Search for Low-Mass Dijet Resonances Using Trigger-Level Jets
with the ATLAS Detector in pp Collisions at $\sqrt{s}$=13 TeV

M. Aaboud et al. *

(ATLAS Collaboration)

<figure><img src="image_1.png" /></figure>

(Received 11 April 2018; published 22 August 2018)

Searches for dijet resonances with sub-TeV masses using the ATLAS detector at the Large Hadron Collider can be statistically limited by the bandwidth available to inclusive single-jet triggers, whose data-collection rates at low transverse momentum are much lower than the rate from standard model multijet production. This Letter describes a new search for dijet resonances where this limitation is overcome by recording only the event information calculated by the jet trigger algorithms, thereby allowing much higher event rates with reduced storage needs. The search targets low-mass dijet resonances in the range 450–1800 GeV. The analyzed data set has an integrated luminosity of up to 29.3 fb⁻¹ and was recorded at a center-of-mass energy of 13 TeV. No excesses are found; limits are set on Gaussian-shaped contributions to the dijet mass distribution from new particles and on a model of dark-matter particles with axial-vector couplings to quarks.

DOI: 10.1103/PhysRevLett.121.081801

*Introduction*.—If new particles beyond those of the standard model (SM) are directly produced in proton-proton (pp) collisions at the Large Hadron Collider (LHC), they must interact with the constituent partons of the proton, and can therefore also decay into the same partons, resulting in two-jet final states. Quantum chromodynamics (QCD) predicts that dijet events have an invariant mass distribution ($m_{jj}$) that falls smoothly, whereas a new state decaying to two partons would emerge as a localized excess in the distribution.

Traditional dijet searches at the LHC focus on the production of heavy particles with masses above 900 GeV [1–3]. LHC searches for lighter resonances with small production cross sections have been hampered by restrictions in the data-taking rate of the ATLAS and CMS detectors. Single-jet triggers with a jet $p_T$ threshold below roughly 380 GeV are prescaled, a procedure whereby only a fraction of the events passing the trigger are recorded; hence, dijet events with an invariant mass below 1 TeV are largely discarded by the trigger system, as indicated in Fig. 1. Therefore, despite the large number of pp collisions produced by the LHC, traditional ATLAS and CMS searches are less sensitive to dijet resonances below 900 GeV than searches at the SPS and Tevatron colliders [4–9]. Alternative trigger strategies to search for low-mass resonances include selecting events with jets recoiling

against either an energetic photon or an additional energetic jet [10–12], or selecting events with decays to heavy-flavor jets [13,14]. In these cases, additional features in the events reduce the data-taking rates, reducing the sensitivity to low-mass resonances.

This Letter describes an innovative data-taking approach to access the invariant mass region below 1 TeV; only a reduced set of information from the trigger system is recorded and subsequently analyzed. The Trigger-object Level Analysis (TLA) approach allows jet events to be recorded at a peak rate of up to twice the total rate of events using the standard approach, while using less than 1% of

<figure><img src="image_2.png" /><figcaption>FIG. 1. Comparison between the number of dijet events in the data used by this analysis (black points), the number of events selected by any single-jet trigger (thicker, blue line), and the events selected by single-jet triggers but corrected for the trigger prescale factors (thinner, red line) as a function of the dijet invariant mass ($m_{jj}$). The definition of $y^*$ is $(y_1 - y_2)/2$, where $y_1$ and $y_2$ are the rapidities of the highest- and second-highest $p_T$ jets.</figcaption></figure>

<footnote>*Full author list given at the end of the article.</footnote>

<footnote>Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP³.</footnote>
the total trigger bandwidth [15]. This strategy is used in dijet resonance searches in $\sqrt{s} = 8$ and 13 TeV LHC pp collision data by the CMS Collaboration [16,17], and it is used by the LHCb Collaboration (e.g. [18]). The analysis presented here uses $29.3 \text{ fb}^{-1}$ of $\sqrt{s} = 13$ TeV pp collision data recorded in 2016 by the ATLAS detector.

**ATLAS detector and data sample.**—The ATLAS detector [19] is a multipurpose detector with a forward-backward symmetric cylindrical geometry and nearly $4\pi$ coverage in solid angle [20], consisting of tracking detectors, calorimeters, and a muon spectrometer. In the pseudorapidity region $|\eta| < 3.2$, high-granularity lead and liquid-argon (LAr) electromagnetic sampling calorimeters are used. A steel and scintillator hadronic tile calorimeter provides coverage in the range $|\eta| < 1.7$. Hadronic calorimetry in the endcap region, $1.5 < |\eta| < 3.2$, and electromagnetic and hadronic calorimetry in the forward region, $3.1 < |\eta| < 4.9$, are provided by LAr sampling calorimeters. A two-level trigger system is used to select events for offline storage [15]. A first-level (L1) trigger based on dedicated hardware identifies jets from $\Delta\eta \times \Delta\phi = 0.2 \times 0.2$ calorimeter segments with a sliding-window algorithm. Events passing the L1 trigger are processed by a software-based high-level trigger (HLT). The HLT system reconstructs jets using the anti-$k_t$ algorithm [21,22] with radius parameter $R = 0.4$. The inputs to this algorithm are groups of contiguous calorimeter cells (topological clusters), in which each cell's inclusion is based on the significance of its energy deposit over calorimeter noise [23]. Jet four-momenta are computed by summing over the four-momenta of the topological clusters that compose the jet, with each cluster pointing to the center of the ATLAS detector and being treated as massless. The HLT jet reconstruction uses the same techniques that the ATLAS offline jet reconstruction applies to similar inputs from recorded data events that include the full detector information [15].

After execution of the HLT jet algorithm, only trigger-level jets with $p_T > 20$ GeV are stored. The stored information includes the four-momentum of each jet and a set of calorimeter variables characterizing the jet [24], such as information about the jet quality and structure. The average size of these events is less than 0.5% of the size of full offline events that contain all detector information. For this analysis, all events containing at least one L1 jet with $E_T > 100$ GeV are selected and recorded, corresponding to a total luminosity of $29.3 \text{ fb}^{-1}$. Events containing a L1 jet with $E_T > 75$ GeV are also selected, in a subset of these data corresponding to $3.6 \text{ fb}^{-1}$ that were collected at the start of the data-taking period. Events with at least one L1 jet with $E_T > 100$ GeV are therefore included in both data sets.

**Calibration procedure.**—After the events are recorded, the trigger-level jet energy and direction are corrected to those of simulated particle-level jets built from stable particles with a lifetime longer than 10 ps, excluding

<figure><img src="image_3.png" /><figcaption>FIG. 2. Calibration stages for EM-scale trigger-level jets, each applied to the four-momentum of the jet. MC refers to the simulation.</figcaption></figure>

muons and neutrinos. Before any calibration, the jet $p_T$ response, defined as the $p_T$ ratio of a trigger-level jet to the same jet [25] reconstructed offline (offline jet), is between 0.95 and 1.05 in the $p_T$ range considered by this analysis. Since the energy scale for trigger-level and offline jet are very similar, the trigger-level jet calibration employs the same procedure and constants as derived for offline jets [26], with some modifications to account for the unavailability of tracking information for trigger-level jets.

In the calibration procedure, summarized in Fig. 2, an event-by-event jet-area-based calibration [27] is used to correct for contributions from additional proton-proton interactions (pileup) in the same and neighboring crossings of proton bunches. Then, the simulation-based calibration derived for offline jets is applied to trigger-level jets to correct both jet energy and direction. Next, calorimeter-based variables are used to reduce the dependence on the trigger-level jet flavor and to minimize the impact of energy leakage. Only variables related to the trigger-level jet energy fractions in the electromagnetic and hadronic calorimeters and the minimum number of calorimeter cells containing 90% of the trigger-level jet energy are used here since track-based variables, which are normally used in the offline calibration, are not available. With this correction, the trigger-level jet energy resolution is improved by 8% at jet $p_T$ values of 85 GeV and up to 40% for jet $p_T$ values of 1 TeV relative to the previous calibration step. Next, the calibration corrections that restore the relative calibration between central and forward jets in data and simulation are derived for offline jets and applied to trigger-level jets. After these calibration steps, any residual difference between trigger-level jets and offline jets is accounted for in a dedicated correction, based on the $p_T$ response and derived from data in bins of jet $\eta$ and $p_T$. The size of this correction is on average 1%, with values reaching up to 4% in the endcap regions of the calorimeter.

Finally, an *in situ* calibration is obtained from the data-to-simulation ratio of the $p_T$ balance between offline jets and well-calibrated objects against which the jets recoil. Three different types of well-calibrated objects are used to span the full $p_T$ range of the jets: Z bosons decaying to electrons or muons, photons, and multijets. A polynomial in $\log(p_T)$ is simultaneously fit to the three input measurements to combine them. The resulting curve is taken as
<figure><img src="image_4.png" /><figcaption>FIG. 3. The *in situ* calibration in the range 85 GeV < jet $p_T$ < 2 TeV, for both the spline (dashed line) and fitted (solid line) combination methods, as described in the text. Data points from the three input measurements are overlaid. The lower panel shows the ratio of the two calibration curves.</figcaption></figure>

the calibration correction to be applied to trigger-level jets. In deriving the final calibration curve, the fit is chosen over the simple spline-based combination procedure used for offline jets in Ref. [26]; this procedure is more robust against localized fluctuations in the jet $p_T$ distribution that result in deviations from the expected smoothly falling invariant mass spectrum. Any dependence of the final mass spectrum on the parametrization of the jet energy scale calibration is tested by comparing different parametrizations on the data as well as on simulations. The fitted *in situ* calibration curve is compared to the spline-based smoothing procedure in Fig. 3. After the full calibration procedure, the energy of trigger-level jets is equivalent to that of offline jets to better than 0.05% for invariant masses of 400 GeV and their difference is negligible for invariant masses of 1 TeV.

**Energy scale and resolution uncertainties** derived for offline jets [26] are applied to trigger-level jets in the signal simulation, with additional uncertainties equivalent to the size of the final trigger-to-offline correction (1%–3%). The uncertainty due to the modeling of pileup effects and due to the jet parton flavor are derived specifically for trigger-level jets and are comparable to those of offline jets. The jet energy scale uncertainty for trigger-level jets at 200 GeV ranges from 1% at $|\eta| < 0.8$ to 2% in the region between the central and endcap regions ($1.0 < |\eta| < 1.5$).

**Event selection.**—The dijet event selection for this analysis is similar to the one used in Ref. [3]. Events must contain at least two trigger-level jets with $|\eta| < 2.8$. The leading trigger-level jet must have either $p_T > 185$ GeV or $p_T > 220$ GeV for the $E_T > 75$ GeV and $E_T > 100$ GeV L1 trigger selections, respectively; this ensures that the L1 triggers are fully efficient. The second leading jet must have a $p_T > 85$ GeV. Events that contain jets induced by calorimeter noise bursts, beam-induced background, or cosmic rays are rejected using the same criteria as in

Ref. [24], but omitting the track-based charged fraction selection, which is not available for trigger-level jets. This has a negligible effect for this analysis, since most of these backgrounds are already removed by requiring two central jets, as described below. The efficiency and purity of jets passing the selection are measured with a tag-and-probe method using data events with the full detector information. The trigger-level jet reconstruction efficiency is 100% for jets with $p_T > 85$ GeV. The fraction of trigger-level jets that are not reconstructed and selected offline is below 0.1%.

This analysis searches for a dijet resonance with a mass between 450 and 1800 GeV. Two different selection criteria are used for different but overlapping ranges of the $m_{jj}$ spectrum. To search for resonances with 700 GeV < $m_{jj} < 1800$ GeV, events are required to have $|y^*| < 0.6$, where $y^* = (y_1 - y_2)/2$ and $y_1$ and $y_2$ are the rapidities of the highest- and second-highest $p_T$ trigger-level jets. To search for lower-mass resonances, with $m_{jj} > 450$ GeV, events with $|y^*| < 0.3$ are selected from the smaller data sample requiring a L1 jet with $E_T > 75$ GeV. The more stringent choice of $|y^*| < 0.3$ selects higher-$p_T$ jets at a given invariant mass and thus provides a mass distribution that is unbiased by the leading-jet selection from $m_{jj} = 450$ GeV.

**Background estimation.**—The invariant mass spectrum expected from SM dijet production is predicted to be smooth and falling. Prior dijet searches at various collision energies [7,28–32] have found a variety of simple functional forms to describe this shape; however, given the statistical precision of the data and the wide invariant mass range covered by this search, none of the single, simple functional forms can provide a good description of the data.

The SM background distribution is determined using a sliding-window fit [3], where a fitted functional form is evaluated at the bin at the center of a window, which then slides in one-bin steps along the $m_{jj}$ distribution. The evaluated background estimates evaluated in each bin are then collated to form the final background estimate. The signal selection with $|y^*| < 0.6$ uses a window size of 19 bins in the $m_{jj}$ spectrum from 531 to 2080 GeV, which spans 34 bins in total. The signal selection with $|y^*| < 0.3$ uses a window size of 27 bins over a total of 40 bins, in the range $400 < m_{jj} < 2080$ GeV. The bin sizes have been chosen according to the simulated invariant mass resolution: $\sigma_{p_T}/p_T = 10.6/p_T \oplus 0.27/\sqrt{p_T} \oplus 0.039$. The sliding window, however, can not be extended beyond the lower edge of the $m_{jj}$ range used in each signal selection. Therefore, for the first 9 (13) bins in the $|y^*| < 0.6$ ($|y^*| < 0.3$) signal selection, which corresponds to one half of the window size, the window is fixed to the lower edge of the spectrum and instead of evaluating the fitted functional form at the window center, it is evaluated for each bin in turn. For invariant masses higher than the $m_{jj}$ range used for the search, the window is allowed to extend
beyond the range, to 2970 (3490) GeV for the $|y^*| < 0.6$ (0.3) signal selection, and the fit is evaluated at the center of the window.

In each sliding window, three functional forms are fit to the data: a five-parameter function of the form

$$f(x) = p_1(1-x)^{p_2} x^{p_3+p_4 \ln x+p_5 \ln x^2}, \quad (1)$$

where $p_i$ are free parameters and $x \equiv m_{jj}/\sqrt{s}$; a four-parameter function, which is the same as Eq. (1) but with $p_5 = 0$; and a four-parameter function used by the UA2 Collaboration [28], defined as

$$f(x) = \frac{p_1}{x^{p_2}} e^{-p_3 x - p_4 x^2}. \quad (2)$$

The function used for each signal selection is the one that yields the best $\chi^2$ over the full fitted $m_{jj}$ range. An alternative function is chosen to evaluate a systematic uncertainty. For the signal selection with $|y^*| < 0.6$, Eq. (1) is used, yielding a $\chi^2 p$ value of 0.13, while the alternative function is the four-parameter function with a $\chi^2 p$ value of 0.11. For the signal selection with $|y^*| < 0.3$, the four-parameter version of Eq. (1) yields the best $\chi^2 p$ value of 0.42 and the alternative function is Eq. (2), with a $\chi^2 p$ value of 0.35.

The size of the sliding window is optimized to yield the best $\chi^2$ value for the full $m_{jj}$ range while still being larger than the width of the expected signals and therefore insensitive to potential signal contributions. This latter requirement is checked by including signal models in pseudo-data samples and studying the dependence of the signal sensitivity on different window sizes.

Systematic uncertainties in the estimate of the background used in setting limits include the uncertainty due to the choice of functional form and uncertainties in the fit parameter values. The effect of the choice of functional form is evaluated by comparing the nominal function to the alternative. The uncertainties in the fit parameter values are evaluated using pseudo-experiments, where the pseudodata are drawn from Poisson fluctuations around the nominal background model.

**Results and limits.**—Figure 4 shows the invariant mass distributions for dijet events in each signal region including the results from the sliding-window background estimates. The $\chi^2 p$ value of the overall background is 0.13 for the $|y^*| < 0.6$ signal selection and 0.42 for the $|y^*| < 0.3$ signal selection, indicating the data agrees well with the background estimate. The most discrepant interval identified by the BumpHunter algorithm [33,34] is 889–1007 GeV for events with $|y^*| < 0.6$. Accounting for statistical uncertainties only, the probability of observing a deviation at least as significant as that observed in data, anywhere in this distribution, is 0.44 and corresponds to significance of $0.16\sigma$. Thus, there is no evidence of any localized excess.

<figure><img src="image_5.png" /><figcaption>FIG. 4. The reconstructed dijet mass distribution (filled points) for events in the $|y^*| < 0.3$ and $|y^*| < 0.6$ signal regions. Solid lines depict the background estimate obtained by a sliding-window fit. Overall agreement between the background estimate and the data is quantified by the $\chi^2 p$ value. The most discrepant localized excess in either signal region identified by the Bump-Hunter algorithm is indicated by the vertical lines. The open points show two possible signal models. The lower panels show the bin-by-bin significances of differences between the data and the background estimate, considering only statistical uncertainties (see Ref. [35]).</figcaption></figure>

Limits are set on both a leptophobic $Z'$ simplified dark-matter model [36] and a generic Gaussian model. The $Z'$ simplified model assumes axial-vector couplings to SM quarks and to a Dirac fermion dark-matter candidate. No interference with the SM is simulated. Signal samples were generated so that the decay rate of the $Z'$ into dark-matter particles is negligible and the dijet production rate and resonance width depend only on the coupling of the $Z'$ to quarks, $g_q$, and the mass of the resonance, $m_{Z'}$ [9]. The model's matrix elements were calculated in MADGRAPH 5 [37] and parton showering was performed in PYTHIA 8 [38] with the A14 set of tuned parameters for underlying event [39] and NNPDF2.3 parton distribution functions [40].

The width of a $Z'$ resonance with $g_q = 0.10$, including parton shower and detector resolution effects, is approximately 7%. Limits are set on the cross section, $\sigma$, times acceptance, A, times branching ratio, B, of the model, and then displayed in the $(g_q, m_{Z'})$ plane [41]. The acceptance for a mass of 550 GeV is 20% for a $Z'$ simplified model with $g_q = 0.10$ for the $|y^*| < 0.3$ signal selection, and 41% for a signal of mass equal to 750 GeV for the $|y^*| < 0.6$ signal selection.

Limits are also set on a generic model where the signal is modeled as a Gaussian contribution to the observed $m_{jj}$ distribution. For a given mean mass, $m_G$, four different Gaussian widths are considered: a width equal to the simulated mass resolution (which ranges between 4% and 6%), and the fixed fractions 5%, 7%, and 10% of $m_G$. As the width increases, the expected signal contribution is distributed across more bins. Wider signals are
therefore less affected by statistical fluctuations from the data in a single bin. The results can be used to set limits on models of new phenomena besides that of the $Z'$ simplified model and are applicable when the resonance is sufficiently narrow and the parton distribution function and nonperturbative effects can be safely truncated or neglected, as described in Ref. [31]. These criteria are often met if the $m_{jj}$ distribution for a signal approaches a Gaussian distribution after applying the kinematic selection criteria of the resonance analysis, so that 95% of the signal lies within 20% of the Gaussian mean mass. Models of new resonances with an intrinsic width much smaller than 5% of its mass should be compared to the results with a width equal to the experimental resolution. For models with a larger width, the limit that best matches their width should be used. More-detailed instructions can be found in Appendix A of Ref. [31].

A Bayesian method is applied to the data and simulation of the signal models at a series of discrete masses to set 95% credibility-level upper limits on the cross section times acceptance [30] for the signals described above. The method uses a constant prior for the signal cross section and Gaussian priors for nuisance parameters corresponding to systematic uncertainties. For both observed and expected limits, the sliding window fit is performed for each value of the mass parameter, adding the tested signal shape with a floating normalization to the functional forms stated above. The expected limits are calculated using pseudoexperiments generated from the fit parameters of those functional forms. The uncertainties on the $Z'$ signal model include the jet energy scale and the luminosity. The impact of the jet energy resolution uncertainty is negligible. For the Gaussian model, a constant jet energy scale uncertainty of 3% is applied in accordance with the measured impact of this uncertainty on the $Z'$ samples. The uncertainty in the integrated luminosity is $\pm 2.2\%$, derived following a methodology similar to that detailed in Ref. [42]. The systematic uncertainties in the background estimate include the choice of the fit function and the uncertainty in the fit parameter values, as described above.

Figure 5 shows limits on the coupling to quarks, $g_q$, as a function of the mass $m_{Z'}$ for the $Z'$ model. Figure 6 shows limits on a possible Gaussian contribution with a width equal to the detector resolution as a function of the mean mass, $m_G$. In both the $Z'$ and Gaussian models, upper limits for masses from 450 to 700 GeV are derived using the distribution with $|y^*| < 0.3$, which is sensitive to the lower masses. Limits for masses above 700 GeV are derived from the $m_{jj}$ distribution with $|y^*| < 0.6$, except for Gaussian signals with a width of 10% where only the $|y^*| < 0.3$ distribution is used.

The limit results show an upward fluctuation at masses of approximately 1 TeV in the $|y^*| < 0.6$ signal region. This is not seen in Fig. 4; when searching for excesses in the data, a background-only hypothesis is used for the sliding

<figure><img src="image_6.png" /><figcaption>FIG. 5. The 95% credibility-level observed and expected upper limits on $g_q$ as a function of $m_{Z'}$ for the $Z'$ model described in the text. The lower-mass part of the limits from Ref. [3] is also shown. Couplings above the solid lines are excluded. The solid and dashed lines represent the observed and expected limits, respectively, and are obtained accounting for the scaling of the signal cross section with $g_q^2$. The different $y^*$ selections are described in the text.</figcaption></figure>

window fit. In the observed and expected limits, the fit includes the signal shape in addition to the background parameterization, and can adapt to local data fluctuations that mimic a signal shape. The $|y^*| < 0.6$ signal region, which uses a smaller sliding-window size, is especially sensitive to the difference in the two approaches. Therefore,

<figure><img src="image_7.png" /><figcaption>FIG. 6. The 95% credibility-level observed upper limits on $\sigma \times A \times B$ for two jets for a hypothetical signal producing a Gaussian contribution to the observed $m_{jj}$ distribution. The limits are shown for a relative width $\sigma_G/m_G$ corresponding to a width equal to the detector mass resolution. While the vertical axis is shared by the two selections, this signal acceptance varies; thus, the two sets of limit points relate to two different interpretations of $\sigma \times A \times B$ (see text for some typical acceptance values used for models considered by this search). The different $y^*$ selections are described in the text.</figcaption></figure>
limits were not set on signals with a width of 10% for the $|y^*| < 0.6$ signal region as the signal is too wide for the sliding-window size.

**Conclusions.**—In conclusion, this analysis searches for resonances with masses between 450 GeV and 1800 GeV in dijet events using trigger-level jets in $29.3 \text{ fb}^{-1}$ of $\sqrt{s} = 13$ TeV proton-proton collision data recorded by the ATLAS detector at the LHC. The invariant mass distribution presents no significant local excesses compared to the estimated SM background. This analysis provides 95% credibility-level limits on $Z'$ signals and cross sections for new processes that would produce a Gaussian contribution to the dijet mass distribution. Over much of the mass range, the sensitivity to the coupling to quarks, $g_q$, is improved by a factor of 2 or more compared to pre-LHC and $\sqrt{s} = 8$ and 13 TeV ATLAS results, and is comparable to CMS searches at $\sqrt{s} = 8$ and 13 TeV using this technique. Gaussian contributions with effective cross sections times acceptance ranging from approximately 6.5 pb at 450 GeV, to 0.4 pb at 700 GeV, to 0.05 pb at 1800 GeV are excluded.

We thank CERN for the very successful operation of the LHC, as well as the support staff from our institutions without whom ATLAS could not be operated efficiently. We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS, CEA-DRF/IRFU, France; SRNSFG, Georgia; BMBF, HGF, and MPG, Germany; GSRT, Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; NWO, Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA, Romania; MES of Russia and NRC KI, Russian Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS and MIZŠ, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SERI, SNSF and Cantons of Bern and Geneva, Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE and NSF, United States of America. In addition, individual groups and members have received support from BCKDF, the Canada Council, CANARIE, CRC, Compute Canada, FQRNT, and the Ontario Innovation Trust, Canada; EPLANET, ERC, ERDF, FP7, Horizon 2020 and Marie Skłodowska-Curie Actions, European Union; Investissements d'Avenir Labex and Idex, ANR, Région Auvergne and Fondation Partager le Savoir, France; DFG and AvH Foundation, Germany; Herakleitos, Thales and Aristeia programmes co-financed by EU-ESF and the Greek NSRF; BSF, GIF and Minerva, Israel; BRF, Norway; CERCA Programme Generalitat

de Catalunya, Generalitat Valenciana, Spain; the Royal Society and Leverhulme Trust, United Kingdom. The crucial computing support from all WLCG partners is acknowledged gratefully, in particular from CERN, the ATLAS Tier-1 facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/GridKA (Germany), INFN-CNAF (Italy), NL-T1 (Netherlands), PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA), the Tier-2 facilities worldwide and large non-WLCG resource providers. Major contributors of computing resources are listed in Ref. [43].

[1] R. M. Harris and K. Kousouris, Searches for dijet resonances at hadron colliders, Int. J. Mod. Phys. A **26**, 5005 (2011).

[2] CMS Collaboration, Search for Narrow Resonances Decaying to Dijets in Proton-Proton Collisions at $\sqrt{s} = 13$ TeV, Phys. Rev. Lett. **116**, 071801 (2016).

[3] ATLAS Collaboration, Search for new phenomena in dijet events using $37 \text{ fb}^{-1}$ of $pp$ collision data collected at $\sqrt{s} = 13$ TeV with the ATLAS detector, Phys. Rev. D **96**, 052004 (2017).

[4] UA1 Collaboration, Angular distributions and structure functions from two jet events at the CERN SPS p anti-p collider, Phys. Lett. B **136**, 294 (1984).

[5] UA1 Collaboration, Two jet mass distributions at the CERN proton-antiproton Collider, Phys. Lett. B **209**, 127 (1988).

[6] UA2 Collaboration, Measurement of jet production properties at the CERN $pp$ collider, Phys. Lett. B **144**, 283 (1984).

[7] CDF Collaboration, Search for new particles decaying into dijets in proton-antiproton collisions at $\sqrt{s} = 1.96$ TeV, Phys. Rev. D **79**, 112002 (2009).

[8] B. A. Dobrescu and F. Yu, Coupling-mass mapping of dijet peak searches, Phys. Rev. D **88**, 035021 (2013).

[9] M. Chala, F. Kahlhoefer, M. McCullough, G. Nardini, and K. Schmidt-Hoberg, Constraining dark sectors with mono-jets and dijets, J. High Energy Phys. **07** (2015) 089.

[10] ATLAS Collaboration, Search for new light resonances decaying to jet pairs and produced in association with a photon or a jet in proton-proton collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector, ATLAS-CONF-2016-070, 2016, https://cds.cern.ch/record/2206221.

[11] CMS Collaboration, Search for low mass vector resonances decaying into quark-antiquark pairs in proton-proton collisions at $\sqrt{s} = 13$ TeV, J. High Energy Phys. **01** (2018) 097.

[12] ATLAS Collaboration, Search for light resonances decaying to boosted quark pairs and produced in association with a photon or a jet in proton-proton collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector, arXiv:1801.08769.

[13] ATLAS Collaboration, Search for resonances in the mass distribution of jet pairs with one or two jets identified as b-jets in proton-proton collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector, arXiv:1805.09299.
[14] CMS Collaboration, Search for Narrow Resonances in the b-Tagged Dijet Mass Spectrum in Proton-Proton Collisions at $\sqrt{s} = 8$ TeV, Phys. Rev. Lett. **120**, 201801 (2018).

[15] ATLAS Collaboration, Performance of the ATLAS Trigger System in 2015, Eur. Phys. J. C **77**, 317 (2017).

[16] CMS Collaboration, Search for Narrow Resonances in Dijet Final States at $\sqrt{s} = 8$ TeV with the Novel CMS Technique of Data Scouting, Phys. Rev. Lett. **117**, 031802 (2016).

[17] CMS Collaboration, Search for narrow and broad dijet resonances in proton-proton collisions at $\sqrt{s} = 13$ TeV and constraints on dark matter mediators and other new particles, arXiv:1806.00843.

[18] LHCb Collaboration, Measurement of forward $J/\psi$ production cross-sections in $pp$ collisions at $\sqrt{s} = 13$ TeV, J. High Energy Phys. **10** (2017) 172.

[19] ATLAS Collaboration, The ATLAS Experiment at the CERN Large Hadron Collider, J. Instrum. **3**, S08003 (2008).

[20] ATLAS uses a right-handed coordinate system with its origin at the nominal interaction point (IP) in the center of the detector and the z axis along the beam pipe. The x axis points from the IP to the center of the LHC ring, and the y axis points upwards. Cylindrical coordinates (r, φ) are used in the transverse plane, φ being the azimuthal angle around the z axis. The pseudorapidity is defined in terms of the polar angle θ as $η = -\ln(\tan(\theta/2))$. The rapidity, y, is defined as $\frac{1}{2}\ln[(E + p_z)/(E - p_z)]$, where E denotes the energy of the jet and p_z the momentum component of the jet along the beam direction. Angular distance is measured in units of $ΔR = \sqrt{(Δη)^2 + (Δφ)^2}$.

[21] M. Cacciari, G. P. Salam, and G. Soyez, The anti-$k_t$ jet clustering algorithm, J. High Energy Phys. **04** (2008) 063.

[22] M. Cacciari and G. Salam, Dispelling the $N^3$ myth for the $k_t$ jet-finder, Phys. Lett. B **641**, 57 (2006).

[23] ATLAS Collaboration, Topological cell clustering in the ATLAS calorimeters and its performance in LHC Run 1, Eur. Phys. J. C **77**, 490 (2017).

[24] ATLAS Collaboration, Selection of jets produced in 13 TeV proton-proton collisions with the ATLAS detector, CERN Report No. ATLAS-CONF-2015-029, 2015, https://cds.cern.ch/record/2037702.

[25] The trigger-level and offline jets are matched within a radius of $ΔR = 0.4$.

[26] ATLAS Collaboration, Jet energy scale measurements and their systematic uncertainties in proton-proton collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector, Phys. Rev. D **96**, 072002 (2017).

[27] ATLAS Collaboration, Performance of pile-up mitigation techniques for jets in $pp$ collisions at $\sqrt{s} = 8$ TeV using the ATLAS detector, Eur. Phys. J. C **76**, 581 (2016).

[28] UA2 Collaboration, A measurement of two jet decays of the W and Z bosons at the CERN $\bar{p}p$ collider, Z. Phys. C **49**, 17 (1991).

[29] CMS Collaboration, Search for resonances in the dijet mass spectrum from 7 TeV $pp$ collisions at CMS, Phys. Lett. B **704**, 123 (2011).

[30] ATLAS Collaboration, A search for new physics in dijet mass and angular distributions in $pp$ collisions at $\sqrt{s} = 7$ TeV measured with the ATLAS detector, New J. Phys. **13**, 053044 (2011).

[31] ATLAS Collaboration, Search for new phenomena in the dijet mass distribution using $pp$ collision data at $\sqrt{s} = 8$ TeV with the ATLAS detector, Phys. Rev. D **91**, 052007 (2015).

[32] CMS Collaboration, Search for narrow resonances using the dijet mass spectrum in $pp$ collisions at $\sqrt{s} = 8$ TeV, Phys. Rev. D **87**, 114015 (2013).

[33] CDF Collaboration, Global search for new physics with $2.0 \text{ fb}^{-1}$ at CDF, Phys. Rev. D **79**, 011101 (2009).

[34] G. Choudalakis, On hypothesis testing, trials factor, hypertests and the BumpHunter, arXiv:1101.0390.

[35] G. Choudalakis and D. Casadei, Plotting the differences between data and expectation, Eur. Phys. J. Plus **127**, 25 (2012).

[36] D. Abercrombie et al., Dark matter benchmark models for early LHC Run-2 searches: Report of the ATLAS/CMS Dark Matter Forum, arXiv:1507.00966.

[37] J. Alwall, R. Frederix, S. Frixione, V. Hirschi, F. Maltoni, O. Mattelaer, H.-S. Shao, T. Stelzer, P. Torrielli, and M. Zaro, The automated computation of tree-level and next-to-leading order differential cross sections, and their matching to parton shower simulations, J. High Energy Phys. **07** (2014) 079.

[38] T. Sjöstrand, S. Mrenna, and P. Skands, A brief introduction to Pythia 8.1, Comput. Phys. Commun. **178**, 852 (2008).

[39] ATLAS Collaboration, ATLAS Pythia 8 tunes to 7 TeV data, CERN Report No. ATL-PHYS-PUB-2014-021, 2014, https://cds.cern.ch/record/1966419.

[40] R. D. Ball et al., Parton distributions with LHC data, Nucl. Phys. B**867**, 244 (2013).

[41] Limits on the coupling are obtained accounting for the scaling of the signal cross section with $g_q^2$.

[42] ATLAS Collaboration, Luminosity determination in $pp$ collisions at $\sqrt{s} = 8$ TeV using the ATLAS detector at the LHC, Eur. Phys. J. C **76**, 653 (2016).

[43] ATLAS Collaboration, ATLAS Computing Acknowledgements, CERN Report No. ATL-GEN-PUB-2016-002, https://cds.cern.ch/record/2202407.

M. Aaboud,³⁴d G. Aad,⁹⁹ B. Abbott,¹²⁴ O. Abdinov,¹³,a B. Abeloos,¹²⁸ S. H. Abidi,¹⁶⁵ O. S. AbouZeid,¹⁴³ N. L. Abraham,¹⁵³

H. Abramowicz,¹⁵⁹ H. Abreu,¹⁵⁸ Y. Abulaiti,⁶ B. S. Acharya,⁶⁴a,⁶⁴b S. Adachi,¹⁶¹ L. Adamczyk,⁸¹a J. Adelman,¹¹⁹

M. Adersberger,¹¹² A. Adiguzel,¹²c T. Adye,¹⁴¹ A. A. Affolder,¹⁴³ Y. Afik,¹⁵⁸ C. Agheorghiesei,²⁷c

J. A. Aguilar-Saavedra,¹³⁶f,¹³⁶a F. Ahmadov,⁷⁷,c G. Aielli,⁷¹a,⁷¹b S. Akatsuka,⁸³ T. P. A. Åkesson,⁹⁴ E. Akilli,⁵²

A. V. Akimov,¹⁰⁸ G. L. Alberghi,²³b,²³a J. Albert,¹⁷⁴ P. Albicocco,⁴⁹ M. J. Alconada Verzini,⁸⁶ S. Alderweireldt,¹¹⁷
M. Aleksa,³⁵ I. N. Aleksandrov,⁷⁷ C. Alexa,²⁷b G. Alexander,¹⁵⁹ T. Alexopoulos,¹⁰ M. Alhroob,¹²⁴ B. Ali,¹³⁸ G. Alimonti,⁶⁶a
J. Alison,³⁶ S. P. Alkire,¹⁴⁵ C. Allaire,¹²⁸ B. M. M. Allbrooke,¹⁵³ B. W. Allen,¹²⁷ P. P. Allport,²¹ A. Aloisio,⁶⁷a,⁶⁷b

A. Alonso,³⁹ F. Alonso,⁸⁶ C. Alpigiani,¹⁴⁵ A. A. Alshehri,⁵⁵ M. I. Alstaty,⁹⁹ B. Alvarez Gonzalez,³⁵ D. Álvarez Piqueras,¹⁷²
M. G. Alviggi,⁶⁷a,⁶⁷b B. T. Amadio,¹⁸ Y. Amaral Coutinho,⁷⁸b L. Ambroz,¹³¹ C. Amelung,²⁶ D. Amidei,¹⁰³
S. P. Amor Dos Santos,¹³⁶a,¹³⁶c S. Amoroso,³⁵ C. S. Amrouche,⁵² C. Anastopoulos,¹⁴⁶ L. S. Ancu,⁵² N. Andari,²¹
T. Andeen,¹¹ C. F. Anders,⁵⁹b J. K. Anders,²⁰ K. J. Anderson,³⁶ A. Andreazza,⁶⁶a,⁶⁶b V. Andrei,⁵⁹a S. Angelidakis,³⁷

I. Angelozzi,¹¹⁸ A. Angerami,³⁸ A. V. Anisenkov,¹²⁰b,¹²⁰a A. Annovi,⁶⁹a C. Antel,⁵⁹a M. T. Anthony,¹⁴⁶ M. Antonelli,⁴⁹

D. J. A. Antrim,¹⁶⁹ F. Anulli,⁷⁰a M. Aoki,⁷⁹ L. Aperio Bella,³⁵ G. Arabidze,¹⁰⁴ Y. Arai,⁷⁹ J. P. Araque,¹³⁶a V. Araujo Ferraz,⁷⁸b

R. Araujo Pereira,⁷⁸b A. T. H. Arce,⁴⁷ R. E. Ardell,⁹¹ F. A. Arduh,⁸⁶ J-F. Arguin,¹⁰⁷ S. Argyropoulos,⁷⁵ A. J. Armbruster,³⁵
L. J. Armitage,⁹⁰ O. Arnaez,¹⁶⁵ H. Arnold,¹¹⁸ M. Arratia,³¹ O. Arslan,²⁴ A. Artamonov,¹⁰⁹,a G. Artoni,¹³¹ S. Artz,⁹⁷
S. Asai,¹⁶¹ N. Asbah,⁴⁴ A. Ashkenazi,¹⁵⁹ E. M. Asimakopoulou,¹⁷⁰ L. Asquith,¹⁵³ K. Assamagan,²⁹ R. Astalos,²⁸a

R. J. Atkin,³²a M. Atkinson,¹⁷¹ N. B. Atlay,¹⁴⁸ K. Augsten,¹³⁸ G. Avolio,³⁵ R. Avramidou,⁵⁸a B. Axen,¹⁸ M. K. Ayoub,¹⁵a
G. Azuelos,¹⁰⁷,d A. E. Baas,⁵⁹a M. J. Baca,²¹ H. Bachacou,¹⁴² K. Bachas,⁶⁵a,⁶⁵b M. Backes,¹³¹ P. Bagnaia,⁷⁰a,⁷⁰b
M. Bahmani,⁸² H. Bahrasemani,¹⁴⁹ A. J. Bailey,¹⁷² J. T. Baines,¹⁴¹ M. Bajic,³⁹ O. K. Baker,¹⁸¹ P. J. Bakker,¹¹⁸

D. Bakshi Gupta,⁹³ E. M. Baldin,¹²⁰b,¹²⁰a P. Balek,¹⁷⁸ F. Balli,¹⁴² W. K. Balunas,¹³³ E. Banas,⁸² A. Bandyopadhyay,²⁴

S. Banerjee,¹⁷⁹e A. A. E. Bannoura,¹⁸⁰ L. Barak,¹⁵⁹ W. M. Barbe,³⁷ E. L. Barberio,¹⁰² D. Barberis,⁵³b,⁵³a M. Barbero,⁹⁹

T. Barillari,¹¹³ M-S. Barisits,³⁵ J. Barkeloo,¹²⁷ T. Barklow,¹⁵⁰ N. Barlow,³¹ R. Barnea,¹⁵⁸ S. L. Barnes,⁵⁸c B. M. Barnett,¹⁴¹
R. M. Barnett,¹⁸ Z. Barnovska-Blenessy,⁵⁸a A. Baroncelli,⁷²a G. Barone,²⁶ A. J. Barr,¹³¹ L. Barranco Navarro,¹⁷²

F. Barreiro,⁹⁶ J. Barreiro Guimarães da Costa,¹⁵a R. Bartoldus,¹⁵⁰ A. E. Barton,⁸⁷ P. Bartos,²⁸a A. Basalaev,¹³⁴ A. Bassalat,¹²⁸

R. L. Bates,⁵⁵ S. J. Batista,¹⁶⁵ S. Batlamous,³⁴e J. R. Batley,³¹ M. Battaglia,¹⁴³ M. Bauce,⁷⁰a,⁷⁰b F. Bauer,¹⁴² K. T. Bauer,¹⁶⁹
H. S. Bawa,¹⁵⁰,f J. B. Beacham,¹²² M. D. Beattie,⁸⁷ T. Beau,¹³² P. H. Beauchemin,¹⁶⁸ P. Bechtle,²⁴ H. C. Beck,⁵¹

H. P. Beck,²⁰,g K. Becker,⁵⁰ M. Becker,⁹⁷ C. Becot,¹²¹ A. Beddall,¹²⁴ A. J. Beddall,¹²⁸ V. A. Bednyakov,⁷⁷ M. Bedognetti,¹¹⁸
C. P. Bee,¹⁵² T. A. Beermann,³⁵ M. Begalli,⁷⁸b M. Begel,²⁹ A. Behera,¹⁵² J. K. Behr,⁴⁴ A. S. Bell,⁹² G. Bella,¹⁵⁹

L. Bellagamba,²³b A. Bellerive,³³ M. Bellomo,¹⁵⁸ K. Belotskiy,¹¹⁰ N. L. Belyaev,¹¹⁰ O. Benary,¹⁵⁹,a D. Benchekroun,³⁴a

M. Bender,¹¹² N. Benekos,¹⁰ Y. Benhammou,¹⁵⁹ E. Benhar Noccioli,¹⁸¹ J. Benitez,⁷⁵ D. P. Benjamin,⁴⁷ M. Benoit,⁵²

J. R. Bensinger,²⁶ S. Bentvelsen,¹¹⁸ L. Beresford,¹³¹ M. Beretta,⁴⁹ D. Berge,⁴⁴ E. Bergeaas Kuutmann,¹⁷⁰ N. Berger,⁵

L. J. Bergsten,²⁶ J. Beringer,¹⁸ S. Berlendis,⁵⁶ N. R. Bernard,¹⁰⁰ G. Bernardi,¹³² C. Bernius,¹⁵⁰ F. U. Bernlochner,²⁴

T. Berry,⁹¹ P. Berta,⁹⁷ C. Bertella,¹⁵a G. Bertoli,⁴³a,⁴³b I. A. Bertram,⁸⁷ G. J. Besjes,³⁹ O. Bessidskaia Bylund,⁴³a,⁴³b

M. Bessner,⁴⁴ N. Besson,¹⁴² A. Bethani,⁹⁸ S. Bethke,¹¹³ A. Betti,²⁴ A. J. Bevan,⁹⁰ J. Beyer,¹¹³ R. M. B. Bianchi,¹³⁵

O. Biebel,¹¹² D. Biedermann,¹⁹ R. Bielski,⁹⁸ K. Bierwagen,⁹⁷ N. V. Biesuz,⁶⁹a,⁶⁹b M. Biglietti,⁷²a T. R. V. Billoud,¹⁰⁷

M. Bindi,⁵¹ A. Bingul,¹²⁴ C. Bini,⁷⁰a,⁷⁰b S. Biondi,²³b,²³a T. Bisanz,⁵¹ J. P. Biswal,¹⁵⁹ C. Bittrich,⁴⁶ D. M. Bjergaard,⁴⁷

J. E. Black,¹⁵⁰ K. M. Black,²⁵ R. E. Blair,⁶ T. Blazek,²⁸a I. Bloch,⁴⁴ C. Blocker,²⁶ A. Blue,⁵⁵ U. Blumenschein,⁹⁰ Blunier,¹⁴⁴a
G. J. Bobbink,¹¹⁸ V. S. Bobrovnikov,¹²⁰b,¹²⁰a S. S. Bocchetta,⁹⁴ A. Bocci,⁴⁷ D. Boerner,¹⁸⁰ D. Bogavac,¹¹²

A. G. Bogdanchikov,¹²⁰b,¹²⁰a C. Bohm,⁴³a V. Boisvert,⁹¹ P. Bokan,¹⁷⁰,h T. Bold,⁸¹a A. S. Boldyrev,¹¹¹ A. E. Bolz,⁵⁹b

M. Bomben,¹³² M. Bona,⁹⁰ J. S. Bonilla,¹²⁷ M. Boonekamp,¹⁴² A. Borisov,¹⁴⁰ G. Borissov,⁸⁷ J. Bortfeldt,³⁵ D. Bortoletto,¹³¹

V. Bortolotto,⁷¹a,⁷¹b,⁶¹c,⁷¹b D. Boscherini,²³b M. Bosman,¹⁴ J. D. Bossio Sola,³⁰ J. Boudreau,¹³⁵ E. V. Bouhova-Thacker,⁸⁷

D. Boumediene,³⁷ C. Bourdarios,¹²⁸ S. K. Boutle,⁵⁵ A. Boveia,¹²² J. Boyd,³⁵ I. R. Boyko,⁷⁷ A. J. Bozson,⁹¹ J. Bracinik,²¹
N. Brahimi,⁹⁹ A. Brandt,⁸ G. Brandt,¹⁸⁰ O. Brandt,⁵⁹a F. Braren,⁴⁴ U. Bratzler,¹⁶² B. Brau,¹⁰⁰ J. E. Brau,¹²⁷

W. D. Breaden Madden,⁵⁵ K. Brendlinger,⁴⁴ A. J. Brennan,¹⁰² L. Brenner,⁴⁴ R. Brenner,¹⁷⁰ S. Bressler,¹⁷⁸ B. Brickwedde,⁹⁷

D. L. Briglin,²¹ D. Britton,⁵⁵ D. Britzger,⁵⁹b I. Brock,²⁴ R. Brock,¹⁰⁴ G. Brooijmans,³⁸ T. Brooks,⁹¹ W. K. Brooks,¹⁴⁴b

E. Brost,¹¹⁹ J. H. Broughton,²¹ P. A. Bruckman de Renstrom,⁸² D. Bruncko,²⁸b A. Bruni,²³b G. Bruni,²³b L. S. Bruni,¹¹⁸

S. Bruno,⁷¹a,⁷¹b B. H. Brunt,³¹ M. Bruschi,²³b N. Bruscino,¹³⁵ P. Bryant,³⁶ L. Bryngemark,⁴⁴ T. Buanes,¹⁷ Q. Buat,³⁵

P. Buchholz,¹⁴⁸ A. G. Buckley,⁵⁵ I. A. Budagov,⁷⁷ F. Buehrer,⁵⁰ M. K. Bugge,¹³⁰ O. Bulekov,¹¹⁰ D. Bullock,⁸ T. J. Burch,¹¹⁹

S. Burdin,⁸⁸ C. D. Burgard,¹¹⁸ A. M. Burger,⁵ B. Burghgrave,¹¹⁹ K. Burka,⁸² S. Burke,¹⁴¹ I. Burmeister,⁴⁵ J. T. P. Burr,¹³¹

D. Büscher,⁵⁰ V. Büscher,⁹⁷ E. Buschmann,⁵¹ P. Bussey,⁵⁵ J. M. Butler,²⁵ C. M. Buttar,⁵⁵ J. M. Butterworth,⁹² P. Butti,³⁵
W. Buttinger,³⁵ A. Buzatu,¹⁵⁵ A. R. Buzykaev,¹²⁰b,¹²⁰a G. Cabras,²³b,²³a S. Cabrera Urbán,¹⁷² D. Caforio,¹³⁸ H. Cai,¹⁷¹

V. M. M. Cairo,² O. Cakir,⁴a N. Calace,⁵² P. Calafiura,¹⁸ A. Calandri,⁹⁹ G. Calderini,¹³² P. Calfayan,⁶³ G. Callea,⁴⁰b,⁴⁰a

L. P. Caloba,⁷⁸b S. Calvente Lopez,⁹⁶ D. Calvet,³⁷ S. Calvet,³⁷ T. P. Calvet,¹⁵² M. Calvetti,⁶⁹a,⁶⁹b R. Camacho Toro,¹³²

S. Camarda,³⁵ P. Camarri,⁷¹a,⁷¹b D. Cameron,¹³⁰ R. Caminal Armadans,¹⁰⁰ C. Camincher,³⁵ S. Campana,³⁵ M. Campanelli,⁹²
A. Camplani,⁶⁶a,⁶⁶b A. Campoverde,¹⁴⁸ V. Canale,⁶⁷a,⁶⁷b M. Cano Bret,⁵⁸c J. Cantero,¹²⁵ T. Cao,¹⁵⁹ Y. Cao,¹⁷¹

M. D. M. Capeans Garrido,³⁵ I. Caprini,²⁷b M. Caprini,²⁷b M. Capua,⁴⁰b,⁴⁰a R. M. Carbone,³⁸ R. Cardarelli,⁷¹a

F. C. Cardillo,⁵⁰ I. Carli,¹³⁹ T. Carli,³⁵ G. Carlino,⁶⁷a B. T. Carlson,¹³⁵ L. Carminati,⁶⁶a,⁶⁶b R. M. D. Carney,⁴³a,⁴³b S. Caron,¹¹⁷

E. Carquin,¹⁴⁴b S. Carrá,⁶⁶a,⁶⁶b G. D. Carrillo-Montoya,³⁵ D. Casadei,³²b M. P. Casado,¹⁴,i A. F. Casha,¹⁶⁵ M. Casolino,¹⁴

D. W. Casper,¹⁶⁹ R. Castelijn,¹¹⁸ V. Castillo Gimenez,¹⁷² N. F. Castro,¹³⁶a,¹³⁶e A. Catinaccio,³⁵ J. R. Catmore,¹³⁰ A. Cattai,³⁵
J. Caudron,²⁴ V. Cavaliere,²⁹ E. Cavallaro,¹⁴ D. Cavalli,⁶⁶a M. Cavalli-Sforza,¹⁴ V. Cavasinni,⁶⁹a,⁶⁹b E. Celebi,¹²b

F. Ceradini,⁷²a,⁷²b L. Cerda Alberich,¹⁷² A. S. Cerqueira,⁷⁸a A. Cerri,¹⁵³ L. Cerrito,⁷¹a,⁷¹b F. Cerutti,¹⁸ A. Cervelli,²³b,²³a

S. A. Cetin,¹²b A. Chafaq,³⁴a D. Chakraborty,¹¹⁹ S. K. Chan,⁵⁷ W. S. Chan,¹¹⁸ Y. L. Chan,⁶¹a P. Chang,¹⁷¹ J. D. Chapman,³¹

D. G. Charlton,²¹ C. C. Chau,³³ C. A. Chavez Barajas,¹⁵³ S. Che,¹²² A. Chegwidden,¹⁰⁴ S. Chekanov,⁶ S. V. Chekulaev,¹⁶⁶a
G. A. Chelkov,⁷⁷j M. A. Chelstowska,³⁵ C. Chen,⁵⁸a C. H. Chen,⁷⁶ H. Chen,²⁹ J. Chen,⁵⁸a J. Chen,³⁸ S. Chen,¹³³

S. J. Chen,¹⁵c X. Chen,¹⁵b, k Y. Chen,⁸⁰ Y.-H. Chen,⁴⁴ H. C. Cheng,¹⁰³ H. J. Cheng,¹⁵d A. Cheplakov,⁷⁷ E. Cheremushkina,¹⁴⁰
R. Cherkaoui El Moursli,³⁴e E. Cheu,⁷ K. Cheung,⁶² L. Chevalier,¹⁴² V. Chiarella,⁴⁹ G. Chiarelli,⁶⁹a G. Chiodini,⁶⁵a

A. S. Chisholm,³⁵ A. Chitan,²⁷b I. Chiu,¹⁶¹ Y. H. Chiu,¹⁷⁴ M. V. Chizhov,⁷⁷ K. Choi,⁶³ A. R. Chomont,¹²⁸ S. Chouridou,¹⁶⁰

Y. S. Chow,¹¹⁸ V. Christodoulou,⁹² M. C. Chu,⁶¹a J. Chudoba,¹³⁷ A. J. Chuinard,¹⁰¹ J. J. Chwastowski,⁸² L. Chytka,¹²⁶

D. Cinca,⁴⁵ V. Cindro,⁸⁹ I. A. Cioară,²⁴ A. Ciocio,¹⁸ F. Cirotto,⁶⁷a,⁶⁷b Z. H. Citron,¹⁷⁸ M. Citterio,⁶⁶a A. Clark,⁵²

M. R. Clark,³⁸ P. J. Clark,⁴⁸ C. Clement,⁴³a,⁴³b Y. Coadou,⁹⁹ M. Cobal,⁶⁴a,⁶⁴c A. Coccaro,⁵³b,⁵³a J. Cochran,⁷⁶

A. E. C. Coimbra,¹⁷⁸ L. Colasurdo,¹¹⁷ B. Cole,³⁸ A. P. Colijn,¹¹⁸ J. Collot,⁵⁶ P. Conde Muiño,¹³⁶a,¹³⁶b E. Coniavitis,⁵⁰

S. H. Connell,³²b I. A. Connelly,⁹⁸ S. Constantinescu,²⁷b F. Conventi,⁶⁷a,¹ A. M. Cooper-Sarkar,¹³¹ F. Cormier,¹⁷³

K. J. R. Cormier,¹⁶⁵ M. Corradi,⁷⁰a,⁷⁰b E. E. Corrigan,⁹⁴ F. Corriveau,¹⁰¹,m A. Cortes-Gonzalez,³⁵ M. J. Costa,¹⁷²

D. Costanzo,¹⁴⁶ G. Cottin,³¹ G. Cowan,⁹¹ B. E. Cox,⁹⁸ J. Crane,⁹⁸ K. Cranmer,¹²¹ S. J. Crawley,⁵⁵ R. A. Creager,¹³³

G. Cree,³³ S. Crépé-Renaudin,⁵⁶ F. Crescioli,¹³² M. Cristinziani,²⁴ V. Croft,¹²¹ G. Crosetti,⁴⁰b,⁴⁰a A. Cueto,⁹⁶

T. Cuhadar Donszelmann,¹⁴⁶ A. R. Cukierman,¹⁵⁰ M. Curatolo,⁴⁹ J. Cúth,⁹⁷ S. Czekierda,⁸² P. Czodrowski,³⁵

M. J. Da Cunha Sargedas De Sousa,⁵⁸b,¹³⁶b C. Da Via,⁹⁸ W. Dabrowski,⁸¹a T. Dado,²⁸a,¹ S. Dahbi,³⁴e T. Dai,¹⁰³ F. Dallaire,¹⁰⁷

C. Dallapiccola,¹⁰⁰ M. Dam,³⁹ G. D'amen,²³b,²³a J. R. Dandoy,¹³³ M. F. Daneri,³⁰ N. P. Dang,¹⁷⁹,e N. D. Dann,⁹⁸

M. Danninger,¹⁷³ V. Dao,³⁵ G. Darbo,⁵³b S. Darmora,⁸ O. Dartsi,⁵ A. Dattagupta,¹²⁷ T. Daubney,⁴⁴ S. D'Auria,⁵⁵ W. Davey,²⁴

C. David,⁴⁴ T. Davidek,¹³⁹ D. R. Davis,⁴⁷ E. Dawe,¹⁰² I. Dawson,¹⁴⁶ K. De,⁸ R. De Asmundis,⁶⁷a A. De Benedetti,¹²⁴

S. De Castro,²³b,²³a S. De Cecco,⁷⁰a,⁷⁰b N. De Groot,¹¹⁷ P. de Jong,¹¹⁸ H. De la Torre,¹⁰⁴ F. De Lorenzi,⁷⁶ A. De Maria,⁵¹,n

D. De Pedis,⁷⁰a A. De Salvo,⁷⁰a U. De Sanctis,⁷¹a,⁷¹b A. De Santo,¹⁵³ K. De Vasconcelos Corga,⁹⁹ J. B. De Vivie De Regie,¹²⁸

C. Debenedetti,¹⁴³ D. V. Dedovich,⁷⁷ N. Dehghanian,³ M. Del Gaudio,⁴⁰b,⁴⁰a J. Del Peso,⁹⁶ D. Delgove,¹²⁸ F. Deliot,¹⁴²

C. M. Delitzsch,⁷ M. Della Pietra,⁶⁷a,⁶⁷b D. Della Volpe,⁵² A. Dell'Acqua,³⁵ L. Dell'Asta,²⁵ M. Delmastro,⁵ C. Delporte,¹²⁸

P. A. Delsart,⁵⁶ D. A. DeMarco,¹⁶⁵ S. Demers,¹⁸¹ M. Demichev,⁷⁷ S. P. Denisov,¹⁴⁰ D. Denysiuk,¹¹⁸ L. D'Eramo,¹³²

D. Derendarz,⁸² J. E. Derkaoui,³⁴d F. Derue,¹³² P. Dervan,⁸⁸ K. Desch,²⁴ C. Deterre,⁴⁴ K. Dette,¹⁶⁵ M. R. Devesa,³⁰

P. O. Deviveiros,³⁵ A. Dewhurst,¹⁴¹ S. Dhaliwal,²⁶ F. A. Di Bello,⁵² A. Di Ciaccio,⁷¹a,⁷¹b L. Di Ciaccio,⁵

W. K. Di Clemente,¹³³ C. Di Donato,⁶⁷a,⁶⁷b A. Di Girolamo,³⁵ B. Di Micco,⁷²a,⁷²b R. Di Nardo,³⁵ K. F. Di Petrillo,⁵⁷

A. Di Simone,⁵⁰ R. Di Sipio,¹⁶⁵ D. Di Valentino,³³ C. Diaconu,⁹⁹ M. Diamond,¹⁶⁵ F. A. Dias,³⁹ T. Dias Do Vale,¹³⁶a

M. A. Diaz,¹⁴⁴a J. Dickinson,¹⁸ E. B. Diehl,¹⁰³ J. Dietrich,¹⁹ S. Díez Cornell,⁴⁴ A. Dimitrievska,¹⁸ J. Dingfelder,²⁴ F. Dittus,³⁵

F. Djama,⁹⁹ T. Djobava,¹⁵⁷b J. I. Djuvsland,⁵⁹a M. A. B. Do Vale,⁷⁸c M. Dobre,²⁷b D. Dodsworth,²⁶ C. Doglioni,⁹⁴

J. Dolejsi,¹³⁹ Z. Dolezal,¹³⁹ M. Donadelli,⁷⁸d J. Donini,³⁷ A. D'onofrio,⁹⁰ M. D'Onofrio,⁸⁸ J. Dopke,¹⁴¹ A. Doria,⁶⁷a

M. T. Dova,⁸⁶ A. T. Doyle,⁵⁵ E. Drechsler,⁵¹ E. Dreyer,¹⁴⁹ T. Dreyer,⁵¹ M. Dris,¹⁰ Y. Du,⁵⁸b J. Duarte-Campderros,¹⁵⁹

F. Dubinin,¹⁰⁸ A. Dubreuil,⁵² E. Duchovni,¹⁷⁸ G. Duckeck,¹¹² A. Ducourthial,¹³² O. A. Ducu,¹⁰⁷,o D. Duda,¹¹⁸ A. Dudarev,³⁵

A. C. Dudder,⁹⁷ E. M. Duffield,¹⁸ L. Duflot,¹²⁸ M. Dührssen,³⁵ C. Dülsen,¹⁸⁰ M. Dumancic,¹⁷⁸ A. E. Dumitriu,²⁷b, p

A. K. Duncan,⁵⁵ M. Dunford,⁵⁹a A. Duperrin,⁹⁹ H. Duran Yildiz,⁴a M. Düren,⁵⁴ A. Durglishvili,¹⁵⁷b D. Duschinger,⁴⁶

B. Dutta,⁴⁴ D. Duvnjak,¹ M. Dyndal,⁴⁴ B. S. Dziedzic,⁸² C. Eckardt,⁴⁴ K. M. Ecker,¹¹³ R. C. Edgar,¹⁰³ T. Eifert,³⁵ G. Eigen,¹⁷
K. Einsweiler,¹⁸ T. Ekelof,¹⁷⁰ M. El Kacimi,³⁴c R. El Kosseifi,⁹⁹ V. Ellajosyula,⁹⁹ M. Ellert,¹⁷⁰ F. Ellinghaus,¹⁸⁰

A. A. Elliot,¹⁷⁴ N. Ellis,³⁵ J. Elmsheuser,²⁹ M. Elsing,³⁵ D. Emeliyanov,¹⁴¹ Y. Enari,¹⁶¹ J. S. Ennis,¹⁷⁶ M. B. Epland,⁴⁷
J. Erdmann,⁴⁵ A. Ereditato,²⁰ S. Errede,¹⁷¹ M. Escalier,¹²⁸ C. Escobar,¹²⁷ B. Esposito,⁴⁹ O. Estrada Pastor,¹⁷²

A. I. Etienvre,¹⁴² E. Etzion,¹⁵⁹ H. Evans,⁶³ A. Ezhilov,¹³⁴ M. Ezzi,³⁴e F. Fabbri,²³b,²³a L. Fabbri,²³b,²³a V. Fabiani,¹¹⁷

G. Facini,⁹² R. M. Faisca Rodrigues Pereira,¹³⁶a R. M. Fakhruvdinov,¹⁴⁰ S. Falciano,⁷⁰a P. J. Falke,⁵ S. Falke,⁵ J. Faltova,¹³⁹

Y. Fang,¹⁵a M. Fanti,⁶⁶a,⁶⁶b A. Farbin,⁸ A. Farilla,⁷²a E. M. Farina,⁶⁸a,⁶⁸b T. Farooque,¹⁰⁴ S. Farrell,¹⁸ S. M. Farrington,¹⁷⁶
P. Farthouat,³⁵ F. Fassi,³⁴e P. Fassnacht,³⁵ D. Fassouliotis,⁹ M. Faucci Giannelli,⁴⁸ A. Favareto,⁵³b,⁵³a W. J. Fawcett,⁵²

L. Fayard,¹²⁸ O. L. Fedin,¹³⁴,q W. Fedorko,¹⁷³ M. Feickert,⁴¹ S. Feigl,¹³⁰ L. Feligioni,⁹⁹ C. Feng,⁵⁸b E. J. Feng,³⁵ M. Feng,⁴⁷

M. J. Fenton,⁵⁵ A. B. Fenyuk,¹⁴⁰ L. Feremenga,⁸ J. Ferrando,⁴⁴ A. Ferrari,¹⁷⁰ P. Ferrari,¹¹⁸ R. Ferrari,⁶⁸a

D. E. Ferreira de Lima,⁵⁹b A. Ferrer,¹⁷² D. Ferrere,⁵² C. Ferretti,¹⁰³ F. Fiedler,⁹⁷ A. Filipčič,⁸⁹ F. Filthaut,¹¹⁷

M. Fincke-Keeler,¹⁷⁴ K. D. Finelli,²⁵ M. C. N. Fiolhais,¹³⁶a,¹³⁶c,r L. Fiorini,¹⁷² C. Fischer,¹⁴ W. C. Fisher,¹⁰⁴ N. Flaschel,⁴⁴

I. Fleck,¹⁴⁸ P. Fleischmann,¹⁰³ R. R. M. Fletcher,¹³³ T. Flick,¹⁸⁰ B. M. Flierl,¹¹² L. M. Flores,¹³³ L. R. Flores Castillo,⁶¹a

N. Fomin,¹⁷ G. T. Forcolin,⁹⁸ A. Formica,¹⁴² F. A. Förster,¹⁴ A. C. Forti,⁹⁸ A. G. Foster,²¹ D. Fournier,¹²⁸ H. Fox,⁸⁷

S. Fracchia,¹⁴⁶ P. Francavilla,⁶⁹a,⁶⁹b M. Franchini,²³b,²³a S. Franchino,⁵⁹a D. Francis,³⁵ L. Franconi,¹³⁰ M. Franklin,⁵⁷

M. Frate,¹⁶⁹ M. Fraternali,⁶⁸a,⁶⁸b D. Freeborn,⁹² S. M. Fressard-Batraneanu,³⁵ B. Freund,¹⁰⁷ W. S. Freund,⁷⁸b

D. Froidevaux,³⁵ J. A. Frost,¹³¹ C. Fukunaga,¹⁶² T. Fusayasu,¹¹⁴ J. Fuster,¹⁷² O. Gabizon,¹⁵⁸ A. Gabrielli,²³b,²³a

A. Gabrielli,¹⁸ G. P. Gach,⁸¹a S. Gadatsch,⁵² P. Gadow,¹¹³ G. Gagliardi,⁵³b,⁵³a L. G. Gagnon,¹⁰⁷ C. Galea,²⁷b

B. Galhardo,¹³⁶a,¹³⁶c E. J. Gallas,¹³¹ B. J. Gallop,¹⁴¹ P. Gallus,¹³⁸ G. Galster,³⁹ R. Gamboa Goni,⁹⁰ K. K. Gan,¹²²

S. Ganguly,¹⁷⁸ Y. Gao,⁸⁸ Y. S. Gao,¹⁵⁰,f C. García,¹⁷² J. E. García Navarro,¹⁷² J. A. García Pascual,¹⁵a M. Garcia-Sciveres,¹⁸

R. W. Gardner,³⁶ N. Garelli,¹⁵⁰ V. Garonne,¹³⁰ K. Gasnikova,⁴⁴ A. Gaudiello,⁵³b,⁵³a G. Gaudio,⁶⁸a I. L. Gavrilenko,¹⁰⁸

A. Gavrilyuk,¹⁰⁹ C. Gay,¹⁷³ G. Gaycken,²⁴ E. N. Gazis,¹⁰ C. N. P. Gee,¹⁴¹ J. Geisen,⁵¹ M. Geisen,⁹⁷ M. P. Geisler,⁵⁹a

K. Gellerstedt,⁴³a,⁴³b C. Gemme,⁵³b M. H. Genest,⁵⁶ C. Geng,¹⁰³ S. Gentile,⁷⁰a,⁷⁰b C. Gentsos,¹⁶⁰ S. George,⁹¹ D. Gerbaudo,¹⁴

G. Gessner,⁴⁵ S. Ghasemi,¹⁴⁸ M. Ghneimat,²⁴ B. Giacobbe,²³b S. Giagu,⁷⁰a,⁷⁰b N. Giangiacomi,²³b,²³a P. Giannetti,⁶⁹a

S. M. Gibson,⁹¹ M. Gignac,¹⁴³ D. Gillberg,³³ G. Gilles,¹⁸⁰ D. M. Gingrich,³d M. P. Giordani,⁶⁴a,⁶⁴c F. M. Giorgi,²³b

P. F. Giraud,¹⁴² P. Giromini,⁵⁷ G. Giugliarelli,⁶⁴a,⁶⁴c D. Giugni,⁶⁶a F. Giuli,¹³¹ M. Giulini,⁵⁹b S. Gkaitatzis,¹⁶⁰ I. Gkialas,⁹,⁵

E. L. Gkougkousis,¹⁴ P. Gkountoumis,¹⁰ L. K. Gladilin,¹¹¹ C. Glasman,⁹⁶ J. Glatzer,¹⁴ P. C. F. Glaysher,⁴⁴ A. Glazov,⁴⁴

M. Goblirsch-Kolb,²⁶ J. Godlewski,⁸² S. Goldfarb,¹⁰² T. Golling,⁵² D. Golubkov,¹⁴⁰ A. Gomes,¹³⁶a,¹³⁶b,¹³⁶d

R. Goncalves Gama,⁷⁸a R. Gonçalo,¹³⁶a G. Gonella,⁵⁰ L. Gonella,²¹ A. Gongadze,⁷⁷ F. Gonnella,²¹ J. L. Gonski,⁵⁷

S. González de la Hoz,¹⁷² S. Gonzalez-Sevilla,⁵² L. Goossens,³⁵ P. A. Gorbounov,¹⁰⁹ H. A. Gordon,²⁹ B. Gorini,³⁵

E. Gorini,⁶⁵a,⁶⁵b A. Gorišek,⁸⁹ A. T. Goshaw,⁴⁷ C. Gössling,⁴⁵ M. I. Gostkin,⁷⁷ C. A. Gottardo,²⁴ C. R. Goudet,¹²⁸

D. Goujdami,³⁴c A. G. Goussiou,¹⁴⁵ N. Govender,³²b,t C. Goy,⁵ E. Gozani,¹⁵⁸ I. Grabowska-Bold,⁸¹a P. O. J. Gradin,¹⁷⁰

E. C. Graham,⁸⁸ J. Gramling,¹⁶⁹ E. Gramstad,¹³⁰ S. Grancagnolo,¹⁹ V. Gratchev,¹³⁴ P. M. Gravila,²⁷f C. Gray,⁵⁵ H. M. Gray,¹⁸

Z. D. Greenwood,⁹³,u C. Grefe,²⁴ K. Gregersen,⁹² I. M. Gregor,⁴⁴ P. Grenier,¹⁵⁰ K. Grevtsov,⁴⁴ J. Griffiths,⁸ A. A. Grillo,¹⁴³

K. Grimm,¹⁵⁰ S. Grinstein,¹⁴,v Ph. Gris,³⁷ J.-F. Grivaz,¹²⁸ S. Groh,⁹⁷ E. Gross,¹⁷⁸ J. Grosse-Knetter,⁵¹ G. C. Grossi,⁹³

Z. J. Grout,⁹² C. Grud,¹⁰³ A. Grummer,¹¹⁶ L. Guan,¹⁰³ W. Guan,¹⁷⁹ J. Guenther,³⁵ A. Guerguichon,¹²⁸ F. Guescini,¹⁶⁶a

D. Guest,¹⁶⁹ R. Gugel,⁵⁰ B. Gui,¹²² T. Guillemin,⁵ S. Guindon,³⁵ U. Gul,⁵⁵ C. Gumpert,³⁵ J. Guo,⁵⁸c W. Guo,¹⁰³ Y. Guo,⁵⁸a,w

Z. Guo,⁹⁹ R. Gupta,⁴¹ S. Gurbuz,¹²c G. Gustavino,¹²⁴ B. J. Gutelman,¹⁵⁸ P. Gutierrez,¹²⁴ C. Gutschow,⁹² C. Guyot,¹⁴²

M. P. Guzik,⁸¹a C. Gwenlan,¹³¹ C. B. Gwilliam,⁸⁸ A. Haas,¹²¹ C. Haber,¹⁸ H. K. Hadavand,⁸ N. Haddad,³⁴e A. Hadef,⁵⁸a

S. Hageböck,²⁴ M. Hagihara,¹⁶⁷ H. Hakobyan,¹⁸²,a M. Haleem,¹⁷⁵ J. Haley,¹²⁵ G. Halladjian,¹⁰⁴ G. D. Hallewell,⁹⁹

K. Hamacher,¹⁸⁰ P. Hamal,¹²⁶ K. Hamano,¹⁷⁴ A. Hamilton,³²a G. N. Hamity,¹⁴⁶ K. Han,⁵⁸a,x L. Han,⁵⁸a S. Han,¹⁵d

K. Hanagaki,⁷⁹,y M. Hance,¹⁴³ D. M. Handl,¹¹² B. Haney,¹³³ R. Hankache,¹³² P. Hanke,⁵⁹a E. Hansen,⁹⁴ J. B. Hansen,³⁹

J. D. Hansen,³⁹ M. C. Hansen,²⁴ P. H. Hansen,³⁹ K. Hara,¹⁶⁷ A. S. Hard,¹⁷⁹ T. Harenberg,¹⁸⁰ S. Harkusha,¹⁰⁵ P. F. Harrison,¹⁷⁶

N. M. Hartmann,¹¹² Y. Hasegawa,¹⁴⁷ A. Hasib,⁴⁸ S. Hassani,¹⁴² S. Haug,²⁰ R. Hauser,¹⁰⁴ L. Hauswald,⁴⁶ L. B. Havener,³⁸

M. Havranek,¹³⁸ C. M. Hawkes,²¹ R. J. Hawkings,³⁵ D. Hayden,¹⁰⁴ C. Hayes,¹⁵² C. P. Hays,¹³¹ J. M. Hays,⁹⁰

H. S. Hayward,⁸⁸ S. J. Haywood,¹⁴¹ M. P. Heath,⁴⁸ V. Hedberg,⁹⁴ L. Heelan,⁸ S. Heer,²⁴ K. K. Heidegger,⁵⁰ J. Heilman,³³

S. Heim,⁴⁴ T. Heim,¹⁸ B. Heinemann,⁴⁴,z J. J. Heinrich,¹¹² L. Heinrich,¹²¹ C. Heinz,⁵⁴ J. Hejbal,¹³⁷ L. Helary,³⁵ A. Held,¹⁷³

S. Hellesund,¹³⁰ S. Hellman,⁴³a,⁴³b C. Helsens,³⁵ R. C. W. Henderson,⁸⁷ Y. Heng,¹⁷⁹ S. Henkelmann,¹⁷³

A. M. Henriques Correia,³⁵ G. H. Herbert,¹⁹ H. Herde,²⁶ V. Herget,¹⁷⁵ Y. Hernández Jiménez,³²c H. Herr,⁹⁷ G. Herten,⁵⁰

R. Hertenberger,¹¹² L. Hervas,³⁵ T. C. Herwig,¹³³ G. G. Hesketh,⁹² N. P. Hessey,¹⁶⁶a J. W. Hetherly,⁴¹ S. Higashino,⁷⁹

E. Higón-Rodriguez,¹⁷² K. Hildebrand,³⁶ E. Hill,¹⁷⁴ J. C. Hill,³¹ K. H. Hiller,⁴⁴ S. J. Hillier,²¹ M. Hils,⁴⁶ I. Hinchliffe,¹⁸

M. Hirose,¹²⁹ D. Hirschbuehl,¹⁸⁰ B. Hiti,⁸⁹ O. Hladik,¹³⁷ D. R. Hlaluku,³²c X. Hoad,⁴⁸ J. Hobbs,¹⁵² N. Hod,¹⁶⁶a

M. C. Hodgkinson,¹⁴⁶ A. Hoecker,³⁵ M. R. Hoeferkamp,¹¹⁶ F. Hoenig,¹¹² D. Hohn,²⁴ D. Hohov,¹²⁸ T. R. Holmes,³⁶

M. Holzbock,¹¹² M. Homann,⁴⁵ S. Honda,¹⁶⁷ T. Honda,⁷⁹ T. M. Hong,¹³⁵ A. Hönle,¹¹³ B. H. Hooberman,¹⁷¹

W. H. Hopkins,¹²⁷ Y. Horii,¹¹⁵ P. Horn,⁴⁶ A. J. Horton,¹⁴⁹ L. A. Horyn,³⁶ J-Y. Hostachy,⁵⁶ A. Hostiuc,¹⁴⁵ S. Hou,¹⁵⁵

A. Hoummada,³⁴a J. Howarth,⁹⁸ J. Hoya,⁸⁶ M. Hrabovsky,¹²⁶ J. Hrdinka,³⁵ I. Hristova,¹⁹ J. Hrivnac,¹²⁸ A. Hrynevich,¹⁰⁶
T. Hryn'ova,⁵ P. J. Hsu,⁶² S.-C. Hsu,¹⁴⁵ Q. Hu,²⁹ S. Hu,⁵⁸c Y. Huang,¹⁵a Z. Hubacek,¹³⁸ F. Hubaut,⁹⁹ M. Huebner,²⁴ F. Huegging,²⁴ T. B. Huffman,¹³¹ E. W. Hughes,³⁸ M. Huhtinen,³⁵ R. F. H. Hunter,³³ P. Huo,¹⁵² A. M. Hupe,³³ N. Huseynov,⁷⁷,c J. Huston,¹⁰⁴ J. Huth,⁷⁵ R. Hyneman,¹⁰³ G. Iacobucci,⁵² G. Iakovidis,²⁹ I. Ibragimov,¹⁴⁸

L. Iconovidou-Fayard,¹²⁸ Z. Idrissi,³⁴c P. Iengo,³⁵ R. Ignazzi,³⁹ O. Igonkina,¹¹⁸,aa R. Iguchi,¹⁶¹ T. Iizawa,¹⁷⁷ Y. Ikegami,⁷⁹ M. Ikeno,⁷⁹ D. Iliadis,¹⁶⁰ N. Ilic,¹⁵⁰ F. Iltzsche,⁴⁶ G. Introzzi,⁶⁸a,⁶⁸b M. Iodice,⁷²a K. Iordanidou,³⁸ V. Ippolito,⁷⁰a,⁷⁰b

M. F. Isacson,¹⁷⁰ N. Ishijima,¹²⁹ M. Ishino,¹⁶¹ M. Ishitsuka,¹⁶³ C. Issever,¹³¹ S. Istin,¹²c,bb F. Ito,¹⁶⁷ J. M. Iturbe Ponce,⁶¹a

R. Iuppa,⁷³a,⁷³b A. Ivina,¹⁷⁸ H. Iwasaki,⁷⁹ J. M. Izen,⁴² V. Izzo,⁶⁷a S. Jabbar,³ P. Jacka,¹³⁷ P. Jackson,¹ R. M. Jacobs,²⁴ V. Jain,² G. Jäkel,¹⁸⁰ K. B. Jakobi,⁹⁷ K. Jakobs,⁵⁰ S. Jakobsen,⁷⁴ T. Jakoubek,¹³⁷ D. O. Jamin,¹²⁵ D. K. Jana,⁹³ R. Jansky,⁵² J. Janssen,²⁴ M. Janus,⁵¹ P. A. Janus,⁸¹a G. Jarlskog,⁹⁴ N. Javadov,⁷⁷,c T. Javûrek,⁵⁰ M. Javurkova,⁵⁰ F. Jeanneau,¹⁴²

L. Jeanty,¹⁸ J. Jejelava,¹⁵⁷a,cc A. Jelinskas,¹⁷⁶ P. Jenni,⁵⁰,dd J. Jeong,⁴⁴ C. Jeske,¹⁷⁶ S. Jézéquel,⁵ H. Ji,¹⁷⁹ J. Jia,¹⁵² H. Jiang,⁷⁶

Y. Jiang,⁵⁸a Z. Jiang,¹⁵⁰ S. Jiggins,⁵⁰ F. A. Jimenez Morales,³⁷ J. Jimenez Pena,¹⁷² S. Jin,¹⁵c A. Jinaru,²⁷b O. Jinnouchi,¹⁶³ H. Jivan,³²c P. Johansson,¹⁴⁶ K. A. Johns,⁷ C. A. Johnson,⁶³ W. J. Johnson,¹⁴⁵ K. Jon-And,⁴³a,⁴³b R. W. L. Jones,⁸⁷

S. D. Jones,¹⁵³ S. Jones,⁷ T. J. Jones,⁸⁸ J. Jongmanns,⁵⁹a P. M. Jorge,¹³⁶a,¹³⁶b J. Jovicevic,¹⁶⁶a X. Ju,¹⁷⁹ J. J. Junggeburth,¹¹³ A. Juste Rozas,¹⁴,v A. Kaczmarska,⁸² M. Kado,¹²⁸ H. Kagan,¹²² M. Kagan,¹⁵⁰ T. Kaji,¹⁷⁷ E. Kajomovitz,¹⁵⁸

C. W. Kalderon,⁹⁴ A. Kaluza,⁹⁷ S. Kama,⁴¹ A. Kamenshchikov,¹⁴⁰ L. Kanjir,⁹⁹ Y. Kano,¹⁶¹ V. A. Kantserov,¹¹⁰ J. Kanzaki,⁷⁹ B. Kaplan,¹²¹ L. S. Kaplan,¹⁷⁹ D. Kar,³²c M. J. Kareem,¹⁶⁶b E. Karentzos,¹⁰ S. N. Karpov,⁷⁷ Z. M. Karpova,⁷⁷ V. Kartvelishvili,⁸⁷ A. N. Karyukhin,¹⁴⁰ K. Kasahara,¹⁶⁷ L. Kashif,¹⁷⁹ R. D. Kass,¹²² A. Kastanas,¹⁵¹ Y. Kataoka,¹⁶¹

C. Kato,¹⁶¹ J. Katzy,⁴⁴ K. Kawade,⁸⁰ K. Kawagoe,⁸⁵ T. Kawamoto,¹⁶¹ G. Kawamura,⁵¹ E. F. Kay,⁸⁸ V. F. Kazanin,¹²⁰b,¹²⁰a

R. Keeler,¹⁷⁴ R. Kehoe,⁴¹ J. S. Keller,³³ E. Kellermann,⁹⁴ J. J. Kempster,²¹ J. Kendrick,²¹ O. Kepka,¹³⁷ S. Kersten,¹⁸⁰ B. P. Kerševan,⁸⁹ R. A. Keyes,¹⁰¹ M. Khader,¹⁷¹ F. Khalil-Zada,¹³ A. Khanov,¹²⁵ A. G. Kharlamov,¹²⁰b,¹²⁰a

T. Kharlamova,¹²⁰b,¹²⁰a A. Khodinov,¹⁶⁴ T. J. Khoo,⁵² V. Khovanskiy,¹⁰⁹,a E. Khramov,⁷⁷ J. Khubua,¹⁵⁷b S. Kido,⁸⁰

M. Kiehn,⁵² C. R. Kilby,⁹¹ S. H. Kim,¹⁶⁷ Y. K. Kim,³⁶ N. Kimura,⁶⁴a,⁶⁴c O. M. Kind,¹⁹ B. T. King,⁸⁸ D. Kirchmeier,⁴⁶ J. Kirk,¹⁴¹ A. E. Kiryunin,¹¹³ T. Kishimoto,¹⁶¹ D. Kisielewska,⁸¹a V. Kitali,⁴⁴ O. Kivernyk,⁵ E. Kladiva,²⁸b

T. Klapdor-Kleingrothaus,⁵⁰ M. H. Klein,¹⁰³ M. Klein,⁸⁸ U. Klein,⁸⁸ K. Kleinknecht,⁹⁷ P. Klimek,¹¹⁹ A. Klimentov,²⁹ R. Klingenberg,⁴⁵,a T. Klingl,²⁴ T. Klioutchnikova,³⁵ F. F. Klitzner,¹¹² P. Kluit,¹¹⁸ S. Kluth,¹¹³ E. Kneringer,⁷⁴

E. B. F. G. Knoops,⁹⁹ A. Knue,⁵⁰ A. Kobayashi,¹⁶¹ D. Kobayashi,⁸⁵ T. Kobayashi,¹⁶¹ M. Kobel,⁴⁶ M. Kocian,¹⁵⁰ P. Kody,¹³⁹

T. Koffas,³³ E. Koffeman,¹¹⁸ N. M. Köhler,¹¹³ T. Koi,¹⁵⁰ M. Kolb,⁵⁹b I. Koletsou,⁵ T. Kondo,⁷⁹ N. Kondrashova,⁵⁸c K. Köneke,⁵⁰ A. C. König,¹¹⁷ T. Kono,⁷⁹ R. Konoplich,¹²¹,ee N. Konstantinidis,⁹² B. Konya,⁹⁴ R. Kopeliansky,⁶³

S. Koperny,⁸¹a K. Korcyl,⁸² K. Kordas,¹⁶⁰ A. Korn,⁹² I. Korolkov,¹⁴ E. V. Korolkova,¹⁴⁶ O. Kortner,¹¹³ S. Kortner,¹¹³

T. Kosek,¹³⁹ V. V. Kostyukhin,²⁴ A. Kotwal,⁴⁷ A. Koulouris,¹⁰ A. Kourkoumeli-Charalampidi,⁶⁸a,⁶⁸b C. Kourkoumelis,⁹

E. Kourlitis,¹⁴⁶ V. Kouskoura,²⁹ A. B. Kowalewska,⁸² R. Kowalewski,¹⁷⁴ T. Z. Kowalski,⁸¹a C. Kozakai,¹⁶¹ W. Kozanecki,¹⁴²

A. S. Kozhin,¹⁴⁰ V. A. Kramarenko,¹¹¹ G. Kramberger,⁸⁹ D. Krasnopevtsev,¹¹⁰ M. W. Krasny,¹³² A. Krasznahorkay,³⁵

D. Krauss,¹¹³ J. A. Kremer,⁸¹a J. Kretzschmar,⁸⁸ P. Krieger,¹⁶⁵ K. Krizka,¹⁸ K. Kroeninger,⁴⁵ H. Kroha,¹¹³ J. Kroll,¹³⁷ J. Kroll,¹³³ J. Krstic,¹⁶ U. Kruchonak,⁷⁷ H. Krüger,²⁴ N. Krumnack,⁷⁶ M. C. Kruse,⁴⁷ T. Kubota,¹⁰² S. Kuday,⁴b

J. T. Kuechler,¹⁸⁰ S. Kuehn,³⁵ A. Kugel,⁵⁹a F. Kuger,¹⁷⁵ T. Kuhl,⁴⁴ V. Kukhtin,⁷⁷ R. Kukla,⁹⁰ Y. Kulchitsky,¹⁵⁰

S. Kuleshov,¹⁴⁴b Y. P. Kulinich,¹⁷¹ M. Kuna,⁵⁶ T. Kunigo,⁸³ A. Kupco,¹³⁷ T. Kupfer,⁴⁵ O. Kuprash,¹⁵⁹ H. Kurashige,⁸⁰

L. L. Kurchaninov,¹⁶⁶a Y. A. Kurochkin,¹⁵⁰ M. G. Kurth,¹⁵d E. S. Kuwertz,¹⁷⁴ M. Kuze,¹⁶³ J. Kvita,¹²⁶ T. Kwan,¹⁷⁴

A. La Rosa,¹¹³ J. L. La Rosa Navarro,⁷⁸d L. La Rotonda,⁴⁰b,⁴⁰a F. La Ruffa,⁴⁰b,⁴⁰a C. Lacasta,¹⁷² F. Lacava,⁷⁰a,⁷⁰b J. Lacey,⁴⁴

D. P. J. Lack,⁹⁸ H. Lacker,¹⁹ D. Lacour,¹³² E. Ladygin,⁷⁷ R. Lafaye,⁵ B. Laforge,¹³² T. Lagouri,³²c S. Lai,⁵¹ S. Lammers,⁶³ W. Lampl,⁷ E. Lançon,²⁹ U. Landgraf,⁵⁰ M. P. J. Landon,⁹⁰ M. C. Lanfermann,⁵² V. S. Lang,⁴⁴ J. C. Lange,¹⁴

R. J. Langenberg,³⁵ A. J. Lankford,¹⁶⁹ F. Lanni,²⁹ K. Lantzsch,²⁴ A. Lanza,⁶⁸a A. Lapertosa,⁵³b,⁵³a S. Laplace,¹³²

J. F. Laporte,¹⁴² T. Lari,⁶⁶a F. Lasagni Manghi,²³b,²³a M. Lassnig,³⁵ T. S. Lau,⁶¹a A. Laudrain,¹²⁸ A. T. Law,¹⁴³ P. Laycock,⁸⁸ M. Lazzaroni,⁶⁶a,⁶⁶b B. Le,¹⁰² O. Le Dortz,¹³² E. Le Guirriec,⁹⁹ E. P. Le Quilleuc,¹⁴² M. LeBlanc,⁷ T. LeCompte,⁶

F. Ledroit-Guillon,⁵⁶ C. A. Lee,²⁹ G. R. Lee,¹⁴⁴a L. Lee,⁵⁷ S. C. Lee,¹⁵⁵ B. Lefebvre,¹⁰¹ M. Lefebvre,¹⁷⁴ F. Legger,¹¹²

C. Leggett,¹⁸ G. Lehmann Miotto,³⁵ W. A. Leight,⁴⁴ A. Leisos,¹⁶⁰,ff M. A. L. Leite,⁷⁸d R. Leitner,¹³⁹ D. Lellouch,¹⁷⁸

B. Lemmer,⁵¹ K. J. C. Leney,⁹² T. Lenz,²⁴ B. Lenzi,³⁵ R. Leone,⁷ S. Leone,⁶⁹a C. Leonidopoulos,⁴⁸ G. Lerner,¹⁵³ C. Leroy,¹⁰⁷

R. Les,¹⁶⁵ A. A. J. Lesage,¹⁴² C. G. Lester,³¹ M. Levchenko,¹³⁴ J. Levêque,⁵ D. Levin,¹⁰³ L. J. Levinson,¹⁷⁸ D. Lewis,⁹⁰

B. Li,¹⁰³ C.-Q. Li,⁵⁸a H. Li,⁵⁸b L. Li,⁵⁸c Q. Li,¹⁵d Q. Y. Li,⁵⁸a S. Li,⁵⁸d,⁵⁸c X. Li,⁵⁸c Y. Li,¹⁴⁸ Z. Liang,¹⁵a B. Liberti,⁷¹a

A. Liblong,¹⁶⁵ K. Lie,⁶¹c S. Liem,¹¹⁸ A. Limosani,¹⁵⁴ C. Y. Lin,³¹ K. Lin,¹⁰⁴ S. C. Lin,¹⁵⁶ T. H. Lin,⁹⁷ R. A. Linck,⁶³
B. E. Lindquist,¹⁵² A. L. Lionti,⁵² E. Lipeles,¹³³ A. Lipniacka,¹⁷ M. Lisovyi,⁵⁹b T. M. Liss,¹⁷¹,gg A. Lister,¹⁷³ A. M. Litke,¹⁴³

J. D. Little,⁸ B. Liu,⁷⁶ B. L. Liu,⁶ H. B. Liu,²⁹ H. Liu,¹⁰³ J. B. Liu,⁵⁸a J. K. K. Liu,¹³¹ K. Liu,¹³² M. Liu,⁵⁸a P. Liu,¹⁸

Y. L. Liu,⁵⁸a Y. W. Liu,⁵⁸a M. Livan,⁶⁸a,⁶⁸b A. Lleres,⁵⁶ J. Llorente Merino,¹⁵a S. L. Lloyd,⁹⁰ C. Y. Lo,⁶¹b F. Lo Sterzo,⁴¹

E. M. Lobodzinska,⁴⁴ P. Loch,⁷ F. K. Loebinger,⁹⁸ A. Loesle,⁵⁰ K. M. Loew,²⁶ T. Lohse,¹⁹ K. Lohwasser,¹⁴⁶ M. Lokajicek,¹³⁷

B. A. Long,²⁵ J. D. Long,¹⁷¹ R. E. Long,⁸⁷ L. Longo,⁶⁵a,⁶⁵b K. A. Looper,¹²² J. A. Lopez,¹⁴⁴b I. Lopez Paz,¹⁴

A. Lopez Solis,¹³² J. Lorenz,¹¹² N. Lorenzo Martinez,⁵ M. Losada,²² P. J. Lösel,¹¹² X. Lou,⁴⁴ X. Lou,¹⁵a A. Lounis,¹²⁸

J. Love,⁶ P. A. Love,⁸⁷ J. J. Lozano Bahilo,¹⁷² H. Lu,⁶¹a N. Lu,¹⁰³ Y. J. Lu,⁶² H. J. Lubatti,¹⁴⁵ C. Luci,⁷⁰a,⁷⁰b A. Lucotte,⁵⁶

C. Luedtke,⁵⁰ F. Luehring,⁶³ I. Luise,¹³² W. Lukas,⁷⁴ L. Luminari,⁷⁰a B. Lund-Jensen,¹⁵¹ M. S. Lutz,¹⁰⁰ P. M. Luzi,¹³²

D. Lynn,²⁹ R. Lysak,¹³⁷ E. Lytken,⁹⁴ F. Lyu,¹⁵a V. Lyubushkin,⁷⁷ H. Ma,²⁹ L. L. Ma,⁵⁸b Y. Ma,⁵⁸b G. Maccarrone,⁴⁹

A. Macchiolo,¹¹³ C. M. Macdonald,¹⁴⁶ J. Machado Miguens,¹³³,¹³⁶b D. Madaffari,¹⁷² R. Madar,³⁷ W. F. Mader,⁴⁶

A. Madsen,⁴⁴ N. Madysa,⁴⁶ J. Maeda,⁸⁰ S. Maeland,¹⁷ T. Maeno,²⁹ A. S. Maevskiy,¹¹¹ V. Magerl,⁵⁰ C. Maidantchik,⁷⁸b

T. Maier,¹¹² A. Maio,¹³⁶a,¹³⁶b,¹³⁶d O. Majersky,²⁸a S. Majewski,¹²⁷ Y. Makida,⁷⁹ N. Makovec,¹²⁸ B. Malaescu,¹³²

Pa. Malecki,⁸² V. P. Maleev,¹³⁴ F. Malek,⁵⁶ U. Mallik,⁷⁵ D. Malon,⁶ C. Malone,³¹ S. Maltezos,¹⁰ S. Malyukov,³⁵

J. Mamuzic,¹⁷² G. Mancini,⁴⁹ I. Mandić,⁸⁹ J. Maneira,¹³⁶a L. Manhaes de Andrade Filho,⁷⁸a J. Manjarres Ramos,⁴⁶

K. H. Mankinen,⁹⁴ A. Mann,¹¹² A. Manousos,⁷⁴ B. Mansoulie,¹⁴² J. D. Mansour,¹⁵a M. Mantoani,⁵¹ S. Manzoni,⁶⁶a,⁶⁶b

G. Marceca,³⁰ L. March,⁵² L. Marchese,¹³¹ G. Marchiori,¹³² M. Marcisovsky,¹³⁷ C. A. Marin Tobon,³⁵ M. Marjanovic,³⁷

D. E. Marley,¹⁰³ F. Marroquim,⁷⁸b Z. Marshall,¹⁸ M. U. F. Martensson,¹⁷⁰ S. Marti-Garcia,¹⁷² C. B. Martin,¹²²

T. A. Martin,¹⁷⁶ V. J. Martin,⁴⁸ B. Martin dit Latour,¹⁷ M. Martinez,¹⁴,ν V. I. Martinez Outschoorn,¹⁰⁰ S. Martin-Haugh,¹⁴¹

V. S. Martoiu,²⁷b A. C. Martyniuk,⁹² A. Marzin,³⁵ L. Masetti,⁹⁷ T. Mashimo,¹⁶¹ R. Mashinistov,¹⁰⁸ J. Masik,⁹⁸

A. L. Maslennikov,¹²⁰b,¹²⁰a L. H. Mason,¹⁰² L. Massa,⁷¹a,⁷¹b P. Mastrandrea,⁵ A. Mastroberardino,⁴⁰b,⁴⁰a T. Masubuchi,¹⁶¹

P. Mättig,¹⁸⁰ J. Maurer,²⁷b B. Maček,⁸⁹ S. J. Maxfield,⁸⁸ D. A. Maximov,¹²⁰b,¹²⁰a R. Mazini,¹⁵⁵ I. Maznas,¹⁶⁰ S. M. Mazza,¹⁴³

N. C. Mc Fadden,¹¹⁶ G. Mc Goldrick,¹⁶⁵ S. P. Mc Kee,¹⁰³ A. McCarn,¹⁰³ T. G. McCarthy,¹¹³ L. I. McClymont,⁹²

E. F. McDonald,¹⁰² J. A. Mcfayden,³⁵ G. Mchedlidze,⁵¹ M. A. McKay,⁴¹ K. D. McLean,¹⁷⁴ S. J. McMahon,¹⁴¹

P. C. McNamara,¹⁰² C. J. McNicol,¹⁷⁶ R. A. McPherson,¹⁷⁴,ml J. E. Mdhluli,³²c Z. A. Meadows,¹⁰⁰ S. Meehan,¹⁴⁵ T. Megy,⁵⁰

S. Mehlhase,¹¹² A. Mehta,⁸⁸ T. Meideck,⁵⁶ B. Meirose,⁴² D. Melini,¹⁷²,hh B. R. Mellado Garcia,³²c J. D. Mellenthin,⁵¹

M. Melo,²⁸a F. Meloni,²⁰ A. Melzer,²⁴ S. B. Menary,⁹⁸ L. Meng,⁸⁸ X. T. Meng,¹⁰³ A. Mengarelli,²³b,²³a S. Menke,¹¹³

E. Meoni,⁴⁰b,⁴⁰a S. Mergelmeyer,¹⁹ C. Merlassino,²⁰ P. Mermod,⁵² L. Merola,⁶⁷a,⁶⁷b C. Meroni,⁶⁶a F. S. Merritt,³⁶

A. Messina,⁷⁰a,⁷⁰b J. Metcalfe,⁶ A. S. Mete,¹⁶⁹ C. Meyer,¹³³ J. Meyer,¹⁵⁸ J-P. Meyer,¹⁴² H. Meyer Zu Theenhausen,⁵⁹a

F. Miano,¹⁵³ R. P. Middleton,¹⁴¹ L. Mijović,⁴⁸ G. Mikenberg,¹⁷⁸ M. Mikestikova,¹³⁷ M. Mikuž,⁸⁹ M. Milesi,¹⁰² A. Milic,¹⁶⁵

D. A. Millar,⁹⁰ D. W. Miller,³⁶ A. Milov,¹⁷⁸ D. A. Milstead,⁴³a,⁴³b A. A. Minaenko,¹⁴⁰ I. A. Minashvili,¹⁵⁷b A. I. Mincer,¹²¹

B. Mindur,⁸¹a M. Mineev,⁷⁷ Y. Minegishi,¹⁶¹ Y. Ming,¹⁷⁹ L. M. Mir,¹⁴ A. Mirto,⁶⁵a,⁶⁵b K. P. Mistry,¹³³ T. Mitani,¹⁷⁷

J. Mitrevski,¹¹² V. A. Mitsou,¹⁷² A. Miucci,²⁰ P. S. Miyagawa,¹⁴⁶ A. Mizukami,⁷⁹ J. U. Mjörnmark,⁹⁴ T. Mkrtchyan,¹⁸²

M. Mlynarikova,¹³⁹ T. Moa,⁴³a,⁴³b K. Mochizuki,¹⁰⁷ P. Mogg,⁵⁰ S. Mohapatra,³⁸ S. Molander,⁴³a,⁴³b R. Moles-Valls,²⁴

M. C. Mondragon,¹⁰⁴ K. Mönig,⁴⁴ J. Monk,³⁹ E. Monnier,⁹⁹ A. Montalbano,¹⁴⁹ J. Montejo Berlingen,³⁵ F. Monticelli,⁸⁶

S. Monzani,⁶⁶a R. W. Moore,³ N. Morange,¹²⁸ D. Moreno,²² M. Moreno Llácer,³⁵ P. Morettini,⁵³b M. Morgenstern,¹¹⁸

S. Morgenstern,³⁵ D. Mori,¹⁴⁹ T. Mori,¹⁶¹ M. Morii,⁵⁷ M. Morinaga,¹⁷⁷ V. Morisbak,¹³⁰ A. K. Morley,³⁵ G. Mornacchi,³⁵

J. D. Morris,⁹⁰ L. Morvaj,¹⁵² P. Moschovakos,¹⁰ M. Mosidze,¹⁵⁷b H. J. Moss,¹⁴⁶ J. Moss,¹⁵⁰,ii K. Motohashi,¹⁶³ R. Mount,¹⁵⁰

E. Mountricha,²⁹ E. J. W. Moyse,¹⁰⁰ S. Muanza,⁹⁹ F. Mueller,¹¹³ J. Mueller,¹³⁵ R. S. P. Mueller,¹¹² D. Muenstermann,⁸⁷

P. Mullen,⁵⁵ G. A. Mullier,²⁰ F. J. Munoz Sanchez,⁹⁸ P. Murin,²⁸b W. J. Murray,¹⁷⁶,¹⁴¹ A. Murrone,⁶⁶a,⁶⁶b M. Muškinja,⁸⁹

C. Mwewa,³²a A. G. Myagkov,¹⁴⁰,jj J. Myers,¹²⁷ M. Myska,¹³⁸ B. P. Nachman,¹⁸ O. Nackenhorst,⁴⁵ K. Nagai,¹³¹

R. Nagai,⁷⁹,kk K. Nagano,⁷⁹ Y. Nagasaka,⁶⁰ K. Nagata,¹⁶⁷ M. Nagel,⁵⁰ E. Nagy,⁹⁹ A. M. Nairz,³⁵ Y. Nakahama,¹¹⁵

K. Nakamura,⁷⁹ T. Nakamura,¹⁶¹ I. Nakano,¹²³ F. Napolitano,⁵⁹a R. F. Naranjo Garcia,⁴⁴ R. Narayan,¹¹ D. I. Narrias Villar,⁵⁹a

I. Naryshkin,¹³⁴ T. Naumann,⁴⁴ G. Navarro,²² R. Nayyar,⁷ H. A. Neal,¹⁰³ P. Y. Nechaeva,¹⁰⁸ T. J. Neep,¹⁴² A. Negri,⁶⁸a,⁶⁸b

M. Negrini,²³b S. Nektarijevic,¹¹⁷ C. Nellist,⁵¹ M. E. Nelson,¹³¹ S. Nemecek,¹³⁷ P. Nemethy,¹²¹ M. Nessi,³⁵,ll

M. S. Neubauer,¹⁷¹ M. Neumann,¹⁸⁰ P. R. Newman,²¹ T. Y. Ng,⁶¹c Y. S. Ng,¹⁹ H. D. N. Nguyen,⁹⁹ T. Nguyen Manh,¹⁰⁷

E. Nibigira,³⁷ R. B. Nickerson,¹³¹ R. Nicolaidou,¹⁴² J. Nielsen,¹⁴³ N. Nikiforou,¹¹ V. Nikolaenko,¹⁴⁰,jj I. Nikolic-Audit,¹³²

K. Nikolopoulos,²¹ P. Nilsson,²⁹ H. R. Nindhito,⁵² Y. Ninomiya,⁷⁹ A. Nisati,⁷⁰a N. Nishu,⁵⁸c R. Nisius,¹¹³ I. Nitsche,⁴⁵

T. Nitta,¹⁷⁷ T. Nobe,¹⁶¹ Y. Noguchi,⁸³ M. Nomachi,¹²⁹ I. Nomidis,³³ M. A. Nomura,²⁹ T. Nooney,⁹⁰ M. Nordberg,³⁵

N. Norjoharuddeen,¹³¹ T. Novak,⁸⁹ O. Novgorodova,⁴⁶ R. Novotny,¹³⁸ M. Nozaki,⁷⁹ L. Nozka,¹²⁶ K. Ntekas,¹⁶⁹ E. Nurse,⁹²
F. Nuti,¹⁰² F. G. Oakham,³³,d H. Oberlack,¹¹³ T. Obermann,²⁴ J. Ocariz,¹³² A. Ochi,⁸⁰ I. Ochoa,³⁸ J. P. Ochoa-Ricoux,¹⁴⁴a

K. O'Connor,²⁶ S. Oda,⁸⁵ S. Odaka,⁷⁹ A. Oh,⁹⁸ S. H. Oh,⁴⁷ C. C. Ohm,¹⁵¹ H. Oide,⁵³b,⁵³a H. Okawa,¹⁶⁷ Y. Okazaki,⁸³

Y. Okumura,¹⁶¹ T. Okuyama,⁷⁹ A. Olariu,²⁷b L. F. Oleiro Seabra,¹³⁶a S. A. Olivares Pino,¹⁴⁴a D. Oliveira Damazio,²⁹

J. L. Oliver,¹ M. J. R. Olsson,³⁶ A. Olszewski,⁸² J. Olszowska,⁸² D. C. O'Neil,¹⁴⁹ A. Onofre,¹³⁶a,¹³⁶e K. Onogi,¹¹⁵

P. U. E. Onyisi,¹¹ H. Oppen,¹³⁰ M. J. Oreglia,³⁶ Y. Oren,¹⁵⁹ D. Orestano,⁷²a,⁷²b E. C. Orgill,⁹⁸ N. Orlando,⁶¹b

A. A. O'Rourke,⁴⁴ R. S. Orr,¹⁶⁵ B. Osculati,⁵³b,⁵³a,a V. O'Shea,⁵⁵ R. Ospanov,⁵⁸a G. Otero y Garzon,³⁰ H. Otono,⁸⁵

M. Ouchrif,³⁴d F. Ould-Saada,¹³⁰ A. Ouraou,¹⁴² Q. Ouyang,¹⁵a M. Owen,⁵⁵ R. E. Owen,²¹ V. E. Ozcan,¹²c N. Ozturk,⁸

J. Pacalt,¹²⁶ H. A. Pacey,³¹ K. Pachal,¹⁴⁹ A. Pacheco Pages,¹⁴ L. Pacheco Rodriguez,¹⁴² C. Padilla Aranda,¹⁴

S. Pagan Griso,¹⁸ M. Paganini,¹⁸¹ G. Palacino,⁶³ S. Palazzo,⁴⁰b,⁴⁰a S. Palestini,³⁵ M. Palka,⁸¹b D. Pallin,³⁷ I. Panagoulias,¹⁰

C. E. Pandini,³⁵ J. G. Panduro Vazquez,⁹¹ P. Pani,³⁵ L. Paolozzi,⁵² T. D. Papadopoulou,¹⁰ K. Papageorgiou,⁹,s

A. Paramonov,⁶ D. Paredes Hernandez,⁶¹b B. Parida,⁵⁸c A. J. Parker,⁸⁷ K. A. Parker,⁴⁴ M. A. Parker,³¹ F. Parodi,⁵³b,⁵³a

J. A. Parsons,³⁸ U. Parzefall,⁵⁰ V. R. Pascuzzi,¹⁶⁵ J. M. P. Pasner,¹⁴³ E. Pasqualucci,⁷⁰a S. Passaggio,⁵³b F. Pastore,⁹¹

P. Pasuwan,⁴³a,⁴³b S. Pataraia,⁹⁷ J. R. Pater,⁹⁸ A. Pathak,¹⁷⁹e T. Pauly,³⁵ B. Pearson,¹¹³ M. Pedersen,¹³⁰ S. Pedraza Lopez,¹⁷²

R. Pedro,¹³⁶a,¹³⁶b S. V. Peleganchuk,¹²⁰b,¹²⁰a O. Penc,¹³⁷ C. Peng,¹⁵d H. Peng,⁵⁸a B. S. Peralva,⁷⁸a M. M. Perego,¹⁴²

A. P. Pereira Peixoto,¹³⁶a D. V. Perepelitsa,²⁹ F. Peri,¹⁹ L. Perini,⁶⁶a,⁶⁶b H. Pernegger,³⁵ S. Perrella,⁶⁷a,⁶⁷b

V. D. Peshekhonov,⁷⁷,a K. Peters,⁴⁴ R. F. Y. Peters,⁹⁸ B. A. Petersen,³⁵ T. C. Petersen,³⁹ E. Petit,⁵⁶ A. Petridis,¹ C. Petridou,¹⁶⁰

P. Petroff,¹²⁸ E. Petrolo,⁷⁰a M. Petrov,¹³¹ F. Petrucci,⁷²a,⁷²b N. E. Pettersson,¹⁰⁰ A. Peyaud,¹⁴² R. Pezoa,¹⁴⁴b T. Pham,¹⁰²

F. H. Phillips,¹⁰⁴ P. W. Phillips,¹⁴¹ G. Piacquadio,¹⁵² E. Pianori,¹⁸ A. Picazio,¹⁰⁰ M. A. Pickering,¹³¹ R. Piegaia,³⁰

J. E. Pilcher,³⁶ A. D. Pilkington,⁹⁸ M. Pinamonti,⁷¹a,⁷¹b J. L. Pinfold,³ M. Pitt,¹⁷⁸ M-A. Pleier,²⁹ V. Pleskot,¹³⁹

E. Plotnikova,⁷⁷ D. Pluth,⁷⁶ P. Podberezko,¹²⁰b,¹²⁰a R. Poettgen,⁹⁴ R. Poggi,⁶⁸a,⁶⁸b L. Poggioli,¹²⁸ I. Pogrebnyak,¹⁰⁴ D. Pohl,²⁴

I. Pokharel,⁵¹ G. Polesello,⁶⁸a A. Poley,⁴⁴ A. Policicchio,⁴⁰b,⁴⁰a R. Polifka,³⁵ A. Polini,²³b C. S. Pollard,⁴⁴ V. Polychronakos,²⁹

D. Ponomarenko,¹¹⁰ L. Pontecorvo,⁷⁰a G. A. Popeneciu,²⁷d D. M. Portillo Quintero,¹³² S. Pospisil,¹³⁸ K. Potamianos,⁴⁴

I. N. Potrap,⁷⁷ C. J. Potter,³¹ H. Potti,¹¹ T. Poulsen,⁹⁴ J. Poveda,³⁵ T. D. Powell,¹⁴⁶ M. E. Pozo Astigarraga,³⁵ P. Pralavorio,⁹⁹

S. Prell,⁷⁶ D. Price,⁹⁸ M. Primavera,⁶⁵a S. Prince,¹⁰¹ N. Proklova,¹¹⁰ K. Prokofiev,⁶¹c F. Prokoshin,¹⁴⁴b S. Protopopescu,²⁹

J. Proudfoot,⁶ M. Przybycien,⁸¹a A. Puri,¹⁷¹ P. Puzo,¹²⁸ J. Qian,¹⁰³ Y. Qin,⁹⁸ A. Quadt,⁵¹ M. Queitsch-Maitland,⁴⁴

A. Qureshi,¹ P. Rados,¹⁰² F. Ragusa,⁶⁶a,⁶⁶b G. Rahal,⁹⁵ J. A. Raine,⁹⁸ S. Rajagopalan,²⁹ T. Rashid,¹²⁸ S. Raspopov,⁵

M. G. Ratti,⁶⁶a,⁶⁶b D. M. Rauch,⁴⁴ F. Rauscher,¹¹² S. Rave,⁹⁷ B. Ravina,¹⁴⁶ I. Ravinovich,¹⁷⁸ J. H. Rawling,⁹⁸ M. Raymond,³⁵

A. L. Read,¹³⁰ N. P. Readioff,⁵⁶ M. Reale,⁶⁵a,⁶⁵b D. M. Rebuzzi,⁶⁸a,⁶⁸b A. Redelbach,¹⁷⁵ G. Redlinger,²⁹ R. Reece,¹⁴³

R. G. Reed,³²c K. Reeves,⁴² L. Rehnisch,¹⁹ J. Reichert,¹³³ A. Reiss,⁹⁷ C. Rembser,³⁵ H. Ren,¹⁵d M. Rescigno,⁷⁰a

S. Resconi,⁶⁶a E. D. Resseguie,¹³³ S. Rettie,¹⁷³ E. Reynolds,²¹ O. L. Rezanova,¹²⁰b,¹²⁰a P. Reznicek,¹³⁹ R. Richter,¹¹³

S. Richter,⁹² E. Richter-Was,⁸¹b O. Ricken,²⁴ M. Ridel,¹³² P. Rieck,¹¹³ C. J. Riegel,¹⁸⁰ O. Rifki,⁴⁴ M. Rijssenbeek,¹⁵²

A. Rimoldi,⁶⁸a,⁶⁸b M. Rimoldi,²⁰ L. Rinaldi,²³b G. Ripellino,¹⁵¹ B. Ristić,⁸⁷ E. Ritsch,³⁵ I. Riu,¹⁴ J. C. Rivera Vergara,¹⁴⁴a

F. Rizatdinova,¹²⁵ E. Rizvi,⁹⁰ C. Rizzi,¹⁴ R. T. Roberts,⁹⁸ S. H. Robertson,¹⁰¹,m A. Robichaud-Veronneau,¹⁰¹ D. Robinson,³¹

J. E. M. Robinson,⁴⁴ A. Robson,⁵⁵ E. Rocco,⁹⁷ C. Roda,⁶⁹a,⁶⁹b Y. Rodina,⁹⁹ S. Rodriguez Bosca,¹⁷² A. Rodriguez Perez,¹⁴

D. Rodriguez Rodriguez,¹⁷² A. M. Rodríguez Vera,¹⁶⁶b S. Roe,³⁵ C. S. Rogan,⁵⁷ O. Røhne,¹³⁰ R. Röhrig,¹¹³

C. P. A. Roland,⁶³ J. Roloff,⁵⁷ A. Romaniouk,¹¹⁰ M. Romano,²³b,²³a N. Rompotis,⁸⁸ M. Ronzani,¹²¹ L. Roos,¹³² S. Rosati,⁷⁰a

K. Rosbach,⁵⁰ P. Rose,¹⁴³ N-A. Rosien,⁵¹ E. Rossi,⁶⁷a,⁶⁷b L. P. Rossi,⁵³b L. Rossini,⁶⁶a,⁶⁶b J. H. N. Rosten,³¹ R. Rosten,¹⁴⁵

M. Rotaru,²⁷b J. Rothberg,¹⁴⁵ D. Rousseau,¹²⁸ D. Roy,³²c A. Rozanov,⁹⁹ Y. Rozen,¹⁵⁸ X. Ruan,³²c F. Rubbo,¹⁵⁰ F. Rühr,⁵⁰

A. Ruiz-Martinez,³³ Z. Rurikova,⁵⁰ N. A. Rusakovich,⁷⁷ H. L. Russell,¹⁰¹ J. P. Rutherford,⁷ N. Ruthmann,³⁵

E. M. Rüttinger,⁴⁴,mm Y. F. Ryabov,¹³⁴ M. Rybar,¹⁷¹ G. Rybkin,¹²⁸ S. Ryu,⁶ A. Ryzhov,¹⁴⁰ G. F. Rzehorz,⁵¹ P. Sabatini,⁵¹

G. Sabato,¹¹⁸ S. Sacerdoti,¹²⁸ H. F.-W. Sadrozinski,¹⁴³ R. Sadykov,⁷⁷ F. Safai Tehrani,⁷⁰a P. Saha,¹¹⁹ M. Sahinsoy,⁵⁹a

A. Sahu,¹⁸⁰ M. Saimpert,⁴⁴ M. Saito,¹⁶¹ T. Saito,¹⁶¹ H. Sakamoto,¹⁶¹ A. Sakharov,¹²¹,ee D. Salamani,⁵² G. Salamanna,⁷²a,⁷²b

J. E. Salazar Loyola,¹⁴⁴b D. Salek,¹¹⁸ P. H. Sales De Bruin,¹⁷⁰ D. Salihagic,¹¹³ A. Salnikov,¹⁵⁰ J. Salt,¹⁷² D. Salvatore,⁴⁰b,⁴⁰a

F. Salvatore,¹⁵³ A. Salvucci,⁶¹a,⁶¹b,⁶¹c A. Salzburger,³⁵ D. Sammel,⁵⁰ D. Sampsonidis,¹⁶⁰ D. Sampsonidou,¹⁶⁰ J. Sánchez,¹⁷²

A. Sanchez Pineda,⁶⁴a,⁶⁴c H. Sandaker,¹³⁰ C. O. Sander,⁴⁴ M. Sandhoff,¹⁸⁰ C. Sandoval,²² D. P. C. Sankey,¹⁴¹

M. Sannino,⁵³b,⁵³a Y. Sano,¹¹⁵ A. Sansoni,⁴⁹ C. Santoni,³⁷ H. Santos,¹³⁶a I. Santoyo Castillo,¹⁵³ A. Sapronov,⁷⁷

J. G. Saraiva,¹³⁶a,¹³⁶d O. Sasaki,⁷⁹ K. Sato,¹⁶⁷ E. Sauvan,⁵ P. Savard,¹⁶⁵,d N. Savic,¹¹³ R. Sawada,¹⁶¹ C. Sawyer,¹⁴¹

L. Sawyer,⁹³,u C. Sbarra,²³b A. Sbrizzi,²³b,²³a T. Scanlon,⁹² D. A. Scannicchio,¹⁶⁹ J. Schaarschmidt,¹⁴⁵ P. Schacht,¹¹³

B. M. Schachtner,¹¹² D. Schaefer,³⁶ L. Schaefer,¹³³ J. Schaeffer,⁹⁷ S. Schaepe,³⁵ U. Schäfer,⁹⁷ A. C. Schaffer,¹²⁸
D. Schaile,¹¹² R. D. Schamberger,¹⁵² N. Scharnberg,⁹⁸ V. A. Schegelsky,¹³⁴ D. Scheirich,¹³⁹ F. Schenck,¹⁹ M. Schernau,¹⁶⁹

C. Schiavi,⁵³b,⁵³a S. Schier,¹⁴³ L. K. Schildgen,²⁴ Z. M. Schillaci,²⁶ E. J. Schioppa,³⁵ M. Schioppa,⁴⁰b,⁴⁰a K. E. Schleicher,⁵⁰

S. Schlenker,³⁵ K. R. Schmidt-Sommerfeld,¹¹³ K. Schmieden,³⁵ C. Schmitt,⁹⁷ S. Schmitt,⁴⁴ S. Schmitz,⁹⁷ U. Schnoor,⁵⁰

L. Schoeffel,¹⁴² A. Schoening,⁵⁹b E. Schopf,²⁴ M. Schott,⁹⁷ J. F. P. Schouwenberg,¹¹⁷ J. Schovancova,³⁵ S. Schramm,⁵²

N. Schuh,⁹⁷ A. Schulte,⁹⁷ H-C. Schultz-Coulon,⁵⁹a M. Schumacher,⁵⁰ B. A. Schumm,¹⁴³ Ph. Schune,¹⁴² A. Schwartzman,¹⁵⁰

T. A. Schwarz,¹⁰³ H. Schweiger,⁹⁸ Ph. Schwemling,¹⁴² R. Schwienhorst,¹⁰⁴ A. Sciandra,²⁴ G. Sciolla,²⁶

M. Scornajenghi,⁴⁰b,⁴⁰a F. Scuri,⁶⁹a F. Scutti,¹⁰² L. M. Scyboz,¹¹³ J. Searcy,¹⁰³ C. D. Sebastiani,⁷⁰a,⁷⁰b P. Seema,²⁴

S. C. Seidel,¹¹⁶ A. Seiden,¹⁴³ T. Seiss,³⁶ J. M. Seixas,⁷⁸b G. Sekhniaidze,⁶⁷a K. Sekhon,¹⁰³ S. J. Sekula,⁴¹

N. Semprini-Cesari,²³b,²³a S. Sen,⁴⁷ S. Senkin,³⁷ C. Serfon,¹³⁰ L. Serin,¹²⁸ L. Serkin,⁶⁴a,⁶⁴b M. Sessa,⁷²a,⁷²b H. Severini,¹²⁴

F. Sforza,¹⁶⁸ A. Sfyrla,⁵² E. Shabalina,⁵¹ J. D. Shahinian,¹⁴³ N. W. Shaikh,⁴³a,⁴³b L. Y. Shan,¹⁵a R. Shang,¹⁷¹ J. T. Shank,²⁵

M. Shapiro,¹⁸ A. S. Sharma,¹ A. Sharma,¹³¹ P. B. Shatalov,¹⁰⁹ K. Shaw,⁶⁴a,⁶⁴b S. M. Shaw,⁹⁸ A. Shcherbakova,¹³⁴

C. Y. Shehu,¹⁵³ Y. Shen,¹²⁴ N. Sherafati,³³ A. D. Sherman,²⁵ P. Sherwood,⁹² L. Shi,¹⁵⁵,nn S. Shimizu,⁸⁰ C. O. Shimmin,¹⁸¹

M. Shimojima,¹¹⁴ I. P. J. Shipsey,¹³¹ S. Shirabe,⁸⁵ M. Shiyakova,⁷⁷ J. Shlomi,¹⁷⁸ A. Shmeleva,¹⁰⁸ D. Shoaleh Saadi,¹⁰⁷

M. J. Shochet,³⁶ S. Shojaii,¹⁰² D. R. Shope,¹²⁴ S. Shrestha,¹²² E. Shulga,¹¹⁰ P. Sicho,¹³⁷ A. M. Sickles,¹⁷¹ P. E. Sidebo,¹⁵¹

E. Sideras Haddad,³²c O. Sidiropoulou,¹⁷⁵ A. Sidoti,²³b,²³a F. Siegert,⁴⁶ Dj. Sijacki,¹⁶ J. Silva,¹³⁶a M. Silva Jr.,¹⁷⁹

S. B. Silverstein,⁴³a L. Simic,⁷⁷ S. Simion,¹²⁸ E. Simioni,⁹⁷ M. Simon,⁹⁷ P. Sinervo,¹⁶⁵ N. B. Sinev,¹²⁷ M. Sioli,²³b,²³a

G. Siragusa,¹⁷⁵ I. Siral,¹⁰³ S. Yu. Sivoklokov,¹¹¹ J. Sjölin,⁴³a,⁴³b M. B. Skinner,⁸⁷ P. Skubic,¹²⁴ M. Slater,²¹ T. Slavicek,¹³⁸

M. Slawinska,⁸² K. Sliwa,¹⁶⁸ R. Slovak,¹³⁹ V. Smakhtin,¹⁷⁸ B. H. Smart,⁵ J. Smiesko,²⁸a N. Smirnov,¹¹⁰ S. Yu. Smirnov,¹¹⁰

Y. Smirnov,¹¹⁰ L. N. Smirnova,¹¹¹ O. Smirnova,⁹⁴ J. W. Smith,⁵¹ M. N. K. Smith,³⁸ R. W. Smith,³⁸ M. Smizanska,⁸⁷

K. Smolek,¹³⁸ A. A. Snesarev,¹⁰⁸ I. M. Snyder,¹²⁷ S. Snyder,²⁹ R. Sobie,¹⁷⁴,m A. M. Soffa,¹⁶⁹ A. Soffer,¹⁵⁹ A. Søgaard,⁴⁸

D. A. Soh,¹⁵⁵ G. Sokhrannyi,⁸⁹ C. A. Solans Sanchez,³⁵ M. Solar,¹³⁸ E. Yu. Soldatov,¹¹⁰ U. Soldevila,¹⁷² A. A. Solodkov,¹⁴⁰

A. Soloshenko,⁷⁷ O. V. Solovyanov,¹⁴⁰ V. Solovyev,¹³⁴ P. Sommer,¹⁴⁶ H. Son,¹⁶⁸ W. Song,¹⁴¹ A. Sopczak,¹³⁸ F. Sopkova,²⁸b

D. Sosa,⁵⁹b C. L. Sotiropoulou,⁶⁹a,⁶⁹b S. Sottocornola,⁶⁸a,⁶⁸b R. Soualah,⁶⁴a,⁶⁴c,oo A. M. Soukharev,¹²⁰b,¹²⁰a D. South,⁴⁴

B. C. Sowden,⁹¹ S. Spagnolo,⁶⁵a,⁶⁵b M. Spalla,¹¹³ M. Spangenberg,¹⁷⁶ F. Spanò,⁹¹ D. Sperlich,¹⁹ F. Spettel,¹¹³

T. M. Spieker,⁵⁹a R. Spighi,²³b G. Spigo,³⁵ L. A. Spiller,¹⁰² M. Spousta,¹³⁹ A. Stabile,⁶⁶a,⁶⁶b R. Stamen,⁵⁹a S. Stamm,¹⁹

E. Stanecka,⁸² R. W. Stanek,⁶ C. Stanescu,⁷²a M. M. Stanitzki,⁴⁴ B. S. Stapf,¹¹⁸ S. Stapnes,¹³⁰ E. A. Starchenko,¹⁴⁰

G. H. Stark,³⁶ J. Stark,⁵⁶ S. H. Stark,³⁹ P. Staroba,¹³⁷ P. Starovoitov,⁵⁹a S. Stärz,³⁵ R. Staszewski,⁸² M. Stegler,⁴⁴

P. Steinberg,²⁹ B. Stelzer,¹⁴⁹ H. J. Stelzer,³⁵ O. Stelzer-Chilton,¹⁶⁶a H. Stenzel,⁵⁴ T. J. Stevenson,⁹⁰ G. A. Stewart,⁵⁵

M. C. Stockton,¹²⁷ G. Stoicea,²⁷b P. Stolte,⁵¹ S. Stonjek,¹¹³ A. Straessner,⁴⁶ J. Strandberg,¹⁵¹ S. Strandberg,⁴³a,⁴³b

M. Strauss,¹²⁴ P. Strizenec,²⁸b R. Ströhmer,¹⁷⁵ D. M. Strom,¹²⁷ R. Stroynowski,⁴¹ A. Strubig,⁴⁸ S. A. Stucci,²⁹ B. Stugu,¹⁷

J. Stupak,¹²⁴ N. A. Styles,⁴⁴ D. Su,¹⁵⁰ J. Su,¹³⁵ S. Suchek,⁵⁹a Y. Sugaya,¹²⁹ M. Suk,¹³⁸ V. V. Sulin,¹⁰⁸ D. M. S. Sultan,⁵²

S. Sultansoy,⁴c T. Sumida,⁸³ S. Sun,¹⁰³ X. Sun,³ K. Suruliz,¹⁵³ C. J. E. Suster,¹⁵⁴ M. R. Sutton,¹⁵³ S. Suzuki,⁷⁹ M. Svatos,¹³⁷

M. Swiatlowski,³⁶ S. P. Swift,² A. Sydorenko,⁹⁷ I. Sykora,²⁸a T. Sykora,¹³⁹ D. Ta,⁹⁷ K. Tackmann,⁴⁴,pp J. Taenzer,¹⁵⁹

A. Taffard,¹⁶⁹ R. Tafirout,¹⁶⁶a E. Tahirovic,⁹⁰ N. Taiblum,¹⁵⁹ H. Takai,²⁹ R. Takashima,⁸⁴ E. H. Takasugi,¹¹³ K. Takeda,⁸⁰

T. Takeshita,¹⁴⁷ Y. Takubo,⁷⁹ M. Talby,⁹⁹ A. A. Talyshev,¹²⁰b,¹²⁰a J. Tanaka,¹⁶¹ M. Tanaka,¹⁶³ R. Tanaka,¹²⁸ R. Tanioka,⁸⁰

B. B. Tannenwald,¹²² S. Tapia Araya,¹⁴⁴b S. Tapprogge,⁹⁷ A. Tarek Abouelfadl Mohamed,¹³² S. Tarem,¹⁵⁸ G. Tarna,²⁷b,p

G. F. Tartarelli,⁶⁶a P. Tas,¹³⁹ M. Tasevsky,¹³⁷ T. Tashiro,⁸³ E. Tassi,⁴⁰b,⁴⁰a A. Tavares Delgado,¹³⁶a,¹³⁶b Y. Tayalati,³⁴e

A. C. Taylor,¹¹⁶ A. J. Taylor,⁴⁸ G. N. Taylor,¹⁰² P. T. E. Taylor,¹⁰² W. Taylor,¹⁶⁶b A. S. Tee,⁸⁷ P. Teixeira-Dias,⁹¹ D. Temple,¹⁴⁹

H. Ten Kate,³⁵ P. K. Teng,¹⁵⁵ J. J. Teoh,¹²⁹ F. Tepel,¹⁸⁰ S. Terada,⁷⁹ K. Terashi,¹⁶¹ J. Terron,⁹⁶ S. Terzo,¹⁴ M. Testa,⁴⁹

R. J. Teuscher,¹⁶⁵,m S. J. Thais,¹⁸¹ T. Theveneaux-Pelzer,⁴⁴ F. Thiele,³⁹ J. P. Thomas,²¹ A. S. Thompson,⁵⁵ P. D. Thompson,²¹

L. A. Thomsen,¹⁸¹ E. Thomson,¹³³ Y. Tian,³⁸ R. E. Ticse Torres,⁵¹ V. O. Tikhomirov,¹⁰⁸,qq Yu. A. Tikhonov,¹²⁰b,¹²⁰a

S. Timoshenko,¹¹⁰ P. Tipton,¹⁸¹ S. Tisserant,⁹⁹ K. Todome,¹⁶³ S. Todorova-Nova,⁵ S. Todt,⁴⁶ J. Tojo,⁸⁵ S. Tokár,²⁸a

K. Tokushuku,⁷⁹ E. Tolley,¹²² M. Tomoto,¹¹⁵ L. Tompkins,¹⁵⁰ K. Toms,¹¹⁶ B. Tong,⁵⁷ P. Tornambe,⁵⁰ E. Torrence,¹²⁷

H. Torres,⁴⁶ E. Torró Pastor,¹⁴⁵ C. Tosciri,¹³¹ J. Toth,⁹⁹,rr F. Touchard,⁹⁹ D. R. Tovey,¹⁴⁶ C. J. Treado,¹²¹ T. Trefzger,¹⁷⁵

F. Tresoldi,¹⁵³ A. Tricoli,²⁹ I. M. Trigger,¹⁶⁶a S. Trincaz-Duvoid,¹³² M. F. Tripiana,¹⁴ W. Trischuk,¹⁶⁵ B. Trocmé,⁵⁶

A. Trofymov,¹²⁸ C. Troncon,⁶⁶a M. Trovatelli,¹⁷⁴ F. Trovato,¹⁵³ L. Truong,³²b M. Trzebinski,⁸² A. Trzupek,⁸² F. Tsai,⁴⁴

J. C.-L. Tseng,¹³¹ P. V. Tsiareshka,¹⁵⁰ N. Tsirintanis,⁹ V. Tsiskaridze,¹⁵² E. G. Tskhadadze,¹⁵⁷a I. I. Tsukerman,¹⁰⁹

V. Tsulaia,¹⁸ S. Tsuno,⁷⁹ D. Tsybychev,¹⁵² Y. Tu,⁶¹b A. Tudorache,²⁷b V. Tudorache,²⁷b T. T. Tulbure,²⁷a A. N. Tuna,⁵⁷

S. Turchikhin,⁷⁷ D. Turgeman,¹⁷⁸ I. Turk Cakir,⁴b,ss R. Turra,⁶⁶a P. M. Tuts,³⁸ E. Tzovara,⁹⁷ G. Ucchielli,²³b,²³a I. Ueda,⁷⁹
M. Ughetto,43a,43b F. Ukegawa,167 G. Unal,35 A. Undrus,29 G. Unel,169 F. C. Ungaro,102 Y. Unno,79 K. Uno,161 J. Urban,28b

P. Urquijo,102 P. Urrejola,97 G. Usai,8 J. Usui,79 L. Vacavant,99 V. Vacek,138 B. Vachon,101 K. O. H. Vadla,130 A. Vaidya,92

C. Valderanis,112 E. Valdes Santurio,43a,43b M. Valente,52 S. Valentinetti,23b,23a A. Valero,172 L. Valéry,44 R. A. Vallance,21

A. Vallier,5 J. A. Valls Ferrer,172 T. R. Van Daalen,14 W. Van Den Wollenberg,118 H. Van der Graaf,118 P. Van Gemmeren,6
J. Van Nieuwkoop,149 I. Van Vulpen,118 M. C. van Woerden,118 M. Vanadia,71a,71b W. Vandelli,35 A. Vaniachine,164

P. Vankov,118 R. Vari,70a E. W. Varnes,7 C. Varni,53b,53a T. Varol,41 D. Varouchas,128 A. Vartapetian,8 K. E. Varvell,154

G. A. Vasquez,144b J. G. Vasquez,181 F. Vazeille,37 D. Vazquez Furelos,14 T. Vazquez Schroeder,101 J. Veatch,51

V. Vecchio,72a,72b L. M. Veloce,165 F. Veloso,136a,136c S. Veneziano,70a A. Ventura,65a,65b M. Venturi,174 N. Venturi,35

V. Vercesi,68a M. Verducci,72a,72b W. Verkerke,118 A. T. Vermeulen,118 J. C. Vermeulen,118 M. C. Vetterli,149,d

N. Viaux Maira,144b O. Viazlo,94 I. Vichou,171.a T. Vickey,146 O. E. Vickey Boeriu,146 G. H. A. Viehhauser,131 S. Viel,18

L. Vigani,131 M. Villa,23b,23a M. Villaplana Perez,66a,66b E. Vilucchi,49 M. G. Vincter,33 V. B. Vinogradov,77

A. Vishwakarma,44 C. Vittori,23b,23a I. Vivarelli,153 S. Vlachos,10 M. Vogel,180 P. Vokac,138 G. Volpi,14

S. E. Von Buddenbrock,32c E. Von Toerne,24 V. Vorobel,139 K. Vorobev,110 M. Vos,172 J. H. Vossebeld,88 N. Vranjes,16

M. Vranjes Milosavljevic,16 V. Vrba,138 M. Vreeswijk,118 T. Šfiligoj,89 R. Vuillermet,35 I. Vukotic,36 T. Ženiš,28a

L. Živković,16 P. Wagner,24 W. Wagner,180 J. Wagner-Kuhr,112 H. Wahlberg,86 S. Wahrmund,46 K. Wakamiya,80 J. Walder,87

R. Walker,112 W. Walkowiak,148 V. Wallangen,43a,43b A. M. Wang,57 C. Wang,58b,p F. Wang,179 H. Wang,18 H. Wang,3

J. Wang,154 J. Wang,59b P. Wang,41 Q. Wang,124 R.-J. Wang,132 R. Wang,58a R. Wang,6 S. M. Wang,155 W. Wang,155,tt

W. X. Wang,58a,uu Y. Wang,58a Z. Wang,58c C. Wanotayaroj,44 A. Warburton,101 C. P. Ward,31 D. R. Wardrope,92

A. Washbrook,48 P. M. Watkins,21 A. T. Watson,21 M. F. Watson,21 G. Watts,145 S. Watts,98 B. M. Waugh,92 A. F. Webb,11

S. Webb,97 C. Weber,181 M. S. Weber,20 S. A. Weber,33 S. M. Weber,59a J. S. Webster,6 A. R. Weidberg,131 B. Weinert,63

J. Weingarten,51 M. Weirich,97 C. Weiser,50 P. S. Wells,35 T. Wenaus,29 T. Wengler,35 S. Wenig,35 N. Wermes,24

M. D. Werner,76 P. Werner,35 M. Wessels,59a T. D. Weston,20 K. Whalen,127 N. L. Whallon,145 A. M. Wharton,87

A. S. White,103 A. White,8 M. J. White,1 R. White,144b D. Whiteson,169 B. W. Whitmore,87 F. J. Wickens,141

W. Wiedenmann,179 M. Wielers,141 C. Wiglesworth,39 L. A. M. Wiik-Fuchs,50 A. Wildauer,113 F. Wilk,98 H. G. Wilkens,35

H. H. Williams,133 S. Williams,31 C. Willis,104 S. Willocq,100 J. A. Wilson,21 I. Wingerter-Seez,5 E. Winkels,153

F. Winklmeier,127 O. J. Winston,153 B. T. Winter,24 M. Wittgen,150 M. Wobisch,93 A. Wolf,97 T. M. H. Wolf,118 R. Wolff,99

M. W. Wolter,82 H. Wolters,136a,136c V. W. S. Wong,173 N. L. Woods,143 S. D. Worm,21 B. K. Wosiek,82 K. W. Woźniak,82

K. Wraight,55 M. Wu,36 S. L. Wu,179 X. Wu,52 Y. Wu,58a T. R. Wyatt,98 B. M. Wynne,48 S. Xella,39 Z. Xi,103 L. Xia,176

D. Xu,15a H. Xu,58a L. Xu,29 T. Xu,142 W. Xu,103 B. Yabsley,154 S. Yacoob,32a K. Yajima,129 D. P. Yallup,92 D. Yamaguchi,163

Y. Yamaguchi,163 A. Yamamoto,79 T. Yamanaka,161 F. Yamane,80 M. Yamatani,161 T. Yamazaki,161 Y. Yamazaki,80 Z. Yan,25
H. J. Yang,58c,58d H. T. Yang,18 S. Yang,75 Y. Yang,161 Y. Yang,155 Z. Yang,17 W-M. Yao,18 Y. C. Yap,44 Y. Yasu,79

E. Yatsenko,5 J. Ye,41 S. Ye,29 I. Yeletskikh,77 E. Yigitbasi,25 E. Yildirim,97 K. Yorita,177 K. Yoshihara,133 C. J. S. Young,35

C. Young,150 J. Yu,8 J. Yu,76 X. Yue,59a S. P. Y. Yuen,24 I. Yusuff,31,vv B. Zabinski,82 G. Zacharis,10 E. Zaffaroni,52

R. Zaidan,14 A. M. Zaitsev,140,ii N. Zakharchuk,44 J. Zalieckas,17 S. Zambito,57 D. Zanzi,35 D. R. Zaripovas,55 C. Zeitnitz,180

G. Zemaityte,131 J. C. Zeng,171 Q. Zeng,150 O. Zenin,140 D. Zerwas,128 M. Zgubič,131 D. F. Zhang,58b D. Zhang,103

F. Zhang,179 G. Zhang,58a,uu H. Zhang,15c J. Zhang,6 L. Zhang,50 L. Zhang,58a M. Zhang,171 P. Zhang,15c R. Zhang,58a,p

R. Zhang,24 X. Zhang,58b Y. Zhang,15d Z. Zhang,128 X. Zhao,41 Y. Zhao,58b,128,x Z. Zhao,58a A. Zhemchugov,77 B. Zhou,103

C. Zhou,179 L. Zhou,41 M. S. Zhou,15d M. Zhou,152 N. Zhou,58c Y. Zhou,7 C. G. Zhu,58b H. L. Zhu,58a H. Zhu,15a J. Zhu,103

Y. Zhu,58a X. Zhuang,15a K. Zhukov,108 V. Zhulanov,120b,120a A. Zibell,175 D. Zieminska,63 N. I. Zimine,77 S. Zimmermann,50

Z. Zinonos,113 M. Zinser,97 M. Ziolkowski,148 G. Zobernig,179 A. Zoccoli,23b,23a K. Zoch,51 T. G. Zorbas,146 R. Zou,36

M. Zur Nedden,19 and L. Zwalinski35

(ATLAS Collaboration)

<footnote n="1">¹Department of Physics, University of Adelaide, Adelaide, Australia</footnote>

<footnote n="2">²Physics Department, SUNY Albany, Albany, New York, USA</footnote>

<footnote n="3">³Department of Physics, University of Alberta, Edmonton, Alberta, Canada</footnote>

<footnote n="44">⁴⁴Department of Physics, Ankara University, Ankara, Turkey</footnote>

<footnote n="4">⁴ᵇIstanbul Aydin University, Istanbul, Turkey</footnote>
⁴ᶜDivision of Physics, TOBB University of Economics and Technology, Ankara, Turkey

⁵LAPP, Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, Annecy, France

⁶High Energy Physics Division, Argonne National Laboratory, Argonne, Illinois, USA

⁷Department of Physics, University of Arizona, Tucson, Arizona, USA

⁸Department of Physics, University of Texas at Arlington, Arlington, Texas, USA

⁹Physics Department, National and Kapodistrian University of Athens, Athens, Greece

¹⁰Physics Department, National Technical University of Athens, Zografou, Greece

¹¹Department of Physics, University of Texas at Austin, Austin, Texas, USA

¹²ªBahcesehir University, Faculty of Engineering and Natural Sciences, Istanbul, Turkey

¹²ᵇIstanbul Bilgi University, Faculty of Engineering and Natural Sciences, Istanbul, Turkey

¹²ᶜDepartment of Physics, Bogazici University, Istanbul, Turkey

¹²ᵈDepartment of Physics Engineering, Gaziantep University, Gaziantep, Turkey

¹³ªInstitute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan

¹⁴Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, Barcelona, Spain

¹⁵ªInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, China

¹⁵ᵇPhysics Department, Tsinghua University, Beijing, China

¹⁵ᶜDepartment of Physics, Nanjing University, Nanjing, China

¹⁵ᵈUniversity of Chinese Academy of Science (UCAS), Beijing, China

¹⁶ªInstitute of Physics, University of Belgrade, Belgrade, Serbia

¹⁷Department for Physics and Technology, University of Bergen, Bergen, Norway

¹⁸Physics Division, Lawrence Berkeley National Laboratory and University of California, Berkeley, California, USA

¹⁹ªInstitut für Physik, Humboldt Universität zu Berlin, Berlin, Germany

²⁰Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University of Bern, Bern, Switzerland

²¹School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom

²²Centro de Investigaciónes, Universidad Antonio Nariño, Bogota, Colombia

²³ªDipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy

²³ᵇINFN Sezione di Bologna, Italy

²⁴Physikalisches Institut, Universität Bonn, Bonn, Germany

²⁵Department of Physics, Boston University, Boston, Massachusetts, USA

²⁶Department of Physics, Brandeis University, Waltham, Massachusetts, USA

²⁷ªTransilvania University of Brasov, Brasov, Romania

²⁷ᵇHoria Hulubei National Institute of Physics and Nuclear Engineering, Bucharest, Romania

²⁷ᶜDepartment of Physics, Alexandru Ioan Cuza University of Iasi, Iasi, Romania

²⁷ᵈNational Institute for Research and Development of Isotopic and Molecular Technologies, Physics Department, Cluj-Napoca, Romania

²⁷ᵉUniversity Politehnică Bucharest, Bucharest, Romania

²⁷ᵉWest University in Timisoara, Timisoara, Romania

²⁸ªFaculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovak Republic

²⁸ᵇDepartment of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic

²⁹Physics Department, Brookhaven National Laboratory, Upton, New York, USA

³⁰Departamento de Física, Universidad de Buenos Aires, Buenos Aires, Argentina

³¹Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom

³²ªDepartment of Physics, University of Cape Town, Cape Town, South Africa

³²ᵇDepartment of Mechanical Engineering Science, University of Johannesburg, Johannesburg, South Africa

³²ᶜSchool of Physics, University of the Witwatersrand, Johannesburg, South Africa

³³Department of Physics, Carleton University, Ottawa, Ontario, Canada

³⁴ªFaculté des Sciences Ain Chock, Réseau Universitaire de Physique des Hautes Energies-Université Hassan II, Casablanca, Morocco

³⁴ᵇCentre National de l'Energie des Sciences Techniques Nucleaires (CNESTEN), Rabat, Morocco

³⁴ᶜFaculté des Sciences Semlalia, Université Cadi Ayyad, LPHEA-Marrakech, Morocco

³⁴ᵈFaculté des Sciences, Université Mohamed Premier and LPTPM, Oujda, Morocco

³⁴ᵉFaculté des sciences, Université Mohammed V, Rabat, Morocco

³⁵CERN, Geneva, Switzerland

³⁶Enrico Fermi Institute, University of Chicago, Chicago, Illinois, USA

³⁷LPC, Université Clermont Auvergne, CNRS/IN2P3, Clermont-Ferrand, France

³⁸Névis Laboratory, Columbia University, Irvington, New York, USA

³⁹Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark

⁴⁰ªDipartimento di Fisica, Università della Calabria, Rende, Italy
⁴⁰ᵇINFN Gruppo Collegato di Cosenza, Laboratori Nazionali di Frascati, Italy

⁴¹Physics Department, Southern Methodist University, Dallas, Texas, USA

⁴²Physics Department, University of Texas at Dallas, Richardson, Texas, USA

⁴³ᵃDepartment of Physics, Stockholm University, Sweden

⁴³ᵇOskar Klein Centre, Stockholm, Sweden

⁴⁴Deutsches Elektronen-Synchrotron DESY, Hamburg and Zeuthen, Germany

⁴⁵Lehrstuhl für Experimentelle Physik IV, Technische Universität Dortmund, Dortmund, Germany

⁴⁶Institut für Kern- und Teilchenphysik, Technische Universität Dresden, Dresden, Germany

⁴⁷Department of Physics, Duke University, Durham, North Carolina, USA

⁴⁸SUPA - School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom

⁴⁹INFN e Laboratori Nazionali di Frascati, Frascati, Italy

⁵⁰Physikalisches Institut, Albert-Ludwigs-Universität Freiburg, Freiburg, Germany

⁵¹II. Physikalisches Institut, Georg-August-Universität Göttingen, Göttingen, Germany

⁵²Département de Physique Nucléaire et Corpusculaire, Université de Genève, Genève, Switzerland

⁵³ᵃDipartimento di Fisica, Università di Genova, Genova, Italy

⁵³ᵇINFN Sezione di Genova, Italy

⁵⁴II. Physikalisches Institut, Justus-Liebig-Universität Giessen, Giessen, Germany

⁵⁵SUPA - School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom

⁵⁶LPSC, Université Grenoble Alpes, CNRS/IN2P3, Grenoble INP, Grenoble, France

⁵⁷Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge, Massachusetts, USA

⁵⁸ᵃDepartment of Modern Physics and State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei, China

⁵⁸ᵇInstitute of Frontier and Interdisciplinary Science and Key Laboratory of Particle Physics and Particle Irradiation (MOE), Shandong University, Qingdao, China

⁵⁸ᶜSchool of Physics and Astronomy, Shanghai Jiao Tong University, KLPPAC-MoE, SKLPPC, Shanghai, China

⁵⁸ᵈTsung-Dao Lee Institute, Shanghai, China

⁵⁹ᵃKirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany

⁵⁹ᵇPhysikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany

⁶⁰Faculty of Applied Information Science, Hiroshima Institute of Technology, Hiroshima, Japan

⁶¹ᵃDepartment of Physics, Chinese University of Hong Kong, Shatin, N.T., Hong Kong, China

⁶¹ᵇDepartment of Physics, University of Hong Kong, Hong Kong, China

⁶¹ᶜDepartment of Physics and Institute for Advanced Study, Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong, China

⁶²Department of Physics, National Tsing Hua University, Hsinchu, Taiwan

⁶³Department of Physics, Indiana University, Bloomington, Indiana, USA

⁶⁴ᵃINFN Gruppo Collegato di Udine, Sezione di Trieste, Udine, Italy

⁶⁴ᵇICTP, Trieste, Italy

⁶⁴ᶜDipartimento di Chimica, Fisica e Ambiente, Università di Udine, Udine, Italy

⁶⁵ᵃINFN Sezione di Lecce, Italy

⁶⁵ᵇDipartimento di Matematica e Fisica, Università del Salento, Lecce, Italy

⁶⁶ᵃINFN Sezione di Milano, Italy

⁶⁶ᵇDipartimento di Fisica, Università di Milano, Milano, Italy

⁶⁷ᵃINFN Sezione di Napoli, Italy

⁶⁷ᵇDipartimento di Fisica, Università di Napoli, Napoli, Italy

⁶⁸ᵃINFN Sezione di Pavia, Italy

⁶⁸ᵇDipartimento di Fisica, Università di Pavia, Pavia, Italy

⁶⁹ᵃINFN Sezione di Pisa, Italy

⁶⁹ᵇDipartimento di Fisica E. Fermi, Università di Pisa, Pisa, Italy

⁷⁰ᵃINFN Sezione di Roma, Italy

⁷⁰ᵇDipartimento di Fisica, Sapienza Università di Roma, Roma, Italy

⁷¹ᵃINFN Sezione di Roma Tor Vergata, Italy

⁷¹ᵇDipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy

⁷²ᵃINFN Sezione di Roma Tre, Italy

⁷²ᵇDipartimento di Matematica e Fisica, Università Roma Tre, Roma, Italy

⁷³ᵃINFN-TIFPA, Italy

⁷³ᵇUniversità degli Studi di Trento, Trento, Italy

⁷⁴Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität, Innsbruck, Austria

⁷⁵University of Iowa, Iowa, City Iowa, USA

⁷⁶Department of Physics and Astronomy, Iowa State University, Ames, Iowa, USA

⁷⁷Joint Institute for Nuclear Research, Dubna, Russia
78aDepartamento de Engenharia Elétrica, Universidade Federal de Juiz de Fora (UFJF), Juiz de Fora, Brazil

78bUniversidade Federal do Rio De Janeiro COPPE/EE/IF, Rio de Janeiro, Brazil

78cUniversidade Federal de São João del Rei (UFSJ), São João del Rei, Brazil

78dInstituto de Física, Universidade de São Paulo, São Paulo, Brazil

79KEK, High Energy Accelerator Research Organization, Tsukuba, Japan

80Graduate School of Science, Kobe University, Kobe, Japan

81aAGH University of Science and Technology, Faculty of Physics and Applied Computer Science, Krakow, Poland

81bMarian Smoluchowski Institute of Physics, Jagiellonian University, Krakow, Poland

82Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland

83Faculty of Science, Kyoto University, Kyoto, Japan

84Kyoto University of Education, Kyoto, Japan

85Research Center for Advanced Particle Physics and Department of Physics, Kyushu University, Fukuoka, Japan

86Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina

87Physics Department, Lancaster University, Lancaster, United Kingdom

88Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom

89Department of Experimental Particle Physics, Jožef Stefan Institute and Department of Physics, University of Ljubljana, Ljubljana, Slovenia

90School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom

91Department of Physics, Royal Holloway University of London, Egham, United Kingdom

92Department of Physics and Astronomy, University College London, London, United Kingdom

93Louisiana Tech University, Ruston, Louisiana, USA

94Fysiska institutionen, Lunds universitet, Lund, Sweden

95Centre de Calcul de l'Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Villeurbanne, France

96Departamento de Física Teorica C-15 and CIAFF, Universidad Autónoma de Madrid, Madrid, Spain

97Institut für Physik, Universität Mainz, Mainz, Germany

98School of Physics and Astronomy, University of Manchester, Manchester, United Kingdom

99CPPM, Aix-Marseille Université, CNRS/IN2P3, Marseille, France

100Department of Physics, University of Massachusetts, Amherst, Massachusetts, USA

101Department of Physics, McGill University, Montreal, Quebec, Canada

102School of Physics, University of Melbourne, Victoria, Australia

103Department of Physics, University of Michigan, Ann Arbor, Michigan, USA

104Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA

105B.I. Stepanov Institute of Physics, National Academy of Sciences of Belarus, Minsk, Belarus

106Research Institute for Nuclear Problems of Byelorussian State University, Minsk, Belarus

107Group of Particle Physics, University of Montreal, Montreal, Quebec, Canada

108P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russia

109Institute for Theoretical and Experimental Physics (ITEP), Moscow, Russia

110National Research Nuclear University MEPhI, Moscow, Russia

111D.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University, Moscow, Russia

112Fakultät für Physik, Ludwig-Maximilians-Universität München, München, Germany

113Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), München, Germany

114Nagasaki Institute of Applied Science, Nagasaki, Japan

115Graduate School of Science and Kobayashi-Maskawa Institute, Nagoya University, Nagoya, Japan

116Department of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico, USA

117Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen/Nikhef, Nijmegen, Netherlands

118Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, Netherlands

119Department of Physics, Northern Illinois University, DeKalb, Illinois, USA

120aBudker Institute of Nuclear Physics, SB RAS, Novosibirsk, Russia

120bNovosibirsk State University Novosibirsk, Russia

121Department of Physics, New York University, New York, New York, USA

122Ohio State University, Columbus, Ohio, USA

123Faculty of Science, Okayama University, Okayama, Japan

124Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, Oklahoma, USA

125Department of Physics, Oklahoma State University, Stillwater, Oklahoma, USA

126Palacký University, RCPTM, Joint Laboratory of Optics, Olomouc, Czech Republic

127Center for High Energy Physics, University of Oregon, Eugene, Oregon, USA

128LAL, Université Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, Orsay, France

129Graduate School of Science, Osaka University, Osaka, Japan
¹³⁰Department of Physics, University of Oslo, Oslo, Norway

¹³¹Department of Physics, Oxford University, Oxford, United Kingdom

¹³²LPNHE, Sorbonne Université, Paris Diderot Sorbonne Paris Cité, CNRS/IN2P3, Paris, France

¹³³Department of Physics, University of Pennsylvania, Philadelphia, Pennsylvania, USA

¹³⁴Konstantinov Nuclear Physics Institute of National Research Centre “Kurchatov Institute”,
PNPI, St. Petersburg, Russia

¹³⁵Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania, USA

¹³⁶ªLaboratório de Instrumentação e Física Experimental de Partículas - LIP, Portugal

¹³⁶ᵇDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Lisboa, Portugal

¹³⁶ᶜDepartamento de Física, Universidade de Coimbra, Coimbra, Portugal

¹³⁶ᵈCentro de Física Nuclear da Universidade de Lisboa, Lisboa, Portugal

¹³⁶ᵉDepartamento de Física, Universidade do Minho, Braga, Portugal

¹³⁶fDepartamento de Física Teórica y del Cosmos, Universidad de Granada, Granada (Spain), Spain

¹³⁶gDep Física and CEFITEC de Faculdade de Ciências e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal

¹³⁷Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic

¹³⁸Czech Technical University in Prague, Prague, Czech Republic

¹³⁹Charles University, Faculty of Mathematics and Physics, Prague, Czech Republic

¹⁴⁰State Research Center Institute for High Energy Physics, NRC KI, Protvino, Russia

¹⁴¹Particle Physics Department, Rutherford Appleton Laboratory, Didcot, United Kingdom

¹⁴²IRFU, CEA, Université Paris-Saclay, Gif-sur-Yvette, France

¹⁴³Santa Cruz Institute for Particle Physics, University of California Santa Cruz, Santa Cruz, California, USA

¹⁴⁴ªDepartamento de Física, Pontificia Universidad Católica de Chile, Santiago, Chile

¹⁴⁴ᵇDepartamento de Física, Universidad Técnica Federico Santa María, Valparaíso, Chile

¹⁴⁵Department of Physics, University of Washington, Seattle, Washington, USA

¹⁴⁶Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom

¹⁴⁷Department of Physics, Shinshu University, Nagano, Japan

¹⁴⁸Department Physik, Universität Siegen, Siegen, Germany

¹⁴⁹Department of Physics, Simon Fraser University, Burnaby British Columbia, Canada

¹⁵⁰SLAC National Accelerator Laboratory, Stanford, California, USA

¹⁵¹Physics Department, Royal Institute of Technology, Stockholm, Sweden

¹⁵²Departments of Physics and Astronomy, Stony Brook University, Stony Brook, New York, USA

¹⁵³Department of Physics and Astronomy, University of Sussex, Brighton, United Kingdom

¹⁵⁴School of Physics, University of Sydney, Sydney, Australia

¹⁵⁵Institute of Physics, Academia Sinica, Taipei, Taiwan

¹⁵⁶Academia Sinica Grid Computing, Institute of Physics, Academia Sinica, Taipei, Taiwan

¹⁵⁷ªE. Andronikashvili Institute of Physics, Iv. Javakhishvili Tbilisi State University, Tbilisi, Georgia

¹⁵⁷ᵇHigh Energy Physics Institute, Tbilisi State University, Tbilisi, Georgia

¹⁵⁸Department of Physics, Technion, Israel Institute of Technology, Haifa, Israel

¹⁵⁹Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel

¹⁶⁰Department of Physics, Aristotle University of Thessaloniki, Thessaloniki, Greece

¹⁶¹International Center for Elementary Particle Physics and Department of Physics, University of Tokyo, Tokyo, Japan

¹⁶²Graduate School of Science and Technology, Tokyo Metropolitan University, Tokyo, Japan

¹⁶³Department of Physics, Tokyo Institute of Technology, Tokyo, Japan

¹⁶⁴Tomsk State University, Tomsk, Russia

¹⁶⁵Department of Physics, University of Toronto, Toronto, Ontario, Canada

¹⁶⁶ªTRIUMF, Vancouver, British Columbia, Canada

¹⁶⁶ᵇDepartment of Physics and Astronomy, York University, Toronto, Ontario, Canada

¹⁶⁷Division of Physics and Tomonaga Center for the History of the Universe, Faculty of Pure and Applied Sciences,
University of Tsukuba, Tsukuba, Japan

¹⁶⁸Department of Physics and Astronomy, Tufts University, Medford, Massachusetts, USA

¹⁶⁹Department of Physics and Astronomy, University of California Irvine, Irvine, California, USA

¹⁷⁰Department of Physics and Astronomy, University of Uppsala, Uppsala, Sweden

¹⁷¹Department of Physics, University of Illinois, Urbana, Illinois, USA

¹⁷²Instituto de Física Corpuscular (IFIC), Centro Mixto Universidad de Valencia - CSIC, Valencia, Spain

¹⁷³Department of Physics, University of British Columbia, Vancouver, British Columbia, Canada

¹⁷⁴Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia, Canada

¹⁷⁵Fakultät für Physik und Astronomie, Julius-Maximilians-Universität Würzburg, Würzburg, Germany

¹⁷⁶Department of Physics, University of Warwick, Coventry, United Kingdom

¹⁷⁷Waseda University, Tokyo, Japan

¹⁷⁸Department of Particle Physics, Weizmann Institute of Science, Rehovot, Israel
<sup>179</sup>Department of Physics, University of Wisconsin, Madison, Wisconsin, USA

<sup>180</sup>Fakultät für Mathematik und Naturwissenschaften, Fachgruppe Physik, Bergische Universität Wuppertal,
Wuppertal, Germany

<sup>181</sup>Department of Physics, Yale University, New Haven, Connecticut, USA

<sup>182</sup>Yerevan Physics Institute, Yerevan, Armenia

<sup>a</sup>Deceased.

<sup>b</sup>Also at Department of Physics, King's College London, London, United Kingdom.

<sup>c</sup>Also at Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan.

<sup>d</sup>Also at TRIUMF, Vancouver, British Columbia, Canada.

<sup>e</sup>Also at Department of Physics and Astronomy, University of Louisville, Louisville, Kentucky, USA.

<sup>f</sup>Also at Department of Physics, California State University, Fresno, California, USA.

<sup>g</sup>Also at Department of Physics, University of Fribourg, Fribourg, Switzerland.

<sup>h</sup>Also at II. Physikalisches Institut, Georg-August-Universität Göttingen, Göttingen, Germany.

<sup>i</sup>Also at Departament de Fisica de la Universitat Autonoma de Barcelona, Barcelona, Spain.

<sup>j</sup>Also at Tomsk State University, Tomsk, and Moscow Institute of Physics and Technology State University, Dolgoprudny, Russia.

<sup>k</sup>Also at The Collaborative Innovation Center of Quantum Matter (CICQM), Beijing, China.

<sup>l</sup>Also at Universita di Napoli Parthenope, Napoli, Italy.

<sup>m</sup>Also at Institute of Particle Physics (IPP), Canada.

<sup>n</sup>Also at Dipartimento di Fisica E. Fermi, Università di Pisa, Pisa, Italy.

<sup>o</sup>Also at Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest, Romania.

<sup>p</sup>Also at CPPM, Aix-Marseille Université, CNRS/IN2P3, Marseille, France.

<sup>q</sup>Also at Department of Physics, St. Petersburg State Polytechnical University, St. Petersburg, Russia.

<sup>r</sup>Also at Borough of Manhattan Community College, City University of New York, New York, USA.

<sup>s</sup>Also at Department of Financial and Management Engineering, University of the Aegean, Chios, Greece.

<sup>t</sup>Also at Centre for High Performance Computing, CSIR Campus, Rosebank, Cape Town, South Africa.

<sup>u</sup>Also at Louisiana Tech University, Ruston, Louisiana, USA.

<sup>v</sup>Also at Institutocia Catalana de Recerca i Estudis Avancats, ICREA, Barcelona, Spain.

<sup>w</sup>Also at Department of Physics, University of Michigan, Ann Arbor, Michigan, USA.

<sup>x</sup>Also at LAL, Université Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, Orsay, France.

<sup>y</sup>Also at Graduate School of Science, Osaka University, Osaka, Japan.

<sup>z</sup>Also at Physikalisches Institut, Albert-Ludwigs-Universität Freiburg, Freiburg, Germany.

<sup>aa</sup>Also at Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen/Nikhef, Nijmegen, Netherlands.

<sup>bb</sup>Also at Near East University, Nicosia, North Cyprus, Mersin, Turkey.

<sup>cc</sup>Also at Institute of Theoretical Physics, Ilia State University, Tbilisi, Georgia.

<sup>dd</sup>Also at CERN, Geneva, Switzerland.

<sup>ee</sup>Also at Manhattan College, New York, New York, USA.

<sup>ff</sup>Also at Hellenic Open University, Patras, Greece.

<sup>gg</sup>Also at The City College of New York, New York, New York, USA.

<sup>hh</sup>Also at Departamento de Física Teorica y del Cosmos, Universidad de Granada, Granada (Spain), Spain.

<sup>i</sup>Also at Department of Physics, California State University, Sacramento, California, USA.

<sup>j</sup>Also at Moscow Institute of Physics and Technology State University, Dolgoprudny, Russia.

<sup>kk</sup>Also at Ochadai Academic Production, Ochanomizu University, Tokyo, Japan.

<sup>l</sup>Also at Département de Physique Nucléaire et Corpusculaire, Université de Genève, Genève, Switzerland.

<sup>mm</sup>Also at Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom.

<sup>nn</sup>Also at School of Physics, Sun Yat-sen University, Guangzhou, China.

<sup>oo</sup>Also at Department of Applied Physics and Astronomy, University of Sharjah, Sharjah, United Arab Emirates.

<sup>pp</sup>Also at Institut für Experimentalphysik, Universität Hamburg, Hamburg, Germany.

<sup>qq</sup>Also at National Research Nuclear University MEPhI, Moscow, Russia.

<sup>r</sup>Also at Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Budapest, Hungary.

<sup>ss</sup>Also at Giresun University, Faculty of Engineering, Giresun, Turkey.

<sup>t</sup>Also at Department of Physics, Nanjing University, Nanjing, China.

<sup>uu</sup>Also at Institute of Physics, Academia Sinica, Taipei, Taiwan.

<sup>vv</sup>Also at Department of Physics, University of Malaya, Kuala Lumpur, Malaysia.