[110,120)forC1C1WWgrid">SR-DF-1J-[110,120) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[120,140)forC1C1WWgrid">SR-DF-1J-[120,140) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[140,160)forC1C1WWgrid">SR-DF-1J-[140,160) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[160,180)forC1C1WWgrid">SR-DF-1J-[160,180) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[180,220)forC1C1WWgrid">SR-DF-1J-[180,220) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[220,260)forC1C1WWgrid">SR-DF-1J-[220,260) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[260,inf)forC1C1WWgrid">SR-DF-1J-[260,inf) </a><br/> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[100,inf)forC1C1WWgrid">SR-SF-0J-[100,inf) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[160,inf)forC1C1WWgrid">SR-SF-0J-[160,inf) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[100,120)forC1C1WWgrid">SR-SF-0J-[100,120) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[120,160)forC1C1WWgrid">SR-SF-0J-[120,160) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[100,105)forC1C1WWgrid">SR-SF-0J-[100,105) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[105,110)forC1C1WWgrid">SR-SF-0J-[105,110) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[110,120)forC1C1WWgrid">SR-SF-0J-[110,120) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[120,140)forC1C1WWgrid">SR-SF-0J-[120,140) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[140,160)forC1C1WWgrid">SR-SF-0J-[140,160) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[160,180)forC1C1WWgrid">SR-SF-0J-[160,180) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[180,220)forC1C1WWgrid">SR-SF-0J-[180,220) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[220,260)forC1C1WWgrid">SR-SF-0J-[220,260) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[260,inf)forC1C1WWgrid">SR-SF-0J-[260,inf) </a><br/> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[100,inf)forC1C1WWgrid">SR-SF-1J-[100,inf) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[160,inf)forC1C1WWgrid">SR-SF-1J-[160,inf) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[100,120)forC1C1WWgrid">SR-SF-1J-[100,120) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[120,160)forC1C1WWgrid">SR-SF-1J-[120,160) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[100,105)forC1C1WWgrid">SR-SF-1J-[100,105) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[105,110)forC1C1WWgrid">SR-SF-1J-[105,110) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[110,120)forC1C1WWgrid">SR-SF-1J-[110,120) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[120,140)forC1C1WWgrid">SR-SF-1J-[120,140) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[140,160)forC1C1WWgrid">SR-SF-1J-[140,160) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[160,180)forC1C1WWgrid">SR-SF-1J-[160,180) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[180,220)forC1C1WWgrid">SR-SF-1J-[180,220) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[220,260)forC1C1WWgrid">SR-SF-1J-[220,260) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[260,inf)forC1C1WWgrid">SR-SF-1J-[260,inf) </a><br/> <li> <b>Efficiency</b> <br/> <a href="89413?version=1&table=EfficiencySR-DF-0J-[100,inf)forC1C1WWgrid">SR-DF-0J-[100,inf) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[160,inf)forC1C1WWgrid">SR-DF-0J-[160,inf) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[100,120)forC1C1WWgrid">SR-DF-0J-[100,120) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[120,160)forC1C1WWgrid">SR-DF-0J-[120,160) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[100,105)forC1C1WWgrid">SR-DF-0J-[100,105) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[105,110)forC1C1WWgrid">SR-DF-0J-[105,110) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[110,120)forC1C1WWgrid">SR-DF-0J-[110,120) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[120,140)forC1C1WWgrid">SR-DF-0J-[120,140) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[140,160)forC1C1WWgrid">SR-DF-0J-[140,160) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[160,180)forC1C1WWgrid">SR-DF-0J-[160,180) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[180,220)forC1C1WWgrid">SR-DF-0J-[180,220) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[220,260)forC1C1WWgrid">SR-DF-0J-[220,260) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[260,inf)forC1C1WWgrid">SR-DF-0J-[260,inf) </a><br/> <a href="89413?version=1&table=EfficiencySR-DF-1J-[100,inf)forC1C1WWgrid">SR-DF-1J-[100,inf) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[160,inf)forC1C1WWgrid">SR-DF-1J-[160,inf) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[100,120)forC1C1WWgrid">SR-DF-1J-[100,120) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[120,160)forC1C1WWgrid">SR-DF-1J-[120,160) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[100,105)forC1C1WWgrid">SR-DF-1J-[100,105) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[105,110)forC1C1WWgrid">SR-DF-1J-[105,110) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[110,120)forC1C1WWgrid">SR-DF-1J-[110,120) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[120,140)forC1C1WWgrid">SR-DF-1J-[120,140) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[140,160)forC1C1WWgrid">SR-DF-1J-[140,160) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[160,180)forC1C1WWgrid">SR-DF-1J-[160,180) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[180,220)forC1C1WWgrid">SR-DF-1J-[180,220) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[220,260)forC1C1WWgrid">SR-DF-1J-[220,260) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[260,inf)forC1C1WWgrid">SR-DF-1J-[260,inf) </a><br/> <a href="89413?version=1&table=EfficiencySR-SF-0J-[100,inf)forC1C1WWgrid">SR-SF-0J-[100,inf) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[160,inf)forC1C1WWgrid">SR-SF-0J-[160,inf) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[100,120)forC1C1WWgrid">SR-SF-0J-[100,120) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[120,160)forC1C1WWgrid">SR-SF-0J-[120,160) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[100,105)forC1C1WWgrid">SR-SF-0J-[100,105) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[105,110)forC1C1WWgrid">SR-SF-0J-[105,110) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[110,120)forC1C1WWgrid">SR-SF-0J-[110,120) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[120,140)forC1C1WWgrid">SR-SF-0J-[120,140) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[140,160)forC1C1WWgrid">SR-SF-0J-[140,160) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[160,180)forC1C1WWgrid">SR-SF-0J-[160,180) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[180,220)forC1C1WWgrid">SR-SF-0J-[180,220) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[220,260)forC1C1WWgrid">SR-SF-0J-[220,260) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[260,inf)forC1C1WWgrid">SR-SF-0J-[260,inf) </a><br/> <a href="89413?version=1&table=EfficiencySR-SF-1J-[100,inf)forC1C1WWgrid">SR-SF-1J-[100,inf) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[160,inf)forC1C1WWgrid">SR-SF-1J-[160,inf) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[100,120)forC1C1WWgrid">SR-SF-1J-[100,120) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[120,160)forC1C1WWgrid">SR-SF-1J-[120,160) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[100,105)forC1C1WWgrid">SR-SF-1J-[100,105) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[105,110)forC1C1WWgrid">SR-SF-1J-[105,110) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[110,120)forC1C1WWgrid">SR-SF-1J-[110,120) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[120,140)forC1C1WWgrid">SR-SF-1J-[120,140) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[140,160)forC1C1WWgrid">SR-SF-1J-[140,160) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[160,180)forC1C1WWgrid">SR-SF-1J-[160,180) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[180,220)forC1C1WWgrid">SR-SF-1J-[180,220) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[220,260)forC1C1WWgrid">SR-SF-1J-[220,260) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[260,inf)forC1C1WWgrid">SR-SF-1J-[260,inf) </a><br/> </ul> <b>Cutflow:</b> <ul> <li><a href="89413?version=1&table=Cutflow1">Cutflow for direct chargino-pair production via W decay $m(\tilde{\chi}^{\pm}_1,\tilde{\chi}^{0}_1)=(300,50) GeV$</a> <li><a href="89413?version=1&table=Cutflow1">Cutflow for direct chargino-pair production via slepton decay $m(\tilde{\chi}^{\pm}_1,\tilde{l},\tilde{\chi}^{0}_1)=(600,300,1) GeV$</a> <li><a href="89413?version=1&table=Cutflow1">Cutflow for direct slepton-pair production $m(\tilde{l},\tilde{\chi}^{0}_1)=(400,200) GeV$</a> </ul> <b>Truth Code snippets</b> are available under "Resources" (purple button on the left)

- - - - - - - - Overview of HEPData Record - - - - - - - - <br/><br/> <b>Background Fit results:</b> <ul> <li><a href="89413?version=1&table=Backgroundfit1">CRs</a> <li><a href="89413?version=1&table=Backgroundfit2">VRs</a> <li><a href="89413?version=1&table=Backgroundfit5">inclusive DF-0J SRs</a> <li><a href="89413?version=1&table=Backgroundfit6">inclusive DF-1J SRs</a> <li><a href="89413?version=1&table=Backgroundfit3">inclusive SF-0J SRs</a> <li><a href="89413?version=1&table=Backgroundfit4">inclusive SF-1J SRs</a> </ul> <b>Kinematic distributions in VRs:</b> <ul> <li><a href="89413?version=1&table=VRkinematics1">$m_{T2}$ in VR-top-low</a> <li><a href="89413?version=1&table=VRkinematics2">$m_{T2}$ in VR-top-high</a> <li><a href="89413?version=1&table=VRkinematics3">$E_T^{miss}$ in VR-WW-0J</a> <li><a href="89413?version=1&table=VRkinematics4">$E_T^{miss}$ in VR-WW-1J</a> <li><a href="89413?version=1&table=VRkinematics5">$E_T^{miss}$ sig in VR-VZ</a> <li><a href="89413?version=1&table=VRkinematics6">$E_T^{miss}$ sig in VR-top-WW</a> </ul> <b>Kinematic distributions in SRs:</b> <ul> <li><a href="89413?version=1&table=SRkinematics1">$m_{T2}$ in SR-SF-0J</a> <li><a href="89413?version=1&table=SRkinematics2">$m_{T2}$ in SR-SF-1J</a> <li><a href="89413?version=1&table=SRkinematics3">$m_{T2}$ in SR-DF-0J</a> <li><a href="89413?version=1&table=SRkinematics4">$m_{T2}$ in SR-DF-1J</a> </ul> <b>Systematic uncertaities:</b> <ul> <li><a href="89413?version=1&table=Systematic uncertainties">dominant systematic uncertainties in the inclusive SRs</a> </ul> <b>Exclusion contours:</b> <ul> <li><a href="89413?version=1&table=Exclusioncontour(obs)1">expected exclusion contour direct chargino-pair production via W decay grid</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)1">observed exclusion contour direct chargino-pair production via W decay grid</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)2">expected exclusion contour direct chargino-pair production via slepton decay grid</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)2">observed exclusion contour direct chargino-pair production via slepton decay grid</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)3">expected exclusion contour direct slepton-pair production grid</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)3">observed exclusion contour direct slepton-pair production grid</a> </ul> <br/><br/><b>AUXILIARY MATERIAL</b><br/> <b>Background Fit in binned SRs:</b> <ul> <li><a href="89413?version=1&table=Backgroundfit7">binned DF-0J SRs</a> <li><a href="89413?version=1&table=Backgroundfit8">binned DF-1J SRs</a> <li><a href="89413?version=1&table=Backgroundfit9">binned SF-0J SRs</a> <li><a href="89413?version=1&table=Backgroundfit10">binned SF-1J SRs</a> </ul> <b>Exclusion contours:</b> <ul> <li><a href="89413?version=1&table=Exclusioncontour(obs)4">expected exclusion contour left-handed slepton-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)4">observed exclusion contour left-handed slepton-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)5">expected exclusion contour right-handed slepton-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)5">observed exclusion contour right-handed slepton-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)6">expected exclusion contour selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)6">observed exclusion contour selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)7">expected exclusion contour left-handed selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)7">observed exclusion contour left-handed selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)8">expected exclusion contour right-handed selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)8">observed exclusion contour right-handed selectron-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)9">expected exclusion contour smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)9">observed exclusion contour smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)10">expected exclusion contour left-handed smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)10">observed exclusion contour left-handed smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(obs)11">expected exclusion contour right-handed smuon-pair production</a> <li><a href="89413?version=1&table=Exclusioncontour(exp)11">observed exclusion contour right-handed smuon-pair production</a> </ul> <b>Cross section upper limits:</b> <ul> <li><a href="89413?version=1&table=xsecupperlimits1">upper limits on signal cross section for direct chargino-pair production via W decay</a> <li><a href="89413?version=1&table=xsecupperlimits2">upper limits on signal cross section for direct chargino-pair production via slepton decay</a> <li><a href="89413?version=1&table=xsecupperlimits3">upper limits on signal cross section for direct slepton-pair production</a> </ul> <b>Acceptances and Efficiencies for direct chargino-pair production via W decay grid </b> <ul> <li> <b>Acceptance</b> <br/> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[100,inf)forC1C1WWgrid">SR-DF-0J-[100,inf) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[160,inf)forC1C1WWgrid">SR-DF-0J-[160,inf) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[100,120)forC1C1WWgrid">SR-DF-0J-[100,120) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[120,160)forC1C1WWgrid">SR-DF-0J-[120,160) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[100,105)forC1C1WWgrid">SR-DF-0J-[100,105) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[105,110)forC1C1WWgrid">SR-DF-0J-[105,110) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[110,120)forC1C1WWgrid">SR-DF-0J-[110,120) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[120,140)forC1C1WWgrid">SR-DF-0J-[120,140) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[140,160)forC1C1WWgrid">SR-DF-0J-[140,160) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[160,180)forC1C1WWgrid">SR-DF-0J-[160,180) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[180,220)forC1C1WWgrid">SR-DF-0J-[180,220) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[220,260)forC1C1WWgrid">SR-DF-0J-[220,260) </a> <a href="89413?version=1&table=AcceptanceSR-DF-0J-[260,inf)forC1C1WWgrid">SR-DF-0J-[260,inf) </a><br/> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[100,inf)forC1C1WWgrid">SR-DF-1J-[100,inf) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[160,inf)forC1C1WWgrid">SR-DF-1J-[160,inf) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[100,120)forC1C1WWgrid">SR-DF-1J-[100,120) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[120,160)forC1C1WWgrid">SR-DF-1J-[120,160) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[100,105)forC1C1WWgrid">SR-DF-1J-[100,105) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[105,110)forC1C1WWgrid">SR-DF-1J-[105,110) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[110,120)forC1C1WWgrid">SR-DF-1J-[110,120) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[120,140)forC1C1WWgrid">SR-DF-1J-[120,140) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[140,160)forC1C1WWgrid">SR-DF-1J-[140,160) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[160,180)forC1C1WWgrid">SR-DF-1J-[160,180) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[180,220)forC1C1WWgrid">SR-DF-1J-[180,220) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[220,260)forC1C1WWgrid">SR-DF-1J-[220,260) </a> <a href="89413?version=1&table=AcceptanceSR-DF-1J-[260,inf)forC1C1WWgrid">SR-DF-1J-[260,inf) </a><br/> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[100,inf)forC1C1WWgrid">SR-SF-0J-[100,inf) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[160,inf)forC1C1WWgrid">SR-SF-0J-[160,inf) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[100,120)forC1C1WWgrid">SR-SF-0J-[100,120) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[120,160)forC1C1WWgrid">SR-SF-0J-[120,160) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[100,105)forC1C1WWgrid">SR-SF-0J-[100,105) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[105,110)forC1C1WWgrid">SR-SF-0J-[105,110) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[110,120)forC1C1WWgrid">SR-SF-0J-[110,120) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[120,140)forC1C1WWgrid">SR-SF-0J-[120,140) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[140,160)forC1C1WWgrid">SR-SF-0J-[140,160) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[160,180)forC1C1WWgrid">SR-SF-0J-[160,180) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[180,220)forC1C1WWgrid">SR-SF-0J-[180,220) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[220,260)forC1C1WWgrid">SR-SF-0J-[220,260) </a> <a href="89413?version=1&table=AcceptanceSR-SF-0J-[260,inf)forC1C1WWgrid">SR-SF-0J-[260,inf) </a><br/> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[100,inf)forC1C1WWgrid">SR-SF-1J-[100,inf) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[160,inf)forC1C1WWgrid">SR-SF-1J-[160,inf) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[100,120)forC1C1WWgrid">SR-SF-1J-[100,120) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[120,160)forC1C1WWgrid">SR-SF-1J-[120,160) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[100,105)forC1C1WWgrid">SR-SF-1J-[100,105) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[105,110)forC1C1WWgrid">SR-SF-1J-[105,110) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[110,120)forC1C1WWgrid">SR-SF-1J-[110,120) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[120,140)forC1C1WWgrid">SR-SF-1J-[120,140) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[140,160)forC1C1WWgrid">SR-SF-1J-[140,160) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[160,180)forC1C1WWgrid">SR-SF-1J-[160,180) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[180,220)forC1C1WWgrid">SR-SF-1J-[180,220) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[220,260)forC1C1WWgrid">SR-SF-1J-[220,260) </a> <a href="89413?version=1&table=AcceptanceSR-SF-1J-[260,inf)forC1C1WWgrid">SR-SF-1J-[260,inf) </a><br/> <li> <b>Efficiency</b> <br/> <a href="89413?version=1&table=EfficiencySR-DF-0J-[100,inf)forC1C1WWgrid">SR-DF-0J-[100,inf) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[160,inf)forC1C1WWgrid">SR-DF-0J-[160,inf) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[100,120)forC1C1WWgrid">SR-DF-0J-[100,120) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[120,160)forC1C1WWgrid">SR-DF-0J-[120,160) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[100,105)forC1C1WWgrid">SR-DF-0J-[100,105) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[105,110)forC1C1WWgrid">SR-DF-0J-[105,110) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[110,120)forC1C1WWgrid">SR-DF-0J-[110,120) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[120,140)forC1C1WWgrid">SR-DF-0J-[120,140) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[140,160)forC1C1WWgrid">SR-DF-0J-[140,160) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[160,180)forC1C1WWgrid">SR-DF-0J-[160,180) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[180,220)forC1C1WWgrid">SR-DF-0J-[180,220) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[220,260)forC1C1WWgrid">SR-DF-0J-[220,260) </a> <a href="89413?version=1&table=EfficiencySR-DF-0J-[260,inf)forC1C1WWgrid">SR-DF-0J-[260,inf) </a><br/> <a href="89413?version=1&table=EfficiencySR-DF-1J-[100,inf)forC1C1WWgrid">SR-DF-1J-[100,inf) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[160,inf)forC1C1WWgrid">SR-DF-1J-[160,inf) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[100,120)forC1C1WWgrid">SR-DF-1J-[100,120) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[120,160)forC1C1WWgrid">SR-DF-1J-[120,160) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[100,105)forC1C1WWgrid">SR-DF-1J-[100,105) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[105,110)forC1C1WWgrid">SR-DF-1J-[105,110) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[110,120)forC1C1WWgrid">SR-DF-1J-[110,120) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[120,140)forC1C1WWgrid">SR-DF-1J-[120,140) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[140,160)forC1C1WWgrid">SR-DF-1J-[140,160) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[160,180)forC1C1WWgrid">SR-DF-1J-[160,180) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[180,220)forC1C1WWgrid">SR-DF-1J-[180,220) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[220,260)forC1C1WWgrid">SR-DF-1J-[220,260) </a> <a href="89413?version=1&table=EfficiencySR-DF-1J-[260,inf)forC1C1WWgrid">SR-DF-1J-[260,inf) </a><br/> <a href="89413?version=1&table=EfficiencySR-SF-0J-[100,inf)forC1C1WWgrid">SR-SF-0J-[100,inf) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[160,inf)forC1C1WWgrid">SR-SF-0J-[160,inf) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[100,120)forC1C1WWgrid">SR-SF-0J-[100,120) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[120,160)forC1C1WWgrid">SR-SF-0J-[120,160) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[100,105)forC1C1WWgrid">SR-SF-0J-[100,105) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[105,110)forC1C1WWgrid">SR-SF-0J-[105,110) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[110,120)forC1C1WWgrid">SR-SF-0J-[110,120) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[120,140)forC1C1WWgrid">SR-SF-0J-[120,140) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[140,160)forC1C1WWgrid">SR-SF-0J-[140,160) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[160,180)forC1C1WWgrid">SR-SF-0J-[160,180) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[180,220)forC1C1WWgrid">SR-SF-0J-[180,220) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[220,260)forC1C1WWgrid">SR-SF-0J-[220,260) </a> <a href="89413?version=1&table=EfficiencySR-SF-0J-[260,inf)forC1C1WWgrid">SR-SF-0J-[260,inf) </a><br/> <a href="89413?version=1&table=EfficiencySR-SF-1J-[100,inf)forC1C1WWgrid">SR-SF-1J-[100,inf) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[160,inf)forC1C1WWgrid">SR-SF-1J-[160,inf) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[100,120)forC1C1WWgrid">SR-SF-1J-[100,120) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[120,160)forC1C1WWgrid">SR-SF-1J-[120,160) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[100,105)forC1C1WWgrid">SR-SF-1J-[100,105) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[105,110)forC1C1WWgrid">SR-SF-1J-[105,110) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[110,120)forC1C1WWgrid">SR-SF-1J-[110,120) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[120,140)forC1C1WWgrid">SR-SF-1J-[120,140) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[140,160)forC1C1WWgrid">SR-SF-1J-[140,160) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[160,180)forC1C1WWgrid">SR-SF-1J-[160,180) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[180,220)forC1C1WWgrid">SR-SF-1J-[180,220) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[220,260)forC1C1WWgrid">SR-SF-1J-[220,260) </a> <a href="89413?version=1&table=EfficiencySR-SF-1J-[260,inf)forC1C1WWgrid">SR-SF-1J-[260,inf) </a><br/> </ul> <b>Cutflow:</b> <ul> <li><a href="89413?version=1&table=Cutflow1">Cutflow for direct chargino-pair production via W decay $m(\tilde{\chi}^{\pm}_1,\tilde{\chi}^{0}_1)=(300,50) GeV$</a> <li><a href="89413?version=1&table=Cutflow1">Cutflow for direct chargino-pair production via slepton decay $m(\tilde{\chi}^{\pm}_1,\tilde{l},\tilde{\chi}^{0}_1)=(600,300,1) GeV$</a> <li><a href="89413?version=1&table=Cutflow1">Cutflow for direct slepton-pair production $m(\tilde{l},\tilde{\chi}^{0}_1)=(400,200) GeV$</a> </ul> <b>SimpleAnalysis framework implementation</b> of the search SRs is available under "Resources" (purple button on the left)

- - - - - - - - Overview of HEPData Record - - - - - - - - <br/><br/> <b>Background Fit results:</b> <ul> <li><a href="89413?version=3&table=Background fit 1">CRs</a> <li><a href="89413?version=3&table=Background fit 2">VRs</a> <li><a href="89413?version=3&table=Background fit 5">inclusive DF-0J SRs</a> <li><a href="89413?version=3&table=Background fit 6">inclusive DF-1J SRs</a> <li><a href="89413?version=3&table=Background fit 3">inclusive SF-0J SRs</a> <li><a href="89413?version=3&table=Background fit 4">inclusive SF-1J SRs</a> </ul> <b>Kinematic distributions in VRs:</b> <ul> <li><a href="89413?version=3&table=VR kinematics 1">$m_{T2}$ in VR-top-low</a> <li><a href="89413?version=3&table=VR kinematics 2">$m_{T2}$ in VR-top-high</a> <li><a href="89413?version=3&table=VR kinematics 3">$E_T^{miss}$ in VR-WW-0J</a> <li><a href="89413?version=3&table=VR kinematics 4">$E_T^{miss}$ in VR-WW-1J</a> <li><a href="89413?version=3&table=VR kinematics 5">$E_T^{miss}$ sig in VR-VZ</a> <li><a href="89413?version=3&table=VR kinematics 6">$E_T^{miss}$ sig in VR-top-WW</a> </ul> <b>Kinematic distributions in SRs:</b> <ul> <li><a href="89413?version=3&table=SR kinematics 1">$m_{T2}$ in SR-SF-0J</a> <li><a href="89413?version=3&table=SR kinematics 2">$m_{T2}$ in SR-SF-1J</a> <li><a href="89413?version=3&table=SR kinematics 3">$m_{T2}$ in SR-DF-0J</a> <li><a href="89413?version=3&table=SR kinematics 4">$m_{T2}$ in SR-DF-1J</a> </ul> <b>Systematic uncertaities:</b> <ul> <li><a href="89413?version=3&table=Systematic uncertainties">dominant systematic uncertainties in the inclusive SRs</a> </ul> <b>Exclusion contours:</b> <ul> <li><a href="89413?version=3&table=Exclusion contour (exp) 1">expected exclusion contour direct chargino-pair production via W decay grid</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 1">observed exclusion contour direct chargino-pair production via W decay grid</a> <li><a href="89413?version=3&table=Exclusion contour (exp) 2">expected exclusion contour direct chargino-pair production via slepton decay grid</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 2">observed exclusion contour direct chargino-pair production via slepton decay grid</a> <li><a href="89413?version=3&table=Exclusion contour (exp) 3">expected exclusion contour direct slepton-pair production grid</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 3">observed exclusion contour direct slepton-pair production grid</a> </ul> <br/><br/><b>AUXILIARY MATERIAL</b><br/> <b>Background Fit in binned SRs:</b> <ul> <li><a href="89413?version=3&table=Background fit 7">binned DF-0J SRs</a> <li><a href="89413?version=3&table=Background fit 8">binned DF-1J SRs</a> <li><a href="89413?version=3&table=Background fit 9">binned SF-0J SRs</a> <li><a href="89413?version=3&table=Background fit 10">binned SF-1J SRs</a> </ul> <b>Exclusion contours:</b> <ul> <li><a href="89413?version=3&table=Exclusion contour (exp) 4">expected exclusion contour left-handed slepton-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 4">observed exclusion contour left-handed slepton-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (exp) 5">expected exclusion contour right-handed slepton-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 5">observed exclusion contour right-handed slepton-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (exp) 6">expected exclusion contour selectron-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 6">observed exclusion contour selectron-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (exp) 7">expected exclusion contour left-handed selectron-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 7">observed exclusion contour left-handed selectron-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (exp) 8">expected exclusion contour right-handed selectron-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 8">observed exclusion contour right-handed selectron-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (exp) 9">expected exclusion contour smuon-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 9">observed exclusion contour smuon-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (exp) 10">expected exclusion contour left-handed smuon-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 10">observed exclusion contour left-handed smuon-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (exp) 11">expected exclusion contour right-handed smuon-pair production</a> <li><a href="89413?version=3&table=Exclusion contour (obs) 11">observed exclusion contour right-handed smuon-pair production</a> </ul> <b>Cross section upper limits:</b> <ul> <li><a href="89413?version=3&table=xsec upper limits 1">upper limits on signal cross section for direct chargino-pair production via W decay</a> <li><a href="89413?version=3&table=xsec upper limits 2">upper limits on signal cross section for direct chargino-pair production via slepton decay</a> <li><a href="89413?version=3&table=xsec upper limits 3">upper limits on signal cross section for direct slepton-pair production</a> </ul> <b>Acceptances and Efficiencies for direct chargino-pair production via W decay grid </b> <ul> <li> <b>Acceptance</b> <br/> <a href="89413?version=3&table=Acceptance SR-DF-0J-[100,inf) for C1C1WW grid">SR-DF-0J-[100,inf) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[160,inf) for C1C1WW grid">SR-DF-0J-[160,inf) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[100,120) for C1C1WW grid">SR-DF-0J-[100,120) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[120,160) for C1C1WW grid">SR-DF-0J-[120,160) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[100,105) for C1C1WW grid">SR-DF-0J-[100,105) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[105,110) for C1C1WW grid">SR-DF-0J-[105,110) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[110,120) for C1C1WW grid">SR-DF-0J-[110,120) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[120,140) for C1C1WW grid">SR-DF-0J-[120,140) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[140,160) for C1C1WW grid">SR-DF-0J-[140,160) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[160,180) for C1C1WW grid">SR-DF-0J-[160,180) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[180,220) for C1C1WW grid">SR-DF-0J-[180,220) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[220,260) for C1C1WW grid">SR-DF-0J-[220,260) </a> <a href="89413?version=3&table=Acceptance SR-DF-0J-[260,inf) for C1C1WW grid">SR-DF-0J-[260,inf) </a><br/> <a href="89413?version=3&table=Acceptance SR-DF-1J-[100,inf) for C1C1WW grid">SR-DF-1J-[100,inf) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[160,inf) for C1C1WW grid">SR-DF-1J-[160,inf) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[100,120) for C1C1WW grid">SR-DF-1J-[100,120) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[120,160) for C1C1WW grid">SR-DF-1J-[120,160) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[100,105) for C1C1WW grid">SR-DF-1J-[100,105) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[105,110) for C1C1WW grid">SR-DF-1J-[105,110) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[110,120) for C1C1WW grid">SR-DF-1J-[110,120) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[120,140) for C1C1WW grid">SR-DF-1J-[120,140) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[140,160) for C1C1WW grid">SR-DF-1J-[140,160) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[160,180) for C1C1WW grid">SR-DF-1J-[160,180) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[180,220) for C1C1WW grid">SR-DF-1J-[180,220) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[220,260) for C1C1WW grid">SR-DF-1J-[220,260) </a> <a href="89413?version=3&table=Acceptance SR-DF-1J-[260,inf) for C1C1WW grid">SR-DF-1J-[260,inf) </a><br/> <a href="89413?version=3&table=Acceptance SR-SF-0J-[100,inf) for C1C1WW grid">SR-SF-0J-[100,inf) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[160,inf) for C1C1WW grid">SR-SF-0J-[160,inf) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[100,120) for C1C1WW grid">SR-SF-0J-[100,120) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[120,160) for C1C1WW grid">SR-SF-0J-[120,160) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[100,105) for C1C1WW grid">SR-SF-0J-[100,105) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[105,110) for C1C1WW grid">SR-SF-0J-[105,110) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[110,120) for C1C1WW grid">SR-SF-0J-[110,120) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[120,140) for C1C1WW grid">SR-SF-0J-[120,140) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[140,160) for C1C1WW grid">SR-SF-0J-[140,160) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[160,180) for C1C1WW grid">SR-SF-0J-[160,180) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[180,220) for C1C1WW grid">SR-SF-0J-[180,220) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[220,260) for C1C1WW grid">SR-SF-0J-[220,260) </a> <a href="89413?version=3&table=Acceptance SR-SF-0J-[260,inf) for C1C1WW grid">SR-SF-0J-[260,inf) </a><br/> <a href="89413?version=3&table=Acceptance SR-SF-1J-[100,inf) for C1C1WW grid">SR-SF-1J-[100,inf) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[160,inf) for C1C1WW grid">SR-SF-1J-[160,inf) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[100,120) for C1C1WW grid">SR-SF-1J-[100,120) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[120,160) for C1C1WW grid">SR-SF-1J-[120,160) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[100,105) for C1C1WW grid">SR-SF-1J-[100,105) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[105,110) for C1C1WW grid">SR-SF-1J-[105,110) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[110,120) for C1C1WW grid">SR-SF-1J-[110,120) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[120,140) for C1C1WW grid">SR-SF-1J-[120,140) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[140,160) for C1C1WW grid">SR-SF-1J-[140,160) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[160,180) for C1C1WW grid">SR-SF-1J-[160,180) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[180,220) for C1C1WW grid">SR-SF-1J-[180,220) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[220,260) for C1C1WW grid">SR-SF-1J-[220,260) </a> <a href="89413?version=3&table=Acceptance SR-SF-1J-[260,inf) for C1C1WW grid">SR-SF-1J-[260,inf) </a><br/> <li> <b>Efficiency</b> <br/> <a href="89413?version=3&table=Efficiency SR-DF-0J-[100,inf) for C1C1WW grid">SR-DF-0J-[100,inf) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[160,inf) for C1C1WW grid">SR-DF-0J-[160,inf) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[100,120) for C1C1WW grid">SR-DF-0J-[100,120) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[120,160) for C1C1WW grid">SR-DF-0J-[120,160) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[100,105) for C1C1WW grid">SR-DF-0J-[100,105) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[105,110) for C1C1WW grid">SR-DF-0J-[105,110) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[110,120) for C1C1WW grid">SR-DF-0J-[110,120) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[120,140) for C1C1WW grid">SR-DF-0J-[120,140) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[140,160) for C1C1WW grid">SR-DF-0J-[140,160) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[160,180) for C1C1WW grid">SR-DF-0J-[160,180) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[180,220) for C1C1WW grid">SR-DF-0J-[180,220) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[220,260) for C1C1WW grid">SR-DF-0J-[220,260) </a> <a href="89413?version=3&table=Efficiency SR-DF-0J-[260,inf) for C1C1WW grid">SR-DF-0J-[260,inf) </a><br/> <a href="89413?version=3&table=Efficiency SR-DF-1J-[100,inf) for C1C1WW grid">SR-DF-1J-[100,inf) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[160,inf) for C1C1WW grid">SR-DF-1J-[160,inf) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[100,120) for C1C1WW grid">SR-DF-1J-[100,120) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[120,160) for C1C1WW grid">SR-DF-1J-[120,160) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[100,105) for C1C1WW grid">SR-DF-1J-[100,105) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[105,110) for C1C1WW grid">SR-DF-1J-[105,110) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[110,120) for C1C1WW grid">SR-DF-1J-[110,120) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[120,140) for C1C1WW grid">SR-DF-1J-[120,140) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[140,160) for C1C1WW grid">SR-DF-1J-[140,160) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[160,180) for C1C1WW grid">SR-DF-1J-[160,180) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[180,220) for C1C1WW grid">SR-DF-1J-[180,220) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[220,260) for C1C1WW grid">SR-DF-1J-[220,260) </a> <a href="89413?version=3&table=Efficiency SR-DF-1J-[260,inf) for C1C1WW grid">SR-DF-1J-[260,inf) </a><br/> <a href="89413?version=3&table=Efficiency SR-SF-0J-[100,inf) for C1C1WW grid">SR-SF-0J-[100,inf) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[160,inf) for C1C1WW grid">SR-SF-0J-[160,inf) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[100,120) for C1C1WW grid">SR-SF-0J-[100,120) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[120,160) for C1C1WW grid">SR-SF-0J-[120,160) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[100,105) for C1C1WW grid">SR-SF-0J-[100,105) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[105,110) for C1C1WW grid">SR-SF-0J-[105,110) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[110,120) for C1C1WW grid">SR-SF-0J-[110,120) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[120,140) for C1C1WW grid">SR-SF-0J-[120,140) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[140,160) for C1C1WW grid">SR-SF-0J-[140,160) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[160,180) for C1C1WW grid">SR-SF-0J-[160,180) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[180,220) for C1C1WW grid">SR-SF-0J-[180,220) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[220,260) for C1C1WW grid">SR-SF-0J-[220,260) </a> <a href="89413?version=3&table=Efficiency SR-SF-0J-[260,inf) for C1C1WW grid">SR-SF-0J-[260,inf) </a><br/> <a href="89413?version=3&table=Efficiency SR-SF-1J-[100,inf) for C1C1WW grid">SR-SF-1J-[100,inf) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[160,inf) for C1C1WW grid">SR-SF-1J-[160,inf) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[100,120) for C1C1WW grid">SR-SF-1J-[100,120) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[120,160) for C1C1WW grid">SR-SF-1J-[120,160) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[100,105) for C1C1WW grid">SR-SF-1J-[100,105) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[105,110) for C1C1WW grid">SR-SF-1J-[105,110) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[110,120) for C1C1WW grid">SR-SF-1J-[110,120) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[120,140) for C1C1WW grid">SR-SF-1J-[120,140) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[140,160) for C1C1WW grid">SR-SF-1J-[140,160) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[160,180) for C1C1WW grid">SR-SF-1J-[160,180) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[180,220) for C1C1WW grid">SR-SF-1J-[180,220) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[220,260) for C1C1WW grid">SR-SF-1J-[220,260) </a> <a href="89413?version=3&table=Efficiency SR-SF-1J-[260,inf) for C1C1WW grid">SR-SF-1J-[260,inf) </a><br/> </ul> <b>Cutflow:</b> <ul> <li><a href="89413?version=3&table=Cutflow 1">Cutflow for direct chargino-pair production via W decay $m(\tilde{\chi}^{\pm}_1,\tilde{\chi}^{0}_1)=(300,50) GeV$</a> <li><a href="89413?version=3&table=Cutflow 2">Cutflow for direct chargino-pair production via slepton decay $m(\tilde{\chi}^{\pm}_1,\tilde{l},\tilde{\chi}^{0}_1)=(600,300,1) GeV$</a> <li><a href="89413?version=3&table=Cutflow 3">Cutflow for direct slepton-pair production $m(\tilde{l},\tilde{\chi}^{0}_1)=(400,200) GeV$</a> </ul> <b>SimpleAnalysis framework implementation</b> of the search SRs is available under "Resources" (purple button on the left)

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Version 3
Search for bottom-squark pair production with the ATLAS detector in final states containing Higgs bosons, $b$-jets and missing transverse momentum

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
JHEP 12 (2019) 060, 2019.
Inspire Record 1748602 DOI 10.17182/hepdata.89408

The result of a search for the pair production of the lightest supersymmetric partner of the bottom quark ($\tilde{b}_{1}$) using 139 fb$^{-1}$ of proton-proton data collected at $\sqrt{s} = 13$ TeV by the ATLAS detector is reported. In the supersymmetric scenarios considered both of the bottom-squarks decay into a $b$-quark and the second-lightest neutralino, $\tilde{b}_{1} \rightarrow b + \tilde{\chi}^{0}_{2}$. Each $\tilde{\chi}^{0}_{2}$ is assumed to subsequently decay with 100% branching ratio into a Higgs boson ($h$) like the one in the Standard Model and the lightest neutralino: $\tilde{\chi}^{0}_{2} \rightarrow h + \tilde{\chi}^{0}_{1}$. The $\tilde{\chi}^{0}_{1}$ is assumed to be the lightest supersymmetric particle (LSP) and is stable. Two signal mass configurations are targeted: the first has a constant LSP mass of 60 GeV; and the second has a constant mass difference between the $\tilde{\chi}^{0}_{2}$ and $\tilde{\chi}^{0}_{1}$ of 130 GeV. The final states considered contain no charged leptons, three or more $b$-jets, and large missing transverse momentum. No significant excess of events over the Standard Model background expectation is observed in any of the signal regions considered. Limits at the 95% confidence level are placed in the supersymmetric models considered, and bottom-squarks with mass up to 1.5 TeV are excluded.

144 data tables

Distributions of ${E}_{\mathrm{T}}^{\mathrm{miss}}$ after the background-only fit. The backgrounds which contribute only a small amount (diboson, W+jets and ttbar+W/Z/h) are grouped and labelled as `Other'.

Distributions of ${E}_{\mathrm{T}}^{\mathrm{miss}}$ after the background-only fit. The backgrounds which contribute only a small amount (diboson, W+jets and ttbar+W/Z/h) are grouped and labelled as `Other'.

Distributions of ${E}_{\mathrm{T}}^{\mathrm{miss}}$ after the background-only fit. The backgrounds which contribute only a small amount (diboson, W+jets and ttbar+W/Z/h) are grouped and labelled as `Other'.

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Search for displaced vertices of oppositely charged leptons from decays of long-lived particles in $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector

The ATLAS collaboration Aad, Georges ; Abbott, Brad ; Abbott, Dale Charles ; et al.
Phys.Lett.B 801 (2020) 135114, 2020.
Inspire Record 1745920 DOI 10.17182/hepdata.90606

A search for long-lived particles decaying into an oppositely charged lepton pair, $\mu\mu$, $ee$, or $e\mu$, is presented using 32.8 fb$^{-1}$ of $pp$ collision data collected at $\sqrt{s}=13$ TeV by the ATLAS detector at the LHC. Candidate leptons are required to form a vertex, within the inner tracking volume of ATLAS, displaced from the primary $pp$ interaction region. No lepton pairs with an invariant mass greater than 12 GeV are observed, consistent with the background expectations derived from data. The detection efficiencies for generic resonances with lifetimes ($c\tau$) of 100-1000 mm decaying into a dilepton pair with masses between 0.1-1.0 TeV are presented as a function of $p_T$ and decay radius of the resonances to allow the extraction of upper limits on the cross sections for theoretical models. The result is also interpreted in a supersymmetric model in which the lightest neutralino, produced via squark-antisquark production, decays into $\ell^{+}\ell^{'-}\nu$ ($\ell, \ell^{'} = e$, $\mu$) with a finite lifetime due to the presence of R-parity violating couplings. Cross-section limits are presented for specific squark and neutralino masses. For a 700 GeV squark, neutralinos with masses of 50-500 GeV and mean proper lifetimes corresponding to $c\tau$ values between 1 mm to 6 m are excluded. For a 1.6 TeV squark, $c\tau$ values between 3 mm to 1 m are excluded for 1.3 TeV neutralinos.

0 data tables

Version 2
Search for heavy charged long-lived particles in the ATLAS detector in 31.6 fb$^{-1}$ of proton-proton collision data at $\sqrt{s} = 13$ TeV

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
Phys.Rev.D 99 (2019) 092007, 2019.
Inspire Record 1718558 DOI 10.17182/hepdata.86565

A search for heavy charged long-lived particles is performed using a data sample of 36.1 fb$^{-1}$ of proton-proton collisions at $\sqrt{s} = 13$ TeV collected by the ATLAS experiment at the Large Hadron Collider. The search is based on observables related to ionization energy loss and time of flight, which are sensitive to the velocity of heavy charged particles traveling significantly slower than the speed of light. Multiple search strategies for a wide range of lifetimes, corresponding to path lengths of a few meters, are defined as model-independently as possible, by referencing several representative physics cases that yield long-lived particles within supersymmetric models, such as gluinos/squarks ($R$-hadrons), charginos and staus. No significant deviations from the expected Standard Model background are observed. Upper limits at 95% confidence level are provided on the production cross sections of long-lived $R$-hadrons as well as directly pair-produced staus and charginos. These results translate into lower limits on the masses of long-lived gluino, sbottom and stop $R$-hadrons, as well as staus and charginos of 2000 GeV, 1250 GeV, 1340 GeV, 430 GeV and 1090 GeV, respectively.

30 data tables

- - - - - - - - Overview of HEPData Record - - - - - - - - <br/><br/> <b>Lower mass requirement for signal regions.</b> <ul> <li><a href="86565?version=1&table=Table1">Gluinos and squarks</a></li> <li><a href="86565?version=1&table=Table2">Staus and charginos</a></li> </ul> <b>Discovery regions:</b> <ul> <li><a href="86565?version=1&table=Table3">Yields</a></li> <li><a href="86565?version=1&table=Table6">p0-values and limits</a></li> </ul> <b>Signal yield tables:</b> <ul> <li><a href="86565?version=1&table=Table4">MS-agnostic R-hadron search</a></li> <li><a href="86565?version=1&table=Table5">Full-detector R-hadron search</a></li> <li><a href="86565?version=1&table=Table7">MS-agnostic search for metastable gluino R-hadrons</a></li> <li><a href="86565?version=1&table=Table8">Full-detector direct-stau search</a></li> <li><a href="86565?version=1&table=Table9">Full-detector chargino search</a></li> </ul> <b>Limits:</b> <ul> <li><a href="86565?version=1&table=Table10">Gluino R-hadron search</a></li> <li><a href="86565?version=1&table=Table11">Sbottom R-hadron search</a></li> <li><a href="86565?version=1&table=Table12">Stop R-hadron search</a></li> <li><a href="86565?version=1&table=Table13">Stau search</a></li> <li><a href="86565?version=1&table=Table14">Chargino search</a></li> <li><a href="86565?version=1&table=Table15">Meta-stable gluino R-hadron search</a></li> <li><a href="86565?version=1&table=Table17">Meta-stable gluino R-hadron search</a></li> </ul> <b>Acceptance and efficiency:</b> <ul> <li><a href="86565?version=1&table=Table16">MS-agnostic R-hadron search</a></li> </ul> <b>Truth quantities:</b> <ul> <li><a href="86565?version=1&table=Table18">Flavor composition of 800 GeV stop R-hadrons simulated using the generic model</a></li> <li><a href="86565?version=1&table=Table19">Flavor composition of 800 GeV anti-stop R-hadrons simulated using the generic model</a></li> <li><a href="86565?version=1&table=Table20">Flavor composition of 800 GeV stop R-hadrons simulated using the Regge model</a></li> <li><a href="86565?version=1&table=Table21">Flavor composition of 800 GeV anti-stop R-hadrons simulated using the Regge model</a></li> </ul> <b>Reinterpretation material:</b> <ul> <li><a href="86565?version=1&table=Table22">ETmiss trigger efficiency as function of true ETmiss</a></li> <li><a href="86565?version=1&table=Table23">Single-muon trigger efficiency as function of |eta| and beta</a></li> <li><a href="86565?version=1&table=Table24">Candidate reconstruction efficiency for ID+Calo selection</a></li> <li><a href="86565?version=1&table=Table25">Candidate reconstruction efficiency for loose selection</a></li> <li><a href="86565?version=1&table=Table26">Efficiency for a loose candidate to be promoted to a tight candidate</a></li> <li><a href="86565?version=1&table=Table27">Resolution and average of reconstructed dE/dx mass for a given simulated mass for ID+calo candidates</a></li> <li><a href="86565?version=1&table=Table28">Resolution and average of reconstructed ToF mass for a given simulated mass for ID+calo candidates</a></li> <li><a href="86565?version=1&table=Table29">Resolution and average of reconstructed ToF mass for a given simulated mass for FullDet candidates</a></li> </ul> <p><b>Pseudo-code snippets</b> and <b>example SLHA setups</b> are available in the "Resources" linked on the left, and more detailed reinterpretation material is available at <a href="http://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/SUSY-2016-32/hepdata_info.pdf">http://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/SUSY-2016-32/hepdata_info.pdf</a>.</p>

Lower mass requirement for signal regions.

Lower mass requirement for signal regions.

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Search for supersymmetry in events with a photon, jets, b-jets, and missing transverse momentum in proton-proton collisions at 13 TeV

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
Eur.Phys.J.C 79 (2019) 444, 2019.
Inspire Record 1716137 DOI 10.17182/hepdata.88396

A search for supersymmetry is presented based on events with at least one photon, jets, and large missing transverse momentum produced in proton-proton collisions at a center-of-mass energy of 13 TeV. The data correspond to an integrated luminosity of 35.9 fb$^{-1}$ and were recorded at the LHC with the CMS detector in 2016. The analysis characterizes signal-like events by categorizing the data into various signal regions based on the number of jets, the number of b-tagged jets, and the missing transverse momentum. No significant excess of events is observed with respect to the expectations from standard model processes. Limits are placed on the gluino and top squark pair production cross sections using several simplified models of supersymmetric particle production with gauge-mediated supersymmetry breaking. Depending on the model and the mass of the next-to-lightest supersymmetric particle, the production of gluinos with masses as large as 2120 GeV and the production of top squarks with masses as large as 1230 GeV are excluded at 95% confidence level.

36 data tables

Values of the predicted SM background events from various sources and observed events in each of the 25 signal regions.

Observed $95\%$ CL upper limit on the production cross section of gluinos in T5qqqqHG model.

Expected $95\%$ CL upper limit on the production cross section of gluinos in T5qqqqHG model.

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Search for an exotic decay of the Higgs boson to a pair of light pseudoscalars in the final state with two muons and two b quarks in pp collisions at 13 TeV

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
Phys.Lett.B 795 (2019) 398-423, 2019.
Inspire Record 1709317 DOI 10.17182/hepdata.91235

A search for exotic decays of the Higgs boson to a pair of light pseudoscalar particles a$_1$ is performed under the hypothesis that one of the pseudoscalars decays to a pair of opposite sign muons and the other decays to b$\overline{\mathrm{b}}$. Such signatures are predicted in a number of extensions of the standard model (SM), including next-to-minimal supersymmetry and two-Higgs-doublet models with an additional scalar singlet. The results are based on a data set of proton-proton collisions corresponding to an integrated luminosity of 35.9 fb$^{-1}$, accumulated with the CMS experiment at the CERN LHC in 2016 at a centre-of-mass energy of 13 TeV. No statistically significant excess is observed with respect to the SM backgrounds in the search region for pseudoscalar masses from 20 GeV to half of the Higgs boson mass. Upper limits at 95% confidence level are set on the product of the production cross section and branching fraction, $\sigma_{\mathrm{h}}\mathcal{B}$(h $\to$ a$_1$ a$_1$ $\to$ $\mu^+\mu^-\mathrm{b}\bar{\mathrm{b}}$), ranging from 5 to 33 fb, depending on the pseudoscalar mass. Corresponding limits on the branching fraction, assuming the SM prediction for $\sigma_{\mathrm{h}}$, are (1$-$7)$\times$ 10$^{-4}$.

2 data tables

Observed and expected upper limits at 95% CL on the product of the Higgs boson production cross section and B(h->aa->mumubb)

Observed and expected upper limits at 95% CL on the branching fraction of (h->aa->mumubb)


Search for heavy charged long-lived particles in proton-proton collisions at $\sqrt{s} = 13$ TeV using an ionisation measurement with the ATLAS detector

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
Phys.Lett.B 788 (2019) 96-116, 2019.
Inspire Record 1686832 DOI 10.17182/hepdata.83962

This Letter presents a search for heavy charged long-lived particles produced in proton-proton collisions at $\sqrt{s} = 13$ TeV at the LHC using a data sample corresponding to an integrated luminosity of 36.1 fb$^{-1}$ collected by the ATLAS experiment in 2015 and 2016. These particles are expected to travel with a velocity significantly below the speed of light, and therefore have a specific ionisation higher than any high-momentum Standard Model particle of unit charge. The pixel subsystem of the ATLAS detector is used in this search to measure the ionisation energy loss of all reconstructed charged particles which traverse the pixel detector. Results are interpreted assuming the pair production of $R$-hadrons as composite colourless states of a long-lived gluino and Standard Model partons. No significant deviation from Standard Model background expectations is observed, and lifetime-dependent upper limits on $R$-hadron production cross-sections and gluino masses are set, assuming the gluino always decays in two quarks and a stable neutralino. $R$-hadrons with lifetimes above 1.0 ns are excluded at the 95% confidence level, with lower limits on the gluino mass ranging between 1290 GeV and 2060 GeV. In the case of stable $R$-hadrons, the lower limit on the gluino mass at the 95% confidence level is 1890 GeV.

26 data tables

The number of events in each CR, VR, and SR for the predicted background, for the expected contribution from the signal model normalised to $36.1$ fb$^{-1}$, and in the observed data. The predicted background includes the statistical and systematic uncertainties, respectively. The uncertainty in the signal yield includes all systematic uncertainties except that in the theoretical cross-section.

The number of events in each CR, VR, and SR for the predicted background, for the expected contribution from the signal model normalised to $36.1$ fb$^{-1}$, and in the observed data. The predicted background includes the statistical and systematic uncertainties, respectively. The uncertainty in the signal yield includes all systematic uncertainties except that in the theoretical cross-section.

Expected number of $R$-hadron signal events at different stages of the selection, normalised to $36.1$ fb$^{-1}$. Shown for three different signal points is the number of events expected and the number of events expected in which the selected track has been matched to a generated $R$-hadron. If the gluino decays, it decays to a 100 GeV $\tilde{\chi}^{0}$ and SM quarks.

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Search for pair production of higgsinos in final states with at least three $b$-tagged jets in $\sqrt{s} = 13$ TeV $pp$ collisions using the ATLAS detector

The ATLAS collaboration Aaboud, M. ; Aad, Georges ; Abbott, Brad ; et al.
Phys.Rev.D 98 (2018) 092002, 2018.
Inspire Record 1677389 DOI 10.17182/hepdata.83418

A search for pair production of the supersymmetric partners of the Higgs boson (higgsinos $\tilde{H}$) in gauge-mediated scenarios is reported. Each higgsino is assumed to decay to a Higgs boson and a gravitino. Two complementary analyses, targeting high- and low-mass signals, are performed to maximize sensitivity. The two analyses utilize LHC $pp$ collision data at a center-of-mass energy $\sqrt{s} = 13$ TeV, the former with an integrated luminosity of 36.1 fb$^{-1}$ and the latter with 24.3 fb$^{-1}$, collected with the ATLAS detector in 2015 and 2016. The search is performed in events containing missing transverse momentum and several energetic jets, at least three of which must be identified as $b$-quark jets. No significant excess is found above the predicted background. Limits on the cross-section are set as a function of the mass of the $\tilde{H}$ in simplified models assuming production via mass-degenerate higgsinos decaying to a Higgs boson and a gravitino. Higgsinos with masses between 130 and 230 GeV and between 290 and 880 GeV are excluded at the 95% confidence level. Interpretations of the limits in terms of the branching ratio of the higgsino to a $Z$ boson or a Higgs boson are also presented, and a 45% branching ratio to a Higgs boson is excluded for $m_{\tilde{H}} \approx 400$ GeV.

16 data tables

Distribution of m(h1) for events passing the preselection criteria of the high-mass analysis.

Distribution of effective mass for events passing the preselection criteria of the high-mass analysis.

Exclusion limits on higgsino pair production. The results of the low-mass analysis are used below m(higgsino) = 300 GeV, while those of the high-mass analysis are used above. The figure shows the observed and expected 95% upper limits on the higgsino pair production cross-section as a function of m(higgsino).

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Search for new phenomena using the invariant mass distribution of same-flavour opposite-sign dilepton pairs in events with missing transverse momentum in $\sqrt{s}=13$ TeV $pp$ collisions with the ATLAS detector

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
Eur.Phys.J.C 78 (2018) 625, 2018.
Inspire Record 1675352 DOI 10.17182/hepdata.81726

A search for new phenomena in final states containing an $e^+e^-$ or $\mu^+\mu^-$ pair, jets, and large missing transverse momentum is presented. This analysis makes use of proton--proton collision data with an integrated luminosity of $36.1 \; \mathrm{fb}^{-1}$, collected during 2015 and 2016 at a centre-of-mass energy $\sqrt{s}$ = 13 TeV with the ATLAS detector at the Large Hadron Collider. The search targets the pair production of supersymmetric coloured particles (squarks or gluinos) and their decays into final states containing an $e^+e^-$ or $\mu^+\mu^-$ pair and the lightest neutralino ($\tilde{\chi}_1^0$) via one of two next-to-lightest neutralino ($\tilde{\chi}_2^0$) decay mechanisms: $\tilde{\chi}_2^0 \rightarrow Z \tilde{\chi}_1^0$, where the $Z$ boson decays leptonically leading to a peak in the dilepton invariant mass distribution around the $Z$ boson mass; and $\tilde{\chi}_2^0 \rightarrow \ell^+\ell^- \tilde{\chi}_1^0$ with no intermediate $\ell^+\ell^-$ resonance, yielding a kinematic endpoint in the dilepton invariant mass spectrum. The data are found to be consistent with the Standard Model expectation. Results are interpreted using simplified models, and exclude gluinos and squarks with masses as large as 1.85 TeV and 1.3 TeV at 95% confidence level, respectively.

43 data tables

Observed and expected dilepton mass distributions, with the bin boundaries considered for the interpretation, in SR-low. All statistical and systematic uncertainties of the expected background are included in the hatched band. An example signal from the slepton model with m(gluino) = 1200 GeV and m(neutralino1) = 900 GeV is overlaid.

Observed and expected dilepton mass distributions, with the bin boundaries considered for the interpretation, in SR-med. All statistical and systematic uncertainties of the expected background are included in the hatched band. An example signal from the slepton model with m(gluino) = 1600 GeV and m(neutralino1) = 900 GeV, and from an on-$Z$ model with m(gluino) = 1640 GeV and m(neutralino1) = 1160 GeV, is overlaid.

Observed and expected dilepton mass distributions, with the bin boundaries considered for the interpretation, in SR-high. All statistical and systematic uncertainties of the expected background are included in the hatched band. An example signal from the slepton model with m(gluino) = 1800 GeV and m(neutralino1) = 500 GeV, and from an on-$Z$ model with m(gluino) = 1650 GeV and m(neutralino1) = 550 GeV, is overlaid.

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Version 3
Search for supersymmetry in final states with charm jets and missing transverse momentum in 13 TeV $pp$ collisions with the ATLAS detector

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
JHEP 09 (2018) 050, 2018.
Inspire Record 1672099 DOI 10.17182/hepdata.83011

A search for supersymmetric partners of top quarks decaying as $\tilde{t}_1\to c\tilde\chi^0_1$ and supersymmetric partners of charm quarks decaying as $\tilde{c}_1\to c\tilde\chi^0_1$, where $\tilde\chi^0_1$ is the lightest neutralino, is presented. The search uses 36.1 ${\rm fb}^{-1}$ $pp$ collision data at a centre-of-mass energy of 13 TeV collected by the ATLAS experiment at the Large Hadron Collider and is performed in final states with jets identified as containing charm hadrons. Assuming a 100% branching ratio to $c\tilde\chi^0_1$, top and charm squarks with masses up to 850 GeV are excluded at 95% confidence level for a massless lightest neutralino. For $m_{\tilde{t}_1,\tilde{c}_1}-m_{\tilde\chi^0_1}

132 data tables

Acceptance for best expected CLS SR in the $\tilde{t}_1/\tilde{c}_1-\tilde{\chi}_1^0$ mass plane.

Acceptance for SR1 in the $\tilde{t}_1/\tilde{c}_1-\tilde{\chi}_1^0$ mass plane.

Acceptance for SR1 in the $\tilde{t}_1/\tilde{c}_1-\tilde{\chi}_1^0$ mass plane.

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Search for supersymmetry in events with four or more leptons in $\sqrt{s}=13$ TeV $pp$ collisions with ATLAS

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
Phys.Rev.D 98 (2018) 032009, 2018.
Inspire Record 1667045 DOI 10.17182/hepdata.82585

Results from a search for supersymmetry in events with four or more charged leptons (electrons, muons and taus) are presented. The analysis uses a data sample corresponding to 36.1 fb$^{-1}$ of proton-proton collisions delivered by the Large Hadron Collider at $\sqrt{s}=13$ TeV and recorded by the ATLAS detector. Four-lepton signal regions with up to two hadronically decaying taus are designed to target a range of supersymmetric scenarios that can be either enriched in or depleted of events involving the production and decay of a $Z$ boson. Data yields are consistent with Standard Model expectations and results are used to set upper limits on the event yields from processes beyond the Standard Model. Exclusion limits are set at the 95% confidence level in simplified models of General Gauge Mediated supersymmetry, where higgsino masses are excluded up to 295 GeV. In $R$-parity-violating simplified models with decays of the lightest supersymmetric particle to charged leptons, lower limits of 1.46 TeV, 1.06 TeV, and 2.25 TeV are placed on wino, slepton and gluino masses, respectively.

76 data tables

The $m_{\mathrm{eff}}$ distribution for events passing the signal region requirements except the $m_{\mathrm{eff}}$ requirement in SR0A and SR0B. Distributions for data, the estimated SM backgrounds, and an example SUSY scenario are shown. "Other" is the sum of the $tWZ$, $t\bar{t}WW$, and $t\bar{t}t\bar{t}$ backgrounds. The last bin captures the overflow events. Both the statistical and systematic uncertainties in the SM background are included in the shaded band. The red arrows indicate the $m_{\mathrm{eff}}$ selections in the signal regions.

The $E_{\mathrm{T}}^{\mathrm{miss}}$ distribution for events passing the signal region requirements except the $E_{\mathrm{T}}^{\mathrm{miss}}$ requirement in SR0C and SR0D. Distributions for data, the estimated SM backgrounds, and an example SUSY scenario are shown. "Other" is the sum of the $tWZ$, $t\bar{t}WW$, and $t\bar{t}t\bar{t}$ backgrounds. The last bin captures the overflow events. Both the statistical and systematic uncertainties in the SM background are included in the shaded band. The red arrows indicate the $E_{\mathrm{T}}^{\mathrm{miss}}$ selections in the signal regions.

The $m_{\mathrm{eff}}$ distribution for events passing the signal region requirements except the $m_{\mathrm{eff}}$ requirement in SR1. Distributions for data, the estimated SM backgrounds, and an example SUSY scenario are shown. "Other" is the sum of the $tWZ$, $t\bar{t}WW$, and $t\bar{t}t\bar{t}$ backgrounds. The last bin captures the overflow events. Both the statistical and systematic uncertainties in the SM background are included in the shaded band. The red arrows indicate the $m_{\mathrm{eff}}$ selections in the signal region.

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Search for photonic signatures of gauge-mediated supersymmetry in 13 TeV $pp$ collisions with the ATLAS detector

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
Phys.Rev.D 97 (2018) 092006, 2018.
Inspire Record 1654357 DOI 10.17182/hepdata.81626

A search is presented for photonic signatures, motivated by generalized models of gauge-mediated supersymmetry breaking. This search makes use of proton-proton collision data at $\sqrt{s}$ = 13 TeV corresponding to an integrated luminosity of 36.1 fb$^{-1}$ recorded by the ATLAS detector at the LHC, and it explores models dominated by both strong and electroweak production of supersymmetric partner states. Experimental signatures incorporating an isolated photon and significant missing transverse momentum are explored. These signatures include events with an additional photon or additional jet activity not associated with any specific underlying quark flavor. No significant excess of events is observed above the Standard Model prediction, and 95% confidence-level upper limits of between 0.083 fb and 0.32 fb are set on the visible cross section of contributions from physics beyond the Standard Model. These results are interpreted in terms of lower limits on the masses of gluinos, squarks, and gauginos in the context of generalized models of gauge-mediated supersymmetry, which reach as high as 2.3 TeV for strongly produced and 1.3 TeV for weakly produced supersymmetric partner pairs.

45 data tables

Distribution of the total visible transverse energy $H_{\mathrm{T}}$ for selected diphoton events, after requiring $\Delta\phi_{\mathrm{min}} (\mathrm{jet}, E_{\mathrm{T}}^{\mathrm{miss}}) > 0.5$ but before application of a requirement on $E_{\mathrm{T}}^{\mathrm{miss}}$ and $\Delta\phi_{\mathrm{min}} (\gamma, E_{\mathrm{T}}^{\mathrm{miss}})$ ($\gamma\gamma$ pre-selection). Also shown are the expected $H_{\mathrm{T}}$ distributions of contributing SM processes as well as those for two points each in the parameter spaces of the gluino-bino and wino-bino GGM models (mass values in GeV). Events outside the range of the displayed region are included in the highest-value bin.

Distribution of $R_{\mathrm{T}}^{4}$ for the sample satisfying all $\mathrm{SR}^{\gamma j}_{L}$ selection criteria except the $R_{\mathrm{T}}^{4}$ requirement itself, but with a relaxed requirement of $E_{\mathrm{T}}^{\mathrm{miss}} > 100$ GeV. Also shown are the expected $R_{\mathrm{T}}^{4}$ distributions of contributing SM processes as well as those for two 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, while the values of the $\tilde{\chi}^{0}_{1}$ mass arise from the choices $\mu = 400$ and $\mu = 600$ GeV, combined with the constraint that the branching fraction of $\tilde{\chi}^{0}_{1} \to \gamma\tilde{G}$ be 50%. The vertical dashed line and left-pointing arrow shows the region of the $R_{\mathrm{T}}^{4}$ observable selected for inclusion in $\mathrm{SR}^{\gamma j}_{L}$. Uncertainties are shown as hatched bands for the various expected sources of SM background (statistical only) and as error bars for data. The lower panels show the ratio of the data to the SM prediction.

Comparisons between expected and observed content of the validation and signal regions for the diphoton analysis. The uncertainties in the numbers of expected 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.

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Search for $R$-parity violating supersymmetry in pp collisions at $\sqrt{s} = $ 13 TeV using b jets in a final state with a single lepton, many jets, and high sum of large-radius jet masses

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
Phys.Lett.B 783 (2018) 114-139, 2018.
Inspire Record 1644901 DOI 10.17182/hepdata.81002

Results are reported from a search for physics beyond the standard model in proton-proton collisions at a center-of-mass energy of $\sqrt{s} = $ 13 TeV. The search uses a signature of a single lepton, large jet and bottom quark jet multiplicities, and high sum of large-radius jet masses, without any requirement on the missing transverse momentum in an event. The data sample corresponds to an integrated luminosity of 35.9 fb$^{-1}$ recorded by the CMS experiment at the LHC. No significant excess beyond the prediction from standard model processes is observed. The results are interpreted in terms of upper limits on the production cross section for $R$-parity violating supersymmetric extensions of the standard model using a benchmark model of gluino pair production, in which each gluino decays promptly via $ {\mathrm{\widetilde{g}}} \rightarrow \mathrm{t} \mathrm{b} \mathrm{s} $. Gluinos with a mass below 1610 GeV are excluded at 95% confidence level.

5 data tables

Figure 8. Observed cross section upper limits at 95% CL for a model of gluino pair production with gluino->tbs compared to the gluino pair production cross section.

Figure 8. Expected limits at 95% CL and their ±1 sigma variations for a model of gluino pair production with gluino->tbs compared to the gluino pair production cross section.

Figure 8. Expected limits at 95% CL and their ±2 sigma variations for a model of gluino pair production with gluino->tbs compared to the gluino pair production cross section.

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Version 5
Search for long-lived charginos based on a disappearing-track signature in $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
JHEP 06 (2018) 022, 2018.
Inspire Record 1641262 DOI 10.17182/hepdata.78375

This paper presents a search for direct electroweak gaugino or gluino pair production with a chargino nearly mass-degenerate with a stable neutralino. It is based on an integrated luminosity of 36.1 $\mathrm{fb}^{-1}$ of $pp$ collisions at $\sqrt{s} = 13$ TeV collected by the ATLAS experiment at the LHC. The final state of interest is a disappearing track accompanied by at least one jet with high transverse momentum from initial-state radiation or by four jets from the gluino decay chain. The use of short track segments reconstructed from the innermost tracking layers significantly improves the sensitivity to short chargino lifetimes. The results are found to be consistent with Standard Model predictions. Exclusion limits are set at 95% confidence level on the mass of charginos and gluinos for different chargino lifetimes. For a pure wino with a lifetime of about 0.2 ns, chargino masses up to 460 GeV are excluded. For the strong production channel, gluino masses up to 1.65 TeV are excluded assuming a chargino mass of 460 GeV and lifetime of 0.2 ns.

235 data tables

Pixel-tracklet $p_{T}$ spectrum of fake tracklet in electroweak channel in the low-Emiss region.

Pixel-tracklet $p_{T}$ spectrum of fake tracklet in electroweak channel in the low-Emiss region.

Pixel-tracklet $p_{T}$ spectrum of fake tracklet in electroweak channel in the low-Emiss region.

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Search for supersymmetry in proton-proton collisions at 13 TeV using identified top quarks

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
Phys.Rev.D 97 (2018) 012007, 2018.
Inspire Record 1633588 DOI 10.17182/hepdata.79808

A search for supersymmetry is presented based on proton-proton collision events containing identified hadronically decaying top quarks, no leptons, and an imbalance $p_\mathrm{T}^\text{miss}$ in transverse momentum. The data were collected with the CMS detector at the CERN LHC at a center-of-mass energy of 13 TeV, and correspond to an integrated luminosity of 35.9 fb$^{-1}$. Search regions are defined in terms of the multiplicity of bottom quark jet and top quark candidates, the $p_\mathrm{T}^\text{miss}$, the scalar sum of jet transverse momenta, and the $m_{\mathrm{T2}}$ mass variable. No statistically significant excess of events is observed relative to the expectation from the standard model. Lower limits on the masses of supersymmetric particles are determined at 95% confidence level in the context of simplified models with top quark production. For a model with direct top squark pair production followed by the decay of each top squark to a top quark and a neutralino, top squark masses up to 1020 GeV and neutralino masses up to 430 GeV are excluded. For a model with pair production of gluinos followed by the decay of each gluino to a top quark-antiquark pair and a neutralino, gluino masses up to 2040 GeV and neutralino masses up to 1150 GeV are excluded. These limits extend previous results.

20 data tables

Figure 8. The 95% CL upper limit on the production cross section of the T2tt simplified model as a function of the top squark and LSP masses. No interpretation is provided for signal models for which |mStop−mLSP−mTop|≤ 25 GeV and mStop≤ 275 GeV because signal events are essentially indistinguishable from SM ttbar events in this region, rendering the signal event acceptance difficult to model.

Figure 8. Observed exclusion region at 95% CL assuming 100% branching fraction.

Figure 8. Expected exclusion region at 95% CL assuming 100% branching fraction.

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A search for pair-produced resonances in four-jet final states at $\sqrt{s}$=13 TeV with the ATLAS detector

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
Eur.Phys.J.C 78 (2018) 250, 2018.
Inspire Record 1631641 DOI 10.17182/hepdata.79059

A search for massive coloured resonances which are pair-produced and decay into two jets is presented. The analysis uses 36.7 fb$^{-1}$ of $\sqrt{s}=$ 13 TeV pp collision data recorded by the ATLAS experiment at the LHC in 2015 and 2016. No significant deviation from the background prediction is observed. Results are interpreted in a SUSY simplified model where the lightest supersymmetric particle is the top squark, $\tilde{t}$, which decays promptly into two quarks through $R$-parity-violating couplings. Top squarks with masses in the range 100 GeV < $m_{\tilde{t}}$ < 410 GeV are excluded at 95% confidence level. If the decay is into a $b$-quark and a light quark, a dedicated selection requiring two $b$-tags is used to exclude masses in the ranges 100 GeV < $m_{\tilde{t}}$ < 470 GeV and 480 GeV < $m_{\tilde{t}}$ < 610 GeV. Additional limits are set on the pair-production of massive colour-octet resonances.

16 data tables

- - - - - - - - - - - - - - - - - - - - <p><b>Cutflows:</b><br> <a href="79059?version=1&table=CutflowTable1">Stop 100GeV</a><br> <a href="79059?version=1&table=CutflowTable2">Stop 500GeV</a><br> <a href="79059?version=1&table=CutflowTable3">Coloron 1500GeV</a><br> </p> <p><b>Event Yields:</b><br> <a href="79059?version=1&table=SRdistribution1">Inclusive stop SR</a><br> <a href="79059?version=1&table=SRdistribution2">Inclusive coloron SR </a><br> <a href="79059?version=1&table=SRdistribution3">b-tagged stop SR</a><br> </p> <p><b>Acceptances and Efficiencies:</b><br> <a href="79059?version=1&table=Acceptance1">Inclusive stop SR, before mass window</a><br> <a href="79059?version=1&table=Acceptance2">Inclusive stop SR, after mass window</a><br> <a href="79059?version=1&table=Acceptance3">Inclusive coloron SR, before mass window</a><br> <a href="79059?version=1&table=Acceptance4">Inclusive coloron SR, after mass window</a><br> <a href="79059?version=1&table=Acceptance5">b-tagged stop SR, before mass window</a><br> <a href="79059?version=1&table=Acceptance6">b-tagged stop SR, after mass window</a><br> </p> <p><b>Cross section upper limits:</b><br> <a href="79059?version=1&table=Limitoncrosssection1">Inclusive stop SR</a><br> <a href="79059?version=1&table=Limitoncrosssection2">Inclusive coloron SR</a><br> <a href="79059?version=1&table=Limitoncrosssection3">b-tagged stop SR</a><br> </p> <p><b>Truth Code</b> and <b>SLHA Files</b> for the cutflows are available under "Resources" (purple button on the left) </p>

Cutflow table for a pair produced top squark of 100 GeV decaying into a b- and an s-quark.

Cutflow table for a pair produced top squark of 500 GeV decaying into a b- and an s-quark.

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Version 3
A search for $B-L$ $R$-parity-violating top squarks in $\sqrt{s} = 13$ TeV $pp$ collisions with the ATLAS experiment

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
Phys.Rev.D 97 (2018) 032003, 2018.
Inspire Record 1630899 DOI 10.17182/hepdata.78376

A search is presented for the direct pair production of the stop, the supersymmetric partner of the top quark, that decays through an $R$-parity-violating coupling to a final state with two leptons and two jets, at least one of which is identified as a $b$-jet. The dataset corresponds to an integrated luminosity of 36.1 fb$^{-1}$ of proton-proton collisions at a center-of-mass energy of $\sqrt{s} = 13$ TeV, collected in 2015 and 2016 by the ATLAS detector at the LHC. No significant excess is observed over the Standard Model background, and exclusion limits are set on stop pair production at a 95% confidence level. Lower limits on the stop mass are set between 600 GeV and 1.5 TeV for branching ratios above 10% for decays to an electron or muon and a $b$-quark.

212 data tables

Signal acceptance (in %) in the (BRe,BRtau) plane for a 800 GeV stop, for the SR800 signal region.

Expected exclusion limit contour in the (BRe,BRtau) plane for a 600 GeV stop. All limits are computed at 95% CL.

Expected exclusion limit contour in the (BRe,BRtau) plane for a 600 GeV stop. All limits are computed at 95% CL.

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Version 2
Search for long-lived, massive particles in events with displaced vertices and missing transverse momentum in $\sqrt{s}$ = 13 TeV $pp$ collisions with the ATLAS detector

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
Phys.Rev.D 97 (2018) 052012, 2018.
Inspire Record 1630632 DOI 10.17182/hepdata.78697

A search for long-lived, massive particles predicted by many theories beyond the Standard Model is presented. The search targets final states with large missing transverse momentum and at least one high-mass displaced vertex with five or more tracks, and uses 32.8 fb$^{-1}$ of $\sqrt{s}$ = 13 TeV $pp$ collision data collected by the ATLAS detector at the LHC. The observed yield is consistent with the expected background. The results are used to extract 95\% CL exclusion limits on the production of long-lived gluinos with masses up to 2.37 TeV and lifetimes of $\mathcal{O}(10^{-2})$-$\mathcal{O}(10)$ ns in a simplified model inspired by Split Supersymmetry.

72 data tables

Vertex reconstruction efficiency as a function of radial position $R$ with and without the special LRT processing for one $R$-hadron signal sample with $m_{\tilde{g}} = 1.2$ TeV, $m_{\tilde{\chi}_{1}^{0}} = 100$ GeV and $\tau_{\tilde{g}} = 1$ ns. The efficiency is defined as the probability for a true LLP decay to be matched with a reconstructed DV fulfilling the vertex preselection criteria in events with a reconstructed primary vertex.

Vertex reconstruction efficiency as a function of radial position $R$ for two $R$-hadron signal samples with $m_{\tilde{g}} = 1.2$ TeV, $\tau_{\tilde{g}} = 1$ ns and different neutralino masses. The efficiency is defined as the probability for a true LLP decay to be matched with a reconstructed DV fulfilling the vertex preselection criteria in events with a reconstructed primary vertex.

Fractions of selected events for several signal MC samples with a gluino lifetime $\tau = 1$ ns, illustrating how $\mathcal{A}\times\varepsilon$ varies with the model parameters.

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Version 7
Search for a scalar partner of the top quark in the jets plus missing transverse momentum final state at $\sqrt{s}$=13 TeV with the ATLAS detector

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
JHEP 12 (2017) 085, 2017.
Inspire Record 1623207 DOI 10.17182/hepdata.79538

A search for pair production of a scalar partner of the top quark in events with four or more jets plus missing transverse momentum is presented. An analysis of 36.1 fb$^{-1}$ of $\sqrt{s}$=13 TeV proton-proton collisions collected using the ATLAS detector at the LHC yields no significant excess over the expected Standard Model background. To interpret the results a simplified supersymmetric model is used where the top squark is assumed to decay via $\tilde{t}_1 \rightarrow t^{(*)} \tilde\chi^0_1$ and $\tilde{t}_1\rightarrow b\tilde\chi^\pm_1 \rightarrow b W^{(*)} \tilde\chi^0_1$, where $\tilde\chi^0_1$ ($\chi^\pm_1$) denotes the lightest neutralino (chargino). Exclusion limits are placed in terms of the top-squark and neutralino masses. Assuming a branching ratio of 100% to $t \tilde\chi^0_1$, top-squark masses in the range 450-950 GeV are excluded for $\tilde\chi^0_1$ masses below 160 GeV. In the case where $m_{\tilde{t}_1}\sim m_t+m_{\tilde\chi^0_1}$, top-squark masses in the range 235-590 GeV are excluded.

581 data tables

Distribution of $E_\text{T}^\text{miss}$ for SRA-TT after the likelihood fit. The stacked histograms show the SM expectation and the hatched uncertainty band around the SM expectation shows the MC statistical and detector-related systematic uncertainties. A representative signal point is shown for each distribution.

Distribution of $E_\text{T}^\text{miss}$ for SRA-TT after the likelihood fit. The stacked histograms show the SM expectation and the hatched uncertainty band around the SM expectation shows the MC statistical and detector-related systematic uncertainties. A representative signal point is shown for each distribution.

Distribution of $E_\text{T}^\text{miss}$ for SRA-TT after the likelihood fit. The stacked histograms show the SM expectation and the hatched uncertainty band around the SM expectation shows the MC statistical and detector-related systematic uncertainties. A representative signal point is shown for each distribution.

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Version 2
Search for supersymmetry in events with $b$-tagged jets and missing transverse momentum in $pp$ collisions at $\sqrt{s}=13$ TeV with the ATLAS detector

The ATLAS collaboration Aaboud, Morad ; Aad, Georges ; Abbott, Brad ; et al.
JHEP 11 (2017) 195, 2017.
Inspire Record 1620694 DOI 10.17182/hepdata.79165

A search for the supersymmetric partners of the Standard Model bottom and top quarks is presented. The search uses 36.1 fb$^{-1}$ of $pp$ collision data at $\sqrt{s}=13$ TeV collected by the ATLAS experiment at the Large Hadron Collider. Direct production of pairs of bottom and top squarks ($\tilde{b}_{1}$ and $\tilde{t}_{1}$) is searched for in final states with $b$-tagged jets and missing transverse momentum. Distinctive selections are defined with either no charged leptons (electrons or muons) in the final state, or one charged lepton. The zero-lepton selection targets models in which the $\tilde{b}_{1}$ is the lightest squark and decays via $\tilde{b}_{1} \rightarrow b \tilde{\chi}^{0}_{1}$, where $\tilde{\chi}^{0}_{1}$ is the lightest neutralino. The one-lepton final state targets models where bottom or top squarks are produced and can decay into multiple channels, $\tilde{b}_{1} \rightarrow b \tilde{\chi}^{0}_{1}$ and $\tilde{b}_{1} \rightarrow t \tilde{\chi}^{\pm}_{1}$, or $\tilde{t}_{1} \rightarrow t \tilde{\chi}^{0}_{1}$ and $\tilde{t}_{1} \rightarrow b \tilde{\chi}^{\pm}_{1}$, where $\tilde{\chi}^{\pm}_{1}$ is the lightest chargino and the mass difference $m_{\tilde{\chi}^{\pm}_{1}}- m_{\tilde{\chi}^{0}_{1}}$ is set to 1 GeV. No excess above the expected Standard Model background is observed. Exclusion limits at 95\% confidence level on the mass of third-generation squarks are derived in various supersymmetry-inspired simplified models.

202 data tables

- - - - - - - - - - - - - - - - - - - - <br/><b>Acceptance:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=Acceptance1">b0L-SRA350</a> <a href="79165?version=1&table=Acceptance2">b0L-SRA450</a> <a href="79165?version=1&table=Acceptance3">b0L-SRA550</a> <a href="79165?version=1&table=Acceptance4">b0L-SRB</a> <a href="79165?version=1&table=Acceptance5">b0L-SRC</a> <a href="79165?version=1&table=Acceptance6">b0L-best</a><br/><i>asymmetric:</i> <a href="79165?version=1&table=Acceptance7">b1L-SRA300-2j</a> <a href="79165?version=1&table=Acceptance8">b1L-SRA450</a> <a href="79165?version=1&table=Acceptance9">b1L-SRA600</a> <a href="79165?version=1&table=Acceptance10">b1L-SRA750</a> <a href="79165?version=1&table=Acceptance11">b1L-SRB</a> <a href="79165?version=1&table=Acceptance12">b1L-best</a><br/><br/><b>Efficiency:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=Efficiency1">b0L-SRA350</a> <a href="79165?version=1&table=Efficiency2">b0L-SRA450</a> <a href="79165?version=1&table=Efficiency3">b0L-SRA550</a> <a href="79165?version=1&table=Efficiency4">b0L-SRB</a> <a href="79165?version=1&table=Efficiency5">b0L-SRC</a> <a href="79165?version=1&table=Efficiency6">b0L-best</a><br/><i>asymmetric:</i> <a href="79165?version=1&table=Efficiency7">b1L-SRA300-2j</a> <a href="79165?version=1&table=Efficiency8">b1L-SRA450</a> <a href="79165?version=1&table=Efficiency9">b1L-SRA600</a> <a href="79165?version=1&table=Efficiency10">b1L-SRA750</a> <a href="79165?version=1&table=Efficiency11">b1L-SRB</a> <a href="79165?version=1&table=Efficiency12">b1L-best</a><br/><br/><b>Best SR Mapping:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=BestSR4">b0L</a><br/><i>asymmetric:</i> <a href="79165?version=1&table=BestSR1">b1L</a> <a href="79165?version=1&table=BestSR2">b0L</a> <a href="79165?version=1&table=BestSR3">combined</a><br/><br/><b>Exclusion Contour:</b><br/><i>symmetric:</i> b0L-SRA350&nbsp;<a href="79165?version=1&table=Contour1">exp</a>&nbsp;<a href="79165?version=1&table=Contour2">obs</a> b0L-SRA450&nbsp;<a href="79165?version=1&table=Contour5">exp</a>&nbsp;<a href="79165?version=1&table=Contour6">obs</a> b0L-SRA550&nbsp;<a href="79165?version=1&table=Contour9">exp</a>&nbsp;<a href="79165?version=1&table=Contour10">obs</a> b0L-SRB&nbsp;<a href="79165?version=1&table=Contour11">exp</a>&nbsp;<a href="79165?version=1&table=Contour12">obs</a> b0L-SRC&nbsp;<a href="79165?version=1&table=Contour15">exp</a>&nbsp;<a href="79165?version=1&table=Contour16">obs</a> b0L-best&nbsp;<a href="79165?version=1&table=Contour17">exp</a>&nbsp;<a href="79165?version=1&table=Contour18">obs</a><br/><i>asymmetric:</i> b0L-SRA350&nbsp;<a href="79165?version=1&table=Contour3">exp</a>&nbsp;<a href="79165?version=1&table=Contour4">obs</a> b0L-SRA450&nbsp;<a href="79165?version=1&table=Contour7">exp</a>&nbsp;<a href="79165?version=1&table=Contour8">obs</a> b0L-SRB&nbsp;<a href="79165?version=1&table=Contour13">exp</a>&nbsp;<a href="79165?version=1&table=Contour14">obs</a> b0L-best&nbsp;<a href="79165?version=1&table=Contour19">exp</a>&nbsp;<a href="79165?version=1&table=Contour20">obs</a> b1L-SRA300-2j&nbsp;<a href="79165?version=1&table=Contour21">exp</a>&nbsp;<a href="79165?version=1&table=Contour22">obs</a> b1L-SRA450&nbsp;<a href="79165?version=1&table=Contour23">exp</a>&nbsp;<a href="79165?version=1&table=Contour24">obs</a> b1L-SRA600&nbsp;<a href="79165?version=1&table=Contour25">exp</a>&nbsp;<a href="79165?version=1&table=Contour26">obs</a> b1L-SRA750&nbsp;<a href="79165?version=1&table=Contour27">exp</a>&nbsp;<a href="79165?version=1&table=Contour28">obs</a> b1L-SRB&nbsp;<a href="79165?version=1&table=Contour29">exp</a>&nbsp;<a href="79165?version=1&table=Contour30">obs</a> b1L-best&nbsp;<a href="79165?version=1&table=Contour31">exp</a>&nbsp;<a href="79165?version=1&table=Contour32">obs</a> A-LowMass&nbsp;<a href="79165?version=1&table=Contour33">exp</a>&nbsp;<a href="79165?version=1&table=Contour34">obs</a> A-HighMass&nbsp;<a href="79165?version=1&table=Contour35">exp</a>&nbsp;<a href="79165?version=1&table=Contour36">obs</a> B combination&nbsp;<a href="79165?version=1&table=Contour37">exp</a>&nbsp;<a href="79165?version=1&table=Contour38">obs</a> Best combination&nbsp;<a href="79165?version=1&table=Contour39">exp</a>&nbsp;<a href="79165?version=1&table=Contour40">obs</a><br/><br/><b>SR Distribution:</b><br/><a href="79165?version=1&table=SRdistribution1">b0L-SRA</a>: $m_{\mathrm{CT}}$ <a href="79165?version=1&table=SRdistribution2">b0L-SRB</a>: $\mathrm{min[m_{T}(jet_{1-4}, E_{T}^{miss})]}$ <a href="79165?version=1&table=SRdistribution3">b0L-SRC</a>: ${\cal A}$ <a href="79165?version=1&table=SRdistribution4">b1L-SRA300-2j</a>: $\mathrm{m_{bb}}$ <a href="79165?version=1&table=SRdistribution5">b1L-SRA</a>: $\mathrm{m_{eff}}$ <a href="79165?version=1&table=SRdistribution6">b1L-SRB</a>: $\mathrm{m_{T}}$<br/><br/><b>Cross section upper limit:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=Limitoncrosssection1">b0L-best</a> <a href="79165?version=1&table=Limitoncrosssection2">b0L-SRA350</a> <a href="79165?version=1&table=Limitoncrosssection3">b0L-SRA450</a> <a href="79165?version=1&table=Limitoncrosssection4">b0L-SRA550</a> <a href="79165?version=1&table=Limitoncrosssection5">b0L-SRB</a> <a href="79165?version=1&table=Limitoncrosssection6">b0L-SRC</a><br/><i>asymmetric:</i> <a href="79165?version=1&table=Limitoncrosssection7">b0L-best</a> <a href="79165?version=1&table=Limitoncrosssection8">b0L-SRA350</a> <a href="79165?version=1&table=Limitoncrosssection9">b0L-SRA450</a> <a href="79165?version=1&table=Limitoncrosssection10">b0L-SRB</a> <a href="79165?version=1&table=Limitoncrosssection11">b1L-best</a> <a href="79165?version=1&table=Limitoncrosssection12">b1L-SRA300-2j</a> <a href="79165?version=1&table=Limitoncrosssection13">b1L-SRA450</a> <a href="79165?version=1&table=Limitoncrosssection14">b1L-SRA600</a> <a href="79165?version=1&table=Limitoncrosssection15">b1L-SRA750</a> <a href="79165?version=1&table=Limitoncrosssection16">b1L-SRB</a> <a href="79165?version=1&table=Limitoncrosssection17">best combination</a> <a href="79165?version=1&table=Limitoncrosssection18">A-LowMass</a> <a href="79165?version=1&table=Limitoncrosssection19">A-HighMass</a> <a href="79165?version=1&table=Limitoncrosssection20">B combination</a><br/><br/><b>Cutflow:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=CutflowTable1">b0L-SRA (1 TeV, 1 GeV)</a> <a href="79165?version=1&table=CutflowTable2">b0L-SRB (700 GeV, 450 GeV)</a> <a href="79165?version=1&table=CutflowTable3">b0L-SRC (450 GeV, 430 GeV)</a><br/><i>mixed:</i> <a href="79165?version=1&table=CutflowTable4">b1L-SRA (700 GeV, 300 GeV)</a> <a href="79165?version=1&table=CutflowTable5">b1L-SRA300-2j (700 GeV, 300 GeV)</a> <a href="79165?version=1&table=CutflowTable6">b0L-SRA (700 GeV, 300 GeV)</a><br/><br/><b>Truth Code</b> and <b>SLHA Files</b> for the cutflows are available under "Resources" (purple button on the left)

- - - - - - - - - - - - - - - - - - - - <br/><b>Acceptance:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=Acceptance1">b0L-SRA350</a> <a href="79165?version=1&table=Acceptance2">b0L-SRA450</a> <a href="79165?version=1&table=Acceptance3">b0L-SRA550</a> <a href="79165?version=1&table=Acceptance4">b0L-SRB</a> <a href="79165?version=1&table=Acceptance5">b0L-SRC</a> <a href="79165?version=1&table=Acceptance6">b0L-best</a><br/><i>asymmetric:</i> <a href="79165?version=1&table=Acceptance7">b1L-SRA300-2j</a> <a href="79165?version=1&table=Acceptance8">b1L-SRA450</a> <a href="79165?version=1&table=Acceptance9">b1L-SRA600</a> <a href="79165?version=1&table=Acceptance10">b1L-SRA750</a> <a href="79165?version=1&table=Acceptance11">b1L-SRB</a> <a href="79165?version=1&table=Acceptance12">b1L-best</a><br/><br/><b>Efficiency:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=Efficiency1">b0L-SRA350</a> <a href="79165?version=1&table=Efficiency2">b0L-SRA450</a> <a href="79165?version=1&table=Efficiency3">b0L-SRA550</a> <a href="79165?version=1&table=Efficiency4">b0L-SRB</a> <a href="79165?version=1&table=Efficiency5">b0L-SRC</a> <a href="79165?version=1&table=Efficiency6">b0L-best</a><br/><i>asymmetric:</i> <a href="79165?version=1&table=Efficiency7">b1L-SRA300-2j</a> <a href="79165?version=1&table=Efficiency8">b1L-SRA450</a> <a href="79165?version=1&table=Efficiency9">b1L-SRA600</a> <a href="79165?version=1&table=Efficiency10">b1L-SRA750</a> <a href="79165?version=1&table=Efficiency11">b1L-SRB</a> <a href="79165?version=1&table=Efficiency12">b1L-best</a><br/><br/><b>Best SR Mapping:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=BestSR4">b0L</a><br/><i>asymmetric:</i> <a href="79165?version=1&table=BestSR1">b1L</a> <a href="79165?version=1&table=BestSR2">b0L</a> <a href="79165?version=1&table=BestSR3">combined</a><br/><br/><b>Exclusion Contour:</b><br/><i>symmetric:</i> b0L-SRA350&nbsp;<a href="79165?version=1&table=Contour1">exp</a>&nbsp;<a href="79165?version=1&table=Contour2">obs</a> b0L-SRA450&nbsp;<a href="79165?version=1&table=Contour5">exp</a>&nbsp;<a href="79165?version=1&table=Contour6">obs</a> b0L-SRA550&nbsp;<a href="79165?version=1&table=Contour9">exp</a>&nbsp;<a href="79165?version=1&table=Contour10">obs</a> b0L-SRB&nbsp;<a href="79165?version=1&table=Contour11">exp</a>&nbsp;<a href="79165?version=1&table=Contour12">obs</a> b0L-SRC&nbsp;<a href="79165?version=1&table=Contour15">exp</a>&nbsp;<a href="79165?version=1&table=Contour16">obs</a> b0L-best&nbsp;<a href="79165?version=1&table=Contour17">exp</a>&nbsp;<a href="79165?version=1&table=Contour18">obs</a><br/><i>asymmetric:</i> b0L-SRA350&nbsp;<a href="79165?version=1&table=Contour3">exp</a>&nbsp;<a href="79165?version=1&table=Contour4">obs</a> b0L-SRA450&nbsp;<a href="79165?version=1&table=Contour7">exp</a>&nbsp;<a href="79165?version=1&table=Contour8">obs</a> b0L-SRB&nbsp;<a href="79165?version=1&table=Contour13">exp</a>&nbsp;<a href="79165?version=1&table=Contour14">obs</a> b0L-best&nbsp;<a href="79165?version=1&table=Contour19">exp</a>&nbsp;<a href="79165?version=1&table=Contour20">obs</a> b1L-SRA300-2j&nbsp;<a href="79165?version=1&table=Contour21">exp</a>&nbsp;<a href="79165?version=1&table=Contour22">obs</a> b1L-SRA450&nbsp;<a href="79165?version=1&table=Contour23">exp</a>&nbsp;<a href="79165?version=1&table=Contour24">obs</a> b1L-SRA600&nbsp;<a href="79165?version=1&table=Contour25">exp</a>&nbsp;<a href="79165?version=1&table=Contour26">obs</a> b1L-SRA750&nbsp;<a href="79165?version=1&table=Contour27">exp</a>&nbsp;<a href="79165?version=1&table=Contour28">obs</a> b1L-SRB&nbsp;<a href="79165?version=1&table=Contour29">exp</a>&nbsp;<a href="79165?version=1&table=Contour30">obs</a> b1L-best&nbsp;<a href="79165?version=1&table=Contour31">exp</a>&nbsp;<a href="79165?version=1&table=Contour32">obs</a> A-LowMass&nbsp;<a href="79165?version=1&table=Contour33">exp</a>&nbsp;<a href="79165?version=1&table=Contour34">obs</a> A-HighMass&nbsp;<a href="79165?version=1&table=Contour35">exp</a>&nbsp;<a href="79165?version=1&table=Contour36">obs</a> B combination&nbsp;<a href="79165?version=1&table=Contour37">exp</a>&nbsp;<a href="79165?version=1&table=Contour38">obs</a> Best combination&nbsp;<a href="79165?version=1&table=Contour39">exp</a>&nbsp;<a href="79165?version=1&table=Contour40">obs</a><br/><br/><b>SR Distribution:</b><br/><a href="79165?version=1&table=SRdistribution1">b0L-SRA</a>: $m_{\mathrm{CT}}$ <a href="79165?version=1&table=SRdistribution2">b0L-SRB</a>: $\mathrm{min[m_{T}(jet_{1-4}, E_{T}^{miss})]}$ <a href="79165?version=1&table=SRdistribution3">b0L-SRC</a>: ${\cal A}$ <a href="79165?version=1&table=SRdistribution4">b1L-SRA300-2j</a>: $\mathrm{m_{bb}}$ <a href="79165?version=1&table=SRdistribution5">b1L-SRA</a>: $\mathrm{m_{eff}}$ <a href="79165?version=1&table=SRdistribution6">b1L-SRB</a>: $\mathrm{m_{T}}$<br/><br/><b>Cross section upper limit:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=Limitoncrosssection1">b0L-best</a> <a href="79165?version=1&table=Limitoncrosssection2">b0L-SRA350</a> <a href="79165?version=1&table=Limitoncrosssection3">b0L-SRA450</a> <a href="79165?version=1&table=Limitoncrosssection4">b0L-SRA550</a> <a href="79165?version=1&table=Limitoncrosssection5">b0L-SRB</a> <a href="79165?version=1&table=Limitoncrosssection6">b0L-SRC</a><br/><i>asymmetric:</i> <a href="79165?version=1&table=Limitoncrosssection7">b0L-best</a> <a href="79165?version=1&table=Limitoncrosssection8">b0L-SRA350</a> <a href="79165?version=1&table=Limitoncrosssection9">b0L-SRA450</a> <a href="79165?version=1&table=Limitoncrosssection10">b0L-SRB</a> <a href="79165?version=1&table=Limitoncrosssection11">b1L-best</a> <a href="79165?version=1&table=Limitoncrosssection12">b1L-SRA300-2j</a> <a href="79165?version=1&table=Limitoncrosssection13">b1L-SRA450</a> <a href="79165?version=1&table=Limitoncrosssection14">b1L-SRA600</a> <a href="79165?version=1&table=Limitoncrosssection15">b1L-SRA750</a> <a href="79165?version=1&table=Limitoncrosssection16">b1L-SRB</a> <a href="79165?version=1&table=Limitoncrosssection17">best combination</a> <a href="79165?version=1&table=Limitoncrosssection18">A-LowMass</a> <a href="79165?version=1&table=Limitoncrosssection19">A-HighMass</a> <a href="79165?version=1&table=Limitoncrosssection20">B combination</a><br/><br/><b>Cutflow:</b><br/><i>symmetric:</i> <a href="79165?version=1&table=CutflowTable1">b0L-SRA (1 TeV, 1 GeV)</a> <a href="79165?version=1&table=CutflowTable2">b0L-SRB (700 GeV, 450 GeV)</a> <a href="79165?version=1&table=CutflowTable3">b0L-SRC (450 GeV, 430 GeV)</a><br/><i>mixed:</i> <a href="79165?version=1&table=CutflowTable4">b1L-SRA (700 GeV, 300 GeV)</a> <a href="79165?version=1&table=CutflowTable5">b1L-SRA300-2j (700 GeV, 300 GeV)</a> <a href="79165?version=1&table=CutflowTable6">b0L-SRA (700 GeV, 300 GeV)</a><br/><br/><b>Truth Code</b> and <b>SLHA Files</b> for the cutflows are available under "Resources" (purple button on the left)

Signal acceptance (in %) in the ( M(SBOTTOM), M(NEUTRALINO) ) mass plane for the symmetric decay of the sbottom into bottom quark and neutralino, for the b0L-SRA350 signal region.

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Search for supersymmetry in events with at least one photon, missing transverse momentum, and large transverse event activity in proton-proton collisions at sqrt(s) = 13 TeV

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
JHEP 12 (2017) 142, 2017.
Inspire Record 1610629 DOI 10.17182/hepdata.79807

A search for physics beyond the standard model in final states with at least one photon, large transverse momentum imbalance, and large total transverse event activity is presented. Such topologies can be produced in gauge-mediated supersymmetry models in which pair-produced gluinos or squarks decay to photons and gravitinos via short-lived neutralinos. The data sample corresponds to an integrated luminosity of 35.9 inverse femtobarns of proton-proton collisions at sqrt(s) = 13 TeV recorded by the CMS experiment at the LHC in 2016. No significant excess of events above the expected standard model background is observed. The data are interpreted in simplified models of gluino and squark pair production, in which gluinos or squarks decay via neutralinos to photons. Gluino masses of up to 1.50-2.00 TeV and squark masses up to 1.30-1.65 TeV are excluded at 95% confidence level, depending on the neutralino mass and branching fraction.

14 data tables

Observed data compared to the background prediction. The expectation for the T5Wg signal scenario with a gluino mass of 1600 GeV and a gaugino mass of 100 GeV and the T6gg signal scenario with a squark mass of 1750 GeV and a neutralino mass of 1650 GeV are shown. The last three bins of the low-H_T^gamma selection are displayed, corresponding to three of the search regions The rightmost bin includes all events with ptmiss > 600GeV.

Observed data compared to the background prediction. The expectation for the T5Wg signal scenario with a gluino mass of 1600 GeV and a gaugino mass of 100 GeV and the T6gg signal scenario with a squark mass of 1750 GeV and a neutralino mass of 1650 GeV are shown. The last three bins of the high-H_T^gamma selection are displayed, corresponding to three of the search regions The rightmost bin includes all events with ptmiss > 600GeV.

Exclusion limits on the SUSY cross section at 95% CL for the T6gg model.

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Search for top squark pair production in pp collisions at sqrt(s)=13 TeV using single lepton events

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
JHEP 10 (2017) 019, 2017.
Inspire Record 1605128 DOI 10.17182/hepdata.79417

A search for top squark pair production in pp collisions at sqrt(s) = 13 TeV is performed using events with a single isolated electron or muon, jets, and a large transverse momentum imbalance. The results are based on data collected in 2016 with the CMS detector at the LHC, corresponding to an integrated luminosity of 35.9 inverse femtobarns. No significant excess of events is observed above the expectation from standard model processes. Exclusion limits are set in the context of supersymmetric models of pair production of top squarks that decay either to a top quark and a neutralino or to a bottom quark and a chargino. Depending on the details of the model, we exclude top squarks with masses as high as 1120 GeV. Detailed information is also provided to facilitate theoretical interpretations in other scenarios of physics beyond the standard model.

10 data tables

Result of the background estimates and data yields corresponding to 35.9 $\text{fb}^\text{$-$1}$ for the 27 signal regions.

Result of the background estimates and data yields corresponding to 35.9 $\text{fb}^\text{$-$1}$ for the 4 signal regions dedicated to compressed spectra.

The observed exclusion limits at 95% CL assuming 100% branching fraction for direct top squark pair production with decay $\widetilde{t}\widetilde{t} \rightarrow t \widetilde{\chi_1^0} t \widetilde{\chi_1^0}$.

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Search for Supersymmetry in $pp$ Collisions at $\sqrt{s}=13\text{ }\text{ }\mathrm{TeV}$ in the Single-Lepton Final State Using the Sum of Masses of Large-Radius Jets

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
Phys.Rev.Lett. 119 (2017) 151802, 2017.
Inspire Record 1599402 DOI 10.17182/hepdata.79414

Results are reported from a search for supersymmetric particles in proton-proton collisions in the final state with a single lepton; multiple jets, including at least one b-tagged jet; and large missing transverse momentum. The search uses a sample of proton-proton collision data at sqrt(s) = 13 TeV recorded by the CMS experiment at the LHC, corresponding to an integrated luminosity of 35.9 inverse femtobarns. The observed event yields in the signal regions are consistent with those expected from standard model backgrounds. The results are interpreted in the context of simplified models of supersymmetry involving gluino pair production, with gluino decay into either on- or off-mass-shell top squarks. Assuming that the top squarks decay into a top quark plus a stable, weakly interacting neutralino, scenarios with gluino masses up to about 1.9 TeV are excluded at 95% confidence level for neutralino masses up to about 1 TeV.

11 data tables

Figure 2. Cross section upper limit (95% CL) on T1tttt cross section

Figure 2. Excluded gluino and neutralino masses at 95% CL for the T1tttt.

Figure 2. +1 sigma excluded gluino and neutralino masses at 95% CL for the T1tttt.

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Search for supersymmetry in multijet events with missing transverse momentum in proton-proton collisions at 13 TeV

The CMS collaboration Sirunyan, Albert M ; Tumasyan, Armen ; Adam, Wolfgang ; et al.
Phys.Rev.D 96 (2017) 032003, 2017.
Inspire Record 1594909 DOI 10.17182/hepdata.79412

A search for supersymmetry is presented based on multijet events with large missing transverse momentum produced in proton-proton collisions at a center-of-mass energy of sqrt(s) = 13 TeV. The data, corresponding to an integrated luminosity of 35.9 inverse femtobarns, were collected with the CMS detector at the CERN LHC in 2016. The analysis utilizes four-dimensional exclusive search regions defined in terms of the number of jets, the number of tagged bottom quark jets, the scalar sum of jet transverse momenta, and the magnitude of the vector sum of jet transverse momenta. No evidence for a significant excess of events is observed relative to the expectation from the standard model. Limits on the cross sections for the pair production of gluinos and squarks are derived in the context of simplified models. Assuming the lightest supersymmetric particle to be a weakly interacting neutralino, 95% confidence level lower limits on the gluino mass as large as 1800 to 1960 GeV are derived, and on the squark mass as large as 960 to 1390 GeV, depending on the production and decay scenario.

70 data tables

Observed number of events and pre-fit background predictions in the $N_{jet}=2$ search bins.

Observed number of events and pre-fit background predictions in the $3\leq N_{jet}\leq4$ search bins.

Observed number of events and pre-fit background predictions in the $5\leq N_{jet}\leq6$ search bins.

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A search for new phenomena in pp collisions at sqrt(s) = 13 TeV in final states with missing transverse momentum and at least one jet using the alphaT variable

The CMS collaboration Khachatryan, Vardan ; Sirunyan, Albert M ; Tumasyan, Armen ; et al.
Eur.Phys.J.C 77 (2017) 294, 2017.
Inspire Record 1495423 DOI 10.17182/hepdata.77606

A search for new phenomena is performed in final states containing one or more jets and an imbalance in transverse momentum in pp collisions at a centre-of-mass energy of 13 TeV. The analysed data sample, recorded with the CMS detector at the CERN LHC, corresponds to an integrated luminosity of 2.3 inverse femtobarns. Several kinematic variables are employed to suppress the dominant background, multijet production, as well as to discriminate between other standard model and new physics processes. The search provides sensitivity to a broad range of new-physics models that yield a stable weakly interacting massive particle. The number of observed candidate events is found to agree with the expected contributions from standard model processes, and the result is interpreted in the mass parameter space of fourteen simplified supersymmetric models that assume the pair production of gluinos or squarks and a range of decay modes. For models that assume gluino pair production, masses up to 1575 and 975 GeV are excluded for gluinos and neutralinos, respectively. For models involving the pair production of top squarks and compressed mass spectra, top squark masses up to 400 GeV are excluded.

97 data tables

Summary of the lower bounds of the first and final bins in $H_{\mathrm{T}}$ in [GeV] (the latter in parentheses) as a function of $n_{\text{jet}}$ and $n_{\text{b}}$.

Systematic uncertainties (in percent) in the transfer ($\mathcal{T}$) factors used in the method to estimate the SM backgrounds with genuine $\vec{p}_t^{miss}$ in the signal region. The quoted ranges provide representative values of the observed variations as a function of $n_{\mathrm{jet}}$ and $H_{\mathrm{T}}$.

A summary of the simplified SUSY models used to interpret the results of this search. All on-shell SUSY particles in the decay are stated.

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Search for supersymmetry in pp collisions at sqrt(s) = 13 TeV in the single-lepton final state using the sum of masses of large-radius jets

The CMS collaboration Khachatryan, Vardan ; Sirunyan, Albert M ; Tumasyan, Armen ; et al.
JHEP 08 (2016) 122, 2016.
Inspire Record 1459054 DOI 10.17182/hepdata.77195

Results are reported from a search for supersymmetric particles in proton-proton collisions in the final state with a single, high transverse momentum lepton; multiple jets, including at least one b-tagged jet; and large missing transverse momentum. The data sample corresponds to an integrated luminosity of 2.3 inverse femtobarns at sqrt(s) = 13 TeV, recorded by the CMS experiment at the LHC. The search focuses on processes leading to high jet multiplicities, such as gluino pair production with gluinos to t t-bar neutralino[1]. The quantity M[J], defined as the sum of the masses of the large-radius jets in the event, is used in conjunction with other kinematic variables to provide discrimination between signal and background and as a key part of the background estimation method. The observed event yields in the signal regions in data are consistent with those expected for standard model backgrounds, estimated from control regions in data. Exclusion limits are obtained for a simplified model corresponding to gluino pair production with three-body decays into top quarks and neutralinos. Gluinos with a mass below 1600 GeV are excluded at a 95% confidence level for scenarios with low neutralino[1] mass, and neutralinos with a mass below 800 GeV are excluded for a gluino mass of about 1300 GeV. For models with two-body gluino decays producing on-shell top squarks, the excluded region is only weakly sensitive to the top squark mass.

12 data tables

Event yields obtained from simulated event samples, as the event selection criteria are applied. The category Other includes Drell-Yan, $t\bar{t}H(\rightarrow b\bar{b})$, $t\bar{t}t\bar{t}$, $WZ$, and $WW$. The yields for $t\bar{t}$ events in fully hadronic final states are included in the QCD multijet category. The category $t\bar{t}{\rm V}$ includes $t\bar{t}W$, $t\bar{t}Z$, and $t\bar{t}\gamma$. The benchmark signal models, T1tttt(NC) and T1tttt(C), are described in Section 3. The event selection requirements listed above the horizontal line in the middle of the table are defined as the baseline selection. The background estimates before the $H_{T}$ requirement are not specified because some of the simulated event samples do not extend to the low $H_{T}$ region. Given the size of the MC samples described in Section 3, rows with zero yield have statistical uncertainties of at most 0.16 events, and below 0.05 events in most cases.

Observed and predicted event yields for the signal regions (R4) and background regions (R1--R3) in data (2.3 $\textrm{fb}^{-1}$) in 200<MET<400 GeV region. Expected yields for the two SUSY T1tttt benchmark scenarios are also given. The results from two types of fits are reported: the predictive fit (PF) and the version of the global fit (GF) performed under the assumption of the null hypothesis ($r=0$). The predictive fit uses the observed yields in regions R1, R2, and R3 only and is effectively just a propagation of uncertainties. The global fit uses all four regions. The values of $\kappa$ obtained from the simulation fit are also listed. The first uncertainty in $\kappa$ is statistical, while the second corresponds to the total systematic uncertainty.

Observed and predicted event yields for the signal regions (R4) and background regions (R1--R3) in data (2.3 $\textrm{fb}^{-1}$) in MET>400 GeV region. Expected yields for the two SUSY T1tttt benchmark scenarios are also given. The results from two types of fits are reported: the predictive fit (PF) and the version of the global fit (GF) performed under the assumption of the null hypothesis ($r=0$). The predictive fit uses the observed yields in regions R1, R2, and R3 only and is effectively just a propagation of uncertainties. The global fit uses all four regions. The values of $\kappa$ obtained from the simulation fit are also listed. The first uncertainty in $\kappa$ is statistical, while the second corresponds to the total systematic uncertainty.

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Search for supersymmetry in the multijet and missing transverse momentum final state in pp collisions at 13 TeV

The CMS collaboration Khachatryan, Vardan ; Sirunyan, Albert M ; Tumasyan, Armen ; et al.
Phys.Lett.B 758 (2016) 152-180, 2016.
Inspire Record 1422778 DOI 10.17182/hepdata.76545

A search for new physics is performed based on all-hadronic events with large missing transverse momentum produced in proton-proton collisions at sqrt(s) = 13 TeV. The data sample, corresponding to an integrated luminosity of 2.3 inverse femtobarns, was collected with the CMS detector at the CERN LHC in 2015. The data are examined in search regions of jet multiplicity, tagged bottom quark jet multiplicity, missing transverse momentum, and the scalar sum of jet transverse momenta. The observed numbers of events in all search regions are found to be consistent with the expectations from standard model processes. Exclusion limits are presented for simplified supersymmetric models of gluino pair production. Depending on the assumed gluino decay mechanism, and for a massless, weakly interacting, lightest neutralino, lower limits on the gluino mass from 1440 to 1600 GeV are obtained, significantly extending previous limits.

7 data tables

Expected prefit background and observed event counts for Njet = 4-6.

Expected prefit background and observed event counts for Njet = 7-8.

Expected prefit background and observed event counts for Njet > 9.

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