\AtlasVersion

2.0 \PreprintIdNumberCERN-EP-2020-066 \AtlasJournalRefJHEP 11 (2020) 005 \AtlasDOI10.1007/JHEP11(2020)005 \AtlasRefCodeEXOT-2019-16

Search for new non-resonant phenomena in high-mass dilepton final states with the ATLAS detector

The ATLAS Collaboration

Abstract

A search for new physics with non-resonant signals in dielectron and dimuon final states in the mass range above 2 TeV is presented. This is the first search for non-resonant signals in dilepton final states at the LHC to use a background estimate from the data. The data, corresponding to an integrated luminosity of 139 fb^-1, were recorded by the ATLAS experiment in proton–proton collisions at a center-of-mass energy of $\sqrt{s}=13$ TeV during Run 2 of the Large Hadron Collider. The benchmark signal signature is a two-quark and two-lepton contact interaction, which would enhance the dilepton event rate at the TeV mass scale. To model the contribution from background processes a functional form is fit to the dilepton invariant-mass spectra in data in a mass region below the region of interest. It is then extrapolated to a high-mass signal region to obtain the expected background there. No significant deviation from the expected background is observed in the data. Upper limits at 95% CL on the number of events and the visible cross-section times branching fraction for processes involving new physics are provided. Observed (expected) 95% CL lower limits on the contact interaction energy scale reach $35.8$ ( $37.6$ ) TeV.

1 Introduction

Signatures with dilepton (dielectron and dimuon) final states have been central in shaping the Standard Model (SM) over many years, from discoveries of new particles [1, 2, 3, 4, 5], through many precision measurements [6, 7, 8, 9], and in searches for new physics beyond the SM (BSM) [10, 11, 12, 13]. This has been the case owing to the clean and fully reconstructable experimental signature with excellent detection efficiency. This paper presents a novel search for new phenomena in final states with two electrons or two muons in 139 fb^-1 of data collected in proton–proton ( $pp$ ) collisions at the LHC at a center-of-mass energy $\sqrt{s}=13$ TeV between 2015 and 2018. The work presented here complements the ATLAS search for heavy resonances [10] using the same dataset and selection criteria. The new physics signature investigated is a broad, non-resonant excess of events over a smoothly falling dilepton invariant-mass spectrum, which is dominated by the Drell–Yan (DY) process. The search results in this paper are provided in a model-independent format. These results are further interpreted in the context of the frequently tested benchmark models with effective four-fermion ‘contact’ interactions (CI) [14, 15].

A number of changes are introduced with respect to the previous ATLAS result with an integrated luminosity of 36.1 fb^-1 [13]. The result presented here is the first non-resonant dilepton search at the LHC to use a background estimate from the data using a functional form. The signals considered are expected to manifest themselves only as a deviation from the expected gradient of the high-mass tail of the dilepton mass spectrum. Therefore, the background at high masses is estimated from a low-mass control region (CR) where the signal contribution is expected to be negligible. Contrary to previous ATLAS searches for non-resonant signals in dilepton final states, this search is performed in a single-bin high-mass signal region (SR). Both the function and region choices are optimised to maximise the expected sensitivity to observe CI processes. The extrapolated background is integrated in the SR to provide an estimate of the expected number of background events. The signal would be seen as an excess over this expected background estimate. This CR/SR approach is essential in the case of (typically small) non-resonant signals, as when the entire mass range is fit, similar to Ref. [10], a non-resonant signal can be absorbed into the background model. Moreover, the choice of a single-bin signal region removes the dependence on the shape of the mass distribution and simplifies the entire search, while at the same time providing model-independent results.

Further, this analysis has been moved from a Bayesian statistical framework to a frequentist statistical framework, which removes the dependence on signal priors. In the case where the interference between signal and SM processes is not negligible, e.g. for CI, the choice of one prior over another is less justified [16, 13]. With respect to the previous study [13] that used simulation to estimate the background, the approach presented here reduces the dependence on simulation by estimating the background from the data. A comparison showed little difference in sensitivity between the two approaches.

Finally, the transition to a background estimation from the data exchanges the systematic uncertainties in the predictions from simulation for statistical uncertainties in data. The dominant uncertainty in the expected background in the new analysis is due to statistical fluctuations in the CR. Next in importance is the uncertainty in the degree to which the extrapolation from the CR can produce a background estimate different from the underlying distribution, leading to a signal-like deflection in the SR. This uncertainty is quantified using the simulated background and its uncertainties. The uncertainty third in importance is due to a possible signal contamination in the CR.

2 Contact Interactions

In the SM, it is assumed that quarks and leptons are fundamental point-like particles and hence have no structure. However, if quarks and leptons are composite, with at least one common constituent, the interaction of these constituents could manifest itself through an effective four-fermion contact interaction at energies well below the compositeness scale [14, 15], $\Lambda$ , the energy scale below which fermion constituents are bound. A broad class of CI models can be described by the CI Lagrangian of the form of Eq. (1):

$\displaystyle\mathcal{L}=\frac{g^{2}}{\Lambda^{2}}\{$	$\displaystyle\eta_{\text{LL}}\left(\bar{q}_{\text{L}}\gamma_{\mu}q_{\text{L}}\right)\left(\bar{\ell}_{\text{L}}\gamma^{\mu}\ell_{\text{L}}\right)+$	(1)
	$\displaystyle\eta_{\text{RR}}\left(\bar{q}_{\text{R}}\gamma_{\mu}q_{\text{R}}\right)\left(\bar{\ell}_{\text{R}}\gamma^{\mu}\ell_{\text{R}}\right)+$
	$\displaystyle\eta_{\text{LR}}\left(\bar{q}_{\text{L}}\gamma_{\mu}q_{\text{L}}\right)\left(\bar{\ell}_{\text{R}}\gamma^{\mu}\ell_{\text{R}}\right)+$
	$\displaystyle\eta_{\text{RL}}\left(\bar{q}_{\text{\text{R}}}\gamma_{\mu}q_{\text{\text{R}}}\right)\left(\bar{\ell}_{\text{L}}\gamma^{\mu}\ell_{\text{L}}\right)\},$

where $g$ is a coupling constant chosen such that $g^{2}/4\pi=1$ , $\gamma$ are the $4\times 4$ Dirac matrices and the spinors $\psi_{\text{L},\text{R}}$ ( $\psi=q,\ell$ ) are the left-handed and right-handed fermion fields, respectively. The parameters $\eta_{ij}$ , where $i$ and $j$ are L or R, define the chiral structure (left or right) of the new interaction. Specific models are chosen by assigning the parameters to be $-1$ , $0$ or $+1$ .

In the context of CI searches with dilepton final states at the LHC, the terms in Eq. (1) take the form of $\eta_{ij}\left(\bar{q}_{i}\gamma_{\mu}q_{i}\right)\left(\bar{\ell}_{j}\gamma^{\mu}\ell_{j}\right)$ , where $q_{i}$ and $\ell_{j}$ are the quark and lepton fields, respectively. The differential cross-section for the process $q\bar{q}\rightarrow\ell^{+}\ell^{-}$ , in the presence of CI, can be separated into the SM DY term plus terms involving the CI. This separation can be seen in Eq. (2):

\displaystyle\frac{\text{d}\sigma}{\text{d}m_{\ell\ell}}=\frac{\text{d}\sigma_{\textrm{DY}}}{\text{d}m_{\ell\ell}}-\eta_{ij}\frac{F_{\textrm{I}}}{\Lambda^{2}}+\frac{F_{\textrm{C}}}{\Lambda^{4}},

(2)

where the first term accounts for the DY process, the second term corresponds to the interference between the DY and CI processes, and the third term corresponds to the pure CI contribution. The latter two terms include $F_{\textrm{I}}$ and $F_{\textrm{C}}$ , respectively, which are functions of the differential cross-section with respect to $m_{\ell\ell}$ with no dependence on $\Lambda$ [14]. The interference can be constructive or destructive and it is determined by the sign of $\eta_{ij}$ .

Previously, the ATLAS and CMS experiments have searched for CI with the partial Run 2 datasets at $\sqrt{s}=13$ TeV [13, 12]. The most stringent exclusion limits for $q\bar{q}\ell^{+}\ell^{-}$ CI, in which all quark flavours contribute, come from the previous ATLAS non-resonant dilepton analysis conducted using 36 fb^-1 at $\sqrt{s}=13$ TeV. The observed lower limits on $\Lambda$ range from 24 to 40 TeV depending on the specific signal model [13].

3 ATLAS detector

ATLAS [17, 18, 19] is a multipurpose detector with a forward--backward symmetric cylindrical geometry with respect to the LHC beam axis.¹¹ 1 ATLAS uses a right-handed coordinate system with its origin at the nominal interaction point (IP) in the center of the detector and the $z$ -axis along the beam pipe. The $x$ -axis points from the IP to the center of the LHC ring, and the $y$ -axis points upwards. Cylindrical coordinates $(r,\phi)$ are used in the transverse plane, $\phi$ being the azimuthal angle around the $z$ -axis. The pseudorapidity is defined in terms of the polar angle $\theta$ as $\eta=-\ln\tan(\theta/2)$ . Angular distance is measured in units of $\Delta R\equiv\sqrt{(\Delta\eta)^{2}+(\Delta\phi)^{2}}$ . The innermost layers consist of tracking detectors in the pseudorapidity range $|\eta|<2.5$ . This inner detector (ID) is surrounded by a thin superconducting solenoid that provides a $2\text{\,}\mathrm{T}$ axial magnetic field. It is enclosed by the electromagnetic and hadronic calorimeters, which cover $|\eta|<4.9$ . The outermost layers of ATLAS consist of an external muon spectrometer (MS) with $|\eta|<2.7$ , incorporating three large toroidal magnetic assemblies with eight coils each. The field integral of the toroids ranges between 2.0 and 6.0 Tm for most of the acceptance. The MS includes precision tracking chambers and fast detectors for triggering. A two-level trigger system [20] selects events to be recorded at an average rate of $1\text{\,}\mathrm{kHz}$ .

4 Data and simulation

The data and simulated event samples used in this analysis are the same as those used in Ref. [10]. The integrated luminosity of the dataset is determined to be $139.0\pm 2.4$ fb^-1, following a methodology similar to that detailed in Ref. [21]. The uncertainty in the combined 2015–2018 integrated luminosity is 1.7% [22], obtained using the LUCID-2 detector [23] for the primary luminosity measurements.

Similarly to Ref. [10], this search relies on background estimated from the data. Simulated events for the signal and background processes are used to select the fit functions, study background compositions, estimate part of the uncertainties and evaluate the signal efficiencies. All simulation-based background contributions are scaled by their respective cross-sections and summed to obtain the simulated background $m_{\ell\ell}$ distribution. The main simulated backgrounds in decreasing order of contribution to the full mass spectrum are: Drell–Yan (DY), top-quark pair ( $t\bar{t}$ ), single-top-quark and diboson production. The multi-jet and $W+$ jets processes in the dielectron channel are estimated from the data using the matrix method similarly to Ref. [13]. The contribution of such processes to the analysis is estimated using a likelihood fit. The same processes in the dimuon channel, as well as processes with $\tau$ -leptons in both channels, have a negligible impact and are not considered. The Monte Carlo (MC) event generators for the hard-scattering process and the programs used for parton showering are listed in Table 1 with their respective parton distribution functions (PDFs). ‘Afterburner’ generators such as Photos [24] for the final-state photon radiation (FSR) modeling, MadSpin [25] to preserve top-quark spin correlations, and EvtGen [26] for the modeling of $c$ - and $b$ -hadron decays, are also included in the simulation.

Table 1: The programs and PDFs used to generate the hard-scatter matrix element (ME) and to simulate parton showering (PS) in the signal and background processes. The top-quark mass is set to 172.5 GeV.

Background Process	ME Generator and ME PDFs	PS and non-perturbative effect with PDFs
NLO Drell–Yan	Powheg-Box [27, 28], CT10 [29], Photos	Pythia v8.186 [30], CTEQ6L1 [31, 32], EvtGen1.2.0
$t\bar{t}$	Powheg-Box, NNPDF3.0NLO [33]	Pythia v8.230, NNPDF23LO [34], EvtGen1.6.0
Single top $s$ -channel, $Wt$	Powheg-Box, NNPDF3.0NLO	Pythia v8.230, NNPDF23LO, EvtGen1.6.0
Single top $t$ -channel	Powheg-Box, NNPDF3.04fNLO, MadSpin	Pythia v8.230, NNPDF23LO, EvtGen1.6.0
Diboson ( $WW$ , $WZ$ and $ZZ$ )	Sherpa 2.1.1 [35], CT10	Sherpa 2.1.1, CT10
Signal Process
LO Drell–Yan	Pythia v8.186, NNPDF23LO	Pythia v8.186, NNPDF23LO, EvtGen1.2.0
LO CI	Pythia v8.186, NNPDF23LO	Pythia v8.186, NNPDF23LO, EvtGen1.2.0

The DY [36] and diboson [37] samples were generated in slices of dilepton mass to increase the sample statistics in the high-mass region. Next-to-next-to-leading-order (NNLO) corrections in quantum chromodynamic (QCD) theory, and next-to-leading-order (NLO) corrections in electroweak (EW) theory, were calculated and applied to the DY events. The corrections were computed with VRAP v0.9 [38] and the CT14 NNLO PDF set [39] in the case of QCD effects, whereas they were computed with MCSANC [40] in the case of quantum electrodynamic effects due to initial-state radiation, interference between initial- and final-state radiation and Sudakov logarithm single-loop corrections. These are calculated as mass-dependent K-factors, and reweight simulated events before reconstruction. The top-quark samples [41] are normalised to the cross-sections calculated at NNLO in QCD including resummation of the next-to-next-to-leading logarithmic soft gluon terms as provided by Top++2.0 [42].

All fully simulated event samples include the effect of multiple $pp$ interactions in the same or neighbouring bunch crossings. These effects are collectively referred to as pile-up. The simulation of pile-up collisions was performed with Pythia v8.186 using the ATLAS A3 set of tuned parameters [43] and the NNPDF23LO PDF set, and weighted to reproduce the average number of pile-up interactions per bunch crossing observed in data. The generated events were passed through a full detector simulation [44] based on Geant 4 [45].

In order to reduce statistical uncertainties, a large additional DY sample is used where the detector response is modeled by smearing the dilepton invariant-mass with mass-dependent corrections for the acceptance and efficiency, instead of using the CPU-intensive Geant 4 simulation. The relative dilepton mass resolution used in the smearing procedure is defined as $(m_{\ell\ell}-m_{\ell\ell}^{\mathrm{true}})/m_{\ell\ell}^{\mathrm{true}}$ , where $m_{\ell\ell}^{\mathrm{true}}$ is the generated dilepton mass at Born level before FSR. The mass resolution is parameterised as a sum of a Gaussian distribution, which describes the detector response, and a Crystal Ball function composed of a secondary Gaussian distribution with a power-law low-mass tail, which accounts for bremsstrahlung effects or for the effect of poor resolution in the muon momentum at high $p_{\text{T}}$ . The parameterisation of the relative dilepton mass resolution as a function of $m_{\ell\ell}^{\mathrm{true}}$ is determined by a fit of the function described above to simulated DY events at NLO. A similar procedure is used to produce a mass-smeared $t\bar{t}$ sample. These two samples replace the equivalent ones produced with the full detector simulation wherever applicable in the remainder of the analysis. The number of events in these samples is more than 55 times the number of events in data. These samples would have been difficult to produce with the full detector simulation because of the large number of events required and the limited computing resources.

Signal $m_{\ell\ell}$ distribution shapes are obtained by a matrix-element reweighting [13] of the leading-order (LO) DY samples generated in slices of dilepton mass. This reweighting includes the full interference between the non-resonant signal and the background DY process. The weight function is the ratio of the analytical matrix-elements of the full CI (including the DY component) and the DY process only, both at LO. It takes as an input the generated dilepton mass at Born level before FSR, the incoming quarks’ flavour and the CI model parameters ( $\Lambda$ , chirality states and the interference structure). These weights are applied to the LO DY events to transform these into the CI signal shapes, in steps of $2$ TeV between $\Lambda=12$ TeV and $\Lambda=100$ TeV. Dilepton mass-dependent higher-order QCD production corrections for the signals are computed with the same methodology as for the DY background, correcting from LO to NNLO. Similarly, electroweak corrections for the signals are applied in the CI reweighting along with the interference effects, correcting from LO to NLO. These signal shapes are used for optimisations as well as for calculations of the cross-section and acceptance times efficiency.

The statistical analysis used in this work requires a continuous description of the CI signal shape between the fixed (reweighted) signal shapes, for the values of $\Lambda$ mentioned above. A bin-by-bin morphing procedure is used to obtain a smooth description as a function of $\Lambda$ , linearly interpolating between the fixed signal shapes from simulation. In the case of constructive interference the morphing is almost redundant since the signal behaviour between different $\Lambda$ values can be approximated with a relatively simple relationship between the signal strength and $\Lambda$ . However, in the case of destructive interference there is no straightforward relationship between the signal strength and $\Lambda$ , and so the morphing approach is essential. The morphing is only performed for values of $\Lambda$ inside the range of the reweighted signals described above.

5 Object reconstruction and event selection

A complete description of the object definition and event selection is given in Ref. [10]. These criteria are identical to the ones used in this work and a brief description follows. The dataset was collected during LHC Run 2 in stable beam conditions, with all detector systems operating normally and while fulfilling all quality requirements. Events in the dielectron channel were recorded using a dielectron trigger, while events in the dimuon channel were required to pass at least one of two single-muon triggers. Further, it is required that at least one $pp$ interaction vertex be reconstructed in the event. The events are required to contain at least two same-flavour charged leptons consistent with the primary vertex. The object definitions, single-lepton selection and corrections are given in Ref. [10]. The reconstruction of the same energy deposits as multiple objects is resolved using overlap-removal procedures. If more than two leptons are present in the event, the two leptons with the largest $E_{\text{T}}$ ( $p_{\text{T}}$ ) in the electron (muon) channel are selected to form the dilepton pair. In events with a dielectron pair and a dimuon pair, the dielectron pair is selected because of the better resolution and higher efficiency for electrons. A selected muon pair must contain oppositely charged muons. For an electron pair, the opposite-charge requirement is not applied because of the higher probability of charge misidentification for high- $E_{\text{T}}$ electrons. The reconstructed mass of the dilepton system after the full analysis selection, $m_{\ell\ell}$ , is required to be above 130 GeV to avoid the $Z$ boson peak region, which cannot be described by the same parameterisation as the high-mass part of the dilepton distributions.

6 Background modeling

The dilepton invariant mass distribution in data is fit by a parametric background-model function in a low-mass control region (CR). The resulting background model is then extrapolated from the CR to higher-mass single-bin signal regions (SRs). The normalisation of the background model in the CR is determined by the number of data events in the CR only. All fits are performed within the RooFit [46] framework. Different choices of CR and SR are considered in order to maximise the expected sensitivity for each lepton channel and for different choices of the CI model parameters. In the destructive interference cases, if a CR includes a significant part of the destructive component of the signal shape, the integral of the number of expected signal events in the SR is reduced. Therefore, the optimisation procedure allows a gap between the CR and SR to avoid the cancellation due to the range where the signal contributes destructively. The final CR and SR choices are checked to ensure that the possible presence of a non-resonant signal does not bias the background estimation in the CR and consequently also in the SR. An illustration of the division into CR and SR is shown in Figure 1.

Figure 1: A schematic illustration of a possible set of mass ranges in this analysis. The monotonically falling total background shape is shown by the solid black line, while an example of a CI signal plus the total background shape is shown by the dotted red line. This CI signal shape corresponds to the last two terms in Eq. (2) for a destructive interference case. The two axes in the figure are shown in logarithmic scale. The data is fit in a low-mass control region (shaded blue area) where a potential bias from the presence of a signal is negligible. The resulting background shape is extrapolated from the control region into the high-mass signal region (shaded red area). The gap illustrated between the CR and the SR is found to be the preferred case for the destructive interference cases only.

An optimisation procedure is performed in two consecutive steps. In the first step, the fit function is chosen out of about 50 initial functions, which are all checked in a set of about 15 potential CR and SR configurations. Once the function choice is fixed, the CR and SR choice is optimised in a second step using this function. The description of these two steps is given below.

The procedure to determine the functional form of the background is as follows. The smooth functional form used to model the background is chosen from about 50 candidate functions. Each function is fit to the dilepton mass background template, consisting of the sum of all the simulated background contributions, in a variety of CRs and extrapolated to the respective SRs. The data and simulation are both fit using a binned-likelihood maximisation with a bin width of $1\,\text{Ge\kern-1.00006ptV}$ . The distribution of the pulls, defined as (fit–simulation)/fit for each bin, is obtained for each potential configuration of CR and SR. A function that results in pulls below 3 across all the ranges considered (CRs and SRs) is marked as acceptable. This requirement is particularly important in the SRs to veto functions that exhibit unphysical behaviour at the tail. Additionally, it is important to ensure a good description of the simulated background template in the CRs. Out of about 50 initial functions, five are found to satisfy this requirement equally well. The residual mis-modeling by the selected function is measured later and taken as an uncertainty. The final function is chosen to be the same one used in Ref. [10] and it is given in Eq. (3):

\displaystyle f_{\textrm{b}}(m_{\ell\ell})

\displaystyle=f_{\mathrm{BW},Z}(m_{\ell\ell})\cdot\left(1-x^{c}\right)^{b}\cdot x^{\sum_{i=0}^{3}p_{i}\log(x)^{i}},

(3)

where $x=m_{\ell\ell}/\sqrt{s}$ . The first term, $f_{\mathrm{BW},Z}(m_{\ell\ell})$ , is a non-relativistic Breit–Wigner function with $m_{Z}=91.1876\,\text{Ge\kern-1.00006ptV}$ and $\Gamma_{Z}=2.4952\,\text{Ge\kern-1.00006ptV}$ [47]. The second term, $(1-x^{c})^{b}$ , ensures that the background shape evaluates to zero at $x\to 1$ . The parameters $b$ and $c$ are fixed to values obtained from fits to the simulated background. In the third term, the parameters $p_{i}$ with $i=0,..,3$ are left free in the fits. The function $f_{\textrm{b}}(m_{\ell\ell})$ is treated as a probability density function in the fits performed in the CR. This function is then normalised in the CR to $N_{\textrm{CR}}$ , the number of events in the CR in data (or simulation where applicable), where it is assumed that the CR is completely dominated by background events.

After the function choice has been made, the procedure to define the CR and SR is as follows. The two boundaries of the CR ( $\textrm{CR}_{\textrm{min}}$ and $\textrm{CR}_{\textrm{max}}$ ) and the lower boundary of the SR ( $\textrm{SR}_{\textrm{min}}$ ) are chosen to optimise the expected sensitivity for each of the CI signals considered. The $\textrm{CR}_{\textrm{min}}$ value is varied between 160 GeV (well above the $Z$ peak) and 500 GeV, while $\textrm{CR}_{\textrm{max}}$ is varied between 1 TeV and 2.9 TeV. The CR is not wide enough to constrain the fit for $\textrm{CR}_{\textrm{max}}$ values below 1 TeV, while above 2.9 TeV the possible new signals contribute significantly. In all cases, the upper boundary of the SR is fixed to 6 TeV, beyond the highest-mass events expected in data, while $\textrm{SR}_{\textrm{min}}$ can lie at any point above $\textrm{CR}_{\textrm{max}}$ . The boundaries of the CR are varied to test for a possible dependence of the background estimation in the SR and it is found that the estimation remains stable against these variations.

To avoid a bias from possible signal contamination in the CR, the CR and SR choice is validated using a signal injection test for each of the configurations tested. The signals are injected in the range $18\mathrm{\penalty\ \text{Te\kern-1.00006ptV}}\leq\Lambda\leq 40\mathrm{\penalty\ \text{Te\kern-1.00006ptV}}$ . A collection of background+signal distributions are produced by simulation for various $\Lambda$ values of interest. An extension of Eq. (3), with an added signal component, is used to fit these distributions:

\displaystyle f_{\textrm{b+s}}(m_{\ell\ell},\Lambda)=N_{\textrm{b}}\cdot f_{\textrm{b}}(m_{\ell\ell})+N_{\textrm{s}}(\Lambda)\cdot f_{\textrm{s}}(m_{\ell\ell},\Lambda),

(4)

where $f_{\textrm{s}}(m_{\ell\ell},\Lambda)$ is the signal probability density function and $N_{\textrm{s}}(\Lambda)$ is the number of signal events in the CR. Both $f_{\textrm{s}}(m_{\ell\ell},\Lambda)$ and $N_{\textrm{s}}(\Lambda)$ are determined from simulation. The parameter $N_{\textrm{b}}$ is the number of background events in the CR with the constraint $N_{\textrm{b}}+N_{\textrm{s}}(\Lambda)=N_{\textrm{CR}}$ . The full shape is fitted in the CR using the background+signal model and compared with the nominal case, where there is no signal injected and where the fit model is the background-only one. If a significant difference is found between the background estimated with the injected signal fit and the nominal background-only fit, the configuration is excluded. The difference between these two background estimates is assessed to be significant when it is larger than the systematic uncertainty of the background component in the background+signal model. This procedure is repeated iteratively while varying two out of the three mass boundary parameters ( $\textrm{CR}_{\textrm{min}}$ , $\textrm{CR}_{\textrm{max}}$ and $\textrm{SR}_{\textrm{min}}$ ). It is found that the background component of the background+signal model does not differ significantly from the simulated background, both in the presence and absence of an injected signal.

Each chirality choice of the CI model is tested with an independent CR and SR configuration. It is found that for models with destructive interference a mass gap between the CR and SR of $\sim 1300$ GeV is preferred by the optimisation procedure, while in the case of constructive interference the optimal choice is where $\textrm{SR}_{\textrm{min}}$ coincides with $\textrm{CR}_{\textrm{max}}$ . The resulting ranges for the different chirality options are similar at the level of a few tens of GeV. The final result is insensitive to the choice of CR within these small differences, and therefore these are merged as listed in Table 2 to simplify the subsequent procedures.

Table 2: CR and SR ranges (in units of GeV). For all configurations

\textrm{SR}_{\textrm{max}}=6000

GeV.

Channel	Constructive interference			Destructive interference
Channel	$\textrm{CR}_{\textrm{min}}$	$\textrm{CR}_{\textrm{max}}$	$\textrm{SR}_{\textrm{min}}$	$\textrm{CR}_{\textrm{min}}$	$\textrm{CR}_{\textrm{max}}$	$\textrm{SR}_{\textrm{min}}$
$e^{+}e^{-}$	280	2200	2200	310	1450	2770
$\mu^{+}\mu^{-}$	310	2070	2070	320	1250	2570

The function given in Eq. (3) is the only background model used to estimate the final expected background in the SR for each of these configurations.

7 Uncertainties

Uncertainties related to the background modeling in the SR result from three main sources as discussed below. For all background variations discussed, where the extrapolation procedure is performed, it is verified that the $\chi^{2}/N_{\textrm{DoF}}$ of the fits to each of the background variations in the CR is close to unity. The uncertainties related to the signal model are also presented.

7.1 Statistical uncertainty of the expected background

Statistical fluctuations in the data lead to variations of the fitted background model in the CR. This in turn has an impact on the extrapolated background in the SR. To estimate the impact of this statistical uncertainty, $\sigma_{\textrm{b}}^{\textrm{Stat}}$ , the following procedure is performed for each region configuration. First, the data is fit in the CR, extrapolated, and integrated in the SR, giving the nominal background expectation in the SR. The nominal background $m_{\ell\ell}$ distribution shape in the CR is then used as a probability density function from which an ensemble of pseudo-datasets can be generated. The normalisation of this function corresponds to that of the observed data in the CR. Finally, the background model is fit to each of the pseudo-datasets in the ensemble individually, extrapolated, and integrated in the SR. The distribution of the pseudo-background expectations is confirmed to be centerd around the nominal background expectation, indicating no bias. The standard deviation of the distribution is taken as the statistical uncertainty. For the dielectron and dimuon channels, the statistical uncertainty ranges from 14% to 20% (34% to 60%) of the nominal background for the constructive (destructive) SRs of the analysis.

7.2 Induced spurious-signal uncertainty in the expected background

The second uncertainty in the expected background corresponds to the degree to which the background model can induce a signal-like excess or deficit when extrapolated to the SR. This uncertainty is hereafter called ‘induced spurious-signal’ ( $\sigma_{\textrm{b}}^{\textrm{ISS}}$ ). This uncertainty results from the extrapolation procedure and it is measured on the nominal simulated background and its systematic variations.

The uncertainties associated with the simulated background shape are derived from simulated variations on the background shape. These uncertainties are used to generate an ensemble of possible (pseudo-) background shapes. Each pseudo-background shape is constructed from the nominal simulated background shape, summed with weighted uncertainties. The weight for each uncertainty is randomly sampled from a normal distribution, with a mean of zero and standard deviation of one, in the range of $[-1,1]$ . The resulting background shape is used to generate a pseudo-dataset that is fit and extrapolated to the SR.

The difference in expected background between the fit and the pseudo-background SR integral is then taken as the induced spurious-signal per pseudo-background. The mean and standard deviation of the distribution from all pseudo-backgrounds are summed in quadrature and the result is taken as $\sigma_{\textrm{b}}^{\textrm{ISS}}$ . The mean is considered to take into account a possible systematic shift in the estimate besides its spread.

The variations considered are due to theoretical and experimental uncertainties in the simulated background as well as the uncertainties in the backgrounds from multi-jet and $W$ +jets processes. The largest source of uncertainty in the simulated background is theoretical, and it is particularly large at the high end of the dilepton mass spectrum. The second largest source of uncertainty in the simulated background is experimental, and is mostly due to high- $p_{\text{T}}$ muon identification in the dimuon channel. The third largest source is the uncertainty in the multi-jet and $W$ +jets background components, and is estimated from the data.

The following variations are considered for the theoretical uncertainties for the DY component only: the eigenvector variations of the nominal PDF set, variations of PDF scales, the strong coupling ( $\alpha_{\textrm{S}}(M_{Z})$ ), electroweak corrections, photon-induced corrections [Martin:2005pi], as well as the effect of choosing different PDF sets. For all PDF variations, the modified DY component is used along with the other nominal background components. These theoretical uncertainties are the same for both dilepton channels at generator level, but they result in different uncertainties at reconstruction level due to the different resolutions of the dielectron and dimuon channels. Further details of this procedure can be found in Ref. [13]. The size of these uncertainties in the total simulated background is $\leq 19\%$ ( $\leq 15\%$ ) below 4000 GeV for the dielectron (dimuon) channel.

Among the experimental uncertainty sources in the dielectron channel, the dominant ones are the electron identification at low dielectron masses ( $\leq 5\%$ , below $\sim 2000$ GeV) and the uncertainty in the electromagnetic energy scale at higher dielectron masses ( $\leq 15\%$ ). In the muon channel, the dominant experimental uncertainties arise from the muon reconstruction efficiency at low dimuon masses ( $\leq 20\%$ , below $\sim 4000$ GeV) and from the identification of high- $p_{\text{T}}$ muons at higher dimuon masses ( $\leq 50\%$ ).

The relative uncertainty of the simulated background due to the multi-jet and $W$ +jets component rises from $\sim 1\%$ at 1 TeV to $\sim 10\%$ at 4 TeV. For the multi-jet and $W$ +jets component variations, the modified shape is used each time along with the other nominal background components from simulation. This contribution is the smallest amongst all other variations in the CR.

The $\sigma_{\textrm{b}}^{\textrm{ISS}}$ uncertainty is $\sim 4\%$ $(\sim 6\%)$ for the constructive $e^{+}e^{-}$ ( $\mu^{+}\mu^{-}$ ) channels, and is $\sim 7\%$ $(\sim 24\%)$ for the destructive channels. The large difference between the $\mu^{+}\mu^{-}$ and $e^{+}e^{-}$ channels in the destructive case is owing to the smaller CR in the $\mu^{+}\mu^{-}$ case as can be seen in Table 2. Consequently, the $\mu^{+}\mu^{-}$ background fit in the CR is less constrained, allowing for more freedom in the extrapolation to the SR.

7.3 CR bias uncertainty in the expected background

Finally, the ‘CR bias uncertainty’ ( $\sigma_{\textrm{b}}^{\textrm{CRB}}$ ) in the expected background is a measure of the residual difference between the two fit models, with and without a signal component. A possible signal may bias the background estimation from the background-only model, while the background estimation from the background+signal model should remain unbiased. In simulation, this difference is negligible by construction owing to the optimisation of the CR boundaries. When fitting the data with the two models, however, a small difference between the background-only model and the background component of the background+signal model can still exist. This difference is taken as an additional uncertainty. To measure it, the background+signal model from Eq. (4) is fit to the data in the CR and the background component is extrapolated to the SR. After the extrapolation and integration in the SR, the resulting background estimation is compared with the one resulting from the background-only model from Eq. (3). The differences are taken as an uncertainty only in the case of the CI interpretation since it is model-dependent. The $\sigma_{\textrm{b}}^{\textrm{CRB}}$ uncertainty is smaller than 4% of the nominal background for all SRs of the analysis.

7.4 Uncertainties in the signal yield

The expected number of simulated CI signal events in the SR is also affected by theoretical and experimental uncertainties. The signal yield is obtained by integrating the simulated signal in the single-bin SR. This is also performed for all theoretical and experimental systematic variations of the signal. The uncertainty in the signal yield is obtained from the sum in quadrature of the differences between the yields obtained in all variations and the nominal yield. Both the theoretical and experimental components of the signal uncertainty are determined as discussed above for the background in the context of $\sigma_{\textrm{b}}^{\textrm{ISS}}$ . The theoretical uncertainties, $\sigma_{\textrm{s}}^{\textrm{Theory}}$ , are presented for reference in Table 3, but are not used in the statistical analysis. The experimental uncertainties of the signal are $\leq 9\%$ for the electron channel and $\leq 22\%$ for the muon channel.

The breakdown of the relative uncertainty in both the background estimate and the expected signal yield is shown in Table 3, sorted by impact. For all cases, the relative uncertainties in the destructive SRs are larger than those in the constructive SRs. This is due to both the smaller size of the SR leading to less background and hence larger relative uncertainty, and the smaller size of the CR leading to a weaker constraint on the background model.

Table 3: Summary of the relative uncertainties in the background estimate and signal in each SR, where

\sigma_{\textrm{b}}^{\textrm{Stat}}

is the ‘statistical uncertainty’,

\sigma_{\textrm{b}}^{\textrm{ISS}}

is the ‘induced spurious-signal uncertainty’ and

\sigma_{\textrm{b}}^{\textrm{CRB}}

is the ‘control region bias uncertainty’. Experimental and theoretical uncertainties are shown as well, with the latter averaged across CI chirality scenarios and quoted for

\Lambda=30

TeV only.

Channel	Interference	Background uncertainties			Signal uncertainties
Channel	Interference	$\sigma_{\textrm{b}}^{\textrm{Stat}}$	$\sigma_{\textrm{b}}^{\textrm{ISS}}$	$\sigma_{\textrm{b}}^{\textrm{CRB}}$	$\sigma_{\textrm{s}}^{\textrm{Experiment}}$		$\sigma_{\textrm{s}}^{\textrm{Theory}}$
$e^{+}e^{-}$	Constructive	14%	4%	2%	8	%	+11 –10	% %
$e^{+}e^{-}$	Destructive	34%	7%	1%	8	%	+14 –13	% %
$\mu^{+}\mu^{-}$	Constructive	21%	6%	2%	+20 –17	% %	+10 –9	% %
$\mu^{+}\mu^{-}$	Destructive	58%	24%	4%	+27 –22	% %	+13 –12	% %

8 Results

The dilepton invariant-mass distributions for events that pass the full analysis selection are shown in Figure 2. The candidate with the highest reconstructed mass is a dielectron candidate with $m_{ee}=4.06\,\text{Te\kern-1.00006ptV}$ . The candidate with the highest reconstructed mass in the dimuon channel has an invariant mass of $m_{\mu\mu}=2.75\,\text{Te\kern-1.00006ptV}$ .

((a))

((b))

((c))

((d))

Figure 2: Distributions of the invariant mass of dilepton pairs passing the full selection for dielectrons (left) and dimuons (right), and showing CR and SR for constructive interference (top) and destructive interference (bottom). Figures (c) and (d) show the region between the SR and CR, but this is not used by the fit. The data points are plotted at the center of each bin as the number of events divided by the bin width, which is constant in

\log{(m_{\ell\ell})}

. The error bars indicate statistical uncertainties only. A few CI benchmark signal shapes are shown, scaled to the data luminosity and superimposed by subtracting the LO DY component and adding the resulting shape to the background shape obtained from the fit. These signals have LL chirality with

\Lambda=

18, 22, and 26 TeV for the constructive case and

\Lambda=

16, 20, and

26

TeV for the destructive case. The background-only fit is shown in solid red, with the light red area being its uncertainty. The boundaries of the CR and SR corresponding to the signals used are shown in dotted vertical lines for reference and marked by arrows. The differences between the data and the fit results in units of standard deviations of the statistical uncertainty are shown in the bottom panels.

For the statistical analysis, a likelihood function is constructed using a single-bin Poissonian counting-experiment approach. The uncertainties are accounted for as Gaussian constraints taken as nuisance parameters. The compatibility of finding the observed data and the background-only hypothesis is tested by fitting the data with the background model. The p-value of each observation is defined as the probability, given the background-only hypothesis, of observing an excess at least as large as that seen in the data. The significance is the Gaussian cumulative density function of the p-value. In the absense of an excess, upper limits at 95% confidence level (CL) on the number of signal events in the SR are determined using the profile-likelihood-ratio test statistic [48] with the $\text{CL}_{\text{s}}$ method [49, 50]. These limits are converted to lower limits on the CI scale, $\Lambda$ . The $\text{CL}_{\text{s}}$ is computed using $400{,}000$ pseudo-experiments, appropriate for the case where the expected background is small. The statistical uncertainty, due to the observed number of events in data and $\sigma_{\textrm{b}}^{\textrm{Stat}}$ , has the largest impact on the search sensitivity. The combined likelihood of the $e^{+}e^{-}$ and $\mu^{+}\mu^{-}$ measurements given the expected background is the product of the likelihood of the individual channel measurements. The signal expectation for both channels is determined by a shared $\Lambda$ value while the nuisance parameters for each channel remain independent.

The number of events in the SR for the data and the background, and the corresponding significance is given in Table 4. No significant excess is observed. The upper limits on the visible cross-section times branching fraction $(\sigma_{\textrm{vis}}\times\mathcal{B})$ and the number of signal events ( $N_{\textrm{sig}}$ ) in different SRs are given in Table 5 and are shown in Figure 3. The expected yields of a few signals, as well as their values of the acceptance times efficiency in the SR, are also given in Table 5. Figure 4 and Table 6 summarise the lower limits on $\Lambda$ for the different SRs used in the analysis. The observed limit on $\Lambda$ ranges from $22.3$ TeV to $35.8$ TeV.

Table 4: The dielectron and dimuon event yields for the data, the expected background and the respective significance in the different SRs used in the analysis. The p-value of each observation is defined as the probability, given the background-only hypothesis, of an observation at least as large as that seen in the data. The significance is the Gaussian cumulative density function of the p-value, and negative significances correspond to deficits.

SR	Data	Background		Significance
$e^{+}e^{-}$ Const.	19	12.4	$\pm 1.9$	1.28
$e^{+}e^{-}$ Dest.	2	3.1	$\pm 1.1$	– 0.72
$\mu^{+}\mu^{-}$ Const.	6	9.6	$\pm 2.1$	– 0.99
$\mu^{+}\mu^{-}$ Dest.	1	1.4	$\pm 0.9$	– 0.58

Figure 3: Model-independent upper limits at 95% CL on the number of signal events in the (constructive/destructive interference) SRs used in the analysis for dielectrons and dimuons.

Table 5: The observed model-independent upper limit at 95% CL on the visible cross-section times branching fraction

(\sigma_{\textrm{vis}}\times\mathcal{B})

and the number of signal events

(N_{\textrm{sig}})

in the dielectron and dimuon SRs used in the analysis. The expected yields for a few CI signal points (LL chirality only) are listed along with the values of the signal acceptance times efficiency

(\mathcal{A}\times\epsilon_{\textrm{sig}})

for reference.

SR	Limit on $\sigma_{\textrm{vis}}\times\mathcal{B}$ [fb]		Limit on $N_{\textrm{sig}}$		Signal (LL chirality only)
	Exp.	Obs.	Exp.	Obs.	$\Lambda=20\penalty\ \text{Te\kern-0.79727ptV}$		$\Lambda=30\penalty\ \text{Te\kern-0.79727ptV}$		$\Lambda=40\penalty\ \text{Te\kern-0.79727ptV}$
	Exp.	Obs.	Exp.	Obs.	$N_{\text{sig}}$	$\mathcal{A}\times\epsilon_{\text{sig}}$ [%]	$N_{\text{sig}}$	$\mathcal{A}\times\epsilon_{\text{sig}}$ [%]	$N_{\text{sig}}$	$\mathcal{A}\times\epsilon_{\text{sig}}$ [%]
$e^{+}e^{-}$ Const.	0.067	0.115	9.3	$16.0$	$39.1$	69	$10.3$	69	$4.4$	69
$e^{+}e^{-}$ Dest.	0.036	0.032	5.0	$4.4$	$9.6$	70	$1.0$	70	$-0.1$	69
$\mu^{+}\mu^{-}$ Const.	0.057	0.042	8.0	$5.8$	$28.5$	43	$7.7$	43	$3.4$	43
$\mu^{+}\mu^{-}$ Dest.	0.029	0.027	4.0	$3.8$	$7.1$	43	$0.6$	42	$-0.2$	44

((a))

((b))

((c))

Figure 4: Lower limits at 95

\%

CL on

\Lambda

for (a) the dielectron channel (b) the dimuon channel and (c) the combined dilepton channels for different signal chiralities in the (constructive/destructive interference) SRs of the analysis.

Table 6: Expected and observed lower limits at 95

\%

CL on

\Lambda

in TeV for the dielectron and dimuon channels separately and the combined dilepton channel and for CI signal hypotheses with constructive and destructive interference and different chiralities.

Int.	Channel	Exp./Obs.	LL	LR	RL	RR
Constructive	$ee$	Expected	31.1	28.9	28.7	30.9
	$ee$	Observed	26.1	24.7	24.6	26.0
	$\mu\mu$	Expected	29.2	27.1	27.0	29.0
	$\mu\mu$	Observed	32.7	30.0	29.8	32.6
	$\ell\ell$	Expected	37.6	34.0	33.7	37.3
	$\ell\ell$	Observed	35.8	32.5	32.3	35.5
Destructive	$ee$	Expected	23.0	24.4	24.4	23.2
	$ee$	Observed	23.5	25.1	25.1	23.7
	$\mu\mu$	Expected	22.0	23.6	23.6	22.2
	$\mu\mu$	Observed	22.3	23.9	23.9	22.5
	$\ell\ell$	Expected	25.6	28.0	28.0	25.9
	$\ell\ell$	Observed	26.0	28.8	28.8	26.5

More information is given in the supplemental material ²² 2 https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/EXOT-2019-16/. This includes information concerning the signal shape and its yields, the fit function parameter values, a comparison of the resulting background with the background from simulation and, finally, the evolution of sensitivity to $\Lambda$ for different data-taking campaigns, ranging from 5 fb^-1 at 7 TeV to the results presented here.

9 Conclusion

A search for new non-resonant signals in dielectron and dimuon final states with invariant mass larger than 2 TeV is performed by the ATLAS experiment using the 139 fb^-1 of proton–proton collision data collected during Run 2 of the LHC at $\sqrt{s}=13$ TeV. A functional form is fitted to the dilepton low-mass distribution in data and extrapolated to higher masses to model the contribution from background processes. No significant excess is observed above the expected background. Upper limits are set on the number of signal events, as well as lower limits on the CI scale $\Lambda$ . The acceptance times efficiency values for the corresponding signal shapes are provided. The strongest limits are set on the combined left-left chirality constructive model. These observed (expected) limits exclude this model for $\Lambda$ up to $35.8$ ( $37.6$ ) TeV at 95% CL.

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; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; ANID, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS and CEA-DRF/IRFU, France; SRNSFG, Georgia; BMBF, HGF and MPG, Germany; GSRT, Greece; RGC and Hong Kong SAR, China; ISF and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; NWO, Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA, Romania; JINR; MES of Russia and NRC KI, Russian Federation; MESTD, Serbia; MSSR, Slovakia; ARRS and MIZŠ, Slovenia; DST/NRF, South Africa; MICINN, Spain; SRC and Wallenberg Foundation, Sweden; SERI, SNSF and Cantons of Bern and Geneva, Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE and NSF, United States of America. In addition, individual groups and members have received support from BCKDF, CANARIE, Compute Canada, CRC and IVADO, Canada; Beijing Municipal Science & Technology Commission, China; COST, ERC, ERDF, Horizon 2020 and Marie Skłodowska-Curie Actions, European Union; Investissements d’Avenir Labex, Investissements d’Avenir Idex and ANR, France; DFG and AvH Foundation, Germany; Herakleitos, Thales and Aristeia programmes co-financed by EU-ESF and the Greek NSRF, Greece; BSF-NSF and GIF, Israel; La Caixa Banking Foundation, CERCA Programme Generalitat de Catalunya and PROMETEO and GenT Programmes Generalitat Valenciana, Spain; Göran Gustafssons Stiftelse, Sweden; The Royal Society and Leverhulme Trust, United Kingdom.

The crucial computing support from all WLCG partners is acknowledged gratefully, in particular from CERN, the ATLAS Tier-1 facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/GridKA (Germany), INFN-CNAF (Italy), NL-T1 (Netherlands), PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA), the Tier-2 facilities worldwide and large non-WLCG resource providers. Major contributors of computing resources are listed in Ref. [51].

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The ATLAS Collaboration

G. Aad ${}^{\textrm{\scriptsize 102}}$ , B. Abbott ${}^{\textrm{\scriptsize 128}}$ , D.C. Abbott ${}^{\textrm{\scriptsize 103}}$ , A. Abed Abud ${}^{\textrm{\scriptsize 36}}$ , K. Abeling ${}^{\textrm{\scriptsize 53}}$ , D.K. Abhayasinghe ${}^{\textrm{\scriptsize 94}}$ , S.H. Abidi ${}^{\textrm{\scriptsize 166}}$ , O.S. AbouZeid ${}^{\textrm{\scriptsize 40}}$ , N.L. Abraham ${}^{\textrm{\scriptsize 155}}$ , H. Abramowicz ${}^{\textrm{\scriptsize 160}}$ , H. Abreu ${}^{\textrm{\scriptsize 159}}$ , Y. Abulaiti ${}^{\textrm{\scriptsize 6}}$ , B.S. Acharya ${}^{\textrm{\scriptsize 67a,67b,n}}$ , B. Achkar ${}^{\textrm{\scriptsize 53}}$ , L. Adam ${}^{\textrm{\scriptsize 100}}$ , C. Adam Bourdarios ${}^{\textrm{\scriptsize 5}}$ , L. Adamczyk ${}^{\textrm{\scriptsize 84a}}$ , L. Adamek ${}^{\textrm{\scriptsize 166}}$ , J. Adelman ${}^{\textrm{\scriptsize 121}}$ , M. Adersberger ${}^{\textrm{\scriptsize 114}}$ , A. Adiguzel ${}^{\textrm{\scriptsize 12c}}$ , S. Adorni ${}^{\textrm{\scriptsize 54}}$ , T. Adye ${}^{\textrm{\scriptsize 143}}$ , A.A. Affolder ${}^{\textrm{\scriptsize 145}}$ , Y. Afik ${}^{\textrm{\scriptsize 159}}$ , C. Agapopoulou ${}^{\textrm{\scriptsize 65}}$ , M.N. Agaras ${}^{\textrm{\scriptsize 38}}$ , A. Aggarwal ${}^{\textrm{\scriptsize 119}}$ , C. Agheorghiesei ${}^{\textrm{\scriptsize 27c}}$ , J.A. Aguilar-Saavedra ${}^{\textrm{\scriptsize 139f,139a,ad}}$ , A. Ahmad ${}^{\textrm{\scriptsize 36}}$ , F. Ahmadov ${}^{\textrm{\scriptsize 80}}$ , W.S. Ahmed ${}^{\textrm{\scriptsize 104}}$ , X. Ai ${}^{\textrm{\scriptsize 18}}$ , G. Aielli ${}^{\textrm{\scriptsize 74a,74b}}$ , S. Akatsuka ${}^{\textrm{\scriptsize 86}}$ , T.P.A. Åkesson ${}^{\textrm{\scriptsize 97}}$ , E. Akilli ${}^{\textrm{\scriptsize 54}}$ , A.V. Akimov ${}^{\textrm{\scriptsize 111}}$ , K. Al Khoury ${}^{\textrm{\scriptsize 65}}$ , G.L. Alberghi ${}^{\textrm{\scriptsize 23b,23a}}$ , J. Albert ${}^{\textrm{\scriptsize 175}}$ , M.J. Alconada Verzini ${}^{\textrm{\scriptsize 160}}$ , S. Alderweireldt ${}^{\textrm{\scriptsize 36}}$ , M. Aleksa ${}^{\textrm{\scriptsize 36}}$ , I.N. Aleksandrov ${}^{\textrm{\scriptsize 80}}$ , C. Alexa ${}^{\textrm{\scriptsize 27b}}$ , T. Alexopoulos ${}^{\textrm{\scriptsize 10}}$ , A. Alfonsi ${}^{\textrm{\scriptsize 120}}$ , F. Alfonsi ${}^{\textrm{\scriptsize 23b,23a}}$ , M. Alhroob ${}^{\textrm{\scriptsize 128}}$ , B. Ali ${}^{\textrm{\scriptsize 141}}$ , S. Ali ${}^{\textrm{\scriptsize 157}}$ , M. Aliev ${}^{\textrm{\scriptsize 165}}$ , G. Alimonti ${}^{\textrm{\scriptsize 69a}}$ , C. Allaire ${}^{\textrm{\scriptsize 36}}$ , B.M.M. Allbrooke ${}^{\textrm{\scriptsize 155}}$ , B.W. Allen ${}^{\textrm{\scriptsize 131}}$ , P.P. Allport ${}^{\textrm{\scriptsize 21}}$ , A. Aloisio ${}^{\textrm{\scriptsize 70a,70b}}$ , F. Alonso ${}^{\textrm{\scriptsize 89}}$ , C. Alpigiani ${}^{\textrm{\scriptsize 147}}$ , E. Alunno Camelia ${}^{\textrm{\scriptsize 74a,74b}}$ , M. Alvarez Estevez ${}^{\textrm{\scriptsize 99}}$ , M.G. Alviggi ${}^{\textrm{\scriptsize 70a,70b}}$ , Y. Amaral Coutinho ${}^{\textrm{\scriptsize 81b}}$ , A. Ambler ${}^{\textrm{\scriptsize 104}}$ , L. Ambroz ${}^{\textrm{\scriptsize 134}}$ , C. Amelung ${}^{\textrm{\scriptsize 26}}$ , D. Amidei ${}^{\textrm{\scriptsize 106}}$ , S.P. Amor Dos Santos ${}^{\textrm{\scriptsize 139a}}$ , S. Amoroso ${}^{\textrm{\scriptsize 46}}$ , C.S. Amrouche ${}^{\textrm{\scriptsize 54}}$ , F. An ${}^{\textrm{\scriptsize 79}}$ , C. Anastopoulos ${}^{\textrm{\scriptsize 148}}$ , N. Andari ${}^{\textrm{\scriptsize 144}}$ , T. Andeen ${}^{\textrm{\scriptsize 11}}$ , J.K. Anders ${}^{\textrm{\scriptsize 20}}$ , S.Y. Andrean ${}^{\textrm{\scriptsize 45a,45b}}$ , A. Andreazza ${}^{\textrm{\scriptsize 69a,69b}}$ , V. Andrei ${}^{\textrm{\scriptsize 61a}}$ , C.R. Anelli ${}^{\textrm{\scriptsize 175}}$ , S. Angelidakis ${}^{\textrm{\scriptsize 9}}$ , A. Angerami ${}^{\textrm{\scriptsize 39}}$ , A.V. Anisenkov ${}^{\textrm{\scriptsize 122b,122a}}$ , A. Annovi ${}^{\textrm{\scriptsize 72a}}$ , C. Antel ${}^{\textrm{\scriptsize 54}}$ , M.T. Anthony ${}^{\textrm{\scriptsize 148}}$ , E. Antipov ${}^{\textrm{\scriptsize 129}}$ , M. Antonelli ${}^{\textrm{\scriptsize 51}}$ , D.J.A. Antrim ${}^{\textrm{\scriptsize 170}}$ , F. Anulli ${}^{\textrm{\scriptsize 73a}}$ , M. Aoki ${}^{\textrm{\scriptsize 82}}$ , J.A. Aparisi Pozo ${}^{\textrm{\scriptsize 173}}$ , M.A. Aparo ${}^{\textrm{\scriptsize 155}}$ , L. Aperio Bella ${}^{\textrm{\scriptsize 46}}$ , N. Aranzabal Barrio ${}^{\textrm{\scriptsize 36}}$ , V. Araujo Ferraz ${}^{\textrm{\scriptsize 81a}}$ , R. Araujo Pereira ${}^{\textrm{\scriptsize 81b}}$ , C. Arcangeletti ${}^{\textrm{\scriptsize 51}}$ , A.T.H. Arce ${}^{\textrm{\scriptsize 49}}$ , F.A. Arduh ${}^{\textrm{\scriptsize 89}}$ , J-F. Arguin ${}^{\textrm{\scriptsize 110}}$ , S. Argyropoulos ${}^{\textrm{\scriptsize 52}}$ , J.-H. Arling ${}^{\textrm{\scriptsize 46}}$ , A.J. Armbruster ${}^{\textrm{\scriptsize 36}}$ , A. Armstrong ${}^{\textrm{\scriptsize 170}}$ , O. Arnaez ${}^{\textrm{\scriptsize 166}}$ , H. Arnold ${}^{\textrm{\scriptsize 120}}$ , Z.P. Arrubarrena Tame ${}^{\textrm{\scriptsize 114}}$ , G. Artoni ${}^{\textrm{\scriptsize 134}}$ , K. Asai ${}^{\textrm{\scriptsize 126}}$ , S. Asai ${}^{\textrm{\scriptsize 162}}$ , T. Asawatavonvanich ${}^{\textrm{\scriptsize 164}}$ , N. Asbah ${}^{\textrm{\scriptsize 59}}$ , E.M. Asimakopoulou ${}^{\textrm{\scriptsize 171}}$ , L. Asquith ${}^{\textrm{\scriptsize 155}}$ , J. Assahsah ${}^{\textrm{\scriptsize 35d}}$ , K. Assamagan ${}^{\textrm{\scriptsize 29}}$ , R. Astalos ${}^{\textrm{\scriptsize 28a}}$ , R.J. Atkin ${}^{\textrm{\scriptsize 33a}}$ , M. Atkinson ${}^{\textrm{\scriptsize 172}}$ , N.B. Atlay ${}^{\textrm{\scriptsize 19}}$ , H. Atmani ${}^{\textrm{\scriptsize 65}}$ , K. Augsten ${}^{\textrm{\scriptsize 141}}$ , V.A. Austrup ${}^{\textrm{\scriptsize 181}}$ , G. Avolio ${}^{\textrm{\scriptsize 36}}$ , M.K. Ayoub ${}^{\textrm{\scriptsize 15a}}$ , G. Azuelos ${}^{\textrm{\scriptsize 110,al}}$ , H. Bachacou ${}^{\textrm{\scriptsize 144}}$ , K. Bachas ${}^{\textrm{\scriptsize 161}}$ , M. Backes ${}^{\textrm{\scriptsize 134}}$ , F. Backman ${}^{\textrm{\scriptsize 45a,45b}}$ , P. Bagnaia ${}^{\textrm{\scriptsize 73a,73b}}$ , M. Bahmani ${}^{\textrm{\scriptsize 85}}$ , H. Bahrasemani ${}^{\textrm{\scriptsize 151}}$ , A.J. Bailey ${}^{\textrm{\scriptsize 173}}$ , V.R. Bailey ${}^{\textrm{\scriptsize 172}}$ , J.T. Baines ${}^{\textrm{\scriptsize 143}}$ , C. Bakalis ${}^{\textrm{\scriptsize 10}}$ , O.K. Baker ${}^{\textrm{\scriptsize 182}}$ , P.J. Bakker ${}^{\textrm{\scriptsize 120}}$ , E. Bakos ${}^{\textrm{\scriptsize 16}}$ , D. Bakshi Gupta ${}^{\textrm{\scriptsize 8}}$ , S. Balaji ${}^{\textrm{\scriptsize 156}}$ , E.M. Baldin ${}^{\textrm{\scriptsize 122b,122a}}$ , P. Balek ${}^{\textrm{\scriptsize 179}}$ , F. Balli ${}^{\textrm{\scriptsize 144}}$ , W.K. Balunas ${}^{\textrm{\scriptsize 134}}$ , J. Balz ${}^{\textrm{\scriptsize 100}}$ , E. Banas ${}^{\textrm{\scriptsize 85}}$ , M. Bandieramonte ${}^{\textrm{\scriptsize 138}}$ , A. Bandyopadhyay ${}^{\textrm{\scriptsize 24}}$ , Sw. Banerjee ${}^{\textrm{\scriptsize 180,i}}$ , L. Barak ${}^{\textrm{\scriptsize 160}}$ , W.M. Barbe ${}^{\textrm{\scriptsize 38}}$ , E.L. Barberio ${}^{\textrm{\scriptsize 105}}$ , D. Barberis ${}^{\textrm{\scriptsize 55b,55a}}$ , M. Barbero ${}^{\textrm{\scriptsize 102}}$ , G. Barbour ${}^{\textrm{\scriptsize 95}}$ , T. Barillari ${}^{\textrm{\scriptsize 115}}$ , M-S. Barisits ${}^{\textrm{\scriptsize 36}}$ , J. Barkeloo ${}^{\textrm{\scriptsize 131}}$ , T. Barklow ${}^{\textrm{\scriptsize 152}}$ , R. Barnea ${}^{\textrm{\scriptsize 159}}$ , B.M. Barnett ${}^{\textrm{\scriptsize 143}}$ , R.M. Barnett ${}^{\textrm{\scriptsize 18}}$ , Z. Barnovska-Blenessy ${}^{\textrm{\scriptsize 60a}}$ , A. Baroncelli ${}^{\textrm{\scriptsize 60a}}$ , G. Barone ${}^{\textrm{\scriptsize 29}}$ , A.J. Barr ${}^{\textrm{\scriptsize 134}}$ , L. Barranco Navarro ${}^{\textrm{\scriptsize 45a,45b}}$ , F. Barreiro ${}^{\textrm{\scriptsize 99}}$ , J. Barreiro Guimarães da Costa ${}^{\textrm{\scriptsize 15a}}$ , U. Barron ${}^{\textrm{\scriptsize 160}}$ , S. Barsov ${}^{\textrm{\scriptsize 137}}$ , F. Bartels ${}^{\textrm{\scriptsize 61a}}$ , R. Bartoldus ${}^{\textrm{\scriptsize 152}}$ , G. Bartolini ${}^{\textrm{\scriptsize 102}}$ , A.E. Barton ${}^{\textrm{\scriptsize 90}}$ , P. Bartos ${}^{\textrm{\scriptsize 28a}}$ , A. Basalaev ${}^{\textrm{\scriptsize 46}}$ , A. Basan ${}^{\textrm{\scriptsize 100}}$ , A. Bassalat ${}^{\textrm{\scriptsize 65,ai}}$ , M.J. Basso ${}^{\textrm{\scriptsize 166}}$ , R.L. Bates ${}^{\textrm{\scriptsize 57}}$ , S. Batlamous ${}^{\textrm{\scriptsize 35e}}$ , J.R. Batley ${}^{\textrm{\scriptsize 32}}$ , B. Batool ${}^{\textrm{\scriptsize 150}}$ , M. Battaglia ${}^{\textrm{\scriptsize 145}}$ , M. Bauce ${}^{\textrm{\scriptsize 73a,73b}}$ , F. Bauer ${}^{\textrm{\scriptsize 144}}$ , K.T. Bauer ${}^{\textrm{\scriptsize 170}}$ , H.S. Bawa ${}^{\textrm{\scriptsize 31}}$ , A. Bayirli ${}^{\textrm{\scriptsize 12c}}$ , J.B. Beacham ${}^{\textrm{\scriptsize 49}}$ , T. Beau ${}^{\textrm{\scriptsize 135}}$ , P.H. Beauchemin ${}^{\textrm{\scriptsize 169}}$ , F. Becherer ${}^{\textrm{\scriptsize 52}}$ , P. Bechtle ${}^{\textrm{\scriptsize 24}}$ , H.C. Beck ${}^{\textrm{\scriptsize 53}}$ , H.P. Beck ${}^{\textrm{\scriptsize 20,p}}$ , K. Becker ${}^{\textrm{\scriptsize 177}}$ , C. Becot ${}^{\textrm{\scriptsize 46}}$ , A. Beddall ${}^{\textrm{\scriptsize 12d}}$ , A.J. Beddall ${}^{\textrm{\scriptsize 12a}}$ , V.A. Bednyakov ${}^{\textrm{\scriptsize 80}}$ , M. Bedognetti ${}^{\textrm{\scriptsize 120}}$ , C.P. Bee ${}^{\textrm{\scriptsize 154}}$ , T.A. Beermann ${}^{\textrm{\scriptsize 181}}$ , M. Begalli ${}^{\textrm{\scriptsize 81b}}$ , M. Begel ${}^{\textrm{\scriptsize 29}}$ , A. Behera ${}^{\textrm{\scriptsize 154}}$ , J.K. Behr ${}^{\textrm{\scriptsize 46}}$ , F. Beisiegel ${}^{\textrm{\scriptsize 24}}$ , M. Belfkir ${}^{\textrm{\scriptsize 5}}$ , A.S. Bell ${}^{\textrm{\scriptsize 95}}$ , G. Bella ${}^{\textrm{\scriptsize 160}}$ , L. Bellagamba ${}^{\textrm{\scriptsize 23b}}$ , A. Bellerive ${}^{\textrm{\scriptsize 34}}$ , P. Bellos ${}^{\textrm{\scriptsize 9}}$ , K. Beloborodov ${}^{\textrm{\scriptsize 122b,122a}}$ , K. Belotskiy ${}^{\textrm{\scriptsize 112}}$ , N.L. Belyaev ${}^{\textrm{\scriptsize 112}}$ , D. Benchekroun ${}^{\textrm{\scriptsize 35a}}$ , N. Benekos ${}^{\textrm{\scriptsize 10}}$ , Y. Benhammou ${}^{\textrm{\scriptsize 160}}$ , D.P. Benjamin ${}^{\textrm{\scriptsize 6}}$ , M. Benoit ${}^{\textrm{\scriptsize 54}}$ , J.R. Bensinger ${}^{\textrm{\scriptsize 26}}$ , S. Bentvelsen ${}^{\textrm{\scriptsize 120}}$ , L. Beresford ${}^{\textrm{\scriptsize 134}}$ , M. Beretta ${}^{\textrm{\scriptsize 51}}$ , D. Berge ${}^{\textrm{\scriptsize 19}}$ , E. Bergeaas Kuutmann ${}^{\textrm{\scriptsize 171}}$ , N. Berger ${}^{\textrm{\scriptsize 5}}$ , B. Bergmann ${}^{\textrm{\scriptsize 141}}$ , L.J. Bergsten ${}^{\textrm{\scriptsize 26}}$ , J. Beringer ${}^{\textrm{\scriptsize 18}}$ , S. Berlendis ${}^{\textrm{\scriptsize 7}}$ , G. Bernardi ${}^{\textrm{\scriptsize 135}}$ , C. Bernius ${}^{\textrm{\scriptsize 152}}$ , F.U. Bernlochner ${}^{\textrm{\scriptsize 24}}$ , T. Berry ${}^{\textrm{\scriptsize 94}}$ , P. Berta ${}^{\textrm{\scriptsize 100}}$ , C. Bertella ${}^{\textrm{\scriptsize 15a}}$ , A. Berthold ${}^{\textrm{\scriptsize 48}}$ , I.A. Bertram ${}^{\textrm{\scriptsize 90}}$ , O. Bessidskaia Bylund ${}^{\textrm{\scriptsize 181}}$ , N. Besson ${}^{\textrm{\scriptsize 144}}$ , A. Bethani ${}^{\textrm{\scriptsize 101}}$ , S. Bethke ${}^{\textrm{\scriptsize 115}}$ , A. Betti ${}^{\textrm{\scriptsize 42}}$ , A.J. Bevan ${}^{\textrm{\scriptsize 93}}$ , J. Beyer ${}^{\textrm{\scriptsize 115}}$ , D.S. Bhattacharya ${}^{\textrm{\scriptsize 176}}$ , P. Bhattarai ${}^{\textrm{\scriptsize 26}}$ , V.S. Bhopatkar ${}^{\textrm{\scriptsize 6}}$ , R. Bi ${}^{\textrm{\scriptsize 138}}$ , R.M. Bianchi ${}^{\textrm{\scriptsize 138}}$ , O. Biebel ${}^{\textrm{\scriptsize 114}}$ , D. Biedermann ${}^{\textrm{\scriptsize 19}}$ , R. Bielski ${}^{\textrm{\scriptsize 36}}$ , K. Bierwagen ${}^{\textrm{\scriptsize 100}}$ , N.V. Biesuz ${}^{\textrm{\scriptsize 72a,72b}}$ , M. Biglietti ${}^{\textrm{\scriptsize 75a}}$ , T.R.V. Billoud ${}^{\textrm{\scriptsize 110}}$ , M. Bindi ${}^{\textrm{\scriptsize 53}}$ , A. Bingul ${}^{\textrm{\scriptsize 12d}}$ , C. Bini ${}^{\textrm{\scriptsize 73a,73b}}$ , S. Biondi ${}^{\textrm{\scriptsize 23b,23a}}$ , C.J. Birch-sykes ${}^{\textrm{\scriptsize 101}}$ , M. Birman ${}^{\textrm{\scriptsize 179}}$ , T. Bisanz ${}^{\textrm{\scriptsize 53}}$ , J.P. Biswal ${}^{\textrm{\scriptsize 3}}$ , D. Biswas ${}^{\textrm{\scriptsize 180,i}}$ , A. Bitadze ${}^{\textrm{\scriptsize 101}}$ , C. Bittrich ${}^{\textrm{\scriptsize 48}}$ , K. Bjørke ${}^{\textrm{\scriptsize 133}}$ , T. Blazek ${}^{\textrm{\scriptsize 28a}}$ , I. Bloch ${}^{\textrm{\scriptsize 46}}$ , C. Blocker ${}^{\textrm{\scriptsize 26}}$ , A. Blue ${}^{\textrm{\scriptsize 57}}$ , U. Blumenschein ${}^{\textrm{\scriptsize 93}}$ , G.J. Bobbink ${}^{\textrm{\scriptsize 120}}$ , V.S. Bobrovnikov ${}^{\textrm{\scriptsize 122b,122a}}$ , S.S. Bocchetta ${}^{\textrm{\scriptsize 97}}$ , D. Bogavac ${}^{\textrm{\scriptsize 14}}$ , A.G. Bogdanchikov ${}^{\textrm{\scriptsize 122b,122a}}$ , C. Bohm ${}^{\textrm{\scriptsize 45a}}$ , V. Boisvert ${}^{\textrm{\scriptsize 94}}$ , P. Bokan ${}^{\textrm{\scriptsize 53,171,53}}$ , T. Bold ${}^{\textrm{\scriptsize 84a}}$ , A.E. Bolz ${}^{\textrm{\scriptsize 61b}}$ , M. Bomben ${}^{\textrm{\scriptsize 135}}$ , M. Bona ${}^{\textrm{\scriptsize 93}}$ , J.S. Bonilla ${}^{\textrm{\scriptsize 131}}$ , M. Boonekamp ${}^{\textrm{\scriptsize 144}}$ , C.D. Booth ${}^{\textrm{\scriptsize 94}}$ , H.M. Borecka-Bielska ${}^{\textrm{\scriptsize 91}}$ , L.S. Borgna ${}^{\textrm{\scriptsize 95}}$ , A. Borisov ${}^{\textrm{\scriptsize 123}}$ , G. Borissov ${}^{\textrm{\scriptsize 90}}$ , J. Bortfeldt ${}^{\textrm{\scriptsize 36}}$ , D. Bortoletto ${}^{\textrm{\scriptsize 134}}$ , D. Boscherini ${}^{\textrm{\scriptsize 23b}}$ , M. Bosman ${}^{\textrm{\scriptsize 14}}$ , J.D. Bossio Sola ${}^{\textrm{\scriptsize 104}}$ , K. Bouaouda ${}^{\textrm{\scriptsize 35a}}$ , J. Boudreau ${}^{\textrm{\scriptsize 138}}$ , E.V. Bouhova-Thacker ${}^{\textrm{\scriptsize 90}}$ , D. Boumediene ${}^{\textrm{\scriptsize 38}}$ , S.K. Boutle ${}^{\textrm{\scriptsize 57}}$ , A. Boveia ${}^{\textrm{\scriptsize 127}}$ , J. Boyd ${}^{\textrm{\scriptsize 36}}$ , D. Boye ${}^{\textrm{\scriptsize 33c}}$ , I.R. Boyko ${}^{\textrm{\scriptsize 80}}$ , A.J. Bozson ${}^{\textrm{\scriptsize 94}}$ , J. Bracinik ${}^{\textrm{\scriptsize 21}}$ , N. Brahimi ${}^{\textrm{\scriptsize 60d}}$ , G. Brandt ${}^{\textrm{\scriptsize 181}}$ , O. Brandt ${}^{\textrm{\scriptsize 32}}$ , F. Braren ${}^{\textrm{\scriptsize 46}}$ , B. Brau ${}^{\textrm{\scriptsize 103}}$ , J.E. Brau ${}^{\textrm{\scriptsize 131}}$ , W.D. Breaden Madden ${}^{\textrm{\scriptsize 57}}$ , K. Brendlinger ${}^{\textrm{\scriptsize 46}}$ , L. Brenner ${}^{\textrm{\scriptsize 36}}$ , R. Brenner ${}^{\textrm{\scriptsize 171}}$ , S. Bressler ${}^{\textrm{\scriptsize 179}}$ , B. Brickwedde ${}^{\textrm{\scriptsize 100}}$ , D.L. Briglin ${}^{\textrm{\scriptsize 21}}$ , D. Britton ${}^{\textrm{\scriptsize 57}}$ , D. Britzger ${}^{\textrm{\scriptsize 115}}$ , I. Brock ${}^{\textrm{\scriptsize 24}}$ , R. Brock ${}^{\textrm{\scriptsize 107}}$ , G. Brooijmans ${}^{\textrm{\scriptsize 39}}$ , W.K. Brooks ${}^{\textrm{\scriptsize 146d}}$ , E. Brost ${}^{\textrm{\scriptsize 29}}$ , P.A. Bruckman de Renstrom ${}^{\textrm{\scriptsize 85}}$ , B. Brüers ${}^{\textrm{\scriptsize 46}}$ , D. Bruncko ${}^{\textrm{\scriptsize 28b}}$ , A. Bruni ${}^{\textrm{\scriptsize 23b}}$ , G. Bruni ${}^{\textrm{\scriptsize 23b}}$ , L.S. Bruni ${}^{\textrm{\scriptsize 120}}$ , S. Bruno ${}^{\textrm{\scriptsize 74a,74b}}$ , M. Bruschi ${}^{\textrm{\scriptsize 23b}}$ , N. Bruscino ${}^{\textrm{\scriptsize 73a,73b}}$ , L. Bryngemark ${}^{\textrm{\scriptsize 152}}$ , T. Buanes ${}^{\textrm{\scriptsize 17}}$ , Q. Buat ${}^{\textrm{\scriptsize 36}}$ , P. Buchholz ${}^{\textrm{\scriptsize 150}}$ , A.G. Buckley ${}^{\textrm{\scriptsize 57}}$ , I.A. Budagov ${}^{\textrm{\scriptsize 80}}$ , M.K. Bugge ${}^{\textrm{\scriptsize 133}}$ , F. Bührer ${}^{\textrm{\scriptsize 52}}$ , O. Bulekov ${}^{\textrm{\scriptsize 112}}$ , B.A. Bullard ${}^{\textrm{\scriptsize 59}}$ , T.J. Burch ${}^{\textrm{\scriptsize 121}}$ , S. Burdin ${}^{\textrm{\scriptsize 91}}$ , C.D. Burgard ${}^{\textrm{\scriptsize 120}}$ , A.M. Burger ${}^{\textrm{\scriptsize 129}}$ , B. Burghgrave ${}^{\textrm{\scriptsize 8}}$ , J.T.P. Burr ${}^{\textrm{\scriptsize 46}}$ , C.D. Burton ${}^{\textrm{\scriptsize 11}}$ , J.C. Burzynski ${}^{\textrm{\scriptsize 103}}$ , V. Büscher ${}^{\textrm{\scriptsize 100}}$ , E. Buschmann ${}^{\textrm{\scriptsize 53}}$ , P.J. Bussey ${}^{\textrm{\scriptsize 57}}$ , J.M. Butler ${}^{\textrm{\scriptsize 25}}$ , C.M. Buttar ${}^{\textrm{\scriptsize 57}}$ , J.M. Butterworth ${}^{\textrm{\scriptsize 95}}$ , P. Butti ${}^{\textrm{\scriptsize 36}}$ , W. Buttinger ${}^{\textrm{\scriptsize 36}}$ , C.J. Buxo Vazquez ${}^{\textrm{\scriptsize 107}}$ , A. Buzatu ${}^{\textrm{\scriptsize 157}}$ , A.R. Buzykaev ${}^{\textrm{\scriptsize 122b,122a}}$ , G. Cabras ${}^{\textrm{\scriptsize 23b,23a}}$ , S. Cabrera Urbán ${}^{\textrm{\scriptsize 173}}$ , D. Caforio ${}^{\textrm{\scriptsize 56}}$ , H. Cai ${}^{\textrm{\scriptsize 138}}$ , V.M.M. Cairo ${}^{\textrm{\scriptsize 152}}$ , O. Cakir ${}^{\textrm{\scriptsize 4a}}$ , N. Calace ${}^{\textrm{\scriptsize 36}}$ , P. Calafiura ${}^{\textrm{\scriptsize 18}}$ , G. Calderini ${}^{\textrm{\scriptsize 135}}$ , P. Calfayan ${}^{\textrm{\scriptsize 66}}$ , G. Callea ${}^{\textrm{\scriptsize 57}}$ , L.P. Caloba ${}^{\textrm{\scriptsize 81b}}$ , A. Caltabiano ${}^{\textrm{\scriptsize 74a,74b}}$ , S. Calvente Lopez ${}^{\textrm{\scriptsize 99}}$ , D. Calvet ${}^{\textrm{\scriptsize 38}}$ , S. Calvet ${}^{\textrm{\scriptsize 38}}$ , T.P. Calvet ${}^{\textrm{\scriptsize 102}}$ , M. Calvetti ${}^{\textrm{\scriptsize 72a,72b}}$ , R. Camacho Toro ${}^{\textrm{\scriptsize 135}}$ , S. Camarda ${}^{\textrm{\scriptsize 36}}$ , D. Camarero Munoz ${}^{\textrm{\scriptsize 99}}$ , P. Camarri ${}^{\textrm{\scriptsize 74a,74b}}$ , M.T. Camerlingo ${}^{\textrm{\scriptsize 75a,75b}}$ , D. Cameron ${}^{\textrm{\scriptsize 133}}$ , C. Camincher ${}^{\textrm{\scriptsize 36}}$ , S. Campana ${}^{\textrm{\scriptsize 36}}$ , M. Campanelli ${}^{\textrm{\scriptsize 95}}$ , A. Camplani ${}^{\textrm{\scriptsize 40}}$ , V. Canale ${}^{\textrm{\scriptsize 70a,70b}}$ , A. Canesse ${}^{\textrm{\scriptsize 104}}$ , M. Cano Bret ${}^{\textrm{\scriptsize 78}}$ , J. Cantero ${}^{\textrm{\scriptsize 129}}$ , T. Cao ${}^{\textrm{\scriptsize 160}}$ , Y. Cao ${}^{\textrm{\scriptsize 91}}$ , M.D.M. Capeans Garrido ${}^{\textrm{\scriptsize 36}}$ , M. Capua ${}^{\textrm{\scriptsize 41b,41a}}$ , R. Cardarelli ${}^{\textrm{\scriptsize 74a}}$ , F. Cardillo ${}^{\textrm{\scriptsize 148}}$ , G. Carducci ${}^{\textrm{\scriptsize 41b,41a}}$ , I. Carli ${}^{\textrm{\scriptsize 142}}$ , T. Carli ${}^{\textrm{\scriptsize 36}}$ , G. Carlino ${}^{\textrm{\scriptsize 70a}}$ , B.T. Carlson ${}^{\textrm{\scriptsize 138}}$ , E.M. Carlson ${}^{\textrm{\scriptsize 175,167a}}$ , L. Carminati ${}^{\textrm{\scriptsize 69a,69b}}$ , R.M.D. Carney ${}^{\textrm{\scriptsize 152}}$ , S. Caron ${}^{\textrm{\scriptsize 119}}$ , E. Carquin ${}^{\textrm{\scriptsize 146d}}$ , S. Carrá ${}^{\textrm{\scriptsize 46}}$ , G. Carratta ${}^{\textrm{\scriptsize 23b,23a}}$ , J.W.S. Carter ${}^{\textrm{\scriptsize 166}}$ , T.M. Carter ${}^{\textrm{\scriptsize 50}}$ , M.P. Casado ${}^{\textrm{\scriptsize 14,f}}$ , A.F. Casha ${}^{\textrm{\scriptsize 166}}$ , F.L. Castillo ${}^{\textrm{\scriptsize 173}}$ , L. Castillo Garcia ${}^{\textrm{\scriptsize 14}}$ , V. Castillo Gimenez ${}^{\textrm{\scriptsize 173}}$ , N.F. Castro ${}^{\textrm{\scriptsize 139a,139e}}$ , A. Catinaccio ${}^{\textrm{\scriptsize 36}}$ , J.R. Catmore ${}^{\textrm{\scriptsize 133}}$ , A. Cattai ${}^{\textrm{\scriptsize 36}}$ , V. Cavaliere ${}^{\textrm{\scriptsize 29}}$ , V. Cavasinni ${}^{\textrm{\scriptsize 72a,72b}}$ , E. Celebi ${}^{\textrm{\scriptsize 12b}}$ , F. Celli ${}^{\textrm{\scriptsize 134}}$ , K. Cerny ${}^{\textrm{\scriptsize 130}}$ , A.S. Cerqueira ${}^{\textrm{\scriptsize 81a}}$ , A. Cerri ${}^{\textrm{\scriptsize 155}}$ , L. Cerrito ${}^{\textrm{\scriptsize 74a,74b}}$ , F. Cerutti ${}^{\textrm{\scriptsize 18}}$ , A. Cervelli ${}^{\textrm{\scriptsize 23b,23a}}$ , S.A. Cetin ${}^{\textrm{\scriptsize 12b}}$ , Z. Chadi ${}^{\textrm{\scriptsize 35a}}$ , D. Chakraborty ${}^{\textrm{\scriptsize 121}}$ , J. Chan ${}^{\textrm{\scriptsize 180}}$ , W.S. Chan ${}^{\textrm{\scriptsize 120}}$ , W.Y. Chan ${}^{\textrm{\scriptsize 91}}$ , J.D. Chapman ${}^{\textrm{\scriptsize 32}}$ , B. Chargeishvili ${}^{\textrm{\scriptsize 158b}}$ , D.G. Charlton ${}^{\textrm{\scriptsize 21}}$ , T.P. Charman ${}^{\textrm{\scriptsize 93}}$ , C.C. Chau ${}^{\textrm{\scriptsize 34}}$ , S. Che ${}^{\textrm{\scriptsize 127}}$ , S. Chekanov ${}^{\textrm{\scriptsize 6}}$ , S.V. Chekulaev ${}^{\textrm{\scriptsize 167a}}$ , G.A. Chelkov ${}^{\textrm{\scriptsize 80,ag}}$ , B. Chen ${}^{\textrm{\scriptsize 79}}$ , C. Chen ${}^{\textrm{\scriptsize 60a}}$ , C.H. Chen ${}^{\textrm{\scriptsize 79}}$ , H. Chen ${}^{\textrm{\scriptsize 29}}$ , J. Chen ${}^{\textrm{\scriptsize 60a}}$ , J. Chen ${}^{\textrm{\scriptsize 39}}$ , J. Chen ${}^{\textrm{\scriptsize 26}}$ , S. Chen ${}^{\textrm{\scriptsize 136}}$ , S.J. Chen ${}^{\textrm{\scriptsize 15c}}$ , X. Chen ${}^{\textrm{\scriptsize 15b}}$ , Y. Chen ${}^{\textrm{\scriptsize 60a}}$ , Y-H. Chen ${}^{\textrm{\scriptsize 46}}$ , H.C. Cheng ${}^{\textrm{\scriptsize 63a}}$ , H.J. Cheng ${}^{\textrm{\scriptsize 15a}}$ , A. Cheplakov ${}^{\textrm{\scriptsize 80}}$ , E. Cheremushkina ${}^{\textrm{\scriptsize 123}}$ , R. Cherkaoui El Moursli ${}^{\textrm{\scriptsize 35e}}$ , E. Cheu ${}^{\textrm{\scriptsize 7}}$ , K. Cheung ${}^{\textrm{\scriptsize 64}}$ , T.J.A. Chevalérias ${}^{\textrm{\scriptsize 144}}$ , L. Chevalier ${}^{\textrm{\scriptsize 144}}$ , V. Chiarella ${}^{\textrm{\scriptsize 51}}$ , G. Chiarelli ${}^{\textrm{\scriptsize 72a}}$ , G. Chiodini ${}^{\textrm{\scriptsize 68a}}$ , A.S. Chisholm ${}^{\textrm{\scriptsize 21}}$ , A. Chitan ${}^{\textrm{\scriptsize 27b}}$ , I. Chiu ${}^{\textrm{\scriptsize 162}}$ , Y.H. Chiu ${}^{\textrm{\scriptsize 175}}$ , M.V. Chizhov ${}^{\textrm{\scriptsize 80}}$ , K. Choi ${}^{\textrm{\scriptsize 11}}$ , A.R. Chomont ${}^{\textrm{\scriptsize 73a,73b}}$ , Y.S. Chow ${}^{\textrm{\scriptsize 120}}$ , L.D. Christopher ${}^{\textrm{\scriptsize 33e}}$ , M.C. Chu ${}^{\textrm{\scriptsize 63a}}$ , X. Chu ${}^{\textrm{\scriptsize 15a,15d}}$ , J. Chudoba ${}^{\textrm{\scriptsize 140}}$ , J.J. Chwastowski ${}^{\textrm{\scriptsize 85}}$ , L. Chytka ${}^{\textrm{\scriptsize 130}}$ , D. Cieri ${}^{\textrm{\scriptsize 115}}$ , K.M. Ciesla ${}^{\textrm{\scriptsize 85}}$ , D. Cinca ${}^{\textrm{\scriptsize 47}}$ , V. Cindro ${}^{\textrm{\scriptsize 92}}$ , I.A. Cioară ${}^{\textrm{\scriptsize 27b}}$ , A. Ciocio ${}^{\textrm{\scriptsize 18}}$ , F. Cirotto ${}^{\textrm{\scriptsize 70a,70b}}$ , Z.H. Citron ${}^{\textrm{\scriptsize 179,j}}$ , M. Citterio ${}^{\textrm{\scriptsize 69a}}$ , D.A. Ciubotaru ${}^{\textrm{\scriptsize 27b}}$ , B.M. Ciungu ${}^{\textrm{\scriptsize 166}}$ , A. Clark ${}^{\textrm{\scriptsize 54}}$ , M.R. Clark ${}^{\textrm{\scriptsize 39}}$ , P.J. Clark ${}^{\textrm{\scriptsize 50}}$ , S.E. Clawson ${}^{\textrm{\scriptsize 101}}$ , C. Clement ${}^{\textrm{\scriptsize 45a,45b}}$ , Y. Coadou ${}^{\textrm{\scriptsize 102}}$ , M. Cobal ${}^{\textrm{\scriptsize 67a,67c}}$ , A. Coccaro ${}^{\textrm{\scriptsize 55b}}$ , J. Cochran ${}^{\textrm{\scriptsize 79}}$ , R. Coelho Lopes De Sa ${}^{\textrm{\scriptsize 103}}$ , H. Cohen ${}^{\textrm{\scriptsize 160}}$ , A.E.C. Coimbra ${}^{\textrm{\scriptsize 36}}$ , B. Cole ${}^{\textrm{\scriptsize 39}}$ , A.P. Colijn ${}^{\textrm{\scriptsize 120}}$ , J. Collot ${}^{\textrm{\scriptsize 58}}$ , P. Conde Muiño ${}^{\textrm{\scriptsize 139a,139h}}$ , S.H. Connell ${}^{\textrm{\scriptsize 33c}}$ , I.A. Connelly ${}^{\textrm{\scriptsize 57}}$ , S. Constantinescu ${}^{\textrm{\scriptsize 27b}}$ , F. Conventi ${}^{\textrm{\scriptsize 70a,am}}$ , A.M. Cooper-Sarkar ${}^{\textrm{\scriptsize 134}}$ , F. Cormier ${}^{\textrm{\scriptsize 174}}$ , K.J.R. Cormier ${}^{\textrm{\scriptsize 166}}$ , L.D. Corpe ${}^{\textrm{\scriptsize 95}}$ , M. Corradi ${}^{\textrm{\scriptsize 73a,73b}}$ , E.E. Corrigan ${}^{\textrm{\scriptsize 97}}$ , F. Corriveau ${}^{\textrm{\scriptsize 104,ab}}$ , M.J. Costa ${}^{\textrm{\scriptsize 173}}$ , F. Costanza ${}^{\textrm{\scriptsize 5}}$ , D. Costanzo ${}^{\textrm{\scriptsize 148}}$ , G. Cowan ${}^{\textrm{\scriptsize 94}}$ , J.W. Cowley ${}^{\textrm{\scriptsize 32}}$ , J. Crane ${}^{\textrm{\scriptsize 101}}$ , K. Cranmer ${}^{\textrm{\scriptsize 125}}$ , R.A. Creager ${}^{\textrm{\scriptsize 136}}$ , S. Crépé-Renaudin ${}^{\textrm{\scriptsize 58}}$ , F. Crescioli ${}^{\textrm{\scriptsize 135}}$ , M. Cristinziani ${}^{\textrm{\scriptsize 24}}$ , V. Croft ${}^{\textrm{\scriptsize 169}}$ , G. Crosetti ${}^{\textrm{\scriptsize 41b,41a}}$ , A. Cueto ${}^{\textrm{\scriptsize 5}}$ , T. Cuhadar Donszelmann ${}^{\textrm{\scriptsize 170}}$ , H. Cui ${}^{\textrm{\scriptsize 15a,15d}}$ , A.R. Cukierman ${}^{\textrm{\scriptsize 152}}$ , W.R. Cunningham ${}^{\textrm{\scriptsize 57}}$ , S. Czekierda ${}^{\textrm{\scriptsize 85}}$ , P. Czodrowski ${}^{\textrm{\scriptsize 36}}$ , M.M. Czurylo ${}^{\textrm{\scriptsize 61b}}$ , M.J. Da Cunha Sargedas De Sousa ${}^{\textrm{\scriptsize 60b}}$ , J.V. Da Fonseca Pinto ${}^{\textrm{\scriptsize 81b}}$ , C. Da Via ${}^{\textrm{\scriptsize 101}}$ , W. Dabrowski ${}^{\textrm{\scriptsize 84a}}$ , F. Dachs ${}^{\textrm{\scriptsize 36}}$ , T. Dado ${}^{\textrm{\scriptsize 47}}$ , S. Dahbi ${}^{\textrm{\scriptsize 33e}}$ , T. Dai ${}^{\textrm{\scriptsize 106}}$ , C. Dallapiccola ${}^{\textrm{\scriptsize 103}}$ , M. Dam ${}^{\textrm{\scriptsize 40}}$ , G. 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De la Torre ${}^{\textrm{\scriptsize 107}}$ , A. De Maria ${}^{\textrm{\scriptsize 15c}}$ , D. De Pedis ${}^{\textrm{\scriptsize 73a}}$ , A. De Salvo ${}^{\textrm{\scriptsize 73a}}$ , U. De Sanctis ${}^{\textrm{\scriptsize 74a,74b}}$ , M. De Santis ${}^{\textrm{\scriptsize 74a,74b}}$ , A. De Santo ${}^{\textrm{\scriptsize 155}}$ , J.B. De Vivie De Regie ${}^{\textrm{\scriptsize 65}}$ , C. Debenedetti ${}^{\textrm{\scriptsize 145}}$ , D.V. Dedovich ${}^{\textrm{\scriptsize 80}}$ , A.M. Deiana ${}^{\textrm{\scriptsize 42}}$ , J. Del Peso ${}^{\textrm{\scriptsize 99}}$ , Y. Delabat Diaz ${}^{\textrm{\scriptsize 46}}$ , D. Delgove ${}^{\textrm{\scriptsize 65}}$ , F. Deliot ${}^{\textrm{\scriptsize 144}}$ , C.M. Delitzsch ${}^{\textrm{\scriptsize 7}}$ , M. Della Pietra ${}^{\textrm{\scriptsize 70a,70b}}$ , D. Della Volpe ${}^{\textrm{\scriptsize 54}}$ , A. Dell’Acqua ${}^{\textrm{\scriptsize 36}}$ , L. Dell’Asta ${}^{\textrm{\scriptsize 74a,74b}}$ , M. Delmastro ${}^{\textrm{\scriptsize 5}}$ , C. Delporte ${}^{\textrm{\scriptsize 65}}$ , P.A. Delsart ${}^{\textrm{\scriptsize 58}}$ , D.A. DeMarco ${}^{\textrm{\scriptsize 166}}$ , S. Demers ${}^{\textrm{\scriptsize 182}}$ , M. Demichev ${}^{\textrm{\scriptsize 80}}$ , G. Demontigny ${}^{\textrm{\scriptsize 110}}$ , S.P. Denisov ${}^{\textrm{\scriptsize 123}}$ , L. D’Eramo ${}^{\textrm{\scriptsize 121}}$ , D. Derendarz ${}^{\textrm{\scriptsize 85}}$ , J.E. Derkaoui ${}^{\textrm{\scriptsize 35d}}$ , F. Derue ${}^{\textrm{\scriptsize 135}}$ , P. Dervan ${}^{\textrm{\scriptsize 91}}$ , K. Desch ${}^{\textrm{\scriptsize 24}}$ , K. Dette ${}^{\textrm{\scriptsize 166}}$ , C. Deutsch ${}^{\textrm{\scriptsize 24}}$ , M.R. Devesa ${}^{\textrm{\scriptsize 30}}$ , P.O. Deviveiros ${}^{\textrm{\scriptsize 36}}$ , F.A. Di Bello ${}^{\textrm{\scriptsize 73a,73b}}$ , A. Di Ciaccio ${}^{\textrm{\scriptsize 74a,74b}}$ , L. Di Ciaccio ${}^{\textrm{\scriptsize 5}}$ , W.K. 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Dunford ${}^{\textrm{\scriptsize 61a}}$ , A. Duperrin ${}^{\textrm{\scriptsize 102}}$ , H. Duran Yildiz ${}^{\textrm{\scriptsize 4a}}$ , M. Düren ${}^{\textrm{\scriptsize 56}}$ , A. Durglishvili ${}^{\textrm{\scriptsize 158b}}$ , D. Duschinger ${}^{\textrm{\scriptsize 48}}$ , B. Dutta ${}^{\textrm{\scriptsize 46}}$ , D. Duvnjak ${}^{\textrm{\scriptsize 1}}$ , G.I. Dyckes ${}^{\textrm{\scriptsize 136}}$ , M. Dyndal ${}^{\textrm{\scriptsize 36}}$ , S. Dysch ${}^{\textrm{\scriptsize 101}}$ , B.S. Dziedzic ${}^{\textrm{\scriptsize 85}}$ , M.G. Eggleston ${}^{\textrm{\scriptsize 49}}$ , T. Eifert ${}^{\textrm{\scriptsize 8}}$ , G. Eigen ${}^{\textrm{\scriptsize 17}}$ , K. Einsweiler ${}^{\textrm{\scriptsize 18}}$ , T. Ekelof ${}^{\textrm{\scriptsize 171}}$ , H. El Jarrari ${}^{\textrm{\scriptsize 35e}}$ , V. Ellajosyula ${}^{\textrm{\scriptsize 171}}$ , M. Ellert ${}^{\textrm{\scriptsize 171}}$ , F. Ellinghaus ${}^{\textrm{\scriptsize 181}}$ , A.A. Elliot ${}^{\textrm{\scriptsize 93}}$ , N. Ellis ${}^{\textrm{\scriptsize 36}}$ , J. Elmsheuser ${}^{\textrm{\scriptsize 29}}$ , M. Elsing ${}^{\textrm{\scriptsize 36}}$ , D. Emeliyanov ${}^{\textrm{\scriptsize 143}}$ , A. Emerman ${}^{\textrm{\scriptsize 39}}$ , Y. Enari ${}^{\textrm{\scriptsize 162}}$ , M.B. Epland ${}^{\textrm{\scriptsize 49}}$ , J. Erdmann ${}^{\textrm{\scriptsize 47}}$ , A. Ereditato ${}^{\textrm{\scriptsize 20}}$ , P.A. Erland ${}^{\textrm{\scriptsize 85}}$ , M. Errenst ${}^{\textrm{\scriptsize 36}}$ , M. Escalier ${}^{\textrm{\scriptsize 65}}$ , C. Escobar ${}^{\textrm{\scriptsize 173}}$ , O. Estrada Pastor ${}^{\textrm{\scriptsize 173}}$ , E. Etzion ${}^{\textrm{\scriptsize 160}}$ , H. Evans ${}^{\textrm{\scriptsize 66}}$ , M.O. Evans ${}^{\textrm{\scriptsize 155}}$ , A. Ezhilov ${}^{\textrm{\scriptsize 137}}$ , F. Fabbri ${}^{\textrm{\scriptsize 57}}$ , L. Fabbri ${}^{\textrm{\scriptsize 23b,23a}}$ , V. Fabiani ${}^{\textrm{\scriptsize 119}}$ , G. Facini ${}^{\textrm{\scriptsize 177}}$ , R.M. Faisca Rodrigues Pereira ${}^{\textrm{\scriptsize 139a}}$ , R.M. Fakhrutdinov ${}^{\textrm{\scriptsize 123}}$ , S. Falciano ${}^{\textrm{\scriptsize 73a}}$ , P.J. Falke ${}^{\textrm{\scriptsize 24}}$ , S. Falke ${}^{\textrm{\scriptsize 36}}$ , J. Faltova ${}^{\textrm{\scriptsize 142}}$ , Y. Fang ${}^{\textrm{\scriptsize 15a}}$ , Y. Fang ${}^{\textrm{\scriptsize 15a}}$ , G. Fanourakis ${}^{\textrm{\scriptsize 44}}$ , M. Fanti ${}^{\textrm{\scriptsize 69a,69b}}$ , M. Faraj ${}^{\textrm{\scriptsize 67a,67c,q}}$ , A. Farbin ${}^{\textrm{\scriptsize 8}}$ , A. Farilla ${}^{\textrm{\scriptsize 75a}}$ , E.M. Farina ${}^{\textrm{\scriptsize 71a,71b}}$ , T. Farooque ${}^{\textrm{\scriptsize 107}}$ , S.M. Farrington ${}^{\textrm{\scriptsize 50}}$ , P. Farthouat ${}^{\textrm{\scriptsize 36}}$ , F. Fassi ${}^{\textrm{\scriptsize 35e}}$ , P. Fassnacht ${}^{\textrm{\scriptsize 36}}$ , D. Fassouliotis ${}^{\textrm{\scriptsize 9}}$ , M. Faucci Giannelli ${}^{\textrm{\scriptsize 50}}$ , W.J. Fawcett ${}^{\textrm{\scriptsize 32}}$ , L. Fayard ${}^{\textrm{\scriptsize 65}}$ , O.L. Fedin ${}^{\textrm{\scriptsize 137,o}}$ , W. Fedorko ${}^{\textrm{\scriptsize 174}}$ , A. Fehr ${}^{\textrm{\scriptsize 20}}$ , M. Feickert ${}^{\textrm{\scriptsize 172}}$ , L. Feligioni ${}^{\textrm{\scriptsize 102}}$ , A. Fell ${}^{\textrm{\scriptsize 148}}$ , C. Feng ${}^{\textrm{\scriptsize 60b}}$ , M. Feng ${}^{\textrm{\scriptsize 49}}$ , M.J. Fenton ${}^{\textrm{\scriptsize 170}}$ , A.B. Fenyuk ${}^{\textrm{\scriptsize 123}}$ , S.W. Ferguson ${}^{\textrm{\scriptsize 43}}$ , J. Ferrando ${}^{\textrm{\scriptsize 46}}$ , A. Ferrante ${}^{\textrm{\scriptsize 172}}$ , A. Ferrari ${}^{\textrm{\scriptsize 171}}$ , P. Ferrari ${}^{\textrm{\scriptsize 120}}$ , R. Ferrari ${}^{\textrm{\scriptsize 71a}}$ , D.E. Ferreira de Lima ${}^{\textrm{\scriptsize 61b}}$ , A. Ferrer ${}^{\textrm{\scriptsize 173}}$ , D. 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Freund ${}^{\textrm{\scriptsize 81b}}$ , E.M. Freundlich ${}^{\textrm{\scriptsize 47}}$ , D.C. Frizzell ${}^{\textrm{\scriptsize 128}}$ , D. Froidevaux ${}^{\textrm{\scriptsize 36}}$ , J.A. Frost ${}^{\textrm{\scriptsize 134}}$ , M. Fujimoto ${}^{\textrm{\scriptsize 126}}$ , C. Fukunaga ${}^{\textrm{\scriptsize 163}}$ , E. Fullana Torregrosa ${}^{\textrm{\scriptsize 173}}$ , T. Fusayasu ${}^{\textrm{\scriptsize 116}}$ , J. Fuster ${}^{\textrm{\scriptsize 173}}$ , A. Gabrielli ${}^{\textrm{\scriptsize 23b,23a}}$ , A. Gabrielli ${}^{\textrm{\scriptsize 36}}$ , S. Gadatsch ${}^{\textrm{\scriptsize 54}}$ , P. Gadow ${}^{\textrm{\scriptsize 115}}$ , G. Gagliardi ${}^{\textrm{\scriptsize 55b,55a}}$ , L.G. Gagnon ${}^{\textrm{\scriptsize 110}}$ , G.E. Gallardo ${}^{\textrm{\scriptsize 134}}$ , E.J. Gallas ${}^{\textrm{\scriptsize 134}}$ , B.J. Gallop ${}^{\textrm{\scriptsize 143}}$ , G. Galster ${}^{\textrm{\scriptsize 40}}$ , R. Gamboa Goni ${}^{\textrm{\scriptsize 93}}$ , K.K. Gan ${}^{\textrm{\scriptsize 127}}$ , S. Ganguly ${}^{\textrm{\scriptsize 179}}$ , J. Gao ${}^{\textrm{\scriptsize 60a}}$ , Y. Gao ${}^{\textrm{\scriptsize 50}}$ , Y.S. Gao ${}^{\textrm{\scriptsize 31,l}}$ , F.M. Garay Walls ${}^{\textrm{\scriptsize 146a}}$ , C. García ${}^{\textrm{\scriptsize 173}}$ , J.E. García Navarro ${}^{\textrm{\scriptsize 173}}$ , J.A. García Pascual ${}^{\textrm{\scriptsize 15a}}$ , C. Garcia-Argos ${}^{\textrm{\scriptsize 52}}$ , M. Garcia-Sciveres ${}^{\textrm{\scriptsize 18}}$ , R.W. Gardner ${}^{\textrm{\scriptsize 37}}$ , N. Garelli ${}^{\textrm{\scriptsize 152}}$ , S. Gargiulo ${}^{\textrm{\scriptsize 52}}$ , C.A. Garner ${}^{\textrm{\scriptsize 166}}$ , V. Garonne ${}^{\textrm{\scriptsize 133}}$ , S.J. Gasiorowski ${}^{\textrm{\scriptsize 147}}$ , P. Gaspar ${}^{\textrm{\scriptsize 81b}}$ , A. Gaudiello ${}^{\textrm{\scriptsize 55b,55a}}$ , G. Gaudio ${}^{\textrm{\scriptsize 71a}}$ , I.L. Gavrilenko ${}^{\textrm{\scriptsize 111}}$ , A. 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Ghosh ${}^{\textrm{\scriptsize 78}}$ , B. Giacobbe ${}^{\textrm{\scriptsize 23b}}$ , S. Giagu ${}^{\textrm{\scriptsize 73a,73b}}$ , N. Giangiacomi ${}^{\textrm{\scriptsize 23b,23a}}$ , P. Giannetti ${}^{\textrm{\scriptsize 72a}}$ , A. Giannini ${}^{\textrm{\scriptsize 70a,70b}}$ , G. Giannini ${}^{\textrm{\scriptsize 14}}$ , S.M. Gibson ${}^{\textrm{\scriptsize 94}}$ , M. Gignac ${}^{\textrm{\scriptsize 145}}$ , D.T. Gil ${}^{\textrm{\scriptsize 84b}}$ , D. Gillberg ${}^{\textrm{\scriptsize 34}}$ , G. Gilles ${}^{\textrm{\scriptsize 181}}$ , D.M. Gingrich ${}^{\textrm{\scriptsize 3,al}}$ , M.P. Giordani ${}^{\textrm{\scriptsize 67a,67c}}$ , P.F. Giraud ${}^{\textrm{\scriptsize 144}}$ , G. Giugliarelli ${}^{\textrm{\scriptsize 67a,67c}}$ , D. Giugni ${}^{\textrm{\scriptsize 69a}}$ , F. Giuli ${}^{\textrm{\scriptsize 74a,74b}}$ , S. Gkaitatzis ${}^{\textrm{\scriptsize 161}}$ , I. Gkialas ${}^{\textrm{\scriptsize 9,g}}$ , E.L. Gkougkousis ${}^{\textrm{\scriptsize 14}}$ , P. 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Goy ${}^{\textrm{\scriptsize 5}}$ , I. Grabowska-Bold ${}^{\textrm{\scriptsize 84a}}$ , E.C. Graham ${}^{\textrm{\scriptsize 91}}$ , J. Gramling ${}^{\textrm{\scriptsize 170}}$ , E. Gramstad ${}^{\textrm{\scriptsize 133}}$ , S. Grancagnolo ${}^{\textrm{\scriptsize 19}}$ , M. Grandi ${}^{\textrm{\scriptsize 155}}$ , V. Gratchev ${}^{\textrm{\scriptsize 137}}$ , P.M. Gravila ${}^{\textrm{\scriptsize 27f}}$ , F.G. Gravili ${}^{\textrm{\scriptsize 68a,68b}}$ , C. Gray ${}^{\textrm{\scriptsize 57}}$ , H.M. Gray ${}^{\textrm{\scriptsize 18}}$ , C. Grefe ${}^{\textrm{\scriptsize 24}}$ , K. Gregersen ${}^{\textrm{\scriptsize 97}}$ , I.M. Gregor ${}^{\textrm{\scriptsize 46}}$ , P. Grenier ${}^{\textrm{\scriptsize 152}}$ , K. Grevtsov ${}^{\textrm{\scriptsize 46}}$ , C. Grieco ${}^{\textrm{\scriptsize 14}}$ , N.A. Grieser ${}^{\textrm{\scriptsize 128}}$ , A.A. Grillo ${}^{\textrm{\scriptsize 145}}$ , K. Grimm ${}^{\textrm{\scriptsize 31,k}}$ , S. Grinstein ${}^{\textrm{\scriptsize 14,w}}$ , J.-F. Grivaz ${}^{\textrm{\scriptsize 65}}$ , S. Groh ${}^{\textrm{\scriptsize 100}}$ , E. Gross ${}^{\textrm{\scriptsize 179}}$ , J. Grosse-Knetter ${}^{\textrm{\scriptsize 53}}$ , Z.J. Grout ${}^{\textrm{\scriptsize 95}}$ , C. Grud ${}^{\textrm{\scriptsize 106}}$ , A. Grummer ${}^{\textrm{\scriptsize 118}}$ , J.C. Grundy ${}^{\textrm{\scriptsize 134}}$ , L. Guan ${}^{\textrm{\scriptsize 106}}$ , W. Guan ${}^{\textrm{\scriptsize 180}}$ , C. Gubbels ${}^{\textrm{\scriptsize 174}}$ , J. Guenther ${}^{\textrm{\scriptsize 36}}$ , A. Guerguichon ${}^{\textrm{\scriptsize 65}}$ , J.G.R. Guerrero Rojas ${}^{\textrm{\scriptsize 173}}$ , F. Guescini ${}^{\textrm{\scriptsize 115}}$ , D. Guest ${}^{\textrm{\scriptsize 170}}$ , R. Gugel ${}^{\textrm{\scriptsize 100}}$ , T. Guillemin ${}^{\textrm{\scriptsize 5}}$ , S. Guindon ${}^{\textrm{\scriptsize 36}}$ , U. Gul ${}^{\textrm{\scriptsize 57}}$ , J. Guo ${}^{\textrm{\scriptsize 60c}}$ , W. Guo ${}^{\textrm{\scriptsize 106}}$ , Y. Guo ${}^{\textrm{\scriptsize 60a}}$ , Z. Guo ${}^{\textrm{\scriptsize 102}}$ , R. Gupta ${}^{\textrm{\scriptsize 46}}$ , S. Gurbuz ${}^{\textrm{\scriptsize 12c}}$ , G. Gustavino ${}^{\textrm{\scriptsize 128}}$ , M. Guth ${}^{\textrm{\scriptsize 52}}$ , P. Gutierrez ${}^{\textrm{\scriptsize 128}}$ , C. Gutschow ${}^{\textrm{\scriptsize 95}}$ , C. Guyot ${}^{\textrm{\scriptsize 144}}$ , C. Gwenlan ${}^{\textrm{\scriptsize 134}}$ , C.B. Gwilliam ${}^{\textrm{\scriptsize 91}}$ , E.S. Haaland ${}^{\textrm{\scriptsize 133}}$ , A. Haas ${}^{\textrm{\scriptsize 125}}$ , C. Haber ${}^{\textrm{\scriptsize 18}}$ , H.K. Hadavand ${}^{\textrm{\scriptsize 8}}$ , A. Hadef ${}^{\textrm{\scriptsize 60a}}$ , M. Haleem ${}^{\textrm{\scriptsize 176}}$ , J. Haley ${}^{\textrm{\scriptsize 129}}$ , J.J. Hall ${}^{\textrm{\scriptsize 148}}$ , G. Halladjian ${}^{\textrm{\scriptsize 107}}$ , G.D. Hallewell ${}^{\textrm{\scriptsize 102}}$ , K. Hamano ${}^{\textrm{\scriptsize 175}}$ , H. Hamdaoui ${}^{\textrm{\scriptsize 35e}}$ , M. Hamer ${}^{\textrm{\scriptsize 24}}$ , G.N. Hamity ${}^{\textrm{\scriptsize 50}}$ , K. Han ${}^{\textrm{\scriptsize 60a,v}}$ , L. Han ${}^{\textrm{\scriptsize 60a}}$ , S. Han ${}^{\textrm{\scriptsize 18}}$ , Y.F. Han ${}^{\textrm{\scriptsize 166}}$ , K. Hanagaki ${}^{\textrm{\scriptsize 82,t}}$ , M. Hance ${}^{\textrm{\scriptsize 145}}$ , D.M. Handl ${}^{\textrm{\scriptsize 114}}$ , M.D. Hank ${}^{\textrm{\scriptsize 37}}$ , R. Hankache ${}^{\textrm{\scriptsize 135}}$ , E. Hansen ${}^{\textrm{\scriptsize 97}}$ , J.B. Hansen ${}^{\textrm{\scriptsize 40}}$ , J.D. Hansen ${}^{\textrm{\scriptsize 40}}$ , M.C. Hansen ${}^{\textrm{\scriptsize 24}}$ , P.H. Hansen ${}^{\textrm{\scriptsize 40}}$ , E.C. Hanson ${}^{\textrm{\scriptsize 101}}$ , K. Hara ${}^{\textrm{\scriptsize 168}}$ , T. Harenberg ${}^{\textrm{\scriptsize 181}}$ , S. Harkusha ${}^{\textrm{\scriptsize 108}}$ , P.F. 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Heath ${}^{\textrm{\scriptsize 50}}$ , V. Hedberg ${}^{\textrm{\scriptsize 97}}$ , S. Heer ${}^{\textrm{\scriptsize 24}}$ , A.L. Heggelund ${}^{\textrm{\scriptsize 133}}$ , C. Heidegger ${}^{\textrm{\scriptsize 52}}$ , K.K. Heidegger ${}^{\textrm{\scriptsize 52}}$ , W.D. Heidorn ${}^{\textrm{\scriptsize 79}}$ , J. Heilman ${}^{\textrm{\scriptsize 34}}$ , S. Heim ${}^{\textrm{\scriptsize 46}}$ , T. Heim ${}^{\textrm{\scriptsize 18}}$ , B. Heinemann ${}^{\textrm{\scriptsize 46,aj}}$ , J.G. Heinlein ${}^{\textrm{\scriptsize 136}}$ , J.J. Heinrich ${}^{\textrm{\scriptsize 131}}$ , L. Heinrich ${}^{\textrm{\scriptsize 36}}$ , J. Hejbal ${}^{\textrm{\scriptsize 140}}$ , L. Helary ${}^{\textrm{\scriptsize 46}}$ , A. Held ${}^{\textrm{\scriptsize 125}}$ , S. Hellesund ${}^{\textrm{\scriptsize 133}}$ , C.M. Helling ${}^{\textrm{\scriptsize 145}}$ , S. Hellman ${}^{\textrm{\scriptsize 45a,45b}}$ , C. Helsens ${}^{\textrm{\scriptsize 36}}$ , R.C.W. Henderson ${}^{\textrm{\scriptsize 90}}$ , Y. Heng ${}^{\textrm{\scriptsize 180}}$ , L. Henkelmann ${}^{\textrm{\scriptsize 32}}$ , A.M. Henriques Correia ${}^{\textrm{\scriptsize 36}}$ , H. Herde ${}^{\textrm{\scriptsize 26}}$ , Y. Hernández Jiménez ${}^{\textrm{\scriptsize 33e}}$ , H. Herr ${}^{\textrm{\scriptsize 100}}$ , M.G. Herrmann ${}^{\textrm{\scriptsize 114}}$ , T. Herrmann ${}^{\textrm{\scriptsize 48}}$ , G. Herten ${}^{\textrm{\scriptsize 52}}$ , R. Hertenberger ${}^{\textrm{\scriptsize 114}}$ , L. Hervas ${}^{\textrm{\scriptsize 36}}$ , T.C. Herwig ${}^{\textrm{\scriptsize 136}}$ , G.G. Hesketh ${}^{\textrm{\scriptsize 95}}$ , N.P. Hessey ${}^{\textrm{\scriptsize 167a}}$ , H. Hibi ${}^{\textrm{\scriptsize 83}}$ , A. Higashida ${}^{\textrm{\scriptsize 162}}$ , S. Higashino ${}^{\textrm{\scriptsize 82}}$ , E. Higón-Rodriguez ${}^{\textrm{\scriptsize 173}}$ , K. Hildebrand ${}^{\textrm{\scriptsize 37}}$ , J.C. Hill ${}^{\textrm{\scriptsize 32}}$ , K.K. Hill ${}^{\textrm{\scriptsize 29}}$ , K.H. 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Honig ${}^{\textrm{\scriptsize 52}}$ , A. Hönle ${}^{\textrm{\scriptsize 115}}$ , B.H. Hooberman ${}^{\textrm{\scriptsize 172}}$ , W.H. Hopkins ${}^{\textrm{\scriptsize 6}}$ , Y. Horii ${}^{\textrm{\scriptsize 117}}$ , P. Horn ${}^{\textrm{\scriptsize 48}}$ , L.A. Horyn ${}^{\textrm{\scriptsize 37}}$ , S. Hou ${}^{\textrm{\scriptsize 157}}$ , A. Hoummada ${}^{\textrm{\scriptsize 35a}}$ , J. Howarth ${}^{\textrm{\scriptsize 57}}$ , J. Hoya ${}^{\textrm{\scriptsize 89}}$ , M. Hrabovsky ${}^{\textrm{\scriptsize 130}}$ , J. Hrdinka ${}^{\textrm{\scriptsize 77}}$ , J. Hrivnac ${}^{\textrm{\scriptsize 65}}$ , A. Hrynevich ${}^{\textrm{\scriptsize 109}}$ , T. Hryn’ova ${}^{\textrm{\scriptsize 5}}$ , P.J. Hsu ${}^{\textrm{\scriptsize 64}}$ , S.-C. Hsu ${}^{\textrm{\scriptsize 147}}$ , Q. Hu ${}^{\textrm{\scriptsize 29}}$ , S. Hu ${}^{\textrm{\scriptsize 60c}}$ , Y.F. Hu ${}^{\textrm{\scriptsize 15a,15d,an}}$ , D.P. Huang ${}^{\textrm{\scriptsize 95}}$ , Y. Huang ${}^{\textrm{\scriptsize 60a}}$ , Y. Huang ${}^{\textrm{\scriptsize 15a}}$ , Z. Hubacek ${}^{\textrm{\scriptsize 141}}$ , F. Hubaut ${}^{\textrm{\scriptsize 102}}$ , M. Huebner ${}^{\textrm{\scriptsize 24}}$ , F. Huegging ${}^{\textrm{\scriptsize 24}}$ , T.B. Huffman ${}^{\textrm{\scriptsize 134}}$ , M. Huhtinen ${}^{\textrm{\scriptsize 36}}$ , R. Hulsken ${}^{\textrm{\scriptsize 58}}$ , R.F.H. Hunter ${}^{\textrm{\scriptsize 34}}$ , P. Huo ${}^{\textrm{\scriptsize 154}}$ , N. Huseynov ${}^{\textrm{\scriptsize 80,ac}}$ , J. Huston ${}^{\textrm{\scriptsize 107}}$ , J. Huth ${}^{\textrm{\scriptsize 59}}$ , R. Hyneman ${}^{\textrm{\scriptsize 106}}$ , S. Hyrych ${}^{\textrm{\scriptsize 28a}}$ , G. Iacobucci ${}^{\textrm{\scriptsize 54}}$ , G. Iakovidis ${}^{\textrm{\scriptsize 29}}$ , I. Ibragimov ${}^{\textrm{\scriptsize 150}}$ , L. Iconomidou-Fayard ${}^{\textrm{\scriptsize 65}}$ , P. Iengo ${}^{\textrm{\scriptsize 36}}$ , R. Ignazzi ${}^{\textrm{\scriptsize 40}}$ , O. Igonkina ${}^{\textrm{\scriptsize 120,y,*}}$ , R. Iguchi ${}^{\textrm{\scriptsize 162}}$ , T. Iizawa ${}^{\textrm{\scriptsize 54}}$ , Y. Ikegami ${}^{\textrm{\scriptsize 82}}$ , M. Ikeno ${}^{\textrm{\scriptsize 82}}$ , D. Iliadis ${}^{\textrm{\scriptsize 161}}$ , N. Ilic ${}^{\textrm{\scriptsize 119,166,ab}}$ , F. Iltzsche ${}^{\textrm{\scriptsize 48}}$ , H. Imam ${}^{\textrm{\scriptsize 35a}}$ , G. Introzzi ${}^{\textrm{\scriptsize 71a,71b}}$ , M. Iodice ${}^{\textrm{\scriptsize 75a}}$ , K. Iordanidou ${}^{\textrm{\scriptsize 167a}}$ , V. Ippolito ${}^{\textrm{\scriptsize 73a,73b}}$ , M.F. Isacson ${}^{\textrm{\scriptsize 171}}$ , M. Ishino ${}^{\textrm{\scriptsize 162}}$ , W. Islam ${}^{\textrm{\scriptsize 129}}$ , C. Issever ${}^{\textrm{\scriptsize 19,46}}$ , S. Istin ${}^{\textrm{\scriptsize 159}}$ , F. Ito ${}^{\textrm{\scriptsize 168}}$ , J.M. Iturbe Ponce ${}^{\textrm{\scriptsize 63a}}$ , R. Iuppa ${}^{\textrm{\scriptsize 76a,76b}}$ , A. Ivina ${}^{\textrm{\scriptsize 179}}$ , H. Iwasaki ${}^{\textrm{\scriptsize 82}}$ , J.M. Izen ${}^{\textrm{\scriptsize 43}}$ , V. Izzo ${}^{\textrm{\scriptsize 70a}}$ , P. Jacka ${}^{\textrm{\scriptsize 140}}$ , P. Jackson ${}^{\textrm{\scriptsize 1}}$ , R.M. Jacobs ${}^{\textrm{\scriptsize 46}}$ , B.P. Jaeger ${}^{\textrm{\scriptsize 151}}$ , V. Jain ${}^{\textrm{\scriptsize 2}}$ , G. Jäkel ${}^{\textrm{\scriptsize 181}}$ , K.B. Jakobi ${}^{\textrm{\scriptsize 100}}$ , K. Jakobs ${}^{\textrm{\scriptsize 52}}$ , T. Jakoubek ${}^{\textrm{\scriptsize 179}}$ , J. Jamieson ${}^{\textrm{\scriptsize 57}}$ , K.W. Janas ${}^{\textrm{\scriptsize 84a}}$ , R. Jansky ${}^{\textrm{\scriptsize 54}}$ , M. Janus ${}^{\textrm{\scriptsize 53}}$ , P.A. Janus ${}^{\textrm{\scriptsize 84a}}$ , G. Jarlskog ${}^{\textrm{\scriptsize 97}}$ , A.E. Jaspan ${}^{\textrm{\scriptsize 91}}$ , N. Javadov ${}^{\textrm{\scriptsize 80,ac}}$ , T. Javůrek ${}^{\textrm{\scriptsize 36}}$ , M. Javurkova ${}^{\textrm{\scriptsize 103}}$ , F. Jeanneau ${}^{\textrm{\scriptsize 144}}$ , L. Jeanty ${}^{\textrm{\scriptsize 131}}$ , J. Jejelava ${}^{\textrm{\scriptsize 158a}}$ , P. Jenni ${}^{\textrm{\scriptsize 52,c}}$ , N. Jeong ${}^{\textrm{\scriptsize 46}}$ , S. Jézéquel ${}^{\textrm{\scriptsize 5}}$ , H. Ji ${}^{\textrm{\scriptsize 180}}$ , J. Jia ${}^{\textrm{\scriptsize 154}}$ , H. Jiang ${}^{\textrm{\scriptsize 79}}$ , Y. Jiang ${}^{\textrm{\scriptsize 60a}}$ , Z. Jiang ${}^{\textrm{\scriptsize 152}}$ , S. Jiggins ${}^{\textrm{\scriptsize 52}}$ , F.A. Jimenez Morales ${}^{\textrm{\scriptsize 38}}$ , J. Jimenez Pena ${}^{\textrm{\scriptsize 115}}$ , S. Jin ${}^{\textrm{\scriptsize 15c}}$ , A. Jinaru ${}^{\textrm{\scriptsize 27b}}$ , O. Jinnouchi ${}^{\textrm{\scriptsize 164}}$ , H. Jivan ${}^{\textrm{\scriptsize 33e}}$ , P. Johansson ${}^{\textrm{\scriptsize 148}}$ , K.A. Johns ${}^{\textrm{\scriptsize 7}}$ , C.A. Johnson ${}^{\textrm{\scriptsize 66}}$ , R.W.L. Jones ${}^{\textrm{\scriptsize 90}}$ , S.D. Jones ${}^{\textrm{\scriptsize 155}}$ , T.J. Jones ${}^{\textrm{\scriptsize 91}}$ , J. Jongmanns ${}^{\textrm{\scriptsize 61a}}$ , J. Jovicevic ${}^{\textrm{\scriptsize 36}}$ , X. Ju ${}^{\textrm{\scriptsize 18}}$ , J.J. Junggeburth ${}^{\textrm{\scriptsize 115}}$ , A. Juste Rozas ${}^{\textrm{\scriptsize 14,w}}$ , A. Kaczmarska ${}^{\textrm{\scriptsize 85}}$ , M. Kado ${}^{\textrm{\scriptsize 73a,73b}}$ , H. Kagan ${}^{\textrm{\scriptsize 127}}$ , M. Kagan ${}^{\textrm{\scriptsize 152}}$ , A. Kahn ${}^{\textrm{\scriptsize 39}}$ , C. Kahra ${}^{\textrm{\scriptsize 100}}$ , T. Kaji ${}^{\textrm{\scriptsize 178}}$ , E. Kajomovitz ${}^{\textrm{\scriptsize 159}}$ , C.W. Kalderon ${}^{\textrm{\scriptsize 29}}$ , A. Kaluza ${}^{\textrm{\scriptsize 100}}$ , A. Kamenshchikov ${}^{\textrm{\scriptsize 123}}$ , M. Kaneda ${}^{\textrm{\scriptsize 162}}$ , N.J. Kang ${}^{\textrm{\scriptsize 145}}$ , S. Kang ${}^{\textrm{\scriptsize 79}}$ , Y. Kano ${}^{\textrm{\scriptsize 117}}$ , J. Kanzaki ${}^{\textrm{\scriptsize 82}}$ , L.S. Kaplan ${}^{\textrm{\scriptsize 180}}$ , D. Kar ${}^{\textrm{\scriptsize 33e}}$ , K. Karava ${}^{\textrm{\scriptsize 134}}$ , M.J. Kareem ${}^{\textrm{\scriptsize 167b}}$ , I. Karkanias ${}^{\textrm{\scriptsize 161}}$ , S.N. Karpov ${}^{\textrm{\scriptsize 80}}$ , Z.M. Karpova ${}^{\textrm{\scriptsize 80}}$ , V. Kartvelishvili ${}^{\textrm{\scriptsize 90}}$ , A.N. Karyukhin ${}^{\textrm{\scriptsize 123}}$ , A. Kastanas ${}^{\textrm{\scriptsize 45a,45b}}$ , C. Kato ${}^{\textrm{\scriptsize 60d,60c}}$ , J. Katzy ${}^{\textrm{\scriptsize 46}}$ , K. Kawade ${}^{\textrm{\scriptsize 149}}$ , K. Kawagoe ${}^{\textrm{\scriptsize 88}}$ , T. Kawaguchi ${}^{\textrm{\scriptsize 117}}$ , T. Kawamoto ${}^{\textrm{\scriptsize 144}}$ , G. Kawamura ${}^{\textrm{\scriptsize 53}}$ , E.F. Kay ${}^{\textrm{\scriptsize 175}}$ , S. Kazakos ${}^{\textrm{\scriptsize 14}}$ , V.F. 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Khoo ${}^{\textrm{\scriptsize 54}}$ , G. Khoriauli ${}^{\textrm{\scriptsize 176}}$ , E. Khramov ${}^{\textrm{\scriptsize 80}}$ , J. Khubua ${}^{\textrm{\scriptsize 158b}}$ , S. Kido ${}^{\textrm{\scriptsize 83}}$ , M. Kiehn ${}^{\textrm{\scriptsize 54}}$ , C.R. Kilby ${}^{\textrm{\scriptsize 94}}$ , E. Kim ${}^{\textrm{\scriptsize 164}}$ , Y.K. Kim ${}^{\textrm{\scriptsize 37}}$ , N. Kimura ${}^{\textrm{\scriptsize 95}}$ , B.T. King ${}^{\textrm{\scriptsize 91,*}}$ , A. Kirchhoff ${}^{\textrm{\scriptsize 53}}$ , D. Kirchmeier ${}^{\textrm{\scriptsize 48}}$ , J. Kirk ${}^{\textrm{\scriptsize 143}}$ , A.E. Kiryunin ${}^{\textrm{\scriptsize 115}}$ , T. Kishimoto ${}^{\textrm{\scriptsize 162}}$ , D.P. Kisliuk ${}^{\textrm{\scriptsize 166}}$ , V. Kitali ${}^{\textrm{\scriptsize 46}}$ , C. Kitsaki ${}^{\textrm{\scriptsize 10}}$ , O. Kivernyk ${}^{\textrm{\scriptsize 24}}$ , T. Klapdor-Kleingrothaus ${}^{\textrm{\scriptsize 52}}$ , M. Klassen ${}^{\textrm{\scriptsize 61a}}$ , C. Klein ${}^{\textrm{\scriptsize 34}}$ , M.H. Klein ${}^{\textrm{\scriptsize 106}}$ , M. Klein ${}^{\textrm{\scriptsize 91}}$ , U. Klein ${}^{\textrm{\scriptsize 91}}$ , K. Kleinknecht ${}^{\textrm{\scriptsize 100}}$ , P. Klimek ${}^{\textrm{\scriptsize 121}}$ , A. Klimentov ${}^{\textrm{\scriptsize 29}}$ , T. Klingl ${}^{\textrm{\scriptsize 24}}$ , T. Klioutchnikova ${}^{\textrm{\scriptsize 36}}$ , F.F. Klitzner ${}^{\textrm{\scriptsize 114}}$ , P. Kluit ${}^{\textrm{\scriptsize 120}}$ , S. Kluth ${}^{\textrm{\scriptsize 115}}$ , E. Kneringer ${}^{\textrm{\scriptsize 77}}$ , E.B.F.G. Knoops ${}^{\textrm{\scriptsize 102}}$ , A. Knue ${}^{\textrm{\scriptsize 52}}$ , D. Kobayashi ${}^{\textrm{\scriptsize 88}}$ , T. Kobayashi ${}^{\textrm{\scriptsize 162}}$ , M. Kobel ${}^{\textrm{\scriptsize 48}}$ , M. Kocian ${}^{\textrm{\scriptsize 152}}$ , T. Kodama ${}^{\textrm{\scriptsize 162}}$ , P. Kodys ${}^{\textrm{\scriptsize 142}}$ , D.M. Koeck ${}^{\textrm{\scriptsize 155}}$ , P.T. Koenig ${}^{\textrm{\scriptsize 24}}$ , T. Koffas ${}^{\textrm{\scriptsize 34}}$ , N.M. Köhler ${}^{\textrm{\scriptsize 36}}$ , M. Kolb ${}^{\textrm{\scriptsize 144}}$ , I. Koletsou ${}^{\textrm{\scriptsize 5}}$ , T. Komarek ${}^{\textrm{\scriptsize 130}}$ , T. Kondo ${}^{\textrm{\scriptsize 82}}$ , K. Köneke ${}^{\textrm{\scriptsize 52}}$ , A.X.Y. Kong ${}^{\textrm{\scriptsize 1}}$ , A.C. König ${}^{\textrm{\scriptsize 119}}$ , T. Kono ${}^{\textrm{\scriptsize 126}}$ , V. Konstantinides ${}^{\textrm{\scriptsize 95}}$ , N. Konstantinidis ${}^{\textrm{\scriptsize 95}}$ , B. Konya ${}^{\textrm{\scriptsize 97}}$ , R. Kopeliansky ${}^{\textrm{\scriptsize 66}}$ , S. Koperny ${}^{\textrm{\scriptsize 84a}}$ , K. Korcyl ${}^{\textrm{\scriptsize 85}}$ , K. Kordas ${}^{\textrm{\scriptsize 161}}$ , G. Koren ${}^{\textrm{\scriptsize 160}}$ , A. Korn ${}^{\textrm{\scriptsize 95}}$ , I. Korolkov ${}^{\textrm{\scriptsize 14}}$ , E.V. Korolkova ${}^{\textrm{\scriptsize 148}}$ , N. 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Kremer ${}^{\textrm{\scriptsize 100}}$ , J. Kretzschmar ${}^{\textrm{\scriptsize 91}}$ , P. Krieger ${}^{\textrm{\scriptsize 166}}$ , F. Krieter ${}^{\textrm{\scriptsize 114}}$ , A. Krishnan ${}^{\textrm{\scriptsize 61b}}$ , K. Krizka ${}^{\textrm{\scriptsize 18}}$ , K. Kroeninger ${}^{\textrm{\scriptsize 47}}$ , H. Kroha ${}^{\textrm{\scriptsize 115}}$ , J. Kroll ${}^{\textrm{\scriptsize 140}}$ , J. Kroll ${}^{\textrm{\scriptsize 136}}$ , K.S. Krowpman ${}^{\textrm{\scriptsize 107}}$ , U. Kruchonak ${}^{\textrm{\scriptsize 80}}$ , H. Krüger ${}^{\textrm{\scriptsize 24}}$ , N. Krumnack ${}^{\textrm{\scriptsize 79}}$ , M.C. Kruse ${}^{\textrm{\scriptsize 49}}$ , J.A. Krzysiak ${}^{\textrm{\scriptsize 85}}$ , O. Kuchinskaia ${}^{\textrm{\scriptsize 165}}$ , S. Kuday ${}^{\textrm{\scriptsize 4b}}$ , D. Kuechler ${}^{\textrm{\scriptsize 46}}$ , J.T. Kuechler ${}^{\textrm{\scriptsize 46}}$ , S. Kuehn ${}^{\textrm{\scriptsize 36}}$ , T. Kuhl ${}^{\textrm{\scriptsize 46}}$ , V. Kukhtin ${}^{\textrm{\scriptsize 80}}$ , Y. Kulchitsky ${}^{\textrm{\scriptsize 108,ae}}$ , S. Kuleshov ${}^{\textrm{\scriptsize 146b}}$ , Y.P. Kulinich ${}^{\textrm{\scriptsize 172}}$ , M. Kuna ${}^{\textrm{\scriptsize 58}}$ , T. Kunigo ${}^{\textrm{\scriptsize 86}}$ , A. Kupco ${}^{\textrm{\scriptsize 140}}$ , T. Kupfer ${}^{\textrm{\scriptsize 47}}$ , O. Kuprash ${}^{\textrm{\scriptsize 52}}$ , H. Kurashige ${}^{\textrm{\scriptsize 83}}$ , L.L. Kurchaninov ${}^{\textrm{\scriptsize 167a}}$ , Y.A. Kurochkin ${}^{\textrm{\scriptsize 108}}$ , A. Kurova ${}^{\textrm{\scriptsize 112}}$ , M.G. Kurth ${}^{\textrm{\scriptsize 15a,15d}}$ , E.S. Kuwertz ${}^{\textrm{\scriptsize 36}}$ , M. Kuze ${}^{\textrm{\scriptsize 164}}$ , A.K. Kvam ${}^{\textrm{\scriptsize 147}}$ , J. Kvita ${}^{\textrm{\scriptsize 130}}$ , T. Kwan ${}^{\textrm{\scriptsize 104}}$ , F. La Ruffa ${}^{\textrm{\scriptsize 41b,41a}}$ , C. Lacasta ${}^{\textrm{\scriptsize 173}}$ , F. 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Lanni ${}^{\textrm{\scriptsize 29}}$ , K. Lantzsch ${}^{\textrm{\scriptsize 24}}$ , A. Lanza ${}^{\textrm{\scriptsize 71a}}$ , A. Lapertosa ${}^{\textrm{\scriptsize 55b,55a}}$ , S. Laplace ${}^{\textrm{\scriptsize 135}}$ , J.F. Laporte ${}^{\textrm{\scriptsize 144}}$ , T. Lari ${}^{\textrm{\scriptsize 69a}}$ , F. Lasagni Manghi ${}^{\textrm{\scriptsize 23b,23a}}$ , M. Lassnig ${}^{\textrm{\scriptsize 36}}$ , T.S. Lau ${}^{\textrm{\scriptsize 63a}}$ , A. Laudrain ${}^{\textrm{\scriptsize 65}}$ , A. Laurier ${}^{\textrm{\scriptsize 34}}$ , M. Lavorgna ${}^{\textrm{\scriptsize 70a,70b}}$ , S.D. Lawlor ${}^{\textrm{\scriptsize 94}}$ , M. Lazzaroni ${}^{\textrm{\scriptsize 69a,69b}}$ , B. Le ${}^{\textrm{\scriptsize 101}}$ , E. Le Guirriec ${}^{\textrm{\scriptsize 102}}$ , A. Lebedev ${}^{\textrm{\scriptsize 79}}$ , M. LeBlanc ${}^{\textrm{\scriptsize 7}}$ , T. LeCompte ${}^{\textrm{\scriptsize 6}}$ , F. Ledroit-Guillon ${}^{\textrm{\scriptsize 58}}$ , A.C.A. 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Leonidopoulos ${}^{\textrm{\scriptsize 50}}$ , A. Leopold ${}^{\textrm{\scriptsize 135}}$ , C. Leroy ${}^{\textrm{\scriptsize 110}}$ , R. Les ${}^{\textrm{\scriptsize 107}}$ , C.G. Lester ${}^{\textrm{\scriptsize 32}}$ , M. Levchenko ${}^{\textrm{\scriptsize 137}}$ , J. Levêque ${}^{\textrm{\scriptsize 5}}$ , D. Levin ${}^{\textrm{\scriptsize 106}}$ , L.J. Levinson ${}^{\textrm{\scriptsize 179}}$ , D.J. Lewis ${}^{\textrm{\scriptsize 21}}$ , B. Li ${}^{\textrm{\scriptsize 15b}}$ , B. Li ${}^{\textrm{\scriptsize 106}}$ , C-Q. Li ${}^{\textrm{\scriptsize 60a}}$ , F. Li ${}^{\textrm{\scriptsize 60c}}$ , H. Li ${}^{\textrm{\scriptsize 60a}}$ , H. Li ${}^{\textrm{\scriptsize 60b}}$ , J. Li ${}^{\textrm{\scriptsize 60c}}$ , K. Li ${}^{\textrm{\scriptsize 147}}$ , L. Li ${}^{\textrm{\scriptsize 60c}}$ , M. Li ${}^{\textrm{\scriptsize 15a,15d}}$ , Q. Li ${}^{\textrm{\scriptsize 15a,15d}}$ , Q.Y. Li ${}^{\textrm{\scriptsize 60a}}$ , S. Li ${}^{\textrm{\scriptsize 60d,60c}}$ , X. Li ${}^{\textrm{\scriptsize 46}}$ , Y. Li ${}^{\textrm{\scriptsize 46}}$ , Z. Li ${}^{\textrm{\scriptsize 60b}}$ , Z. Li ${}^{\textrm{\scriptsize 134}}$ , Z. Li ${}^{\textrm{\scriptsize 104}}$ , Z. Liang ${}^{\textrm{\scriptsize 15a}}$ , M. Liberatore ${}^{\textrm{\scriptsize 46}}$ , B. Liberti ${}^{\textrm{\scriptsize 74a}}$ , A. Liblong ${}^{\textrm{\scriptsize 166}}$ , K. Lie ${}^{\textrm{\scriptsize 63c}}$ , S. Lim ${}^{\textrm{\scriptsize 29}}$ , C.Y. Lin ${}^{\textrm{\scriptsize 32}}$ , K. Lin ${}^{\textrm{\scriptsize 107}}$ , R.A. Linck ${}^{\textrm{\scriptsize 66}}$ , R.E. Lindley ${}^{\textrm{\scriptsize 7}}$ , J.H. Lindon ${}^{\textrm{\scriptsize 21}}$ , A. Linss ${}^{\textrm{\scriptsize 46}}$ , A.L. Lionti ${}^{\textrm{\scriptsize 54}}$ , E. Lipeles ${}^{\textrm{\scriptsize 136}}$ , A. Lipniacka ${}^{\textrm{\scriptsize 17}}$ , T.M. Liss ${}^{\textrm{\scriptsize 172,ak}}$ , A. Lister ${}^{\textrm{\scriptsize 174}}$ , J.D. Little ${}^{\textrm{\scriptsize 8}}$ , B. Liu ${}^{\textrm{\scriptsize 79}}$ , B.L. Liu ${}^{\textrm{\scriptsize 6}}$ , H.B. Liu ${}^{\textrm{\scriptsize 29}}$ , J.B. Liu ${}^{\textrm{\scriptsize 60a}}$ , J.K.K. Liu ${}^{\textrm{\scriptsize 37}}$ , K. Liu ${}^{\textrm{\scriptsize 60d}}$ , M. Liu ${}^{\textrm{\scriptsize 60a}}$ , P. Liu ${}^{\textrm{\scriptsize 15a}}$ , Y. Liu ${}^{\textrm{\scriptsize 46}}$ , Y. Liu ${}^{\textrm{\scriptsize 15a,15d}}$ , Y.L. Liu ${}^{\textrm{\scriptsize 106}}$ , Y.W. Liu ${}^{\textrm{\scriptsize 60a}}$ , M. Livan ${}^{\textrm{\scriptsize 71a,71b}}$ , A. Lleres ${}^{\textrm{\scriptsize 58}}$ , J. Llorente Merino ${}^{\textrm{\scriptsize 151}}$ , S.L. Lloyd ${}^{\textrm{\scriptsize 93}}$ , C.Y. Lo ${}^{\textrm{\scriptsize 63b}}$ , E.M. Lobodzinska ${}^{\textrm{\scriptsize 46}}$ , P. Loch ${}^{\textrm{\scriptsize 7}}$ , S. Loffredo ${}^{\textrm{\scriptsize 74a,74b}}$ , T. Lohse ${}^{\textrm{\scriptsize 19}}$ , K. Lohwasser ${}^{\textrm{\scriptsize 148}}$ , M. Lokajicek ${}^{\textrm{\scriptsize 140}}$ , J.D. Long ${}^{\textrm{\scriptsize 172}}$ , R.E. Long ${}^{\textrm{\scriptsize 90}}$ , I. Longarini ${}^{\textrm{\scriptsize 73a,73b}}$ , L. Longo ${}^{\textrm{\scriptsize 36}}$ , K.A. Looper ${}^{\textrm{\scriptsize 127}}$ , I. Lopez Paz ${}^{\textrm{\scriptsize 101}}$ , A. Lopez Solis ${}^{\textrm{\scriptsize 148}}$ , J. Lorenz ${}^{\textrm{\scriptsize 114}}$ , N. Lorenzo Martinez ${}^{\textrm{\scriptsize 5}}$ , A.M. Lory ${}^{\textrm{\scriptsize 114}}$ , P.J. Lösel ${}^{\textrm{\scriptsize 114}}$ , A. Lösle ${}^{\textrm{\scriptsize 52}}$ , X. Lou ${}^{\textrm{\scriptsize 46}}$ , X. Lou ${}^{\textrm{\scriptsize 15a}}$ , A. Lounis ${}^{\textrm{\scriptsize 65}}$ , J. Love ${}^{\textrm{\scriptsize 6}}$ , P.A. Love ${}^{\textrm{\scriptsize 90}}$ , J.J. Lozano Bahilo ${}^{\textrm{\scriptsize 173}}$ , M. Lu ${}^{\textrm{\scriptsize 60a}}$ , Y.J. Lu ${}^{\textrm{\scriptsize 64}}$ , H.J. Lubatti ${}^{\textrm{\scriptsize 147}}$ , C. Luci ${}^{\textrm{\scriptsize 73a,73b}}$ , F.L. Lucio Alves ${}^{\textrm{\scriptsize 15c}}$ , A. Lucotte ${}^{\textrm{\scriptsize 58}}$ , F. Luehring ${}^{\textrm{\scriptsize 66}}$ , I. Luise ${}^{\textrm{\scriptsize 135}}$ , L. Luminari ${}^{\textrm{\scriptsize 73a}}$ , B. Lund-Jensen ${}^{\textrm{\scriptsize 153}}$ , M.S. Lutz ${}^{\textrm{\scriptsize 160}}$ , D. Lynn ${}^{\textrm{\scriptsize 29}}$ , H. Lyons ${}^{\textrm{\scriptsize 91}}$ , R. Lysak ${}^{\textrm{\scriptsize 140}}$ , E. Lytken ${}^{\textrm{\scriptsize 97}}$ , F. Lyu ${}^{\textrm{\scriptsize 15a}}$ , V. Lyubushkin ${}^{\textrm{\scriptsize 80}}$ , T. Lyubushkina ${}^{\textrm{\scriptsize 80}}$ , H. Ma ${}^{\textrm{\scriptsize 29}}$ , L.L. Ma ${}^{\textrm{\scriptsize 60b}}$ , Y. Ma ${}^{\textrm{\scriptsize 95}}$ , D.M. Mac Donell ${}^{\textrm{\scriptsize 175}}$ , G. Maccarrone ${}^{\textrm{\scriptsize 51}}$ , A. Macchiolo ${}^{\textrm{\scriptsize 115}}$ , C.M. Macdonald ${}^{\textrm{\scriptsize 148}}$ , J.C. MacDonald ${}^{\textrm{\scriptsize 148}}$ , J. Machado Miguens ${}^{\textrm{\scriptsize 136}}$ , D. Madaffari ${}^{\textrm{\scriptsize 173}}$ , R. Madar ${}^{\textrm{\scriptsize 38}}$ , W.F. Mader ${}^{\textrm{\scriptsize 48}}$ , M. Madugoda Ralalage Don ${}^{\textrm{\scriptsize 129}}$ , N. Madysa ${}^{\textrm{\scriptsize 48}}$ , J. Maeda ${}^{\textrm{\scriptsize 83}}$ , T. Maeno ${}^{\textrm{\scriptsize 29}}$ , M. Maerker ${}^{\textrm{\scriptsize 48}}$ , V. Magerl ${}^{\textrm{\scriptsize 52}}$ , N. Magini ${}^{\textrm{\scriptsize 79}}$ , J. Magro ${}^{\textrm{\scriptsize 67a,67c,q}}$ , D.J. Mahon ${}^{\textrm{\scriptsize 39}}$ , C. Maidantchik ${}^{\textrm{\scriptsize 81b}}$ , T. Maier ${}^{\textrm{\scriptsize 114}}$ , A. Maio ${}^{\textrm{\scriptsize 139a,139b,139d}}$ , K. Maj ${}^{\textrm{\scriptsize 84a}}$ , O. Majersky ${}^{\textrm{\scriptsize 28a}}$ , S. Majewski ${}^{\textrm{\scriptsize 131}}$ , Y. Makida ${}^{\textrm{\scriptsize 82}}$ , N. Makovec ${}^{\textrm{\scriptsize 65}}$ , B. Malaescu ${}^{\textrm{\scriptsize 135}}$ , Pa. Malecki ${}^{\textrm{\scriptsize 85}}$ , V.P. Maleev ${}^{\textrm{\scriptsize 137}}$ , F. Malek ${}^{\textrm{\scriptsize 58}}$ , D. Malito ${}^{\textrm{\scriptsize 41b,41a}}$ , U. Mallik ${}^{\textrm{\scriptsize 78}}$ , D. Malon ${}^{\textrm{\scriptsize 6}}$ , C. Malone ${}^{\textrm{\scriptsize 32}}$ , S. Maltezos ${}^{\textrm{\scriptsize 10}}$ , S. Malyukov ${}^{\textrm{\scriptsize 80}}$ , J. Mamuzic ${}^{\textrm{\scriptsize 173}}$ , G. Mancini ${}^{\textrm{\scriptsize 70a,70b}}$ , I. Mandić ${}^{\textrm{\scriptsize 92}}$ , L. Manhaes de Andrade Filho ${}^{\textrm{\scriptsize 81a}}$ , I.M. Maniatis ${}^{\textrm{\scriptsize 161}}$ , J. Manjarres Ramos ${}^{\textrm{\scriptsize 48}}$ , K.H. Mankinen ${}^{\textrm{\scriptsize 97}}$ , A. Mann ${}^{\textrm{\scriptsize 114}}$ , A. Manousos ${}^{\textrm{\scriptsize 77}}$ , B. Mansoulie ${}^{\textrm{\scriptsize 144}}$ , I. Manthos ${}^{\textrm{\scriptsize 161}}$ , S. Manzoni ${}^{\textrm{\scriptsize 120}}$ , A. Marantis ${}^{\textrm{\scriptsize 161}}$ , G. Marceca ${}^{\textrm{\scriptsize 30}}$ , L. Marchese ${}^{\textrm{\scriptsize 134}}$ , G. Marchiori ${}^{\textrm{\scriptsize 135}}$ , M. Marcisovsky ${}^{\textrm{\scriptsize 140}}$ , L. Marcoccia ${}^{\textrm{\scriptsize 74a,74b}}$ , C. Marcon ${}^{\textrm{\scriptsize 97}}$ , C.A. Marin Tobon ${}^{\textrm{\scriptsize 36}}$ , M. Marjanovic ${}^{\textrm{\scriptsize 128}}$ , Z. Marshall ${}^{\textrm{\scriptsize 18}}$ , M.U.F. Martensson ${}^{\textrm{\scriptsize 171}}$ , S. Marti-Garcia ${}^{\textrm{\scriptsize 173}}$ , C.B. Martin ${}^{\textrm{\scriptsize 127}}$ , T.A. Martin ${}^{\textrm{\scriptsize 177}}$ , V.J. Martin ${}^{\textrm{\scriptsize 50}}$ , B. Martin dit Latour ${}^{\textrm{\scriptsize 17}}$ , L. Martinelli ${}^{\textrm{\scriptsize 75a,75b}}$ , M. Martinez ${}^{\textrm{\scriptsize 14,w}}$ , P. Martinez Agullo ${}^{\textrm{\scriptsize 173}}$ , V.I. Martinez Outschoorn ${}^{\textrm{\scriptsize 103}}$ , S. Martin-Haugh ${}^{\textrm{\scriptsize 143}}$ , V.S. Martoiu ${}^{\textrm{\scriptsize 27b}}$ , A.C. Martyniuk ${}^{\textrm{\scriptsize 95}}$ , A. Marzin ${}^{\textrm{\scriptsize 36}}$ , S.R. Maschek ${}^{\textrm{\scriptsize 115}}$ , L. Masetti ${}^{\textrm{\scriptsize 100}}$ , T. Mashimo ${}^{\textrm{\scriptsize 162}}$ , R. Mashinistov ${}^{\textrm{\scriptsize 111}}$ , J. Masik ${}^{\textrm{\scriptsize 101}}$ , A.L. Maslennikov ${}^{\textrm{\scriptsize 122b,122a}}$ , L. Massa ${}^{\textrm{\scriptsize 23b,23a}}$ , P. Massarotti ${}^{\textrm{\scriptsize 70a,70b}}$ , P. Mastrandrea ${}^{\textrm{\scriptsize 72a,72b}}$ , A. Mastroberardino ${}^{\textrm{\scriptsize 41b,41a}}$ , T. Masubuchi ${}^{\textrm{\scriptsize 162}}$ , D. Matakias ${}^{\textrm{\scriptsize 29}}$ , A. Matic ${}^{\textrm{\scriptsize 114}}$ , N. Matsuzawa ${}^{\textrm{\scriptsize 162}}$ , P. Mättig ${}^{\textrm{\scriptsize 24}}$ , J. Maurer ${}^{\textrm{\scriptsize 27b}}$ , B. Maček ${}^{\textrm{\scriptsize 92}}$ , D.A. Maximov ${}^{\textrm{\scriptsize 122b,122a}}$ , R. Mazini ${}^{\textrm{\scriptsize 157}}$ , I. Maznas ${}^{\textrm{\scriptsize 161}}$ , S.M. Mazza ${}^{\textrm{\scriptsize 145}}$ , J.P. Mc Gowan ${}^{\textrm{\scriptsize 104}}$ , S.P. Mc Kee ${}^{\textrm{\scriptsize 106}}$ , T.G. McCarthy ${}^{\textrm{\scriptsize 115}}$ , W.P. McCormack ${}^{\textrm{\scriptsize 18}}$ , E.F. McDonald ${}^{\textrm{\scriptsize 105}}$ , J.A. Mcfayden ${}^{\textrm{\scriptsize 36}}$ , G. Mchedlidze ${}^{\textrm{\scriptsize 158b}}$ , M.A. McKay ${}^{\textrm{\scriptsize 42}}$ , K.D. McLean ${}^{\textrm{\scriptsize 175}}$ , S.J. McMahon ${}^{\textrm{\scriptsize 143}}$ , P.C. McNamara ${}^{\textrm{\scriptsize 105}}$ , C.J. McNicol ${}^{\textrm{\scriptsize 177}}$ , R.A. McPherson ${}^{\textrm{\scriptsize 175,ab}}$ , J.E. Mdhluli ${}^{\textrm{\scriptsize 33e}}$ , Z.A. Meadows ${}^{\textrm{\scriptsize 103}}$ , S. Meehan ${}^{\textrm{\scriptsize 36}}$ , T. Megy ${}^{\textrm{\scriptsize 38}}$ , S. Mehlhase ${}^{\textrm{\scriptsize 114}}$ , A. Mehta ${}^{\textrm{\scriptsize 91}}$ , B. Meirose ${}^{\textrm{\scriptsize 43}}$ , D. Melini ${}^{\textrm{\scriptsize 159}}$ , B.R. Mellado Garcia ${}^{\textrm{\scriptsize 33e}}$ , J.D. Mellenthin ${}^{\textrm{\scriptsize 53}}$ , M. Melo ${}^{\textrm{\scriptsize 28a}}$ , F. Meloni ${}^{\textrm{\scriptsize 46}}$ , A. Melzer ${}^{\textrm{\scriptsize 24}}$ , E.D. Mendes Gouveia ${}^{\textrm{\scriptsize 139a,139e}}$ , L. Meng ${}^{\textrm{\scriptsize 36}}$ , X.T. Meng ${}^{\textrm{\scriptsize 106}}$ , S. Menke ${}^{\textrm{\scriptsize 115}}$ , E. Meoni ${}^{\textrm{\scriptsize 41b,41a}}$ , S. Mergelmeyer ${}^{\textrm{\scriptsize 19}}$ , S.A.M. Merkt ${}^{\textrm{\scriptsize 138}}$ , C. Merlassino ${}^{\textrm{\scriptsize 134}}$ , P. Mermod ${}^{\textrm{\scriptsize 54}}$ , L. Merola ${}^{\textrm{\scriptsize 70a,70b}}$ , C. Meroni ${}^{\textrm{\scriptsize 69a}}$ , G. Merz ${}^{\textrm{\scriptsize 106}}$ , O. Meshkov ${}^{\textrm{\scriptsize 113,111}}$ , J.K.R. Meshreki ${}^{\textrm{\scriptsize 150}}$ , J. Metcalfe ${}^{\textrm{\scriptsize 6}}$ , A.S. Mete ${}^{\textrm{\scriptsize 6}}$ , C. Meyer ${}^{\textrm{\scriptsize 66}}$ , J-P. Meyer ${}^{\textrm{\scriptsize 144}}$ , M. Michetti ${}^{\textrm{\scriptsize 19}}$ , R.P. Middleton ${}^{\textrm{\scriptsize 143}}$ , L. Mijović ${}^{\textrm{\scriptsize 50}}$ , G. Mikenberg ${}^{\textrm{\scriptsize 179}}$ , M. Mikestikova ${}^{\textrm{\scriptsize 140}}$ , M. Mikuž ${}^{\textrm{\scriptsize 92}}$ , H. Mildner ${}^{\textrm{\scriptsize 148}}$ , A. Milic ${}^{\textrm{\scriptsize 166}}$ , C.D. Milke ${}^{\textrm{\scriptsize 42}}$ , D.W. Miller ${}^{\textrm{\scriptsize 37}}$ , A. Milov ${}^{\textrm{\scriptsize 179}}$ , D.A. Milstead ${}^{\textrm{\scriptsize 45a,45b}}$ , R.A. Mina ${}^{\textrm{\scriptsize 152}}$ , A.A. Minaenko ${}^{\textrm{\scriptsize 123}}$ , I.A. Minashvili ${}^{\textrm{\scriptsize 158b}}$ , A.I. Mincer ${}^{\textrm{\scriptsize 125}}$ , B. Mindur ${}^{\textrm{\scriptsize 84a}}$ , M. Mineev ${}^{\textrm{\scriptsize 80}}$ , Y. Minegishi ${}^{\textrm{\scriptsize 162}}$ , L.M. Mir ${}^{\textrm{\scriptsize 14}}$ , M. Mironova ${}^{\textrm{\scriptsize 134}}$ , A. Mirto ${}^{\textrm{\scriptsize 68a,68b}}$ , K.P. Mistry ${}^{\textrm{\scriptsize 136}}$ , T. Mitani ${}^{\textrm{\scriptsize 178}}$ , J. Mitrevski ${}^{\textrm{\scriptsize 114}}$ , V.A. Mitsou ${}^{\textrm{\scriptsize 173}}$ , M. Mittal ${}^{\textrm{\scriptsize 60c}}$ , O. Miu ${}^{\textrm{\scriptsize 166}}$ , A. Miucci ${}^{\textrm{\scriptsize 20}}$ , P.S. Miyagawa ${}^{\textrm{\scriptsize 93}}$ , A. Mizukami ${}^{\textrm{\scriptsize 82}}$ , J.U. Mjörnmark ${}^{\textrm{\scriptsize 97}}$ , T. Mkrtchyan ${}^{\textrm{\scriptsize 61a}}$ , M. Mlynarikova ${}^{\textrm{\scriptsize 142}}$ , T. Moa ${}^{\textrm{\scriptsize 45a,45b}}$ , S. Mobius ${}^{\textrm{\scriptsize 53}}$ , K. Mochizuki ${}^{\textrm{\scriptsize 110}}$ , P. Mogg ${}^{\textrm{\scriptsize 114}}$ , S. Mohapatra ${}^{\textrm{\scriptsize 39}}$ , R. Moles-Valls ${}^{\textrm{\scriptsize 24}}$ , K. Mönig ${}^{\textrm{\scriptsize 46}}$ , E. Monnier ${}^{\textrm{\scriptsize 102}}$ , A. Montalbano ${}^{\textrm{\scriptsize 151}}$ , J. Montejo Berlingen ${}^{\textrm{\scriptsize 36}}$ , M. Montella ${}^{\textrm{\scriptsize 95}}$ , F. Monticelli ${}^{\textrm{\scriptsize 89}}$ , S. Monzani ${}^{\textrm{\scriptsize 69a}}$ , N. Morange ${}^{\textrm{\scriptsize 65}}$ , D. Moreno ${}^{\textrm{\scriptsize 22a}}$ , M. Moreno Llácer ${}^{\textrm{\scriptsize 173}}$ , C. Moreno Martinez ${}^{\textrm{\scriptsize 14}}$ , P. Morettini ${}^{\textrm{\scriptsize 55b}}$ , M. Morgenstern ${}^{\textrm{\scriptsize 159}}$ , S. Morgenstern ${}^{\textrm{\scriptsize 48}}$ , D. Mori ${}^{\textrm{\scriptsize 151}}$ , M. Morii ${}^{\textrm{\scriptsize 59}}$ , M. Morinaga ${}^{\textrm{\scriptsize 178}}$ , V. Morisbak ${}^{\textrm{\scriptsize 133}}$ , A.K. Morley ${}^{\textrm{\scriptsize 36}}$ , G. Mornacchi ${}^{\textrm{\scriptsize 36}}$ , A.P. Morris ${}^{\textrm{\scriptsize 95}}$ , L. Morvaj ${}^{\textrm{\scriptsize 154}}$ , P. Moschovakos ${}^{\textrm{\scriptsize 36}}$ , B. Moser ${}^{\textrm{\scriptsize 120}}$ , M. Mosidze ${}^{\textrm{\scriptsize 158b}}$ , T. Moskalets ${}^{\textrm{\scriptsize 144}}$ , H.J. Moss ${}^{\textrm{\scriptsize 148}}$ , J. Moss ${}^{\textrm{\scriptsize 31,m}}$ , E.J.W. Moyse ${}^{\textrm{\scriptsize 103}}$ , S. Muanza ${}^{\textrm{\scriptsize 102}}$ , J. Mueller ${}^{\textrm{\scriptsize 138}}$ , R.S.P. Mueller ${}^{\textrm{\scriptsize 114}}$ , D. Muenstermann ${}^{\textrm{\scriptsize 90}}$ , G.A. Mullier ${}^{\textrm{\scriptsize 97}}$ , D.P. Mungo ${}^{\textrm{\scriptsize 69a,69b}}$ , J.L. Munoz Martinez ${}^{\textrm{\scriptsize 14}}$ , F.J. Munoz Sanchez ${}^{\textrm{\scriptsize 101}}$ , P. Murin ${}^{\textrm{\scriptsize 28b}}$ , W.J. Murray ${}^{\textrm{\scriptsize 177,143}}$ , A. Murrone ${}^{\textrm{\scriptsize 69a,69b}}$ , J.M. Muse ${}^{\textrm{\scriptsize 128}}$ , M. Muškinja ${}^{\textrm{\scriptsize 18}}$ , C. Mwewa ${}^{\textrm{\scriptsize 33a}}$ , A.G. Myagkov ${}^{\textrm{\scriptsize 123,ag}}$ , A.A. Myers ${}^{\textrm{\scriptsize 138}}$ , J. Myers ${}^{\textrm{\scriptsize 131}}$ , M. Myska ${}^{\textrm{\scriptsize 141}}$ , B.P. Nachman ${}^{\textrm{\scriptsize 18}}$ , O. Nackenhorst ${}^{\textrm{\scriptsize 47}}$ , A.Nag Nag ${}^{\textrm{\scriptsize 48}}$ , K. Nagai ${}^{\textrm{\scriptsize 134}}$ , K. Nagano ${}^{\textrm{\scriptsize 82}}$ , Y. Nagasaka ${}^{\textrm{\scriptsize 62}}$ , J.L. Nagle ${}^{\textrm{\scriptsize 29}}$ , E. Nagy ${}^{\textrm{\scriptsize 102}}$ , A.M. Nairz ${}^{\textrm{\scriptsize 36}}$ , Y. Nakahama ${}^{\textrm{\scriptsize 117}}$ , K. Nakamura ${}^{\textrm{\scriptsize 82}}$ , T. Nakamura ${}^{\textrm{\scriptsize 162}}$ , H. Nanjo ${}^{\textrm{\scriptsize 132}}$ , F. Napolitano ${}^{\textrm{\scriptsize 61a}}$ , R.F. Naranjo Garcia ${}^{\textrm{\scriptsize 46}}$ , R. Narayan ${}^{\textrm{\scriptsize 42}}$ , I. Naryshkin ${}^{\textrm{\scriptsize 137}}$ , T. Naumann ${}^{\textrm{\scriptsize 46}}$ , G. Navarro ${}^{\textrm{\scriptsize 22a}}$ , P.Y. Nechaeva ${}^{\textrm{\scriptsize 111}}$ , F. Nechansky ${}^{\textrm{\scriptsize 46}}$ , T.J. Neep ${}^{\textrm{\scriptsize 21}}$ , A. Negri ${}^{\textrm{\scriptsize 71a,71b}}$ , M. Negrini ${}^{\textrm{\scriptsize 23b}}$ , C. Nellist ${}^{\textrm{\scriptsize 119}}$ , C. Nelson ${}^{\textrm{\scriptsize 104}}$ , M.E. Nelson ${}^{\textrm{\scriptsize 45a,45b}}$ , S. Nemecek ${}^{\textrm{\scriptsize 140}}$ , M. Nessi ${}^{\textrm{\scriptsize 36,e}}$ , M.S. Neubauer ${}^{\textrm{\scriptsize 172}}$ , F. Neuhaus ${}^{\textrm{\scriptsize 100}}$ , M. Neumann ${}^{\textrm{\scriptsize 181}}$ , R. Newhouse ${}^{\textrm{\scriptsize 174}}$ , P.R. Newman ${}^{\textrm{\scriptsize 21}}$ , C.W. Ng ${}^{\textrm{\scriptsize 138}}$ , Y.S. Ng ${}^{\textrm{\scriptsize 19}}$ , Y.W.Y. Ng ${}^{\textrm{\scriptsize 170}}$ , B. Ngair ${}^{\textrm{\scriptsize 35e}}$ , H.D.N. Nguyen ${}^{\textrm{\scriptsize 102}}$ , T. Nguyen Manh ${}^{\textrm{\scriptsize 110}}$ , E. Nibigira ${}^{\textrm{\scriptsize 38}}$ , R.B. Nickerson ${}^{\textrm{\scriptsize 134}}$ , R. Nicolaidou ${}^{\textrm{\scriptsize 144}}$ , D.S. Nielsen ${}^{\textrm{\scriptsize 40}}$ , J. Nielsen ${}^{\textrm{\scriptsize 145}}$ , M. Niemeyer ${}^{\textrm{\scriptsize 53}}$ , N. Nikiforou ${}^{\textrm{\scriptsize 11}}$ , V. Nikolaenko ${}^{\textrm{\scriptsize 123,ag}}$ , I. Nikolic-Audit ${}^{\textrm{\scriptsize 135}}$ , K. Nikolopoulos ${}^{\textrm{\scriptsize 21}}$ , P. Nilsson ${}^{\textrm{\scriptsize 29}}$ , H.R. Nindhito ${}^{\textrm{\scriptsize 54}}$ , Y. Ninomiya ${}^{\textrm{\scriptsize 82}}$ , A. Nisati ${}^{\textrm{\scriptsize 73a}}$ , N. Nishu ${}^{\textrm{\scriptsize 60c}}$ , R. Nisius ${}^{\textrm{\scriptsize 115}}$ , I. Nitsche ${}^{\textrm{\scriptsize 47}}$ , T. Nitta ${}^{\textrm{\scriptsize 178}}$ , T. Nobe ${}^{\textrm{\scriptsize 162}}$ , D.L. Noel ${}^{\textrm{\scriptsize 32}}$ , Y. Noguchi ${}^{\textrm{\scriptsize 86}}$ , I. Nomidis ${}^{\textrm{\scriptsize 135}}$ , M.A. Nomura ${}^{\textrm{\scriptsize 29}}$ , M. Nordberg ${}^{\textrm{\scriptsize 36}}$ , J. Novak ${}^{\textrm{\scriptsize 92}}$ , T. Novak ${}^{\textrm{\scriptsize 92}}$ , O. Novgorodova ${}^{\textrm{\scriptsize 48}}$ , R. Novotny ${}^{\textrm{\scriptsize 141}}$ , L. Nozka ${}^{\textrm{\scriptsize 130}}$ , K. Ntekas ${}^{\textrm{\scriptsize 170}}$ , E. Nurse ${}^{\textrm{\scriptsize 95}}$ , F.G. Oakham ${}^{\textrm{\scriptsize 34,al}}$ , H. Oberlack ${}^{\textrm{\scriptsize 115}}$ , J. Ocariz ${}^{\textrm{\scriptsize 135}}$ , A. Ochi ${}^{\textrm{\scriptsize 83}}$ , I. Ochoa ${}^{\textrm{\scriptsize 39}}$ , J.P. Ochoa-Ricoux ${}^{\textrm{\scriptsize 146a}}$ , K. O’Connor ${}^{\textrm{\scriptsize 26}}$ , S. Oda ${}^{\textrm{\scriptsize 88}}$ , S. Odaka ${}^{\textrm{\scriptsize 82}}$ , S. Oerdek ${}^{\textrm{\scriptsize 53}}$ , A. Ogrodnik ${}^{\textrm{\scriptsize 84a}}$ , A. Oh ${}^{\textrm{\scriptsize 101}}$ , S.H. Oh ${}^{\textrm{\scriptsize 49}}$ , C.C. Ohm ${}^{\textrm{\scriptsize 153}}$ , H. Oide ${}^{\textrm{\scriptsize 164}}$ , M.L. Ojeda ${}^{\textrm{\scriptsize 166}}$ , H. Okawa ${}^{\textrm{\scriptsize 168}}$ , Y. Okazaki ${}^{\textrm{\scriptsize 86}}$ , M.W. O’Keefe ${}^{\textrm{\scriptsize 91}}$ , Y. Okumura ${}^{\textrm{\scriptsize 162}}$ , T. Okuyama ${}^{\textrm{\scriptsize 82}}$ , A. Olariu ${}^{\textrm{\scriptsize 27b}}$ , L.F. Oleiro Seabra ${}^{\textrm{\scriptsize 139a}}$ , S.A. Olivares Pino ${}^{\textrm{\scriptsize 146a}}$ , D. Oliveira Damazio ${}^{\textrm{\scriptsize 29}}$ , J.L. Oliver ${}^{\textrm{\scriptsize 1}}$ , M.J.R. Olsson ${}^{\textrm{\scriptsize 170}}$ , A. Olszewski ${}^{\textrm{\scriptsize 85}}$ , J. Olszowska ${}^{\textrm{\scriptsize 85}}$ , Ö.O. Öncel ${}^{\textrm{\scriptsize 24}}$ , D.C. O’Neil ${}^{\textrm{\scriptsize 151}}$ , A.P. O’neill ${}^{\textrm{\scriptsize 134}}$ , A. Onofre ${}^{\textrm{\scriptsize 139a,139e}}$ , P.U.E. Onyisi ${}^{\textrm{\scriptsize 11}}$ , H. Oppen ${}^{\textrm{\scriptsize 133}}$ , R.G. Oreamuno Madriz ${}^{\textrm{\scriptsize 121}}$ , M.J. Oreglia ${}^{\textrm{\scriptsize 37}}$ , G.E. Orellana ${}^{\textrm{\scriptsize 89}}$ , D. Orestano ${}^{\textrm{\scriptsize 75a,75b}}$ , N. Orlando ${}^{\textrm{\scriptsize 14}}$ , R.S. Orr ${}^{\textrm{\scriptsize 166}}$ , V. O’Shea ${}^{\textrm{\scriptsize 57}}$ , R. Ospanov ${}^{\textrm{\scriptsize 60a}}$ , G. Otero y Garzon ${}^{\textrm{\scriptsize 30}}$ , H. Otono ${}^{\textrm{\scriptsize 88}}$ , P.S. Ott ${}^{\textrm{\scriptsize 61a}}$ , G.J. Ottino ${}^{\textrm{\scriptsize 18}}$ , M. Ouchrif ${}^{\textrm{\scriptsize 35d}}$ , J. Ouellette ${}^{\textrm{\scriptsize 29}}$ , F. Ould-Saada ${}^{\textrm{\scriptsize 133}}$ , A. Ouraou ${}^{\textrm{\scriptsize 144}}$ , Q. Ouyang ${}^{\textrm{\scriptsize 15a}}$ , M. Owen ${}^{\textrm{\scriptsize 57}}$ , R.E. Owen ${}^{\textrm{\scriptsize 143}}$ , V.E. Ozcan ${}^{\textrm{\scriptsize 12c}}$ , N. Ozturk ${}^{\textrm{\scriptsize 8}}$ , J. Pacalt ${}^{\textrm{\scriptsize 130}}$ , H.A. Pacey ${}^{\textrm{\scriptsize 32}}$ , K. Pachal ${}^{\textrm{\scriptsize 49}}$ , A. Pacheco Pages ${}^{\textrm{\scriptsize 14}}$ , C. Padilla Aranda ${}^{\textrm{\scriptsize 14}}$ , S. Pagan Griso ${}^{\textrm{\scriptsize 18}}$ , G. Palacino ${}^{\textrm{\scriptsize 66}}$ , S. Palazzo ${}^{\textrm{\scriptsize 50}}$ , S. Palestini ${}^{\textrm{\scriptsize 36}}$ , M. Palka ${}^{\textrm{\scriptsize 84b}}$ , P. Palni ${}^{\textrm{\scriptsize 84a}}$ , C.E. Pandini ${}^{\textrm{\scriptsize 54}}$ , J.G. Panduro Vazquez ${}^{\textrm{\scriptsize 94}}$ , P. Pani ${}^{\textrm{\scriptsize 46}}$ , G. Panizzo ${}^{\textrm{\scriptsize 67a,67c}}$ , L. Paolozzi ${}^{\textrm{\scriptsize 54}}$ , C. Papadatos ${}^{\textrm{\scriptsize 110}}$ , K. Papageorgiou ${}^{\textrm{\scriptsize 9,g}}$ , S. Parajuli ${}^{\textrm{\scriptsize 42}}$ , A. Paramonov ${}^{\textrm{\scriptsize 6}}$ , C. Paraskevopoulos ${}^{\textrm{\scriptsize 10}}$ , D. Paredes Hernandez ${}^{\textrm{\scriptsize 63b}}$ , S.R. Paredes Saenz ${}^{\textrm{\scriptsize 134}}$ , B. Parida ${}^{\textrm{\scriptsize 179}}$ , T.H. Park ${}^{\textrm{\scriptsize 166}}$ , A.J. Parker ${}^{\textrm{\scriptsize 31}}$ , M.A. Parker ${}^{\textrm{\scriptsize 32}}$ , F. Parodi ${}^{\textrm{\scriptsize 55b,55a}}$ , E.W. Parrish ${}^{\textrm{\scriptsize 121}}$ , J.A. Parsons ${}^{\textrm{\scriptsize 39}}$ , U. Parzefall ${}^{\textrm{\scriptsize 52}}$ , L. Pascual Dominguez ${}^{\textrm{\scriptsize 135}}$ , V.R. Pascuzzi ${}^{\textrm{\scriptsize 18}}$ , J.M.P. Pasner ${}^{\textrm{\scriptsize 145}}$ , F. Pasquali ${}^{\textrm{\scriptsize 120}}$ , E. Pasqualucci ${}^{\textrm{\scriptsize 73a}}$ , S. Passaggio ${}^{\textrm{\scriptsize 55b}}$ , F. Pastore ${}^{\textrm{\scriptsize 94}}$ , P. Pasuwan ${}^{\textrm{\scriptsize 45a,45b}}$ , S. Pataraia ${}^{\textrm{\scriptsize 100}}$ , J.R. Pater ${}^{\textrm{\scriptsize 101}}$ , A. Pathak ${}^{\textrm{\scriptsize 180,i}}$ , J. Patton ${}^{\textrm{\scriptsize 91}}$ , T. Pauly ${}^{\textrm{\scriptsize 36}}$ , J. Pearkes ${}^{\textrm{\scriptsize 152}}$ , B. Pearson ${}^{\textrm{\scriptsize 115}}$ , M. Pedersen ${}^{\textrm{\scriptsize 133}}$ , L. Pedraza Diaz ${}^{\textrm{\scriptsize 119}}$ , R. Pedro ${}^{\textrm{\scriptsize 139a}}$ , T. Peiffer ${}^{\textrm{\scriptsize 53}}$ , S.V. Peleganchuk ${}^{\textrm{\scriptsize 122b,122a}}$ , O. Penc ${}^{\textrm{\scriptsize 140}}$ , H. Peng ${}^{\textrm{\scriptsize 60a}}$ , B.S. Peralva ${}^{\textrm{\scriptsize 81a}}$ , M.M. Perego ${}^{\textrm{\scriptsize 65}}$ , A.P. Pereira Peixoto ${}^{\textrm{\scriptsize 139a}}$ , L. Pereira Sanchez ${}^{\textrm{\scriptsize 45a,45b}}$ , D.V. Perepelitsa ${}^{\textrm{\scriptsize 29}}$ , E. Perez Codina ${}^{\textrm{\scriptsize 167a}}$ , F. Peri ${}^{\textrm{\scriptsize 19}}$ , L. Perini ${}^{\textrm{\scriptsize 69a,69b}}$ , H. Pernegger ${}^{\textrm{\scriptsize 36}}$ , S. Perrella ${}^{\textrm{\scriptsize 36}}$ , A. Perrevoort ${}^{\textrm{\scriptsize 120}}$ , K. Peters ${}^{\textrm{\scriptsize 46}}$ , R.F.Y. Peters ${}^{\textrm{\scriptsize 101}}$ , B.A. Petersen ${}^{\textrm{\scriptsize 36}}$ , T.C. Petersen ${}^{\textrm{\scriptsize 40}}$ , E. Petit ${}^{\textrm{\scriptsize 102}}$ , V. Petousis ${}^{\textrm{\scriptsize 141}}$ , A. Petridis ${}^{\textrm{\scriptsize 1}}$ , C. Petridou ${}^{\textrm{\scriptsize 161}}$ , F. Petrucci ${}^{\textrm{\scriptsize 75a,75b}}$ , M. Pettee ${}^{\textrm{\scriptsize 182}}$ , N.E. Pettersson ${}^{\textrm{\scriptsize 103}}$ , K. Petukhova ${}^{\textrm{\scriptsize 142}}$ , A. Peyaud ${}^{\textrm{\scriptsize 144}}$ , R. Pezoa ${}^{\textrm{\scriptsize 146d}}$ , L. Pezzotti ${}^{\textrm{\scriptsize 71a,71b}}$ , T. Pham ${}^{\textrm{\scriptsize 105}}$ , F.H. Phillips ${}^{\textrm{\scriptsize 107}}$ , P.W. Phillips ${}^{\textrm{\scriptsize 143}}$ , M.W. Phipps ${}^{\textrm{\scriptsize 172}}$ , G. Piacquadio ${}^{\textrm{\scriptsize 154}}$ , E. Pianori ${}^{\textrm{\scriptsize 18}}$ , A. Picazio ${}^{\textrm{\scriptsize 103}}$ , R.H. Pickles ${}^{\textrm{\scriptsize 101}}$ , R. Piegaia ${}^{\textrm{\scriptsize 30}}$ , D. Pietreanu ${}^{\textrm{\scriptsize 27b}}$ , J.E. Pilcher ${}^{\textrm{\scriptsize 37}}$ , A.D. Pilkington ${}^{\textrm{\scriptsize 101}}$ , M. Pinamonti ${}^{\textrm{\scriptsize 67a,67c}}$ , J.L. Pinfold ${}^{\textrm{\scriptsize 3}}$ , C. Pitman Donaldson ${}^{\textrm{\scriptsize 95}}$ , M. Pitt ${}^{\textrm{\scriptsize 160}}$ , L. Pizzimento ${}^{\textrm{\scriptsize 74a,74b}}$ , M.-A. Pleier ${}^{\textrm{\scriptsize 29}}$ , V. Pleskot ${}^{\textrm{\scriptsize 142}}$ , E. Plotnikova ${}^{\textrm{\scriptsize 80}}$ , P. Podberezko ${}^{\textrm{\scriptsize 122b,122a}}$ , R. Poettgen ${}^{\textrm{\scriptsize 97}}$ , R. Poggi ${}^{\textrm{\scriptsize 54}}$ , L. Poggioli ${}^{\textrm{\scriptsize 135}}$ , I. Pogrebnyak ${}^{\textrm{\scriptsize 107}}$ , D. Pohl ${}^{\textrm{\scriptsize 24}}$ , I. Pokharel ${}^{\textrm{\scriptsize 53}}$ , G. Polesello ${}^{\textrm{\scriptsize 71a}}$ , A. Poley ${}^{\textrm{\scriptsize 151,167a}}$ , A. Policicchio ${}^{\textrm{\scriptsize 73a,73b}}$ , R. Polifka ${}^{\textrm{\scriptsize 142}}$ , A. Polini ${}^{\textrm{\scriptsize 23b}}$ , C.S. Pollard ${}^{\textrm{\scriptsize 46}}$ , V. Polychronakos ${}^{\textrm{\scriptsize 29}}$ , D. Ponomarenko ${}^{\textrm{\scriptsize 112}}$ , L. Pontecorvo ${}^{\textrm{\scriptsize 36}}$ , S. Popa ${}^{\textrm{\scriptsize 27a}}$ , G.A. Popeneciu ${}^{\textrm{\scriptsize 27d}}$ , L. Portales ${}^{\textrm{\scriptsize 5}}$ , D.M. Portillo Quintero ${}^{\textrm{\scriptsize 58}}$ , S. Pospisil ${}^{\textrm{\scriptsize 141}}$ , K. Potamianos ${}^{\textrm{\scriptsize 46}}$ , I.N. Potrap ${}^{\textrm{\scriptsize 80}}$ , C.J. Potter ${}^{\textrm{\scriptsize 32}}$ , H. Potti ${}^{\textrm{\scriptsize 11}}$ , T. Poulsen ${}^{\textrm{\scriptsize 97}}$ , J. Poveda ${}^{\textrm{\scriptsize 173}}$ , T.D. Powell ${}^{\textrm{\scriptsize 148}}$ , G. Pownall ${}^{\textrm{\scriptsize 46}}$ , M.E. Pozo Astigarraga ${}^{\textrm{\scriptsize 36}}$ , P. Pralavorio ${}^{\textrm{\scriptsize 102}}$ , S. Prell ${}^{\textrm{\scriptsize 79}}$ , D. Price ${}^{\textrm{\scriptsize 101}}$ , M. Primavera ${}^{\textrm{\scriptsize 68a}}$ , M.L. Proffitt ${}^{\textrm{\scriptsize 147}}$ , N. Proklova ${}^{\textrm{\scriptsize 112}}$ , K. Prokofiev ${}^{\textrm{\scriptsize 63c}}$ , F. Prokoshin ${}^{\textrm{\scriptsize 80}}$ , S. Protopopescu ${}^{\textrm{\scriptsize 29}}$ , J. Proudfoot ${}^{\textrm{\scriptsize 6}}$ , M. Przybycien ${}^{\textrm{\scriptsize 84a}}$ , D. Pudzha ${}^{\textrm{\scriptsize 137}}$ , A. Puri ${}^{\textrm{\scriptsize 172}}$ , P. Puzo ${}^{\textrm{\scriptsize 65}}$ , D. Pyatiizbyantseva ${}^{\textrm{\scriptsize 112}}$ , J. Qian ${}^{\textrm{\scriptsize 106}}$ , Y. Qin ${}^{\textrm{\scriptsize 101}}$ , A. Quadt ${}^{\textrm{\scriptsize 53}}$ , M. Queitsch-Maitland ${}^{\textrm{\scriptsize 36}}$ , A. Qureshi ${}^{\textrm{\scriptsize 1}}$ , M. Racko ${}^{\textrm{\scriptsize 28a}}$ , F. Ragusa ${}^{\textrm{\scriptsize 69a,69b}}$ , G. Rahal ${}^{\textrm{\scriptsize 98}}$ , J.A. Raine ${}^{\textrm{\scriptsize 54}}$ , S. Rajagopalan ${}^{\textrm{\scriptsize 29}}$ , A. Ramirez Morales ${}^{\textrm{\scriptsize 93}}$ , K. Ran ${}^{\textrm{\scriptsize 15a,15d}}$ , D.M. Rauch ${}^{\textrm{\scriptsize 46}}$ , F. Rauscher ${}^{\textrm{\scriptsize 114}}$ , S. Rave ${}^{\textrm{\scriptsize 100}}$ , B. Ravina ${}^{\textrm{\scriptsize 148}}$ , I. Ravinovich ${}^{\textrm{\scriptsize 179}}$ , J.H. Rawling ${}^{\textrm{\scriptsize 101}}$ , M. Raymond ${}^{\textrm{\scriptsize 36}}$ , A.L. Read ${}^{\textrm{\scriptsize 133}}$ , N.P. Readioff ${}^{\textrm{\scriptsize 58}}$ , M. Reale ${}^{\textrm{\scriptsize 68a,68b}}$ , D.M. Rebuzzi ${}^{\textrm{\scriptsize 71a,71b}}$ , G. Redlinger ${}^{\textrm{\scriptsize 29}}$ , K. Reeves ${}^{\textrm{\scriptsize 43}}$ , J. Reichert ${}^{\textrm{\scriptsize 136}}$ , D. Reikher ${}^{\textrm{\scriptsize 160}}$ , A. Reiss ${}^{\textrm{\scriptsize 100}}$ , A. Rej ${}^{\textrm{\scriptsize 150}}$ , C. Rembser ${}^{\textrm{\scriptsize 36}}$ , A. Renardi ${}^{\textrm{\scriptsize 46}}$ , M. Renda ${}^{\textrm{\scriptsize 27b}}$ , M.B. Rendel ${}^{\textrm{\scriptsize 115}}$ , S. Resconi ${}^{\textrm{\scriptsize 69a}}$ , E.D. Resseguie ${}^{\textrm{\scriptsize 18}}$ , S. Rettie ${}^{\textrm{\scriptsize 95}}$ , B. Reynolds ${}^{\textrm{\scriptsize 127}}$ , E. Reynolds ${}^{\textrm{\scriptsize 21}}$ , O.L. Rezanova ${}^{\textrm{\scriptsize 122b,122a}}$ , P. Reznicek ${}^{\textrm{\scriptsize 142}}$ , E. Ricci ${}^{\textrm{\scriptsize 76a,76b}}$ , R. Richter ${}^{\textrm{\scriptsize 115}}$ , S. Richter ${}^{\textrm{\scriptsize 46}}$ , E. Richter-Was ${}^{\textrm{\scriptsize 84b}}$ , M. Ridel ${}^{\textrm{\scriptsize 135}}$ , P. Rieck ${}^{\textrm{\scriptsize 115}}$ , O. Rifki ${}^{\textrm{\scriptsize 46}}$ , M. Rijssenbeek ${}^{\textrm{\scriptsize 154}}$ , A. Rimoldi ${}^{\textrm{\scriptsize 71a,71b}}$ , M. Rimoldi ${}^{\textrm{\scriptsize 46}}$ , L. Rinaldi ${}^{\textrm{\scriptsize 23b}}$ , T.T. Rinn ${}^{\textrm{\scriptsize 172}}$ , G. Ripellino ${}^{\textrm{\scriptsize 153}}$ , I. Riu ${}^{\textrm{\scriptsize 14}}$ , P. Rivadeneira ${}^{\textrm{\scriptsize 46}}$ , J.C. Rivera Vergara ${}^{\textrm{\scriptsize 175}}$ , F. Rizatdinova ${}^{\textrm{\scriptsize 129}}$ , E. Rizvi ${}^{\textrm{\scriptsize 93}}$ , C. Rizzi ${}^{\textrm{\scriptsize 36}}$ , S.H. Robertson ${}^{\textrm{\scriptsize 104,ab}}$ , M. Robin ${}^{\textrm{\scriptsize 46}}$ , D. Robinson ${}^{\textrm{\scriptsize 32}}$ , C.M. Robles Gajardo ${}^{\textrm{\scriptsize 146d}}$ , M. Robles Manzano ${}^{\textrm{\scriptsize 100}}$ , A. Robson ${}^{\textrm{\scriptsize 57}}$ , A. Rocchi ${}^{\textrm{\scriptsize 74a,74b}}$ , E. Rocco ${}^{\textrm{\scriptsize 100}}$ , C. Roda ${}^{\textrm{\scriptsize 72a,72b}}$ , S. Rodriguez Bosca ${}^{\textrm{\scriptsize 173}}$ , A.M. Rodríguez Vera ${}^{\textrm{\scriptsize 167b}}$ , S. Roe ${}^{\textrm{\scriptsize 36}}$ , J. Roggel ${}^{\textrm{\scriptsize 181}}$ , O. Røhne ${}^{\textrm{\scriptsize 133}}$ , R. Röhrig ${}^{\textrm{\scriptsize 115}}$ , R.A. Rojas ${}^{\textrm{\scriptsize 146d}}$ , B. Roland ${}^{\textrm{\scriptsize 52}}$ , C.P.A. Roland ${}^{\textrm{\scriptsize 66}}$ , J. Roloff ${}^{\textrm{\scriptsize 29}}$ , A. Romaniouk ${}^{\textrm{\scriptsize 112}}$ , M. Romano ${}^{\textrm{\scriptsize 23b,23a}}$ , N. Rompotis ${}^{\textrm{\scriptsize 91}}$ , M. Ronzani ${}^{\textrm{\scriptsize 125}}$ , L. Roos ${}^{\textrm{\scriptsize 135}}$ , S. Rosati ${}^{\textrm{\scriptsize 73a}}$ , G. Rosin ${}^{\textrm{\scriptsize 103}}$ , B.J. Rosser ${}^{\textrm{\scriptsize 136}}$ , E. Rossi ${}^{\textrm{\scriptsize 46}}$ , E. Rossi ${}^{\textrm{\scriptsize 75a,75b}}$ , E. Rossi ${}^{\textrm{\scriptsize 70a,70b}}$ , L.P. Rossi ${}^{\textrm{\scriptsize 55b}}$ , L. Rossini ${}^{\textrm{\scriptsize 69a,69b}}$ , R. Rosten ${}^{\textrm{\scriptsize 14}}$ , M. Rotaru ${}^{\textrm{\scriptsize 27b}}$ , B. Rottler ${}^{\textrm{\scriptsize 52}}$ , D. Rousseau ${}^{\textrm{\scriptsize 65}}$ , G. Rovelli ${}^{\textrm{\scriptsize 71a,71b}}$ , A. Roy ${}^{\textrm{\scriptsize 11}}$ , D. Roy ${}^{\textrm{\scriptsize 33e}}$ , A. Rozanov ${}^{\textrm{\scriptsize 102}}$ , Y. Rozen ${}^{\textrm{\scriptsize 159}}$ , X. Ruan ${}^{\textrm{\scriptsize 33e}}$ , F. Rühr ${}^{\textrm{\scriptsize 52}}$ , A. Ruiz-Martinez ${}^{\textrm{\scriptsize 173}}$ , A. 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Savard ${}^{\textrm{\scriptsize 166,al}}$ , R. Sawada ${}^{\textrm{\scriptsize 162}}$ , C. Sawyer ${}^{\textrm{\scriptsize 143}}$ , L. Sawyer ${}^{\textrm{\scriptsize 96,af}}$ , I. Sayago Galvan ${}^{\textrm{\scriptsize 173}}$ , C. Sbarra ${}^{\textrm{\scriptsize 23b}}$ , A. Sbrizzi ${}^{\textrm{\scriptsize 67a,67c}}$ , T. Scanlon ${}^{\textrm{\scriptsize 95}}$ , J. Schaarschmidt ${}^{\textrm{\scriptsize 147}}$ , P. Schacht ${}^{\textrm{\scriptsize 115}}$ , D. Schaefer ${}^{\textrm{\scriptsize 37}}$ , L. Schaefer ${}^{\textrm{\scriptsize 136}}$ , S. Schaepe ${}^{\textrm{\scriptsize 36}}$ , U. Schäfer ${}^{\textrm{\scriptsize 100}}$ , A.C. Schaffer ${}^{\textrm{\scriptsize 65}}$ , D. Schaile ${}^{\textrm{\scriptsize 114}}$ , R.D. Schamberger ${}^{\textrm{\scriptsize 154}}$ , E. Schanet ${}^{\textrm{\scriptsize 114}}$ , N. Scharmberg ${}^{\textrm{\scriptsize 101}}$ , V.A. Schegelsky ${}^{\textrm{\scriptsize 137}}$ , D. Scheirich ${}^{\textrm{\scriptsize 142}}$ , F. Schenck ${}^{\textrm{\scriptsize 19}}$ , M. Schernau ${}^{\textrm{\scriptsize 170}}$ , C. Schiavi ${}^{\textrm{\scriptsize 55b,55a}}$ , L.K. Schildgen ${}^{\textrm{\scriptsize 24}}$ , Z.M. Schillaci ${}^{\textrm{\scriptsize 26}}$ , E.J. Schioppa ${}^{\textrm{\scriptsize 68a,68b}}$ , M. Schioppa ${}^{\textrm{\scriptsize 41b,41a}}$ , K.E. Schleicher ${}^{\textrm{\scriptsize 52}}$ , S. Schlenker ${}^{\textrm{\scriptsize 36}}$ , K.R. Schmidt-Sommerfeld ${}^{\textrm{\scriptsize 115}}$ , K. Schmieden ${}^{\textrm{\scriptsize 36}}$ , C. Schmitt ${}^{\textrm{\scriptsize 100}}$ , S. Schmitt ${}^{\textrm{\scriptsize 46}}$ , J.C. Schmoeckel ${}^{\textrm{\scriptsize 46}}$ , L. Schoeffel ${}^{\textrm{\scriptsize 144}}$ , A. Schoening ${}^{\textrm{\scriptsize 61b}}$ , P.G. Scholer ${}^{\textrm{\scriptsize 52}}$ , E. Schopf ${}^{\textrm{\scriptsize 134}}$ , M. Schott ${}^{\textrm{\scriptsize 100}}$ , J.F.P. Schouwenberg ${}^{\textrm{\scriptsize 119}}$ , J. Schovancova ${}^{\textrm{\scriptsize 36}}$ , S. Schramm ${}^{\textrm{\scriptsize 54}}$ , F. Schroeder ${}^{\textrm{\scriptsize 181}}$ , A. Schulte ${}^{\textrm{\scriptsize 100}}$ , H-C. Schultz-Coulon ${}^{\textrm{\scriptsize 61a}}$ , M. Schumacher ${}^{\textrm{\scriptsize 52}}$ , B.A. Schumm ${}^{\textrm{\scriptsize 145}}$ , Ph. Schune ${}^{\textrm{\scriptsize 144}}$ , A. Schwartzman ${}^{\textrm{\scriptsize 152}}$ , T.A. Schwarz ${}^{\textrm{\scriptsize 106}}$ , Ph. Schwemling ${}^{\textrm{\scriptsize 144}}$ , R. Schwienhorst ${}^{\textrm{\scriptsize 107}}$ , A. Sciandra ${}^{\textrm{\scriptsize 145}}$ , G. Sciolla ${}^{\textrm{\scriptsize 26}}$ , M. Scornajenghi ${}^{\textrm{\scriptsize 41b,41a}}$ , F. Scuri ${}^{\textrm{\scriptsize 72a}}$ , F. Scutti ${}^{\textrm{\scriptsize 105}}$ , L.M. Scyboz ${}^{\textrm{\scriptsize 115}}$ , C.D. Sebastiani ${}^{\textrm{\scriptsize 91}}$ , P. Seema ${}^{\textrm{\scriptsize 19}}$ , S.C. Seidel ${}^{\textrm{\scriptsize 118}}$ , A. Seiden ${}^{\textrm{\scriptsize 145}}$ , B.D. Seidlitz ${}^{\textrm{\scriptsize 29}}$ , T. Seiss ${}^{\textrm{\scriptsize 37}}$ , C. Seitz ${}^{\textrm{\scriptsize 46}}$ , J.M. Seixas ${}^{\textrm{\scriptsize 81b}}$ , G. Sekhniaidze ${}^{\textrm{\scriptsize 70a}}$ , S.J. Sekula ${}^{\textrm{\scriptsize 42}}$ , N. Semprini-Cesari ${}^{\textrm{\scriptsize 23b,23a}}$ , S. Sen ${}^{\textrm{\scriptsize 49}}$ , C. Serfon ${}^{\textrm{\scriptsize 29}}$ , L. Serin ${}^{\textrm{\scriptsize 65}}$ , L. Serkin ${}^{\textrm{\scriptsize 67a,67b}}$ , M. Sessa ${}^{\textrm{\scriptsize 60a}}$ , H. Severini ${}^{\textrm{\scriptsize 128}}$ , S. Sevova ${}^{\textrm{\scriptsize 152}}$ , F. Sforza ${}^{\textrm{\scriptsize 55b,55a}}$ , A. Sfyrla ${}^{\textrm{\scriptsize 54}}$ , E. Shabalina ${}^{\textrm{\scriptsize 53}}$ , J.D. Shahinian ${}^{\textrm{\scriptsize 145}}$ , N.W. Shaikh ${}^{\textrm{\scriptsize 45a,45b}}$ , D. Shaked Renous ${}^{\textrm{\scriptsize 179}}$ , L.Y. Shan ${}^{\textrm{\scriptsize 15a}}$ , M. Shapiro ${}^{\textrm{\scriptsize 18}}$ , A. Sharma ${}^{\textrm{\scriptsize 134}}$ , A.S. Sharma ${}^{\textrm{\scriptsize 1}}$ , P.B. Shatalov ${}^{\textrm{\scriptsize 124}}$ , K. Shaw ${}^{\textrm{\scriptsize 155}}$ , S.M. Shaw ${}^{\textrm{\scriptsize 101}}$ , M. Shehade ${}^{\textrm{\scriptsize 179}}$ , Y. Shen ${}^{\textrm{\scriptsize 128}}$ , A.D. Sherman ${}^{\textrm{\scriptsize 25}}$ , P. Sherwood ${}^{\textrm{\scriptsize 95}}$ , L. Shi ${}^{\textrm{\scriptsize 95}}$ , S. Shimizu ${}^{\textrm{\scriptsize 82}}$ , C.O. Shimmin ${}^{\textrm{\scriptsize 182}}$ , Y. Shimogama ${}^{\textrm{\scriptsize 178}}$ , M. Shimojima ${}^{\textrm{\scriptsize 116}}$ , I.P.J. Shipsey ${}^{\textrm{\scriptsize 134}}$ , S. Shirabe ${}^{\textrm{\scriptsize 164}}$ , M. Shiyakova ${}^{\textrm{\scriptsize 80,z}}$ , J. Shlomi ${}^{\textrm{\scriptsize 179}}$ , A. Shmeleva ${}^{\textrm{\scriptsize 111}}$ , M.J. Shochet ${}^{\textrm{\scriptsize 37}}$ , J. Shojaii ${}^{\textrm{\scriptsize 105}}$ , D.R. Shope ${}^{\textrm{\scriptsize 128}}$ , S. Shrestha ${}^{\textrm{\scriptsize 127}}$ , E.M. Shrif ${}^{\textrm{\scriptsize 33e}}$ , E. Shulga ${}^{\textrm{\scriptsize 179}}$ , P. Sicho ${}^{\textrm{\scriptsize 140}}$ , A.M. Sickles ${}^{\textrm{\scriptsize 172}}$ , E. Sideras Haddad ${}^{\textrm{\scriptsize 33e}}$ , O. Sidiropoulou ${}^{\textrm{\scriptsize 36}}$ , A. Sidoti ${}^{\textrm{\scriptsize 23b,23a}}$ , F. Siegert ${}^{\textrm{\scriptsize 48}}$ , Dj. Sijacki ${}^{\textrm{\scriptsize 16}}$ , M.Jr. Silva ${}^{\textrm{\scriptsize 180}}$ , M.V. Silva Oliveira ${}^{\textrm{\scriptsize 36}}$ , S.B. Silverstein ${}^{\textrm{\scriptsize 45a}}$ , S. Simion ${}^{\textrm{\scriptsize 65}}$ , R. Simoniello ${}^{\textrm{\scriptsize 100}}$ , C.J. Simpson-allsop ${}^{\textrm{\scriptsize 21}}$ , S. Simsek ${}^{\textrm{\scriptsize 12b}}$ , P. Sinervo ${}^{\textrm{\scriptsize 166}}$ , V. Sinetckii ${}^{\textrm{\scriptsize 113}}$ , S. Singh ${}^{\textrm{\scriptsize 151}}$ , M. Sioli ${}^{\textrm{\scriptsize 23b,23a}}$ , I. Siral ${}^{\textrm{\scriptsize 131}}$ , S.Yu. Sivoklokov ${}^{\textrm{\scriptsize 113}}$ , J. Sjölin ${}^{\textrm{\scriptsize 45a,45b}}$ , A. Skaf ${}^{\textrm{\scriptsize 53}}$ , E. Skorda ${}^{\textrm{\scriptsize 97}}$ , P. Skubic ${}^{\textrm{\scriptsize 128}}$ , M. Slawinska ${}^{\textrm{\scriptsize 85}}$ , K. Sliwa ${}^{\textrm{\scriptsize 169}}$ , R. Slovak ${}^{\textrm{\scriptsize 142}}$ , V. Smakhtin ${}^{\textrm{\scriptsize 179}}$ , B.H. Smart ${}^{\textrm{\scriptsize 143}}$ , J. Smiesko ${}^{\textrm{\scriptsize 28b}}$ , N. Smirnov ${}^{\textrm{\scriptsize 112}}$ , S.Yu. Smirnov ${}^{\textrm{\scriptsize 112}}$ , Y. Smirnov ${}^{\textrm{\scriptsize 112}}$ , L.N. Smirnova ${}^{\textrm{\scriptsize 113,r}}$ , O. Smirnova ${}^{\textrm{\scriptsize 97}}$ , H.A. Smith ${}^{\textrm{\scriptsize 134}}$ , M. Smizanska ${}^{\textrm{\scriptsize 90}}$ , K. Smolek ${}^{\textrm{\scriptsize 141}}$ , A. Smykiewicz ${}^{\textrm{\scriptsize 85}}$ , A.A. Snesarev ${}^{\textrm{\scriptsize 111}}$ , H.L. Snoek ${}^{\textrm{\scriptsize 120}}$ , I.M. Snyder ${}^{\textrm{\scriptsize 131}}$ , S. Snyder ${}^{\textrm{\scriptsize 29}}$ , R. Sobie ${}^{\textrm{\scriptsize 175,ab}}$ , A. Soffer ${}^{\textrm{\scriptsize 160}}$ , A. Søgaard ${}^{\textrm{\scriptsize 50}}$ , F. Sohns ${}^{\textrm{\scriptsize 53}}$ , C.A. Solans Sanchez ${}^{\textrm{\scriptsize 36}}$ , E.Yu. Soldatov ${}^{\textrm{\scriptsize 112}}$ , U. Soldevila ${}^{\textrm{\scriptsize 173}}$ , A.A. Solodkov ${}^{\textrm{\scriptsize 123}}$ , A. Soloshenko ${}^{\textrm{\scriptsize 80}}$ , O.V. Solovyanov ${}^{\textrm{\scriptsize 123}}$ , V. Solovyev ${}^{\textrm{\scriptsize 137}}$ , P. Sommer ${}^{\textrm{\scriptsize 148}}$ , H. Son ${}^{\textrm{\scriptsize 169}}$ , W. Song ${}^{\textrm{\scriptsize 143}}$ , W.Y. Song ${}^{\textrm{\scriptsize 167b}}$ , A. Sopczak ${}^{\textrm{\scriptsize 141}}$ , A.L. 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Stanislaus ${}^{\textrm{\scriptsize 134}}$ , M.M. Stanitzki ${}^{\textrm{\scriptsize 46}}$ , M. Stankaityte ${}^{\textrm{\scriptsize 134}}$ , B. Stapf ${}^{\textrm{\scriptsize 120}}$ , E.A. Starchenko ${}^{\textrm{\scriptsize 123}}$ , G.H. Stark ${}^{\textrm{\scriptsize 145}}$ , J. Stark ${}^{\textrm{\scriptsize 58}}$ , P. Staroba ${}^{\textrm{\scriptsize 140}}$ , P. Starovoitov ${}^{\textrm{\scriptsize 61a}}$ , S. Stärz ${}^{\textrm{\scriptsize 104}}$ , R. Staszewski ${}^{\textrm{\scriptsize 85}}$ , G. Stavropoulos ${}^{\textrm{\scriptsize 44}}$ , M. Stegler ${}^{\textrm{\scriptsize 46}}$ , P. Steinberg ${}^{\textrm{\scriptsize 29}}$ , A.L. Steinhebel ${}^{\textrm{\scriptsize 131}}$ , B. Stelzer ${}^{\textrm{\scriptsize 151}}$ , H.J. Stelzer ${}^{\textrm{\scriptsize 138}}$ , O. Stelzer-Chilton ${}^{\textrm{\scriptsize 167a}}$ , H. Stenzel ${}^{\textrm{\scriptsize 56}}$ , T.J. Stevenson ${}^{\textrm{\scriptsize 155}}$ , G.A. Stewart ${}^{\textrm{\scriptsize 36}}$ , M.C. Stockton ${}^{\textrm{\scriptsize 36}}$ , G. Stoicea ${}^{\textrm{\scriptsize 27b}}$ , M. Stolarski ${}^{\textrm{\scriptsize 139a}}$ , S. Stonjek ${}^{\textrm{\scriptsize 115}}$ , A. Straessner ${}^{\textrm{\scriptsize 48}}$ , J. Strandberg ${}^{\textrm{\scriptsize 153}}$ , S. Strandberg ${}^{\textrm{\scriptsize 45a,45b}}$ , M. Strauss ${}^{\textrm{\scriptsize 128}}$ , T. Strebler ${}^{\textrm{\scriptsize 102}}$ , P. Strizenec ${}^{\textrm{\scriptsize 28b}}$ , R. Ströhmer ${}^{\textrm{\scriptsize 176}}$ , D.M. Strom ${}^{\textrm{\scriptsize 131}}$ , R. Stroynowski ${}^{\textrm{\scriptsize 42}}$ , A. Strubig ${}^{\textrm{\scriptsize 50}}$ , S.A. Stucci ${}^{\textrm{\scriptsize 29}}$ , B. Stugu ${}^{\textrm{\scriptsize 17}}$ , J. Stupak ${}^{\textrm{\scriptsize 128}}$ , N.A. Styles ${}^{\textrm{\scriptsize 46}}$ , D. Su ${}^{\textrm{\scriptsize 152}}$ , W. Su ${}^{\textrm{\scriptsize 60c,147}}$ , S. Suchek ${}^{\textrm{\scriptsize 61a}}$ , V.V. Sulin ${}^{\textrm{\scriptsize 111}}$ , M.J. Sullivan ${}^{\textrm{\scriptsize 91}}$ , D.M.S. Sultan ${}^{\textrm{\scriptsize 54}}$ , S. Sultansoy ${}^{\textrm{\scriptsize 4c}}$ , T. Sumida ${}^{\textrm{\scriptsize 86}}$ , S. Sun ${}^{\textrm{\scriptsize 106}}$ , X. Sun ${}^{\textrm{\scriptsize 101}}$ , K. Suruliz ${}^{\textrm{\scriptsize 155}}$ , C.J.E. Suster ${}^{\textrm{\scriptsize 156}}$ , M.R. Sutton ${}^{\textrm{\scriptsize 155}}$ , S. Suzuki ${}^{\textrm{\scriptsize 82}}$ , M. Svatos ${}^{\textrm{\scriptsize 140}}$ , M. Swiatlowski ${}^{\textrm{\scriptsize 167a}}$ , S.P. Swift ${}^{\textrm{\scriptsize 2}}$ , T. Swirski ${}^{\textrm{\scriptsize 176}}$ , A. Sydorenko ${}^{\textrm{\scriptsize 100}}$ , I. Sykora ${}^{\textrm{\scriptsize 28a}}$ , M. Sykora ${}^{\textrm{\scriptsize 142}}$ , T. Sykora ${}^{\textrm{\scriptsize 142}}$ , D. Ta ${}^{\textrm{\scriptsize 100}}$ , K. Tackmann ${}^{\textrm{\scriptsize 46,x}}$ , J. Taenzer ${}^{\textrm{\scriptsize 160}}$ , A. 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Tasevsky ${}^{\textrm{\scriptsize 140}}$ , T. Tashiro ${}^{\textrm{\scriptsize 86}}$ , E. Tassi ${}^{\textrm{\scriptsize 41b,41a}}$ , A. Tavares Delgado ${}^{\textrm{\scriptsize 139a}}$ , Y. Tayalati ${}^{\textrm{\scriptsize 35e}}$ , A.J. Taylor ${}^{\textrm{\scriptsize 50}}$ , G.N. Taylor ${}^{\textrm{\scriptsize 105}}$ , W. Taylor ${}^{\textrm{\scriptsize 167b}}$ , H. Teagle ${}^{\textrm{\scriptsize 91}}$ , A.S. Tee ${}^{\textrm{\scriptsize 90}}$ , R. Teixeira De Lima ${}^{\textrm{\scriptsize 152}}$ , P. Teixeira-Dias ${}^{\textrm{\scriptsize 94}}$ , H. Ten Kate ${}^{\textrm{\scriptsize 36}}$ , J.J. Teoh ${}^{\textrm{\scriptsize 120}}$ , S. Terada ${}^{\textrm{\scriptsize 82}}$ , K. Terashi ${}^{\textrm{\scriptsize 162}}$ , J. Terron ${}^{\textrm{\scriptsize 99}}$ , S. Terzo ${}^{\textrm{\scriptsize 14}}$ , M. Testa ${}^{\textrm{\scriptsize 51}}$ , R.J. Teuscher ${}^{\textrm{\scriptsize 166,ab}}$ , S.J. Thais ${}^{\textrm{\scriptsize 182}}$ , N. Themistokleous ${}^{\textrm{\scriptsize 50}}$ , T. Theveneaux-Pelzer ${}^{\textrm{\scriptsize 46}}$ , F. Thiele ${}^{\textrm{\scriptsize 40}}$ , D.W. Thomas ${}^{\textrm{\scriptsize 94}}$ , J.O. Thomas ${}^{\textrm{\scriptsize 42}}$ , J.P. Thomas ${}^{\textrm{\scriptsize 21}}$ , E.A. Thompson ${}^{\textrm{\scriptsize 46}}$ , P.D. Thompson ${}^{\textrm{\scriptsize 21}}$ , E. Thomson ${}^{\textrm{\scriptsize 136}}$ , E.J. Thorpe ${}^{\textrm{\scriptsize 93}}$ , R.E. Ticse Torres ${}^{\textrm{\scriptsize 53}}$ , V.O. Tikhomirov ${}^{\textrm{\scriptsize 111,ah}}$ , Yu.A. Tikhonov ${}^{\textrm{\scriptsize 122b,122a}}$ , S. Timoshenko ${}^{\textrm{\scriptsize 112}}$ , P. Tipton ${}^{\textrm{\scriptsize 182}}$ , S. Tisserant ${}^{\textrm{\scriptsize 102}}$ , K. Todome ${}^{\textrm{\scriptsize 23b,23a}}$ , S. Todorova-Nova ${}^{\textrm{\scriptsize 142}}$ , S. Todt ${}^{\textrm{\scriptsize 48}}$ , J. Tojo ${}^{\textrm{\scriptsize 88}}$ , S. Tokár ${}^{\textrm{\scriptsize 28a}}$ , K. Tokushuku ${}^{\textrm{\scriptsize 82}}$ , E. Tolley ${}^{\textrm{\scriptsize 127}}$ , R. Tombs ${}^{\textrm{\scriptsize 32}}$ , K.G. Tomiwa ${}^{\textrm{\scriptsize 33e}}$ , M. Tomoto ${}^{\textrm{\scriptsize 117}}$ , L. Tompkins ${}^{\textrm{\scriptsize 152}}$ , P. Tornambe ${}^{\textrm{\scriptsize 103}}$ , E. Torrence ${}^{\textrm{\scriptsize 131}}$ , H. Torres ${}^{\textrm{\scriptsize 48}}$ , E. Torró Pastor ${}^{\textrm{\scriptsize 147}}$ , C. Tosciri ${}^{\textrm{\scriptsize 134}}$ , J. Toth ${}^{\textrm{\scriptsize 102,aa}}$ , D.R. Tovey ${}^{\textrm{\scriptsize 148}}$ , A. Traeet ${}^{\textrm{\scriptsize 17}}$ , C.J. Treado ${}^{\textrm{\scriptsize 125}}$ , T. Trefzger ${}^{\textrm{\scriptsize 176}}$ , F. Tresoldi ${}^{\textrm{\scriptsize 155}}$ , A. Tricoli ${}^{\textrm{\scriptsize 29}}$ , I.M. Trigger ${}^{\textrm{\scriptsize 167a}}$ , S. Trincaz-Duvoid ${}^{\textrm{\scriptsize 135}}$ , D.A. Trischuk ${}^{\textrm{\scriptsize 174}}$ , W. Trischuk ${}^{\textrm{\scriptsize 166}}$ , B. Trocmé ${}^{\textrm{\scriptsize 58}}$ , A. Trofymov ${}^{\textrm{\scriptsize 65}}$ , C. Troncon ${}^{\textrm{\scriptsize 69a}}$ , F. Trovato ${}^{\textrm{\scriptsize 155}}$ , L. Truong ${}^{\textrm{\scriptsize 33c}}$ , M. Trzebinski ${}^{\textrm{\scriptsize 85}}$ , A. Trzupek ${}^{\textrm{\scriptsize 85}}$ , F. Tsai ${}^{\textrm{\scriptsize 46}}$ , J.C-L. Tseng ${}^{\textrm{\scriptsize 134}}$ , P.V. Tsiareshka ${}^{\textrm{\scriptsize 108,ae}}$ , A. Tsirigotis ${}^{\textrm{\scriptsize 161,u}}$ , V. Tsiskaridze ${}^{\textrm{\scriptsize 154}}$ , E.G. Tskhadadze ${}^{\textrm{\scriptsize 158a}}$ , M. Tsopoulou ${}^{\textrm{\scriptsize 161}}$ , I.I. Tsukerman ${}^{\textrm{\scriptsize 124}}$ , V. Tsulaia ${}^{\textrm{\scriptsize 18}}$ , S. Tsuno ${}^{\textrm{\scriptsize 82}}$ , D. Tsybychev ${}^{\textrm{\scriptsize 154}}$ , Y. Tu ${}^{\textrm{\scriptsize 63b}}$ , A. Tudorache ${}^{\textrm{\scriptsize 27b}}$ , V. Tudorache ${}^{\textrm{\scriptsize 27b}}$ , T.T. Tulbure ${}^{\textrm{\scriptsize 27a}}$ , A.N. Tuna ${}^{\textrm{\scriptsize 59}}$ , S. Turchikhin ${}^{\textrm{\scriptsize 80}}$ , D. Turgeman ${}^{\textrm{\scriptsize 179}}$ , I. Turk Cakir ${}^{\textrm{\scriptsize 4b,s}}$ , R.J. Turner ${}^{\textrm{\scriptsize 21}}$ , R. Turra ${}^{\textrm{\scriptsize 69a}}$ , P.M. Tuts ${}^{\textrm{\scriptsize 39}}$ , S. Tzamarias ${}^{\textrm{\scriptsize 161}}$ , E. Tzovara ${}^{\textrm{\scriptsize 100}}$ , K. Uchida ${}^{\textrm{\scriptsize 162}}$ , F. Ukegawa ${}^{\textrm{\scriptsize 168}}$ , G. Unal ${}^{\textrm{\scriptsize 36}}$ , M. Unal ${}^{\textrm{\scriptsize 11}}$ , A. Undrus ${}^{\textrm{\scriptsize 29}}$ , G. Unel ${}^{\textrm{\scriptsize 170}}$ , F.C. Ungaro ${}^{\textrm{\scriptsize 105}}$ , Y. Unno ${}^{\textrm{\scriptsize 82}}$ , K. Uno ${}^{\textrm{\scriptsize 162}}$ , J. Urban ${}^{\textrm{\scriptsize 28b}}$ , P. Urquijo ${}^{\textrm{\scriptsize 105}}$ , G. Usai ${}^{\textrm{\scriptsize 8}}$ , Z. Uysal ${}^{\textrm{\scriptsize 12d}}$ , V. Vacek ${}^{\textrm{\scriptsize 141}}$ , B. Vachon ${}^{\textrm{\scriptsize 104}}$ , K.O.H. Vadla ${}^{\textrm{\scriptsize 133}}$ , T. Vafeiadis ${}^{\textrm{\scriptsize 36}}$ , A. Vaidya ${}^{\textrm{\scriptsize 95}}$ , C. Valderanis ${}^{\textrm{\scriptsize 114}}$ , E. Valdes Santurio ${}^{\textrm{\scriptsize 45a,45b}}$ , M. Valente ${}^{\textrm{\scriptsize 54}}$ , S. Valentinetti ${}^{\textrm{\scriptsize 23b,23a}}$ , A. Valero ${}^{\textrm{\scriptsize 173}}$ , L. Valéry ${}^{\textrm{\scriptsize 46}}$ , R.A. Vallance ${}^{\textrm{\scriptsize 21}}$ , A. Vallier ${}^{\textrm{\scriptsize 36}}$ , J.A. Valls Ferrer ${}^{\textrm{\scriptsize 173}}$ , T.R. Van Daalen ${}^{\textrm{\scriptsize 14}}$ , P. Van Gemmeren ${}^{\textrm{\scriptsize 6}}$ , I. Van Vulpen ${}^{\textrm{\scriptsize 120}}$ , M. Vanadia ${}^{\textrm{\scriptsize 74a,74b}}$ , W. Vandelli ${}^{\textrm{\scriptsize 36}}$ , M. Vandenbroucke ${}^{\textrm{\scriptsize 144}}$ , E.R. Vandewall ${}^{\textrm{\scriptsize 129}}$ , A. Vaniachine ${}^{\textrm{\scriptsize 165}}$ , D. Vannicola ${}^{\textrm{\scriptsize 73a,73b}}$ , R. Vari ${}^{\textrm{\scriptsize 73a}}$ , E.W. Varnes ${}^{\textrm{\scriptsize 7}}$ , C. Varni ${}^{\textrm{\scriptsize 55b,55a}}$ , T. Varol ${}^{\textrm{\scriptsize 157}}$ , D. Varouchas ${}^{\textrm{\scriptsize 65}}$ , K.E. Varvell ${}^{\textrm{\scriptsize 156}}$ , M.E. Vasile ${}^{\textrm{\scriptsize 27b}}$ , G.A. Vasquez ${}^{\textrm{\scriptsize 175}}$ , F. Vazeille ${}^{\textrm{\scriptsize 38}}$ , D. Vazquez Furelos ${}^{\textrm{\scriptsize 14}}$ , T. Vazquez Schroeder ${}^{\textrm{\scriptsize 36}}$ , J. Veatch ${}^{\textrm{\scriptsize 53}}$ , V. Vecchio ${}^{\textrm{\scriptsize 101}}$ , M.J. Veen ${}^{\textrm{\scriptsize 120}}$ , L.M. Veloce ${}^{\textrm{\scriptsize 166}}$ , F. Veloso ${}^{\textrm{\scriptsize 139a,139c}}$ , S. Veneziano ${}^{\textrm{\scriptsize 73a}}$ , A. Ventura ${}^{\textrm{\scriptsize 68a,68b}}$ , A. Verbytskyi ${}^{\textrm{\scriptsize 115}}$ , V. Vercesi ${}^{\textrm{\scriptsize 71a}}$ , M. Verducci ${}^{\textrm{\scriptsize 72a,72b}}$ , C.M. Vergel Infante ${}^{\textrm{\scriptsize 79}}$ , C. Vergis ${}^{\textrm{\scriptsize 24}}$ , W. Verkerke ${}^{\textrm{\scriptsize 120}}$ , A.T. Vermeulen ${}^{\textrm{\scriptsize 120}}$ , J.C. Vermeulen ${}^{\textrm{\scriptsize 120}}$ , C. Vernieri ${}^{\textrm{\scriptsize 152}}$ , M.C. Vetterli ${}^{\textrm{\scriptsize 151,al}}$ , N. Viaux Maira ${}^{\textrm{\scriptsize 146d}}$ , T. Vickey ${}^{\textrm{\scriptsize 148}}$ , O.E. Vickey Boeriu ${}^{\textrm{\scriptsize 148}}$ , G.H.A. Viehhauser ${}^{\textrm{\scriptsize 134}}$ , L. Vigani ${}^{\textrm{\scriptsize 61b}}$ , M. Villa ${}^{\textrm{\scriptsize 23b,23a}}$ , M. Villaplana Perez ${}^{\textrm{\scriptsize 3}}$ , E.M. Villhauer ${}^{\textrm{\scriptsize 50}}$ , E. Vilucchi ${}^{\textrm{\scriptsize 51}}$ , M.G. Vincter ${}^{\textrm{\scriptsize 34}}$ , G.S. Virdee ${}^{\textrm{\scriptsize 21}}$ , A. Vishwakarma ${}^{\textrm{\scriptsize 50}}$ , C. Vittori ${}^{\textrm{\scriptsize 23b,23a}}$ , I. Vivarelli ${}^{\textrm{\scriptsize 155}}$ , M. Vogel ${}^{\textrm{\scriptsize 181}}$ , P. Vokac ${}^{\textrm{\scriptsize 141}}$ , S.E. von Buddenbrock ${}^{\textrm{\scriptsize 33e}}$ , E. Von Toerne ${}^{\textrm{\scriptsize 24}}$ , V. Vorobel ${}^{\textrm{\scriptsize 142}}$ , K. Vorobev ${}^{\textrm{\scriptsize 112}}$ , M. Vos ${}^{\textrm{\scriptsize 173}}$ , J.H. Vossebeld ${}^{\textrm{\scriptsize 91}}$ , M. Vozak ${}^{\textrm{\scriptsize 101}}$ , N. Vranjes ${}^{\textrm{\scriptsize 16}}$ , M. Vranjes Milosavljevic ${}^{\textrm{\scriptsize 16}}$ , V. Vrba ${}^{\textrm{\scriptsize 141}}$ , M. Vreeswijk ${}^{\textrm{\scriptsize 120}}$ , R. Vuillermet ${}^{\textrm{\scriptsize 36}}$ , I. Vukotic ${}^{\textrm{\scriptsize 37}}$ , S. Wada ${}^{\textrm{\scriptsize 168}}$ , P. Wagner ${}^{\textrm{\scriptsize 24}}$ , W. Wagner ${}^{\textrm{\scriptsize 181}}$ , J. Wagner-Kuhr ${}^{\textrm{\scriptsize 114}}$ , S. Wahdan ${}^{\textrm{\scriptsize 181}}$ , H. Wahlberg ${}^{\textrm{\scriptsize 89}}$ , R. Wakasa ${}^{\textrm{\scriptsize 168}}$ , V.M. Walbrecht ${}^{\textrm{\scriptsize 115}}$ , J. Walder ${}^{\textrm{\scriptsize 90}}$ , R. Walker ${}^{\textrm{\scriptsize 114}}$ , S.D. Walker ${}^{\textrm{\scriptsize 94}}$ , W. Walkowiak ${}^{\textrm{\scriptsize 150}}$ , V. Wallangen ${}^{\textrm{\scriptsize 45a,45b}}$ , A.M. Wang ${}^{\textrm{\scriptsize 59}}$ , A.Z. Wang ${}^{\textrm{\scriptsize 180}}$ , C. Wang ${}^{\textrm{\scriptsize 60a}}$ , C. Wang ${}^{\textrm{\scriptsize 60c}}$ , F. Wang ${}^{\textrm{\scriptsize 180}}$ , H. Wang ${}^{\textrm{\scriptsize 18}}$ , H. Wang ${}^{\textrm{\scriptsize 3}}$ , J. Wang ${}^{\textrm{\scriptsize 63a}}$ , P. Wang ${}^{\textrm{\scriptsize 42}}$ , Q. Wang ${}^{\textrm{\scriptsize 128}}$ , R.-J. Wang ${}^{\textrm{\scriptsize 100}}$ , R. Wang ${}^{\textrm{\scriptsize 60a}}$ , R. Wang ${}^{\textrm{\scriptsize 6}}$ , S.M. Wang ${}^{\textrm{\scriptsize 157}}$ , W.T. Wang ${}^{\textrm{\scriptsize 60a}}$ , W. Wang ${}^{\textrm{\scriptsize 15c}}$ , W.X. Wang ${}^{\textrm{\scriptsize 60a}}$ , Y. Wang ${}^{\textrm{\scriptsize 60a}}$ , Z. Wang ${}^{\textrm{\scriptsize 106}}$ , C. Wanotayaroj ${}^{\textrm{\scriptsize 46}}$ , A. Warburton ${}^{\textrm{\scriptsize 104}}$ , C.P. Ward ${}^{\textrm{\scriptsize 32}}$ , D.R. Wardrope ${}^{\textrm{\scriptsize 95}}$ , N. Warrack ${}^{\textrm{\scriptsize 57}}$ , A.T. Watson ${}^{\textrm{\scriptsize 21}}$ , M.F. Watson ${}^{\textrm{\scriptsize 21}}$ , G. Watts ${}^{\textrm{\scriptsize 147}}$ , B.M. Waugh ${}^{\textrm{\scriptsize 95}}$ , A.F. Webb ${}^{\textrm{\scriptsize 11}}$ , C. Weber ${}^{\textrm{\scriptsize 29}}$ , M.S. Weber ${}^{\textrm{\scriptsize 20}}$ , S.A. Weber ${}^{\textrm{\scriptsize 34}}$ , S.M. Weber ${}^{\textrm{\scriptsize 61a}}$ , A.R. Weidberg ${}^{\textrm{\scriptsize 134}}$ , J. Weingarten ${}^{\textrm{\scriptsize 47}}$ , M. Weirich ${}^{\textrm{\scriptsize 100}}$ , C. Weiser ${}^{\textrm{\scriptsize 52}}$ , P.S. Wells ${}^{\textrm{\scriptsize 36}}$ , T. Wenaus ${}^{\textrm{\scriptsize 29}}$ , B. Wendland ${}^{\textrm{\scriptsize 47}}$ , T. Wengler ${}^{\textrm{\scriptsize 36}}$ , S. Wenig ${}^{\textrm{\scriptsize 36}}$ , N. Wermes ${}^{\textrm{\scriptsize 24}}$ , M. Wessels ${}^{\textrm{\scriptsize 61a}}$ , T.D. Weston ${}^{\textrm{\scriptsize 20}}$ , K. Whalen ${}^{\textrm{\scriptsize 131}}$ , N.L. Whallon ${}^{\textrm{\scriptsize 147}}$ , A.M. Wharton ${}^{\textrm{\scriptsize 90}}$ , A.S. White ${}^{\textrm{\scriptsize 106}}$ , A. White ${}^{\textrm{\scriptsize 8}}$ , M.J. White ${}^{\textrm{\scriptsize 1}}$ , D. Whiteson ${}^{\textrm{\scriptsize 170}}$ , B.W. Whitmore ${}^{\textrm{\scriptsize 90}}$ , W. Wiedenmann ${}^{\textrm{\scriptsize 180}}$ , C. Wiel ${}^{\textrm{\scriptsize 48}}$ , M. Wielers ${}^{\textrm{\scriptsize 143}}$ , N. Wieseotte ${}^{\textrm{\scriptsize 100}}$ , C. Wiglesworth ${}^{\textrm{\scriptsize 40}}$ , L.A.M. Wiik-Fuchs ${}^{\textrm{\scriptsize 52}}$ , H.G. Wilkens ${}^{\textrm{\scriptsize 36}}$ , L.J. Wilkins ${}^{\textrm{\scriptsize 94}}$ , H.H. Williams ${}^{\textrm{\scriptsize 136}}$ , S. Williams ${}^{\textrm{\scriptsize 32}}$ , S. Willocq ${}^{\textrm{\scriptsize 103}}$ , P.J. Windischhofer ${}^{\textrm{\scriptsize 134}}$ , I. Wingerter-Seez ${}^{\textrm{\scriptsize 5}}$ , E. Winkels ${}^{\textrm{\scriptsize 155}}$ , F. Winklmeier ${}^{\textrm{\scriptsize 131}}$ , B.T. Winter ${}^{\textrm{\scriptsize 52}}$ , M. Wittgen ${}^{\textrm{\scriptsize 152}}$ , M. Wobisch ${}^{\textrm{\scriptsize 96}}$ , A. Wolf ${}^{\textrm{\scriptsize 100}}$ , R. Wölker ${}^{\textrm{\scriptsize 134}}$ , J. Wollrath ${}^{\textrm{\scriptsize 52}}$ , M.W. Wolter ${}^{\textrm{\scriptsize 85}}$ , H. Wolters ${}^{\textrm{\scriptsize 139a,139c}}$ , V.W.S. Wong ${}^{\textrm{\scriptsize 174}}$ , N.L. Woods ${}^{\textrm{\scriptsize 145}}$ , S.D. Worm ${}^{\textrm{\scriptsize 46}}$ , B.K. Wosiek ${}^{\textrm{\scriptsize 85}}$ , K.W. Woźniak ${}^{\textrm{\scriptsize 85}}$ , K. Wraight ${}^{\textrm{\scriptsize 57}}$ , S.L. Wu ${}^{\textrm{\scriptsize 180}}$ , X. Wu ${}^{\textrm{\scriptsize 54}}$ , Y. Wu ${}^{\textrm{\scriptsize 60a}}$ , J. Wuerzinger ${}^{\textrm{\scriptsize 134}}$ , T.R. Wyatt ${}^{\textrm{\scriptsize 101}}$ , B.M. Wynne ${}^{\textrm{\scriptsize 50}}$ , S. Xella ${}^{\textrm{\scriptsize 40}}$ , L. Xia ${}^{\textrm{\scriptsize 177}}$ , J. Xiang ${}^{\textrm{\scriptsize 63c}}$ , X. Xiao ${}^{\textrm{\scriptsize 106}}$ , X. Xie ${}^{\textrm{\scriptsize 60a}}$ , I. Xiotidis ${}^{\textrm{\scriptsize 155}}$ , D. Xu ${}^{\textrm{\scriptsize 15a}}$ , H. Xu ${}^{\textrm{\scriptsize 60a}}$ , H. Xu ${}^{\textrm{\scriptsize 60a}}$ , L. Xu ${}^{\textrm{\scriptsize 29}}$ , T. Xu ${}^{\textrm{\scriptsize 144}}$ , W. Xu ${}^{\textrm{\scriptsize 106}}$ , Z. Xu ${}^{\textrm{\scriptsize 60b}}$ , Z. Xu ${}^{\textrm{\scriptsize 152}}$ , B. Yabsley ${}^{\textrm{\scriptsize 156}}$ , S. Yacoob ${}^{\textrm{\scriptsize 33a}}$ , K. Yajima ${}^{\textrm{\scriptsize 132}}$ , D.P. Yallup ${}^{\textrm{\scriptsize 95}}$ , N. Yamaguchi ${}^{\textrm{\scriptsize 88}}$ , Y. Yamaguchi ${}^{\textrm{\scriptsize 164}}$ , A. Yamamoto ${}^{\textrm{\scriptsize 82}}$ , M. Yamatani ${}^{\textrm{\scriptsize 162}}$ , T. Yamazaki ${}^{\textrm{\scriptsize 162}}$ , Y. Yamazaki ${}^{\textrm{\scriptsize 83}}$ , J. Yan ${}^{\textrm{\scriptsize 60c}}$ , Z. Yan ${}^{\textrm{\scriptsize 25}}$ , H.J. Yang ${}^{\textrm{\scriptsize 60c,60d}}$ , H.T. Yang ${}^{\textrm{\scriptsize 18}}$ , S. Yang ${}^{\textrm{\scriptsize 60a}}$ , T. Yang ${}^{\textrm{\scriptsize 63c}}$ , X. Yang ${}^{\textrm{\scriptsize 60b,58}}$ , Y. Yang ${}^{\textrm{\scriptsize 162}}$ , Z. Yang ${}^{\textrm{\scriptsize 60a}}$ , W-M. Yao ${}^{\textrm{\scriptsize 18}}$ , Y.C. Yap ${}^{\textrm{\scriptsize 46}}$ , Y. Yasu ${}^{\textrm{\scriptsize 82}}$ , E. Yatsenko ${}^{\textrm{\scriptsize 60c}}$ , H. Ye ${}^{\textrm{\scriptsize 15c}}$ , J. Ye ${}^{\textrm{\scriptsize 42}}$ , S. Ye ${}^{\textrm{\scriptsize 29}}$ , I. Yeletskikh ${}^{\textrm{\scriptsize 80}}$ , M.R. Yexley ${}^{\textrm{\scriptsize 90}}$ , E. Yigitbasi ${}^{\textrm{\scriptsize 25}}$ , P. Yin ${}^{\textrm{\scriptsize 39}}$ , K. Yorita ${}^{\textrm{\scriptsize 178}}$ , K. Yoshihara ${}^{\textrm{\scriptsize 79}}$ , C.J.S. Young ${}^{\textrm{\scriptsize 36}}$ , C. Young ${}^{\textrm{\scriptsize 152}}$ , J. Yu ${}^{\textrm{\scriptsize 79}}$ , R. Yuan ${}^{\textrm{\scriptsize 60b,h}}$ , X. Yue ${}^{\textrm{\scriptsize 61a}}$ , M. Zaazoua ${}^{\textrm{\scriptsize 35e}}$ , B. Zabinski ${}^{\textrm{\scriptsize 85}}$ , G. Zacharis ${}^{\textrm{\scriptsize 10}}$ , E. Zaffaroni ${}^{\textrm{\scriptsize 54}}$ , J. Zahreddine ${}^{\textrm{\scriptsize 135}}$ , A.M. Zaitsev ${}^{\textrm{\scriptsize 123,ag}}$ , T. Zakareishvili ${}^{\textrm{\scriptsize 158b}}$ , N. Zakharchuk ${}^{\textrm{\scriptsize 34}}$ , S. Zambito ${}^{\textrm{\scriptsize 36}}$ , D. Zanzi ${}^{\textrm{\scriptsize 36}}$ , D.R. Zaripovas ${}^{\textrm{\scriptsize 57}}$ , S.V. Zeißner ${}^{\textrm{\scriptsize 47}}$ , C. Zeitnitz ${}^{\textrm{\scriptsize 181}}$ , G. Zemaityte ${}^{\textrm{\scriptsize 134}}$ , J.C. Zeng ${}^{\textrm{\scriptsize 172}}$ , O. Zenin ${}^{\textrm{\scriptsize 123}}$ , T. Ženiš ${}^{\textrm{\scriptsize 28a}}$ , D. Zerwas ${}^{\textrm{\scriptsize 65}}$ , M. Zgubič ${}^{\textrm{\scriptsize 134}}$ , B. Zhang ${}^{\textrm{\scriptsize 15c}}$ , D.F. Zhang ${}^{\textrm{\scriptsize 15b}}$ , G. Zhang ${}^{\textrm{\scriptsize 15b}}$ , J. Zhang ${}^{\textrm{\scriptsize 6}}$ , Kaili. Zhang ${}^{\textrm{\scriptsize 15a}}$ , L. Zhang ${}^{\textrm{\scriptsize 15c}}$ , L. Zhang ${}^{\textrm{\scriptsize 60a}}$ , M. Zhang ${}^{\textrm{\scriptsize 172}}$ , R. Zhang ${}^{\textrm{\scriptsize 180}}$ , S. Zhang ${}^{\textrm{\scriptsize 106}}$ , X. Zhang ${}^{\textrm{\scriptsize 60c}}$ , X. Zhang ${}^{\textrm{\scriptsize 60b}}$ , Y. Zhang ${}^{\textrm{\scriptsize 15a,15d}}$ , Z. Zhang ${}^{\textrm{\scriptsize 63a}}$ , Z. Zhang ${}^{\textrm{\scriptsize 65}}$ , P. Zhao ${}^{\textrm{\scriptsize 49}}$ , Z. Zhao ${}^{\textrm{\scriptsize 60a}}$ , A. Zhemchugov ${}^{\textrm{\scriptsize 80}}$ , Z. Zheng ${}^{\textrm{\scriptsize 106}}$ , D. Zhong ${}^{\textrm{\scriptsize 172}}$ , B. Zhou ${}^{\textrm{\scriptsize 106}}$ , C. Zhou ${}^{\textrm{\scriptsize 180}}$ , H. Zhou ${}^{\textrm{\scriptsize 7}}$ , M.S. Zhou ${}^{\textrm{\scriptsize 15a,15d}}$ , M. Zhou ${}^{\textrm{\scriptsize 154}}$ , N. Zhou ${}^{\textrm{\scriptsize 60c}}$ , Y. Zhou ${}^{\textrm{\scriptsize 7}}$ , C.G. Zhu ${}^{\textrm{\scriptsize 60b}}$ , C. Zhu ${}^{\textrm{\scriptsize 15a,15d}}$ , H.L. Zhu ${}^{\textrm{\scriptsize 60a}}$ , H. Zhu ${}^{\textrm{\scriptsize 15a}}$ , J. Zhu ${}^{\textrm{\scriptsize 106}}$ , Y. Zhu ${}^{\textrm{\scriptsize 60a}}$ , X. Zhuang ${}^{\textrm{\scriptsize 15a}}$ , K. Zhukov ${}^{\textrm{\scriptsize 111}}$ , V. Zhulanov ${}^{\textrm{\scriptsize 122b,122a}}$ , D. Zieminska ${}^{\textrm{\scriptsize 66}}$ , N.I. Zimine ${}^{\textrm{\scriptsize 80}}$ , S. Zimmermann ${}^{\textrm{\scriptsize 52}}$ , Z. Zinonos ${}^{\textrm{\scriptsize 115}}$ , M. Ziolkowski ${}^{\textrm{\scriptsize 150}}$ , L. Živković ${}^{\textrm{\scriptsize 16}}$ , G. Zobernig ${}^{\textrm{\scriptsize 180}}$ , A. Zoccoli ${}^{\textrm{\scriptsize 23b,23a}}$ , K. Zoch ${}^{\textrm{\scriptsize 53}}$ , T.G. Zorbas ${}^{\textrm{\scriptsize 148}}$ , R. Zou ${}^{\textrm{\scriptsize 37}}$ , L. Zwalinski ${}^{\textrm{\scriptsize 36}}$ .

¹Department of Physics, University of Adelaide, Adelaide; Australia.

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

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

⁴^(a)Department of Physics, Ankara University, Ankara;^(b)Istanbul Aydin University, Application and Research Center for Advanced Studies, Istanbul;^(c)Division of Physics, TOBB University of Economics and Technology, Ankara; Turkey.

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

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

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

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

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

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

¹¹Department of Physics, University of Texas at Austin, Austin TX; United States of America.

¹²^(a)Bahcesehir University, Faculty of Engineering and Natural Sciences, Istanbul;^(b)Istanbul Bilgi University, Faculty of Engineering and Natural Sciences, Istanbul;^(c)Department of Physics, Bogazici University, Istanbul;^(d)Department of Physics Engineering, Gaziantep University, Gaziantep; Turkey.

¹³Institute of Physics, Azerbaijan Academy of Sciences, Baku; Azerbaijan.

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

¹⁵^(a)Institute of High Energy Physics, Chinese Academy of Sciences, Beijing;^(b)Physics Department, Tsinghua University, Beijing;^(c)Department of Physics, Nanjing University, Nanjing;^(d)University of Chinese Academy of Science (UCAS), Beijing; China.

¹⁶Institute of Physics, University of Belgrade, Belgrade; Serbia.

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

¹⁸Physics Division, Lawrence Berkeley National Laboratory and University of California, Berkeley CA; United States of America.

¹⁹Institut für Physik, Humboldt Universität zu Berlin, Berlin; Germany.

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

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

²²^(a)Facultad de Ciencias y Centro de Investigaciónes, Universidad Antonio Nariño, Bogotá;^(b)Departamento de Física, Universidad Nacional de Colombia, Bogotá, Colombia; Colombia.

²³^(a)INFN Bologna and Universita’ di Bologna, Dipartimento di Fisica;^(b)INFN Sezione di Bologna; Italy.

²⁴Physikalisches Institut, Universität Bonn, Bonn; Germany.

²⁵Department of Physics, Boston University, Boston MA; United States of America.

²⁶Department of Physics, Brandeis University, Waltham MA; United States of America.

²⁷^(a)Transilvania University of Brasov, Brasov;^(b)Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest;^(c)Department of Physics, Alexandru Ioan Cuza University of Iasi, Iasi;^(d)National Institute for Research and Development of Isotopic and Molecular Technologies, Physics Department, Cluj-Napoca;^(e)University Politehnica Bucharest, Bucharest;^(f)West University in Timisoara, Timisoara; Romania.

²⁸^(a)Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava;^(b)Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice; Slovak Republic.

²⁹Physics Department, Brookhaven National Laboratory, Upton NY; United States of America.

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

³¹California State University, CA; United States of America.

³²Cavendish Laboratory, University of Cambridge, Cambridge; United Kingdom.

³³^(a)Department of Physics, University of Cape Town, Cape Town;^(b)iThemba Labs, Western Cape;^(c)Department of Mechanical Engineering Science, University of Johannesburg, Johannesburg;^(d)University of South Africa, Department of Physics, Pretoria;^(e)School of Physics, University of the Witwatersrand, Johannesburg; South Africa.

³⁴Department of Physics, Carleton University, Ottawa ON; Canada.

³⁵^(a)Faculté des Sciences Ain Chock, Réseau Universitaire de Physique des Hautes Energies - Université Hassan II, Casablanca;^(b)Faculté des Sciences, Université Ibn-Tofail, Kénitra;^(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, Rabat; Morocco.

³⁶CERN, Geneva; Switzerland.

³⁷Enrico Fermi Institute, University of Chicago, Chicago IL; United States of America.

³⁸LPC, Université Clermont Auvergne, CNRS/IN2P3, Clermont-Ferrand; France.

³⁹Nevis Laboratory, Columbia University, Irvington NY; United States of America.

⁴⁰Niels Bohr Institute, University of Copenhagen, Copenhagen; Denmark.

⁴¹^(a)Dipartimento di Fisica, Università della Calabria, Rende;^(b)INFN Gruppo Collegato di Cosenza, Laboratori Nazionali di Frascati; Italy.

⁴²Physics Department, Southern Methodist University, Dallas TX; United States of America.

⁴³Physics Department, University of Texas at Dallas, Richardson TX; United States of America.

⁴⁴National Centre for Scientific Research ”Demokritos”, Agia Paraskevi; Greece.

⁴⁵^(a)Department of Physics, Stockholm University;^(b)Oskar Klein Centre, Stockholm; Sweden.

⁴⁶Deutsches Elektronen-Synchrotron DESY, Hamburg and Zeuthen; Germany.

⁴⁷Lehrstuhl für Experimentelle Physik IV, Technische Universität Dortmund, Dortmund; Germany.

⁴⁸Institut für Kern- und Teilchenphysik, Technische Universität Dresden, Dresden; Germany.

⁴⁹Department of Physics, Duke University, Durham NC; United States of America.

⁵⁰SUPA - School of Physics and Astronomy, University of Edinburgh, Edinburgh; United Kingdom.

⁵¹INFN e Laboratori Nazionali di Frascati, Frascati; Italy.

⁵²Physikalisches Institut, Albert-Ludwigs-Universität Freiburg, Freiburg; Germany.

⁵³II. Physikalisches Institut, Georg-August-Universität Göttingen, Göttingen; Germany.

⁵⁴Département de Physique Nucléaire et Corpusculaire, Université de Genève, Genève; Switzerland.

⁵⁵^(a)Dipartimento di Fisica, Università di Genova, Genova;^(b)INFN Sezione di Genova; Italy.

⁵⁶II. Physikalisches Institut, Justus-Liebig-Universität Giessen, Giessen; Germany.

⁵⁷SUPA - School of Physics and Astronomy, University of Glasgow, Glasgow; United Kingdom.

⁵⁸LPSC, Université Grenoble Alpes, CNRS/IN2P3, Grenoble INP, Grenoble; France.

⁵⁹Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge MA; United States of America.

⁶⁰^(a)Department of Modern Physics and State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei;^(b)Institute of Frontier and Interdisciplinary Science and Key Laboratory of Particle Physics and Particle Irradiation (MOE), Shandong University, Qingdao;^(c)School of Physics and Astronomy, Shanghai Jiao Tong University, KLPPAC-MoE, SKLPPC, Shanghai;^(d)Tsung-Dao Lee Institute, Shanghai; China.

⁶¹^(a)Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg;^(b)Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg; Germany.

⁶²Faculty of Applied Information Science, Hiroshima Institute of Technology, Hiroshima; Japan.

⁶³^(a)Department of Physics, Chinese University of Hong Kong, Shatin, N.T., Hong Kong;^(b)Department of Physics, University of Hong Kong, Hong Kong;^(c)Department of Physics and Institute for Advanced Study, Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong; China.

⁶⁴Department of Physics, National Tsing Hua University, Hsinchu; Taiwan.

⁶⁵IJCLab, Université Paris-Saclay, CNRS/IN2P3, 91405, Orsay; France.

⁶⁶Department of Physics, Indiana University, Bloomington IN; United States of America.

⁶⁷^(a)INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine;^(b)ICTP, Trieste;^(c)Dipartimento Politecnico di Ingegneria e Architettura, Università di Udine, Udine; Italy.

⁶⁸^(a)INFN Sezione di Lecce;^(b)Dipartimento di Matematica e Fisica, Università del Salento, Lecce; Italy.

⁶⁹^(a)INFN Sezione di Milano;^(b)Dipartimento di Fisica, Università di Milano, Milano; Italy.

⁷⁰^(a)INFN Sezione di Napoli;^(b)Dipartimento di Fisica, Università di Napoli, Napoli; Italy.

⁷¹^(a)INFN Sezione di Pavia;^(b)Dipartimento di Fisica, Università di Pavia, Pavia; Italy.

⁷²^(a)INFN Sezione di Pisa;^(b)Dipartimento di Fisica E. Fermi, Università di Pisa, Pisa; Italy.

⁷³^(a)INFN Sezione di Roma;^(b)Dipartimento di Fisica, Sapienza Università di Roma, Roma; Italy.

⁷⁴^(a)INFN Sezione di Roma Tor Vergata;^(b)Dipartimento di Fisica, Università di Roma Tor Vergata, Roma; Italy.

⁷⁵^(a)INFN Sezione di Roma Tre;^(b)Dipartimento di Matematica e Fisica, Università Roma Tre, Roma; Italy.

⁷⁶^(a)INFN-TIFPA;^(b)Università degli Studi di Trento, Trento; Italy.

⁷⁷Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität, Innsbruck; Austria.

⁷⁸University of Iowa, Iowa City IA; United States of America.

⁷⁹Department of Physics and Astronomy, Iowa State University, Ames IA; United States of America.

⁸⁰Joint Institute for Nuclear Research, Dubna; Russia.

⁸¹^(a)Departamento de Engenharia Elétrica, Universidade Federal de Juiz de Fora (UFJF), Juiz de Fora;^(b)Universidade Federal do Rio De Janeiro COPPE/EE/IF, Rio de Janeiro;^(c)Universidade Federal de São João del Rei (UFSJ), São João del Rei;^(d)Instituto de Física, Universidade de São Paulo, São Paulo; Brazil.

⁸²KEK, High Energy Accelerator Research Organization, Tsukuba; Japan.

⁸³Graduate School of Science, Kobe University, Kobe; Japan.

⁸⁴^(a)AGH University of Science and Technology, Faculty of Physics and Applied Computer Science, Krakow;^(b)Marian Smoluchowski Institute of Physics, Jagiellonian University, Krakow; Poland.

⁸⁵Institute of Nuclear Physics Polish Academy of Sciences, Krakow; Poland.

⁸⁶Faculty of Science, Kyoto University, Kyoto; Japan.

⁸⁷Kyoto University of Education, Kyoto; Japan.

⁸⁸Research Center for Advanced Particle Physics and Department of Physics, Kyushu University, Fukuoka ; Japan.

⁸⁹Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata; Argentina.

⁹⁰Physics Department, Lancaster University, Lancaster; United Kingdom.

⁹¹Oliver Lodge Laboratory, University of Liverpool, Liverpool; United Kingdom.

⁹²Department of Experimental Particle Physics, Jožef Stefan Institute and Department of Physics, University of Ljubljana, Ljubljana; Slovenia.

⁹³School of Physics and Astronomy, Queen Mary University of London, London; United Kingdom.

⁹⁴Department of Physics, Royal Holloway University of London, Egham; United Kingdom.

⁹⁵Department of Physics and Astronomy, University College London, London; United Kingdom.

⁹⁶Louisiana Tech University, Ruston LA; United States of America.

⁹⁷Fysiska institutionen, Lunds universitet, Lund; Sweden.

⁹⁸Centre de Calcul de l’Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Villeurbanne; France.

⁹⁹Departamento de Física Teorica C-15 and CIAFF, Universidad Autónoma de Madrid, Madrid; Spain.

¹⁰⁰Institut für Physik, Universität Mainz, Mainz; Germany.

¹⁰¹School of Physics and Astronomy, University of Manchester, Manchester; United Kingdom.

¹⁰²CPPM, Aix-Marseille Université, CNRS/IN2P3, Marseille; France.

¹⁰³Department of Physics, University of Massachusetts, Amherst MA; United States of America.

¹⁰⁴Department of Physics, McGill University, Montreal QC; Canada.

¹⁰⁵School of Physics, University of Melbourne, Victoria; Australia.

¹⁰⁶Department of Physics, University of Michigan, Ann Arbor MI; United States of America.

¹⁰⁷Department of Physics and Astronomy, Michigan State University, East Lansing MI; United States of America.

¹⁰⁸B.I. Stepanov Institute of Physics, National Academy of Sciences of Belarus, Minsk; Belarus.

¹⁰⁹Research Institute for Nuclear Problems of Byelorussian State University, Minsk; Belarus.

¹¹⁰Group of Particle Physics, University of Montreal, Montreal QC; Canada.

¹¹¹P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow; Russia.

¹¹²National Research Nuclear University MEPhI, Moscow; Russia.

¹¹³D.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University, Moscow; Russia.

¹¹⁴Fakultät für Physik, Ludwig-Maximilians-Universität München, München; Germany.

¹¹⁵Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), München; Germany.

¹¹⁶Nagasaki Institute of Applied Science, Nagasaki; Japan.

¹¹⁷Graduate School of Science and Kobayashi-Maskawa Institute, Nagoya University, Nagoya; Japan.

¹¹⁸Department of Physics and Astronomy, University of New Mexico, Albuquerque NM; United States of America.

¹¹⁹Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen/Nikhef, Nijmegen; Netherlands.

¹²⁰Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam; Netherlands.

¹²¹Department of Physics, Northern Illinois University, DeKalb IL; United States of America.

¹²²^(a)Budker Institute of Nuclear Physics and NSU, SB RAS, Novosibirsk;^(b)Novosibirsk State University Novosibirsk; Russia.

¹²³Institute for High Energy Physics of the National Research Centre Kurchatov Institute, Protvino; Russia.

¹²⁴Institute for Theoretical and Experimental Physics named by A.I. Alikhanov of National Research Centre ”Kurchatov Institute”, Moscow; Russia.

¹²⁵Department of Physics, New York University, New York NY; United States of America.

¹²⁶Ochanomizu University, Otsuka, Bunkyo-ku, Tokyo; Japan.

¹²⁷Ohio State University, Columbus OH; United States of America.

¹²⁸Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman OK; United States of America.

¹²⁹Department of Physics, Oklahoma State University, Stillwater OK; United States of America.

¹³⁰Palacký University, RCPTM, Joint Laboratory of Optics, Olomouc; Czech Republic.

¹³¹Institute for Fundamental Science, University of Oregon, Eugene, OR; United States of America.

¹³²Graduate School of Science, Osaka University, Osaka; Japan.

¹³³Department of Physics, University of Oslo, Oslo; Norway.

¹³⁴Department of Physics, Oxford University, Oxford; United Kingdom.

¹³⁵LPNHE, Sorbonne Université, Université de Paris, CNRS/IN2P3, Paris; France.

¹³⁶Department of Physics, University of Pennsylvania, Philadelphia PA; United States of America.

¹³⁷Konstantinov Nuclear Physics Institute of National Research Centre ”Kurchatov Institute”, PNPI, St. Petersburg; Russia.

¹³⁸Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh PA; United States of America.

¹³⁹^(a)Laboratório de Instrumentação e Física Experimental de Partículas - LIP, Lisboa;^(b)Departamento de Física, Faculdade de Ciências, Universidade de Lisboa, Lisboa;^(c)Departamento de Física, Universidade de Coimbra, Coimbra;^(d)Centro de Física Nuclear da Universidade de Lisboa, Lisboa;^(e)Departamento de Física, Universidade do Minho, Braga;^(f)Departamento de Física Teórica y del Cosmos, Universidad de Granada, Granada (Spain);^(g)Dep Física and CEFITEC of Faculdade de Ciências e Tecnologia, Universidade Nova de Lisboa, Caparica;^(h)Instituto Superior Técnico, Universidade de Lisboa, Lisboa; Portugal.

¹⁴⁰Institute of Physics of the Czech Academy of Sciences, Prague; Czech Republic.

¹⁴¹Czech Technical University in Prague, Prague; Czech Republic.

¹⁴²Charles University, Faculty of Mathematics and Physics, Prague; Czech Republic.

¹⁴³Particle Physics Department, Rutherford Appleton Laboratory, Didcot; United Kingdom.

¹⁴⁴IRFU, CEA, Université Paris-Saclay, Gif-sur-Yvette; France.

¹⁴⁵Santa Cruz Institute for Particle Physics, University of California Santa Cruz, Santa Cruz CA; United States of America.

¹⁴⁶^(a)Departamento de Física, Pontificia Universidad Católica de Chile, Santiago;^(b)Universidad Andres Bello, Department of Physics, Santiago;^(c)Instituto de Alta Investigación, Universidad de Tarapacá;^(d)Departamento de Física, Universidad Técnica Federico Santa María, Valparaíso; Chile.

¹⁴⁷Department of Physics, University of Washington, Seattle WA; United States of America.

¹⁴⁸Department of Physics and Astronomy, University of Sheffield, Sheffield; United Kingdom.

¹⁴⁹Department of Physics, Shinshu University, Nagano; Japan.

¹⁵⁰Department Physik, Universität Siegen, Siegen; Germany.

¹⁵¹Department of Physics, Simon Fraser University, Burnaby BC; Canada.

¹⁵²SLAC National Accelerator Laboratory, Stanford CA; United States of America.

¹⁵³Physics Department, Royal Institute of Technology, Stockholm; Sweden.

¹⁵⁴Departments of Physics and Astronomy, Stony Brook University, Stony Brook NY; United States of America.

¹⁵⁵Department of Physics and Astronomy, University of Sussex, Brighton; United Kingdom.

¹⁵⁶School of Physics, University of Sydney, Sydney; Australia.

¹⁵⁷Institute of Physics, Academia Sinica, Taipei; Taiwan.

¹⁵⁸^(a)E. Andronikashvili Institute of Physics, Iv. Javakhishvili Tbilisi State University, Tbilisi;^(b)High Energy Physics Institute, Tbilisi State University, Tbilisi; Georgia.

¹⁵⁹Department of Physics, Technion, Israel Institute of Technology, Haifa; Israel.

¹⁶⁰Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv; Israel.

¹⁶¹Department of Physics, Aristotle University of Thessaloniki, Thessaloniki; Greece.

¹⁶²International Center for Elementary Particle Physics and Department of Physics, University of Tokyo, Tokyo; Japan.

¹⁶³Graduate School of Science and Technology, Tokyo Metropolitan University, Tokyo; Japan.

¹⁶⁴Department of Physics, Tokyo Institute of Technology, Tokyo; Japan.

¹⁶⁵Tomsk State University, Tomsk; Russia.

¹⁶⁶Department of Physics, University of Toronto, Toronto ON; Canada.

¹⁶⁷^(a)TRIUMF, Vancouver BC;^(b)Department of Physics and Astronomy, York University, Toronto ON; Canada.

¹⁶⁸Division of Physics and Tomonaga Center for the History of the Universe, Faculty of Pure and Applied Sciences, University of Tsukuba, Tsukuba; Japan.

¹⁶⁹Department of Physics and Astronomy, Tufts University, Medford MA; United States of America.

¹⁷⁰Department of Physics and Astronomy, University of California Irvine, Irvine CA; United States of America.

¹⁷¹Department of Physics and Astronomy, University of Uppsala, Uppsala; Sweden.

¹⁷²Department of Physics, University of Illinois, Urbana IL; United States of America.

¹⁷³Instituto de Física Corpuscular (IFIC), Centro Mixto Universidad de Valencia - CSIC, Valencia; Spain.

¹⁷⁴Department of Physics, University of British Columbia, Vancouver BC; Canada.

¹⁷⁵Department of Physics and Astronomy, University of Victoria, Victoria BC; Canada.

¹⁷⁶Fakultät für Physik und Astronomie, Julius-Maximilians-Universität Würzburg, Würzburg; Germany.

¹⁷⁷Department of Physics, University of Warwick, Coventry; United Kingdom.

¹⁷⁸Waseda University, Tokyo; Japan.

¹⁷⁹Department of Particle Physics, Weizmann Institute of Science, Rehovot; Israel.

¹⁸⁰Department of Physics, University of Wisconsin, Madison WI; United States of America.

¹⁸¹Fakultät für Mathematik und Naturwissenschaften, Fachgruppe Physik, Bergische Universität Wuppertal, Wuppertal; Germany.

¹⁸²Department of Physics, Yale University, New Haven CT; United States of America.

^a Also at Borough of Manhattan Community College, City University of New York, New York NY; United States of America.

^b Also at Centro Studi e Ricerche Enrico Fermi; Italy.

^c Also at CERN, Geneva; Switzerland.

^d Also at CPPM, Aix-Marseille Université, CNRS/IN2P3, Marseille; France.

^e Also at Département de Physique Nucléaire et Corpusculaire, Université de Genève, Genève; Switzerland.

^f Also at Departament de Fisica de la Universitat Autonoma de Barcelona, Barcelona; Spain.

^g Also at Department of Financial and Management Engineering, University of the Aegean, Chios; Greece.

^h Also at Department of Physics and Astronomy, Michigan State University, East Lansing MI; United States of America.

ⁱ Also at Department of Physics and Astronomy, University of Louisville, Louisville, KY; United States of America.

^j Also at Department of Physics, Ben Gurion University of the Negev, Beer Sheva; Israel.

^k Also at Department of Physics, California State University, East Bay; United States of America.

^l Also at Department of Physics, California State University, Fresno; United States of America.

^m Also at Department of Physics, California State University, Sacramento; United States of America.

ⁿ Also at Department of Physics, King’s College London, London; United Kingdom.

^o Also at Department of Physics, St. Petersburg State Polytechnical University, St. Petersburg; Russia.

^p Also at Department of Physics, University of Fribourg, Fribourg; Switzerland.

^q Also at Dipartimento di Matematica, Informatica e Fisica, Università di Udine, Udine; Italy.

^r Also at Faculty of Physics, M.V. Lomonosov Moscow State University, Moscow; Russia.

^s Also at Giresun University, Faculty of Engineering, Giresun; Turkey.

^t Also at Graduate School of Science, Osaka University, Osaka; Japan.

^u Also at Hellenic Open University, Patras; Greece.

^v Also at IJCLab, Université Paris-Saclay, CNRS/IN2P3, 91405, Orsay; France.

^w Also at Institucio Catalana de Recerca i Estudis Avancats, ICREA, Barcelona; Spain.

^x Also at Institut für Experimentalphysik, Universität Hamburg, Hamburg; Germany.

^y Also at Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen/Nikhef, Nijmegen; Netherlands.

^z Also at Institute for Nuclear Research and Nuclear Energy (INRNE) of the Bulgarian Academy of Sciences, Sofia; Bulgaria.

^aa Also at Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Budapest; Hungary.

^ab Also at Institute of Particle Physics (IPP); Canada.

^ac Also at Institute of Physics, Azerbaijan Academy of Sciences, Baku; Azerbaijan.

^ad Also at Instituto de Fisica Teorica, IFT-UAM/CSIC, Madrid; Spain.

^ae Also at Joint Institute for Nuclear Research, Dubna; Russia.

^af Also at Louisiana Tech University, Ruston LA; United States of America.

^ag Also at Moscow Institute of Physics and Technology State University, Dolgoprudny; Russia.

^ah Also at National Research Nuclear University MEPhI, Moscow; Russia.

^ai Also at Physics Department, An-Najah National University, Nablus; Palestine.

^aj Also at Physikalisches Institut, Albert-Ludwigs-Universität Freiburg, Freiburg; Germany.

^ak Also at The City College of New York, New York NY; United States of America.

^al Also at TRIUMF, Vancouver BC; Canada.

^am Also at Universita di Napoli Parthenope, Napoli; Italy.

^an Also at University of Chinese Academy of Sciences (UCAS), Beijing; China.

^∗ Deceased