EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN)

arXiv:submit/0524428 [hep-ex] 31 Jul 2012

Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC

The CMS Collaboration

Abstract

Results are presented from searches for the standard model Higgs boson in proton

proton collisions at s = 7 and 8 TeV in the CMS experiment at the LHC, using data samples corresponding to integrated luminosities of up to 5.1 fb1 at 7 TeV and

5.3 fb1 at 8 TeV. The search is performed in five decay modes: γγ, ZZ, WW, τ+τ, and bb. An excess of events is observed above the expected background, a local significance of 5.0 standard deviations, at a mass near 125 GeV, signalling the production of a new particle. The expected significance for a standard model Higgs boson of that mass is 5.8 standard deviations. The excess is most significant in the two decay modes with the best mass resolution, γγ and ZZ; a fit to these signals gives a mass of

125.3 ± 0.4 (stat.) ± 0.5 (syst.) GeV. The decay to two photons indicates that the new particle is a boson with spin different from one.

This paper is dedicated to the memory of our colleagues who worked on CMS but have since passed away.

In recognition of their many contributions to the achievement of this observation.

Submitted to Physics Letters B

See Appendix A for the list of collaboration members

1 Introduction

The standard model (SM) of elementary particles has provided a remarkably accurate description of results from many accelerator and non-accelerator based experiments. The SM comprises quarks and leptons as the building blocks of matter, and describes their interactions through the exchange of force carriers: the photon for electromagnetic interactions, the W and Z gauge bosons for weak interactions, and the gluons for strong interactions. The electromagnetic and weak interactions are unified in the electroweak theory. Although the predictions of the SM have been extensively confirmed, the question of how the W and Z gauge bosons acquire mass whilst the photon remains massless is still open.

Nearly fifty years ago it was proposed [1–6] that spontaneous symmetry breaking in gauge theories could be achieved through the introduction of a complex scalar doublet field. Ap plying this proposal to the electroweak theory [7–9] leads to the generation of the W and Z masses, and to the prediction of the existence of the SM Higgs boson (H). The scalar field also gives mass to the fundamental fermions through the Yukawa interaction. The mass mH of the SM Higgs boson is not predicted by theory. However, general considerations [10–13] suggest that mH should be smaller than 1 TeV, while precision electroweak measurements imply that mH < 152 GeV at 95% confidence level (CL) [14]. Over the past twenty years, direct searches for the Higgs boson have been carried out at the LEP collider, leading to a lower bound of mH > 114.4 GeV at 95% CL [15], and at the Tevatron proton-antiproton collider, excluding the mass range 162–166 GeV at 95% CL [16].

The discovery or exclusion of the SM Higgs boson is one of the primary scientific goals of the Large Hadron Collider (LHC). Previous direct searches at the LHC were based on data from proton-proton collisions corresponding to an integrated luminosity of 5 fb1 collected at

a centre-of-mass energy s = 7 TeV. The CMS experiment excluded at 95% CL a range of masses from 127 to 600 GeV [17]. The ATLAS experiment excluded at 95% CL the ranges 111.4– 116.6, 119.4–122.1 and 129.2–541 GeV [18]. Within the remaining allowed mass region, an excess of events near 125 GeV was reported by both experiments. In 2012 the proton-proton centre-ofmass energy was increased to 8 TeV and by the end of June an additional integrated luminosity of more than 5 fb1 had been recorded by each of these experiments, thereby enhancing significantly the sensitivity of the search for the Higgs boson.

This paper reports the results of a search for the SM Higgs boson using samples collected by

the CMS experiment, comprising data recorded at s = 7 and 8 TeV. The search is performed in five decay modes, H γγ, ZZ, WW, τ+τ, and bb, in the low-mass range from 110 up to 160 GeV. In this mass range the Higgs boson production cross section is predicted to range

from 21 (27) to 12 (15) pb at s = 7 (8) TeV [19]. The natural width of the SM Higgs boson in this mass range is a few MeV and the width of any observed peak would be entirely dominated by instrumental mass resolution. In what follows, f stands for electrons or muons, H τ+τis denoted as H ττ,H bb as H bb, etc. For the final states ZZ and WW in the low-mass region, one or more of the Z or W bosons is off mass shell.

With respect to the published analyses [20–24], most analyses have been re-optimized, incor porating improvements in reconstruction performance and event selection, and mitigating the more challenging conditions due to the higher LHC intensities in 2012. The new analyses presented herein, of 8 TeV samples, and of 7 TeV samples featuring modified event selection criteria, were performed in a “blind” way: the algorithms and selection procedures were formally approved and fixed before the results from data in the signal region were examined. In the previously published analyses similar but less formal procedures were followed.

Within the context of this search for the SM Higgs boson, we report the observation of an excess of events above the expected background, consistent with the production of a new particle with mass near 125 GeV. The observed local significance is 5.0 standard deviations (σ), compared with an expected significance of 5.8 σ. The evidence is strongest in the two final states with the best mass resolution, namely H γγ with a significance of 4.1 σ and H ZZ (with the Z bosons decaying to electrons or muons) with a significance of 3.2 σ. The decay to two photons indicates that the new particle is a boson with spin different from one.

2 The CMS experiment

The possibility of detection of the SM Higgs boson played a crucial role in the conceptual design of the CMS experiment as a benchmark to test the performance of the detector [25–27]. Since the SM Higgs boson mass is not predicted by theory and its production cross section and natural width vary widely over the allowed mass range, a search was envisaged over a large range of masses and in diverse decay modes: pairs of photons, Z bosons, W bosons, τ leptons, and b quarks. Planning in view of the analysis of all these channels ensured a detector capable of observing a Higgs boson over a broad mass range and able to detect most potential signals of new physics.

The central feature of the CMS apparatus [28] is a superconducting solenoid of 6 m inter nal diameter, which provides a magnetic field of 3.8 T. Within the field volume are a silicon pixel and strip tracker, a lead tungstate crystal electromagnetic calorimeter (ECAL), and a brass/scintillator hadron calorimeter (HCAL). Muons are measured in gas-ionization detectors embedded in the steel flux-return yoke. Extensive forward calorimeters complement the coverage provided by the barrel and endcap detectors.

Charged particles are tracked within the pseudorapidity range |η| < 2.5, where η = ln[tan(θ/2)], and θ is the polar angle measured from the positive z axis (along the anticlockwise beam direction). The silicon pixel tracker comprises 66 million 100 × 150 µm2 pixels, arranged in three barrel layers and two endcap disks at each end. The silicon strip tracker, organized in ten barrel layers and twelve endcap disks at each end, comprises 9.3 million strips with pitch between 80 and 180 µm, with a total silicon surface area of 198 m2. The tracker has a track-finding efficiency larger than 99% for muons with transverse momentum, pT, greater than 1 GeV, a transverse momentum resolution between 2 and 3% for charged tracks of pT 100 GeV in the central region (|η| < 1.5), and a very good b-jet-identification capability. Measurements of the impact parameters of charged tracks and secondary vertices are used to identify jets that are likely to contain the hadronisation and decay products of b quarks (“b jets”). A b-jet tagging efficiency of more than 50% is achieved with a rejection factor for light-quark jets of 200, as measured in tt events in data [29]. The dimuon mass resolution at the Υ mass, dominated by instrumental effects, is measured to be 0.6% in the barrel region [30], consistent with the design goal.

The ECAL is a fine-grained hermetic calorimeter consisting of 75 848 lead tungstate crystals, arranged in a quasi-projective geometry and distributed in a barrel region (|η| < 1.48) and two endcaps that extend up to |η| = 3.0. The front-face cross section of the crystals is 22 × 22 mm2 in the barrel region and 28.6 × 28.6 mm2 in the endcaps. Preshower detectors consisting of two planes of silicon sensors interleaved with a total of three radiation lengths of lead absorber are located in front of the endcaps. Electromagnetic showers are very narrow in lead tungstate (Moli`ere radius of 21mm), helping in particle identification and in the implementation of isolation criteria. In the central barrel region the energy resolution of electrons that do not radiate substantially in the tracker material indicates that the resolution of unconverted photons is consistent with design goals. For such photons the diphoton mass resolution is estimated to be

1.1 GeV at a mass of 125 GeV.

The HCAL barrel and endcaps are sampling calorimeters consisting of brass and scintillator plates, covering |η| < 3.0. Their thickness varies from 7 to 11 interaction lengths, depending on η; a scintillator “tail catcher” placed outside the coil of the solenoid, just in front of the innermost muon detector, extends the instrumented thickness to more than 10 interaction lengths everywhere. Iron forward calorimeters with quartz fibers, read out by photomultipliers, extend the calorimeter coverage up to |η| = 5.0.

Muons are measured in the range |η| < 2.4, with detection planes based on three technologies: drift tubes (|η| < 1.2), cathode strip chambers (0.9 < |η| < 2.4), and resistive plate chambers (|η| < 1.6). The first two technologies provide a precise position measurement and trigger whilst the third one provides precise timing information as well as a second and independent trigger. The muon system consists of four stations in the barrel and endcaps, designed to ensure robust triggering and detection of muons over a large angular range. In the barrel region each muon station consists of twelve drift-tube layers, except for the outermost station, which has eight layers. In the endcaps, each muon station consists of six detection planes. The precision of the r-φ measurement is 100 µm in the drift tubes and varies from 60 to 140 µm in the cathode strip chambers.

The CMS trigger and data acquisition systems ensure that potentially interesting events are recorded with high efficiency. The first level (L1) trigger, comprising the calorimeter, muon, and global trigger processors, uses coarse-granularity information to select the most interesting events in less than 4 µs. The detector data are pipelined to ensure negligible deadtime up to a L1 rate of 100 kHz. After L1 triggering, data are transferred from the readout electronics of all subdetectors, through the readout network, to the high-level-trigger processor farm, which operates offline-quality reconstruction algorithms to decrease the event rate to around 0.5 kHz, before data storage.

The CMS experiment employs a highly distributed computing infrastructure, with a primary Tier-0 centre at CERN, supplemented by seven Tier-1, more than 50 Tier-2, and many Tier3 centres at national laboratories and universities throughout the world. The CMS software running on this high-performance computing system executes numerous tasks, including the reconstruction and analysis of the collected data, as well as the generation and detailed detector simulation of Monte Carlo (MC) event samples.

3 Event reconstruction

The CMS “particle-flow” event description algorithm [31, 32] is used to reconstruct and identify each single particle with an optimized combination of all subdetector information. In this process, the identification of the particle (photon, electron, muon, charged hadron, neutral hadron), plays an important role in the determination of the particle momentum. The reconstructed particles are henceforth referred to as objects.

Jets are reconstructed by clustering the particle-flow objects with the anti-kT algorithm [33] using a distance parameter of 0.5. Additional selection criteria are applied to each event to remove spurious features originating from isolated noise patterns in certain HCAL regions, and from anomalous signals caused by particles depositing energy in the silicon avalanche photodiodes used in the ECAL barrel region. The average number of pp interactions per LHC bunch crossing is estimated to be about 9 and 19 in the 7 TeV (2011) and 8 TeV (2012) data sets, respectively. Energy from overlapping pp interactions (“pileup”), and from the underlying event, is subtracted using the FASTJET technique [34–36], which is based on the calculation of the η-dependent transverse momentum density, evaluated on an event-by-event basis.

The jet momentum is determined as the vector sum of all particle momenta in the jet. Jet energy corrections are derived from simulation studies and from in situ measurements using the energy balance of dijet and Z/γ +jet events [37]. These corrections are between 5% and 10% of the true momentum over the whole pT spectrum and detector acceptance. The jet momentum

e

resolution achieved is σ(pT)/pT = 85%/ pT/GeV 4% for central jets. A selection is applied to separate jets originating in the primary interaction from those due to energy deposits associated with pileup. The discrimination is based on the differences in the jet shapes, in the relative multiplicity of charged and neutral components, and in the fraction of transverse momentum carried by the hardest components. Within the tracker acceptance the jet tracks are also required to be consistent with originating at the primary vertex.

The missing transverse energy vector is taken as the negative vector sum of all particle transverse momenta, and its magnitude is referred to as Emiss. The typical missing transverse energy

T

resolution is around 0.5 ΣET GeV [38], where ΣET is the scalar sum of all particle transverse momenta in GeV.

The energy deposited in the ECAL is clustered both with general clustering algorithms [39] and with algorithms that constrain the clusters in η and φ to the shapes expected from electrons and photons with high pT [40]. These specialised algorithms are used to cluster electromagnetic showers without any hypothesis regarding whether the particle originating from the interaction point was a photon or an electron; doing this for electrons from Z ee events provides a measurement of the photon trigger, reconstruction, and identification efficiencies, as well as of the photon energy scale and resolution. The width of the reconstructed Z resonance is used to quantify the performance of the ECAL, using decays to two electrons whose energies are measured using the ECAL alone, with only their directions being determined from the tracks. In the 7 TeV data set, the dielectron mass resolution at the Z boson mass is 1.56 GeV in the barrel and

2.57 GeV in the endcaps, while in the 8 TeV sample, reconstructed with preliminary calibration constants, the corresponding values are 1.61 and 3.75 GeV. For electrons, the reconstruction combines the clusters in the ECAL and the trajectory in the silicon tracker [41]. Trajectories in the tracker volume are reconstructed using a model of electron energy loss and fitted with a Gaussian sum filter [42]. The electron momentum is determined from the combination of ECAL and tracker measurements.

Muon candidates are reconstructed with two algorithms, one in which the tracks in the silicon detector are matched to segments in the muon chambers, and another in which a combined fit is performed to the signals found in both the silicon tracker and muon systems [39]. The efficiency to reconstruct a muon of pT > 5 GeV is larger than 95%, while the probability to misidentify a hadron as a muon is below 0.1%. For pT > 200 GeV the precision of the momentum measurement improves when the silicon tracker signals are complemented with the information from the muon chambers.

Selection based on isolation of lepton and photon objects is used extensively. The scalar sum of the transverse momenta of the particles reconstructed within a distance ΔR of the object, sometimes normalised to the pT of the object, is required to not exceed some value. The distance ΔR

e

is defined as ΔR =(Δη)2 +(Δφ)2, where Δη and Δφ are the pseudorapidity and azimuthal angle differences between the particle direction and the object direction. Typical values of ΔR used are 0.3 or 0.4.

The measurement of the integrated luminosity in CMS is based on a pixel cluster counting method, which exploits the large number of silicon pixels, and hence their low occupancy in a pp collision [43]. The cross section normalisation is derived from van der Meer scans [44]. The uncertainties on the luminosity measurements are 2.2% and 4.4% for the 7 TeV and 8 TeV data sets, respectively.

4 Searches for the standard model Higgs boson

Initial phenomenological discussions of Higgs boson production and decay can be found in Refs. [45–52]. Four main mechanisms are predicted for Higgs boson production in pp colli sions: the gluon-gluon fusion mechanism, which has the largest cross section, followed in turn by vector-boson fusion (VBF), associated WH and ZH production (VH), and production in association with top quarks (ttH). The cross sections for the individual production mechanisms and the decay branching fractions, together with their uncertainties, have been computed fol lowing Refs. [53–97] and are compiled in Refs. [19, 98].

The particular set of sensitive decay modes of the SM Higgs boson depends strongly on mH. The results presented in this paper are based on five most sensitive decay modes in the low-mass region: H γγ;H ZZ followed by ZZ decays to 4f;H WW followed by decays to 2f2ν;H ττ followed by at least one leptonic τ decay; and H bb followed by b-quark fragmentation into jets. This list is presented in Table 1 and comprises the full set of decay modes and subchannels, or categories, for which both the 7 and 8 TeV data sets have been analysed. Other lower sensitivity subchannels (ttH, H bb; W/ZH, H ττ; W/ZH, H WW 2f2ν;H ZZ 2f2q) have also been studied, so far only in the 7 TeV data, and are not included here. Adding these analyses in the combination results in an improvement of

0.1 σ in the overall expected local significance at mH = 125 GeV.

Table 1: Summary of the subchannels, or categories, used in the analysis of each decay mode.

Decay Production No. of mH range Int. Lum. (fb1) mode tagging subchannels (GeV) 7 TeV 8 TeV

γγ untagged dijet (VBF) 4 1 or 2 110–150 5.1 5.3
ZZ untagged 3 110–600 5.1 5.3
WW untagged dijet (VBF) 4 1 or 2 110–600 4.9 5.1

untagged 16

ττ 110–145 4.9 5.1

dijet (VBF) 4 bb lepton, Emiss (VH) 10 110–135 5.0 5.1

T

For a given value of mH, the search sensitivity depends on the production cross section, the decay branching fraction into the chosen final state, the signal selection efficiency, the mass resolution, and the level of background from identical or similar final-state topologies.

Samples of MC events used to represent signal and background are fully simulated using GEANT 4 [99]. The simulations include pileup interactions matching the distribution of the number of such interactions observed in data. The description of the Higgs boson signal is obtained from MC simulation using, for most of the decay modes and production processes, the next-to-leading-order (NLO) matrix-element generator POWHEG [100 , 101], interfaced with PYTHIA 6.4 [102]. For the dominant gluon-gluon fusion process, the transverse momentum spectrum of the Higgs boson in the 7 TeV MC samples is reweighted to the next-to-next-toleading-logarithmic (NNLL) + NLO distribution computed with HqT [67 , 68, 103] and F EHIPRO [104 , 105], except in the H ZZ analysis, where the effect is marginal. The agreement of the pT spectrum in the simulation at 8 TeV with the NNLL + NLO distribution makes reweighting unnecessary. The improved agreement is due to a modification in the POWHEG setup recommended in Ref. [98]. The simulation of associated-production signal samples uses PYTHIA, and all signal samples for H bb are made using POWHEG interfaced to HERWIG ++ [106]. Samples used for background studies are generated with PYTHIA, POWHEG, and MADGRAPH [107]. The uncertainty in the signal cross section related to the choice of parton distribution functions is determined with the PDF4LHC prescription [92–96].

The overall statistical methodology [108] used in this paper was developed by the CMS and ATLAS Collaborations in the context of the LHC Higgs Combination Group. A more concise summary of CMS usage in the search for a Higgs boson is given in Ref. [17]. The modified frequentist criterion CLs [109 , 110] is used for the calculation of exclusion limits. Systematic uncertainties are incorporated as nuisance parameters and are treated according to the frequentist paradigm. The combination of searches requires simultaneous analysis of the data selected by all individual analyses, accounting for all statistical and systematic uncertainties and their correlations. The probability for a background fluctuation to be at least as large as the observed maximum excess is termed the local p-value, and that for an excess anywhere in a specified mass range the global p-value. This probability can be evaluated by generating sets of simulated data incorporating all correlations between analyses optimized for different Higgs boson masses. The global p-value (for the specified region) is greater than the local p-value, and this fact is often referred to as the look-elsewhere effect (LEE) [111]. Both the local and global p-values can be expressed as a corresponding number of standard deviations using the one-sided Gaussian tail convention. The magnitude of a possible Higgs boson signal is characterised by the production cross section times the relevant branching fractions, relative to the SM expectation, denoted σ/σSM and referred to as the signal strength. The results presented in this paper are obtained using asymptotic formulae [112], including a few updates recently introduced in the ROOSTATS package [113].

Figure 1 shows the expected local p-values in the mass range 110–145 GeV for the five decay modes reported here. The expected significance of a SM Higgs boson signal at mH = 125 GeV when the five decay modes are combined is 5.6 σ. The highest sensitivity in this mass range is achieved in the ZZ, γγ, and WW channels. Because of the excellent mass resolution (1–2 GeV) achieved in the γγ and ZZ channels, they play a special role in the low-mass region, where the natural width of the SM Higgs boson is predicted to be a few MeV. The expected signature in these channels is therefore a narrow resonance above background, with a width consistent with the detector resolution.

5 Decay modes with high mass resolution

5.1 H γγ

In the H γγ analysis a search is made for a narrow peak in the diphoton invariant mass distribution in the range 110–150 GeV, on a large irreducible background from QCD production of two photons. There is also a reducible background where one or more of the reconstructed photons originate from misidentification of jet fragments. Early detailed studies indicated this to be one of the most promising channels in the search for a SM Higgs boson in the low-mass range [114].

5.1 H γγ 7

Figure 1: Expected local p-values for a SM Higgs boson as a function of mH, for the five decay modes and their combination.

To enhance the sensitivity of the analysis, candidate diphoton events are separated into mutually exclusive categories of different expected signal-to-background ratios, based on the properties of the reconstructed photons and on the presence of two jets satisfying criteria aimed at selecting events in which a Higgs boson is produced through the VBF process. The analysis uses multivariate techniques for the selection and classification of the events. As an independent cross-check, an analysis is also performed that is almost identical to the one described in Ref. [20], using simpler criteria based on the properties of the reconstructed photons to select and classify events. The multivariate analysis achieves 15% higher sensitivity than the crosscheck analysis.

The reconstructed primary vertex that most probably corresponds to the interaction vertex of the diphoton candidate is identified using the kinematic properties of the tracks associated with that vertex and their correlation with the diphoton kinematics. In addition, if either of the photons converts and the tracks from the conversion are reconstructed and identified, the direction of the converted photon contributes to the identification of the hard-scattering vertex. More details can be found in Ref. [20].

The event selection requires two photon candidates satisfying pT requirements and “loose” photon identification criteria. These photons must be reconstructed within the fiducial region, |η| < 2.5, excluding the barrel-endcap transition region, 1.44 < |η| < 1.57. A pT threshold of mγγ/3 (mγγ/4) is applied to the photon leading (subleading) in pT, where mγγ is the diphoton invariant mass. Scaling the pT thresholds in this way avoids distortion of the shape of the mγγ distribution. In the case of events passing the dijet selection, the requirement on the leading photon is increased to mγγ/2, further reducing background with negligible loss of signal.

Jet selection criteria are applied to the two jets of largest pT in the event within |η| < 4.7. The jet selection requirements are optimized using simulated VBF signal and diphoton background events. The pT thresholds for the two jets are 30 and 20 GeV, and their η separation is required to be greater than 3.5. The dijet invariant mass is required to be greater than 350 and 250 GeV for the 7 and 8 TeV data sets, respectively. The lower dijet invariant mass requirement for the 8 TeV data set reflects the fact that for the analysis of that data set, the dijet event category is divided into two to increase the search sensitivity. This division creates a second “tight” dijettagged category in which the dijet invariant mass must be greater than 500 GeV and both jets must have pT > 30 GeV. Two additional selection criteria, relating the dijet to the diphoton system, are applied: the difference between the average pseudorapidity of the two jets and the pseudorapidity of the diphoton system is required to be less than 2.5, and the difference in azimuthal angle between the diphoton system and the dijet system is required to be greater than 2.6 radians.

A multivariate regression is used to extract the photon energy and a photon-by-photon estimate of the uncertainty in that measurement. The calibration of the photon energy scale uses the Z boson mass as a reference; ECAL showers coming from electrons in Z ee events are clustered and reconstructed in exactly the same way as photon showers. The photon selection efficiency, energy resolution, and associated systematic uncertainties are estimated from data, using Z ee events to derive data/simulation correction factors. The jet reconstruction efficiency, the efficiency to correctly locate the vertex position, and the trigger efficiency, together with the corresponding systematic uncertainties, are also evaluated from data.

For the multivariate analysis, a boosted decision tree (BDT) [115, 116] is trained to give a high output value (score) for signal-like events and for events with good diphoton invariant mass resolution, based on the following observables: (i) the photon quality determined from electromagnetic shower shape and isolation variables; (ii) the expected mass resolution; (iii) the per-event estimate of the probability of locating the diphoton vertex within 10 mm of its true location along the beam direction; and (iv) kinematic characteristics of the photons and the diphoton system. The kinematic variables are constructed so as to contain no information about the invariant mass of the diphoton system. The diphoton events not satisfying the dijet selection are classified into five categories based on the output of the BDT, with category boundaries optimized for sensitivity to a SM Higgs boson. Events in the category with smallest expected signal-to-background ratio are rejected, leaving four categories of events. Dijet-tagged events with BDT scores smaller than the threshold for the fourth category are also rejected. Simulation studies indicate that the background in the selected event categories is dominated by the irreducible background from QCD production of two photons and that fewer than 30% of the diphoton events used in the analysis contain one or more misidentified photons (predominantly from γ+jet production).

Table 2 shows the expected number of signal events in each event category for a SM Higgs boson (of mH = 125 GeV), and the background at mγγ = 125 GeV, estimated from the fit described below. The estimated mass resolution is also shown, measured both by σeff, half the minimum width containing 68% of the signal events, and by the full width at half maximum (FWHM). A large variation in the expected signal-to-background ratio between the categories can be seen, although as a consequence of the optimization of the category boundaries the expected signal significances in each category are rather similar. The differences in the relative signal-to-background ratio between the categories are almost independent of mH.

The background is estimated from data, without the use of MC simulation, by fitting the diphoton invariant mass distribution in each of the categories in a range (100 < mγγ < 180 GeV) extending slightly above and below that in which the search is performed. The choices of the

5.1 H γγ 9

Table 2: Expected numbers of SM Higgs boson events (mH = 125 GeV) and estimated background (at mγγ = 125 GeV) for all event categories of the 7 and 8 TeV data sets. There are two dijet-tagged categories for the 8 TeV data as described in the text, and for both data sets the remaining untagged events are separated into four categories labelled here BDT 0–3, BDT 0 having the largest expected signal-to-background ratio. The composition of the SM Higgs boson signal in terms of the production processes, and its mass resolution, are also given.

Event SM Higgs boson expected signal (mH = 125 GeV) Background mγγ = 125 GeV (events/GeV)
categories Events ggH VBF VH ttH σeff (GeV) FWHM/2.35 (GeV)
7 TeV, 5.1 fb1 BDT 0 BDT 1 BDT 2 BDT 3 Dijet tag 3.2 16.3 21.5 32.8 2.9 61% 17% 19% 3% 88% 6% 6% – 92% 4% 4% – 92% 4% 4% – 27% 72% 1% – 1.21 1.26 1.59 2.47 1.73 1.14 1.08 1.32 2.07 1.37 3.3 ± 0.4 37.5 ± 1.3 74.8 ± 1.9 193.6 ± 3.0 1.7 ± 0.2
8 TeV, 5.3 fb1 BDT 0 BDT 1 BDT 2 BDT 3 Dijet tight Dijet loose 6.1 21.0 30.2 40.0 2.6 3.0 68% 12% 16% 4% 87% 6% 6% 1% 92% 4% 4% – 92% 4% 4% – 23% 77% – – 53% 45% 2% – 1.38 1.53 1.94 2.86 2.06 1.95 1.23 1.31 1.55 2.35 1.57 1.48 7.4 ± 0.6 54.7 ± 1.5 115.2 ± 2.3 256.5 ± 3.4 1.3 ± 0.2 3.7 ± 0.4

function used to model the background and of the fit range are made based on a study of the possible bias on the measured signal strength. Polynomial functions are used. The degree is chosen by requiring that the potential bias be at least a factor of 5 smaller than the statistical accuracy of the fit prediction. The required polynomial degree ranges from 3 to 5.

A further independent analysis (referred to as the sideband background model) is performed using a different approach to the background modelling. Its sensitivity is very similar to that of the standard analysis. It employs a fit to the output of an additional BDT that takes as input the diphoton invariant mass and the diphoton BDT output, and uses a background model derived from the sidebands of the invariant-mass distribution. A fit to the diphoton invariant-mass distribution is used to obtain the background normalisation. This fit is of a power law and excludes a window of width ±2%×mH around the mass hypothesis. The methodology allows a systematic uncertainty to be assigned to the fit shape.

The expected 95% CL upper limit on the signal strength σ/σSM, in the background-only hypothesis, for the combined 7 and 8 TeV data, is less than 1.0 in the range 110 < mH < 140 GeV, with a value of 0.76 at mH = 125 GeV. The observed limit indicates the presence of a significant excess at mH = 125 GeV in both the 7 and 8 TeV data. The features of the observed limit are confirmed by the independent sideband-background-model and cross-check analyses.

The local p-value is shown as a function of mH in Fig. 2 for the 7 and 8 TeV data, and for their combination. The expected significance of the local p-value for a SM Higgs boson of mass 125 GeV is 2.8 σ. The minimum local p-value corresponding to the upward fluctuation of the observed limit at 125 GeV corresponds to 4.1 σ. The significances of the corresponding minimum local p-values seen with the sideband-background-model and the cross-check analysis are 4.6 σ at mH = 125 GeV and 3.7 σ at mH = 124 GeV, respectively. The best-fit signal strength for a SM Higgs boson mass hypothesis of 125 GeV is σ/σSM = 1.6 ± 0.4.

In order to illustrate, in the mγγ distribution, the significance given by the statistical methods,

it is necessary to take into account the large differences in the expected signal-to-background ratios of the event categories shown in Table 2. The events are weighted according to the cate gory in which they fall. A weight proportional to S/(S + B) is used, as suggested in Ref. [117],

Figure 2: The local p-value as a function of mH in the γγ decay mode for the combined 7 and 8 TeV data sets. The additional lines show the values for the two data sets taken individually. The dashed line shows the expected local p-value for the combined data sets, should a SM Higgs boson exist with mass mH.

5.2 H ZZ

In the H ZZ 4f decay mode a search is made for a narrow four-lepton mass peak in the presence of a small continuum background. Early detailed studies outlined the promise of this mode over a wide range of Higgs boson masses [118]. Only the search in the range 110–160 GeV is reported here. Since there are differences in the reducible background rates and mass resolutions between the subchannels 4e, 4µ, and 2e2µ, they are analysed separately. The background sources include an irreducible four-lepton contribution from direct ZZ production via qq and gluon-gluon processes. Reducible contributions arise from Z + bb and tt production where the final states contain two isolated leptons and two b-quark jets producing secondary leptons. Additional background arises from Z+jets and WZ+jets events where jets are misidentified as leptons. Compared to the analysis reported in Ref. [21], the present analysis employs improved muon reconstruction, improved lepton identification and isolation, and a kinematic discriminant exploiting the decay kinematics expected for the signal events. An algorithm to recover final-state radiation (FSR) photons has also been deployed.

Electrons are required to have pT > 7 GeV and |η| < 2.5. The corresponding requirements for muons are pT > 5 GeV and |η| < 2.4. Electrons are selected using a multivariate identifier trained using a sample of W+jets events, and the working point is optimized using Z+jets events. Both muons and electrons are required to be isolated. The combined reconstruction

5.2 H ZZ 11

Figure 3: The diphoton invariant mass distribution with each event weighted by the S/(S + B) value of its category. The lines represent the fitted background and signal, and the coloured bands represent the ±1 and ±2 standard deviation uncertainties on the background estimate. The inset shows the central part of the unweighted invariant mass distribution.

and selection efficiency is measured using electrons and muons in Z boson decays. Muon reconstruction and identification efficiency for muons with pT < 15 GeV is measured using J/ψ decays.

The electron or muon pairs from Z boson decays are required to originate from the same primary vertex. This is ensured by requiring that the significance of the impact parameter with respect to the event vertex satisfy |SIP| < 4 for each lepton, where SIP = I/σI , I is the three-dimensional lepton impact parameter at the point of closest approach to the vertex, and σI its uncertainty.

Final-state radiation from the leptons is recovered and included in the computation of the lepton-pair invariant mass. The FSR recovery is tuned using simulated samples of ZZ 4f and tested on data samples of Z boson decays to electrons and muons. Photons reconstructed within |η| < 2.4 are considered as possibly due to FSR. The photons must satisfy the following

γ

requirements. They must be within ΔR < 0.07 of a muon and have pT > 2 GeV (most photon showers within this distance of an electron having already been automatically clustered with the electron shower); or if their distance from a lepton is in the range 0.07 < ΔR < 0.5, they

γ

must satisfy pT > 4 GeV, and be isolated within ΔR = 0.3. Such photon candidates are combined with the lepton if the resulting three-body invariant mass is less than 100 GeV and closer to the Z boson mass than the mass before the addition of the photon.

The event selection requires two pairs of same-flavour, oppositely charged leptons. The pair with invariant mass closest to the Z boson mass is required to have a mass in the range 40– 120 GeV and the other pair is required to have a mass in the range 12–120 GeV. The ZZ background is evaluated from MC simulation studies. Two different approaches are employed to estimate the reducible and instrumental backgrounds from data. Both start by selecting events in a background control region, well separated from the signal region, by relaxing the isolation and identification criteria for two same-flavour reconstructed leptons. In the first approach, the additional pair of leptons is required to have the same charge (to avoid signal contamination) while in the second, two opposite-charge leptons failing the isolation and identification criteria are required. In addition, a control region with three passing and one failing lepton is used to estimate contributions from backgrounds with three prompt leptons and one misidentified lepton. The event rates measured in the background control region are extrapolated to the signal region using the measured probability for a reconstructed lepton to pass the isolation and identification requirements. This probability is measured in an independent sample. Within uncertainties, comparable background counts in the signal region are estimated by both methods.

The number of selected ZZ 4f candidate events in the mass range 110 < m4f< 160 GeV, in each of the three final states, is given in Table 3, where m4f is the four-lepton invariant mass. The number of predicted background events, in each of the three final states, and their uncertainties are also given, together with the number of signal events expected from a SM Higgs boson of mH = 125 GeV. The m4f distribution is shown in Fig. 4. There is a clear peak at the Z boson mass where the decay Z 4f is reconstructed. This feature of the data is well reproduced by the background estimation. The figure also shows an excess of events above the expected background around 125 GeV. The total background and the numbers of events observed in the three bins where an excess is seen are also shown in Table 3. The combined signal reconstruction and selection efficiency, with respect to the mH = 125 GeV generated signal with mff > 1 GeV as the only cut, is 18% for the 4e channel, 40% for the 4µ channel, and 27% for the 2e2µ channel.

The kinematics of the H ZZ 4f process, for a given invariant mass of the four-lepton

5.2 H ZZ 13

Figure 4: Distribution of the four-lepton invariant mass for the ZZ 4f analysis. The points represent the data, the filled histograms represent the background, and the open histogram shows the signal expectation for a Higgs boson of mass mH = 125 GeV, added to the background expectation. The inset shows the m4f distribution after selection of events with KD > 0.5, as described in the text.

Table 3: The number of selected events, compared to the expected background yields and expected number of signal events (mH = 125 GeV) for each final state in the H ZZ analysis. The estimates of the Z + X background are based on data. These results are given for the mass range from 110 to 160 GeV. The total background and the observed numbers of events are also shown for the three bins (“signal region”) of Fig. 4 where an excess is seen (121.5 < m4f< 130.5 GeV).

Channel 4e 4µ 2e2µ 4f
ZZ background Z + X 2.7 ± 0.3 1.2+1.1 0.8 5.7 ± 0.6 0.9+0.7 0.6 7.2 ± 0.8 2.3+1.8 1.4 15.6 ± 1.4 4.4+2.2 1.7
All backgrounds (110 < m4f < 160 GeV) 4.0 ± 1.0 6.6 ± 0.9 9.7 ± 1.8 20 ± 3
Observed (110 < m4f < 160 GeV) 6 6 9 21
Signal (mH = 125 GeV) 1.36 ± 0.22 2.74 ± 0.32 3.44 ± 0.44 7.54 ± 0.78
All backgrounds (signal region) 0.7 ± 0.2 1.3 ± 0.1 1.9 ± 0.3 3.8 ± 0.5
Observed (signal region) 1 3 5 9

system, is fully described by five angles and the invariant masses of the two lepton pairs [119– 121]. These seven variables provide significant discriminating power between signal and back ground. A kinematic discriminant is constructed based on the probability ratio of the signal and background hypotheses, KD = Psig/(Psig + Pbkg) , as described in Ref. [122]. The likeli hood ratio is defined for each value of m4f. For the signal, the phase-space and Z propagator terms [123] are included in a fully analytic parameterization [120], while the background prob ability is tabulated using a simulation of the qq ZZ/Zγ process. The statistical analysis only includes events with m4f> 100 GeV.

Figure 5 (upper) shows the distribution of m4f versus KD for events selected in the 4f sub- channels. The colour-coded regions show the expected background. Figure 5 (lower) shows the same two-dimensional distribution of events, but this time superimposed on the expected event density from a SM Higgs boson (mH = 125 GeV). A clustering of events is observed around 125 GeV with a high score in the kinematic discriminant, where the background expectation is low and signal expectation high, corresponding to the excess seen in the one-dimensional mass distribution. The m4f distribution of events satisfying KD > 0.5 is shown in the inset in Fig. 4.

There are three final states and two data sets (7 and 8 TeV), and thus the statistical treatment requires six simultaneous two-dimensional maximum-likelihood fits for each value of mH, in the variables m4f and KD. Systematic uncertainties are evaluated from data for the trigger efficiency and for the combined lepton reconstruction, identification, and isolation efficiencies. Systematic uncertainties on the energy/momentum calibration and on the energy resolution are estimated from data. Additional systematic uncertainties arise from limited statistical precision in the reducible background control regions.

The expected 95% CL upper limit on the signal strength σ/σSM, in the background-only hypothesis, for the combined 7 and 8 TeV data, falls steeply between 110 and 140 GeV, and has a value of 0.6 at mH = 125 GeV. The observed upper limit indicates the presence of a significant excess in the range 120 < mH < 130 GeV. The local p-value is shown as a function of mH in Fig. 6 for the 7 and 8 TeV data, and for their combination. The minimum local p-value in the data occurs at mH = 125.6 GeV and has a significance of 3.2 σ (expected 3.8 σ). The combined best-fit signal strength for a SM Higgs boson mass hypothesis of 125.6 GeV is σ/σSM = 0.7+0.4

0.3.

6 Decay modes with low mass resolution

6.1 H WW

The decay mode H WW was first proposed as a promising search channel for study at the LHC in Ref. [124]. It is highly sensitive to a SM Higgs boson in the mass range around the WW threshold of 160 GeV. With the development of tools for lepton identification and Emiss re-

T

construction optimized for LHC pileup conditions, it is possible to extend the sensitivity down to 120 GeV. This decay mode is analysed by selecting events in which both W bosons decay leptonically, resulting in a signature with two isolated, oppositely charged leptons (electrons or muons) and large Emiss due to the undetected neutrinos. A pT threshold of 20 (10) GeV is

T

applied to the lepton leading (subleading) in pT. The analysis of the 7 TeV data is described in Ref. [22] and remains unchanged, while the 8 TeV analysis was modified to cope with more difficult conditions induced by the higher pileup of the 2012 data taking.

Events are classified according to the number of jets (0, 1, or 2) with pT > 30 GeV and within |η| < 4.7 (|η| < 5.0 for the 7 TeV data set), and further separated into same-flavour (ee and µµ)

6.1 H WW 15

Figure 5: The distribution of events selected in the 4f subchannels for the kinematic discriminant, KD, versus m4f. Events in the three final states are marked by filled symbols (defined in the legend). The horizontal error bars indicate the estimated mass resolution. In the upper plot the colour-coded regions show the background expectation; in the lower plot the colourcoded regions show the event density expected from a SM Higgs boson (mH = 125 GeV) (both in arbitrary units).

Figure 6: The observed local p-value for the ZZ decay mode as a function of the SM Higgs boson mass. The dashed line shows the expected local p-values for a SM Higgs boson with a mass mH.

or different-flavour (eµ) categories. Events with more than two jets are rejected. To improve the sensitivity of the analysis, the selection criteria are optimized separately for the different event categories since they are characterised by different dominating backgrounds. The zero-jet eµ category has the best signal sensitivity. Its main backgrounds are irreducible nonresonant WW production and reducible W+jets processes, where a jet is misidentified as a lepton. The one-jet eµ and zero-jet same-flavour categories only contribute to the signal sensitivity at the 10% level because of larger backgrounds, from top-quark decays and Drell–Yan production, respectively. Event selection in the two-jet category is optimized for the VBF production mechanism. This category has the highest expected signal-to-background ratio, but its contribution to the overall sensitivity is small owing to the lower cross section relative to inclusive production.

The projected Emiss variable [22] is used to reduce the Drell–Yan background arising from

T

events where the Emiss vector is aligned with the lepton pT, as well as events with mismeasured

T

Emiss

associated with poorly reconstructed leptons and jets. The projected Emiss is defined as

TT

the transverse component of the Emiss vector with respect to the closest lepton direction, if it is

T

closer than π/2 in azimuthal angle, or the full Emiss otherwise. Since the projected Emiss resolu-

TT

tion is deteriorated by pileup, the minimum of two different projected Emiss definitions is used:

T

the first includes all particle candidates in the event, while the second uses only the charged particle candidates associated with the primary vertex. In the 8 TeV analysis, the minimum projected Emiss defined in this way is then required to be above a threshold that varies by cate-

T

gory. For mH > 140 GeV, projected Emiss is required to be greater than 20 GeV in the eµ channel,

T

and greater than 45 GeV in the same-flavour channels. For mH 140 GeV in the same-flavour channels, where it is more difficult to separate the signal from the Drell–Yan background, a multivariate selection is used, combining kinematic and topological variables. In the two-jet category, a simple selection of Emiss > 45 GeV is applied. To further reduce the Drell–Yan back-

T

ground in the same-flavour final states, events with a dilepton mass within 15 GeV of the Z boson mass are rejected. The background from low-mass resonances is rejected by requiring a dilepton invariant mass greater than 12 GeV.

To suppress the top-quark background, a “top tagging” technique based on soft-muon and b

6.2 H ττ 17

jet tagging is applied. The first method is designed to veto events containing muons from b jets coming from decays of top quarks. The second method uses a b-jet tagging algorithm, which looks within jets for tracks with large impact parameters. The algorithm is applied also in the case of zero-jet events, which may contain low-pT jets below the selection threshold. To reduce the background from WZ production, events with a third lepton passing the identification and isolation requirements are rejected.

Yields for the dominant backgrounds are estimated using control regions in the data. The W+jets contribution is derived from data using a “tight-loose” sample in which one lepton passes the standard criteria and the other does not, but instead satisfies a “loose” set of requirements. The efficiency tloose for a jet that satisfies the loose selection to pass the tight selection is determined using data from an independent loose lepton-trigger sample dominated by jets. The background contamination is then estimated using the events of the “tight-loose” sample weighted by tloose/(1 tloose). The normalisation of the top-quark background is estimated by counting the number of top-tagged events and applying the corresponding top-tagging efficiency. The nonresonant WW contribution is normalised by using events with a dilepton mass larger than 100 GeV, where the Higgs boson signal contamination is negligible, extrapolated to the signal region using simulated samples. The same-flavour Drell–Yan background is normalised using the number of events observed with a dilepton mass within 7.5 GeV of the Z boson mass, after subtracting the non-Drell–Yan contribution. Other minor backgrounds from WZ, ZZ, and Wγ are estimated from simulation.

The 7 TeV data are analysed by training a BDT for each Higgs boson mass hypothesis in the zero-jet and one-jet event categories, while a simple selection strategy is employed in the VBF category [22]. In the BDT analysis, the Higgs boson signal is separated from the background by using a binned maximum-likelihood fit to the classifier distribution. The 8 TeV analysis is based on a simple selection strategy optimized for each mass hypothesis, where additional kinematic and topological requirements are applied to improve the signal-to-background ratio. One of the most sensitive variables to discriminate between H WW decays and nonresonant WW production is the dilepton invariant mass mff, which has a resolution of about 20%. This quan tity is shown in Fig. 7, for the zero-jet e µ category after the full selection for mH = 125 GeV, except for the selection on mff itself. Table 4 shows for the 8 TeV analysis the number of events selected in data, background estimates, and signal predictions for mH = 125 GeV in each analysis category after applying all the selection requirements. About 97% of the signal events selected in the zero-jet eµ category are expected to be produced by the gluon-gluon fusion process, whereas 83% of the signal in the two-jet eµ category is expected to be produced by the VBF process. The 95% CL expected and observed limits for the combination of the 7 and 8 TeV analyses are shown in Fig. 8. A broad excess is observed across the mass range. Given the modest mass resolution in this channel, this excess is consistent with a SM Higgs boson with a mass around 125 GeV. This is illustrated by the dotted curve in Fig. 8 showing the median expected limit under the hypothesis of the presence of a SM Higgs boson with mass 125 GeV. The expected significance for a SM Higgs of mass 125 GeV is 2.4 σ and the observed significance is 1.6 σ.

6.2 H ττ

The decay mode H ττ is searched for in four exclusive subchannels, corresponding to different decays of the τ pair: eµ, µµ,eτh, and µτh, where electrons and muons arise from leptonic τ decays, and τh denotes hadronic τ decays. The latter are reconstructed by selecting τ decays consistent with the hypothesis of three charged pions, or one charged pion and up to two neu tral pions [125]. The search is made in the mass range 110–145 GeV, and a signal should appear Table 4: Observed number of events, background estimates and signal predictions for mH = 125 GeV in each category of the WW analysis of the 8 TeV data set. All the selection requirements have been applied. The combined experimental and theoretical, systematic and statistical uncertainties are shown. The Zγ process includes the dimuon, dielectron, and ττ ff final states.

Category: 0-jet eµ 0-jet ff 1-jet eµ 1-jet ff 2-jet eµ 2-jet ff
WW 87.6 ± 9.5 60.4 ± 6.7 19.5 ± 3.7 9.7 ± 1.9 0.4 ± 0.1 0.3 ± 0.1
WZ + ZZ + Zγ 2.2 ± 0.2 37.7 ± 12.5 2.4 ± 0.3 8.7 ± 4.9 0.1 ± 0.0 3.1 ± 1.8
Top 9.3 ± 2.7 1.9 ± 0.5 22.3 ± 2.0 9.5 ± 1.1 3.4 ± 1.9 2.0 ± 1.2
W + jets 19.1 ± 7.2 10.8 ± 4.3 11.7 ± 4.6 3.9 ± 1.7 0.3 ± 0.3 0.0 ± 0.0
Wγ() 6.0 ± 2.3 4.6 ± 2.5 5.9 ± 3.2 1.3 ± 1.2 0.0 ± 0.0 0.0 ± 0.0
All backgrounds 124.2 ± 12.4 115.5 ± 15.0 61.7 ± 7.0 33.1 ± 5.7 4.1 ± 1.9 5.4 ± 2.2
Signal (mH = 125 GeV) 23.9 ± 5.2 14.9 ± 3.3 10.3 ± 3.0 4.4 ± 1.3 1.5 ± 0.2 0.8 ± 0.1
Data 158 123 54 43 6 7

Figure 7: Distribution of mff for the zero-jet eµ category in the H WW search at 8 TeV. The signal expected from a Higgs boson with a mass mH = 125 GeV is shown added to the background.

6.2 H ττ 19

Figure 8: The 95% CL limit on σ/σSM for a Higgs boson decaying, via a W boson pair, to two leptons and two neutrinos, for the combined 7 and 8 TeV data sets. The symbol σ/σSM denotes the production cross section times the relevant branching fractions, relative to the SM expectation. The background-only expectations are represented by their median (dashed line) and by the 68% and 95% CL bands. The dotted curve shows the median expected limit for a SM Higgs boson with mH = 125 GeV.

as a broad excess in the distribution of the τ-pair invariant mass mττ.

The sensitivity of the search is improved by classifying the events according to jet multiplicity and the transverse momentum of the reconstructed τ. The multiplicity of jets with pT > 30 GeV reflects the production mechanism: events with zero or one jet are likely to come from the gluon-gluon fusion process, while events with two jets are candidates for VBF production. Events including jets with pT > 20 GeV are removed from zero-and one-jet categories. The signal purities in the zero-and one-jet categories are increased, and the mττ resolution is improved, by separating events into low-and high-pT subchannels. The high-pT subchannels are defined by p τh > 40 GeV in channels with a hadronic τ decay, and pµ > 35 (30) GeV in the

TT

eµ (µµ) channel. The mass mττ is reconstructed with an algorithm [126] combining the visible τ decay products and the missing transverse energy, achieving a resolution of about 20% on mττ . Figure 9 shows as an example the reconstructed mττ distribution in the µτh VBF category

Figure 9: Distribution of mττ in the combined 7 and 8 TeV data sets for the µτh VBF category of the H ττ search. The signal expected from a SM Higgs boson (mH = 125 GeV) is added to the background simulation.

Backgrounds in the eµ and µµ channels arise from tt and Drell–Yan production, while W and Z production with a misidentified τh candidate from an electron, muon, or jet dominates in the hadronic channels. Backgrounds from Z ττ decays are modelled with Z µµ events in data where each muon is replaced with particles from simulated decays of a τ with the same momentum as the muon. Reducible backgrounds, comprising W+jets, QCD multijet production, and residual Z ee events, are estimated from the data. An improved signal-tobackground ratio is achieved by including explicitly in the event selection for the VBF production mechanism the pseudorapidity separation between forward jets and the large invariant mass of the dijet system. Table 5 shows the numbers of expected and observed events in the most sensitive event categories (VBF) for the 7 and 8 TeV data sets. The expected signal yields for a SM Higgs boson with mH = 125 GeV are also shown.

6.2 H ττ 21

Table 5: Numbers of expected and observed events in the most sensitive event categories (VBF) in the H ττ analysis for the 7 and 8 TeV data sets. The expected signal yields for a SM Higgs boson with mH = 125 GeV are also shown. Combined statistical and systematic uncertainties on each estimate are reported.

Subchannel eτh µτh eµ µµ
Z ττ QCD W+jets Z+jets Z µµ tt Dibosons 53 ± 5 35 ± 7 46 ± 10 13 ± 2 7.0 ± 1.7 1.2 ± 0.9 100 ± 9 41 ± 9 72 ± 15 2.5 ± 0.6 14 ± 3 2.9 ± 2.1 56 ± 12 7.4 ± 1.4 24 ± 2 11 ± 2 5.3 ± 0.4 70 ± 8 6.7 ± 1.5 2.4 ± 0.9
All backgrounds 156 ± 13 233 ± 20 99 ± 13 85 ± 9
Signal (mH = 125 GeV) 4.3 ± 0.6 7.7 ± 1.1 3.5 ± 0.4 0.8 ± 0.1
Data 142 263 110 83

To search for the presence of a Higgs boson signal in the selected events, a binned maximum-likelihood fit to mττ is performed jointly across the four final states, each with five event categories. Systematic uncertainties are represented by nuisance parameters in the fitting process. The expected and observed 95% CL limits on the signal strength for the combination of all cat egories are shown in Fig. 10. The expected and observed limits are 1.3 and 1.1 times the SM Higgs boson cross section at mass 125 GeV, respectively. The expected significance for a SM Higgs boson of mass 125 GeV is 1.4 σ, and the observed value is zero σ.

6.3 H bb

For mH 135 GeV, the decay H bb has the largest branching fraction of the five search modes, but the signal is overwhelmed by QCD production of bottom quarks. The analysis is therefore designed to search for the associated production of the Higgs boson in events where a dijet resonance is produced at high pT in association with a W or Z boson; this largely suppresses the QCD background. Five independent search channels are explored corresponding to different decays of the vector boson: Z(ff)H, Z(νν)H, and W(fν)H. Events are further separated into two categories based on the pT of the vector boson, ranging from 50–100 GeV for the lowest bin in the Z(ff) search, to greater than 170 GeV for the highest bin in the W(fν)

Emiss

search. For the Z(νν) search, two subchannels are defined as 120 < T < 160 GeV and

Emiss

T > 160 GeV. The two jets comprising the candidate Higgs boson decay are required to be identified as b jets, and the dijet system must satisfy a pT threshold that is optimized within each channel.

Dominant backgrounds arise from production of vector bosons in association with jets, pair-or single-production of top quarks, and diboson production (WW, WZ, ZZ) with one of the bosons decaying hadronically. Significant background rejection is achieved in general by requiring large pT for the dijet, while also requiring that there be minimal additional jet activity and that the vector boson and dijet be back-to-back in azimuth. The effect on the signal efficiency of this selection due to higher-order electroweak [127] and QCD [87] corrections are accounted for in the systematic uncertainties. Further signal discrimination is obtained from the dijet invariant mass, which is expected to peak near mH. A multivariate regression algorithm to better estimate b-jet pT is trained on jets in simulated signal events and achieves a final dijet mass resolution of 8–9% for mH = 125 GeV. The performance of the regression algorithm is checked in data using W/Z+jets and tt events.

A search for the signal is made in the distribution of scores of a BDT trained at discrete mass points. Input variables to the BDT algorithm exploit kinematic and topological information about the vector boson and dijet systems, and the colour-singlet nature of the Higgs boson [128]. The distribution of scores in simulated background events is checked using control regions in the data designed to enrich individual background contributions. Figure 11 shows as an exam ple the BDT scores for the high-pT subchannel of the Z(νν) search in the 8 TeV data set, after all selection criteria have been applied.

The rates for the dominant backgrounds arising from production of W/Z+jets and top-quark pairs are estimated in data, while contributions from single-top and diboson production are estimated from simulation studies. The signal is then searched for as an excess in the BDT score distribution using the predicted shapes for signal and background events, for Higgs boson masses in the range 110–135 GeV.

Combined results for expected and observed 95% CL limits obtained from the 7 and 8 TeV data sets are displayed in Fig. 12. The expected and observed limits are 1.6 and 2.1 times the SM Higgs boson cross section at mass 125 GeV. The expected local p-value for a SM Higgs of mass

6.3 H bb 23

125 GeV corresponds to 1.9 σ, while the observed one corresponds to 0.7 σ.

7 Combined results

The individual results for the channels analysed for the five decay modes, summarised in Ta ble 1, are combined using the methods outlined in Section 4. The combination takes into ac count the experimental statistical and systematic uncertainties as well as the theoretical uncertainties, which are dominated by the imperfect knowledge of the QCD scale and parton distribution functions. The CLs is shown in Fig. 13 as a function of the Higgs boson mass hypothesis. The observed values are shown by the solid points. The dashed line indicates the median of the expected results for the background-only hypothesis, with the green (dark) and yellow (light) bands indicating the ranges in which the CLs values are expected to lie in 68% and 95% of the experiments under the background-only hypothesis. The probabilities for an observation, in the absence of a signal, to lie above or below the 68% (95%) band are 16% (2.5%) each. The thick horizontal lines indicate CLs values of 0.05, 0.01, and 0.001. The mass regions where the observed CLs values are below these lines are excluded with the corresponding (1 CLs) confidence levels. Our previously published results exclude the SM Higgs boson from 127 up to 600 GeV [17]. In the search described here, the SM Higgs boson is excluded at 95% CL in the range 110 < mH < 121.5 GeV. In the range 121.5 < mH < 128 GeV a significant excess is seen and the SM Higgs boson cannot be excluded at 95% CL.

7.1 Significance of the observed excess 25

Figure 13: The CLs values for the SM Higgs boson hypothesis as a function of the Higgs boson mass in the range 110–145 GeV. The background-only expectations are represented by their median (dashed line) and by the 68% and 95% CL bands.

7.1 Significance of the observed excess

The consistency of the observed excess with the background-only hypothesis may be judged from Fig. 14, which shows a scan of the local p-value for the 7 and 8 TeV data sets and their combination. The 7 and 8 TeV data sets exhibit an excess of 3.2 σ and 3.8 σ significance, respectively, for a Higgs boson mass of approximately 125 GeV. In the overall combination the significance is 5.0 σ for mH = 125.5 GeV. Figure 15 gives the local p-value for the five decay modes individually and displays the expected overall p-value.

The largest contributors to the overall excess in the combination are the γγ and ZZ decay modes. They both have very good mass resolution, allowing good localization of the invariant mass of a putative resonance responsible for the excess. Their combined significance reaches

5.0 σ (Fig. 16). The WW decay mode has an exclusion sensitivity comparable to the γγ and ZZ decay modes but does not have a good mass resolution. It has an excess with local significance

1.6 σ for mH 125 GeV. When added to the γγ and ZZ decay modes, the combined significance becomes 5.1 σ. Adding the bb and ττ channels in the combination, the final significance becomes 5.0 σ. Table 6 summarises the expected and observed local p-values for a SM Higgs boson mass hypothesis of 125.5 GeV for the various combinations of channels.

Table 6: The expected and observed local p-values, expressed as the corresponding number of standard deviations of the observed excess from the background-only hypothesis, for mH =

125.5 GeV, for various combinations of decay modes. Decay mode/combination

Expected (σ) Observed (σ)

γγ ZZ 2.8 3.6 4.1 3.1
ττ + bb γγ + ZZ γγ + ZZ + WW γγ + ZZ + WW + ττ + bb 2.4 4.7 5.2 5.8 0.4 5.0 5.1 5.0

The global p-value for the search range 115–130 (110–145) GeV is calculated using the method

7.2 Mass of the observed boson 27

suggested in Ref. [111], and corresponds to 4.6 σ (4.5 σ). These results confirm the very low probability for an excess as large or larger than that observed to arise from a statistical fluctuation of the background. The excess constitutes the observation of a new particle with a mass near 125 GeV, manifesting itself in decays to two photons or ZZ. These two decay modes indicate that the new particle is a boson; the two-photon decay implies that its spin is different from one [129, 130].

7.2 Mass of the observed boson

The mass mX of the observed boson is determined using the γγ and ZZ decay modes, with the former dominating the precision of the measurement. The calibration of the energy scale in the γγ decay mode is achieved with reference to the known Z boson mass, as described in Section 5.1. There are two main sources of systematic uncertainty: (i) imperfect simulation of the differences between electrons and photons and (ii) the need to extrapolate from mZ to mH 125 GeV. The systematic uncertainties are evaluated by making comparisons between data and simulated samples of Z ee and H γγ (mH = 90 GeV). The two uncertainties, which together amount to 0.5%, are assumed to be fully correlated between all the γγ event categories in the 7 and 8 TeV data. For the ZZ 4f decay mode the energy scale (for electrons) and momentum scale (for muons) are calibrated using the leptonic decays of the Z boson, with an assigned uncertainty of 0.4%.

Figure 17 shows the two-dimensional 68% CL regions for the signal strength σ/σSM versus mX for the three channels (untagged γγ, dijet-tagged γγ, and ZZ 4f). The combined 68% CL contour shown in Fig. 17 assumes that the relative event yields among the three channels are those expected from the standard model, while the overall signal strength is a free parameter.

To extract the value of mX in a model-independent way, the signal yields of the three channels are allowed to vary independently. Thus the expected event yields in these channels are scaled by independent factors, while the signal is assumed to be due to a particle with a unique mass mX. The combined best-fit mass is mX = 125.3 ± 0.4 (stat.) ± 0.5 (syst.) GeV.

7.3 Compatibility with the SM Higgs boson hypothesis

A first test of the compatibility of the observed boson with the SM Higgs boson is provided by examination of the best-fit value for the common signal strength σ/σSM, obtained in a com bination of all search channels. Figure 18 shows a scan of the overall σ/σSM obtained in the combination of all channels versus a hypothesised Higgs boson mass mH. The band corresponds to the ±1 σ uncertainty (statistical and systematic). The excesses seen in the 7 TeV and 8 TeV data, and in their combination, around 125 GeV are consistent with unity within the ±1 σ uncertainties. The observed σ/σSM value for an excess at 125.5 GeV in a combination of all data is 0.87 ± 0.23. The different decay channels and data sets have been examined for self-consistency. Figure 19 shows the measured values of σ/σSM results obtained for the different decay modes. These results are consistent, within uncertainties, with the expectations for a SM

8 Conclusions

Results are presented from searches for the standard model Higgs boson in proton-proton col

lisions at s = 7 and 8 TeV in the CMS experiment at the LHC, using data samples corresponding to integrated luminosities of up to 5.1 fb1 at 7 TeV and 5.3 fb1 at 8 TeV. The search

is performed in five decay modes: γγ, ZZ, W+W, τ+τ, and bb. An excess of events is observed above the expected background, with a local significance of 5.0 σ, at a mass near 125 GeV, signalling the production of a new particle. The expected local significance for a standard model Higgs boson of that mass is 5.8 σ. The global p-value in the search range of 115–130 (110–145) GeV corresponds to 4.6 σ (4.5 σ). The excess is most significant in the two decay modes with the best mass resolution, γγ and ZZ, and a fit to these signals gives a mass of 125.3 ± 0.4 (stat.) ± 0.5 (syst.) GeV. The decay to two photons indicates that the new particle is a boson with spin different from one. The results presented here are consistent, within uncertainties, with expectations for a standard model Higgs boson. The collection of further data will enable a more rigorous test of this conclusion and an investigation of whether the properties of the new particle imply physics beyond the standard model.

Acknowledgements

We congratulate our colleagues in the CERN accelerator departments for the excellent performance of the LHC machine. We thank the computing centres in the Worldwide LHC computing Grid for the provisioning and excellent performance of computing infrastructure essential to our analyses. We gratefully acknowledge the contributions of the technical staff at CERN and other CMS institutes. We also thank the administrative staff at CERN and the other CMS institutes and acknowledge support from: BMWF and FWF (Austria); FNRS and FWO (Belgium); CNPq, CAPES, FAPERJ, and FAPESP (Brazil); MES (Bulgaria); CERN; CAS, MoST, and NSFC (China); COLCIENCIAS (Colombia); MSES (Croatia); RPF (Cyprus); MEYS (Czech Republic); MoER, SF0690030s09 and ERDF (Estonia); Academy of Finland, MEC, and HIP (Finland); CEA and CNRS/IN2P3 (France); BMBF, DFG, and HGF (Germany); GSRT (Greece); OTKA and NKTH (Hungary); DAE and DST (India); IPM (Iran); SFI (Ireland); INFN (Italy); NRF and WCU (Korea); LAS (Lithuania); CINVESTAV, CONACYT, SEP, and UASLP-FAI (Mexico); MSI (New Zealand); PAEC (Pakistan); MSHE and NSC (Poland); FCT (Portugal); JINR (Armenia, Belarus, Georgia, Ukraine, Uzbekistan); MON, RosAtom, RAS and RFBR (Russia); MSTD (Serbia); SEIDI and CPAN (Spain); Swiss Funding Agencies (Switzerland); NSC (Taipei); TUBITAK and TAEK (Turkey); NASU (Ukraine); STFC (United Kingdom); DOE and NSF (USA). Individuals have received support from the Marie-Curie programme and the European Research Council (European Union); the Leventis Foundation; the A. P. Sloan Foundation; the Alexander von Humboldt Foundation; the Austrian Science Fund (FWF); the Belgian Federal Science Policy Office; the Fonds pour la Formation `

a la Recherche dans l’Industrie et dans l’Agriculture (FRIA-Belgium); the Agentschap voor Innovatie door Wetenschap en Technologie (IWT-Belgium); the Council of Science and Industrial Research, India; the Compagnia di San Paolo (Torino); and the HOMING PLUS programme of Foundation for Polish Science, cofinanced from European Union, Regional Development Fund.

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A The CMS Collaboration

Yerevan Physics Institute, Yerevan, Armenia

S. Chatrchyan, V. Khachatryan, A.M. Sirunyan, A. Tumasyan

Institut f ¨ur Hochenergiephysik der OeAW, Wien, Austria

W. Adam, E. Aguilo, T. Bergauer, M. Dragicevic, J. Er¨o, C. Fabjan1, M. Friedl, R. Fr ¨,uhwirth1

V.M. Ghete, J. Hammer, M. Hoch, N. H¨ormann, J. Hrubec, M. Jeitler1, W. Kiesenhofer, V. Kn ¨unz,

M. Krammer1, I. Kr¨atschmer, D. Liko, W. Majerotto, I. Mikulec, M. Pernicka, B. Rahbaran,

C. Rohringer, H. Rohringer, R. Sch¨o, A. Taurok, W. Waltenberger, ofbeck, J. Strauss, F. Szoncs´

G. Walzel, E. Widl, C.-E. Wulz1

National Centre for Particle and High Energy Physics, Minsk, Belarus

V. Chekhovsky, I. Emeliantchik, A. Litomin, V. Makarenko, V. Mossolov, N. Shumeiko, A. Solin,

R. Stefanovitch, J. Suarez Gonzalez

Research Institute for Nuclear Problems, Minsk, Belarus

A. Fedorov, M. Korzhik, O. Missevitch, R. Zuyeuski

Universiteit Antwerpen, Antwerpen, Belgium

M. Bansal, S. Bansal, W. Beaumont, T. Cornelis, E.A. De Wolf, D. Druzhkin, X. Janssen,

S. Luyckx, L. Mucibello, S. Ochesanu, B. Roland, R. Rougny, M. Selvaggi, Z. Staykova, H. Van Haevermaet, P. Van Mechelen, N. Van Remortel, A. Van Spilbeeck

Vrije Universiteit Brussel, Brussel, Belgium

F. Blekman, S. Blyweert, J. D’Hondt, O. Devroede, R. Gonzalez Suarez, R. Goorens,

A. Kalogeropoulos, M. Maes, A. Olbrechts, S. Tavernier, W. Van Doninck, L. Van Lancker, P. Van Mulders, G.P. Van Onsem, I. Villella

Universit´e Libre de Bruxelles, Bruxelles, Belgium

B. Clerbaux, G. De Lentdecker, V. Dero, J.P. Dewulf, L. Favart, A.P.R. Gay, T. Hreus, A. L´eonard,

P.E.
Marage, A. Mohammadi, T. Reis, S. Rugovac, L. Thomas, C. Vander Velde, P. Vanlaer,
J.
Wang, J. Wickens

Ghent University, Ghent, Belgium

V. Adler, K. Beernaert, A. Cimmino, S. Costantini, G. Garcia, M. Grunewald, B. Klein,

J. Lellouch, A. Marinov, J. Mccartin, A.A. Ocampo Rios, D. Ryckbosch, N. Strobbe, F. Thyssen,

M. Tytgat, P. Verwilligen, S. Walsh, E. Yazgan, N. Zaganidis

Universit´e Catholique de Louvain, Louvain-la-Neuve, Belgium

S. Basegmez, G. Bruno, R. Castello, L. Ceard, J. De Favereau De Jeneret, C. Delaere, P. Demin,

T. du Pree, D. Favart, L. Forthomme, A. Giammanco2, G. Gr´egoire, J. Hollar, V. Lemaitre, J. Liao,

O. Militaru, C. Nuttens, D. Pagano, A. Pin, K. Piotrzkowski, N. Schul, J.M. Vizan Garcia

Universit´e de Mons, Mons, Belgium

N. Beliy, T. Caebergs, E. Daubie, G.H. Hammad

Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, Brazil

G.A. Alves, L. Brito, M. Correa Martins Junior, D. De Jesus Damiao, T. Martins, M.E. Pol,

M.H.G. Souza

Universidade do Estado do Rio de Janeiro, Rio de Janeiro, Brazil

W.L. Ald´a J unior, W. Carvalho, A. Cust´odio, E.M. Da Costa, C. De Oliveira Martins, S. Fonseca

´De Souza, D. Matos Figueiredo, L. Mundim, H. Nogima, V. Oguri, W.L. Prado Da Silva,

A. Santoro, A. Sznajder

Instituto de Fisica Teorica, Universidade Estadual Paulista, Sao Paulo, Brazil

T.S.
Anjos3, C.A. Bernardes3, F.A. Dias4, T.R. Fernandez Perez Tomei, E. M. Gregores3, R.L. Iope,
C.
Lagana, S.M. Lietti, F. Marinho, P.G. Mercadante3, S.F. Novaes, Sandra S. Padula

Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria

L. Dimitrov, V. Genchev5, P. Iaydjiev5, S. Piperov, M. Rodozov, S. Stoykova, G. Sultanov,

V. Tcholakov, R. Trayanov, I. Vankov, M. Vutova

Institute of System Engineering and Robotics, Sofia, Bulgaria

C. Roumenin, D. Uzunova, R. Zahariev

University of Sofia, Sofia, Bulgaria

A. Dimitrov, R. Hadjiiska, V. Kozhuharov, L. Litov, B. Pavlov, P. Petkov

Institute of High Energy Physics, Beijing, China

J.G.
Bian, G.M. Chen, H.S. Chen, K.L. He, C.H. Jiang, W.G. Li, D. Liang, S. Liang, X. Meng,
G.
Sun, H.S. Sun, J. Tao, J. Wang, X. Wang, Z. Wang, H. Xiao, M. Xu, M. Yang, J. Zang, X. Zhang,
Z.
Zhang, Z. Zhang, W.R. Zhao, Z. Zhu

State Key Lab. of Nucl. Phys. and Tech., Peking University, Beijing, China

C. Asawatangtrakuldee, Y. Ban, J. Cai, S. Guo, Y. Guo, W. Li, H.T. Liu, S. Liu, Y. Mao, S.J. Qian,

H. Teng, D. Wang, Y.L. Ye, L. Zhang, B. Zhu, W. Zou

Universidad de Los Andes, Bogota, Colombia

C. Avila, J.P. Gomez, B. Gomez Moreno, A.F. Osorio Oliveros, J.C. Sanabria

Technical University of Split, Split, Croatia

N. Godinovic, D. Lelas, R. Plestina6, D. Polic, I. Puljak5

University of Split, Split, Croatia

Z. Antunovic, M. Kovac

Institute Rudjer Boskovic, Zagreb, Croatia

V. Brigljevic, S. Duric, K. Kadija, J. Luetic, S. Morovic

University of Cyprus, Nicosia, Cyprus

A. Attikis, M. Galanti, G. Mavromanolakis, J. Mousa, C. Nicolaou, F. Ptochos, P.A. Razis

Charles University, Prague, Czech Republic

M. Finger, M. Finger Jr.

Academy of Scientific Research and Technology of the Arab Republic of Egypt, Egyptian Network of High Energy Physics, Cairo, Egypt

A. Aly, Y. Assran7, A. Awad, S. Elgammal8, A. Ellithi Kamel9, S. Khalil8, M.A. Mahmoud10,

A. Mahrous, A. Radi11,12

National Institute of Chemical Physics and Biophysics, Tallinn, Estonia

A. Hektor, M. Kadastik, K. Kannike, M. M untel, M. Murumaa, M. Raidal, L. Rebane,

¨

A. Strumia, A. Tiko

Department of Physics, University of Helsinki, Helsinki, Finland

P. Eerola, G. Fedi, M. Voutilainen

Helsinki Institute of Physics, Helsinki, Finland

E. Anttila, J. H¨ark¨onen, A. Heikkinen, V. Karim¨aki, H.M. Katajisto, R. Kinnunen,

M.J. Kortelainen, M. Kotam¨en, K. Lassila-Perini, S. Lehti, T. Lind´

aki, T. Lamp´en, P. Luukka, T. Maenp¨¨a, T. Peltola, E. Tuominen, J. Tuominiemi, E. Tuovinen, D. Ungaro, T.P. Vanhala,

L. Wendland

Lappeenranta University of Technology, Lappeenranta, Finland

K. Banzuzi, A. Karjalainen, A. Korpela, T. Tuuva

DSM/IRFU, CEA/Saclay, Gif-sur-Yvette, France

M. Anfreville, M. Besancon, S. Choudhury, M. Dejardin, D. Denegri, B. Fabbro, J.L. Faure,

F. Ferri, S. Ganjour, F.X. Gentit, A. Givernaud, P. Gras, G. Hamel de Monchenault, P. Jarry,

F. Kircher, M.C. Lemaire, E. Locci, J. Malcles, I. Mandjavidze, A. Nayak, J.P. Pansart, J. Rander,

J.M. Reymond, A. Rosowsky, I. Shreyber, M. Titov, P. Verrecchia

Laboratoire Leprince-Ringuet, Ecole Polytechnique, IN2P3-CNRS, Palaiseau, France

J. Badier, S. Baffioni, F. Beaudette, E. Becheva, L. Benhabib, L. Bianchini, M. Bluj13,

C. Broutin, P. Busson, M. Cerutti, D. Chamont, C. Charlot, N. Daci, T. Dahms, M. Dalchenko,

L. Dobrzynski, A. Florent, Y. Geerebaert, R. Granier de Cassagnac, M. Haguenauer, P. Hennion,

G. Milleret, P. Min´e, C. Mironov, I.N. Naranjo, M. Nguyen, C. Ochando, P. Paganini,

T. Romanteau, D. Sabes, R. Salerno, A. Sartirana, Y. Sirois, C. Thiebaux, C. Veelken, A. Zabi

Institut Pluridisciplinaire Hubert Curien, Universit´e de Strasbourg, Universit´e de Haute Alsace Mulhouse, CNRS/IN2P3, Strasbourg, France

J.-L. Agram14, J. Andrea, A. Besson, D. Bloch, D. Bodin, J.-M. Brom, M. Cardaci, E.C. Chabert,

C. Collard, E. Conte14, F. Drouhin14, C. Ferro, J.-C. Fontaine14, D. Gel´e, U. Goerlach,

C. Goetzmann, L. Gross, D. Huss, P. Juillot, E. Kieffer, A.-C. Le Bihan, J. Pansanel, Y. Patois,

P. Van Hove

Centre de Calcul de l’Institut National de Physique Nucleaire et de Physique des Particules, CNRS/IN2P3, Villeurbanne, France, Villeurbanne, France

D. Boutigny, D. Mercier

Universit´e de Lyon, Universit´e Claude Bernard Lyon 1, CNRS-IN2P3, Institut de Physique Nucl´eaire de Lyon, Villeurbanne, France

G. Baulieu, S. Beauceron, N. Beaupere, M. Bedjidian, O. Bondu, G. Boudoul, S. Brochet,

J. Chasserat, R. Chierici5, C. Combaret, D. Contardo, P. Depasse, H. El Mamouni, J. Fay,

S. Gascon, N. Giraud, M. Gouzevitch, R. Haroutunian, B. Ille, T. Kurca, M. Lethuillier, N. Lumb,

H. Mathez, L. Mirabito, S. Perries, L. Sgandurra, V. Sordini, Y. Tschudi, M. Vander Donckt,

P. Verdier, S. Viret

E. Andronikashvili Institute of Physics, Academy of Science, Tbilisi, Georgia

V. Roinishvili, L. Rurua

Institute of High Energy Physics and Informatization, Tbilisi State University, Tbilisi, Georgia

N. Amaglobeli, I. Bagaturia, B. Chiladze, R. Kvatadze, D. Lomidze, R. Shanidze,

Z. Tsamalaidze15

RWTH Aachen University, I. Physikalisches Institut, Aachen, Germany

R. Adolphi, G. Anagnostou, C. Autermann, S. Beranek, R. Brauer, W. Braunschweig, B. Calpas,

M. Edelhoff, L. Feld, N. Heracleous, O. Hindrichs, R. Jussen, W. Karpinski, K. Klein,

K. L ¨ubelsmeyer, J. Merz, A. Ostapchuk, D. Pandoulas, A. Perieanu, F. Raupach, J. Sammet,

S. Schael, D. Schmitz, A. Schultz von Dratzig, R. Siedling, D. Sprenger, H. Weber, B. Wittmer,

M. Wlochal, V. Zhukov16

RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany

M. Ata, P. Biallass, J. Caudron, E. Dietz-Laursonn, D. Duchardt, M. Erdmann, R. Fischer,

A. G ¨uth, T. Hebbeker, C. Heidemann, G. Hilgers, K. Hoepfner, C. Hof, T. Klimkovich,

D. Klingebiel, P. Kreuzer, C. Magass, M. Merschmeyer, A. Meyer, M. Olschewski, P. Papacz,

B. Philipps, H. Pieta, H. Reithler, S.A. Schmitz, L. Sonnenschein, M. Sowa, J. Steggemann,

D. Teyssier, M. Weber

RWTH Aachen University, III. Physikalisches Institut B, Aachen, Germany

M. Bontenackels, V. Cherepanov, Y. Erdogan, G. Fl ¨ugge, H. Geenen, M. Geisler, W. Haj Ahmad,

F. Hoehle, B. Kargoll, T. Kress, Y. Kuessel, A. Nowack, L. Perchalla, O. Pooth, P. Sauerland,

A. Stahl, M.H. Zoeller

Deutsches Elektronen-Synchrotron, Hamburg, Germany

M. Aldaya Martin, J. Behr, W. Behrenhoff, U. Behrens, M. Bergholz17, A. Bethani, K. Borras,

A. Burgmeier, A. Cakir, L. Calligaris, A. Campbell, E. Castro, F. Costanza, D. Dammann, C. Diez Pardos, G. Eckerlin, D. Eckstein, A. Flossdorf, G. Flucke, A. Geiser, I. Glushkov, P. Goettlicher,

A. Grebenyuk, P. Gunnellini, S. Habib, J. Hauk, G. Hellwig, H. Jung, M. Kasemann, P. Katsas,

C. Kleinwort, H. Kluge, A. Knutsson, M. Kr¨amer, D. Kr ucker, E. Kuznetsova, W. Lange,¨

B. Lewendel, W. Lohmann17, B. Lutz, R. Mankel, I. Marfin, M. Marienfeld, I.-A. Melzer-Pellmann, A.B. Meyer, J. Mnich, C. Muhl, A. Mussgiller, S. Naumann-Emme, O. Novgorodova,

J. Olzem, A. Parenti, H. Perrey, A. Petrukhin, D. Pitzl, A. Raspereza, P.M. Ribeiro Cipriano,

C. Riedl, E. Ron, C. Rosemann, M. Rosin, J. Salfeld-Nebgen, R. Schmidt17, T. Schoerner-Sadenius, N. Sen, A. Spiridonov, M. Stein, J. Tomaszewska, D. Volyanskyy, R. Walsh,

C. Wissing, C. Youngman

University of Hamburg, Hamburg, Germany

V. Blobel, J. Draeger, H. Enderle, J. Erfle, U. Gebbert, M. G¨orner, T. Hermanns, R.S. H¨oing,

K. Kaschube, G. Kaussen, H. Kirschenmann, R. Klanner, J. Lange, B. Mura, F. Nowak,

T. Peiffer, N. Pietsch, D. Rathjens, C. Sander, H. Schettler, P. Schleper, E. Schlieckau, A. Schmidt,

M. Schr¨oder, T. Schum, M. Seidel, V. Sola, H. Stadie, G. Steinbr uck, J. Thomsen, L. Vanelderen ¨

Institut f ¨ur Experimentelle Kernphysik, Karlsruhe, Germany

C. Barth, J. Bauer, J. Berger, P. Bl¨um, C. B¨oser, V. Buege, Z.Y. Chen, S. Chowdhury, T. Chwalek,

D. Daeuwel, W. De Boer, A. Descroix, A. Dierlamm, G. Dirkes, M. Fahrer, M. Feindt,

U. Felzmann, M. Frey, A. Furgeri, I. Gebauer, A. Gessler, J. Gruschke, M. Guthoff5, C. Hackstein,

F. Hartmann, F. Hauler, T. Hauth5, S. Heier, S.M. Heindl, M. Heinrich, A. Heiss, H. Held,

K.H.
Hoffmann, S. Honc, U. Husemann, M. Imhof, C. Jung, S. Junghans, I. Katkov16,
U.
Kerzel, D. Knoblauch, J.R. Komaragiri, M. Kr¨aber, T. Kuhr, T. Liamsuwan, P. Lobelle Pardo,
D.
Martschei, A. Menchikov, X. Mol, D. M¨ormann, S. Mueller, Th. M ¨

uller, D. Neuberger,

M.B. Neuland, M. Niegel, A. N ¨urnberg, O. Oberst, A. Oehler, T. Ortega Gomez, J. Ott,

C. Piasecki, A. Poschlad, G. Quast, K. Rabbertz, F. Ratnikov, N. Ratnikova, M. Renz, S. R¨ocker,

F. Roederer, A. Sabellek, C. Saout, A. Scheurer, D. Schieferdecker, P. Schieferdecker, F.

P. Schilling, M. Schmanau, G. Schott, W. Schwerdtfeger, H.J. Simonis, A. Skiba, F.M. Stober,

A. Theel, W.H. Th ¨ummel, D. Troendle, A. Trunov, R. Ulrich, J. Wagner-Kuhr, S. Wayand,

M. Weber, T. Weiler, M. Zeise, E.B. Ziebarth, M. Zvada

Institute of Nuclear Physics ”Demokritos”, Aghia Paraskevi, Greece

G. Daskalakis, T. Geralis, S. Kesisoglou, A. Kyriakis, D. Loukas, I. Manolakos, A. Markou,

C. Markou, C. Mavrommatis, E. Ntomari

University of Athens, Athens, Greece

L. Gouskos, A. Panagiotou, N. Saoulidou

University of Io´annina, Io´annina, Greece

I. Evangelou, C. Foudas, P. Kokkas, N. Manthos, I. Papadopoulos, V. Patras

KFKI Research Institute for Particle and Nuclear Physics, Budapest, Hungary

G. Bencze, C. Hajdu, P. Hidas, D. Horvath18, F. Sikler, V. Veszpremi, G. Vesztergombi19, P. Zalan

Institute of Nuclear Research ATOMKI, Debrecen, Hungary

N. Beni, S. Czellar, A. Fenyvesi, J. Molnar, J. Palinkas, Z. Szillasi

University of Debrecen, Debrecen, Hungary

J. Karancsi, P. Raics, Z.L. Trocsanyi, B. Ujvari, G. Zilizi

Panjab University, Chandigarh, India

S.B.
Beri, V. Bhandari, V. Bhatnagar, N. Dhingra, R. Gupta, M. Kaur, J.M. Kohli, M.Z. Mehta,
N.
Nishu, L.K. Saini, A. Sharma, J.B. Singh

University of Delhi, Delhi, India

Ashok Kumar, Arun Kumar, S. Ahuja, A. Bhardwaj, S. Chatterji, B.C. Choudhary, P. Gupta,

A. Kumar, S. Malhotra, M. Naimuddin, K. Ranjan, V. Sharma, R.K. Shivpuri

Saha Institute of Nuclear Physics, Kolkata, India

S. Banerjee, S. Bhattacharya, S. Dutta, B. Gomber, Sa. Jain, Sh. Jain, R. Khurana, S. Sarkar,

M. Sharan

Bhabha Atomic Research Centre, Mumbai, India

A. Abdulsalam, R.K. Choudhury, D. Dutta, M. Ghodgaonkar, S. Kailas, S.K. Kataria, V. Kumar,

P. Mehta, A.K. Mohanty5, L.M. Pant, P. Shukla, A. Topkar

Tata Institute of Fundamental Research -EHEP, Mumbai, India

T. Aziz, R.M. Chatterjee, S. Chendvankar, P.V. Deshpande, S.N. Ganguli, S. Ganguly, S. Ghosh,

M. Guchait20, A. Gurtu21, G. Kole, M. Maity22, K. Mazumdar, G.B. Mohanty, B. Parida,

M.R. Patil, R. Raghavan, K. Sudhakar, N. Wickramage

Tata Institute of Fundamental Research -HECR, Mumbai, India

B.S. Acharya, S. Banerjee, S. Bheesette, S. Dugad, S.D. Kalmani, M.R. Krishnaswamy,

V.R. Lakkireddi, N.K. Mondal, V.S. Narasimham, N. Panyam, P. Verma

Institute for Research in Fundamental Sciences (IPM), Tehran, Iran

F. Ardalan, H. Arfaei23, H. Bakhshiansohi, S.M. Etesami24, A. Fahim23, M. Hashemi, A. Jafari,

M. Khakzad, M. Mohammadi Najafabadi, S. Paktinat Mehdiabadi, B. Safarzadeh25, M. Zeinali

INFN Sezione di Bari a, Universit`a di Bari b, Politecnico di Bari c, Bari, Italy

M. Abbresciaa,b, L. Barbonea,b, C. Calabriaa,b,5, S.S. Chhibraa,b, A. Colaleoa, D. Creanzaa,c ,

N. De Filippisa,c,5, M. De Palmaa,b , G. De Robertisa , G. Donvitoa , L. Fiorea , G. Iasellia,c ,

F. Loddoa , L. Lusitoa,b , G. Maggia,c , M. Maggia , N. Mannaa,b , B. Marangellia,b , S. Mya,c ,

S. Natalia,b, S. Nuzzoa,b, N. Pacificoa,b, A. Pompilia,b, G. Pugliesea,c, A. Ranieria, F. Romanoa,c ,

G. Selvaggia,b, L. Silvestrisa, G. Singha,b, V. Spinosoa, R. Vendittia,b, G. Zitoa

INFN Sezione di Bologna a, Universit`a di Bologna b, Bologna, Italy

G. Abbiendia, A.C. Benvenutia, D. Bonacorsia,b, S. Braibant-Giacomellia,b, L. Brigliadoria,b ,

P. Capiluppia,b , A. Castroa,b , F.R. Cavalloa , M. Cuffiania,b , G.M. Dallavallea , F. Fabbria ,

A. Fanfania,b , D. Fasanellaa,b,5, P. Giacomellia , C. Grandia , L. Guiduccia,b , S. Marcellinia ,

G. Masettia , M. Meneghellia,b,5, A. Montanaria , F.L. Navarriaa,b , F. Odoricia , A. Perrottaa ,

F. Primaveraa,b, A.M. Rossia,b, T. Rovellia,b, G. Sirolia,b, R. Travaglinia,b

INFN Sezione di Catania a, Universit`a di Catania b, Catania, Italy

S. Albergoa,b, G. Cappelloa,b, M. Chiorbolia,b, S. Costaa,b, F. Notoa, R. Potenzaa,b, M.A. Saizu,

A. Tricomia,b, C. Tuvea,b

INFN Sezione di Firenze a, Universit`a di Firenze b, Firenze, Italy

G. Barbaglia, V. Ciullia,b, C. Civininia, R. D’Alessandroa,b, E. Focardia,b, S. Frosalia,b, E. Galloa ,

C. Gentaa, S. Gonzia,b, M. Meschinia, S. Paolettia, G. Parrinia, R. Ranieria, G. Sguazzonia ,

A. Tropianoa,b

INFN Laboratori Nazionali di Frascati, Frascati, Italy

L. Benussi, S. Bianco, S. Colafranceschi26, F. Fabbri, D. Piccolo

INFN Sezione di Genova, Genova, Italy

P. Fabbricatore, S. Farinon, M. Greco, R. Musenich, S. Tosi

INFN Sezione di Milano-Bicocca a, Universit`a di Milano-Bicocca b, Milano, Italy

A. Benagliaa,b , L. Carbonea , P. D’Angeloa , F. De Guioa,b , L. Di Matteoa,b,5, P. Dinia ,

F.M.
Farinaa,b , S. Fiorendia,b , S. Gennaia,5, A. Ghezzia,b , S. Malvezzia , R.A. Manzonia,b ,
A.
Martellia,b , A. Massironia,b,5, D. Menascea , L. Moronia , P. Negria,b , M. Paganonia,b ,
D.
Pedrinia, A. Pulliaa,b, S. Ragazzia,b, N. Redaellia, S. Salaa, T. Tabarelli de Fatisa,b

INFN Sezione di Napoli a, Universit`a di Napoli ”Federico II” b, Napoli, Italy

S. Buontempoa , C.A. Carrillo Montoyaa , N. Cavalloa,27, A. De Cosaa,b,5, O. Doganguna,b ,

F. Fabozzia,27, A.O.M. Iorioa,b, L. Listaa, S. Meolaa,28, M. Merolaa,b, P. Paoluccia,5

INFN Sezione di Padova a, Universit`a di Padova b, Universit`a di Trento (Trento) c , Padova, Italy

P. Azzia, N. Bacchettaa,5, M. Bellatoa, M. Benettonia, M. Biasottoa,29, D. Biselloa,b, A. Brancaa,5,

R. Carlina,b , P. Checchiaa , T. Dorigoa , U. Dossellia , F. Gasparinia,b , U. Gasparinia,b ,

P. Giubilatoa,b, F. Gonellaa, A. Gozzelinoa, M. Gulminia,29, K. Kanishcheva,c, S. Lacapraraa ,

I. Lazzizzeraa,c, M. Loretia, M. Margonia,b, G. Marona,29, M. Mazzucatoa, A.T. Meneguzzoa,b ,

F. Montecassianoa, M. Passaseoa, J. Pazzinia,b, M. Pegoraroa, N. Pozzobona,b, P. Ronchesea,b ,

F. Simonettoa,b, E. Torassaa, M. Tosia,b,5, S. Vaninia,b, S. Venturaa, P. Zottoa,b, G. Zumerlea,b

INFN Sezione di Pavia a, Universit`a di Pavia b, Pavia, Italy

U. Berzanoa, M. Gabusia,b, S.P. Rattia,b, C. Riccardia,b, P. Torrea,b, P. Vituloa,b

INFN Sezione di Perugia a, Universit`a di Perugia b, Perugia, Italy oa,b

M. Biasinia,b , G.M. Bileia , L. Fan`, P. Laricciaa,b , A. Lucaronia,b,5, G. Mantovania,b ,

M. Menichellia, A. Nappia,b, D. Passeria,b, P. Placidia,b, F. Romeoa,b, A. Sahaa, A. Santocchiaa,b ,

L. Servolia, A. Spieziaa,b, S. Taronia,b, M. Valdataa,b

INFN Sezione di Pisa a, Universit`a di Pisa b, Scuola Normale Superiore di Pisa c, Pisa, Italy

F. Angelinia, S. Arezzinia, P. Azzurria,c, G. Bagliesia, A. Bastia, R. Bellazzinia, J. Bernardinia ,

T. Boccalia, F. Bosia, A. Breza, G. Broccoloa,c, F. Calzolaria, A. Carbonia, R. Castaldia, C. Cerria ,

A. Ciampaa, R.T. D’Agnoloa,c,5, R. Dell’Orsoa, F. Fioria,b,5, L. Fo`aa,c, A. Giassia, S. Giustia ,

A. Kraana, L. Latronicoa, F. Ligabuea,c, S. Linaria, T. Lomtadzea, L. Martinia,30, M. Massaa ,

M.M.
Massaia, E. Mazzonia, A. Messineoa,b, A. Moggia, F. Pallaa, F. Raffaellia, A. Rizzia,b ,
G.
Sanguinettia , G. Segneria , A.T. Serbana,31, P. Spagnoloa , G. Spandrea , P. Squillaciotia,5,
R.
Tenchinia, G. Tonellia,b, A. Venturia, P.G. Verdinia

INFN Sezione di Roma a, Universit`a di Roma ”La Sapienza” b, Roma, Italy

S. Baccaroa,32, L. Baronea,b, A. Bartolonia, F. Cavallaria, I. Dafineia, D. Del Rea,b, M. Diemoza , C. Fanelli, M. Grassia,b,5, E. Longoa,b , P. Meridiania,5, F. Michelia,b , S. Nourbakhsha,b ,

G. Organtinia,b, R. Paramattia, S. Rahatloua,b, M. Sigamania, L. Soffia,b, I.G. Talamoa

INFN Sezione di Torino a, Universit`a di Torino b, Universit`a del Piemonte Orientale (Novara) c, Torino, Italy

N. Amapanea,b , R. Arcidiaconoa,c , S. Argiroa,b , M. Arneodoa,c , C. Biinoa , N. Cartigliaa ,

M. Costaa,b, N. Demariaa, C. Mariottia,5, S. Masellia, E. Migliorea,b, V. Monacoa,b, M. Musicha,5,

M.M.
Obertinoa,c, N. Pastronea, M. Pelliccionia, C. Peronia,b, A. Potenzaa,b, A. Romeroa,b ,
M.
Ruspaa,c, R. Sacchia,b, A. Solanoa,b, A. Staianoa, A. Vilela Pereiraa

INFN Sezione di Trieste a, Universit`a di Trieste b, Trieste, Italy

F. Ambroglinia,b , S. Belfortea , V. Candelisea,b, M. Casarsaa , F. Cossuttia , G. Della Riccaa,b ,

B. Gobboa, C. Kavkaa, M. Maronea,b,5, D. Montaninoa,b,5, A. Penzoa, A. Schizzia,b

Kangwon National University, Chunchon, Korea

T.Y. Kim, S.K. Nam

Kyungpook National University, Daegu, Korea

K. Butanov, S. Chang, J. Chung, S.W. Ham, D. Han, J. Kang, D.H. Kim, G.N. Kim, J.E. Kim,

K.S. Kim, D.J. Kong, M.W. Lee, S. Lee, Y.D. Oh, H. Park, S.R. Ro, D. Son, D.C. Son, J.S. Suh,

Y.C. Yang, H. Yusupov

Chonnam National University, Institute for Universe and Elementary Particles, Kwangju, Korea

J.Y. Kim, Zero J. Kim, S. Song

Korea University, Seoul, Korea

S. Choi, D. Gyun, B. Hong, M. Jo, Y. Jo, M. Kang, H. Kim, T.J. Kim, K.S. Lee, D.H. Moon,

S.K. Park, K.S. Sim

University of Seoul, Seoul, Korea

M. Choi, G. Hahn, S. Kang, H. Kim, J.H. Kim, C. Park, I.C. Park, S. Park, G. Ryu

Sungkyunkwan University, Suwon, Korea

Y. Choi, Y.K. Choi, J. Goh, M.S. Kim, E. Kwon, B. Lee, J. Lee, S. Lee, H. Seo, I. Yu

Vilnius University, Vilnius, Lithuania

M. Janulis, A. Juodagalvis, R. Naujikas

Centro de Investigacion y de Estudios Avanzados del IPN, Mexico City, Mexico

H. Castilla-Valdez, E. De La Cruz-Burelo, I. Heredia-de La Cruz, R. Lopez-Fernandez,

R. Maga˜na Villalba, J. Mart´ınez-Ortega, A. S´anchez-Hern´andez, L.M. Villasenor-Cendejas

Universidad Iberoamericana, Mexico City, Mexico

S. Carrillo Moreno, F. Vazquez Valencia

Benemerita Universidad Autonoma de Puebla, Puebla, Mexico

H.A. Salazar Ibarguen

Universidad Aut´onoma de San Luis Potos´ı, San Luis Potos´ı, Mexico

E. Casimiro Linares, A. Morelos Pineda, M.A. Reyes-Santos

University of Auckland, Auckland, New Zealand

P. Allfrey, D. Krofcheck

University of Canterbury, Christchurch, New Zealand

A.J.
Bell, N. Bernardino Rodrigues, A.P.H. Butler, P.H. Butler, R. Doesburg, D. Pfeiffer,
S.
Reucroft, H. Silverwood, J.C. Williams

National Centre for Physics, Quaid-I-Azam University, Islamabad, Pakistan

M. Ahmad, M.H. Ansari, M.I. Asghar, H.R. Hoorani, S. Khalid, W.A. Khan, T. Khurshid, S. Qazi,

M.A. Shah, M. Shoaib

Institute of Experimental Physics, Faculty of Physics, University of Warsaw, Warsaw, Poland

G. Brona, K. Bunkowski, M. Cwiok, H. Czyrkowski, R. Dabrowski, W. Dominik, K. Doroba,

A. Kalinowski, M. Konecki, J. Krolikowski, W. Oklinski, K. Pozniak33, W. Zabolotny33, P. Zych

Soltan Institute for Nuclear Studies, Warsaw, Poland

H. Bialkowska, B. Boimska, T. Frueboes, R. Gokieli, L. Goscilo, M. G´orski, M. Kazana,

I.M. Kudla, K. Nawrocki, K. Romanowska-Rybinska, M. Szleper, G. Wrochna, P. Zalewski

Warsaw University of Technology, Institute of Electronic Systems, Warsaw, Poland

G. Kasprowicz, R. Romaniuk

Laborat´orio de Instrumenta¸c˜ao e F´ısica Experimental de Part´ıculas, Lisboa, Portugal

R. Alemany-Fernandez, N. Almeida, P. Bargassa, A. David, P. Faccioli, P.G. Ferreira Parracho,

M. Gallinaro, P.Q. Ribeiro, J. Seixas, J. Silva, J. Varela, P. Vischia

Joint Institute for Nuclear Research, Dubna, Russia

S. Afanasiev, I. Belotelov, P. Bunin, Y. Ershov, M. Gavrilenko, A. Golunov, I. Golutvin,

N. Gorbounov, I. Gorbunov, I. Gramenitski, V. Kalagin, A. Kamenev, V. Karjavin,

V. Konoplyanikov, V. Korenkov, G. Kozlov, A. Kurenkov, A. Lanev, A. Makankin, A. Malakhov,

I. Melnitchenko, V.V. Mitsyn, P. Moisenz, D. Oleynik, A. Orlov, V. Palichik, V. Perelygin,

A. Petrosyan, M. Savina, R. Semenov, S. Shmatov, S. Shulha, A. Skachkova, N. Skatchkov,

V. Smetannikov, V. Smirnov, D. Smolin, E. Tikhonenko, S. Vasil’ev, A. Volodko, A. Zarubin,

V. Zhiltsov

Petersburg Nuclear Physics Institute, Gatchina (St Petersburg), Russia

S. Evstyukhin, V. Golovtsov, Y. Ivanov, V. Kim, P. Levchenko, V. Murzin, V. Oreshkin, I. Smirnov,

V. Sulimov, L. Uvarov, S. Vavilov, A. Vorobyev, An. Vorobyev

High Temperature Technology Center of Research & Development Institute of Power Engineering (HTTC RDIPE), Moscow, Russia

Institute for Nuclear Research, Moscow, Russia

Yu. Andreev, A. Anisimov, A. Dermenev, S. Gninenko, N. Golubev, D. Gorbunov, A. Karneyeu,

M. Kirsanov, N. Krasnikov, V. Matveev, A. Pashenkov, G. Pivovarov, V.E. Postoev, V. Rubakov,

V. Shirinyants, A. Solovey, D. Tlisov, A. Toropin, S. Troitsky

Institute for Theoretical and Experimental Physics, Moscow, Russia

V. Epshteyn, M. Erofeeva, V. Gavrilov, V. Kaftanov, I. Kiselevich, V. Kolosov, A. Konoplyannikov, M. Kossov, Y. Kozlov, A. Krokhotin, D. Litvintsev, N. Lychkovskaya, A. Oulianov,

V. Popov, G. Safronov, S. Semenov, N. Stepanov, V. Stolin, E. Vlasov, V. Zaytsev, A. Zhokin

Moscow State University, Moscow, Russia

A. Belyaev, E. Boos, V. Bunichev, A. Demiyanov, M. Dubinin4, L. Dudko, A. Ershov,

A. Gribushin, V. Ilyin, A. Kaminskiy34, V. Klyukhin, O. Kodolova, V. Korotkikh, A. Kryukov,

I. Lokhtin, A. Markina, S. Obraztsov, M. Perfilov, S. Petrushanko, A. Popov, A. Proskuryakov,

L. Sarycheva, V. Savrin, A. Snigirev, I. Vardanyan

P.N. Lebedev Physical Institute, Moscow, Russia

V. Andreev, M. Azarkin, I. Dremin, M. Kirakosyan, A. Leonidov, G. Mesyats, S.V. Rusakov,

A. Vinogradov

State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, Russia

I. Azhgirey, I. Bayshev, S. Bitioukov, V. Grishin5, V. Kachanov, A. Kalinin, D. Konstantinov,

A. Korablev, V. Krychkine, A. Levine, V. Petrov, A. Ryabov, R. Ryutin, A. Sobol, V. Talov,

L. Tourtchanovitch, S. Troshin, N. Tyurin, A. Uzunian, A. Volkov

University of Belgrade, Faculty of Physics and Vinca Institute of Nuclear Sciences, Belgrade, Serbia

P. Adzic35, M. Djordjevic, M. Ekmedzic, D. Krpic35, J. Milosevic, N. Smiljkovic, M. Zupan

Centro de Investigaciones Energ´eticas Medioambientales y Tecnol´ogicas (CIEMAT), Madrid, Spain

M. Aguilar-Benitez, J. Alcaraz Maestre, P. Arce, C. Battilana, E. Calvo, M. Cerrada, M. Chamizo Llatas, N. Colino, B. De La Cruz, A. Delgado Peris, D. Dom´ınguez V´azquez, C. Fernandez Bedoya, J.P. Fern´

andez Ramos, A. Ferrando, J. Flix, M.C. Fouz, P. Garcia-Abia, O. Gonzalez Lopez, S. Goy Lopez, J.M. Hernandez, M.I. Josa, G. Merino, J. Puerta Pelayo, A. Quintario Olmeda, I. Redondo, L. Romero, J. Santaolalla, M.S. Soares, C. Willmott

Universidad Aut´onoma de Madrid, Madrid, Spain

C. Albajar, G. Codispoti, J.F. de Troc´oniz

Universidad de Oviedo, Oviedo, Spain

H. Brun, J. Cuevas, J. Fernandez Menendez, S. Folgueras, I. Gonzalez Caballero, L. Lloret Iglesias, J. Piedra Gomez

Instituto de F´ısica de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander, Spain

J.A.
Brochero Cifuentes, I.J. Cabrillo, A. Calderon, S.H. Chuang, J. Duarte Campderros,
M.
Felcini36, M. Fernandez, G. Gomez, J. Gonzalez Sanchez, A. Graziano, C. Jorda, A. Lopez Virto, J. Marco, R. Marco, C. Martinez Rivero, F. Matorras, F.J. Munoz Sanchez, T. Rodrigo,

A.Y. Rodr´ıguez-Marrero, A. Ruiz-Jimeno, L. Scodellaro, M. Sobron Sanudo, I. Vila, R. Vilar Cortabitarte

CERN, European Organization for Nuclear Research, Geneva, Switzerland

D. Abbaneo, P. Aspell, E. Auffray, G. Auzinger, M. Bachtis, J. Baechler, P. Baillon, A.H. Ball,

D. Barney, J.F. Benitez, C. Bernet6, W. Bialas, G. Bianchi, P. Bloch, A. Bocci, A. Bonato, C. Botta,

H. Breuker, D. Campi, T. Camporesi, E. Cano, G. Cerminara, A. Charkiewicz, T. Christiansen,

J.A.
Coarasa Perez, B. Cur´e, D. D’Enterria, A. Dabrowski, J. Daguin, A. De Roeck, S. Di Guida,
M.
Dobson, N. Dupont-Sagorin, A. Elliott-Peisert, M. Eppard, B. Frisch, W. Funk, A. Gaddi,
M.
Gastal, G. Georgiou, H. Gerwig, M. Giffels, D. Gigi, K. Gill, D. Giordano, M. Girone,
M.
Giunta, F. Glege, R. Gomez-Reino Garrido, P. Govoni, S. Gowdy, R. Guida, J. Gutleber,
M.
Hansen, P. Harris, C. Hartl, J. Harvey, B. Hegner, A. Hinzmann, A. Honma, V. Innocente,
P.
Janot, K. Kaadze, E. Karavakis, K. Kloukinas, K. Kousouris, P. Lecoq, Y.-J. Lee, P. Lenzi,
R.
Loos, C. Lourenc¸o, N. Magini, T. M¨aki, M. Malberti, L. Malgeri, M. Mannelli, A. Marchioro,
J.
Marques Pinho Noite, L. Masetti, F. Meijers, S. Mersi, E. Meschi, L. Moneta, M.U. Mozer,
M.
Mulders, P. Musella, A. Onnela, T. Orimoto, L. Orsini, J.A. Osborne, E. Palencia Cortezon,
E.
Perez, L. Perrozzi, P. Petagna, A. Petrilli, A. Petrucci, A. Pfeiffer, M. Pierini, M. Pimia,¨
D.
Piparo, G. Polese, H. Postema, L. Quertenmont, A. Racz, W. Reece, D. Ricci, J. Rodrigues Antunes, G. Rolandi37, C. Rovelli38, M. Rovere, V. Ryjov, H. Sakulin, D. Samyn, F. Santanastasio,
C.
Sch¨afer, C. Schwick, A. Sciaba, I. Segoni, S. Sekmen, A. Sharma, P. Siegrist, P. Silva, M. Simon,
P.
Sphicas39, D. Spiga, B.G. Taylor, P. Tropea, J. Troska, A. Tsirou, F. Vasey, L. Veillet, G.I. Veres19,
P.
Vichoudis, J.R. Vlimant, P. Wertelaers, H.K. W¨ohri, S.D. Worm40, W.D. Zeuner

Paul Scherrer Institut, Villigen, Switzerland

W. Bertl, K. Deiters, W. Erdmann, D. Feichtinger, K. Gabathuler, R. Horisberger, Q. Ingram,

H.C.
Kaestli, S. K¨onig, D. Kotlinski, U. Langenegger, B. Meier, F. Meier, D. Renker, T. Rohe,
T.
Sakhelashvili41, J. Sibille42

Institute for Particle Physics, ETH Zurich, Zurich, Switzerland

L. ani, F.Behner, B. Betev, B. Blau, P.Bortignon, M.A.Buchmann, B.Casal, N.Chanon, Z.Chen,

D.R.
Da Silva Di Calafiori, S. Dambach43, G. Davatz, A. Deisher, G. Dissertori, M. Dittmar,
L.
Djambazov, M. Doneg`a, M. D ¨

unser, C. Eggel43, J. Eugster, G. Faber, K. Freudenreich, C. Grab,

W. Hintz, D. Hits, H. Hofer, O. Holme, I. Horvath, P. Lecomte, W. Lustermann, C. Marchica43,

A.C.
Marini, P. Martinez Ruiz del Arbol, N. Mohr, F. Moortgat, C. N¨ageli43, P. Nef, F. Nessi-Tedaldi, F. Pandolfi, L. Pape, F. Pauss, M. Peruzzi, T. Punz, F.J. Ronga, U. R¨oser, M. Rossini,
L.
Sala, A.K. Sanchez, M.-C. Sawley, D. Schinzel, A. Starodumov44, B. Stieger, H. Suter,
M.
Takahashi, L. Tauscher, A. Thea, K. Theofilatos, D. Treille, P. Tr ¨

ub43, S. Udriot, C. Urscheler,

G. Viertel, H.P. von Gunten, R. Wallny, H.A. Weber, L. Wehrli, J. Weng, S. Zelepoukine45

Universit¨atZ¨urich,Zurich, Switzerland

C. Amsler, V. Chiochia, S. De Visscher, C. Favaro, M. Ivova Rikova, B. Millan Mejias,

P. Otiougova, P. Robmann, H. Snoek, S. Tupputi, M. Verzetti

National Central University, Chung-Li, Taiwan

Y.H.
Chang, K.H. Chen, W.T. Chen, A. Go, C.M. Kuo, S.W. Li, W. Lin, M.H. Liu, Z.K. Liu, Y.J. Lu,
D.
Mekterovic, A.P. Singh, R. Volpe, J.H. Wu, S.S. Yu

National Taiwan University (NTU), Taipei, Taiwan

P. Bartalini, P. Chang, Y.H. Chang, Y.W. Chang, Y. Chao, K.F. Chen, C. Dietz, Z. Gao5,

U. Grundler, W.-S. Hou, Y. Hsiung, K.Y. Kao, Y.J. Lei, J.j. Liau, S.W. Lin, R.-S. Lu, D. Majumder,

E. Petrakou, X. Shi, J.G. Shiu, Y.M. Tzeng, K. Ueno, Y. Velikzhanin, X. Wan, C.C. Wang,

M. Wang, J.T. Wei, P. Yeh

Chulalongkorn University, Bangkok, Thailand

B. Asavapibhop, E. Simili, N. Srimanobhas

Cukurova University, Adana, Turkey

A. Adiguzel, M.N. Bakirci46, S. Cerci47, C. Dozen, I. Dumanoglu, E. Eskut, S. Girgis,

G. Gokbulut, E. Gurpinar, I. Hos, E.E. Kangal, T. Karaman, G. Karapinar48, A. Kayis Topaksu,

G. Onengut, K. Ozdemir, S. Ozturk49, A. Polatoz, K. Sogut50, D. Sunar Cerci47, B. Tali47,

H. Topakli46, L.N. Vergili, M. Vergili

Middle East Technical University, Physics Department, Ankara, Turkey

I.V.
Akin, T. Aliev, B. Bilin, M. Deniz, H. Gamsizkan, A.M. Guler, K. Ocalan, A. Ozpineci,
M.
Serin, R. Sever, U.E. Surat, M. Zeyrek

Bogazici University, Istanbul, Turkey

M. Deliomeroglu, E. G ¨ulmez, B. Isildak51, M. Kaya52, O. Kaya52, S. Ozkorucuklu53, N. Sonmez54

Istanbul Technical University, Istanbul, Turkey

K. Cankocak

Institute of Single Crystals of National Academy of Science, Kharkov, Ukraine

B. Grynyov

National Scientific Center, Kharkov Institute of Physics and Technology, Kharkov, Ukraine

L. Levchuk, S. Lukyanenko, D. Soroka, P. Sorokin

Centre for Complex Cooperative Systems, University of the West of England, Bristol, United Kingdom

M.K.H. Ahmad, A. Branson, R. McClatchey, M. Odeh, J. Shamdasani, K. Soomro

University of Bristol, Bristol, United Kingdom

T. Barrass, F. Bostock, J.J. Brooke, E. Clement, D. Cussans, H. Flacher, R. Frazier, J. Goldstein,

M. Grimes, G.P. Heath, H.F. Heath, L. Kreczko, W. Lacesso, S. Metson, D.M. Newbold40,

K. Nirunpong, A. Poll, S. Senkin, V.J. Smith, T. Williams

Rutherford Appleton Laboratory, Didcot, United Kingdom

L. Basso55, E. Bateman, K.W. Bell, A. Belyaev55, C. Brew, R.M. Brown, B. Camanzi,

D.J.A. Cockerill, J.F. Connolly, J.A. Coughlan, L.G. Denton, P.S. Flower, M.J. French,

R.J.S. Greenhalgh, R.N.J. Halsall, K. Harder, S. Harper, J.A. Hill, J. Jackson, B.W. Kennedy,

A.L. Lintern, A.B. Lodge, E. Olaiya, M.R. Pearson, D. Petyt, B.C. Radburn-Smith,

C.H. Shepherd-Themistocleous, B.J. Smith, M. Sproston, R. Stephenson, I.R. Tomalin,

M.J. Torbet, J.H. Williams, W.J. Womersley

Imperial College, London, United Kingdom

R. Bainbridge, G. Ball, J. Ballin, D. Bauer, R. Beuselinck, O. Buchmuller, D. Colling, N. Cripps,

M. Cutajar, P. Dauncey, G. Davies, M. Della Negra, S. Fayer, W. Ferguson, J. Fulcher, D. Futyan,

A. Gilbert, A. Guneratne Bryer, G. Hall, Z. Hatherell, J. Hays, G. Iles, M. Jarvis, J. Jones,

G. Karapostoli, M. Kenzie, J. Leaver, L. Lyons, A.-M. Magnan, J. Marrouche, B. Mathias,

D.G.
Miller, R. Nandi, J. Nash, A. Nikitenko44, M. Noy, A. Papageorgiou, J. Pela, M. Pesaresi,
K.
Petridis, M. Pioppi56, D. Rand, D.M. Raymond, S. Rogerson, A. Rose, M.J. Ryan, C. Seez,
P.
Sharp, A. Sparrow, M. Stoye, A. Tapper, C. Timlin, S. Tourneur, M. Vazquez Acosta,
T.
Virdee, S. Wakefield, N. Wardle, T. Whyntie, M. Wingham, O. Zorba

Brunel University, Uxbridge, United Kingdom

M. Chadwick, J.E. Cole, P.R. Hobson, A. Khan, P. Kyberd, D. Leggat, D. Leslie, W. Martin,

I.D. Reid, P. Symonds, L. Teodorescu, M. Turner

Baylor University, Waco, USA

J. Dittmann, K. Hatakeyama, H. Liu, T. Scarborough

The University of Alabama, Tuscaloosa, USA

O. Charaf, C. Henderson, P. Rumerio

Boston University, Boston, USA

A. Avetisyan, T. Bose, E. Carrera Jarrin, C. Fantasia, E. Hazen, A. Heister, J. St. John, P. Lawson,

D. Lazic, J. Rohlf, D. Sperka, L. Sulak, F. Varela Rodriguez, S. Wu

Brown University, Providence, USA

J. Alimena, S. Bhattacharya, D. Cutts, Z. Demiragli, A. Ferapontov, A. Garabedian, U. Heintz,

R. Hooper, S. Jabeen, G. Kukartsev, E. Laird, G. Landsberg, M. Luk, M. Narain, D. Nguyen,

M. Segala, T. Sinthuprasith, T. Speer, K.V. Tsang, Z. Unalan

University of California, Davis, Davis, USA

R. Breedon, G. Breto, M. Calderon De La Barca Sanchez, M. Case, S. Chauhan, M. Chertok,

J. Conway, R. Conway, P.T. Cox, J. Dolen, R. Erbacher, M. Gardner, G. Grim, J. Gunion,

B. Holbrook, W. Ko, A. Kopecky, R. Lander, F.C. Lin, T. Miceli, P. Murray, M. Nikolic, D. Pellett, F. Ricci-tam, J. Rowe, B. Rutherford, M. Searle, J. Smith, M. Squires, M. Tripathi, R. Vasquez Sierra, R. Yohay

University of California, Los Angeles, Los Angeles, USA

V. Andreev, K. Arisaka, D. Cline, R. Cousins, J. Duris, S. Erhan, P. Everaerts, C. Farrell, J. Hauser,

M. Ignatenko, C. Jarvis, J. Kubic, S. Otwinowski, C. Plager, G. Rakness, P. Schlein, P. Traczyk,

V. Valuev, M. Weber, X. Yang, Y. Zheng

University of California, Riverside, Riverside, USA

J. Babb, R. Clare, M.E. Dinardo, J. Ellison, J.W. Gary, F. Giordano, G. Hanson, J.G. Layter, H. Liu,

O.R.
Long, A. Luthra, H. Nguyen, S. Paramesvaran, B.C. Shen, J. Sturdy, S. Sumowidagdo,
R.
Wilken, S. Wimpenny

University of California, San Diego, La Jolla, USA

W. Andrews, J.G. Branson, G.B. Cerati, S. Cittolin, D. Evans, F. Golf, A. Holzner, R. Kelley,

M. Lebourgeois, J. Letts, I. Macneill, B. Mangano, T. Martin, A. Mrak-Tadel, S. Padhi, C. Palmer,

G. Petrucciani, M. Pieri, M. Sani, I. Sfiligoi, V. Sharma, S. Simon, E. Sudano, M. Tadel, Y. Tu,

A. Vartak, S. Wasserbaech57, F. W ¨

urthwein, A. Yagil, J. Yoo

University of California, Santa Barbara, Santa Barbara, USA

D. Barge, R. Bellan, C. Campagnari, M. D’Alfonso, T. Danielson, K. Flowers, P. Geffert,

J. Incandela, C. Justus, P. Kalavase, S.A. Koay, D. Kovalskyi, V. Krutelyov, S. Kyre, S. Lowette,

G. Magazzu, N. Mccoll, V. Pavlunin, F. Rebassoo, J. Ribnik, J. Richman, R. Rossin, D. Stuart,

W. To, C. West, D. White

California Institute of Technology, Pasadena, USA

D. Adamczyk, A. Apresyan, A. Barczyk, A. Bornheim, J. Bunn, Y. Chen, G. Denis, E. Di Marco,

J. Duarte, P. Galvez, M. Gataullin, D. Kcira, I. Legrand, V. Litvine, Y. Ma, Z. Maxa, A. Mott,

A. Mughal, D. Nae, H.B. Newman, S. Ravot, C. Rogan, S.G. Rozsa, S. Shevchenko, K. Shin,

M. Spiropulu, C. Steenberg, M. Thomas, V. Timciuc, F. van Lingen, J. Veverka, B.R. Voicu,

R. Wilkinson, S. Xie, Y. Yang, L. Zhang, K. Zhu, R.Y. Zhu

Carnegie Mellon University, Pittsburgh, USA

B. Akgun, V. Azzolini, A. Calamba, R. Carroll, T. Ferguson, Y. Iiyama, D.W. Jang, S.Y. Jun,

Y.F. Liu, M. Paulini, J. Russ, N. Terentyev, H. Vogel, I. Vorobiev

University of Colorado at Boulder, Boulder, USA

J.P.
Cumalat, B.R. Drell, W.T. Ford, A. Gaz, B. Heyburn, D. Johnson, E. Luiggi Lopez,
U.
Nauenberg, J.G. Smith, K. Stenson, K.A. Ulmer, S.R. Wagner, S.L. Zang

Cornell University, Ithaca, USA

L. Agostino, J. Alexander, A. Chatterjee, N. Eggert, L.K. Gibbons, B. Heltsley, A. Khukhunaishvili, B. Kreis, V. Kuznetsov, N. Mirman, G. Nicolas Kaufman, J.R. Patterson, D. Riley,

A. Ryd, E. Salvati, S. Stroiney, W. Sun, W.D. Teo, J. Thom, J. Thompson, J. Tucker, J. Vaughan,

Y. Weng, L. Winstrom, P. Wittich

Fairfield University, Fairfield, USA

D. Winn

Fermi National Accelerator Laboratory, Batavia, USA

S. Abdullin, M. Albert, M. Albrow, J. Anderson, G. Apollinari, M. Atac, W. Badgett,

J.A.
Bakken, B. Baldin, K. Banicz, L.A.T. Bauerdick, A. Beretvas, J. Berryhill, P.C. Bhat,
M.
Binkley, F. Borcherding, K. Burkett, J.N. Butler, V. Chetluru, H.W.K. Cheung, F. Chlebana,
S.
Cihangir, W. Dagenhart, G. Derylo, C. Dumitrescu, D. Dykstra, D.P. Eartly, J.E. Elias,

V.D. Elvira, G. Eulisse, D. Evans, D. Fagan, I. Fisk, S. Foulkes, J. Freeman, I. Gaines, Y. Gao, P. Gartung, L. Giacchetti, E. Gottschalk, D. Green, Y. Guo, O. Gutsche, A. Hahn, J. Hanlon, R.M. Harris, J. Hirschauer, B. Holzman, B. Hooberman, J. Howell, C.h. Huang, D. Hufnagel, S. Jindariani, M. Johnson, C.D. Jones, U. Joshi, E. Juska, B. Kilminster, B. Klima, S. Kunori, S. Kwan, K. Larson, C. Leonidopoulos, J. Linacre, D. Lincoln, R. Lipton, J.A. Lopez Perez, S. Los, J. Lykken, K. Maeshima, J.M. Marraffino, S. Maruyama, D. Mason, P. McBride, T. McCauley, K. Mishra, S. Moccia, R.K. Mommsen, S. Mrenna, Y. Musienko58, S. Muzaffar, C. Newman-Holmes, V. O’Dell, I. Osborne, J. Pivarski, S. Popescu59, R. Pordes, O. Prokofyev, V. Rapsevicius, A. Ronzhin, P. Rossman, S. Ryu, E. Sexton-Kennedy, S. Sharma, T.M. Shaw, R.P. Smith, A. Soha,

W.J. Spalding, L. Spiegel, W. Tanenbaum, L. Taylor, R. Thompson, A. Tiradani, S. Tkaczyk,

N.V.
Tran, L. Tuura, L. Uplegger, E.W. Vaandering, R. Vidal, J. Whitmore, W. Wu, F. Yang,
J.
Yarba, F. Yumiceva, J.C. Yun, T. Zimmerman

University of Florida, Gainesville, USA

D. Acosta, P. Avery, V. Barashko, D. Bourilkov, M. Chen, T. Cheng, S. Das, M. De Gruttola,

G.P.
Di Giovanni, D. Dobur, S. Dolinsky, A. Drozdetskiy, R.D. Field, M. Fisher, Y. Fu, I.K. Furic,
J.
Gartner, L. Gorn, D. Holmes, J. Hugon, B. Kim, J. Konigsberg, A. Korytov, A. Kropivnitskaya,
T.
Kypreos, J.F. Low, A. Madorsky, K. Matchev, P. Milenovic60, G. Mitselmakher, L. Muniz,
M.
Park, R. Remington, A. Rinkevicius, B. Scurlock, N. Skhirtladze, M. Snowball, J. Stasko,
J.
Yelton, M. Zakaria

Florida International University, Miami, USA

V. Gaultney, S. Hewamanage, L.M. Lebolo, S. Linn, P. Markowitz, G. Martinez, J.L. Rodriguez

Florida State University, Tallahassee, USA

T. Adams, A. Askew, M. Bertoldi, J. Bochenek, J. Chen, W.G.D. Dharmaratna, B. Diamond,

S.V.
Gleyzer, J. Haas, S. Hagopian, V. Hagopian, M. Jenkins, K.F. Johnson, H. Prosper,
S.
Tentindo, V. Veeraraghavan, M. Weinberg

Florida Institute of Technology, Melbourne, USA

M.M. Baarmand, B. Dorney, M. Hohlmann, H. Kalakhety, R. Ralich, I. Vodopiyanov

University of Illinois at Chicago (UIC), Chicago, USA

M.R.
Adams, I.M. Anghel, L. Apanasevich, Y. Bai, V.E. Bazterra, R.R. Betts, I. Bucinskaite,
J.
Callner, R. Cavanaugh, M.H. Chung, O. Evdokimov, E.J. Garcia-Solis, L. Gauthier,
C.E.
Gerber, D.J. Hofman, R. Hollis, A. Iordanova, S. Khalatyan, G.J. Kunde61, F. Lacroix,
M.
Malek, C. O’Brien, C. Silkworth, C. Silvestre, A. Smoron, D. Strom, P. Turner, N. Varelas

The University of Iowa, Iowa City, USA

U. Akgun, E.A. Albayrak, A.S. Ayan, B. Bilki62, W. Clarida, P. Debbins, F. Duru, F.D. Ingram,

E. McCliment, J.-P. Merlo, H. Mermerkaya63, A. Mestvirishvili, M.J. Miller, A. Moeller,

J. Nachtman, C.R. Newsom, E. Norbeck, J. Olson, Y. Onel, F. Ozok64, I. Schmidt, S. Sen, P. Tan,

E. Tiras, J. Wetzel, T. Yetkin, K. Yi

Johns Hopkins University, Baltimore, USA

B.A.
Barnett, B. Blumenfeld, S. Bolognesi, D. Fehling, G. Giurgiu, A.V. Gritsan, Z.J. Guo, G. Hu,
P.
Maksimovic, S. Rappoccio, M. Swartz, A. Whitbeck

The University of Kansas, Lawrence, USA

P. Baringer, A. Bean, G. Benelli, D. Coppage, O. Grachov, R.P. Kenny Iii, M. Murray, D. Noonan,

V. Radicci, S. Sanders, R. Stringer, G. Tinti, J.S. Wood, V. Zhukova

Kansas State University, Manhattan, USA

A.F.
Barfuss, T. Bolton, I. Chakaberia, A. Ivanov, S. Khalil, M. Makouski, Y. Maravin, S. Shrestha,
I.
Svintradze

Lawrence Livermore National Laboratory, Livermore, USA

J. Gronberg, D. Lange, D. Wright

University of Maryland, College Park, USA

A. Baden, R. Bard, M. Boutemeur, B. Calvert, S.C. Eno, J.A. Gomez, T. Grassi, N.J. Hadley,

R.G.
Kellogg, M. Kirn, T. Kolberg, Y. Lu, M. Marionneau, A.C. Mignerey, K. Pedro, A. Peterman,
K.
Rossato, A. Skuja, J. Temple, M.B. Tonjes, S.C. Tonwar, T. Toole, E. Twedt

Massachusetts Institute of Technology, Cambridge, USA

A. Apyan, G. Bauer, J. Bendavid, W. Busza, E. Butz, I.A. Cali, M. Chan, V. Dutta, G. Gomez Ceballos, M. Goncharov, K.A. Hahn, Y. Kim, M. Klute, K. Krajczar65, A. Levin, P.D. Luckey,

T.Ma,
S.Nahn, C.Paus, D. Ralph, C.Roland, G.Roland, M. Rudolph, G.S.F. Stephans, F. St¨ockli,
K.
Sumorok, K. Sung, D. Velicanu, E.A. Wenger, R. Wolf, B. Wyslouch, M. Yang, Y. Yilmaz,

A.S. Yoon, M. Zanetti

University of Minnesota, Minneapolis, USA

D. Bailleux, S.I. Cooper, P. Cushman, B. Dahmes, A. De Benedetti, R. Egeland, G. Franzoni,

A. Gude, J. Haupt, A. Inyakin, S.C. Kao, K. Klapoetke, Y. Kubota, J. Mans, N. Pastika, R. Rusack,

A. Singovsky, N. Tambe, J. Turkewitz

University of Mississippi, University, USA

L.M. Cremaldi, R. Kroeger, L. Perera, R. Rahmat, J. Reidy, D.A. Sanders, D. Summers

University of Nebraska-Lincoln, Lincoln, USA

G. Attebury, E. Avdeeva, K. Bloom, B. Bockelman, S. Bose, J. Butt, D.R. Claes, A. Dominguez,

M. Eads, J. Keller, I. Kravchenko, J. Lazo-Flores, C. Lundstedt, H. Malbouisson, S. Malik,

R. Snihur, G.R. Snow, D. Swanson

State University of New York at Buffalo, Buffalo, USA

U. Baur, A. Godshalk, I. Iashvili, S. Jain, A. Kharchilava, A. Kumar, S.P. Shipkowski, K. Smith

Northeastern University, Boston, USA

G. Alverson, E. Barberis, D. Baumgartel, M. Chasco, J. Haley, J. Moromisato, D. Nash, J. Swain,

D. Trocino, E. Von Goeler, D. Wood, J. Zhang

Northwestern University, Evanston, USA

A. Anastassov, B. Gobbi, A. Kubik, N. Odell, R.A. Ofierzynski, B. Pollack, A. Pozdnyakov,

M. Schmitt, S. Stoynev, M. Velasco, S. Won

University of Notre Dame, Notre Dame, USA

L. Antonelli, B. Baumbaugh, D. Berry, A. Brinkerhoff, K.M. Chan, A.H. Heering, M. Hildreth,

C. Jessop, D.J. Karmgard, N. Kellams, J. Kolb, K. Lannon, W. Luo, S. Lynch, N. Marinelli,

D.M.
Morse, T. Pearson, M. Planer, R. Ruchti, J. Slaunwhite, N. Valls, M. Wayne, M. Wolf,
A.
Woodard

The Ohio State University, Columbus, USA

B. Bylsma, L.S. Durkin, C. Hill, R. Hughes, K. Kotov, T.Y. Ling, D. Puigh, M. Rodenburg,

C.J. Rush, V. Sehgal, C. Vuosalo, G. Williams, B.L. Winer

Princeton University, Princeton, USA

N. Adam, E. Berry, P. Elmer, D. Gerbaudo, V. Halyo, P. Hebda, J. Hegeman, A. Hunt, P. Jindal, D. Lopes Pegna, P. Lujan, D. Marlow, T. Medvedeva, M. Mooney, J. Olsen, P. Pirou´

e, X. Quan,

A. Raval, H. Saka, D. Stickland, C. Tully, J.S. Werner, T. Wildish, Z. Xie, S.C. Zenz, A. Zuranski

University of Puerto Rico, Mayaguez, USA

J.G.
Acosta, M. Bonnett Del Alamo, E. Brownson, X.T. Huang, A. Lopez, H. Mendez,
S.
Oliveros, J.E. Ramirez Vargas, A. Zatserklyaniy

Purdue University, West Lafayette, USA

E. Alagoz, K. Arndt, V.E. Barnes, D. Benedetti, G. Bolla, D. Bortoletto, A. Bujak, M. De Mattia,

A. Everett, L. Gutay, Z. Hu, M. Jones, O. Koybasi, M. Kress, A.T. Laasanen, J. Lee, N. Leonardo,

C. Liu, V. Maroussov, P. Merkel, D.H. Miller, J. Miyamoto, N. Neumeister, C. Rott, A. Roy,

I. Shipsey, D. Silvers, A. Svyatkovskiy, M. Vidal Marono, H.D. Yoo, J. Zablocki, Y. Zheng

Purdue University Calumet, Hammond, USA

S. Guragain, N. Parashar

Rice University, Houston, USA

A. Adair, C. Boulahouache, V. Cuplov, K.M. Ecklund, F.J.M. Geurts, S.J. Lee, W. Li, J.H. Liu,

M. Matveev, B.P. Padley, R. Redjimi, J. Roberts, A. Tumanov, P. Yepes, J. Zabel

University of Rochester, Rochester, USA

B. Betchart, A. Bodek, H. Budd, Y.S. Chung, R. Covarelli, P. de Barbaro, R. Demina,

Y. Eshaq, T. Ferbel, A. Garcia-Bellido, G. Ginther, P. Goldenzweig, Y. Gotra, J. Han, A. Harel,

S. Korjenevski, D.C. Miner, D. Orbaker, W. Sakumoto, P. Slattery, D. Vishnevskiy, M. Zielinski

The Rockefeller University, New York, USA

A. Bhatti, R. Ciesielski, L. Demortier, K. Goulianos, G. Lungu, S. Malik, C. Mesropian

Rutgers, the State University of New Jersey, Piscataway, USA

S. Arora, A. Barker, J.P. Chou, C. Contreras-Campana, E. Contreras-Campana, D. Duggan,

D. Ferencek, Y. Gershtein, R. Gray, E. Halkiadakis, D. Hidas, A. Lath, S. Panwalkar, M. Park,

R. Patel, V. Rekovic, J. Robles, K. Rose, S. Salur, S. Schnetzer, C. Seitz, S. Somalwar, R. Stone,

S. Thomas

University of Tennessee, Knoxville, USA

G. Cerizza, M. Hollingsworth, G. Ragghianti, S. Spanier, Z.C. Yang, A. York

Texas A&M University, College Station, USA

O. Bouhali, R. Eusebi, W. Flanagan, J. Gilmore, T. Kamon66, V. Khotilovich, R. Montalvo,

C.N.
Nguyen, I. Osipenkov, Y. Pakhotin, A. Perloff, J. Roe, A. Safonov, T. Sakuma, S. Sengupta,
I.
Suarez, A. Tatarinov, D. Toback

Texas Tech University, Lubbock, USA

N. Akchurin, J. Damgov, C. Dragoiu, P.R. Dudero, C. Jeong, K. Kovitanggoon, S.W. Lee,

T. Libeiro, Y. Roh, A. Sill, I. Volobouev, R. Wigmans

Vanderbilt University, Nashville, USA

E. Appelt, A.G. Delannoy, D. Engh, C. Florez, W. Gabella, S. Greene, A. Gurrola, W. Johns,

P. Kurt, C. Maguire, A. Melo, M. Sharma, P. Sheldon, B. Snook, S. Tuo, J. Velkovska

University of Virginia, Charlottesville, USA

D. Andelin, M.W. Arenton, M. Balazs, S. Boutle, S. Conetti, B. Cox, B. Francis, J. Goodell,

R. Hirosky, A. Ledovskoy, C. Lin, C. Neu, D. Phillips II, J. Wood

Wayne State University, Detroit, USA

S. Gollapinni, R. Harr, P.E. Karchin, C. Kottachchi Kankanamge Don, P. Lamichhane,

M. Mattson, C. Milst`ene, A. Sakharov

University of Wisconsin, Madison, USA

M. Anderson, D. Belknap, J.N. Bellinger, L. Borrello, D. Bradley, D. Carlsmith, M. Cepeda,

I. Crotty5, S. Dasu, F. Feyzi, E. Friis, T. Gorski, L. Gray, K.S. Grogg, M. Grothe, R. Hall-Wilton,

M. Herndon, A. Herv´e, P. Klabbers, J. Klukas, J. Lackey, A. Lanaro, C. Lazaridis, J. Leonard,

R. Loveless, S. Lusin5, M. Magrans de Abril, W. Maier, A. Mohapatra, I. Ojalvo, F. Palmonari,

G.A. Pierro, D. Reeder, I. Ross, A. Savin, W.H. Smith, J. Swanson, D. Wenman

: Deceased

1: Also at Vienna University of Technology, Vienna, Austria

2: Also at National Institute of Chemical Physics and Biophysics, Tallinn, Estonia

3: Also at Universidade Federal do ABC, Santo Andre, Brazil

4: Also at California Institute of Technology, Pasadena, USA

5: Also at CERN, European Organization for Nuclear Research, Geneva, Switzerland

6: Also at Laboratoire Leprince-Ringuet, Ecole Polytechnique, IN2P3-CNRS, Palaiseau, France

7: Also at Suez Canal University, Suez, Egypt

8: Also at Zewail City of Science and Technology, Zewail, Egypt

9: Also at Cairo University, Cairo, Egypt

10: Also at Fayoum University, El-Fayoum, Egypt

11: Also at British University, Cairo, Egypt

12: Now at Ain Shams University, Cairo, Egypt

13: Also at Soltan Institute for Nuclear Studies, Warsaw, Poland

14: Also at Universit´e de Haute-Alsace, Mulhouse, France

15: Now at Joint Institute for Nuclear Research, Dubna, Russia

16: Also at Moscow State University, Moscow, Russia

17: Also at Brandenburg University of Technology, Cottbus, Germany

18: Also at Institute of Nuclear Research ATOMKI, Debrecen, Hungary

19: Also at E¨otv¨os Lor´and University, Budapest, Hungary

20: Also at Tata Institute of Fundamental Research -HECR, Mumbai, India

21: Now at King Abdulaziz University, Jeddah, Saudi Arabia

22: Also at University of Visva-Bharati, Santiniketan, India

23: Also at Sharif University of Technology, Tehran, Iran

24: Also at Isfahan University of Technology, Isfahan, Iran

25: Also at Plasma Physics Research Center, Science and Research Branch, Islamic Azad University, Teheran, Iran

26: Also at Facolt`a di Roma, Roma, Italy

a Ingegneria Universit`

27: Also at Universit`a della Basilicata, Potenza, Italy

28: Also at Universit`a degli Studi Guglielmo Marconi, Roma, Italy

29: Also at Laboratori Nazionali di Legnaro dell’ INFN, Legnaro, Italy

30: Also at Universit`a degli studi di Siena, Siena, Italy

31: Also at University of Bucharest, Faculty of Physics, Bucuresti-Magurele, Romania

32: Also at ENEA -Casaccia Research Center, S. Maria di Galeria, Italy

33: Also at Warsaw University of Technology, Institute of Electronic Systems, Warsaw, Poland

34: Also at INFN Sezione di Padova; Universit`a di Padova; Universit`a di Trento (Trento), Padova, Italy

35: Also at Faculty of Physics of University of Belgrade, Belgrade, Serbia

36: Also at University of California, Los Angeles, Los Angeles, USA

37: Also at Scuola Normale e Sezione dell’ INFN, Pisa, Italy

38: Also at INFN Sezione di Roma; Universit`a di Roma ”La Sapienza”, Roma, Italy

39: Also at University of Athens, Athens, Greece

40: Also at Rutherford Appleton Laboratory, Didcot, United Kingdom

41: Also at Institute of High Energy Physics and Informatization, Tbilisi State University, Tbilisi, Georgia

42: Also at The University of Kansas, Lawrence, USA

43: Also at Paul Scherrer Institut, Villigen, Switzerland

44: Also at Institute for Theoretical and Experimental Physics, Moscow, Russia

45: Also at University of Wisconsin, Madison, USA

46: Also at Gaziosmanpasa University, Tokat, Turkey

47: Also at Adiyaman University, Adiyaman, Turkey

48: Also at Izmir Institute of Technology, Izmir, Turkey

49: Also at The University of Iowa, Iowa City, USA

50: Also at Mersin University, Mersin, Turkey

51: Also at Ozyegin University, Istanbul, Turkey

52: Also at Kafkas University, Kars, Turkey

53: Also at Suleyman Demirel University, Isparta, Turkey

54: Also at Ege University, Izmir, Turkey

55: Also at School of Physics and Astronomy, University of Southampton, Southampton, United Kingdom

56: Also at INFN Sezione di Perugia; Universit`a di Perugia, Perugia, Italy

57: Also at Utah Valley University, Orem, USA

58: Also at Institute for Nuclear Research, Moscow, Russia

59: Also at Horia Hulubei National Institute of Physics and Nuclear Engineering (IFIN-HH), Bucharest, Romania

60: Also at University of Belgrade, Faculty of Physics and Vinca Institute of Nuclear Sciences, Belgrade, Serbia

61: Also at Los Alamos National Laboratory, Los Alamos, USA

62: Also at Argonne National Laboratory, Argonne, USA

63: Also at Erzincan University, Erzincan, Turkey

64: Also at Mimar Sinan University, Istanbul, Istanbul, Turkey

65: Also at KFKI Research Institute for Particle and Nuclear Physics, Budapest, Hungary

66: Also at Kyungpook National University, Daegu, Korea