# Search for a light charged Higgs boson in the decay channel $H^+ \to c\bar{s}$ in $t\bar{t}$ events using pp collisions at $\sqrt{s} = 7$ TeV with the ATLAS detector

G. Aad, L. Aperio Bella, B. Aubert, N. Berger, J. Colas, M. Delmastro, L. Di Ciaccio, T.K.O. Doan, S. Elles, C. Goy, et al.

► To cite this version:

G. Aad, L. Aperio Bella, B. Aubert, N. Berger, J. Colas, et al., Search for a light charged Higgs boson in the decay channel $H^+ \to c\bar{s}$ in $t\bar{t}$ events using pp collisions at $\sqrt{s} = 7$ TeV with the ATLAS detector. European Physical Journal C: Particles and Fields, 2013, 73, pp.2465. 10.1140/epjc/s10052-013-2465-z. in2p3-00789723

HAL Id: in2p3-00789723

https://hal.in2p3.fr/in2p3-00789723

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# Search for a light charged Higgs boson in the decay channel $H^+ \to c\bar{s}$ in $t\bar{t}$ events using pp collisions at $\sqrt{s} = 7$ TeV with the ATLAS detector

The ATLAS Collaboration

## Abstract

A search for a charged Higgs boson ($H^+$) in $t\bar{t}$ decays is presented, where one of the top quarks decays via $t \to H^+b$, followed by $H^+ \to$ two jets ($c\bar{s}$). The other top quark decays to $Wb$, where the $W$ boson then decays into a lepton ($e/\mu$) and a neutrino. The data were recorded in $pp$ collisions at $\sqrt{s} = 7$ TeV by the ATLAS detector at the LHC in 2011, and correspond to an integrated luminosity of 4.7 fb$^{-1}$. With no observation of a signal, 95% confidence level (CL) upper limits are set on the decay branching ratio of top quarks to charged Higgs bosons varying between 5% and 1% for $H^+$ masses between 90 GeV and 150 GeV, assuming $B(H^+ \to c\bar{s}) = 100\%$.
# Search for a light charged Higgs boson in the decay channel $H^+ \to c\bar{s}$ in $t\bar{t}$ events using pp collisions at $\sqrt{s} = 7$ TeV with the ATLAS detector

The ATLAS Collaboration

¹CERN, 1211 Geneva 23, Switzerland

February 14, 2013

**Abstract** A search for a charged Higgs boson ($H^+$) in $t\bar{t}$ decays is presented, where one of the top quarks decays via $t \to H^+b$, followed by $H^+ \to$ two jets ($c\bar{s}$). The other top quark decays to $Wb$, where the W boson then decays into a lepton ($e/\mu$) and a neutrino. The data were recorded in pp collisions at $\sqrt{s} = 7$ TeV by the ATLAS detector at the LHC in 2011, and correspond to an integrated luminosity of 4.7 fb$^{-1}$. With no observation of a signal, 95% confidence level (CL) upper limits are set on the decay branching ratio of top quarks to charged Higgs bosons varying between 5% and 1% for $H^+$ masses between 90 GeV and 150 GeV, assuming $\mathcal{B}(H^+ \to c\bar{s}) = 100\%$.

PACS 12.60.Fr, 14.65.Ha, 14.80.Da, 14.80.Fd

## 1 Introduction

In the Standard Model (SM), electroweak symmetry breaking (EWSB) occurs through a single complex scalar doublet field and results in a single physical state, the Higgs boson [1–3]. A particle with characteristics of the SM Higgs boson has been discovered by both ATLAS [4] and CMS [5]. Beyond the SM, many models have been proposed, extending the Higgs sector to explain EWSB. The newly discovered boson is compatible with many of these models so that discovering its true nature is crucial to understanding EWSB. Two Higgs-doublet models (2HDM) [6] are simple extensions of the SM with five observable Higgs bosons, of which two are charged ($H^+$ and $H^-$) and three are neutral ($h^0$, $H^0$ and $A^0$). The discovery of a charged Higgs boson would be a signal for new physics beyond the SM.

The Minimal Supersymmetric Standard Model (MSSM) [7] is an example of a 2HDM. At tree level, the MSSM Higgs sector is determined by two independent

parameters, which can be taken to be the mass $m_{H^+}$ and the ratio of the two Higgs doublet vacuum expectation values, parametrized by $\tan\beta$. In the MSSM, a light $H^+$ (defined as $m_{H^+} < m_t$) decays predominantly to $c\bar{s}$, $b\bar{b}W^+$, and $\tau^+\nu$, with the respective branching ratios depending on $\tan\beta$ and $m_{H^+}$. Charge conjugated processes are implied throughout this paper. For $\tan\beta < 1$, $c\bar{s}$ is an important decay mode with $\mathcal{B}(H^+ \to c\bar{s})$ near 70% [8, 9] for $m_{H^+} \simeq 110$ GeV, whereas for $\tan\beta > 3$, $H^+ \to \tau^+\nu$ dominates (90%). For higher $H^+$ masses at low $\tan\beta$, the decay mode $H^+ \to Wb\bar{b}$ can be dominant. A light MSSM charged Higgs boson is viable at a relatively low $\tan\beta \approx 6$ in certain MSSM benchmark scenarios [10] that take into account the discovery of a Higgs boson with a mass of 125 GeV at the LHC.

The LEP experiments placed lower limits on $m_{H^+}$ in any type-II 2HDM [11] varying between 75 GeV and 91 GeV [12–16] depending on the assumed decay branching ratios for the charged Higgs boson. At the Tevatron, searches for charged Higgs bosons have been extended to larger values of $m_{H^+}$. No evidence for a $H^+$ was found and upper limits were set on the branching ratio $\mathcal{B}(t \to H^+b)$ varying between 10% and 30% for a light $H^+$ under the assumption of $\mathcal{B}(H^+ \to c\bar{s}) = 100\%$ [17, 18]. The discovery of a Higgs boson at the LHC is a weak constraint on many 2HDMs, and is compatible with the existence of a light charged Higgs decaying to two jets, especially in type I 2HDMs [19, 20].

In this paper, a search for a charged Higgs boson produced in $t\bar{t}$ decays is presented, where one of the top quarks decays via $t \to H^+b$ with the charged Higgs boson subsequently decaying to two jets ($c\bar{s}$), where again a 100% branching fraction is assumed. The other top quark decays according to the SM via $\bar{t} \to W^-\bar{b}$ with the W boson decaying into a lepton ($e/\mu$) and the cor-
responding neutrino. The signal process therefore has
the same topology as SM $t\bar{t}$ decays in the lepton + jets
channel, where one W decays to two jets and the other
to a lepton and corresponding neutrino, but the invari-
ant mass of the two jets from the $H^+$ peaks at $m_{H^+}$.
The search is performed by comparing the dijet mass
spectrum in the data with the prediction from SM top-
quark decays and with the expectation of a top quark
having a non-zero branching ratio for decay to $H^+b$.

## 2 Detector description and event samples

The data used in the analysis were recorded by the ATLAS detector in proton–proton (pp) collisions at a centre-of-mass energy of $\sqrt{s} = 7$ TeV during the 2011 data-taking period of the Large Hadron Collider (LHC) [21]. Events were required to pass a high-transverse momentum ($p_T$) single-lepton ($e/\mu$) trigger, and to have been recorded when all detector systems critical to muon, electron, and jet identification were operational. The lepton triggers required in the different data taking periods had varying $p_T$ thresholds: 20–22 GeV for the electron trigger and 18 GeV for the muon trigger. The resulting dataset corresponds to an integrated luminosity of $4.7 \text{ fb}^{-1}$ [22, 23].

The ATLAS detector [24] consists of an inner tracking system immersed in a 2 T axial magnetic field provided by a thin solenoid; electromagnetic and hadronic calorimeters; and a muon spectrometer (MS) embedded in a toroidal magnet system. The inner detector tracking system (ID) comprises a silicon pixel detector closest to the beamline, a silicon microstrip detector, and a straw tube transition radiation tracker. The electromagnetic (EM) calorimeters are high-granularity liquid-argon sampling calorimeters with lead as the absorber material in the barrel and endcap regions, and copper in the forward region. The hadronic calorimetry uses two different detector technologies. The barrel calorimeter ($|\eta| < 1.7$)<fnref n="1" /> consists of scintillator tiles interleaved with steel absorber plates. The endcap ($1.5 < |\eta| < 3.2$) and forward ($3.1 < |\eta| < 4.9$) calorimeters both use liquid argon as the active material, and copper and tungsten respectively as the absorber. The MS consists of three large superconducting toroids each with eight coils, and a system of precision tracking and fast trigger chambers.

The largest background to the charged Higgs boson signal is the SM production and decay of $t\bar{t}$ pairs. Additional background contributions (referred to as non-$t\bar{t}$ backgrounds) arise from the production of a single top quark, of a W or Z boson with additional jets, of QCD multi-jets, and of dibosons.

Top-quark pair and single top-quark events (Wt-channel and s-channel) were generated using the MC@N-LO 4.01 [25–28] Monte Carlo (MC) generator coupled to HERWIG 6.520.2 [29] to provide the parton showering and hadronization using the AUET2-CT10 [30, 31] tune; JIMMY [32] was used to model the underlying event. Single top-quark events in the t-channel were generated using ACERMC 3.8 [33] coupled to PYTHIA 6.425 [34] with the AUET2-MRST2007LO** [30, 35] tune. W/Z+jet and diboson events were generated using the leading-order (LO) ALPGEN 2.13 [36] generator interfaced to HERWIG with the AUET2-CTEQ6L1 [30, 37] tune. The W/Z+jet simulated data include dedicated samples for heavy-flavour production ($b\bar{b}$, $c\bar{c}$ and $c$). Signal samples of $t\bar{t} \to H^+bW^-\bar{b}$ were generated using PYTHIA 6.425 for seven different $H^+$ masses from 90 GeV to 150 GeV.

The data are affected by the detector response to multiple *pp* interactions occurring in the same or neighbouring bunch crossings, known as pile-up. Minimum-bias interactions generated by PYTHIA 6.425 [34], which has been tuned to data [38], were overlaid on the simulated signal and background events. The events were weighted to reproduce the distribution of the number of interactions per bunch crossing observed in the data. A GEANT4 simulation [39, 40] is used to model the response of the ATLAS detector, and the samples are reconstructed and analysed in the same way as the data.

## 3 Physics objects and event selection

Jets are reconstructed from topological clusters of calorimeter cells [41] using the anti-$k_t$ algorithm [42, 43] with a radius parameter $R = 0.4$. Topological clusters are built using an algorithm that suppresses detector noise. Jets are corrected back to particle (truth) level using calibrations derived from Monte Carlo simulation and validated with both test-beam [44] and collision-data studies [45]. Events are excluded if they contain a high-$p_T$ jet that fails quality criteria rejecting detector noise and non-collision backgrounds [46]. To suppress the use of jets originating from secondary *pp* interactions, a jet vertex fraction (JVF) algorithm is used. Inner detector tracks, with $p_T > 1$ GeV, are uniquely associated with jets using $\Delta R(\text{jet, track}) < 0.4$, where $\Delta R = \sqrt{(\Delta\phi)^2 + (\Delta\eta)^2}$. The JVF algorithm requires that at least 75% of the sum of the $p_T$ of the tracks associated

<footnote n="1">¹ATLAS uses a right-handed coordinate system with its origin at the nominal interaction point (IP) in the centre of the detector and the z-axis along the beam pipe. The x-axis points from the IP to the centre of the LHC ring, and the y-axis points upward. Cylindrical coordinates (r, φ) are used in the transverse (x, y) plane, φ being the azimuthal angle around the beam pipe. The pseudorapidity is defined in terms of the polar angle θ as η = −ln tan(θ/2).</footnote>
with the jet is from tracks compatible with originat-
ing from the primary vertex of the event. Tagging al-
gorithms identify jets originating from b-quark decays
by selecting jets with tracks from secondary vertices
or those with a large impact parameter significance. A
multivariate algorithm (MV1) [47], which uses a neural
network to combine the weights from multiple tagging
algorithms, is used to identify jets originating from b-
quarks. Jets passing the MV1 selection are referred to
as b-tagged jets. The selection on the discriminating
variable of the algorithm achieves an average per-jet ef-
ficiency of 70% to select b-jets in $t\bar{t}$ events, with a prob-
ability to incorrectly tag light jets of less than 0.1% [48].
Studies have shown that this working point has a 20-
40% efficiency to tag a c-jet, depending on the $p_T$ of
the jet [49].

Muons are required to be identified in both the ID
and MS, and their momentum is obtained through a
combined fit of all hits in both systems. Muons are also
required to satisfy isolation criteria to reject those origi-
nating from heavy-flavour decays and hadrons misiden-
tified as muons. The sum of the transverse momenta
of ID tracks within a cone of $\Delta R = 0.3$ around the
muon, excluding the muon track itself, is required to
be less than 2.5 GeV. The transverse energy measured
in the calorimeters within a cone of $\Delta R = 0.2$, exclud-
ing the energy associated with the muon, is required to
be less than 4 GeV. In addition, muons are removed
if they are found within $\Delta R < 0.4$ of a jet that has
$p_T > 25$ GeV [50, 51].

The reconstruction of electron candidates starts from
a seed cluster in the second layer of the EM calorime-
ter. The cluster is matched to a track found in the ID
and a set of selection criteria are applied to reject elec-
tron candidates originating from jets [52]. Electrons are
required to be isolated in order to suppress the QCD
multi-jet background. The calorimeter isolation is per-
formed using a cone of $\Delta R = 0.2$ and the track isolation
uses a cone of radius $\Delta R = 0.3$. The calorimeter and
track isolation cut values are chosen to achieve 90% effi-
ciency with respect to selected electron candidates [53].
As in the case of muons, the electron itself is excluded
from the sum over the isolation cone.

Energy deposits in the calorimeter are expressed as
four-vectors ($E, \mathbf{p}$), where the direction is determined
from the position of the calorimeter cluster and the
nominal interaction point ($x = y = z = 0$). The clus-
ters are formed assuming $E = |p|$. The missing trans-
verse momentum ($E_T^{\text{miss}}$) is given by the negative of the
vector sum of the calorimeter four-momenta, projected
into the $(x, y)$ plane. The $E_T^{\text{miss}}$ calculation uses the en-
ergy scale appropriate for each physics object described
above. For muons, the momentum measured from the

combined tracking is used as the energy. The remaining
calorimeter cells not associated with any physics object
are included at the electromagnetic energy scale of the
calorimeter [54].

A set of requirements is imposed to select events
containing $t\bar{t}$ decays in the lepton+jets channel [50].
First, events are required to contain a primary vertex
with at least five associated tracks to suppress non-
collision backgrounds. Exactly one electron with a large
transverse energy ($E_T > 25$ GeV) and $|\eta| < 2.5$, exclud-
ing the barrel-endcap transition region $1.37 < |\eta| <
1.52$, or one muon with large transverse momentum
($p_T > 20$ GeV) and $|\eta| < 2.5$ is required. The selected
lepton must match a lepton trigger object that caused
the event to be recorded. Jets present in W/Z+jet events
tend to originate from soft gluon emissions. These back-
grounds are therefore reduced by requiring at least four
jets with $p_T > 25$ GeV and $|\eta| < 2.5$. At least two
jets must be identified as originating from a b-decay us-
ing the MV1 algorithm. To suppress backgrounds from
QCD multi-jet events, the missing transverse momen-
tum is required to be $E_T^{\text{miss}} > 20(30)$ GeV in the muon
(electron) channel. Further reduction of the multi-jet
background is achieved by requiring the transverse mass²
($m_T$) of the lepton and $E_T^{\text{miss}}$ to satisfy $m_T > 30$ GeV
in the electron channel and ($E_T^{\text{miss}} + m_T) > 60$ GeV in
the muon channel. These requirements favour the pres-
ence of a W boson, decaying to $\ell\nu$, in the final state.
The selections are more stringent in the electron chan-
nel because of the larger multi-jet background.

4 Kinematic fit

In the selected events, the two jets originating from
the decay of the $H^+$ must be identified in order to re-
construct the mass. A kinematic fitter [17] is used to
identify and reconstruct the mass of dijets from $W/H^+$
candidates, by fully reconstructing the $t\bar{t}$ system. In the
kinematic fitter, the lepton, $E_T^{\text{miss}}$ (assumed to be from
the neutrino), and four jets are assigned to the decay
particles from the $t\bar{t}$ system. The longitudinal compo-
nent of the neutrino momentum is calculated from the
constraint that the invariant mass of the leptonic W bo-
son decay products must be the experimental value
(80.4 GeV) [55]. This leads to two possible solutions
for this momentum. When complex solutions are re-
turned, the real part of the solution is used in the fit.
The fitter also constrains the invariant mass of the two
systems ($b\ell\nu, bjj$) to be within $\Gamma_t = 1.5$ GeV of the

<footnote>$^2m_T = \sqrt{2p_T^\ell E_T^{\text{miss}}(1 - \cos \Delta\phi)}$ where $\Delta\phi$ is the azimuthal angle between the lepton and the missing transverse momentum</footnote>
top-quark mass 172.5 GeV, which is consistent with the measured top-quark mass [56]. When assigning jets in the fitter, b-tagged jets are assumed to originate from the b-quarks. The best *bbjj* combination is found by minimizing a $\chi^2$ for each assignment of jets to quarks and for the choice of solution for the longitudinal neutrino momentum, where the five highest-$p_T$ jets are considered as possible top-quark decay products. Since the b-jets are only allowed to be assigned to the b-quarks, and the two untagged jets are assigned to quarks from the same charged boson, there are two possible jet configurations overall for events with four jets, two of which are b-tagged. For events with at least five jets, the two highest-$p_T$ jets are always assumed to be from the top-quark decay products ($W/H^+$ boson or b-quark) to reduce the combinatorics in the fit procedure. The combination with the smallest $\chi^2$ value, $\chi^2_{min}$, is selected as the best assignment. The function minimized in the fit is:

$$ \chi^2 = \sum_{i=\ell,4\text{jets}} \frac{(p_T^{i,\text{fit}} - p_T^{i,\text{meas}})^2}{\sigma_i^2} + \sum_{j=x,y} \frac{(p_j^{\text{SEJ,fit}} - p_j^{\text{SEJ,meas}})^2}{\sigma_{\text{SEJ}}^2} + \sum_{k=jjb,b\ell\nu} \frac{(m_k - m_t)^2}{\Gamma_t^2}. \quad (1) $$

In the first term, the fitted transverse momenta of the lepton and the four jets currently under consideration are allowed to vary around the measured values using the corresponding measured resolutions ($\sigma_i$). In the fit only the magnitudes of the object $p_{TS}$ are varied; the angles of the jets and leptons are assumed to be measured with good precision. The vector sum of the momenta of the remaining jets ($p_T > 15$ GeV) in the event, labelled SEJ, is allowed to vary in the second term. The resolution for this term is taken from the nominal jet resolution. Letting the SEJ vary allows the $E_T^{\text{miss}}$ to be recalculated from the fitted values of its dominant components. Jets with lower $p_T$ and energy from calorimeter cells not associated with any physics object are both minor contributions to the $E_T^{\text{miss}}$ and are held fixed in the re-calculation of the $E_T^{\text{miss}}$. The third term constrains the hadronic (jjb) and leptonic (b$\ell\nu$) top-quark candidates to have a mass close to the top-quark mass.

The $\chi^2_{min}$ distribution for selected events in the data agrees well with the expectation from the simulation (see Fig. 1). Events are required to have $\chi^2_{min} < 10$ to remove poorly reconstructed $t\bar{t}$ events. This selection has an efficiency of 63% for SM $t\bar{t}$ events. The fit results in a 12 GeV dijet mass resolution, as shown in

Fig. 2. This is a 20–30% improvement, depending on the mass of the boson studied, compared to the resolution obtained when the same jets are used with their original transverse momentum measurements. After the fit, there is better discrimination between the mass peaks of the W boson from SM decays of $t\bar{t}$ and a 110 GeV $H^+$ boson in this example.

<figure><img src="image_2.png" /><figcaption>**Fig. 1** Comparison of the distribution of $\chi^2_{min}$ from the kinematic fitter for data and the expectation from the background estimates for the combined electron and muon channels. The MC simulation is normalized to the expectation for the SM ($B(t \to H^+b) = 0$). The uncertainty shown on the background estimate is the combination in quadrature of the $\pm 1\sigma$ systematic uncertainties. The final bin also contains the overflow entries.</figcaption></figure>

Table 1 shows the number of events observed in the data and the number of events expected from the SM processes after the selection requirements. The SM $t\bar{t}$ entry includes events from both the lepton + jets and dilepton $t\bar{t}$ decay modes, where the dilepton events can pass the event selection if the events contain additional jets and the second lepton is not identified. Good agreement is observed between the data and the expectation. The table also shows the number of signal events expected for $B(t \to H^+b) = 10\%$. The signal prediction accounts for acceptance differences due to the different kinematics of the $t \to H^+b$ events relative to the SM $t \to Wb$ events.

## 5 Systematic uncertainties

The background estimates and the estimate of the signal efficiency are subject to a number of systematic uncertainties. The QCD multi-jet background is estimated using a data-driven method [57] that employs a likelihood fit to the $E_T^{\text{miss}}$ distribution in the data,
<figure><img src="image_3.png" /></figure>

<figure><img src="image_4.png" /><figcaption>**Fig. 2** Comparison of the dijet mass distribution before (upper part) and after (lower part) the kinematic fit and the $\chi^2 < 10$ selection criterion. The distribution is shown for MC simulations of SM $t\bar{t}$ decays and the $m_{H^+} = 110$ GeV signal ($t\bar{t} \to H^+bW^-\bar{b}$). The curves are normalized to the same area.</figcaption></figure>

using a template for the multi-jet background and templates from MC simulations for all other processes. The uncertainty on the QCD multi-jet background is evaluated to be 50% by studying the effect of pile-up events on the fit results and by performing likelihood fits on the $m_T(W)$ distribution. The dijet mass distribution of multi-jet events is obtained from a control region in the data, where leptons are required to be semi-isolated, such that the transverse momentum of the inner detector tracks in a cone of radius $\Delta R = 0.3$, excluding the lepton, satisfies $0.1 < p_T^{\Delta R=0.3}/p_T(e, \mu) < 0.3$. Leptons in the control region are also required to have a large impact parameter with respect to the identified primary vertex (0.2 mm $< |d_0| < 2$ mm) and an impact parameter significance $|d_0|/\sigma_{d_0} > 3$.

The rate of W+jets events is estimated by a data-driven method [58] that uses the observed difference in the number of W$^+$ and W$^-$ bosons in the data and the charge asymmetry $(W^+ - W^-)/(W^+ + W^-)$, which is calculated to good precision by the MC simulation

<table><caption>**Table 1** The expected numbers of events from SM processes, integrated over the full range of dijet masses and the observed number of events in the data after all the selection requirements. The expected number of events in the case of a signal with $m_{H^+} = 110$ GeV and $B(t \to H^+bW^-\bar{b}) = 10\%$ is also shown. The $t\bar{t} \to W^+bW^-\bar{b}$ numbers include both the lepton + jets and dilepton decay channels. The uncertainties are the sum of the contributions from statistics and systematic uncertainties.</caption><thead><tr><th>Channel</th><th>Muon</th><th>Electron</th></tr></thead><tbody><tr><td>Data</td><td>10107</td><td>5696</td></tr><tr><td>SM t<span style="text-decoration: overline">t</span> → W<sup>+</sup>bW<sup>-</sup><span style="text-decoration: overline">b</span></td><td>8700 ± 1800</td><td>5000 ± 1000</td></tr><tr><td>W/Z + jets</td><td>420 ± 120</td><td>180 ± 50</td></tr><tr><td>Single top quark + Diboson</td><td>370 ± 60</td><td>210 ± 30</td></tr><tr><td>QCD multi-jet</td><td>300 ± 150</td><td>130 ± 60</td></tr><tr><td>Total Expected (SM)</td><td>9800 ± 1800</td><td>5500 ± 1000</td></tr><tr><td>m<sub>H<sup>+</sup></sub> = 110 GeV</td><td></td><td></td></tr><tr><td>B(t → H<sup>+</sup>b) = 10% :</td><td></td><td></td></tr><tr><td style="padding-left: 2em">t<span style="text-decoration: overline">t</span> → H<sup>+</sup>bW<sup>-</sup><span style="text-decoration: overline">b</span></td><td>1400 ± 280</td><td>800 ± 160</td></tr><tr><td style="padding-left: 2em">t<span style="text-decoration: overline">t</span> → W<sup>+</sup>bW<sup>-</sup><span style="text-decoration: overline">b</span></td><td>7000 ± 1400</td><td>4000 ± 800</td></tr><tr><td>Total Expected (B = 10%)</td><td>9500 ± 1700</td><td>5300 ± 1000</td></tr></tbody></table>

of W+jets events. The heavy flavour fraction of the W+jets MC simulation is calibrated using W + 1 jet or W + 2 jets events in the data. The uncertainty on the W+jets background is 26% (28%) for the electron (muon) channel, which includes the uncertainty from the charge asymmetry and heavy flavour fraction components. The shape of the $m_{jj}$ distribution for W+jets events is obtained from simulation.

Uncertainties on the modelling of the detector and on theory give rise to systematic uncertainties on the signal and background rate estimates. The following systematic uncertainties are considered: integrated luminosity (3.9%) [22, 23], trigger efficiency (3.5%/1% for electron/muon), jet energy scale (1–4.6%) [45], jet energy resolution (up to 16% smearing) [59], and b-jet identification efficiency (5–17%). The last three uncertainties depend on the $p_T$ and $\eta$ of the jets. Uncertainties on lepton reconstruction and identification efficiency are determined using a tag and probe method in samples of Z boson and $J/\psi$ decays [60]. The momentum resolution and scales are determined from fits to samples of W boson, Z boson, and $J/\psi$ decays [53, 61]. Additional $p_T$-dependent uncertainties are placed on the b-jet (up to 2.5%) and c-jet (up to 1.3%) energy scales [45]. Uncertainties on the modelling of the $t\bar{t}$ background are estimated using a second MC generator (POWHEG [62–64]) and comparing the effect of using PYTHIA and HERWIG to perform the parton showering and hadronization. Uncertainties on initial and final state radiation (ISR/FSR) are assessed using Ac-
ERMC interfaced to PYTHIA and examining the effects of changing the ISR/FSR parameters in a range consistent with experimental data [65]. The predicted SM $t\bar{t}$ cross-section for pp collisions at $\sqrt{s} = 7$ TeV, obtained from approximate next to next to LO QCD calculations, is $\sigma_{t\bar{t}} = 167_{-18}^{+17}$ pb for a top-quark mass of 172.5 GeV [66]. The uncertainty on the predicted value includes the uncertainty in the renormalization and factorization scales, parton density functions, and the strong coupling constant. An additional uncertainty on the $t\bar{t}$ cross-section (4.5%) is included due to the uncertainty on the top-quark mass. The uncertainty on the top-quark mass is 0.9 GeV from the combined measurement [56] at the Tevatron. However, this result would be biased in the presence of a $H^+ \to c\bar{s}$ signal in the lepton + jets channel, so a larger uncertainty of 1.5 GeV is taken, which is consistent with the latest top-quark mass measurement in the dilepton channel from the CMS experiment [67]. Changing the top-quark mass leads to altered event kinematics, which results in a final uncertainty on the event rate of 1.9%. The effects of these systematic uncertainties on the overall normalization are listed in Table 2. The jet energy calibration, b-jet identification, $t\bar{t}$ background modelling, and ISR/FSR uncertainties also modify the shape of the dijet mass distribution and are therefore determined as a function of $m_{jj}$. The systematic uncertainties that affect the shape of the $m_{jj}$ distribution (top half of Table 2) are more important than the shape-independent uncertainties. The effects of the systematic uncertainties are comparable, within 10%, between the SM and signal $t\bar{t}$ samples. The combined uncertainty on the single top-quark and diboson backgrounds is 15%, which comes mostly from the uncertainties on the cross-section, jet energy scale, and b-tagging. The total uncertainty on the overall normalization of the non-$t\bar{t}$ backgrounds is 30%.

## 6 Results

The data are found to be in good agreement with the distribution of the dijet mass expected from SM processes (see Fig. 3). The fractional uncertainty on the signal-plus-background model is comparable to the background only model. Upper limits on the branching ratio $B(t \to H^+b)$ are extracted as a function of the charged Higgs boson mass. The upper limits are calculated assuming the charged Higgs always decays to $c\bar{s}$. The following likelihood function is used to describe the ex-

<table><caption>**Table 2** Effect of the systematic uncertainties on the event rate of $t\bar{t}$ background and signal ($m_{H^+} = 110$ GeV) events before any reduction from the likelihood fit, described in Sect. 6.</caption><thead><tr><th colspan="2">Systematic Source</th></tr></thead><tbody><tr><td colspan="2">Shape dependent</td></tr><tr><td>Jet energy scale</td><td>±9.5%</td></tr><tr><td>b-jet energy scale</td><td>+0.3, -0.6%</td></tr><tr><td>c-jet energy scale</td><td>+0.1, -0.3%</td></tr><tr><td>Jet energy resolution</td><td>±0.9%</td></tr><tr><td>MC generator</td><td>±4.3%</td></tr><tr><td>Parton shower</td><td>±3.1%</td></tr><tr><td>ISR/FSR</td><td>±8.8%</td></tr><tr><td colspan="2">Shape independent</td></tr><tr><td>b-tagging efficiency (b-jets)</td><td>±11%</td></tr><tr><td>b-tagging efficiency (c-jets)</td><td>±2.4%</td></tr><tr><td>b mistag rate</td><td>±1.8%</td></tr><tr><td>Lepton identification</td><td>±1.4%</td></tr><tr><td>Lepton reconstruction</td><td>±1.0%</td></tr><tr><td>t-quark mass</td><td>±1.9%</td></tr><tr><td>t\bar{t} cross-section</td><td>+10, -11%</td></tr><tr><td>Luminosity</td><td>±3.9%</td></tr></tbody></table>

<figure><img src="image_5.png" /><figcaption>**Fig. 3** The dijet mass distribution from data and the expectation from the SM ($B = 0$). The error bars represent the statistical uncertainty on the data. The uncertainty shown on the background estimate is the combination in quadrature of the $\pm 1\sigma$ systematic uncertainties, accounting for the constraint from the profile likelihood fit. The first and last bins contain the underflow and overflow events respectively.</figcaption></figure>

expected number of events as a function of the branching ratio:

$$ \mathcal{L}(B, \alpha) = \prod_i \frac{\nu_i(B, \alpha)^{n_i} e^{-\nu_i(B, \alpha)}}{n_i!} \prod_j \frac{1}{\sqrt{2\pi}} e^{-\frac{\alpha_j^2}{2}}, \quad (2) $$

where $n_i$ is the number of events observed in bin i of the dijet mass distribution and j labels the sources of systematic uncertainty. The number of expected signal
plus background events in each bin, $\nu_i(\mathcal{B}, \alpha)$, is given by

$$ \nu_i(\mathcal{B}, \alpha) = 2\mathcal{B}(1-\mathcal{B})\sigma_{t\bar{t}}\mathcal{L} A^{H^+} S_i^{H^+} \prod_{j \neq b} \rho_{ji}^{H^+}(\alpha_j) \\ +(1-\mathcal{B})^2 \sigma_{t\bar{t}}\mathcal{L} A^W S_i^W \prod_{j \neq b} \rho_{ji}^W(\alpha_j) + n_i^N \rho_{bi}^N(\alpha_b) \quad (3) $$

where $n_i^N$ is the expected number of non-$t\bar{t}$ background events, $\sigma_{t\bar{t}}$ is the cross-section for $t\bar{t}$ production, $\mathcal{L}$ is the integrated luminosity, $\mathcal{B}$ is the branching ratio of $t \to H^+b$, and $A^{H^+}$ and $A^W$ are the acceptances for signal ($t\bar{t} \to H^+b\ell\nu\bar{b}$) and SM $t\bar{t}$ ($t\bar{t} \to jjb\ell\nu\bar{b}$ and $t\bar{t} \to \ell\bar{\nu}b\ell\nu\bar{b}$) events respectively. The decay mode $t\bar{t} \to H^+bH^-\bar{b}$ does not contribute to the expectation because this mode does not produce a single isolated lepton and hence has a negligible efficiency to pass the selection requirements. The $S_i^{H^+}$ ($S_i^W$) parameter describes the shape of the $m_{jj}$ spectrum (normalized to one) for $H^+$ ($W$) boson production. It gives the relative number of events in bin $i$ according to the normalized $m_{jj}$ distribution. The $\alpha_j$ variables are nuisance parameters representing the systematic uncertainties, which are constrained via the Gaussian terms in Eq. 2. The effect of the systematic uncertainties on the non-$t\bar{t}$ background can be obtained by calculating the effect of each source of uncertainty on each non-$t\bar{t}$ background component, and combining them in quadrature. Since this sum is dominated by the uncertainties on the data-driven $W$+jets and multi-jet background estimates, the combined variation is treated as a single nuisance parameter ($\alpha_b, b \in j$) and is assumed to be uncorrelated from the other systematic uncertainties. The $\rho_{ji}$ functions account for the effect of nuisance parameters on the yields and are defined such that $\rho_{ji}(\alpha_j = \pm 1\sigma)$ represents the $1 \pm 1\sigma$ fractional change in the number of entries in bin $i$ of the dijet mass spectrum due to systematic uncertainty $j$. The physics measurement involves a sufficiently large number of events that this likelihood can constrain the $\alpha_j$ parameters beyond the precision of the subsidiary measurements. The effects of systematic uncertainties are applied coherently in signal and background distributions. The subsidiary measurements of the $\alpha_j$ parameters are taken to be uncorrelated. The fit uses 17 nuisance parameters in total. None of them are shifted by more than one sigma compared to the original values obtained in subsidiary measurements. Maximal reduction of uncertainty is obtained for the jet energy scale parameter which is reduced by 50%.

The limits on the branching ratio are extracted using the CLs technique at 95% confidence level [68, 69]. The consistency of the data with the background model can be determined by comparing the value of the test

<table><caption>**Table 3** Expected and observed 95% CL limits, including systematic uncertainties, on the branching ratio for a top-quark to decay to a charged Higgs boson and a b-quark, assuming that $\mathcal{B}(H^+ \to c\bar{s}) = 100\%$. The limits shown are calculated using the CLs limit-setting procedure.</caption><thead><tr><th>Higgs Mass</th><th>Expected limit (stat.⊕ syst.)</th><th>Observed limit (stat.⊕ syst.)</th></tr></thead><tbody><tr><td>90 GeV</td><td>0.080</td><td>0.051</td></tr><tr><td>100 GeV</td><td>0.034</td><td>0.034</td></tr><tr><td>110 GeV</td><td>0.026</td><td>0.025</td></tr><tr><td>120 GeV</td><td>0.021</td><td>0.018</td></tr><tr><td>130 GeV</td><td>0.023</td><td>0.014</td></tr><tr><td>140 GeV</td><td>0.020</td><td>0.013</td></tr><tr><td>150 GeV</td><td>0.015</td><td>0.012</td></tr></tbody></table>

<figure><img src="image_6.png" /><figcaption>**Fig. 4** The extracted 95% CL upper limits on $\mathcal{B}(t \to H^+b)$, assuming that $\mathcal{B}(H^+ \to c\bar{s}) = 100\%$, are shown for a range of charged Higgs masses from 90 GeV to 150 GeV. The limits shown are calculated using the CLs limit-setting procedure.</figcaption></figure>

statistic (a profile likelihood ratio based on Eq. 2) in the data with the expectation from background-only Monte Carlo simulated experiments. The corresponding probability ($p$-value) for the background to produce the observed mass distribution varies from 67% to 71% as a function of $m_{H^+}$, indicating that there is no significant deviation from the background hypothesis. The expected and observed limits, shown in Table 3 and Fig. 4, are calculated using asymptotic formulae [68]. The expected limits on $\mathcal{B}$, including both statistical and systematic uncertainties, vary between 1–8% depending on $m_{H^+}$; if only the statistical uncertainty is considered these limits are 1–3%. The observed limits, including both statistical and systematic uncertainties, vary between 1–5%. The extracted limits are the most stringent to date on the branching ratio $\mathcal{B}(t \to H^+b)$, assuming $\mathcal{B}(H^+ \to c\bar{s}) = 100\%$. These results can be used to set limits for a generic scalar charged boson decaying to dijets in top-quark decays, as long as the width of the resonance formed is less than the experimental dijet resolution of 12 GeV.
## 7 Conclusions

A search for charged Higgs bosons decaying to $c\bar{s}$ in $t\bar{t}$ production has been presented. The dijet mass distribution is in good agreement with the expectation from the SM and limits are set on the branching ratio $B(t \to H^+b)$, assuming $B(H^+ \to c\bar{s}) = 100\%$. The observed limits range from $B = 5\%$ to 1% for $m_{H^+} = 90$ GeV to 150 GeV. These are the best limits to date on charged Higgs boson production in this channel.

## 8 Acknowledgements

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; BMWF 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, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, DIP and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW, Poland; GRICES and FCT, Portugal; MERTS (MECTS), Romania; MES of Russia and ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MVZT, Slovenia; DST/NRF, South Africa; MICINN, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America.

The crucial computing support from all WLCG partners is acknowledged gratefully, in particular from CERN and 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) and in the Tier-2 facilities worldwide.

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G.J. Bobbink¹⁰⁵, V.S. Bobrovnikov¹⁰⁷, S.S. Bocchetta⁷⁹, A. Bocci⁴⁵, C.R. Boddy¹¹⁸, M. Boehler⁴⁸, J. Boek¹⁷⁵,
T.T. Boek¹⁷⁵, N. Boelaert³⁶, J.A. Bogaerts³⁰, A. Bogdanchikov¹⁰⁷, A. Bogouch⁹⁰,*, C. Bohm¹⁴⁶a, J. Bohm¹²⁵,
V. Boisvert⁷⁶, T. Bold³⁸, V. Boldea²⁶a, N.M. Bolnet¹³⁶, M. Bomben⁷⁸, M. Bona⁷⁵, M. Boonekamp¹³⁶,
S. Bordini⁷⁸, C. Borer¹⁷, A. Borisov¹²⁸, G. Borissov⁷¹, I. Borjanovic¹³a, M. Borri⁸², S. Borroni⁴², J. Bortfeldt⁹⁸,
V. Bortolotto¹³⁴a,¹³⁴b, K. Bos¹⁰⁵, D. Boscherini²⁰a, M. Bosman¹², H. Boterenbrood¹⁰⁵, J. Bouchami⁹³,
J. Boudreau¹²³, E.V. Bouhova-Thacker⁷¹, D. Boumediene³⁴, C. Bourdarios¹¹⁵, N. Bousson⁸³, A. Boveia³¹,
J. Boyd³⁰, I.R. Boyko⁶⁴, I. Bozovic-Jelisavcic¹³b, J. Bracinik¹⁸, P. Branchini¹³⁴a, A. Brandt⁸, G. Brandt¹¹⁸,
O. Brandt⁵⁴, U. Bratzler¹⁵⁶, B. Brau⁸⁴, J.E. Brau¹¹⁴, H.M. Braun¹⁷⁵,*, S.F. Brazzale¹⁶⁴a,¹⁶⁴c, B. Brelier¹⁵⁸,
J. Bremer³⁰, K. Brendlinger¹²⁰, R. Brenner¹⁶⁶, S. Bressler¹⁷², T.M. Bristow¹⁴⁵b, D. Britton⁵³, F.M. Brochu²⁸,
I. Brock²¹, R. Brock⁸⁸, F. Broggi⁸⁹a, C. Bromberg⁸⁸, J. Bronner⁹⁹, G. Brooijmans³⁵, T. Brooks⁷⁶,
W.K. Brooks³²b, G. Brown⁸², P.A. Bruckman de Renstrom³⁹, D. Bruncko¹⁴⁴b, R. Bruneliere⁴⁸, S. Brunet⁶⁰,
A. Bruni²⁰a, G. Bruni²⁰a, M. Bruschi²⁰a, L. Bryngemark⁷⁹, T. Buanes¹⁴, Q. Buat⁵⁵, F. Bucci⁴⁹, J. Buchanan¹¹⁸,
P. Buchholz¹⁴¹, R.M. Buckingham¹¹⁸, A.G. Buckley⁴⁶, S.I. Buda²⁶ª, I.A. Budagov⁶⁴, B. Budick¹⁰⁸, V. Büscher⁸¹, L. Bugge¹¹⁷, O. Bulekov⁹⁶, A.C. Bundock⁷³, M. Bunse⁴³, T. Buran¹¹⁷, H. Burckhart³⁰, S. Burdin⁷³, T. Burgess¹⁴, S. Burke¹²⁹, E. Busato³⁴, P. Bussey⁵³, C.P. Buszello¹⁶⁶, B. Butler¹⁴³, J.M. Butler²², C.M. Buttar⁵³, J.M. Butterworth⁷⁷, W. Buttinger²⁸, M. Byszewski³⁰, S. Cabrera Urbán¹⁶⁷, D. Caforio²⁰ª,²⁰ᵇ, O. Cakir⁴ª, P. Calafiura¹⁵, G. Calderini⁷⁸, P. Calfayan⁹⁸, R. Calkins¹⁰⁶, L.P. Caloba²⁴ª, R. Caloi¹³²ª,¹³²ᵇ, D. Calvet³⁴, S. Calvet³⁴, R. Camacho Toro³⁴, P. Camarri¹³³ª,¹³³ᵇ, D. Cameron¹¹⁷, L.M. Caminada¹⁵, R. Caminal Armadans¹², S. Campana³⁰, M. Campanelli⁷⁷, V. Canale¹⁰²ª,¹⁰²ᵇ, F. Canelli³¹, A. Canepa¹⁵⁹ª, J. Cantero⁸⁰, R. Cantrill⁷⁶, M.D.M. Capeans Garrido³⁰, I. Caprini²⁶ª, M. Caprini²⁶ª, D. Capriotti⁹⁹, M. Capua³⁷ª,³⁷ᵇ, R. Caputo⁸¹, R. Cardarelli¹³³ª, T. Carli³⁰, G. Carlino¹⁰²ª, L. Carminati⁸⁹ª,⁹⁹ᵇ, S. Caron¹⁰⁴, E. Carquin³²ᵇ, G.D. Carrillo-Montoya¹⁴⁵ᵇ, A.A. Carter⁷⁵, J.R. Carter²⁸, J. Carvalho¹²⁴ª,ᵢ, D. Casadei¹⁰⁸, M.P. Casado¹², M. Cascella¹²²ª,¹²²ᵇ, C. Caso⁵⁰ª,⁵⁰ᵇ,*, A.M. Castaneda Hernandez¹⁷³,ⱼ, E. Castaneda-Miranda¹⁷³, V. Castillo Gimenez¹⁶⁷, N.F. Castro¹²⁴ª, G. Cataldi⁷²ª, P. Catastini⁵⁷, A. Catinaccio³⁰, J.R. Catmore³⁰, A. Cattai³⁰, G. Cattani¹³³ª,¹³³ᵇ, S. Caughron⁸⁸, V. Cavaliere¹⁶⁵, P. Cavalleri⁷⁸, D. Cavalli⁸⁹ª, M. Cavalli-Sforza¹², V. Cavasinni¹²²ª,¹²²ᵇ, F. Ceradini¹³⁴ª,¹³⁴ᵇ, A.S. Cerqueira²⁴ᵇ, A. Cerri¹⁵, L. Cerrito⁷⁵, F. Cerutti¹⁵, S.A. Cetin¹⁹ᵇ, A. Chafaq¹³⁵ª, D. Chakraborty¹⁰⁶, I. Chalupkova¹²⁷, K. Chan³, P. Chang¹⁶⁵, B. Chapleau⁸⁵, J.D. Chapman²⁸, J.W. Chapman⁸⁷, D.G. Charlton¹⁸, V. Chavda⁸², C.A. Chavez Barajas³⁰, S. Cheatham⁸⁵, S. Chekanov⁶, S.V. Chekulaev¹⁵⁹ª, G.A. Chelkov⁶⁴, M.A. Chelstowska¹⁰⁴, C. Chen⁶³, H. Chen²⁵, S. Chen³³c, X. Chen¹⁷³, Y. Chen³⁵, Y. Cheng³¹, A. Cheplakov⁶⁴, R. Cherkaoui El Moursli¹³⁵ᵉ, V. Chernyatin²⁵, E. Cheu⁷, S.L. Cheung¹⁵⁸, L. Chevalier¹³⁶, G. Chiefari¹⁰²ª,¹⁰²ᵇ, L. Chikovani⁵¹ª,*, J.T. Childers³⁰, A. Chilingarov⁷¹, G. Chiodini⁷²ª, A.S. Chisholm¹⁸, R.T. Chislett⁷⁷, A. Chitan²⁶ª, M.V. Chizhov⁶⁴, G. Choudalakis³¹, S. Chouridou¹³⁷, I.A. Christidi⁷⁷, A. Christov⁴⁸, D. Chromek-Burckhart³⁰, M.L. Chu¹⁵¹, J. Chudoba¹²⁵, G. Ciapetti¹³²ª,¹³²ᵇ, A.K. Ciftci⁴ª, R. Ciftci⁴ª, D. Cinca³⁴, V. Cindro⁷⁴, A. Ciocio¹⁵, M. Cirilli⁸⁷, P. Cirkovic¹³ᵇ, Z.H. Citron¹⁷², M. Citterio⁸⁹ª, M. Ciubancan²⁶ª, A. Clark⁴⁹, P.J. Clark⁴⁶, R.N. Clarke¹⁵, W. Cleland¹²³, J.C. Clemens⁸³, B. Clement⁵⁵, C. Clement¹⁴⁶ª,¹⁴⁶ᵇ, Y. Coadou⁸³, M. Cobal¹⁶⁴ª,¹⁶⁴ᵇ, A. Coccaro¹³⁸, J. Cochran⁶³, L. Coffey²³, J.G. Cogan¹⁴³, J. Coggeshall¹⁶⁵, J. Colas⁵, S. Cole¹⁰⁶, A.P. Colijn¹⁰⁵, N.J. Collins¹⁸, C. Collins-Tooth⁵³, J. Collot⁵⁵, T. Colombo¹¹⁹ª,¹¹⁹ᵇ, G. Colon⁸⁴, G. Compostella⁹⁹, P. Conde Muiño¹²⁴ª, E. Coniavitis¹⁶⁶, M.C. Conidi¹², S.M. Consonni⁸⁹ª,⁹⁹ᵇ, V. Consorti⁴⁸, S. Constantinescu²⁶ª, C. Conta¹¹⁹ª,¹¹⁹ᵇ, G. Conti⁵⁷, F. Conventi¹⁰²ª,*, M. Cooke¹⁵, B.D. Cooper⁷⁷, A.M. Cooper-Sarkar¹¹⁸, K. Copic¹⁵, T. Cornelissen¹⁷⁵, M. Corradi²⁰ª, F. Corriveau⁸⁵,ᵢ, A. Cortes-Gonzalez¹⁶⁵, G. Cortiana⁹⁹, G. Costa⁸⁹ª, M.J. Costa¹⁶⁷, D. Costanzo¹³⁹, D. Côté³⁰, G. Cottin³²ª, L. Journeyea¹⁶⁹, G. Cowan⁷⁶, B.E. Cox⁸², K. Cranmer¹⁰⁸, F. Crescioli⁷⁸, M. Cristinziani²¹, G. Crosetti³⁷ª,³⁷ᵇ, S. Crépé-Renaudin⁵⁵, C.-M. Cuciuc²⁶ª, C. Cuenca Almenar¹⁷⁶, T. Cuhadar Donszelmann¹³⁹, J. Cummings¹⁷⁶, M. Curatolo⁴⁷, C.J. Curtis¹⁸, C. Cuthbert¹⁵⁰, P. Cwetanski⁶⁰, H. Czirr¹⁴¹, P. Czodrowski⁴⁴, Z. Czyczula¹⁷⁶, S. D'Auria⁵³, M. D'Onofrio⁷³, A. D'Orazio¹³²ª,¹³²ᵇ, M.J. Da Cunha Sargedas De Sousa¹²⁴ª, C. Da Via⁸², W. Dabrowski³⁸, A. Dafinca¹¹⁸, T. Dai⁸⁷, F. Dallaire⁹³, C. Dallapiccola⁸⁴, M. Dam³⁶, M. Dameri⁵⁰ª,⁵⁰ᵇ, D.S. Damiani¹³⁷, H.O. Danielsson³⁰, V. Dao¹⁰⁴, G. Darbo⁵⁰ª, G.L. Darlea²⁶ᵇ, J.A. Dassoulas⁴², W. Davey²¹, T. Davidek¹²⁷, N. Davidson⁸⁶, R. Davidson⁷¹, E. Davies¹¹⁸,₉, M. Davies⁹³, O. Davignon⁷⁸, A.R. Davison⁷⁷, Y. Davygora⁵⁸ª, E. Dawe¹⁴², I. Dawson¹³⁹, R.K. Daya-Ishmukhametova²³, K. De⁸, R. de Asmundis¹⁰²ª, S. De Castro²⁰ª,²⁰ᵇ, S. De Cecco⁷⁸, J. de Graat⁹⁸, N. De Groot¹⁰⁴, P. de Jong¹⁰⁵, C. De La Taille¹¹⁵, H. De la Torre⁸⁰, F. De Lorenzi⁶³, L. De Nooij¹⁰⁵, D. De Pedis¹³²ª, A. De Salvo¹³²ª, U. De Sanctis¹⁶⁴ª,¹⁶⁴ᶜ, A. De Santo¹⁴⁹, J.B. De Vivie De Regie¹¹⁵, G. De Zorzi¹³²ª,¹³²ᵇ, W.J. Dearnaley⁷¹, R. Debbe²⁵, C. Debenedetti⁴⁶, B. Dechenaux⁵⁵, D.V. Dedovich⁶⁴, J. Degenhardt¹²⁰, J. Del Peso⁸⁰, T. Del Prete¹²²ª,¹²²ᵇ, T. Delemontex⁵⁵, M. Deliyergiyev⁷⁴, A. Dell'Acqua³⁰, L. Dell'Asta²², M. Della Pietra¹⁰²ª,*, D. della Volpe¹⁰²ª,¹⁰²ᵇ, M. Delmastro⁵, P.A. Delsart⁵⁵, C. Deluca¹⁰⁵, S. Demers¹⁷⁶, M. Demichev⁶⁴, B. Demirkoz¹²,*, S.P. Denisov¹²⁸, D. Derendarz³⁹, J.E. Derkaoui¹³⁵d, F. Derue⁷⁸, P. Dervan⁷³, K. Desch²¹, E. Devetak¹⁴⁸, P.O. Deviveiros¹⁰⁵, A. Dewhurst¹²⁹, B. DeWilde¹⁴⁸, S. Dhaliwal¹⁵⁸, R. Dhullipudi²⁵,ⁿ, A. Di Ciaccio¹³³ª,¹³³ᵇ, L. Di Ciaccio⁵, C. Di Donato¹⁰²ª,¹⁰²ᵇ, A. Di Girolamo³⁰, B. Di Girolamo³⁰, S. Di Luise¹³⁴ª,¹³⁴ᵇ, A. Di Mattia¹⁵², B. Di Micco³⁰, R. Di Nardo⁴⁷, A. Di Simone¹³³ª,¹³³ᵇ, R. Di Sipio²⁰ª,²⁰ᵇ, M.A. Diaz³²ª, E.B. Diehl⁸⁷, J. Dietrich⁴², T.A. Dietzsch⁵⁸ª, S. Diglio⁸⁶, K. Dindar Yagci⁴⁰, J. Dingfelder²¹, F. Dinut²⁶ª, C. Dionisi¹³²ª,¹³²ᵇ, P. Dita²⁶ª, S. Dita²⁶ª, F. Dittus³⁰, F. Djama⁸³, T. Djobava⁵¹ᵇ, M.A.B. do Vale²⁴ᶜ, A. Do Valle Wemans¹²⁴ª,, T.K.O. Doan⁵, M. Dobbs⁸⁵, D. Dobos³⁰, E. Dobson³⁰,, J. Dodd³⁵, C. Doglioni⁴⁹, T. Doherty⁵³, Y. Doi⁶⁵,*, J. Dolejsi¹²⁷, Z. Dolezal¹²⁷, B.A. Dolgoshein⁹⁶,*, T. Dohmae¹⁵⁵, M. Donadelli²⁴d, J. Donini³⁴, J. Dopke³⁰, A. Doria¹⁰²ª, A. Dos Anjos¹⁷³, A. Dotti¹²²ª,¹²²ᵇ, M.T. Dova⁷⁰, A.D. Doxiadis¹⁰⁵, A.T. Doyle⁵³, N. Dressnandt¹²⁰, M. Dris¹⁰, J. Dubbert⁹⁹,
S. Dube¹⁵, E. Dubreuil³⁴, E. Duchovni¹²⁷, G. Duckeck⁹⁸, D. Duda¹⁷⁵, A. Dudarev³⁰, F. Dudziak⁶³,
M. Dührssen³⁰, I.P. Duerdoth⁸², L. Duflot¹¹⁵, M-A. Dufour⁸⁵, L. Duguid⁷⁶, M. Dunford⁵⁸ᵃ, H. Duran Yildiz⁴ᵃ,
R. Duxfield¹³⁹, M. Dwuznik³⁸, M. Düren⁵², W.L. Ebenstein⁴⁵, J. Ebke⁹⁸, S. Eckweiler⁸¹, W. Edson²,
C.A. Edwards⁷⁶, N.C. Edwards⁵³, W. Ehrenfeld²¹, T. Eifert¹⁴³, G. Eigen¹⁴, K. Einsweiler¹⁵, E. Eisenhandler⁷⁵,
T. Ekelof¹⁶⁶, M. El Kacimi¹³⁵ᶜ, M. Ellert¹⁶⁶, S. Elles⁵, F. Ellinghaus⁸¹, K. Ellis⁷⁵, N. Ellis³⁰, J. Elmsheuser⁹⁸,
M. Elsing³⁰, D. Emeliyanov¹²⁹, R. Engelmann¹⁴⁸, A. Engl⁹⁸, B. Epp⁶¹, J. Erdmann¹⁷⁶, A. Ereditato¹⁷,
D. Eriksson¹⁴⁶ᵃ, J. Ernst², M. Ernst²⁵, J. Ernwein¹³⁶, D. Errede¹⁶⁵, S. Errede¹⁶⁵, E. Ertel⁸¹, M. Escalier¹¹⁵,
H. Esch⁴³, C. Escobar¹²³, X. Espinal Curull¹², B. Esposito⁴⁷, F. Etienne⁸³, A.I. Etienvre¹³⁶, E. Etzion¹⁵³,
D. Evangelakou⁵⁴, H. Evans⁶⁰, L. Fabbri²⁰ᵃ,²⁰ᵇ, C. Fabre³⁰, R.M. Fakhrutdinov¹²⁸, S. Falciano¹³²ᵃ, Y. Fang³³ᵃ,
M. Fanti⁸⁹ᵃ,⁸⁹ᵇ, A. Farbin⁸, A. Farilla¹³⁴ᵃ, J. Farley¹⁴⁸, T. Farooque¹⁵⁸, S. Farrell¹⁶³, S.M. Farrington¹⁷⁰,
P. Farthouat³⁰, F. Fassi¹⁶⁷, P. Fassnacht³⁰, D. Fassouliotis⁹, B. Fatholahzadeh¹⁵⁸, A. Favareto⁸⁹ᵃ,⁸⁹ᵇ,
L. Fayard¹¹⁵, P. Federic¹⁴⁴ᵃ, O.L. Fedin¹²¹, W. Fedorko¹⁶⁸, M. Fehling-Kaschek⁴⁸, L. Feligioni⁸³, C. Feng³³d,
E.J. Feng⁶, A.B. Fenyuk¹²⁸, J. Ferencei¹⁴⁴b, W. Fernando⁶, S. Ferrag⁵³, J. Ferrando⁵³, V. Ferrara⁴²,
A. Ferrari¹⁶⁶, P. Ferrari¹⁰⁵, R. Ferrari¹¹⁹ᵃ, D.E. Ferreira de Lima⁵³, A. Ferrer¹⁶⁷, D. Ferrere⁴⁹, C. Ferretti⁸⁷,
A. Ferretto Parodi⁵⁰ᵃ,⁵⁰ᵇ, M. Fiascaris³¹, F. Fiedler⁸¹, A. Filipčič⁷⁴, F. Filthaut¹⁰⁴, M. Fincke-Keeler¹⁶⁹,
M.C.N. Fiolhais¹²⁴ᵃ,ᵢ, L. Fiorini¹⁶⁷, A. Firan⁴⁰, G. Fischer⁴², M.J. Fisher¹⁰⁹, E.A. Fitzgerald²³, M. Flech¹⁴⁸,
I. Fleck¹⁴¹, J. Fleckner⁸¹, P. Fleischmann¹⁷⁴, S. Fleischmann¹⁷⁵, G. Fletcher⁷⁵, T. Flick¹⁷⁵, A. Floderus⁷⁹,
L.R. Flores Castillo¹⁷³, A.C. Florez Bustos¹⁵⁹b, M.J. Flowerdew⁹⁹, T. Fonseca Martin¹⁷, A. Formica¹³⁶,
A. Forti⁸², D. Fortin¹⁵⁹ᵃ, D. Fournier¹¹⁵, A.J. Fowler⁴⁵, H. Fox⁷¹, P. Francavilla¹², M. Franchini²⁰²ᵃ,²⁰ᵇ,
S. Franchino¹¹⁹ᵃ,¹¹⁹ᵇ, D. Francis³⁰, T. Frank¹⁷², M. Franklin⁵⁷, S. Franz³⁰, M. Fraternali¹¹⁹ᵃ,¹¹⁹ᵇ, S. Fratina¹²⁰,
S.T. French²⁸, C. Friedrich⁴², F. Friedrich⁴⁴, D. Froidevaux³⁰, J.A. Frost²⁸, C. Fukunaga¹⁵⁶,
E. Fullana Torregrosa¹²⁷, B.G. Fulsom¹⁴³, J. Fuster¹⁶⁷, C. Gabaldon³⁰, O. Gabizon¹⁷², S. Gadatsch¹⁰⁵,
T. Gadfort²⁵, S. Gadomski⁴⁹, G. Gagliardi⁵⁰ᵃ,⁵⁰ᵇ, P. Gagnon⁶⁰, C. Galea⁹⁸, B. Galhardo¹²⁴ᵃ, E.J. Gallas¹¹⁸,
V. Gallo¹⁷, B.J. Gallop¹²⁹, P. Gallus¹²⁶, K.K. Gan¹⁰⁹, Y.S. Gao¹⁴³,ₗ, A. Gaponenko¹⁵, F. Garberson¹⁷⁶,
M. Garcia-Sciveres¹⁵, C. García¹⁶⁷, J.E. García Navarro¹⁶⁷, R.W. Gardner³¹, N. Garelli¹⁴³, V. Garonne³⁰,
C. Gatti⁴⁷, G. Gaudio¹¹⁹ᵃ, B. Gaur¹⁴¹, L. Gauthier¹³⁶, P. Gauzzi¹³²ᵃ,¹³²ᵇ, I.L. Gavrilenko⁹⁴, C. Gay¹⁶⁸,
G. Gaycken²¹, E.N. Gazis¹⁰, P. Ge³³d, Z. Gecse¹⁶⁸, C.N.P. Gee¹²⁹, D.A.A. Geerts¹⁰⁵, Ch. Geich-Gimbel²¹,
K. Gellerstedt¹⁴⁶ᵃ,¹⁴⁶ᵇ, C. Gemme⁵⁰ᵃ, A. Gemmell⁵³, M.H. Genest⁵⁵, S. Gentile¹³²ᵃ,¹³²ᵇ, M. George⁵⁴,
S. George⁷⁶, D. Gerbaudo¹², P. Gerlach¹⁷⁵, A. Gershon¹⁵³, C. Geweniger⁵⁸ᵃ, H. Ghazlane¹³⁵b, N. Ghodbane³⁴,
B. Giacobbe²⁰ᵃ, S. Giagu¹³²ᵃ,¹³²ᵇ, V. Giangiobbe¹², F. Gianotti³⁰, B. Gibbard²⁵, A. Gibson¹⁵⁸, S.M. Gibson³⁰,
M. Gilchriese¹⁵, D. Gillberg³⁰, A.R. Gillman¹²⁹, D.M. Gingrich³,f, J. Ginzburg¹⁵³, N. Giokaris⁹,
M.P. Giordani¹⁶⁴ᶜ, R. Giordano¹⁰²ᵃ,¹⁰²ᵇ, F.M. Giorgi¹⁶, P. Giovannini¹⁹⁹, P.F. Giraud¹³⁶, D. Giugni⁸⁹ᵃ,
M. Giunta⁹³, B.K. Gjelsten¹¹⁷, L.K. Gladilin⁹⁷, C. Glasman⁸⁰, J. Glatzer²¹, A. Glazov⁴², G.L. Glonti⁶⁴,
J.R. Goddard⁷⁵, J. Godfrey¹⁴², J. Godlewski³⁰, M. Goebel⁴², T. Göpfert⁴⁴, C. Goeringer⁸¹, C. Gössling⁴³,
S. Goldfarb⁸⁷, T. Golling¹⁷⁶, D. Golubkov¹²⁸, A. Gomes¹²⁴ᵃ,ᶜ, L.S. Gomez Fajardo⁴², R. Gonçalo⁷⁶,
J. Goncalves Pinto Firmino Da Costa⁴², L. Gonella²¹, S. González de la Hoz¹⁶⁷, G. Gonzalez Parra¹²,
M.L. Gonzalez Silva²⁷, S. Gonzalez-Sevilla⁴⁹, J.J. Goodson¹⁴⁸, L. Goossens³⁰, P.A. Gorbounov⁹⁵, H.A. Gordon²⁵,
I. Gorelov¹⁰³, G. Gorfine¹⁷⁵, B. Gorini³⁰, E. Gorini⁷²ᵃ,⁷²ᵇ, A. Gorišek⁷⁴, E. Gornicki³⁹, A.T. Goshaw⁶,
M. Gosselink¹⁰⁵, M.I. Gostkin⁶⁴, I. Gough Eschrich¹⁶³, M. Gouighri¹³⁵ᵃ, D. Goujdami¹³⁵ᶜ, M.P. Goulette⁴⁹,
A.G. Goussiou¹³⁸, C. Goy⁵, S. Gozpinar²³, I. Grabowska-Bold³⁸, P. Grafström²⁰²ᵃ,²⁰ᵇ, K-J. Grahn⁴²,
E. Gramstad¹¹⁷, F. Grancagnolo⁷²ᵃ, S. Grancagnolo¹⁶, V. Grassi¹⁴⁸, V. Gratchev¹²¹, H.M. Gray³⁰, J.A. Gray¹⁴⁸,
E. Graziani¹³⁴ᵃ, O.G. Grebenyuk¹²¹, T. Greenshaw⁷³, Z.D. Greenwood²⁵,ⁿ, K. Gregersen³⁶, I.M. Gregor⁴²,
P. Grenier¹⁴³, J. Griffiths⁸, N. Grigalashvili⁶⁴, A.A. Grillo¹³⁷, K. Grimm⁷¹, S. Grinstein¹², Ph. Gris³⁴,
Y.V. Grishkevich⁹⁷, J.-F. Grivaz¹¹⁵, A. Grohsjean⁴², E. Gross¹⁷², J. Grosse-Knetter⁵⁴, J. Groth-Jensen¹⁷²,
K. Grybel¹⁴¹, D. Guest¹⁷⁶, C. Guicheney³⁴, E. Guido⁵⁰ᵃ,⁵⁰ᵇ, T. Guillemin¹¹⁵, S. Guindon⁵⁴, U. Gul⁵³,
J. Gunther¹²⁵, B. Guo¹⁵⁸, J. Guo³⁵, P. Gutierrez¹¹¹, N. Guttman¹⁵³, O. Gutzwiller¹⁷³, C. Guyot¹³⁶,
C. Gwenlan¹¹⁸, C.B. Gwilliam⁷³, A. Haas¹⁰⁸, S. Haas³⁰, C. Haber¹⁵, H.K. Hadavand⁸, D.R. Hadley¹⁸,
P. Haefner²¹, F. Hahn³⁰, Z. Hajduk³⁹, H. Hakobyan¹⁷⁷, D. Hall¹¹⁸, G. Halladjian⁶², K. Hamacher¹⁷⁵,
P. Hamal¹¹³, K. Hamano⁸⁶, M. Hamer⁵⁴, A. Hamilton¹⁴⁵b,ₗ, S. Hamilton¹⁶¹, L. Han³³b, K. Hanagaki¹¹⁶,
K. Hanawa¹⁶⁰, M. Hance¹⁵, C. Handel⁸¹, P. Hanke⁵⁸ᵃ, J.R. Hansen³⁶, J.B. Hansen³⁶, J.D. Hansen³⁶,
P.H. Hansen³⁶, P. Hansson¹⁴³, K. Hara¹⁶⁰, T. Harenberg¹⁷⁵, S. Harkusha⁹⁰, D. Harper⁸⁷, R.D. Harrington⁴⁶,
O.M. Harris¹³⁸, J. Hartert⁴⁸, F. Hartjes¹⁰⁵, T. Haruyama⁶⁵, A. Harvey⁵⁶, S. Hasegawa¹⁰¹, Y. Hasegawa¹⁴⁰,
S. Hassani¹³⁶, S. Haug¹⁷, M. Hauschild³⁰, R. Hauser⁸⁸, M. Havranek²¹, C.M. Hawkes¹⁸, R.J. Hawkings³⁰,
A.D. Hawkins⁷⁹, T. Hayakawa⁶⁶, T. Hayashi¹⁶⁰, D. Hayden⁷⁶, C.P. Hays¹¹⁸, H.S. Hayward⁷³, S.J. Haywood¹²⁹,
S.J. Head¹⁸, V. Hedberg⁷⁹, L. Heelan⁸, S. Heim¹²⁰, B. Heinemann¹⁵, S. Heisterkamp³⁶, L. Helary²², C. Heller⁹⁸,
M. Heller³⁰, S. Hellman¹⁴⁶a,¹⁴⁶b, D. Hellmich²¹, C. Helsens¹², R.C.W. Henderson⁷¹, M. Henke⁵⁸a, A. Henrichs¹⁷⁶,
A.M. Henriques Correia³⁰, S. Henrot-Versille¹¹⁵, C. Hensel⁵⁴, C.M. Hernandez⁸, Y. Hernández Jiménez¹⁶⁷,
R. Herrberg¹⁶, G. Herten⁴⁸, R. Hertenberger⁹⁸, L. Hervas³⁰, G.G. Hesketh⁷⁷, N.P. Hessey¹⁰⁵, R. Hickling⁷⁵,
E. Higón-Rodriguez¹⁶⁷, J.C. Hill²⁸, K.H. Hiller⁴², S. Hillert²¹, S.J. Hillier¹⁸, I. Hinchliffe¹⁵, E. Hines¹²⁰,
M. Hirose¹¹⁶, F. Hirsch⁴³, D. Hirschbuehl¹⁷⁵, J. Hobbs¹⁴⁸, N. Hod¹⁵³, M.C. Hodgkinson¹³⁹, P. Hodgson¹³⁹,
A. Hoecker³⁰, M.R. Hoeferkamp¹⁰³, J. Hoffman⁴⁰, D. Hoffmann⁸³, M. Hohlfeld⁸¹, M. Holder¹⁴¹,
S.O. Holmgren¹⁴⁶a, T. Holy¹²⁶, J.L. Holzbauer⁸⁸, T.M. Hong¹²⁰, L. Hooft van Huysduynen¹⁰⁸, S. Horner⁴⁸,
J.-Y. Hostachy⁵⁵, S. Hou¹⁵¹, A. Hoummada¹³⁵a, J. Howard¹¹⁸, J. Howarth⁸², I. Hristova¹⁶, J. Hrivnac¹¹⁵,
T. Hryn'ova⁵, P.J. Hsu⁸¹, S.-C. Hsu¹³⁸, D. Hu³⁵, Z. Hubacek³⁰, F. Hubaut⁸³, F. Huegging²¹, A. Huettmann⁴²,
T.B. Huffman¹¹⁸, E.W. Hughes³⁵, G. Hughes⁷¹, M. Huhtinen³⁰, M. Hurwitz¹⁵, N. Huseynov⁶⁴, r, J. Huston⁸⁸,
J. Huth⁵⁷, G. Iacobucci⁴⁹, G. Iakovidis¹⁰, M. Ibbotson⁸², I. Ibragimov¹⁴¹, L. Iconimidou-Fayard¹¹⁵,
J. Idarraga¹¹⁵, P. Iengo¹⁰²a, O. Igonkina¹⁰⁵, Y. Ikegami⁶⁵, M. Ikeno⁶⁵, D. Iliadis¹⁵⁴, N. Ilic¹⁵⁸, T. Ince⁹⁹,
P. Ioannou⁹, M. Iodice¹³⁴a, K. Iordanidou⁹, V. Ippolito¹³²a,¹³²b, A. Irles Quiles¹⁶⁷, C. Isaksson¹⁶⁶, M. Ishino⁶⁷,
M. Ishitsuka¹⁵⁷, R. Ishmukhametov¹⁰⁹, C. Issever¹¹⁸, S. Istin¹⁹a, A.V. Ivashin¹²⁸, W. Iwanski³⁹, H. Iwasaki⁶⁵,
J.M. Izen⁴¹, V. Izzo¹⁰²a, B. Jackson¹²⁰, J.N. Jackson⁷³, P. Jackson¹, M.R. Jaekel³⁰, V. Jain², K. Jakobs⁴⁸,
S. Jakobsen³⁶, T. Jakoubek¹²⁵, J. Jakubek¹²⁶, D.O. Jamin¹⁵¹, D.K. Jana¹¹¹, E. Jansen⁷⁷, H. Jansen³⁰,
J. Janssen²¹, A. Jantsch⁹⁹, M. Janus⁴⁸, R.C. Jared¹⁷³, G. Jarlskog⁷⁹, L. Jeanty⁵⁷, I. Jen-La Plante³¹,
G.-Y. Jeng¹⁵⁰, D. Jennens⁸⁶, P. Jenni³⁰, A.E. Loevschall-Jensen³⁶, P. Jež³⁶, S. Jézéquel⁵, M.K. Jha²⁰a, H. Ji¹⁷³,
W. Ji⁸¹, J. Jia¹⁴⁸, Y. Jiang³³b, M. Jimenez Belenguer⁴², S. Jin³³a, O. Jinnouchi¹⁵⁷, M.D. Joergensen³⁶,
D. Joffe⁴⁰, M. Johansen¹⁴⁶a,¹⁴⁶b, K.E. Johansson¹⁴⁶a, P. Johansson¹³⁹, S. Johnert⁴², K.A. Johns⁷,
K. Jon-And¹⁴⁶a,¹⁴⁶b, G. Jones¹⁷⁰, R.W.L. Jones⁷¹, T.J. Jones⁷³, C. Joram³⁰, P.M. Jorge¹²⁴a, K.D. Joshi⁸²,
J. Jovicevic¹⁴⁷, T. Jovin¹³b, X. Ju¹⁷³, C.A. Jung⁴³, R.M. Jungst³⁰, V. Juranek¹²⁵, P. Jussel⁶¹, A. Juste Rozas¹²,
S. Kabana¹⁷, M. Kaci¹⁶⁷, A. Kaczmarska³⁹, P. Kadlecik³⁶, M. Kado¹¹⁵, H. Kagan¹⁰⁹, M. Kagan⁵⁷,
E. Kajomovitz¹⁵², S. Kalinin¹⁷⁵, L.V. Kalinovskaya⁶⁴, S. Kama⁴⁰, N. Kanaya¹⁵⁵, M. Kaneda³⁰, S. Kaneti²⁸,
T. Kanno¹⁵⁷, V.A. Kantserov⁹⁶, J. Kanzaki⁶⁵, B. Kaplan¹⁰⁸, A. Kapliy³¹, D. Kar⁵³, M. Karagounis²¹,
K. Karakostas¹⁰, M. Karnevskiy⁵⁸b, V. Kartvelishvili⁷¹, A.N. Karyukhin¹²⁸, L. Kashif¹⁷³, G. Kasieczka⁵⁸b,
R.D. Kass¹⁰⁹, A. Kastanas¹⁴, Y. Kataoka¹⁵⁵, J. Katzy⁴², V. Kaushik⁷, K. Kawagoe⁶⁹, T. Kawamoto¹⁵⁵,
G. Kawamura⁸¹, S. Kazama¹⁵⁵, V.F. Kazanin¹⁰⁷, M.Y. Kazarinov⁶⁴, R. Keeler¹⁶⁹, P.T. Keener¹²⁰, R. Kehoe⁴⁰,
M. Keil⁵⁴, G.D. Kekelidze⁶⁴, J.S. Keller¹³⁸, M. Kenyon⁵³, H. Keoshkerian⁵, O. Kepka¹²⁵, N. Kerschen³⁰,
B.P. Kerševan⁷⁴, S. Kersten¹⁷⁵, K. Kessoku¹⁵⁵, J. Keung¹⁵⁸, F. Khalil-zada¹¹, H. Khandanyan¹⁴⁶a,¹⁴⁶b,
A. Khanov¹¹², D. Kharchenko⁶⁴, A. Khodinov⁹⁶, A. Khomich⁵⁸a, T.J. Khoo²⁸, G. Khoriauli²¹,
A. Khoroshilov¹⁷⁵, V. Khovanskiy⁹⁵, E. Khramov⁶⁴, J. Khubua⁵¹b, H. Kim¹⁴⁶a,¹⁴⁶b, S.H. Kim¹⁶⁰, N. Kimura¹⁷¹,
O. Kind¹⁶, B.T. King⁷³, M. King⁶⁶, R.S.B. King¹¹⁸, J. Kirk¹²⁹, A.E. Kiryunin⁹⁹, T. Kishimoto⁶⁶,
D. Kisielewska³⁸, T. Kitamura⁶⁶, T. Kittelmann¹²³, K. Kiuchi¹⁶⁰, E. Kladiva¹⁴⁴b, M. Klein⁷³, U. Klein⁷³,
K. Kleinknecht⁸¹, M. Klemetti⁸⁵, A. Klier¹⁷², P. Klimek¹⁴⁶a,¹⁴⁶b, A. Klimentov²⁵, R. Klingenberg⁴³,
J.A. Klinger⁸², E.B. Klinkby³⁶, T. Klioutchnikova³⁰, P.F. Klok¹⁰⁴, S. Klous¹⁰⁵, E.-E. Kluge⁵⁸a, T. Kluge⁷³,
P. Kluit¹⁰⁵, S. Kluth⁹⁹, E. Kneringer⁶¹, E.B.F.G. Knoop⁸³, A. Knue⁵⁴, B.R. Ko⁴⁵, T. Kobayashi¹⁵⁵,
M. Kobel⁴⁴, M. Kocian¹⁴³, P. Kodys¹²⁷, K. Köneke³⁰, A.C. König¹⁰⁴, S. Koenig⁸¹, L. Köpke⁸¹, F. Koetsveld¹⁰⁴,
P. Koevesarki²¹, T. Koffas²⁹, E. Koffeman¹⁰⁵, L.A. Kogan¹¹⁸, S. Kohlmann¹⁷⁵, F. Kohn⁵⁴, Z. Kohout¹²⁶,
T. Kohriki⁶⁵, T. Koi¹⁴³, G.M. Kolachev¹⁰⁷,*, H. Kolanoski¹⁶, V. Kolesnikov⁶⁴, I. Koletsou⁸⁹a, J. Koll⁸⁸,
A.A. Komar⁹⁴, Y. Komori¹⁵⁵, T. Kondo⁶⁵, T. Kono⁴², s, A.I. Kononov⁴⁸, R. Konoplich¹⁰⁸, t, N. Konstantinidis⁷⁷,
R. Kopeliansky¹⁵², S. Koperny³⁸, K. Korcyl³⁹, K. Kordas¹⁵⁴, A. Korn⁴⁶, A. Korol¹⁰⁷, I. Korolkov¹²,
E.V. Korolkova¹³⁹, V.A. Korotkov¹²⁸, O. Kortner⁹⁹, S. Kortner⁹⁹, V.V. Kostyukhin²¹, S. Kotov⁹⁹,
V.M. Kotov⁶⁴, A. Kotwal⁴⁵, C. Kourkoumelis⁹, V. Kouskoura¹⁵⁴, A. Koutsman¹⁵⁹a, R. Kowalewski¹⁶⁹,
T.Z. Kowalski³⁸, W. Kozanecki¹³⁶, A.S. Kozhin¹²⁸, V. Kral¹²⁶, V.A. Kramarenko⁹⁷, G. Kramberger⁷⁴,
M.W. Krasny⁷⁸, A. Krasznahorkay¹⁰⁸, J.K. Kraus²¹, A. Kravchenko²⁵, S. Kreiss¹⁰⁸, F. Krejci¹²⁶,
J. Kretzschmar⁷³, K. Kreutzfeldt⁵², N. Krieger⁵⁴, P. Krieger¹⁵⁸, K. Kroeninger⁵⁴, H. Kroha⁹⁹, J. Kroll¹²⁰,
J. Kroseberg²¹, J. Krstic¹³a, U. Kruchonak⁶⁴, H. Krüger²¹, T. Kruker¹⁷, N. Krumnack⁶³, Z.V. Krumshteyn⁶⁴,
M.K. Kruse⁴⁵, T. Kubota⁸⁶, S. Kuday⁴a, S. Kuehn⁴⁸, A. Kugel⁵⁸c, T. Kuhl⁴², V. Kukhtin⁶⁴, Y. Kulchitsky⁹⁰,
S. Kuleshov³²b, M. Kuna⁷⁸, J. Kunkle¹²⁰, A. Kupco¹²⁵, H. Kurashige⁶⁶, M. Kurata¹⁶⁰, Y.A. Kurochkin⁹⁰,
V. Kus¹²⁵, E.S. Kuwertz¹⁴⁷, M. Kuze¹⁵⁷, J. Kvita¹⁴², R. Kwee¹⁶, A. La Rosa⁴⁹, L. La Rotonda³⁷a,³⁷b,
L. Labarga<sup>80</sup>, S. Lablak<sup>135a</sup>, C. Lacasta<sup>167</sup>, F. Lacava<sup>132a,132b</sup>, J. Lacey<sup>29</sup>, H. Lacker<sup>16</sup>, D. Lacour<sup>78</sup>, V.R. Lacuesta<sup>167</sup>, E. Ladygin<sup>64</sup>, R. Lafaye<sup>5</sup>, B. Laforge<sup>78</sup>, T. Lagouri<sup>176</sup>, S. Lai<sup>48</sup>, E. Laisne<sup>55</sup>, L. Lambourne<sup>77</sup>, C.L. Lampen<sup>7</sup>, W. Lampl<sup>7</sup>, E. Lancon<sup>136</sup>, U. Landgraf<sup>48</sup>, M.P.J. Landon<sup>75</sup>, V.S. Lang<sup>58a</sup>, C. Lange<sup>42</sup>, A.J. Lankford<sup>163</sup>, F. Lanni<sup>25</sup>, K. Lantzsch<sup>30</sup>, A. Lanza<sup>119a</sup>, S. Laplace<sup>78</sup>, C. Lapoire<sup>21</sup>, J.F. Laporte<sup>136</sup>, T. Lari<sup>89a</sup>, A. Larner<sup>118</sup>, M. Lassnig<sup>30</sup>, P. Laurelli<sup>47</sup>, V. Lavorini<sup>37a,37b</sup>, W. Lavrijsen<sup>15</sup>, P. Laycock<sup>73</sup>, O. Le Dortz<sup>78</sup>, E. Le Guirriec<sup>83</sup>, E. Le Menedeu<sup>12</sup>, T. LeCompte<sup>6</sup>, F. Ledroit-Guillon<sup>55</sup>, H. Lee<sup>105</sup>, J.S.H. Lee<sup>116</sup>, S.C. Lee<sup>151</sup>, L. Lee<sup>176</sup>, M. Lefebvre<sup>169</sup>, M. Legendre<sup>136</sup>, F. Legger<sup>98</sup>, C. Leggett<sup>15</sup>, M. Lehmacher<sup>21</sup>, G. Lehmann Miotto<sup>30</sup>, A.G. Leister<sup>176</sup>, M.A.L. Leite<sup>24d</sup>, R. Leitner<sup>127</sup>, D. Lellouch<sup>172</sup>, B. Lemmer<sup>54</sup>, V. Lendermann<sup>58a</sup>, K.J.C. Leney<sup>145b</sup>, T. Lenz<sup>105</sup>, G. Lenzen<sup>175</sup>, B. Lenzi<sup>30</sup>, K. Leonhardt<sup>44</sup>, S. Leontsinis<sup>10</sup>, F. Lepold<sup>58a</sup>, C. Leroy<sup>93</sup>, J-R. Lessard<sup>169</sup>, C.G. Lester<sup>28</sup>, C.M. Lester<sup>120</sup>, J. Levêque<sup>5</sup>, D. Levin<sup>87</sup>, L.J. Levinson<sup>172</sup>, A. Lewis<sup>118</sup>, G.H. Lewis<sup>108</sup>, A.M. Leyko<sup>21</sup>, M. Leyton<sup>16</sup>, B. Li<sup>33b</sup>, B. Li<sup>83</sup>, H. Li<sup>148</sup>, H.L. Li<sup>31</sup>, S. Li<sup>33b,u</sup>, X. Li<sup>87</sup>, Z. Liang<sup>118,v</sup>, H. Liao<sup>34</sup>, B. Liberti<sup>133a</sup>, P. Lichard<sup>30</sup>, K. Lie<sup>165</sup>, W. Liebig<sup>14</sup>, C. Limbach<sup>21</sup>, A. Limosani<sup>86</sup>, M. Limper<sup>62</sup>, S.C. Lin<sup>151,w</sup>, F. Linde<sup>105</sup>, J.T. Linnemann<sup>88</sup>, E. Lipeles<sup>120</sup>, A. Lipniacka<sup>14</sup>, T.M. Liss<sup>165</sup>, D. Lissauer<sup>25</sup>, A. Lister<sup>49</sup>, A.M. Litke<sup>137</sup>, D. Liu<sup>151</sup>, J.B. Liu<sup>33b</sup>, L. Liu<sup>87</sup>, M. Liu<sup>33b</sup>, Y. Liu<sup>33b</sup>, M. Livan<sup>119a,119b</sup>, S.S.A. Livermore<sup>118</sup>, A. Lleres<sup>55</sup>, J. Llorente Merino<sup>80</sup>, S.L. Lloyd<sup>75</sup>, E. Lobodzinska<sup>42</sup>, P. Loch<sup>7</sup>, W.S. Lockman<sup>137</sup>, T. Loddenkoetter<sup>21</sup>, F.K. Loebinger<sup>82</sup>, A. Loginov<sup>176</sup>, C.W. Loh<sup>168</sup>, T. Lohse<sup>16</sup>, K. Lohwasser<sup>48</sup>, M. Lokajicek<sup>125</sup>, V.P. Lombardo<sup>5</sup>, R.E. Long<sup>71</sup>, L. Lopes<sup>124a</sup>, D. Lopez Mateos<sup>57</sup>, J. Lorenz<sup>98</sup>, N. Lorenzo Martinez<sup>115</sup>, M. Losada<sup>162</sup>, P. Loscutoff<sup>15</sup>, F. Lo Sterzo<sup>132a,132b</sup>, M.J. Losty<sup>159a,*</sup>, X. Lou<sup>41</sup>, A. Lounis<sup>115</sup>, K.F. Loureiro<sup>162</sup>, J. Love<sup>6</sup>, P.A. Love<sup>71</sup>, A.J. Lowe<sup>143,g</sup>, F. Lu<sup>33a</sup>, H.J. Lubatti<sup>138</sup>, C. Luci<sup>132a,132b</sup>, A. Lucotte<sup>55</sup>, D. Ludwig<sup>42</sup>, I. Ludwig<sup>48</sup>, J. Ludwig<sup>48</sup>, F. Luehring<sup>60</sup>, G. Luijckx<sup>105</sup>, W. Lukas<sup>61</sup>, L. Luminari<sup>132a</sup>, E. Lund<sup>117</sup>, B. Lund-Jensen<sup>147</sup>, B. Lundberg<sup>79</sup>, J. Lundberg<sup>146a,146b</sup>, O. Lundberg<sup>146a,146b</sup>, J. Lundquist<sup>36</sup>, M. Lungwitz<sup>81</sup>, D. Lynn<sup>25</sup>, E. Lytken<sup>79</sup>, H. Ma<sup>25</sup>, L.L. Ma<sup>173</sup>, G. Maccarrone<sup>47</sup>, A. Macchiolo<sup>99</sup>, B. Maček<sup>74</sup>, J. Machado Miguens<sup>124a</sup>, D. Macina<sup>30</sup>, R. Mackeprang<sup>36</sup>, R.J. Madaras<sup>15</sup>, H.J. Maddocks<sup>71</sup>, W.F. Mader<sup>44</sup>, A.K. Madsen<sup>166</sup>, M. Maeno<sup>5</sup>, T. Maeno<sup>25</sup>, P. Mättig<sup>175</sup>, S. Mättig<sup>42</sup>, L. Magnoni<sup>163</sup>, E. Magradze<sup>54</sup>, K. Mahboubi<sup>48</sup>, J. Mahlstedt<sup>105</sup>, S. Mahmoud<sup>73</sup>, G. Mahout<sup>18</sup>, C. Maiani<sup>136</sup>, C. Maidantchik<sup>24a</sup>, A. Maio<sup>124a,c</sup>, S. Majewski<sup>25</sup>, Y. Makida<sup>65</sup>, N. Makovec<sup>115</sup>, P. Mal<sup>136</sup>, B. Malaescu<sup>78</sup>, Pa. Malecki<sup>39</sup>, P. Malecki<sup>39</sup>, V.P. Maleev<sup>121</sup>, F. Malek<sup>55</sup>, U. Mallik<sup>62</sup>, D. Malon<sup>6</sup>, C. Malone<sup>143</sup>, S. Maltezos<sup>10</sup>, V. Malyshev<sup>107</sup>, S. Malyukov<sup>30</sup>, J. Mamuzic<sup>13b</sup>, A. Manabe<sup>65</sup>, L. Mandelli<sup>89a</sup>, I. Mandić<sup>74</sup>, R. Mandrysch<sup>62</sup>, J. Maneira<sup>124a</sup>, A. Manfredini<sup>99</sup>, L. Manhaes de Andrade Filho<sup>24b</sup>, J.A. Manjarres Ramos<sup>136</sup>, A. Mann<sup>98</sup>, P.M. Manning<sup>137</sup>, A. Manousakis-Katsikakis<sup>9</sup>, B. Mansoulie<sup>136</sup>, R. Mantifel<sup>85</sup>, A. Mapelli<sup>30</sup>, L. Mapelli<sup>30</sup>, L. March<sup>167</sup>, J.F. Marchand<sup>29</sup>, F. Marchese<sup>133a,133b</sup>, G. Marchiori<sup>78</sup>, M. Marcisovsky<sup>125</sup>, C.P. Marino<sup>169</sup>, F. Marroquim<sup>24a</sup>, Z. Marshall<sup>30</sup>, L.F. Marti<sup>17</sup>, S. Marti-Garcia<sup>167</sup>, B. Martin<sup>30</sup>, B. Martin<sup>88</sup>, J.P. Martin<sup>93</sup>, T.A. Martin<sup>18</sup>, V.J. Martin<sup>46</sup>, B. Martin dit Latour<sup>49</sup>, S. Martin-Haugh<sup>149</sup>, H. Martinez<sup>136</sup>, M. Martinez<sup>12</sup>, V. Martinez Outschoorn<sup>57</sup>, A.C. Martyniuk<sup>169</sup>, M. Marx<sup>82</sup>, F. Marzano<sup>132a</sup>, A. Marzin<sup>111</sup>, L. Masetti<sup>81</sup>, T. Mashimo<sup>155</sup>, R. Mashinistov<sup>94</sup>, J. Masik<sup>82</sup>, A.L. Maslennikov<sup>107</sup>, I. Massa<sup>20a,20b</sup>, G. Massaro<sup>105</sup>, N. Massol<sup>5</sup>, P. Mastrandrea<sup>148</sup>, A. Mastroberardino<sup>37a,37b</sup>, T. Masubuchi<sup>155</sup>, H. Matsunaga<sup>155</sup>, T. Matsushita<sup>66</sup>, C. Mattravers<sup>118,d</sup>, J. Maurer<sup>83</sup>, S.J. Maxfield<sup>73</sup>, D.A. Maximov<sup>107,h</sup>, R. Mazini<sup>151</sup>, M. Mazur<sup>21</sup>, L. Mazzaferro<sup>133a,133b</sup>, M. Mazzanti<sup>89a</sup>, J. Mc Donald<sup>85</sup>, S.P. Mc Kee<sup>87</sup>, A. McCarn<sup>165</sup>, R.L. McCarthy<sup>148</sup>, T.G. McCarthy<sup>29</sup>, N.A. McCubbin<sup>129</sup>, K.W. McFarlane<sup>56,*</sup>, J.A. Mcfayden<sup>139</sup>, G. Mchedlidze<sup>51b</sup>, T. Mclaughlan<sup>18</sup>, S.J. McMahon<sup>129</sup>, R.A. McPherson<sup>169,l</sup>, A. Meade<sup>84</sup>, J. Mechnich<sup>105</sup>, M. Mechtel<sup>175</sup>, M. Medinnis<sup>42</sup>, S. Meehan<sup>31</sup>, R. Meera-Lebbai<sup>111</sup>, T. Meguro<sup>116</sup>, S. Mehlhase<sup>36</sup>, A. Mehta<sup>73</sup>, K. Meier<sup>58a</sup>, B. Meirose<sup>79</sup>, C. Melachrinos<sup>31</sup>, B.R. Mellado Garcia<sup>173</sup>, F. Meloni<sup>89a,89b</sup>, L. Mendoza Navas<sup>162</sup>, Z. Meng<sup>151,x</sup>, A. Mengarelli<sup>20a,20b</sup>, S. Menke<sup>99</sup>, E. Meoni<sup>161</sup>, K.M. Mercurio<sup>57</sup>, P. Mermod<sup>49</sup>, L. Merola<sup>102a,102b</sup>, C. Meroni<sup>89a</sup>, F.S. Merritt<sup>31</sup>, H. Merritt<sup>109</sup>, A. Messina<sup>30,y</sup>, J. Metcalfe<sup>25</sup>, A.S. Mete<sup>163</sup>, C. Meyer<sup>81</sup>, C. Meyer<sup>31</sup>, J-P. Meyer<sup>136</sup>, J. Meyer<sup>174</sup>, J. Meyer<sup>54</sup>, S. Michal<sup>30</sup>, L. Micu<sup>26a</sup>, R.P. Middleton<sup>129</sup>, S. Migas<sup>73</sup>, L. Mijović<sup>136</sup>, G. Mikenberg<sup>172</sup>, M. Mikestikova<sup>125</sup>, M. Mikuž<sup>74</sup>, D.W. Miller<sup>31</sup>, R.J. Miller<sup>88</sup>, W.J. Mills<sup>168</sup>, C. Mills<sup>57</sup>, A. Milov<sup>172</sup>, D.A. Milstead<sup>146a,146b</sup>, D. Milstein<sup>172</sup>, A.A. Minaenko<sup>128</sup>, M. Miñano Moya<sup>167</sup>, I.A. Minashvili<sup>64</sup>, A.I. Mincer<sup>108</sup>, B. Mindur<sup>38</sup>, M. Mineev<sup>64</sup>, Y. Ming<sup>173</sup>, L.M. Mir<sup>12</sup>, G. Mirabelli<sup>132a</sup>, J. Mitrevski<sup>137</sup>, V.A. Mitsou<sup>167</sup>, S. Mitsui<sup>65</sup>, P.S. Miyagawa<sup>139</sup>, J.U. Mjörnmark<sup>79</sup>, T. Moa<sup>146a,146b</sup>, V. Moeller<sup>28</sup>, K. Mönig<sup>42</sup>, N. Möser<sup>21</sup>, S. Mohapatra<sup>148</sup>, W. Mohr<sup>48</sup>, R. Moles-Valls<sup>167</sup>, A. Molfetas<sup>30</sup>, J. Monk<sup>77</sup>, E. Monnier<sup>83</sup>, J. Montejo Berlingen<sup>12</sup>, F. Monticelli<sup>70</sup>, S. Monzani<sup>20a,20b</sup>, R.W. Moore<sup>3</sup>, G.F. Moorhead<sup>86</sup>, C. Mora Herrera<sup>49</sup>, A. Moraes<sup>53</sup>, N. Morange<sup>136</sup>, J. Morel<sup>54</sup>, G. Morello<sup>37a,37b</sup>, D. Moreno<sup>81</sup>, M. Moreno Llácer<sup>167</sup>, P. Morettini<sup>50a</sup>, M. Morgenstern<sup>44</sup>, M. Morii<sup>57</sup>, A.K. Morley<sup>30</sup>, G. Mornacchi<sup>30</sup>, J.D. Morris<sup>75</sup>, L. Morvaj<sup>101</sup>, H.G. Moser<sup>99</sup>,
M. Mosidze⁵¹b, J. Moss¹⁰⁹, R. Mount¹⁴³, E. Mountricha¹⁰,z, S.V. Mouraviev⁹⁴,*, E.J.W. Moyse⁸⁴, F. Mueller⁵⁸a,
J. Mueller¹²³, K. Mueller²¹, T.A. Müller⁹⁸, T. Mueller⁸¹, D. Muenstermann³⁰, Y. Munwes¹⁵³, W.J. Murray¹²⁹,
I. Mussche¹⁰⁵, E. Musto¹⁵², A.G. Myagkov¹²⁸, M. Myska¹²⁵, O. Nackenhorst⁵⁴, J. Nadal¹², K. Nagai¹⁶⁰,
R. Nagai¹⁵⁷, K. Nagano⁶⁵, A. Nagarkar¹⁰⁹, Y. Nagasaka⁵⁹, M. Nagel⁹⁹, A.M. Nairz³⁰, Y. Nakahama³⁰,
K. Nakamura⁶⁵, T. Nakamura¹⁵⁵, I. Nakano¹¹⁰, G. Nanava²¹, A. Napier¹⁶¹, R. Narayan⁵⁸b, M. Nash⁷⁷,d,
T. Nattermann²¹, T. Naumann⁴², G. Navarro¹⁶², H.A. Neal⁸⁷, P.Yu. Nechaeva⁹⁴, T.J. Neep⁸², A. Negri¹¹⁹a,¹¹⁹b,
G. Negri³⁰, M. Negrini²⁰a, S. Nektarijevic⁴⁹, A. Nelson¹⁶³, T.K. Nelson¹⁴³, S. Nemecek¹²⁵, P. Nemethy¹⁰⁸,
A.A. Nepomuceno²⁴a, M. Nessi³⁰,aa, M.S. Neubauer¹⁶⁵, M. Neumann¹⁷⁵, A. Neusiedl⁸¹, R.M. Neves¹⁰⁸,
P. Nevski²⁵, F.M. Newcomer¹²⁰, P.R. Newman¹⁸, V. Nguyen Thi Hong¹³⁶, R.B. Nickerson¹¹⁸, R. Nicolaidou¹³⁶,
B. Nicquevert³⁰, F. Niedercorn¹¹⁵, J. Nielsen¹³⁷, N. Nikiforou³⁵, A. Nikiforov¹⁶, V. Nikolaenko¹²⁸,
I. Nikolic-Audit⁷⁸, K. Nikolics⁴⁹, K. Nikolopoulos¹⁸, H. Nilsen⁴⁸, P. Nilsson⁸, Y. Ninomiya¹⁵⁵, A. Nisati¹³²a,
R. Nisius⁹⁹, T. Nobe¹⁵⁷, L. Nodulman⁶, M. Nomachi¹¹⁶, I. Nomidis¹⁵⁴, S. Norberg¹¹¹, M. Nordberg³⁰,
J. Novakova¹²⁷, M. Nozaki⁶⁵, L. Nozka¹¹³, A.-E. Nuncio-Quiroz²¹, G. Nunes Hanninger⁸⁶, T. Nunnemann⁹⁸,
E. Nurse⁷⁷, B.J. O'Brien⁴⁶, D.C. O'Neil¹⁴², V. O'Shea⁵³, L.B. Oakes⁹⁸, F.G. Oakham²⁹,f, H. Oberlack⁹⁹,
J. Ocariz⁷⁸, A. Ochi⁶⁶, S. Oda⁶⁹, S. Odaka⁶⁵, J. Odier⁸³, H. Ogren⁶⁰, A. Oh⁸², S.H. Oh⁴⁵, C.C. Ohm³⁰,
T. Ohshima¹⁰¹, W. Okamura¹¹⁶, H. Okawa²⁵, Y. Okumura³¹, T. Okuyama¹⁵⁵, A. Olariu²⁶a, A.G. Olchevski⁶⁴,
S.A. Olivares Pino³²a, M. Oliveira¹²⁴a,i, D. Oliveira Damazio²⁵, E. Oliver Garcia¹⁶⁷, D. Olivito¹²⁰,
A. Olszewski³⁹, J. Olszowska³⁹, A. Onofre¹²⁴a,ab, P.U.E. Onyisi³¹,ac, C.J. Oram¹⁵⁹a, M.J. Oreglia³¹, Y. Oren¹⁵³,
D. Orestano¹³⁴a,¹³⁴b, N. Orlando⁷²a,⁷²b, C. Oropeza Barrera⁵³, R.S. Orr¹⁵⁸, B. Osculati⁵⁰a,⁵⁰b, R. Ospanov¹²⁰,
C. Osuna¹², G. Otero y Garzon²⁷, J.P. Ottersbach¹⁰⁵, M. Ouchrif¹³⁵d, E.A. Ouellette¹⁶⁹, F. Ould-Saada¹¹⁷,
A. Ouraou¹³⁶, Q. Ouyang³³a, A. Ovcharova¹⁵, M. Owen⁸², S. Owen¹³⁹, V.E. Ozcan¹⁹a, N. Ozturk⁸,
A. Pacheco Pages¹², C. Padilla Aranda¹², S. Pagan Griso¹⁵, E. Paganis¹³⁹, C. Pahl⁹⁹, F. Paige²⁵, P. Pais⁸⁴,
K. Pajchel¹¹⁷, G. Palacino¹⁵⁹b, C.P. Paleari⁷, S. Palestini³⁰, D. Pallin³⁴, A. Palma¹²⁴a, J.D. Palmer¹⁸,
Y.B. Pan¹⁷³, E. Panagiotopoulou¹⁰, J.G. Panduro Vazquez⁷⁶, P. Pani¹⁰⁵, N. Panikashvili⁸⁷, S. Panitkin²⁵,
D. Pantea²⁶a, A. Papadelis¹⁴⁶a, Th.D. Papadopoulou¹⁰, A. Paramonov⁶, D. Paredes Hernandez³⁴, W. Park²⁵,ad,
M.A. Parker²⁸, F. Parodi⁵⁰a,⁵⁰b, J.A. Parsons³⁵, U. Parzefall⁴⁸, S. Pashapour⁵⁴, E. Pasqualucci¹³²a,
S. Passaggio⁵⁰a, A. Passeri¹³⁴a, F. Pastore¹³⁴a,¹³⁴b,*, Fr. Pastore⁷⁶, G. Pásztor⁴⁹,ae, S. Pataraia¹⁷⁵,
N.D. Patel¹⁵⁰, J.R. Pater⁸², S. Patricelli¹⁰²a,¹⁰²b, T. Pauly³⁰, S. Pedraza Lopez¹⁶⁷, M.I. Pedraza Morales¹⁷³,
S.V. Peleganchuk¹⁰⁷, D. Pelikan¹⁶⁶, H. Peng³³b, B. Penning³¹, A. Penson³⁵, J. Penwell⁶⁰, M. Perantoni²⁴a,
K. Perez³⁵,af, T. Perez Cavalcanti⁴², E. Perez Codina¹⁵⁹a, M.T. Pérez García-Estañ¹⁶⁷, V. Perez Reale³⁵,
L. Perini⁸⁹a,⁸⁹b, H. Pernegger³⁰, R. Perrino⁷²a, P. Perrodo⁵, V.D. Peshekhonov⁶⁴, K. Peters³⁰, B.A. Petersen³⁰,
J. Petersen³⁰, T.C. Petersen³⁶, E. Petit⁵, A. Petridis¹⁵⁴, C. Petridou¹⁵⁴, E. Petrolο¹³²a, F. Petrucci¹³⁴a,¹³⁴b,
D. Petschull⁴², M. Petteni¹⁴², R. Pezoa³²b, A. Phan⁸⁶, P.W. Phillips¹²⁹, G. Piacquadio³⁰, A. Picazio⁴⁹,
E. Piccaro⁷⁵, M. Piccinini²⁰a,²⁰b, S.M. Piec⁴², R. Piegaia²⁷, D.T. Pignotti¹⁰⁹, J.E. Pilcher³¹, A.D. Pilkington⁸²,
J. Pina¹²⁴a,c, M. Pinamonti¹⁶⁴a,¹⁶⁴c, A. Pinder¹¹⁸, J.L. Pinfold³, A. Pingel³⁶, B. Pinto¹²⁴a, C. Pizio⁸⁹a,⁸⁹b,
M.-A. Pleier²⁵, E. Plotnikova⁶⁴, A. Poblaguev²⁵, S. Poddar⁵⁸a, F. Podlyski³⁴, L. Poggioli¹¹⁵, D. Pohl²¹,
M. Pohl⁴⁹, G. Polesello¹¹⁹a, A. Policicchio³⁷a,³⁷b, R. Polifka¹⁵⁸, A. Polini²⁰a, J. Poll⁷⁵, V. Polychronakos²⁵,
D. Pomeroy²³, K. Pommès³⁰, L. Pontecorvo¹³²a, B.G. Pope⁸⁸, G.A. Popeneciu²⁶a, D.S. Popovic¹³a,
A. Poppleton³⁰, X. Portell Bueso³⁰, G.E. Pospelov⁹⁹, S. Pospisil¹²⁶, I.N. Potrap⁹⁹, C.J. Potter¹⁴⁹, C.T. Potter¹¹⁴,
G. Poulard³⁰, J. Poveda⁶⁰, V. Pozdnyakov⁶⁴, R. Prabhu⁷⁷, P. Pralavorio⁸³, A. Pranko¹⁵, S. Prasad³⁰,
R. Pravahan²⁵, S. Prell⁶³, K. Pretzl¹⁷, D. Price⁶⁰, J. Price⁷³, L.E. Price⁶, D. Prieur¹²³, M. Primavera⁷²a,
K. Prokofiev¹⁰⁸, F. Prokoshin³²b, S. Protopopescu²⁵, J. Proudfoot⁶, X. Prudent⁴⁴, M. Przybycien³⁸,
H. Przysiezniak⁵, S. Psoroulas²¹, E. Ptacek¹¹⁴, E. Pueschel⁸⁴, D. Puldon¹⁴⁸, J. Purdham⁸⁷, M. Purohit²⁵,ad,
P. Puzo¹¹⁵, Y. Pylypchenko⁶², J. Qian⁸⁷, A. Quadt⁵⁴, D.R. Quarrie¹⁵, W.B. Quayle¹⁷³, M. Raas¹⁰⁴, V. Radeka²⁵,
V. Radescu⁴², P. Radloff¹¹⁴, F. Ragusa⁸⁹a,⁸⁹b, G. Rahal¹⁷⁸, A.M. Rahimi¹⁰⁹, D. Rahm²⁵, S. Rajagopalan²⁵,
M. Rammensee⁴⁸, M. Rammes¹⁴¹, A.S. Randle-Conde⁴⁰, K. Randrianarivony²⁹, K. Rao¹⁶³, F. Rauscher⁹⁸,
T.C. Rave⁴⁸, M. Raymond³⁰, A.L. Read¹¹⁷, D.M. Rebuzzi¹¹⁹a,¹¹⁹b, A. Redelbach¹⁷⁴, G. Redlinger²⁵, R. Reece¹²⁰,
K. Reeves⁴¹, A. Reinsch¹¹⁴, I. Reisinger⁴³, C. Rembser³⁰, Z.L. Ren¹⁵¹, A. Renaud¹¹⁵, M. Rescigno¹³²a,
S. Resconi⁸⁹a, B. Resende¹³⁶, P. Reznicek⁹⁸, R. Rezvani¹⁵⁸, R. Richter⁹⁹, E. Richter-Was⁵,ag, M. Ridel⁷⁸,
M. Rijssenbeek¹⁴⁸, A. Rimoldi¹¹⁹a,¹¹⁹b, L. Rinaldi²⁰a, R.R. Rios⁴⁰, E. Ritsch⁶¹, I. Riu¹², G. Rivoltella⁸⁹a,⁸⁹b,
F. Rizatdinova¹¹², E. Rizvi⁷⁵, S.H. Robertson⁸⁵,l, A. Robichaud-Veronneau¹¹⁸, D. Robinson²⁸,
J.E.M. Robinson⁸², A. Robson⁵³, J.G. Rocha de Lima¹⁰⁶, C. Roda¹²²a,¹²²b, D. Roda Dos Santos³⁰, A. Roe⁵⁴,
S. Roe³⁰, O. Røhne¹¹⁷, S. Rolli¹⁶¹, A. Romaniouk⁹⁶, M. Romano²⁰a,²⁰b, G. Romeo²⁷, E. Romero Adam¹⁶⁷,
N. Rompotis¹³⁸, L. Roos⁷⁸, E. Ros¹⁶⁷, S. Rosati¹³²a, K. Rosbach⁴⁹, A. Rose¹⁴⁹, M. Rose⁷⁶, G.A. Rosenbaum¹⁵⁸, P.L. Rosendahl¹⁴, O. Rosenthal¹⁴¹, L. Rosselet⁴⁹, V. Rossetti¹², E. Rossi¹³²a,¹³²b, L.P. Rossi⁵⁰a, M. Rotaru²⁶a, I. Roth¹⁷², J. Rothberg¹³⁸, D. Rousseau¹¹⁵, C.R. Royon¹³⁶, A. Rozanov⁸³, Y. Rozen¹⁵², X. Ruan³³a,ah, F. Rubbo¹², I. Rubinskiy⁴², N. Ruckstuhl¹⁰⁵, V.I. Rud⁹⁷, C. Rudolph⁴⁴, M.S. Rudolph¹⁵⁸, F. Rühr⁷, A. Ruiz-Martinez⁶³, L. Rumyantsev⁶⁴, Z. Rurikova⁴⁸, N.A. Rusakovitch⁶⁴, A. Ruschke⁹⁸, J.P. Rutherford⁷, N. Ruthmann⁴⁸, P. Ruzicka¹²⁵, Y.F. Ryabov¹²¹, M. Rybar¹²⁷, G. Rybkin¹¹⁵, N.C. Ryder¹¹⁸, A.F. Saavedra¹⁵⁰, I. Sadeh¹⁵³, H.F.-W. Sadrozinski¹³⁷, R. Sadykov⁶⁴, F. Safai Tehran¹³²a, H. Sakamoto¹⁵⁵, G. Salamanna⁷⁵, A. Salamon¹³³a, M. Saleem¹¹¹, D. Salek³⁰, D. Salihagic⁹⁹, A. Salnikov¹⁴³, J. Salt¹⁶⁷, B.M. Salvachua Ferrando⁶, D. Salvatore³⁷a,³⁷b, F. Salvatore¹⁴⁹, A. Salvucci¹⁰⁴, A. Salzburger³⁰, D. Sampsonidis¹⁵⁴, B.H. Samset¹¹⁷, A. Sanchez¹⁰²a,¹⁰²b, V. Sanchez Martinez¹⁶⁷, H. Sandaker¹⁴, H.G. Sander⁸¹, M.P. Sanders⁹⁸, M. Sandhoff¹⁷⁵, T. Sandoval²⁸, C. Sandoval¹⁶², R. Sandstroem⁹⁹, D.P.C. Sankey¹²⁹, A. Sansoni⁴⁷, C. Santamarina Rios⁸⁵, C. Santoni³⁴, R. Santonico¹³³a,¹³³b, H. Santos¹²⁴a, I. Santoyo Castillo¹⁴⁹, J.G. Saraiva¹²⁴a, T. Sarangi¹⁷³, E. Sarkisyan-Grinbaum⁸, B. Sarrazin²¹, F. Sarri¹²²a,¹²²b, G. Sartisohn¹⁷⁵, O. Sasaki⁶⁵, Y. Sasaki¹⁵⁵, N. Sasao⁶⁷, I. Satsounkevitch⁹⁰, G. Sauvage⁵,*, E. Sauvan⁵, J.B. Sauvan¹¹⁵, P. Savard¹⁵⁸,f, V. Savinov¹²³, D.O. Savu³⁰, L. Sawyer²⁵,n, D.H. Saxon⁵³, J. Saxon¹²⁰, C. Sbarra²⁰a, A. Sbrizzi²⁰a,²⁰b, D.A. Scannicchio¹⁶³, M. Scarcella¹⁵⁰, J. Schaarschmidt¹¹⁵, P. Schacht⁹⁹, D. Schaefer¹²⁰, U. Schäfer⁸¹, A. Schaelicke⁴⁶, S. Schaepe²¹, S. Schaetzel⁵⁸b, A.C. Schaffer¹¹⁵, D. Schaile⁹⁸, R.D. Schamberger¹⁴⁸, V. Scharf⁵⁸a, V.A. Schegelsky¹²¹, D. Scheirich⁸⁷, M. Schernau¹⁶³, M.I. Scherzer³⁵, C. Schiavi⁵⁰a,⁵⁰b, J. Schieck⁹⁸, M. Schioppa³⁷a,³⁷b, S. Schlenker³⁰, E. Schmidt⁴⁸, K. Schmieden²¹, C. Schmitt⁸¹, S. Schmitt⁵⁸b, B. Schneider¹⁷, U. Schnoor⁴⁴, L. Schoeffel¹³⁶, A. Schoening⁵⁸b, A.L.S. Schorlemmer⁵⁴, M. Schott⁸¹, D. Schouten¹⁵⁹a, J. Schovancova¹²⁵, M. Schram⁸⁵, C. Schroeder⁸¹, N. Schroer⁵⁸c, M.J. Schultens²¹, J. Schultes¹⁷⁵, H.-C. Schultz-Coulon⁵⁸a, H. Schulz¹⁶, M. Schumacher⁴⁸, B.A. Schumm¹³⁷, Ph. Schune¹³⁶, A. Schwartzman¹⁴³, Ph. Schwegler⁹⁹, Ph. Schwemling⁷⁸, R. Schwienhorst⁸⁸, J. Schwindling¹³⁶, T. Schwindt²¹, M. Schwoerer⁵, F.G. Sciacca¹⁷, E. Scifo¹¹⁵, G. Sciolla²³, W.G. Scott¹²⁹, J. Searcy¹¹⁴, G. Sedov⁴², E. Sedykh¹²¹, S.C. Seidel¹⁰³, A. Seiden¹³⁷, F. Seifert⁴⁴, J.M. Seixas²⁴a, G. Sekhniaidze¹⁰²a, S.J. Sekula⁴⁰, K.E. Selbach⁴⁶, D.M. Seliverstov¹²¹, B. Sellden¹⁴⁶a, G. Sellers⁷³, M. Seman¹⁴⁴b, N. Semprini-Cesari²⁰a,²⁰b, C. Serfon³⁰, L. Serin¹¹⁵, L. Serkin⁵⁴, R. Seuster¹⁵⁹a, H. Severini¹¹¹, A. Sfyrla³⁰, E. Shabalina⁵⁴, M. Shamim¹¹⁴, L.Y. Shan³³a, J.T. Shank²², Q.T. Shao⁸⁶, M. Shapiro¹⁵, P.B. Shatalov⁹⁵, K. Shaw¹⁶⁴a,¹⁶⁴c, D. Sherman¹⁷⁶, P. Sherwood⁷⁷, S. Shimizu¹⁰¹, M. Shimojima¹⁰⁰, T. Shin⁵⁶, M. Shiyakova⁶⁴, A. Shmeleva⁹⁴, M.J. Shochet³¹, D. Short¹¹⁸, S. Shrestha⁶³, E. Shulga⁹⁶, M.A. Shupe⁷, P. Sicho¹²⁵, A. Sidoti¹³²a, F. Siegert⁴⁸, Dj. Sijacki¹³a, O. Silbert¹⁷², J. Silva¹²⁴a, Y. Silver¹⁵³, D. Silverstein¹⁴³, S.B. Silverstein¹⁴⁶a, V. Simak¹²⁶, O. Simard¹³⁶, Lj. Simic¹³a, S. Simion¹¹⁵, E. Simioni⁸¹, B. Simmons⁷⁷, R. Simoniello⁸⁹a,⁹⁹b, M. Simonyan³⁶, P. Sinervo¹⁵⁸, N.B. Sinev¹¹⁴, V. Sipica¹⁴¹, G. Siragusa¹⁷⁴, A. Sircar²⁵, A.N. Sisakyan⁶⁴,*, S.Yu. Sivoklokov⁹⁷, J. Sjölin¹⁴⁶a,¹⁴⁶b, T.B. Sjursen¹⁴, L.A. Skinnari¹⁵, H.P. Skottowe⁵⁷, K. Skovpen¹⁰⁷, P. Skubic¹¹¹, M. Slater¹⁸, T. Slavicek¹²⁶, K. Sliwa¹⁶¹, V. Smakhtin¹⁷², B.H. Smart⁴⁶, L. Smestad¹¹⁷, S.Yu. Smirnov⁹⁶, Y. Smirnov⁹⁶, L.N. Smirnova⁹⁷,ai, O. Smirnova⁷⁹, B.C. Smith⁵⁷, K.M. Smith⁵³, M. Smizanska⁷¹, K. Smolek¹²⁶, A.A. Snesarev⁹⁴, G. Snidero⁷⁵, S.W. Snow⁸², J. Snow¹¹¹, S. Snyder²⁵, R. Sobie¹⁶⁹,l, J. Sodomka¹²⁶, A. Soffer¹⁵³, C.A. Solans³⁰, M. Solar¹²⁶, J. Solc¹²⁶, E.Yu. Soldatov⁹⁶, U. Soldevila¹⁶⁷, E. Solfaroli Camillocci¹³²a,¹³²b, A.A. Solodkov¹²⁸, O.V. Solovyev¹²⁸, V. Solovyev¹²¹, N. Soni¹, A. Sood¹⁵, V. Sopko¹²⁶, B. Sopko¹²⁶, M. Sosebee⁸, R. Soualah¹⁶⁴a,¹⁶⁴c, P. Soueid⁹³, A. Soukharev¹⁰⁷, D. South⁴², S. Spagnolo⁷²a,⁷²b, F. Spano⁷⁶, R. Spighi²⁰a, G. Spigo³⁰, R. Spiwoks³⁰, M. Spousta¹²⁷,aj, T. Spreitzer¹⁵⁸, B. Spurlock⁸, R.D. St. Denis⁵³, J. Stahlman¹²⁰, R. Stamen⁵⁸a, E. Stanecka³⁹, R.W. Stanek⁶, C. Stanescu¹³⁴a, M. Stanescu-Bellu⁴², M.M. Stanitzki⁴², S. Stapnes¹¹⁷, E.A. Starchenko¹²⁸, J. Stark⁵⁵, P. Staroba¹²⁵, P. Starovoitov⁴², R. Staszewski³⁹, A. Staude⁹⁸, P. Stavina¹⁴⁴a,*, G. Steele⁵³, P. Steinbach⁴⁴, P. Steinberg²⁵, I. Stekl¹²⁶, B. Stelzer¹⁴², H.J. Stelzer⁸⁸, O. Stelzer-Chilton¹⁵⁹a, H. Stenzel⁵², S. Stern⁹⁹, G.A. Stewart³⁰, J.A. Stillings²¹, M.C. Stockton⁸⁵, M. Stoebe⁸⁵, K. Stoerig⁴⁸, G. Stoicea²⁶a, S. Stonjek⁹⁹, P. Strachota¹²⁷, A.R. Stradling⁸, A. Straessner⁴⁴, J. Strandberg¹⁴⁷, S. Strandberg¹⁴⁶a,¹⁴⁶b, A. Strandlie¹¹⁷, M. Strang¹⁰⁹, E. Strauss¹⁴³, M. Strauss¹¹¹, P. Strizenec¹⁴⁴b, R. Ströhmer¹⁷⁴, D.M. Strom¹¹⁴, J.A. Strong⁷⁶,*, R. Stroynowski⁴⁰, B. Stugu¹⁴, I. Stumer²⁵,*, J. Stupak¹⁴⁸, P. Sturm¹⁷⁵, N.A. Styles⁴², D.A. Soh¹⁵¹,v, D. Su¹⁴³, HS. Subramania³, R. Subramaniam²⁵, A. Succurro¹², Y. Sugaya¹¹⁶, C. Suhr¹⁰⁶, M. Suk¹²⁷, V.V. Sulin⁹⁴, S. Sultansoy⁴d, T. Sumida⁶⁷, X. Sun⁵⁵, J.E. Sundermann⁴⁸, K. Suruliz¹³⁹, G. Susinno³⁷a,³⁷b, M.R. Sutton¹⁴⁹, Y. Suzuki⁶⁵, Y. Suzuki⁶⁶, M. Svatos¹²⁵, S. Swedish¹⁶⁸, I. Sykora¹⁴⁴a, T. Sykora¹²⁷, J. Sánchez¹⁶⁷, D. Ta¹⁰⁵, K. Tackmann⁴², A. Taffard¹⁶³, R. Tafirout¹⁵⁹a, N. Taiblum¹⁵³, Y. Takahashi¹⁰¹, H. Takai²⁵, R. Takashima⁶⁸, H. Takeda⁶⁶, T. Takeshita¹⁴⁰, Y. Takubo⁶⁵, M. Talby⁸³, A. Talyshev¹⁰⁷,h, M.C. Tamsett²⁵, K.G. Tan⁸⁶, J. Tanaka¹⁵⁵,
R. Tanaka¹¹⁵, S. Tanaka¹³¹, S. Tanaka⁶⁵, A.J. Tanasijczuk¹⁴², K. Tani⁶⁶, N. Tannoury⁸³, S. Tapprogge⁸¹,
D. Tardif¹⁵⁸, S. Tarem¹⁵², F. Tarrade²⁹, G.F. Tartarelli⁸⁹ª, P. Tas¹²⁷, M. Tasevsky¹²⁵, E. Tassi³⁷a,³⁷b,
Y. Tayalati¹³⁵d, C. Taylor⁷⁷, F.E. Taylor⁹², G.N. Taylor⁸⁶, W. Taylor¹⁵⁹b, M. Teinturier¹¹⁵, F.A. Teischinger³⁰,
M. Teixeira Dias Castanheira⁷⁵, P. Teixeira-Dias⁷⁶, K.K. Temming⁴⁸, H. Ten Kate³⁰, P.K. Teng¹⁵¹, S. Terada⁶⁵,
K. Terashi¹⁵⁵, J. Terron⁸⁰, M. Testa⁴⁷, R.J. Teuscher¹⁵⁸,¹, J. Therhaag²¹, T. Theveneaux-Pelzer⁷⁸, S. Thoma⁴⁸,
J.P. Thomas¹⁸, E.N. Thompson³⁵, P.D. Thompson¹⁸, P.D. Thompson¹⁵⁸, A.S. Thompson⁵³, L.A. Thomsen³⁶,
E. Thomson¹²⁰, M. Thomson²⁸, W.M. Thong⁸⁶, R.P. Thun⁸⁷, F. Tian³⁵, M.J. Tibbetts¹⁵, T. Tic¹²⁵,
V.O. Tikhomirov⁹⁴, Y.A. Tikhonov¹⁰⁷,¹h, S. Timoshenko⁹⁶, E. Tiouchichine⁸³, P. Tipton¹⁷⁶, S. Tisserant⁸³,
T. Todorov⁵, S. Todorova-Nova¹⁶¹, B. Toggerson¹⁶³, J. Tojo⁶⁹, S. Tokár¹⁴⁴a, K. Tokushuku⁶⁵, K. Tollefson⁸⁸,
M. Tomoto¹⁰¹, L. Tompkins³¹, K. Toms¹⁰³, A. Tonoyan¹⁴, C. Topfel¹⁷, N.D. Topilin⁶⁴, E. Torrence¹¹⁴,
H. Torres⁷⁸, E. Torró Pastor¹⁶⁷, J. Toth⁸³,⁶e, F. Touchard⁸³, D.R. Tovey¹³⁹, T. Trefzger¹⁷⁴, L. Tremblet³⁰,
A. Tricoli³⁰, I.M. Trigger¹⁵⁹a, S. Trincaz-Duvoid⁷⁸, M.F. Tripiana⁷⁰, N. Triplett²⁵, W. Trischuk¹⁵⁸, B. Trocmé⁵⁵,
C. Troncon⁸⁹a, M. Trottier-McDonald¹⁴², P. True⁸⁸, M. Trzebinski³⁹, A. Trzupek³⁹, C. Tsarouchas³⁰,
J.C.-L. Tseng¹¹⁸, M. Tsiakiris¹⁰⁵, P.V. Tsiareshka⁹⁰, D. Tsionou⁵,ak, G. Tsipolitis¹⁰, S. Tsiskaridze¹²,
V. Tsiskaridze⁴⁸, E.G. Tskhadadze⁵¹a, I.I. Tsukerman⁹⁵, V. Tsulaia¹⁵, J.-W. Tsung²¹, S. Tsuno⁶⁵,
D. Tsybychev¹⁴⁸, A. Tua¹³⁹, A. Tudorache²⁶a, V. Tudorache²⁶a, J.M. Tuggle³¹, M. Turala³⁹, D. Turecek¹²⁶,
I. Turk Cakir⁴e, R. Turra⁸⁹a,⁸⁹b, P.M. Tuts³⁵, A. Tykhonov⁷⁴, M. Tylmad¹⁴⁶a,¹⁴⁶b, M. Tyndel¹²⁹, G. Tzanakos⁹,
K. Uchida²¹, I. Ueda¹⁵⁵, R. Ueno²⁹, M. Ughetto⁸³, M. Ugland¹⁴, M. Uhlenbrock²¹, F. Ukegawa¹⁶⁰, G. Unal³⁰,
A. Undrus²⁵, G. Unel¹⁶³, F.C. Ungaro⁴⁸, Y. Unno⁶⁵, D. Urbaniec³⁵, P. Urquijo²¹, G. Usai⁸, L. Vacavant⁸³,
V. Vacek¹²⁶, B. Vachon⁸⁵, S. Vahsen¹⁵, S. Valentinetti²⁰a,²⁰b, A. Valero¹⁶⁷, L. Valery³⁴, S. Valkar¹²⁷,
E. Valladolid Gallego¹⁶⁷, S. Vallecorsa¹⁵², J.A. Valls Ferrer¹⁶⁷, R. Van Berg¹²⁰, P.C. Van Der Deijl¹⁰⁵,
R. van der Geer¹⁰⁵, H. van der Graaf¹⁰⁵, R. Van Der Leeuw¹⁰⁵, E. van der Poel¹⁰⁵, D. van der Ster³⁰,
N. van Eldik³⁰, P. van Gemmeren⁶, J. Van Nieuwkoop¹⁴², I. van Vulpen¹⁰⁵, M. Vanadia⁹⁹, W. Vandelli³⁰,
A. Vaniachine⁶, P. Vankov⁴², F. Vannucci⁷⁸, R. Vari¹³²a, E.W. Varnes⁷, T. Varol⁸⁴, D. Varouchas¹⁵,
A. Vartapetian⁸, K.E. Varvell¹⁵⁰, V.I. Vassilakopoulos⁵⁶, F. Vazeille³⁴, T. Vazquez Schroeder⁵⁴, G. Vegni⁸⁹a,⁸⁹b,
J.J. Veillet¹¹⁵, F. Veloso¹²⁴a, R. Veness³⁰, S. Veneziano¹³²a, A. Ventura⁷²a,⁷²b, D. Ventura⁸⁴, M. Venturi⁴⁸,
N. Venturi¹⁵⁸, V. Vercesi¹¹⁹a, M. Verducci¹³⁸, W. Verkerke¹⁰⁵, J.C. Vermeulen¹⁰⁵, A. Vest⁴⁴, M.C. Vetterli¹⁴², f,
I. Vichou¹⁶⁵, T. Vickey¹⁴⁵b,al, O.E. Vickey Boeriu¹⁴⁵b, G.H.A. Viehhauser¹¹⁸, S. Viel¹⁶⁸, M. Villa²⁰a,²⁰b,
M. Villaplana Perez¹⁶⁷, E. Vilucchi⁴⁷, M.G. Vincter²⁹, E. Vinek³⁰, V.B. Vinogradov⁶⁴, M. Virchaux¹³⁶,*,
J. Virzi¹⁵, O. Vitells¹⁷², M. Viti⁴², I. Vivarelli⁴⁸, F. Vives Vaque³, S. Vlachos¹⁰, D. Vladoiu⁹⁸, M. Vlasak¹²⁶,
A. Vogel²¹, P. Vokac¹²⁶, G. Volpi⁴⁷, M. Volpi⁸⁶, G. Volpini⁸⁹a, H. von der Schmitt⁹⁹, H. von Radziewski⁴⁸,
E. von Toerne²¹, V. Vorobel¹²⁷, V. Vorwerk¹², M. Vos¹⁶⁷, R. Voss³⁰, J.H. Vossebeld⁷³, N. Vranjes¹³⁶,
M. Vranjes Milosavljevic¹⁰⁵, V. Vrba¹²⁵, M. Vreeswijk¹⁰⁵, T. Vu Anh⁴⁸, R. Vuillermet³⁰, I. Vukotic³¹,
W. Wagner¹⁷⁵, P. Wagner²¹, H. Wahlen¹⁷⁵, S. Wahrmund⁴⁴, J. Wakabayashi¹⁰¹, S. Walch⁸⁷, J. Walder⁷¹,
R. Walker⁹⁸, W. Walkowiak¹⁴¹, R. Wall¹⁷⁶, P. Waller⁷³, B. Walsh¹⁷⁶, C. Wang⁴⁵, H. Wang¹⁷³, H. Wang⁴⁰,
J. Wang¹⁵¹, J. Wang³³a, R. Wang¹⁰³, S.M. Wang¹⁵¹, T. Wang²¹, A. Warburton⁸⁵, C.P. Ward²⁸,
D.R. Wardrope⁷⁷, M. Warsinsky⁴⁸, A. Washbrook⁴⁶, C. Wasicki⁴², I. Watanabe⁶⁶, P.M. Watkins¹⁸,
A.T. Watson¹⁸, I.J. Watson¹⁵⁰, M.F. Watson¹⁸, G. Watts¹³⁸, S. Watts⁸², A.T. Waugh¹⁵⁰, B.M. Waugh⁷⁷,
M.S. Weber¹⁷, J.S. Webster³¹, A.R. Weidberg¹¹⁸, P. Weigell⁹⁹, J. Weingarten⁵⁴, C. Weiser⁴⁸, P.S. Wells³⁰,
T. Wenaus²⁵, D. Wendland¹⁶, Z. Weng¹⁵¹, v, T. Wengler³⁰, S. Wenig³⁰, N. Wermes²¹, M. Werner⁴⁸, P. Werner³⁰,
M. Werth¹⁶³, M. Wessels⁵⁸a, J. Wetter¹⁶¹, C. Weydert⁵⁵, K. Whalen²⁹, A. White⁸, M.J. White⁸⁶,
S. White¹²²a,¹²²b, S.R. Whitehead¹¹⁸, D. Whiteson¹⁶³, D. Whittington⁶⁰, D. Wicke¹⁷⁵, F.J. Wickens¹²⁹,
W. Wiedenmann¹⁷³, M. Wielers¹²⁹, P. Wienemann²¹, C. Wiglesworth⁷⁵, L.A.M. Wiik-Fuchs²¹, P.A. Wijeratne⁷⁷,
A. Wildauer⁹⁹, M.A. Wildt⁴²,*, I. Wilhelm¹²⁷, H.G. Wilkens³⁰, J.Z. Will⁹⁸, E. Williams³⁵, H.H. Williams¹²⁰,
S. Williams²⁸, W. Willis³⁵, S. Willocq⁴⁸, J.A. Wilson¹⁸, M.G. Wilson¹⁴³, A. Wilson⁸⁷, I. Wingerter-Seez⁵,
S. Winkelmann⁴⁸, F. Winklmeier³⁰, M. Wittgen¹⁴³, S.J. Wollstadt⁸¹, M.W. Wolter³⁹, H. Wolters¹²⁴a, i,
W.C. Wong⁴¹, G. Wooden⁸⁷, B.K. Wosiek³⁹, J. Wotschack³⁰, M.J. Woudstra⁸², K.W. Wozniak³⁹, K. Wraight⁵³,
M. Wright⁵³, B. Wrona⁷³, S.L. Wu¹⁷³, X. Wu⁴⁹, Y. Wu³³b,am, E. Wulf³⁵, B.M. Wynne⁴⁶, S. Xella³⁶, M. Xiao¹³⁶,
S. Xie⁴⁸, C. Xu³³b, z, D. Xu³³a, L. Xu³³b, B. Yabsley¹⁵⁰, S. Yacoob¹⁴⁵a, an, M. Yamada⁶⁵, H. Yamaguchi¹⁵⁵,
A. Yamamoto⁶⁵, K. Yamamoto⁶³, S. Yamamoto¹⁵⁵, T. Yamamura¹⁵⁵, T. Yamanaka¹⁵⁵, K. Yamauchi¹⁰¹,
T. Yamazaki¹⁵⁵, Y. Yamazaki⁶⁶, Z. Yan²², H. Yang³³e, H. Yang¹⁷³, U.K. Yang⁸², Y. Yang¹⁰⁹, Z. Yang¹⁴⁶a,¹⁴⁶b,
S. Yanush⁹¹, L. Yao³³a, Y. Yasu⁶⁵, E. Yatsenko⁴², J. Ye⁴⁰, S. Ye²⁵, A.L. Yen⁵⁷, M. Yilmaz⁴c, R. Yoosoofmiya¹²³,
K. Yorita¹⁷¹, R. Yoshida⁶, K. Yoshihara¹⁵⁵, C. Young¹⁴³, C.J. Young¹¹⁸, S. Youssef²², D. Yu²⁵, D.R. Yu¹⁵,
J. Yu⁸, J. Yu¹¹², L. Yuan⁶⁶, A. Yurkewicz¹⁰⁶, B. Zabinski³⁹, R. Zaidan⁶², A.M. Zaitsev¹²⁸, L. Zanello¹³²a,¹³²b,
D. Zanzi⁹⁹, A. Zaytsev²⁵, C. Zeitnitz¹⁷⁵, M. Zeman¹²⁶, A. Zemla³⁹, O. Zenin¹²⁸, T. Ženiš¹⁴⁴a, Z. Zinonos¹²²a,¹²²b,
D. Zerwas¹¹⁵, G. Zevi della Porta⁵⁷, D. Zhang⁸⁷, H. Zhang⁸⁸, J. Zhang⁶, X. Zhang³³d, Z. Zhang¹¹⁵, L. Zhao¹⁰⁸,
Z. Zhao³³b, A. Zhemchugov⁶⁴, J. Zhong¹¹⁸, B. Zhou⁸⁷, N. Zhou¹⁶³, Y. Zhou¹⁵¹, C.G. Zhu³³d, H. Zhu⁴², J. Zhu⁸⁷,
Y. Zhu³³b, X. Zhuang³³a, V. Zhuravlov⁹⁹, A. Zibell⁹⁸, D. Zieminska⁶⁰, N.I. Zimin⁶⁴, R. Zimmermann²¹,
S. Zimmermann²¹, S. Zimmermann⁴⁸, M. Ziolkowski¹⁴¹, R. Zitoun⁵, L. Živković³⁵, V.V. Zmouchko¹²⁸,*,
G. Zobernig¹⁷³, A. Zoccoli²⁰a,²⁰b, M. zur Nedden¹⁶, V. Zutshi¹⁰⁶, L. Zwalinski³⁰.

¹ School of Chemistry and Physics, University of Adelaide, Adelaide, Australia

² Physics Department, SUNY Albany, Albany NY, United States of America

³ Department of Physics, University of Alberta, Edmonton AB, Canada

⁴ (a) Department of Physics, Ankara University, Ankara; (b) Department of Physics, Dumlupınar University, Kutahya; (c) Department of Physics, Gazi University, Ankara; (d) Division of Physics, TOBB University of Economics and Technology, Ankara; (e) Turkish Atomic Energy Authority, Ankara, Turkey

⁵ LAPP, CNRS/IN2P3 and Université de Savoie, Annecy-le-Vieux, France

⁶ High Energy Physics Division, Argonne National Laboratory, Argonne IL, United States of America

⁷ Department of Physics, University of Arizona, Tucson AZ, United States of America

⁸ Department of Physics, The University of Texas at Arlington, Arlington TX, United States of America

⁹ Physics Department, University of Athens, Athens, Greece

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

¹¹ Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan

¹² Institut de Física d'Altes Energies and Departament de Física de la Universitat Autònoma de Barcelona and ICREA, Barcelona, Spain

¹³ (a) Institute of Physics, University of Belgrade, Belgrade; (b) Vinca Institute of Nuclear Sciences, University of Belgrade, Belgrade, Serbia

¹⁴ Department for Physics and Technology, University of Bergen, Bergen, Norway

¹⁵ Physics Division, Lawrence Berkeley National Laboratory and University of California, Berkeley CA, United States of America

¹⁶ Department of Physics, Humboldt University, Berlin, Germany

¹⁷ Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University of Bern, Bern, Switzerland

¹⁸ School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom

¹⁹ (a) Department of Physics, Bogazici University, Istanbul; (b) Division of Physics, Dogus University, Istanbul;

(c) Department of Physics Engineering, Gaziantep University, Gaziantep; (d) Department of Physics, Istanbul Technical University, Istanbul, Turkey

²⁰ (a) INFN Sezione di Bologna; (b) Dipartimento di Fisica, Università di Bologna, Bologna, Italy

²¹ Physikalisches Institut, University of Bonn, Bonn, Germany

²² Department of Physics, Boston University, Boston MA, United States of America

²³ Department of Physics, Brandeis University, Waltham MA, United States of America

²⁴ (a) Universidade Federal do Rio De Janeiro COPPE/EE/IF, Rio de Janeiro; (b) Federal University of Juiz de Fora (UFJF), Juiz de Fora; (c) Federal University of Sao Joao del Rei (UFSJ), Sao Joao del Rei; (d) Instituto de Fisica, Universidade de Sao Paulo, Sao Paulo, Brazil

²⁵ Physics Department, Brookhaven National Laboratory, Upton NY, United States of America

²⁶ (a) National Institute of Physics and Nuclear Engineering, Bucharest; (b) University Politehnica Bucharest, Bucharest; (c) West University in Timisoara, Timisoara, Romania

²⁷ Departamento de Física, Universidad de Buenos Aires, Buenos Aires, Argentina

²⁸ Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom

²⁹ Department of Physics, Carleton University, Ottawa ON, Canada

³⁰ CERN, Geneva, Switzerland

³¹ Enrico Fermi Institute, University of Chicago, Chicago IL, United States of America

³² (a) Departamento de Física, Pontificia Universidad Católica de Chile, Santiago; (b) Departamento de Física, Universidad Técnica Federico Santa María, Valparaíso, Chile
³³ (a) Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; (b) Department of Modern Physics, University of Science and Technology of China, Anhui; (c) Department of Physics, Nanjing University, Jiangsu; (d) School of Physics, Shandong University, Shandong; (e) Physics Department, Shanghai Jiao Tong University, Shanghai, China

³⁴ Laboratoire de Physique Corpusculaire, Clermont Université and Université Blaise Pascal and CNRS/IN2P3, Clermont-Ferrand, France

³⁵ Nevis Laboratory, Columbia University, Irvington NY, United States of America

³⁶ Niels Bohr Institute, University of Copenhagen, Kobenhavn, Denmark

³⁷ (a) INFN Gruppo Collegato di Cosenza; (b) Dipartimento di Fisica, Università della Calabria, Arcavata di Rende, Italy

³⁸ AGH University of Science and Technology, Faculty of Physics and Applied Computer Science, Krakow, Poland

³⁹ The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Krakow, Poland

⁴⁰ Physics Department, Southern Methodist University, Dallas TX, United States of America

⁴¹ Physics Department, University of Texas at Dallas, Richardson TX, United States of America

⁴² DESY, Hamburg and Zeuthen, Germany

⁴³ Institut für Experimentelle Physik IV, Technische Universität Dortmund, Dortmund, Germany

⁴⁴ Institut für Kern- und Teilchenphysik, Technical University Dresden, Dresden, Germany

⁴⁵ Department of Physics, Duke University, Durham NC, United States of America

⁴⁶ SUPA - School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom

⁴⁷ INFN Laboratori Nazionali di Frascati, Frascati, Italy

⁴⁸ Fakultät für Mathematik und Physik, Albert-Ludwigs-Universität, Freiburg, Germany

⁴⁹ Section de Physique, Université de Genève, Geneva, Switzerland

⁵⁰ (a) INFN Sezione di Genova; (b) Dipartimento di Fisica, Università di Genova, Genova, Italy

⁵¹ (a) E. Andronikashvili Institute of Physics, Iv. Javakhishvili Tbilisi State University, Tbilisi; (b) High Energy Physics Institute, Tbilisi State University, Tbilisi, Georgia

⁵² II Physikalisches Institut, Justus-Liebig-Universität Giessen, Giessen, Germany

⁵³ SUPA - School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom

⁵⁴ II Physikalisches Institut, Georg-August-Universität, Göttingen, Germany

⁵⁵ Laboratoire de Physique Subatomique et de Cosmologie, Université Joseph Fourier and CNRS/IN2P3 and Institut National Polytechnique de Grenoble, Grenoble, France

⁵⁶ Department of Physics, Hampton University, Hampton VA, United States of America

⁵⁷ Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge MA, United States of America

⁵⁸ (a) Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg; (b) Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg; (c) ZITI Institut für technische Informatik, Ruprecht-Karls-Universität Heidelberg, Mannheim, Germany

⁵⁹ Faculty of Applied Information Science, Hiroshima Institute of Technology, Hiroshima, Japan

⁶⁰ Department of Physics, Indiana University, Bloomington IN, United States of America

⁶¹ Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität, Innsbruck, Austria

⁶² University of Iowa, Iowa City IA, United States of America

⁶³ Department of Physics and Astronomy, Iowa State University, Ames IA, United States of America

⁶⁴ Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia

⁶⁵ KEK, High Energy Accelerator Research Organization, Tsukuba, Japan

⁶⁶ Graduate School of Science, Kobe University, Kobe, Japan

⁶⁷ Faculty of Science, Kyoto University, Kyoto, Japan

⁶⁸ Kyoto University of Education, Kyoto, Japan

⁶⁹ Department of Physics, Kyushu University, Fukuoka, Japan

⁷⁰ Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina

⁷¹ Physics Department, Lancaster University, Lancaster, United Kingdom

⁷² (a) INFN Sezione di Lecce; (b) Dipartimento di Matematica e Fisica, Università del Salento, Lecce, Italy

⁷³ Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom

⁷⁴ Department of Physics, Jožef Stefan Institute and University of Ljubljana, Ljubljana, Slovenia

⁷⁵ School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
76 Department of Physics, Royal Holloway University of London, Surrey, United Kingdom

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

78 Laboratoire de Physique Nucléaire et de Hautes Energies, UPMC and Université Paris-Diderot and CNRS/IN2P3, Paris, France

79 Fysiska institutionen, Lunds universitet, Lund, Sweden

80 Departamento de Fisica Teorica C-15, Universidad Autonoma de Madrid, Madrid, Spain

81 Institut für Physik, Universität Mainz, Mainz, Germany

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

83 CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France

84 Department of Physics, University of Massachusetts, Amherst MA, United States of America

85 Department of Physics, McGill University, Montreal QC, Canada

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

87 Department of Physics, The University of Michigan, Ann Arbor MI, United States of America

88 Department of Physics and Astronomy, Michigan State University, East Lansing MI, United States of America

89 (a) INFN Sezione di Milano; (b) Dipartimento di Fisica, Università di Milano, Milano, Italy

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

91 National Scientific and Educational Centre for Particle and High Energy Physics, Minsk, Republic of Belarus

92 Department of Physics, Massachusetts Institute of Technology, Cambridge MA, United States of America

93 Group of Particle Physics, University of Montreal, Montreal QC, Canada

94 P.N. Lebedev Institute of Physics, Academy of Sciences, Moscow, Russia

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

96 Moscow Engineering and Physics Institute (MEPhI), Moscow, Russia

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

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

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

100 Nagasaki Institute of Applied Science, Nagasaki, Japan

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

102 (a) INFN Sezione di Napoli; (b) Dipartimento di Scienze Fisiche, Università di Napoli, Napoli, Italy

103 Department of Physics and Astronomy, University of New Mexico, Albuquerque NM, United States of America

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

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

106 Department of Physics, Northern Illinois University, DeKalb IL, United States of America

107 Budker Institute of Nuclear Physics, SB RAS, Novosibirsk, Russia

108 Department of Physics, New York University, New York NY, United States of America

109 Ohio State University, Columbus OH, United States of America

110 Faculty of Science, Okayama University, Okayama, Japan

111 Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman OK, United States of America

112 Department of Physics, Oklahoma State University, Stillwater OK, United States of America

113 Palacký University, RCPTM, Olomouc, Czech Republic

114 Center for High Energy Physics, University of Oregon, Eugene OR, United States of America

115 LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France

116 Graduate School of Science, Osaka University, Osaka, Japan

117 Department of Physics, University of Oslo, Oslo, Norway

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

119 (a) INFN Sezione di Pavia; (b) Dipartimento di Fisica, Università di Pavia, Pavia, Italy

120 Department of Physics, University of Pennsylvania, Philadelphia PA, United States of America

121 Petersburg Nuclear Physics Institute, Gatchina, Russia

122 (a) INFN Sezione di Pisa; (b) Dipartimento di Fisica E. Fermi, Università di Pisa, Pisa, Italy

123 Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh PA, United States of America
124 (a) Laboratorio de Instrumentacao e Fisica Experimental de Particulas - LIP, Lisboa, Portugal; (b) Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain

125 Institute of Physics, Academy of Sciences of the Czech Republic, Praha, Czech Republic

126 Czech Technical University in Prague, Praha, Czech Republic

127 Faculty of Mathematics and Physics, Charles University in Prague, Praha, Czech Republic

128 State Research Center Institute for High Energy Physics, Protvino, Russia

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

130 Physics Department, University of Regina, Regina SK, Canada

131 Ritsumeikan University, Kusatsu, Shiga, Japan

132 (a) INFN Sezione di Roma I; (b) Dipartimento di Fisica, Università La Sapienza, Roma, Italy

133 (a) INFN Sezione di Roma Tor Vergata; (b) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy

134 (a) INFN Sezione di Roma Tre; (b) Dipartimento di Fisica, Università Roma Tre, Roma, Italy

135 (a) Faculté des Sciences Ain Chock, Réseau Universitaire de Physique des Hautes Energies - Université Hassan II, Casablanca; (b) Centre National de l'Energie des Sciences Techniques Nucleaires, Rabat; (c) Faculté des Sciences Semlalia, Université Cadi Ayyad, LPHEA-Marrakech; (d) Faculté des Sciences, Université Mohamed Premier and LPTPM, Oujda; (e) Faculté des sciences, Université Mohammed V-Agdal, Rabat, Morocco

136 DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l'Univers), CEA Saclay (Commissariat à l'Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France

137 Santa Cruz Institute for Particle Physics, University of California Santa Cruz, Santa Cruz CA, United States of America

138 Department of Physics, University of Washington, Seattle WA, United States of America

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

140 Department of Physics, Shinshu University, Nagano, Japan

141 Fachbereich Physik, Universität Siegen, Siegen, Germany

142 Department of Physics, Simon Fraser University, Burnaby BC, Canada

143 SLAC National Accelerator Laboratory, Stanford CA, United States of America

144 (a) Faculty of Mathematics, Physics & Informatics, Comenius University, Bratislava; (b) Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic

145 (a) Department of Physics, University of Johannesburg, Johannesburg; (b) School of Physics, University of the Witwatersrand, Johannesburg, South Africa

146 (a) Department of Physics, Stockholm University; (b) The Oskar Klein Centre, Stockholm, Sweden

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

148 Departments of Physics & Astronomy and Chemistry, Stony Brook University, Stony Brook NY, United States of America

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

150 School of Physics, University of Sydney, Sydney, Australia

151 Institute of Physics, Academia Sinica, Taipei, Taiwan

152 Department of Physics, Technion: Israel Institute of Technology, Haifa, Israel

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

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

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

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

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

158 Department of Physics, University of Toronto, Toronto ON, Canada

159 (a) TRIUMF, Vancouver BC; (b) Department of Physics and Astronomy, York University, Toronto ON, Canada

160 Faculty of Pure and Applied Sciences, University of Tsukuba, Tsukuba, Japan

161 Department of Physics and Astronomy, Tufts University, Medford MA, United States of America

162 Centro de Investigaciones, Universidad Antonio Narino, Bogota, Colombia

163 Department of Physics and Astronomy, University of California Irvine, Irvine CA, United States of America
<footnote n="164">¹⁶⁴ (a) INFN Gruppo Collegato di Udine; (b) ICTP, Trieste; (c) Dipartimento di Chimica, Fisica e Ambiente, Università di Udine, Udine, Italy</footnote>

<footnote n="165">¹⁶⁵ Department of Physics, University of Illinois, Urbana IL, United States of America</footnote>

<footnote n="166">¹⁶⁶ Department of Physics and Astronomy, University of Uppsala, Uppsala, Sweden</footnote>

<footnote n="167">¹⁶⁷ Instituto de Física Corpuscular (IFIC) and Departamento de Física Atómica, Molecular y Nuclear and Departamento de Ingeniería Electrónica and Instituto de Microelectrónica de Barcelona (IMB-CNM), University of Valencia and CSIC, Valencia, Spain</footnote>

<footnote n="168">¹⁶⁸ Department of Physics, University of British Columbia, Vancouver BC, Canada</footnote>

<footnote n="169">¹⁶⁹ Department of Physics and Astronomy, University of Victoria, Victoria BC, Canada</footnote>

<footnote n="170">¹⁷⁰ Department of Physics, University of Warwick, Coventry, United Kingdom</footnote>

<footnote n="171">¹⁷¹ Waseda University, Tokyo, Japan</footnote>

<footnote n="172">¹⁷² Department of Particle Physics, The Weizmann Institute of Science, Rehovot, Israel</footnote>

<footnote n="173">¹⁷³ Department of Physics, University of Wisconsin, Madison WI, United States of America</footnote>

<footnote n="174">¹⁷⁴ Fakultät für Physik und Astronomie, Julius-Maximilians-Universität, Würzburg, Germany</footnote>

<footnote n="175">¹⁷⁵ Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany</footnote>

<footnote n="176">¹⁷⁶ Department of Physics, Yale University, New Haven CT, United States of America</footnote>

<footnote n="177">¹⁷⁷ Yerevan Physics Institute, Yerevan, Armenia</footnote>

<footnote n="178">¹⁷⁸ Centre de Calcul de l'Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Villeurbanne, France</footnote>

<footnote>a Also at Department of Physics, King's College London, London, United Kingdom</footnote>

<footnote>b Also at Laboratorio de Instrumentacao e Fisica Experimental de Particulas - LIP, Lisboa, Portugal</footnote>

<footnote>c Also at Faculdade de Ciencias and CFNUL, Universidade de Lisboa, Lisboa, Portugal</footnote>

<footnote>d Also at Particle Physics Department, Rutherford Appleton Laboratory, Didcot, United Kingdom</footnote>

<footnote>e Also at Department of Physics, University of Johannesburg, Johannesburg, South Africa</footnote>

<footnote>f Also at TRIUMF, Vancouver BC, Canada</footnote>

<footnote>g Also at Department of Physics, California State University, Fresno CA, United States of America</footnote>

<footnote>h Also at Novosibirsk State University, Novosibirsk, Russia</footnote>

<footnote>i Also at Department of Physics, University of Coimbra, Coimbra, Portugal</footnote>

<footnote>j Also at Department of Physics, UASLP, San Luis Potosi, Mexico</footnote>

<footnote>k Also at Università di Napoli Parthenope, Napoli, Italy</footnote>

<footnote>l Also at Institute of Particle Physics (IPP), Canada</footnote>

<footnote>m Also at Department of Physics, Middle East Technical University, Ankara, Turkey</footnote>

<footnote>n Also at Louisiana Tech University, Ruston LA, United States of America</footnote>

<footnote>o Also at Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal</footnote>

<footnote>p Also at Department of Physics and Astronomy, University College London, London, United Kingdom</footnote>

<footnote>q Also at Department of Physics, University of Cape Town, Cape Town, South Africa</footnote>

<footnote>r Also at Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan</footnote>

<footnote>s Also at Institut für Experimentalphysik, Universität Hamburg, Hamburg, Germany</footnote>

<footnote>t Also at Manhattan College, New York NY, United States of America</footnote>

<footnote>u Also at CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France</footnote>

<footnote>v Also at School of Physics and Engineering, Sun Yat-sen University, Guanzhou, China</footnote>

<footnote>w Also at Academia Sinica Grid Computing, Institute of Physics, Academia Sinica, Taipei, Taiwan</footnote>

<footnote>x Also at School of Physics, Shandong University, Shandong, China</footnote>

<footnote>y Also at Dipartimento di Fisica, Università La Sapienza, Roma, Italy</footnote>

<footnote>z Also at DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l'Univers), CEA Saclay (Commissariat à l'Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France</footnote>

<footnote>aa Also at Section de Physique, Université de Genève, Geneva, Switzerland</footnote>

<footnote>ab Also at Departamento de Fisica, Universidade de Minho, Braga, Portugal</footnote>

<footnote>ac Also at Department of Physics, The University of Texas at Austin, Austin TX, United States of America</footnote>

<footnote>ad Also at Department of Physics and Astronomy, University of South Carolina, Columbia SC, United States of America</footnote>

<footnote>ae Also at Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Budapest, Hungary</footnote>
af Also at California Institute of Technology, Pasadena CA, United States of America

ag Also at Institute of Physics, Jagiellonian University, Krakow, Poland

ah Also at LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France

ai Also at Faculty of Physics, M.V.Lomonosov Moscow State University, Moscow, Russia

aj Also at Nevis Laboratory, Columbia University, Irvington NY, United States of America

ak Also at Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom

al Also at Department of Physics, Oxford University, Oxford, United Kingdom

am Also at Department of Physics, The University of Michigan, Ann Arbor MI, United States of America

an Also at Discipline of Physics, University of KwaZulu-Natal, Durban, South Africa

* Deceased