Descriptor: "Kinematic properties" - Searchworks@Jio Institute Digital Library Search Results

29 results on '"Kinematic properties"'

1. Design and Testing of an Extruded Shaking Vibration-Type Peanut Digging and Harvesting Machine for Saline Soil.

Author: Chang, Zengcun, Sun, Bin, Li, Dongjie, Zheng, Xiaoshuai, Yan, Haipeng, Wang, Dongwei, and Hou, Jialin
Subjects: *PEANUT harvesting, *SOIL vibration, *SOIL salinity, *EXCAVATING machinery, *HARVESTING machinery
Abstract: Aiming to address the problems of poor separation of peanuts and soil and severe damage of pods during peanut harvesting in saline soil, a peanut digging and harvesting machine was designed using extrusion shaking vibration and roller extrusion. Theoretical calculations determined the structural parameters of critical components. The law of motion of the seedling soil assemblage at the stage of separation and transportation was derived by analyzing the kinematic properties. The soil extrusion vibration crushing dispersion and sieving process was analyzed, and the factors affecting soil crushing and separation were determined by establishing the extrusion collision model. One-way and orthogonal tests used soil content, breakage, and loss rates as test indicators. The orthogonal test showed that the working parameters were as follows: working speed was 0.889 m/s, the inclination angle was 21.5°, the working line speed of the sieve surface was 2.00 m/s and the roller gap of the roller squeezing device was 37 mm, the peanut harvesting rate of soil content was 1.36%, the breakage rate was 0.78%, and the loss rate was 1.15%. The paper references developing a peanut harvester for clay-heavy soil with soil separation performance improvement. [ABSTRACT FROM AUTHOR]
Published: 2024
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2. Balıkesir ili ve çevresinin kinematik özelliklerine bağlı gerilme ve deformasyon alanlarının modellenmesi.

Author: Kılıç, Nazlı Ceyla Anadolu
Abstract: In the study, the seismicity of Balıkesir province and its vicinity (38.50°-40.50°N-26.00°-29.00°E) was evaluated according to the principles of the Coulomb Failure Criterion. For this, the dominant stress regime of the study area was initially determined. Coulomb models were made for both the identified earthquakes and the whole study area. In this way, the stress interactions of earthquakes were analysed, current stress distributions were determined, and subregions where the hazard of an earthquake was tried to be defined. The earthquake data set used for the evaluations consists of 65 earthquakes focal mechanism solutions that occured between 1900 and 2022. The Coulomb stress distribution generated for the whole study area was evaluated together with the current seismicity of the study area. For this, a homogeneous earthquake catalog was created. The Coulomb stress models were created at various depths in order to determine the variation of stress with depth, too. The transtensional tectonic regime is dominant in the study area, where earthquakes with 3.1=Mw=4.0 are frequently seen. It is seen that the Bandırma-Yenice line has remarkable seismicity for Balıkesir province and its vicinity, where the seismicity has clearly changed with the 1953 Yenice-Gönen Earthquake. [ABSTRACT FROM AUTHOR]
Published: 2023
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3. Drifter Observations Reveal Intense Vertical Velocity in a Surface Ocean Front.

Author: Tarry, Daniel R., Ruiz, Simón, Johnston, T. M. Shaun, Poulain, Pierre‐Marie, Özgökmen, Tamay, Centurioni, Luca R., Berta, Maristella, Esposito, Giovanni, Farrar, J. Thomas, Mahadevan, Amala, and Pascual, Ananda
Subjects: *VERTICAL motion, *VELOCITY, *MESOSCALE eddies, *COLUMNS, *TIME series analysis
Abstract: Measuring vertical motions represent a challenge as they are typically 3–4 orders of magnitude smaller than the horizontal velocities. Here, we show that surface vertical velocities are intensified at submesoscales and are dominated by high frequency variability. We use drifter observations to calculate divergence and vertical velocities in the upper 15 m of the water column at two different horizontal scales. The drifters, deployed at the edge of a mesoscale eddy in the Alboran Sea, show an area of strong convergence (O $\mathcal{O}$(f)) associated with vertical velocities of −100 m day−1. This study shows that a multilayered‐drifter array can be an effective tool for estimating vertical velocity near the ocean surface. Plain Language Summary: The study of vertical motions in the ocean is a key challenge as they are difficult to measure and predict although their impact is crucial on the exchange of water properties in the water column. Here, we use high resolution drifter observations to calculate vertical velocities in the upper layers of a surface density front. This study shows high values of downward speed combined with a high temporal variability at the surface layer. Key Points: Horizontal divergence and vertical vorticity computed from drifter observationsMaximum downward speeds of 100 m day−1 in the upper 15 m on a subducting regionThe vertical velocity time series shows a high temporal variability, varying from 50 to −100 m day−1 over 4 hr [ABSTRACT FROM AUTHOR]
Published: 2022
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4. Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation.

Author: Mostefa, Telha, Eddine, Aissaoui Djamel, Tayeb, Naas Toufik, Hossain, Shakhawat, Rahman, Arifur, Mohamed, Bachiri, and Kim, Kwang-Yong
Subjects: REYNOLDS number, UNSTEADY flow, NEWTONIAN fluids, PECLET number, LYAPUNOV exponents, LAMINAR flow, FLUID flow, STRAIN rate
Abstract: In this study, a numerical investigation based on the CFD method is carried out to study the unsteady laminar flow of Newtonian fluid with a high viscosity in a three-dimensional simulation of a twisted double planetary mixer, which is composed of two agitating rods inside a moving tank. The considered stirring protocol is a "Continuous sine squared motion" by using the dynamic mesh model and user-defined functions (UDFs)to define the velocity profiles. The chaotic advection is obtained in our active mixers by the temporal modulation of rotational velocities of the moving walls in order to enhance the mixing of the fluid for a low Reynolds number and a high Peclet number. For this goal, we applied the Poincaré section and Lyapunov exponent as reliable mathematic tools for checking mixing quality by tracking a number of massless particles inside the fluid domain. Additionally, we investigated the development of fluid kinematics proprieties, such as vorticity, helicity, strain rate and elongation rate, at various time periods in order to view the impact of temporal modulation on the flow properties. The results of the mentioned simulation showed that it is possible to obtain a chaotic advection after a relatively short time, which can deeply enhance mixing fluid efficiency. [ABSTRACT FROM AUTHOR]
Published: 2022
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5. Topology optimization of multi-dimensional force sensor elastomers based on kinematic properties of parallel mechanism.

Author: Zhu, Dachang, He, Yonglong, and Li, Fangyi
Subjects: *STRAIN energy, *ISOMORPHISM (Mathematics), *KINEMATICS, *ELASTOMERS, *THREE-dimensional modeling
Abstract: The structure and deformation force transfer path of the sensor elastomer are crucial to the sensing performance. In order to simplify the design process of the structure and the transmission path, this paper proposes a new design method based on the kinematic properties of the parallel mechanism for the topology optimization of the multi-dimensional force sensor elastomer. To establish the three-dimensional force/moment sensing transmission path, the differential kinematics Jacobian matrix of the three-translation/three-rotating parallel mechanism is calculated. Combining the Jacobian matrix with the differential strain energy, a novel SIMP algorithm of topology optimization is proposed. Furthermore, a topological model for three-dimensional force sensor is established and solved. Simulation and experimental results show that both elastomer structures have kinematic DOF constraints, and the amount of kinematic variation of the force is proportional to the original parallel mechanism kinematic Jacobian matrix. It is verified that the elastomer structure has motion isomorphism with the original parallel mechanism. The elastomer structure utilizes the inverse kinematics Jacobian matrix to realize the sensing ability, and the experimental evaluation of its sensing ability proves that it can be used as a force sensor. The effectiveness, generalization and simplicity of the proposed design method are verified. [Display omitted] • Combining the kinematic properties, a novel topology optimization method is proposed. • The motion mapping relationship is built between the structure and the parallel mechanism. • The inverse kinematics Jacobian matrix is used to realize the sensing of the structure. • The design process of the multi-dimensional force sensor is simple and convenient. [ABSTRACT FROM AUTHOR]
Published: 2024
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6. Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation

Author: Telha Mostefa, Aissaoui Djamel Eddine, Naas Toufik Tayeb, Shakhawat Hossain, Arifur Rahman, Bachiri Mohamed, and Kwang-Yong Kim
Subjects: twisted double planetary, active mixer, chaotic mixing, Poincaré section, kinematic properties, unsteady flow, Mechanical engineering and machinery, TJ1-1570
Abstract: In this study, a numerical investigation based on the CFD method is carried out to study the unsteady laminar flow of Newtonian fluid with a high viscosity in a three-dimensional simulation of a twisted double planetary mixer, which is composed of two agitating rods inside a moving tank. The considered stirring protocol is a “Continuous sine squared motion” by using the dynamic mesh model and user-defined functions (UDFs)to define the velocity profiles. The chaotic advection is obtained in our active mixers by the temporal modulation of rotational velocities of the moving walls in order to enhance the mixing of the fluid for a low Reynolds number and a high Peclet number. For this goal, we applied the Poincaré section and Lyapunov exponent as reliable mathematic tools for checking mixing quality by tracking a number of massless particles inside the fluid domain. Additionally, we investigated the development of fluid kinematics proprieties, such as vorticity, helicity, strain rate and elongation rate, at various time periods in order to view the impact of temporal modulation on the flow properties. The results of the mentioned simulation showed that it is possible to obtain a chaotic advection after a relatively short time, which can deeply enhance mixing fluid efficiency.
Published: 2022
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7. Submesoscale Vorticity and Divergence in the Alboran Sea: Scale and Depth Dependence

Author: Giovanni Esposito, Maristella Berta, Luca Centurioni, T.M. Shaun Johnston, John Lodise, Tamay Özgökmen, Pierre-Marie Poulain, and Annalisa Griffa
Subjects: drifter triplets, kinematic properties, Alboran sea, divergence, vorticity, submesoscales, Science, General. Including nature conservation, geographical distribution, QH1-199.5
Abstract: The statistics of submesoscale divergence and vorticity (kinematic properties, KPs) in the Alboran Sea (Mediterranean Sea) are investigated, using data from drifters released during two experiments in June 2018 and April 2019 in the framework of the Coherent Lagrangian Pathways from the Surface Ocean to Interior (CALYPSO) project. Surface drifters sampling the first meter of water (CARTHE and CODE) and 15 m drifters (SVP) are considered. The area of interest is dominated by processes of strong frontogenesis and eddy formation as well as mixing, related to the high lateral gradients between Mediterranean and Atlantic waters. Drifter coverage and distribution allow to investigate the dependence of KPs on horizontal scales in a range between 1 and 16 km, that effectively bridges submesoscale and mesoscale processes, and at two depths, of 1 and 15 m. For both experiments, the surface flow is highly ageostrophic at 1 km scale, with positive vorticity skewness indicating the presence of submesoscale features. Surface divergence quickly decreases at increasing scales with a slope compatible with a turbulent process with broadband wavenumber spectrum, suggesting the influence of surface boundary layer processes such as wind effects, waves and Langmuir cells at the smaller scales. Vorticity, on the other hand, has a significantly slower decay, suggesting interaction between submesoscale and mesoscale dynamics. Results at 15 m are characterized by reduced ageostrophic dynamics with respect to the surface, especially for divergence. Submesoscale processes are present but appear attenuated in terms of KP magnitude and skewness. The results are generally consistent for the two experiments, despite the observed differences in the mixed layer stratification, suggesting that submesoscale instabilities occur mostly at surface fronts associated with filaments of Atlantic and Mediterranean waters that are present in both cases. The results are compared with previous literature results in other parts of the world ocean and a synthesis is provided. Good agreement with previous surface results is found, suggesting some general properties for divergence and vorticity scale dependence. The importance of further investigating very high resolution frontal processes at scales of tens of meters, as well as processes of interaction with high wind effects is highlighted.
Published: 2021
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8. The effects of cryopreservation and cold storage on sperm subpopulation structure of common carp (Cyprinus carpio L.).

Author: Marinović, Zoran, Šćekić, Ilija, Lujić, Jelena, Urbányi, Béla, and Horváth, Ákos
Subjects: *CARP, *COLD storage, *SPERMATOZOA, *FROZEN semen, *SPERM motility, *CLUSTER analysis (Statistics)
Abstract: The objectives of this study were to identify the presence of different spermatozoa subpopulations (SPs) according to their kinematic characteristics in the sperm of common carp and to test the effects of cryopreservation and prolonged (6-day) storage at room temperature (RT; 23 °C) and 4 °C on spermatozoa motility and subsequently on SP dynamics. Two-step clustering analyses identified three motile SPs based on their kinematic properties: SP1 contained spermatozoa with low velocity and low/moderate STR/LIN values (slow non-linear SP); SP2 was comprised of spermatozoa with high velocities and high STR/LIN values (fast linear SP); SP3 was characterized with high VCL, and moderate LIN/STR (fast non-linear SP); and an additional SP0 was added comprising immotile spermatozoa. Total motility, progressive motility and VCL decreased after cryopreservation to approximately 50% of their value in fresh sperm, while the frequency of SPs characterized by high values of motility parameters declined in favor of those with low motility values and SP0. Motility values of fresh and cryopreserved spermatozoa which were washed with fresh extender after thawing decreased significantly after 24 h of storage at RT and after 72 h of storage at 4 °C, while cryopreserved sperm which remained in the original cryomedium faced a steep decline in motility after only 2 h of storage. As subpopulation frequencies followed this dynamic, this indicates that cryopreserved sperm should be washed with fresh extender in order to obtain favorable sperm kinematic properties after freezing. • Common carp sperm is not homogenous and contains subpopulations. • A total of three subpopulations with different kinematic properties were identified. • Cryopreservation and cold storage influenced the subpopulation dynamics. • Washing of sperm after cryopreservation enables longer preservation of quality. [ABSTRACT FROM AUTHOR]
Published: 2021
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9. Drifter observations reveal intense vertical velocity in a surface ocean front

Author: Rodriguez Tarry, Daniel, Ruiz, Simon, Johnston, T. M. Shaun, Poulain, Pierre Marie, Ozgokmen, Tamay M., Centurioni, Luca R., Berta, Maristella, Esposito, Giovanni, Farrar, J. Thomas, Mahadevan, Amala, Pascual, Ananda, Rodriguez Tarry, Daniel, Ruiz, Simon, Johnston, T. M. Shaun, Poulain, Pierre Marie, Ozgokmen, Tamay M., Centurioni, Luca R., Berta, Maristella, Esposito, Giovanni, Farrar, J. Thomas, Mahadevan, Amala, and Pascual, Ananda
Abstract: © The Author(s), 2022. This article is distributed under the terms of the Creative Commons Attribution License. The definitive version was published in Tarry, D., Ruiz, S., Johnston, T., Poulain, P., Özgökmen, T., Centurioni, L., Berta, M., Esposito, G., Farrar, J., Mahadevan, A., & Pascual, A. Drifter observations reveal intense vertical velocity in a surface ocean front. Geophysical Research Letters, 49(18), (2022): e2022GL098969, https://doi.org/10.1029/2022gl098969., Measuring vertical motions represent a challenge as they are typically 3–4 orders of magnitude smaller than the horizontal velocities. Here, we show that surface vertical velocities are intensified at submesoscales and are dominated by high frequency variability. We use drifter observations to calculate divergence and vertical velocities in the upper 15 m of the water column at two different horizontal scales. The drifters, deployed at the edge of a mesoscale eddy in the Alboran Sea, show an area of strong convergence (urn:x-wiley:00948276:media:grl64766:grl64766-math-0001(f)) associated with vertical velocities of −100 m day−1. This study shows that a multilayered-drifter array can be an effective tool for estimating vertical velocity near the ocean surface., This research was supported by the Office of Naval Research (ONR) Departmental Research Initiative CALYPSO under program officers Terri Paluszkiewicz and Scott Harper. The authors' ONR Grant No. are as follows: DT, SR, AM, and AP N000141613130, TMSJ N000146101612470, PP N000141812418, TO N000141812138, LRC N000141712517, and N00014191269, MB and GE N000141812782 and N000141812039, and JTF N000141812431.
Published: 2023

10. Kinematic properties of human arm reaching movements in a three-dimensional space.

Author: Kashima, Tadashi, Sugawara, Keita, and Mitoh, Ayumi
Abstract: In this study, kinematic properties of human arm reaching movements have been analyzed by use of experimental results of arm trajectories observed in a three-dimensional (3D) space. In the beginning, hand paths obtained by the experiments are kinematically analyzed to pursue their linearity, and we successfully specify a plane on which a hand moves. In the next place, the hand speed profile is calculated by use of position data observed by the experiment in a 3D space. Besides, the hand speed profile is also analytically produced under the minimum jerk criterion with respect to the displacement along the hand path. These observed and produced trajectories are compared, and the similarity of two trajectories has been demonstrated. As a result of the analyses for path and the speed profile of a hand, kinematic properties of human arm trajectories have been identified. [ABSTRACT FROM AUTHOR]
Published: 2018
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11. Meshing Condition and Kinematic Properties of non-circular Gear.

Author: Medvecká-Beňováx, Silvia
Subjects: GEARING machinery, TRANSFERENCE number, AUTOMOBILE transmission, ECCENTRICS (Machinery), KINEMATICS of machinery
Abstract: The gearing with changing transmission gear ratio are used in the practice, even though the "standard" gearing with constant transmission gear ratio are used more often. The article examines the mesh conditions proposed in elliptical gears, as I speed and power ratios in this proposed gearings. The work is devoted to the analysis of these kinematic conditions in the proposed gearings and examines their differences from "standard" ring gear transmission with a constant transference number. The problem is solved for elliptical, eccentric gear with a continuously variable gear ratio to a range from 0.5 through 1 to 2. [ABSTRACT FROM AUTHOR]
Published: 2016
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12. Behavioural and Electrophysiological effects related to semantic violations during braille reading.

Author: Glyn, Vania, Lim, Vanessa K., Hamm, Jeff P., Mathur, Ashwin, and Hughes, Barry
Subjects: *BRAILLE, *EVOKED potentials (Electrophysiology), *SEMANTICS, *ELECTROENCEPHALOGRAPHY, *COGNITIVE processing of language, *HUMAN kinematics
Abstract: This study investigated the potential to detect event related potentials (ERPs) occurring in response to a specific task in braille reading. This would expand current methodologies for studying the cognitive processes underlying braille reading. An N400 effect paradigm was utilised, whereby proficient blind braille readers read congruent- and incongruent-ending braille sentences. Kinematic and electroencephalography (EEG) data were obtained simultaneously and synchronised. The ERPs differed between the incongruent and congruent sentences in a manner consistent with the N400 effect found with a previous sighted reading paradigm, demonstrating that ERPs can be obtained during braille reading. The frequency of finger reversals and the degree of intermittency in the finger velocity were significantly higher when reading incongruent versus congruent sentence endings. Both reversals and the potential N400 effect may reflect processes involved in semantic unification. These findings have significant implications for the modelling of braille reading. The refinement of the technique will enable other ERPs to be identified and related to behavioural responses, to further our understanding of the braille reading process. [ABSTRACT FROM AUTHOR]
Published: 2015
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13. The role of kinematics in cortical regions for continuous human motion perception.

Author: McAleer, Phil, Pollick, Frank, Love, Scott, Crabbe, Frances, and Zacks, Jeffrey
Subjects: *KINEMATICS, *FUNCTIONAL magnetic resonance imaging, *BRAIN imaging, *MOTION perception (Vision), *CEREBELLUM, *ACTIVITIES of daily living
Abstract: It has been proposed that we make sense of the movements of others by observing fluctuations in the kinematic properties of their actions. At the neural level, activity in the human motion complex (hMT+) and posterior superior temporal sulcus (pSTS) has been implicated in this relationship. However, previous neuroimaging studies have largely utilized brief, diminished stimuli, and the role of relevant kinematic parameters for the processing of human action remains unclear. We addressed this issue by showing extended-duration natural displays of an actor engaged in two common activities, to 12 participants in an fMRI study under passive viewing conditions. Our region-of-interest analysis focused on three neural areas (hMT+, pSTS, and fusiform face area) and was accompanied by a whole-brain analysis. The kinematic properties of the actor, particularly the speed of body part motion and the distance between body parts, were related to activity in hMT+ and pSTS. Whole-brain exploratory analyses revealed additional areas in posterior cortex, frontal cortex, and the cerebellum whose activity was related to these features. These results indicate that the kinematic properties of peoples' movements are continually monitored during everyday activity as a step to determining actions and intent. [ABSTRACT FROM AUTHOR]
Published: 2014
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14. KINEMATIC PROPERTIES OF DAMPED LYMAN ALPHA SYSTEMS.

Author: DAS, SNIGDHA and KHARE, PUSHPA
Subjects: *DARK matter, *QUASARS, *GALAXIES, *GALACTIC halos, *CLOUDS
Abstract: In a previous paper, we determined the statistical distributions for various classes of QSO absorption systems in the framework of the CDM model of the universe with a mass distribution of dark matter halos as given by the Press Schechter mechanism. These were shown to be consistent with the observed distributions for reasonable choices of model parameters. In this paper, we generate Voigt profiles of C IV lines associated with Damped Lyman Alpha systems in the framework of this model, taking into account rotation of disks and random motion of clouds embedded in galactic halos. We compare these with the profiles for a sample of 32 Damped Lyman Alpha systems collected from the literature by performing several statistical tests. These tests compare the width and the degree of asymmetry in the line profiles produced by the rotation of randomly inclined disks and the random velocity of clouds in the galactic halos, with the corresponding quantities in the observed profiles. We find that the kinematic properties predicted by the model are in good agreement with observations provided the disk thickness is about ten thousand times smaller than its radius, which indicates that the material in the disks is concentrated in dense clouds with roughly unit covering factor. [ABSTRACT FROM AUTHOR]
Published: 2006
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15. Compound strut and planar six-bar linkage suspension systems.

Author: MacLaurin, E B
Subjects: AUTOMOBILE springs & suspension, STRUTS (Engineering), KINEMATICS
Abstract: This paper reviews the properties and possible advantages of compound strut and related six-bar linkage suspension systems. [ABSTRACT FROM AUTHOR]
Published: 2003
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16. Mesoscale eddies in the Black Sea: Characteristics and kinematic properties in a high-resolution ocean model.

Author: Sadighrad, Ehsan, Fach, Bettina A., Arkin, Sinan S., Salihoğlu, Baris, and Hüsrevoğlu, Y. Sinan
Subjects: *MESOSCALE eddies, *OCEAN, *EDDIES, *TRACKING algorithms, *ANTICYCLONES, *CYCLONES, *MEANDERING rivers, KUROSHIO
Abstract: Mesoscale eddies are ubiquitous features of oceanic circulation and important contributors to the transport of water and heat as well as chemical and biological constituents. In the Black Sea, mesoscale eddies, filaments and meanders are recognized as main agents facilitating the transport and distribution of nutrients and biomass between coastal regions and the open, deep sea. In this study, a high-resolution ocean model, Nucleus for a European Model of the Ocean (NEMO), is implemented for the Black Sea and used to create a hindcast simulation of circulation dynamics for the 1985–2014 period. This hindcast simulation is validated and then used to produce a detailed statistical investigation of the occurrence and behavior of mesoscale eddies in the Black Sea. For this purpose, an eddy identification and tracking algorithm (EddyScan) is applied and the kinematic properties of all eddies are detected, including eddy number, size, lifetime, excursion distance and their spatial distribution. The analysis shows that, on average, anticyclonic eddies are larger in diameter, have a longer lifetime and travel farther distances from the generation site than cyclonic eddies. However, the number of anticyclonic eddies generated is less than cyclones. Spatial distribution of eddies shows that cyclonic and anticyclonic eddies occupy much of the open Black Sea but few are found on the northwestern shelf. The density of anticyclonic eddies is especially high in the Sevastapol, Sinop, Kizilirmak and Batumi regions; while cyclonic eddy densities are high in the northern Black Sea along the Rim Current, north of the Batumi region, as well as in the center of the western and eastern Black Sea gyres. The number of eddies generated increases in spring and summer and decreases again in fall and winter due to changes in wind stress curl and its impact on Rim Current strength. The temporal evolution of long-lived eddies (>30 days) shows that after their creation, the diameters of cyclonic eddies increase for a period of 2–3 months, after which they reach a stable diameter. On the other hand, anticyclonic eddy diameters increase, on average, for a 5–6-month period and then reach a stable value. The vertical effects of these long-lived eddies generated in the Black Sea generally reach down to 150-200 m and hence intersect with the nitrate maximum and oxygen minimum zone. A first estimation shows that the simulated anticyclonic eddies in the Black Sea may have transported up to four times more water than cyclonic eddies over one year. The mean vertical flux induced by all cyclones generated in one year upwell ~ 0.63 Sv of water, while all anticyclones generated in one year downwell two times as much water or ~ 1.27 Sv over the top 100 m of the water column. This highlights the importance of eddies for the vertical transport of water and associated biochemical properties. In addition, eddies are able to connect different regions of the Black Sea as well as offshore/onshore regions along their paths and are of great importance for nutrient distribution and availability in the Black Sea. • Kinematic properties of mesoscale eddies are investigated with an ocean model. • Anticyclones have larger diameters, a longer lifetime and travel farther distances. • Wind stress curl impacts the number of eddies formed and the Rim Current strength. • Total horizontal transport per year by anticyclones is ~4 times that of cyclones. • Downwelling flux of anticyclones is 4.5 times the upwelling capacity of cyclones. [ABSTRACT FROM AUTHOR]
Published: 2021
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17. Effect of a gas-vortex stabilization method on the kinematic properties of the jet in metal-cutting plasmatrons

Author: Saraev Y., Anakhov, S. V., Matushkin, A. V., Pyckin, Yu. A., Saraev Y., Anakhov, S. V., Matushkin, A. V., and Pyckin, Yu. A.
Abstract: Various methods of gas-vortex stabilization in plasma cutting torches are investigated. The results of the study demonstrate the dependence of the angle of gas injection into the nozzle on the kinematic and kinetic characteristics of plasma jet and, consequently, on the cutting parameters. Increased radial velocity component at the swirler output provides better uniformity of the velocity distribution and kinetic properties of the jet in the affected zone of a cut metal. As a conclusion, it is recommended to use the suggested narrow-jet-plasma technology for cutting thin sheet metals. © 2019 IOP Publishing Ltd., Ministry of Education and Science of the Russian Federation, Minobrnauka: 13.10317.2018/11.12, The work was executed under the support of state assignment of the Ministry of Science and Higher Education of the Russian Federation No. 13.10317.2018/11.12.
Published: 2019

18. Effect of a gas-vortex stabilization method on the kinematic properties of the jet in metal-cutting plasmatrons

Author: A. V. Matushkin, Yu.A. Pyckin, S. V. Anakhov, and Saraev Y.
Subjects: ELECTRIC ARCS, GAS DISCHARGE TUBES, Jet (fluid), STABILIZATION, Materials science, PLASMA JETS, KINETIC CHARACTERISTICS, GAS-VORTEX STABILIZATION, VORTEX FLOW, Kinematics, Mechanics, METAL CUTTING, KINEMATIC PROPERTIES, WELDING, Vortex, KINETIC PROPERTIES, CUTTING PARAMETERS, Stabilization methods, RADIAL VELOCITY, Physics::Plasma Physics, THIN SHEET METAL, PLASMA ARC CUTTING, KINEMATICS, PLASMA TECHNOLOGY, Metal cutting
Abstract: Various methods of gas-vortex stabilization in plasma cutting torches are investigated. The results of the study demonstrate the dependence of the angle of gas injection into the nozzle on the kinematic and kinetic characteristics of plasma jet and, consequently, on the cutting parameters. Increased radial velocity component at the swirler output provides better uniformity of the velocity distribution and kinetic properties of the jet in the affected zone of a cut metal. As a conclusion, it is recommended to use the suggested narrow-jet-plasma technology for cutting thin sheet metals. © 2019 IOP Publishing Ltd. Ministry of Education and Science of the Russian Federation, Minobrnauka: 13.10317.2018/11.12 The work was executed under the support of state assignment of the Ministry of Science and Higher Education of the Russian Federation No. 13.10317.2018/11.12.
Published: 2019

19. The ATLAS(3D) project - III. A census of the stellar angular momentum within the effective radius of early-type galaxies: unveiling the distribution of fast and slow rotators

Author: Emsellem, Eric, Cappellari, Michele, Krajnovic, Davor, Alatalo, Katherine, Blitz, Leo, Bois, Maxime, Bournaud, Frederic, Bureau, Martin, Davies, Roger L., Davis, Timothy A., de Zeeuw, P. T., Khochfar, Sadegh, Kuntschner, Harald, Lablanche, Pierre-Yves, McDermid, Richard M., Morganti, Raffaella, Naab, Thorsten, Oosterloo, Tom, Sarzi, Marc, Scott, Nicholas, Serra, Paolo, van de Ven, Glenn, Weijmans, Anne-Marie, Young, Lisa M., and Kapteyn Astronomical Institute
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, KINEMATIC PROPERTIES, SAURON PROJECT, EXTRA LIGHT, ELLIPTIC GALAXIES, MERGER REMNANTS, galaxies: elliptical and lenticular, cD, VIRGO-CLUSTER SURVEY, MULTI-GAUSSIAN EXPANSION, galaxies: formation, galaxies: structure, DIGITAL SKY SURVEY, RED-SEQUENCE, galaxies: evolution, galaxies: kinematics and dynamics, SIGHT VELOCITY DISTRIBUTIONS, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We provide a census of the apparent stellar angular momentum within 1 Re of a volume-limited sample of 260 early-type galaxies (ETGs) in the nearby Universe, using integral-field spectroscopy obtained in the course of the ATLAS3D project. We exploit the LambdaR parameter to characterise the existence of two families of ETGs: Slow Rotators which exhibit complex stellar velocity fields and often include stellar kinematically Distinct Cores (KDCs), and Fast Rotators which have regular velocity fields. Our complete sample of 260 ETGs leads to a new criterion to disentangle Fast and Slow Rotators which now includes a dependency on the apparent ellipticity (Epsilon). It separates the two classes significantly better than the previous prescription, and than a criterion based on V/Sigma: Slow Rotators and Fast Rotators have LambdaR lower and larger than kFSxSQRT(Epsilon), respectively, where kFS=0.31 for measurements made within 1 Re. We show that the vast majority of early-type galaxies are Fast Rotators: these have regular stellar rotation, with aligned photometric and kinematic axes (Paper II, Krajnovic et al. 2011}, include discs and often bars and represent 86% (224/260) of all early-type galaxies in the volume-limited ATLAS3D sample. Fast Rotators span the full range of apparent ellipticities from 0 to 0.85, and we suggest that they cover intrinsic ellipticities from about 0.35 to 0.85, the most flattened having morphologies consistent with spiral galaxies. Only a small fraction of ETGs are Slow Rotators representing 14% (36/260) of the ATLAS3D sample of ETGs. Of all Slow Rotators, 11% (4/36) exhibit two counter-rotating stellar disc-like components and are rather low mass objects (Mdyn10^10.5 M_Sun), and often (17/32) exhibit KDCs., 28 pages, 23 figures, LaTeX. Accepted for publication in MNRAS. High resolution version can be found on http://purl.com/atlas3d
Published: 2016

20. The ATLAS(3D) project

Subjects: KINEMATIC PROPERTIES, SAURON PROJECT, cD, EXTRA LIGHT, ELLIPTIC GALAXIES, MERGER REMNANTS, VIRGO-CLUSTER SURVEY, MULTI-GAUSSIAN EXPANSION, galaxies: formation, galaxies: structure, DIGITAL SKY SURVEY, galaxies: elliptical and lenticular, RED-SEQUENCE, galaxies: evolution, galaxies: kinematics and dynamics, SIGHT VELOCITY DISTRIBUTIONS
Abstract: We provide a census of the apparent stellar angular momentum within one effective radius of a volume-limited sample of 260 early-type galaxies (ETGs) in the nearby Universe, using the integral-field spectroscopy obtained in the course of the ATLAS(3D) project. We exploit the lambda(R) parameter (previously used via a constant threshold value of 0.1) to characterize the existence of two families of ETGs: slow rotators which exhibit complex stellar velocity fields and often include stellar kinematically distinct cores, and fast rotators which have regular velocity fields. Our complete sample of 260 ETGs leads to a new criterion to disentangle fast and slow rotators which now includes a dependency on the apparent ellipticity epsilon. It separates the two classes significantly better than the previous prescription and better than a criterion based on V/sigma: slow rotators and fast rotators have.R lower and larger than k(FS) x root epsilon, respectively, where k(FS) = 0.31 for measurements made within an effective radius R-e.We show that the vast majority of ETGs are fast rotators: these have the regular stellar rotation, with aligned photometric and kinematic axes (Paper II of this series), include discs and often bars and represent 86 +/- 2 per cent (224/260) of all ETGs in the volume-limited ATLAS(3D) sample. Fast rotators span the full range of apparent ellipticities from epsilon = 0 to 0.85, and we suggest that they cover intrinsic ellipticities from about 0.35 to 0.85, the most flattened having morphologies consistent with spiral galaxies. Only a small fraction of ETGs are slow rotators representing 14 +/- 2 per cent (36/260) of the ATLAS(3D) sample of ETGs. Of all slow rotators, 11 per cent (4/36) exhibit two counter-rotating stellar disc-like components and are rather low-mass objects (M-dyn 10(10.5) M-circle dot), and often (17/32) exhibit kinematically distinct cores. Slow rotators dominate the high-mass end of ETGs in the ATLAS(3D) sample, with only about one-fourth of galaxies with masses above 10(11.5) M-circle dot being fast rotators. We show that the a4 parameter which quantifies the isophote's disciness or boxiness does not seem to be simply related to the observed kinematics, while our new-criterion based on lambda(R) and epsilon is nearly independent of the viewing angles. We further demonstrate that the classification of ETGs into ellipticals and lenticulars is misleading. Slow and fast rotators tend to be classified as ellipticals and lenticulars, respectively, but the contamination is strong enough to affect results solely based on such a scheme: 20 per cent of all fast rotators are classified as ellipticals, and more importantly 66 per cent of all ellipticals in the ATLAS(3D) sample are fast rotators.Fast and slow rotators illustrate the variety of complex processes shaping galactic systems, such as secular evolution, disc instabilities, interaction and merging, gas accretion, stripping and harassment, forming a sequence from high to low (stellar) baryonic angular momentum. Massive slow rotators represent the extreme instances within the red sequence of galaxies which might have suffered from significant merging without being able to rebuild a fastrotating component within one effective radius. We therefore argue for a shift in the paradigm for ETGs, where the vast majority of ETGs are galaxies consistent with nearly oblate systems (with or without bars) and where only a small fraction of them (less than 12 per cent) have central (mildly) triaxial structures.
Published: 2011

21. Galactic bulges from Hubble Space Telescope NICMOS observations

Subjects: VELOCITY DISPERSIONS, DWARF ELLIPTIC GALAXIES, Astrophysics::Cosmology and Extragalactic Astrophysics, BAND SURFACE PHOTOMETRY, KINEMATIC PROPERTIES, DISK-DOMINATED GALAXIES, STRUCTURAL PARAMETERS, COLD DARK-MATTER, FUNDAMENTAL PLANE, galaxies : structure, EARLY-TYPE GALAXIES, galaxies : spiral, Astrophysics::Earth and Planetary Astrophysics, SPIRAL GALAXIES, Astrophysics::Galaxy Astrophysics
Abstract: We investigate bulge and disk scaling relations using a volume-corrected sample of early-to intermediate-type disk galaxies in which, importantly, the biasing flux from additional nuclear components has been modeled and removed. Structural parameters are obtained from a seeing-convolved, bulge + disk + nuclear-component decomposition applied to near-infrared surface brightness profiles spanning similar to 10 pc to the outer disk. Bulge and disk parameters, and bulge-to-disk ratios, are analyzed as a function of bulge luminosity, disk luminosity, galaxy central velocity dispersion, and galaxy Hubble type. Mathematical expressions are given for the stronger relations, which can be used to test and constrain galaxy formation models. Photometric parameters of both bulges and disks are observed to correlate with bulge luminosity and with central velocity dispersion. In contrast, for the unbarred, early to intermediate types covered by the sample, Hubble type does not correlate with bulge and disk components, nor their various ratios. In this sense, the early-to-intermediate spiral Hubble sequence is scale free. However, galaxies themselves are not scale free, the critical scale being the luminosity of the bulge. Bulge luminosity is shown to affect the disk parameters, such that central surface brightness becomes fainter, and scale length bigger, with bulge luminosity. The lack of significant correlations between bulge parameters (size, luminosity, or density) on disk luminosity, remains a challenge for secular evolution models of bulge growth. The average near-infrared bulge-to-total flux ratio for our S0-S0a galaxies is 0.25 (+/- 0.09).
Published: 2007

22. The HST/ACS Coma Cluster Survey - X. Nuclear star clusters in low-mass early-type galaxies: scaling relations

Author: Marc Balcells, Shardha Jogee, Edwin A. Valentijn, Alister W. Graham, John R. Lucey, Gijs Verdoes Kleijn, Anil C. Seth, Reynier F. Peletier, Henry C. Ferguson, Paul Goudfrooij, Mark den Brok, Rafael Guzman, Peter Erwin, Steven Phillipps, Lilian Dominguez, Tim Weinzirl, Carlos Hoyos, David Carter, Thomas H. Puzia, and Astronomy
Subjects: endocrine system, Intergalactic star, FOS: Physical sciences, DWARF ELLIPTIC GALAXIES, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, KINEMATIC PROPERTIES, STRUCTURAL PARAMETERS, SUPERMASSIVE BLACK-HOLES, GLOBULAR-CLUSTERS, Coma Cluster, Astrophysics::Solar and Stellar Astrophysics, star clusters: general. [Galaxies], Galaxy cluster, Astrophysics::Galaxy Astrophysics, QB, Luminous infrared galaxy, Physics, Astronomy, Astronomy and Astrophysics, galaxies: dwarf, HUBBLE-SPACE-TELESCOPE, VIRGO CLUSTER, Astrophysics - Astrophysics of Galaxies, Dwarf spheroidal galaxy, dwarf [Galaxies], HOST GALAXIES, Star cluster, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Globular cluster, nuclei [Galaxies], galaxies: star clusters: general, Elliptical galaxy, MILKY-WAY, Astrophysics::Earth and Planetary Astrophysics, galaxies: nuclei, SPIRAL GALAXIES
Abstract: We present scaling relations between structural properties of nuclear star clusters and their host galaxies for a sample of early-type dwarf galaxies observed as part of the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) Coma Cluster Survey. We have analysed the light profiles of 200 early-type dwarf galaxies in the magnitude range $16.0 < m_{F814W} < 22.6 $ mag, corresponding to $-19.0 < M_{F814W} < -12.4 $ mag. Nuclear star clusters are detected in 80% of the galaxies, thus doubling the sample of HST-observed early-type dwarf galaxies with nuclear star clusters. \changed{We confirm that the} nuclear star cluster detection fraction decreases strongly toward faint magnitudes. The luminosities of nuclear star clusters do not scale linearly with host galaxy luminosity. A linear fit yields L$_{nuc} \sim $L$_{gal}^{0.57\pm0.05}$. The nuclear star cluster-host galaxy luminosity scaling relation for low-mass early-type dwarf galaxies is consistent with formation by globular cluster accretion. We find that at similar luminosities, galaxies with higher S��rsic indices have slightly more luminous nuclear star clusters. Rounder galaxies have on average more luminous clusters. Some of the nuclear star clusters are resolved, despite the distance of Coma. We argue that the relation between nuclear star cluster mass and size is consistent with both formation by globular cluster accretion and in situ formation. Our data are consistent with GC inspiraling being the dominant mechanism at low masses, although the observed trend with S��rsic index suggests that in situ star formation is an important second order effect., Accepted for publication in MNRAS
Published: 2014

23. Measurement of the production cross sections for a Z boson and one or more b jets in pp collisions at at √s = 7 TeV

Author: L. Rebane, Narumon Suwonjandee, Laurent Thomas, Tapas Sarangi, J. Martínez-Ortega, Charles Maguire, Theodoros Geralis, Andrea Rizzi, H. Mendez, Victor Murzin, Amr Radi, I. Grigelionis, S. Frosali, Jordan Tucker, Michal Simon, Alexandre Zabi, Efstathios Stiliaris, Q. Li, Tutanon Sinthuprasith, Nicholas Wardle, Tariq Aziz, Dave M Newbold, L. M. Cremaldi, Mark Olschewski, Katja Klein, Christophe Ochando, Teimuraz Lomtadze, Joram Berger, Marko Dragicevic, Vladimir Rekovic, Ian Shipsey, Willard Johns, Leonardo Benucci, Pasquale Musella, Giacomo Sguazzoni, Alan Campbell, Francesco Santanastasio, Stoyan Stoynev, Tongguang Cheng, Ivan Glushkov, D. Renker, Katarzyna Romanowska-Rybinska, Federico Nguyen, Shalhout Shalhout, Y. Choi, Sergo Jindariani, P. Verdier, Andrius Juodagalvis, A. Nürnberg, Andrea Bocci, V. Halyo, Christopher Silkworth, Nishu Nishu, Vladimir Karjavin, Kerstin Borras, Tommaso Dorigo, Alexis Descroix, Sandra Malvezzi, Gyorgy Bencze, Urs Langenegger, Anil Kumar, Enrique Calvo, E. Friis, Dong-Chul Son, Dimitri Bourilkov, S. Carrillo Moreno, Pietro Faccioli, Hamit Mermerkaya, Mete Yücel, Valentin Knünz, Alberto Zucchetta, Volker Adler, Philip Hebda, Ilya Osipenkov, H. Arfaei, Rino Castaldi, Robert Hirosky, M. Serin, Liliana Teodorescu, A. Tropiano, Sharon Hagopian, Ralf Ulrich, Seth Cooper, Adolf Bornheim, Matti J Kortelainen, Katerina Lipka, Martin Kirakosyan, S. Cihangir, J. Santaolalla, Dooyeon Gyun, Lukas Vanelderen, K. Gabathuler, Hyangkyu Park, Steffen Röcker, Caroline Collard, Georgios Anagnostou, Melody A. Swartz, Maxwell Chertok, Danek Kotlinski, M. Chamizo Llatas, Denis Gelé, Matthew Kenzie, Mauro Emanuele Dinardo, Carmen Albajar, H. Held, Sven Dildick, Jeremy Mans, Agni Bethani, Stephane Perries, Nhan Viet Tran, Carsten Heidemann, Costas Foudas, Junhui Liao, Devdatta Majumder, Christof Roland, Juliette Alimena, Ivan-Kresimir Furic, D. Domínguez Vázquez, Rishi Patel, Y. D. Oh, Ian Macneill, M. Calderon De La Barca Sanchez, Andrew Gilbert, W. L. Aldá, Meenakshi Narain, J. Marrouche, Alessandro Thea, Sunil Somalwar, Willi Bertl, Maria Agnese Ciocci, Kittikul Kovitanggoon, Nicholas Eggert, Maxim Goncharov, I. Ross, Richard D Field, Marco Pieri, Francesco Costanza, Jose Lazo-Flores, Ivan Reid, Dominique Gigi, I. Segoni, Peter Kreuzer, Fabrice Couderc, Gero Flucke, Manfred Paulini, Guido Tonelli, Zeljko Antunovic, Claudia-Elisabeth Wulz, Christoph Paus, Andrew Whitbeck, Viktor Veszpremi, Abdulla Abdulsalam, Gianluca Petrillo, A. Petrukhin, Daniel Teyssier, Victor Perelygin, Alessandra Fanfani, Jacopo Bernardini, Jay Hauser, A. Vilela Pereira, M. Gosselink, Monika Sharma, Tiziano Rovelli, Michal Bluj, Andrey Marinov, Konstantinos Theofilatos, Sandor Czellar, Manuel Giffels, Gennady Mesyats, Alexander Nikitenko, Jasvinder A. Singh, A. S. Yoon, Dipanwita Dutta, Marco Grassi, A. C. Kraan, Shabnam Jabeen, Maciej Misiura, Hongfang Liu, Anna Teresa Meneguzzo, Victor Krychkine, Pierluigi Bortignon, Wolfgang Waltenberger, Piergiulio Lenzi, Matthew Snowball, E. J. Tonelli Manganote, Khristian Kotov, Krzysztof Piotrzkowski, Ekaterina Kuznetsova, Lloyd Stanley Durkin, Yvonne Kuessel, Vincenzo Innocente, Shuai Liu, Ioannis Papadopoulos, X. Aslanoglou, Peter Robmann, Ugo Gasparini, Veikko Karimäki, Nicola Cavallo, Salvatore My, James Dolen, Marco-Andrea Buchmann, Ian R Tomalin, G. G. Da Silveira, Vladimir Palichik, Sue Ann Koay, S. Lacaprara, Raffaello D'Alessandro, Y. Guo, Slawek Tkaczyk, Andrei Sobol, A. De Roeck, William Ferguson, Joseph Goodell, Dmitry Hits, Sara Fiorendi, Tomasz Frueboes, Alberto Ruiz-Jimeno, L. Barbone, Freya Blekman, Ilse Krätschmer, David Michael Morse, Vassili Maroussov, Kai-Feng Chen, Ettore Focardi, Riccardo Paramatti, Andrea Giammanco, Betty Calpas, Jeannine Wagner-Kuhr, John Rander, Josef Strauss, Andrei Starodumov, Andrew Askew, Gurpreet Singh, Cecilia Elena Gerber, U. Tamponi, Keith Rose, Mingshui Chen, Nikita Beliy, Guo-Ming Chen, Arabella Martelli, Victoria Zhukova, Muhammad Ahmad, Felix Hoehle, Suman Bala Beri, Sten Luyckx, Yen-Jie Lee, Jorma Tuominiemi, Maria Cruz Fouz, Joseph Lykken, John Michael Marraffino, J. Temple, Cesar Augusto Bernardes, Aniello Spiezia, J. P. Gomez, Ugur Akgun, Aytul Adiguzel, Gui Nyun Kim, Cosmin Dragoiu, Ajit Mohapatra, J. Rodrigues Antunes, Lucas Taylor, L. Lusito, A. M. Guler, Dmytro Kovalskyi, C. Lagana, Gyorgy Vesztergombi, Luca Malgeri, A. Markou, Tiziano Camporesi, L. Brigliadori, A. J. Bell, Alexei Safonov, T. Y. Kim, S. Arora, Kirti Ranjan, Vasken Hagopian, Janos Erö, Panagiotis Katsas, Roberto Castello, Doga Gulhan, Louis Lyons, Mauro Donegà, Igor Bayshev, Jason Gilmore, Marco Paganoni, Frank Jm Geurts, Stephen Sanders, Wesley H Smith, Vivian O'Dell, Jamila Bashir Butt, Seema Sharma, Livia Soffi, Christopher Seez, Amitabh Lath, S. Qazi, R. Frühwirth, Dean Hidas, Robert Cousins, D. Mekterovic, Zeynep Demiragli, J. C. Yun, J. Olzem, Atanu Modak, Bastian Kargoll, Peter Elmer, Piotr Zalewski, S. Gollapinni, Vitaly Smirnov, Dragos Velicanu, Didar Dobur, S. Goy Lopez, Nuno Leonardo, Marco Cuffiani, D. J. Summers, Don Lincoln, Hafeez R Hoorani, B. Klein, Andrew Rose, Nural Akchurin, Scott Thomas, Piero Giorgio Verdini, T. Dorland, Oliver Buchmuller, Alin Titus Serban, Yajun Mao, T. Schum, Mikhail Kirsanov, I. Gonzalez Caballero, Colin Bernet, Ernesto Migliore, Hans-Jürgen Simonis, Brian Pollack, Chi Lin, T. Speer, Venkatesh Veeraraghavan, Wolfgang Adam, Ian Fisk, Richard Hall-Wilton, Elizabeth Sexton-Kennedy, Julia Velkovska, Sudha Ahuja, Zhenwei Yang, F. M. Stober, N. G. Redaelli, Inga Bucinskaite, H. S. Chen, Austin Ball, Roger Wolf, U. E. Surat, E. Eskut, Daniel John Karmgard, Y. Fu, Halil Saka, Pietro Govoni, Todd Adams, Nathaniel Odell, Manfred Jeitler, Ada Solano, J. Whitmore, B. Fabbro, Fabrizio Palla, Wit Busza, Matthias Wolf, Andrew Melo, Nadia Pastrone, Martti Raidal, Emmanuel Contreras-Campana, Pamela Klabbers, Matevz Tadel, H. El Mamouni, Yongsun Kim, Lev Dudko, Jeremy Andrea, Daryl Hare, Giovanni Petrucciani, Dawn Leslie, P.E. Schlein, Maria Girone, Martina Malberti, Dorian Kcira, J. E. Kim, P. Lobelle Pardo, Andreas Kornmayer, Ashutosh Bhardwaj, Helmut Vogel, Kelly Beernaert, Mikhail Dubinin, Wei Li, Suat Ozkorucuklu, Wei Xie, J. Ellison, Paolo Ronchese, Sanjay Kumar Swain, Jay Dittmann, Marc M Baarmand, W. Zou, Gaetano-Marco Dallavalle, Jose F Benitez, Salvatore Costa, Pawandeep Jandir, Boaz Klima, D. Evans, Richard G Kellogg, Michael Tytgat, David Lange, Robin Erbacher, Andrew Beretvas, Otto Hindrichs, Lukas Bäni, M. Maes, Steve Schnetzer, Saranya Ghosh, Klaas Padeken, Renato Campanini, B. A. Barnett, Marc Dünser, C. Martinez Rivero, Marcos Cerrada, Giorgio Apollinari, R. Carroll, Andrei Gritsan, Viola Sordini, Kristian Harder, Erika Garutti, Guillaume Garcia, Peter Raics, Peicho Petkov, M. Correa Martins, Achille Petrilli, Chun-Hua Jiang, Karl Gill, Mauro Menichelli, Alexander Gude, P. Lawson, Sa. Jain, Ta-Yung Ling, M. Erofeeva, G. Zito, Alessandro Montanari, T. Tabarelli de Fatis, Frederic Jean Ronga, Z. Wan, Rainer Wallny, Pierluigi Zotto, S. Lee, Hwi Dong Yoo, K. Ocalan, A. Hunt, Maryam Zeinali, Patrick Jarry, Luc Pape, Vassili Kachanov, Demetrios Loukas, Burin Asavapibhop, Aram Avetisyan, Daniele Trocino, Silvia Maselli, Benjamin Charles Radburn-Smith, Mikhail Makouski, M. Feindt, M. Eads, Jose Chinellato, Richard Cavanaugh, F. Nowak, D. C. Miner, G. Hu, Indara Suarez, L. Muniz, Roberto Sacchi, P. Bartalini, Natascha Hörmann, Tejinder Virdee, David Sabes, Ali Fahim, Carlos Lourenco, Valentina Dutta, Senta Greene, Sherif Elgammal, Giuseppe Barbagli, Sergey Shmatov, Boris Mangano, Robert Bainbridge, Lingshan Xu, Luca Perniè, Roland Horisberger, Yuan Chao, Georgios Mavromanolakis, Matthew Nguyen, Gobinda Majumder, Olga Evdokimov, Junghwan Goh, Livio Fanò, Ulf Behrens, Lucie Gauthier, A. C. Le Bihan, Alexander Dierlamm, S. Semenov, Emine Gurpinar, Alexis Pompili, B. Gomez Moreno, Sushil Chauhan, Petar Adzic, Nicolò Tosi, Maria Margherita Obertino, Ketino Kaadze, Kajari Mazumdar, C. Kottachchi Kankanamge Don, Nickolas Mccoll, Laurent Forthomme, Yong Ban, M. De Gruttola, Ivan Amos Cali, E. Alagoz, Moritz Guthoff, Marc Weber, Christian Contreras-Campana, Maria Elena Pol, T. Miceli, Mia Tosi, Stefano Ragazzi, Jane Nachtman, S. Won, Stephanie Baffioni, Hannes Schettler, Sergio F Novaes, Donald Belknap, Iasonas Topsis-Giotis, Alexander Toropin, L. Perchalla, A. De Benedetti, Georg Auzinger, Adrian Perieanu, A. Meyer, Vladimir Petrov, Russell Richard Betts, Conor Henderson, Thomas N. Williams, Giancarlo Mantovani, Carlo Battilana, R. Volpe, Seth Conrad Zenz, I. H. D. La Cruz, Norbert Neumeister, S. König, André Holzner, Vardan Khachatryan, Marko Ekmedzic, T. J. Pearson, Alessio Ghezzi, C. Urscheler, Sabino Meola, Marcus Hohlmann, M. Luk, M. Müntel, Neilayan Sen, Roberto Covarelli, Michele Arneodo, J. G. Shiu, Artur Kalinowski, Thomas Bergauer, Teruki Kamon, Srecko Morovic, Esa Tuovinen, R. Ferretti, Samim Erhan, Pedro G Mercadante, Andrew Godshalk, Konstantin Matchev, Bruno Casal, J. Haupt, Morgan Lethuillier, Jean-Marie Brom, Sezen Sekmen, M. Hollingsworth, James Keaveney, T. Danielson, Y. Assran, Hans-Christian Kaestli, W. L. Prado Da Silva, Charles Dietz, Yasar Onel, Pooja Saxena, Michele Gallinaro, A. Ellithi Kamel, Luca Perrozzi, Manfred Krammer, Kevin Sung, Radia Redjimi, V. Khotilovich, Felix Bachmair, Cory Fantasia, K. Sudhakar, Winston Ko, Andrea Schizzi, M. Vidal Marono, S. De Visscher, Sergio Cittolin, Julien Caudron, Armin Burgmeier, Jared Sturdy, S. Mukherjee, Julia Thom, Finn Rebassoo, Albert Ferrando, M. Gabusi, Dmitri Konstantinov, L. K. Gibbons, Sandra S. Padula, Michal Szleper, Philippe Gras, Roberto Chierici, Chia-Ming Kuo, M. Searle, D. Lazic, Johannes Haller, N. Cripps, Philip Baringer, Enrico Robutti, George Stephans, Thomas Weiler, Paolo Vitulo, Florent Lacroix, K. Nirunpong, Werner Sun, Konstanty Sumorok, Semiray Girgis, Paul Edmund Karchin, Christopher Rogan, Paul Papacz, Cheol-Hwan Park, Junquan Tao, J. Fernandez Menendez, William J Spalding, Stephen Wimpenny, Peter Wittich, A. Drozdetskiy, Harvey B Newman, Jeffrey Berryhill, Jordan Nash, Jay Roberts, A. Van Spilbeeck, Sung Keun Park, Stefano Bianco, Cristina Ferro, C. S. Moon, Mihee Jo, Pietro Vischia, Joschka Lingemann, Pierre Juillot, Emmanuel Olaiya, Alexander Schmidt, J. M. Vizan Garcia, Bugra Bilin, Nadir Daci, R. E. Hughes, Kati Lassila-Perini, L. Wendland, Joao Seixas, Francisco Matorras, John A Coughlan, Volker Blobel, Ignacio Redondo, Franco Gonella, Benjamin Stieger, Hyun-Chul Kim, P. M. Ribeiro Cipriano, Francisco Yumiceva, Valentina Gori, Steven Worm, Yurii Maravin, P. Van Mulders, Francesco Fabozzi, F. J. Munoz Sanchez, Marco Rovere, Christine O'Brien, Vadim Oreshkin, Stefaan Tavernier, T. Caebergs, Marco Toliman Lucchini, Matthew Chasco, Lucia Silvestris, G. Kukartsev, Andrea Perrotta, S. Fonseca De Souza, Michael Planer, Jennifer S. Haas, A. Delgado Peris, J. St. John, Oliver Pooth, Alex Garabedian, Egidio Longo, Jan Steggemann, Francesca Ricci-Tam, Ivan Marchesini, Stefan Wayand, Scott Wilbur, Renato Potenza, J. Sibille, G. Merino, Yury Ivanov, Andre Sznajder, Akram Khan, Hermine Katharina Wöhri, Petra Merkel, Pelin Kurt, F. P. Schilling, B. Marangelli, Candan Dozen, D. W. Jang, A. De Cosa, Hannes Sakulin, Michael Wayne Arenton, Henning Flacher, Yanjun Tu, Ilya Gorbunov, Pàl Hidas, Rachel Yohay, T. du Pree, Vladimir Gavrilov, Salvatore Rappoccio, Sergio P Ratti, F. De Guio, Aleko Khukhunaishvili, Neeti Parashar, Frank Chlebana, Nikolaos Manthos, Martin Grunewald, Ulrich Heintz, Carlos Willmott, S. Ochesanu, Giovanni Organtini, Mohammed Mahmoud, David B. Cline, Ritva Kinnunen, Petar Maksimovic, Niklas Pietsch, E. Di Marco, Patrick Janot, Derek Barge, Sunil Bansal, Loukas Gouskos, Vladimir Mossolov, Pierre Lecomte, Fuqiang Wang, Prashant Shukla, Thorsten Chwalek, M. Merola, André Rosowsky, Andrew Ivanov, Simone Paoletti, Rebecca Lane, Guenter Eckerlin, Yuri Gershtein, Georgia Karapostoli, S. Walsh, Annik Olbrechts, Andreas Güth, Peter Timothy Cox, Tilman Rohe, Pierluigi Paolucci, Frank Hartmann, Luciano Orsini, Jing Wang, Lorenzo Foà, Vasile Mihai Ghete, Huseyin Topakli, Markus Friedl, Fuat Ilkehan Vardarlı, Rachel Houtz, G. Nicolas Kaufman, Mohsen Khakzad, Roberto Dell'Orso, Suchandra Dutta, Paolo Spagnolo, C. Justus, Emmanuelle Perez, J. Piedra Gomez, Yusuf Erdogan, T. Martins, Maksim Azarkin, Si Xie, Robert Stone, Frank Meier, Cristina Riccardi, Justin Pilot, Brian L Winer, Andrew Levin, Armen Tumasyan, Paula Eerola, Manoj Sharan, Lindsey Gray, James John Brooke, A. Nappi, Nicolas Chanon, Helena Malbouisson, P. G. Ferreira Parracho, Anne-Marie Magnan, Wagner Carvalho, S. Liang, Alex J. Barker, M. Kress, Camelia Mironov, S. C. Kao, Samantha Dooling, G. Zumerle, Oleg Prokofyev, Wolfram Erdmann, Daniel Meister, C. Jarvis, Nicolo Cartiglia, V. Chetluru, Rajat Gupta, Taimoor Khurshid, Hanno Perrey, R. Doesburg, R. Kroeger, Attilio Santocchia, Jean Fay, Igor Dremin, Abideh Jafari, Jean-Louis Faure, Domenico Giordano, Brian Francis, Andrey Leonidov, Antonio Branca, Jean-Charles Fontaine, Anton Dimitrov, Andrea Gozzelino, Werner Lustermann, Andromachi Tsirou, Tatiana Medvedeva, R. Placakyte, J. S. Wood, Sergey Troshin, Philip Symonds, D. Winn, David D'Enterria, Helio Nogima, A. F. Barfuss, Matthew Fisher, G. Georgiou, Alberto Orso Maria Iorio, Mara Senghi Soares, Serguei Ganjour, Nathan Mirman, Shruti Panwalkar, Cristina Biino, Ivan Mikulec, Francesco Micheli, Paolo Checchia, Gul Gokbulut, Eric Appelt, Denis Rathjens, Claude Nuttens, D. Krpic, Alberto Messineo, Bryan Dahmes, Silvia Taroni, J. Zablocki, Md. Naimuddin, M. Zeise, Hannes Jung, Alexander Zhokin, Martijn Mulders, Darin Baumgartel, G. Broccolo, Eike Schlieckau, Ludivine Ceard, L. 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Weber, Joerg Behr, Universidad de Cantabria, Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut Pluridisciplinaire Hubert Curien (IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre de Calcul de l'IN2P3 (CC-IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), CMS, The, CMS Collaboration, Chatrchyan, S, Iorio, ALBERTO ORSO MARIA, Others, Merola, Mario, Lista, Luca, Özyeğin University, Işıldak, Bora, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Ege Üniversitesi, SCOAP, Khachatryan, V, Sirunyan, A, Tumasyan, A, Adam, W, Bergauer, T, Dragicevic, M, Erö, J, Fabjan, C, Friedl, M, Frühwirth, R, Ghete, V, Hörmann, N, Hrubec, J, Jeitler, M, Kiesenhofer, W, Knünz, V, Krammer, M, Krätschmer, I, Liko, D, Mikulec, I, Rabady, D, Rahbaran, B, Rohringer, C, Rohringer, H, Schöfbeck, R, Strauss, J, Taurok, A, Treberer Treberspurg, W, Waltenberger, W, Wulz, C, Mossolov, V, Shumeiko, N, Gonzalez, J, Alderweireldt, S, Bansal, M, Bansal, S, Cornelis, T, De Wolf, E, Janssen, X, Knutsson, A, Luyckx, S, Mucibello, L, Ochesanu, S, Roland, B, Rougny, R, Staykova, Z, Van Haevermaet, H, Van Mechelen, P, Van Remortel, N, Van Spilbeeck, A, Blekman, F, Blyweert, S, D'Hondt, J, Kalogeropoulos, A, Keaveney, J, Maes, M, Olbrechts, A, Tavernier, S, Van Doninck, W, Van Mulders, P, Van Onsem, G, Villella, I, Caillol, C, Clerbaux, B, De Lentdecker, G, Favart, L, Gay, A, Hreus, T, Léonard, A, Marage, P, Mohammadi, A, Perniè, L, Reis, T, Seva, T, Thomas, L, Velde, C, Vanlaer, P, Wang, J, Adler, V, Beernaert, K, Benucci, L, Cimmino, A, Costantini, S, Dildick, S, Garcia, G, Klein, B, Lellouch, J, Marinov, A, Mccartin, J, Rios, A, Ryckbosch, D, Sigamani, M, Strobbe, N, Thyssen, F, Tytgat, M, Walsh, S, Yazgan, E, Zaganidis, N, Basegmez, S, Beluffi, C, Bruno, G, Castello, R, Caudron, A, Ceard, L, Da Silveira, G, Delaere, C, Du Pree, T, Favart, D, Forthomme, L, Giammanco, A, Hollar, J, Jez, P, Lemaitre, V, Liao, J, Militaru, O, Nuttens, C, Pagano, D, Pin, A, Piotrzkowski, K, Popov, A, Selvaggi, M, Garcia, J, Beliy, N, Caebergs, T, Daubie, E, Hammad, G, Alves, G, M. 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Department of Physics, Massachusetts Institute of Technology. Laboratory for Nuclear Science, Apyan, Aram, Bauer, Gerry P, Busza, Wit, Cali, Ivan Amos, Chan, Matthew Hans, Di Matteo, Leonardo, Dutta, Valentina, Gomez-Ceballos, Guillelmo, Goncharov, Maxim, Gulhan, Doga Can, Kim, Yongsun, Klute, Markus, Lai, Yue Shi, Levin, Andrew Michael, Luckey Jr, P David, Ma, Teng, Nahn, Steven, Paus, Christoph M. E., Ralph, Duncan Kelley, Roland, Christof E, Roland, Gunther M, Stephans, George S. F., Stoeckli, Fabian, Sumorok, Konstanty C, Velicanu, Dragos Alexandru, Wolf, Roger, Wyslouch, Boleslaw, Yang, Ming, Yilmaz, Yetkin, Yoon, A. S., Zanetti, Marco, Wyslouch, Victoria, Department of Physics, Helsinki Institute of Physics, Eija Tuominen / Principal Investigator, Çukurova Üniversitesi, Fen-Edebiyat Fakültesi, Fizik Bölümü, Belforte, S., Candelise, Vieri, Casarsa, M., Cossutti, F., DELLA RICCA, Giuseppe, Gobbo, B., LA LICATA, Chiara, Marone, Matteo, Montanino, Damiana, Penzo, A., Schizzi, Andrea, Umer, Tomo, Zanetti, A., Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), CMS Collaboration, CMS Collaboration (ukupan broj autora: 2222), Karapınar, Güler, Izmir Institute of Technology. Mathematics, Yerevan Phys Inst, Inst Hochenergiephys OeAW, Natl Ctr Particle & High Energy Phys, Univ Antwerp, Vrije Univ Brussel, Univ Libre Brussels, Catholic Univ Louvain, Univ Mons, Centro Brasileiro de Pesquisas Físicas (CBPF), Universidade do Estado do Rio de Janeiro (UERJ), Universidade Estadual Paulista (Unesp), Universidade Federal do ABC (UFABC), Bulgarian Acad Sci, Univ Sofia, Inst High Energy Phys, Peking Univ, Universidad de los Andes, Tech Univ Split, Univ Split, Rudjer Boskovic Inst, Univ Cyprus, Charles Univ Prague, Acad Sci Res & Technol Arab Republ Egypt, NICPB, Univ Helsinki, Helsinki Inst Phys, Lappeenranta Univ Technol, CEA Saclay, Ecole Polytech, Univ Strasbourg, CNRS, Univ Lyon 1, Tbilisi State Univ, RWTH Aachen University, Deutsch Elekt Synchrotron, Univ Hamburg, Univ Karlsruhe, NCSR Demokritos, Univ Athens, Univ Ioannina, Wigner Res Ctr Phys, Inst Nucl Res ATOMKI, Univ Debrecen, Natl Inst Sci Educ & Res, Panjab Univ, University of Delhi, Saha Inst Nucl Phys, Bhabha Atom Res Ctr, Tata Inst Fundamental Res EHEP, Tata Inst Fundamental Res HECR, Inst Res Fundamental Sci IPM, Univ Coll Dublin, Ist Nazl Fis Nucl, Univ Bari, Politecn Bari, Univ Bologna, Univ Catania, CSFNSM, Univ Florence, Univ Genoa, Univ Milano Bicocca, Univ Naples Federico II, Univ Basilicata Potenza, Univ G Marconi Roma, Univ Padua, Univ Trento Trento, Univ Pavia, Univ Perugia, Univ Pisa, Scuola Normale Super Pisa, Univ Rome, Univ Turin, Univ Piemonte Orientale Novara, Univ Trieste, Kangwon Natl Univ, Kyungpook Natl Univ, Chonnam Natl Univ, Korea University, Univ Seoul, Sungkyunkwan Univ, Vilnius Univ, IPN, Univ Iberoamer, Benemerita Univ Autonoma Puebla, Univ Autonoma San Luis Potosi, Univ Auckland, Univ Canterbury, Quaid I Azam Univ, Natl Ctr Nucl Res, Univ Warsaw, Lab Instrumentacao & Fis Expt Particulas, Joint Inst Nucl Res, Petersburg Nucl Phys Inst, Russian Acad Sci, Institute for Theoretical and Experimental Physics (ITEP), PN Lebedev Phys Inst, Moscow MV Lomonosov State Univ, State Res Ctr Russian Federat, University of Belgrade, Vinca Inst Nucl Sci, Ctr Invest Energet Medioambientales & Tecnol CIEM, Univ Autonoma Madrid, Univ Oviedo, Univ Cantabria, CERN, Paul Scherrer Inst, ETH, Univ Zurich, Natl Cent Univ, Natl Taiwan Univ, Chulalongkorn Univ, Cukurova Univ, Middle E Tech Univ, Bogazici Univ, Istanbul Tech Univ, Kharkov Phys & Technol Inst, Univ Bristol, Rutherford Appleton Lab, Univ London Imperial Coll Sci Technol & Med, Brunel Univ, Baylor Univ, Univ Alabama, Boston University, Brown University, Univ Calif Davis, Univ Calif Los Angeles, University of California, Riverside (UCR), Univ Calif San Diego, Univ Calif Santa Barbara, CALTECH, Carnegie Mellon Univ, Univ Colorado, Cornell Univ, Fairfield Univ, Fermilab Natl Accelerator Lab, Univ Florida, Florida Int Univ, Florida State University, Florida Inst Technol, Univ Illinois, Univ Iowa, Johns Hopkins Univ, University of Kansas (KU), Kansas State University, Lawrence Livermore Natl Lab, University of Maryland, MIT, Univ Minnesota, University of Mississippi, Univ Nebraska, SUNY Buffalo, Northeastern University, Northwestern University (NU), Univ Notre Dame, Ohio State Univ, Princeton University, Univ Puerto Rico, Purdue Univ, Purdue University Calumet, Rice University, University of Rochester, Rockefeller Univ, Rutgers State Univ, Univ Tennessee, Texas A&M Univ, Texas Tech Univ, Vanderbilt Univ, University of Virginia (UVA), Wayne State Univ, Univ Wisconsin, Vienna Univ Technol, Universidade Estadual de Campinas (UNICAMP), Zewail City Sci & Technol, Suez Canal Univ, British Univ Egypt, Cairo Univ, Fayoum Univ, Ain Shams Univ, Univ Haute Alsace, Brandenburg Tech Univ Cottbus, Eotvos Lorand Univ, King Abdulaziz Univ, Visva Bharati Univ, Univ Ruhuna, Isfahan Univ Technol, Sharif Univ Technol, Islamic Azad Univ, Univ Siena, Univ Michoacana, St Petersburg State Polytech Univ, Albert Einstein Ctr Fundamental Phys, Gaziosmanpasa Univ, Adiyaman Univ, Mersin Univ, Izmir Inst Technol, Ozyegin Univ, Kafkas Univ, Suleyman Demirel Univ, Ege Univ, Mimar Sinan Univ, Kahramanmaras Sutcu Imam Univ, Univ Southampton, Utah Valley Univ, Argonne Natl Lab, Erzincan Univ, Yildiz Tekn Univ, Texas A&M Univ Qatar, Khachatryan, V. 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Bj, Zucchetta, A. Bj, Gabusi, M. Bk, Ratti, S. P. Bk, Riccardi, C. Bk, Salvini, P. Bk, Vitulo, P. Bk, Biasini, M. Bl, Bilei, G. M. Bl, Ciangottini, D. Bl, Fanò, L. Bl, Lariccia, P. Bl, Mantovani, G. Bl, Menichelli, M. Bl, Romeo, F. Bl, Saha, A. Bl, Santocchia, A. Bl, Spiezia, A. Bl, Androsov, K. Bm, Azzurri, P. Bm, Bagliesi, G. Bm, Bernardini, J. Bm, Boccali, T. Bm, Broccolo, G. Bm, Caiulo, D. Bm, Castaldi, R. Bm, Ciocci, M. A. Bm, Dell’Orso, R. Bm, Donato, S. Bm, Fiori, F. Bm, Foà, L. Bm, Giassi, A. Bm, Grippo, M. T. Bm, Ligabue, Franco, Lomtadze, T. Bm, Martini, L. Bm, Messineo, A. Bm, Moon, C. S. Bm, Palla, F. Bm, Rizzi, A. Bm, Savoy Navarro, A. Bm, Serban, A. T. Bm, Spagnolo, P. Bm, Squillacioti, P. Bm, Tenchini, R. Bm, Tonelli, G. Bm, Venturi, A. Bm, Verdini, P. G. Bm, Vernieri, C. Bm, Barone, L. Bn, Cavallari, F. Bn, D’Imperio, G. Bn, Del Re, D. Bn, Diemoz, M. Bn, Grassi, M. Bn, Jorda, C. Bn, Longo, E. Bn, Margaroli, F. Bn, Meridiani, P. Bn, Micheli, F. Bn, Nourbakhsh, S. 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Br, Kim, T. J. B, Kim, J. Y. Bt, Song, S. Bt, Choi, S. Bu, Gyun, D. Bu, Hong, B. Bu, Jo, M. Bu, Kim, H. Bu, Kim, Y. Bu, Lee, B. Bu, Lee, K. S. Bu, Park, S. K. Bu, Roh, Y. Bu, Choi, M. Bv, Kim, J. H. Bv, Park, I. C. Bv, Park, S. Bv, Ryu, G. Bv, Ryu, M. S. Bv, Choi, Y. Bw, Choi, Y. K. Bw, Goh, J. Bw, Kim, D. Bw, Kwon, E. Bw, Lee, J. Bw, Seo, H. Bw, Yu, I. Bw, Juodagalvis, A. Bx, Komaragiri, J. R. By, Md Ali, M. A. B. By, Castilla Valdez, H. Bz, De La Cruz Burelo, E. Bz, Heredia de La Cruz, I. Bz, Lopez Fernandez, R. Bz, Sanchez Hernandez, A. Bz, Carrillo Moreno, S. Ca, Vazquez Valencia, F. Ca, Pedraza, I. Cb, Salazar Ibarguen, H. A. Cb, Casimiro Linares, E. Cc, Morelos Pineda, A. Cc, Krofcheck, D. Cd, Butler, P. H. Ce, Reucroft, S. Ce, Ahmad, A. Cf, Ahmad, M. Cf, Hassan, Q. Cf, Hoorani, H. R. Cf, Khalid, S. Cf, Khan, W. A. Cf, Khurshid, T. Cf, Shah, M. A. Cf, Shoaib, M. Cf, Bialkowska, H. Cg, Bluj, M. Cg, Boimska, B. Cg, Frueboes, T. Cg, Górski, M. Cg, Kazana, M. Cg, Nawrocki, K. Cg, Romanowska Rybinska, K. Cg, Szleper, M. Cg, Zalewski, P. Cg, Brona, G. Ch, Bunkowski, K. Ch, Cwiok, M. Ch, Dominik, W. Ch, Doroba, K. Ch, Kalinowski, A. Ch, Konecki, M. Ch, Krolikowski, J. Ch, Misiura, M. Ch, Olszewski, M. Ch, Wolszczak, W. Ch, Bargassa, P. Ci, Beirão Da Cruz E. Silva, C. Ci, Faccioli, P. Ci, Ferreira Parracho, P. G. Ci, Gallinaro, M. Ci, Nguyen, F. Ci, Rodrigues Antunes, J. Ci, Seixas, J. Ci, Varela, J. Ci, Vischia, P. Ci, Afanasiev, S. Ci, Bunin, P. Cj, Gavrilenko, M. Cj, Golutvin, I. Cj, Gorbunov, I. Cj, Kamenev, A. Cj, Karjavin, V. Cj, Konoplyanikov, V. Cj, Lanev, A. Cj, Malakhov, A. Cj, Matveev, V. Cj, Moisenz, P. Cj, Palichik, V. Cj, Perelygin, V. Cj, Shmatov, S. Cj, Skatchkov, N. Cj, Smirnov, V. Cj, Zarubin, A. Cj, Golovtsov, V. Ck, Ivanov, Y. Ck, Kim, V. Ck, Levchenko, P. Ck, Murzin, V. Ck, Oreshkin, V. Ck, Smirnov, I. Ck, Sulimov, V. Ck, Uvarov, L. Ck, Vavilov, S. Ck, Vorobyev, A. Ck, Andreev, Y. Cl, Dermenev, A. Cl, Gninenko, S. Cl, Golubev, N. Cl, Kirsanov, M. Cl, Krasnikov, N. Cl, Pashenkov, A. Cl, Tlisov, D. Cl, Toropin, A. Cl, Epshteyn, V. Cm, Gavrilov, V. Cm, Lychkovskaya, N. Cm, Popov, V. Cm, Safronov, G. Cm, Semenov, S. Cm, Spiridonov, A. Cm, Stolin, V. Cm, Vlasov, E. Cm, Zhokin, A. Cm, Andreev, V. Cn, Azarkin, M. Cn, Dremin, I. Cn, Kirakosyan, M. Cn, Leonidov, A. Cn, Mesyats, G. Cn, Rusakov, S. V. Cn, Vinogradov, A. Cn, Belyaev, A. Co, Boos, E. Co, Ershov, A. Co, Gribushin, A. Co, Khein, L. Co, Klyukhin, V. Co, Kodolova, O. Co, Lokhtin, I. Co, Lukina, O. Co, Obraztsov, S. Co, Petrushanko, S. Co, Savrin, V. Co, Snigirev, A. Co, Azhgirey, I. Cp, Bayshev, I. Cp, Bitioukov, S. Cp, Kachanov, V. Cp, Kalinin, A. Cp, Konstantinov, D. Cp, Krychkine, V. Cp, Petrov, V. Cp, Ryutin, R. Cp, Sobol, A. Cp, Tourtchanovitch, L. Cp, Troshin, S. Cp, Tyurin, N. Cp, Uzunian, A. Cp, Volkov, A. Cp, Adzic, P. Cq, Ekmedzic, M. Cq, Milosevic, J. Cq, Rekovic, V. Cq, Alcaraz Maestre, J. Cr, Battilana, C. Cr, Calvo, E. Cr, Cerrada, M. Cr, Chamizo Llatas, M. Cr, Colino, N. Cr, De La Cruz, B. Cr, Delgado Peris, A. Cr, Domínguez Vázquez, D. Cr, Escalante Del Valle, A. Cr, Fernandez Bedoya, C. Cr, Fernández Ramos, J. P. Cr, Flix, J. Cr, Fouz, M. C. Cr, Garcia Abia, P. Cr, Gonzalez Lopez, O. Cr, Goy Lopez, S. Cr, Hernandez, J. M. Cr, Josa, M. I. Cr, Merino, G. Cr, Navarro De Martino, E. Cr, Pérez Calero Yzquierdo, A. Cr, Puerta Pelayo, J. Cr, Quintario Olmeda, A. Cr, Redondo, I. Cr, Romero, L. Cr, Soares, M. S. Cr, Albajar, C. C, de Trocóniz, J. F. C, Missiroli, M. C, Moran, D. C, Brun, H. Ct, Cuevas, J. Ct, Fernandez Menendez, J. Ct, Folgueras, S. Ct, Gonzalez Caballero, I. Ct, Lloret Iglesias, L. Ct, Brochero Cifuentes, J. A. Cu, Cabrillo, I. J. Cu, Calderon, A. Cu, Duarte Campderros, J. Cu, Fernandez, M. Cu, Gomez, G. Cu, Graziano, A. Cu, Lopez Virto, A. Cu, Marco, J. Cu, Marco, R. Cu, Martinez Rivero, C. Cu, Matorras, F. Cu, Munoz Sanchez, F. J. Cu, Piedra Gomez, J. Cu, Rodrigo, T. Cu, Rodríguez Marrero, A. Y. Cu, Ruiz Jimeno, A. Cu, Scodellaro, L. Cu, Vila, I. Cu, Vilar Cortabitarte, R. Cu, Abbaneo, D. Cv, Auffray, E. Cv, Auzinger, G. Cv, Bachtis, M. Cv, Baillon, P. Cv, Ball, A. H. Cv, Barney, D. Cv, Benaglia, A. Cv, Bendavid, J. Cv, Benhabib, L. Cv, Benitez, J. F. Cv, Bernet, C. Cv, Bianchi, G. Cv, Bloch, P. Cv, Bocci, A. Cv, Bonato, A. Cv, Bondu, O. Cv, Botta, C. Cv, Breuker, H. Cv, Camporesi, T. Cv, Cerminara, G. Cv, Colafranceschi, S. Cv, D’Alfonso, M. Cv, D’Enterria, D. Cv, Dabrowski, A. Cv, David, A. Cv, De Guio, F. Cv, De Roeck, A. Cv, De Visscher, S. Cv, Dobson, M. Cv, Dordevic, M. Cv, Dupont Sagorin, N. Cv, Elliott Peisert, A. Cv, Eugster, J. Cv, Franzoni, G. Cv, Funk, W. Cv, Gigi, D. Cv, Gill, K. Cv, Giordano, D. Cv, Girone, M. Cv, Glege, F. Cv, Guida, R. Cv, Gundacker, S. Cv, Guthoff, M. Cv, Hammer, J. Cv, Hansen, M. Cv, Harris, P. Cv, Hegeman, J. Cv, Innocente, V. Cv, Janot, P. Cv, Kousouris, K. Cv, Krajczar, K. Cv, Lecoq, P. Cv, Lourenço, C. Cv, Magini, N. Cv, Malgeri, L. Cv, Mannelli, M. Cv, Marrouche, J. Cv, Masetti, L. Cv, Meijers, F. Cv, Mersi, S. Cv, Meschi, E. Cv, Moortgat, F. Cv, Morovic, S. Cv, Mulders, M. Cv, Musella, P. Cv, Orsini, L. Cv, Pape, L. Cv, Perez, E. Cv, Perrozzi, L. Cv, Petrilli, A. Cv, Petrucciani, G. Cv, Pfeiffer, A. Cv, Pierini, M. Cv, Pimiä, M. Cv, Piparo, D. Cv, Plagge, M. Cv, Racz, A. Cv, Rolandi, G. Cv, Rovere, M. Cv, Sakulin, H. Cv, Schäfer, C. Cv, Schwick, C. Cv, Sharma, A. Cv, Siegrist, P. Cv, Silva, P. Cv, Simon, M. Cv, Sphicas, P. Cv, Spiga, D. Cv, Steggemann, J. Cv, Stieger, B. Cv, Stoye, M. Cv, Takahashi, Y. Cv, Treille, D. Cv, Tsirou, A. Cv, Veres, G. I. Cv, Vlimant, J. R. Cv, Wardle, N. Cv, Wöhri, H. K. Cv, Wollny, H. Cv, Zeuner, W. D. Cv, Bertl, W. Cw, Deiters, K. Cw, Erdmann, W. Cw, Horisberger, R. Cw, Ingram, Q. Cw, Kaestli, H. C. Cw, Kotlinski, D. Cw, Langenegger, U. Cw, Renker, D. Cw, Rohe, T. Cw, Bachmair, F. Cx, Bäni, L. Cx, Bianchini, L. Cx, Bortignon, P. Cx, Buchmann, M. A. Cx, Casal, B. Cx, Chanon, N. 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Fb, Gray, R. Fb, Halkiadakis, E. Fb, Hidas, D. Fb, Kaplan, S. Fb, Lath, A. Fb, Panwalkar, S. Fb, Park, M. Fb, Patel, R. Fb, Salur, S. Fb, Schnetzer, S. Fb, Somalwar, S. Fb, Stone, R. Fb, Thomas, S. Fb, Thomassen, P. Fb, Walker, M. Fb, Rose, K. Fc, Spanier, S. Fc, York, A. Fc, Bouhali, O. Fd, Hernandez, A. C. Fd, Eusebi, R. Fd, Flanagan, W. Fd, Gilmore, J. Fd, Kamon, T. Fd, Khotilovich, V. Fd, Krutelyov, V. Fd, Montalvo, R. Fd, Osipenkov, I. Fd, Pakhotin, Y. Fd, Perloff, A. Fd, Roe, J. Fd, Rose, A. Fd, Safonov, A. Fd, Sakuma, T. Fd, Suarez, I. Fd, Tatarinov, A. Fd, Akchurin, N. Fe, Cowden, C. Fe, Damgov, J. Fe, Dragoiu, C. Fe, Dudero, P. R. Fe, Faulkner, J. Fe, Kovitanggoon, K. Fe, Kunori, S. Fe, Lee, S. W. Fe, Libeiro, T. Fe, Volobouev, I. Fe, Appelt, E. Ff, Delannoy, A. G. Ff, Greene, S. Ff, Gurrola, A. Ff, Johns, W. Ff, Maguire, C. Ff, Mao, Y. Ff, Melo, A. Ff, Sharma, M. Ff, Sheldon, P. Ff, Snook, B. Ff, Tuo, S. Ff, Velkovska, J. Ff, Arenton, M. W. Fg, Boutle, S. Fg, Cox, B. Fg, Francis, B. Fg, Goodell, J. Fg, Hirosky, R. Fg, Ledovskoy, A. Fg, Li, H. Fg, Lin, C. Fg, Neu, C. Fg, Wood, J. Fg, Clarke, C. Fg, Harr, R. Fh, Karchin, P. E. Fh, Kottachchi Kankanamge Don, C. Fh, Lamichhane, P. Fh, Sturdy, J. Fh, Belknap, D. A. Fi, Carlsmith, D. Fi, Cepeda, M. Fi, Dasu, S. Fi, Dodd, L. Fi, Duric, S. Fi, Friis, E. Fi, Hall Wilton, R. Fi, Herndon, M. Fi, Hervé, A. Fi, Klabbers, P. Fi, Lanaro, A. Fi, Lazaridis, C. Fi, Levine, A. Fi, Loveless, R. Fi, Mohapatra, A. Fi, Ojalvo, I. Fi, Perry, T. Fi, Pierro, G. A. Fi, Polese, G. Fi, Ross, I. Fi, Sarangi, T. Fi, Savin, A. Fi, Smith, W. H. Fi, Vuosalo, C. Fi, Woods, N. Fi, UCL - SST/IRMP - Institut de recherche en mathématique et physique, Massachusetts Institute of Technology. School of Science, Bauer, Gerry P., Chan, M., Dutta, V., Kim, Y., Levin, A., Luckey, P. David, Jr., Roland, Christof E., Roland, Gunther M., Stockli, Fabian, Sumorok, Konstanty C., Wolf, R., Yang, M., and Zhukova, Victoria
Subjects: showers [parton], measured [channel cross section], 5 [flavor], Jet physics, Hadron-Hadron Scattering, Jet (particle physics), 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, PARTICLE PHYSICS, LARGE HADRON COLLIDER, CMS, Jets, scattering [p p], [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Parton shower, Monte Carlo, Boson, Physics, Large Hadron Collider, bottom [jet], 3. Good health, Massless particle, CERN LHC Coll, 7000 GeV-cms, Quark, Physique des particules élémentaires, Kinematic properties, LHC, multiplicity [jet], Particle Physics - Experiment, Particle physics, Nuclear and High Energy Physics, Astrophysics::High Energy Astrophysical Phenomena, education, 114 Physical sciences, Nuclear physics, hadroproduction [Z0], 0103 physical sciences, ddc:530, associated production [jet], 010306 general physics, Bosons, Event generator, Nuclear and High Energy Physic, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Jet physic, leptonic decay [Z0], MadGraph, High Energy Physics::Experiment, ratio [cross section], experimental results, Lepton
Abstract: Open Access: This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0).-- et al., The production of a Z boson, decaying into two leptons and produced in association with one or more b jets, is studied using proton-proton collisions delivered by the LHC at a centre-of-mass energy of 7 TeV. The data were recorded in 2011 with the CMS detector and correspond to an integrated luminosity of 5 fb-1. The Z(ℓℓ) + b-jets cross sections (where ℓℓ = μμ or ee) are measured separately for a Z boson produced with exactly one b jet and with at least two b jets. In addition, a cross section ratio is extracted for a Z boson produced with at least one b jet, relative to a Z boson produced with at least one jet. The measured cross sections are compared to various theoretical predictions, and the data favour the predictions in the five-flavour scheme, where b quarks are assumed massless. The kinematic properties of the reconstructed particles are compared with the predictions from the MadGraph event generator using the pythia parton shower simulation., We acknowledge the enduring support for the construction and operation of the LHC and the CMS detector provided by the following funding agencies: the Austrian Federal Ministry of Science and Research; the Belgian Fonds de la Recherche Scientifique, and Fonds voor Wetenschappelijk Onderzoek; the Brazilian Funding Agencies(CNPq, CAPES, FAPERJ, and FAPESP); the Bulgarian Ministry of Education and Science; CERN; the Chinese Academy of Sciences, Ministry of Science and Technology, and National Natural Science Foundation of China; the Colombian Funding Agency (COLCIENCIAS); the Croatian Ministry of Science, Education and Sport; the Research Promotion Foundation, Cyprus; the Ministry of Education and Research, Recurrent financing contract SF0690030s09 and European Regional Development Fund, Estonia; the Academy of Finland, Finnish Ministry of Education and Culture, and Helsinki Institute of Physics; the Institut National de Physique Nucléaire et de Physique des Particules/CNRS, and Commissariat à l’Énergie Atomique et aux Énergies Alternatives/CEA, France; the Bundesministerium für Bildung und Forschung, Deutsche Forschungsgemeinschaft, and Helmholtz-Gemeinschaft Deutscher Forschungszentren, Germany; the General Secretariat for Research and Technology, Greece; the National Scientific Research Foundation, and National Office for Research and Technology, Hungary; the Department of Atomic Energy and the Department of Science and Technology, India; the Institute for Studies in Theoretical Physics and Mathematics, Iran; the Science Foundation, Ireland; the Istituto Nazionale di Fisica Nucleare, Italy; the Korean Ministry of Education, Science and Technology and the World Class University program of NRF, Korea; the Lithuanian Academy of Sciences; the Mexican Funding Agencies (CINVESTAV, CONACYT, SEP, and UASLP-FAI); the Ministry of Science and Innovation, New Zealand; the Pakistan Atomic Energy Commission; the Ministry of Science and Higher Education and the National Science Centre, Poland; the Fundação para a Ciência e a Tecnologia, Portugal; JINR (Armenia, Belarus, Georgia, Ukraine, Uzbekistan); the Ministry of Education and Science of the Russian Federation, the Federal Agency of Atomic Energy of the Russian Federation, Russian Academy of Sciences, and the Russian Foundation for Basic Research; the Ministry of Science and Technological Development of Serbia; the Secretaría de Estado de Investigación, Desarrollo e Innovación and Programa Consolider-Ingenio 2010, Spain; the Swiss Funding Agencies (ETH Board, ETH Zurich, PSI, SNF, UniZH, Canton Zurich, and SER); the National Science Council, Taipei; the Scientific and Technical Research Council of Turkey, and Turkish Atomic Energy Authority; the Science and Technology Facilities Council, UK; the US Department of Energy, and the US National Science Foundation. 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 à la Recherche dans l’Industrie et dans l’Agriculture (FRIA-Belgium); the Agentschap voor Innovatie door Wetenschap en Technologie (IWTBelgium); the Council of Science and Industrial Research, India; the Compagnia di San Paolo (Torino); the HOMING PLUS programme of Foundation for Polish Science, cofinanced from European Union, Regional Development Fund; and the Thalis and Aristeia programmes cofinanced by EU-ESF and the Greek NSRF., Article funded by SCOAP3.
Published: 2014
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24. Galaxy And Mass Assembly (GAMA): Stellar mass functions by Hubble type

Author: Maritza A. Lara-López, Michael J. I. Brown, Aaron S. G. Robotham, Edward N. Taylor, Amanda E. Bauer, Benne W. Holwerda, Ivan K. Baldry, Steven P. Bamford, Alister W. Graham, Mehmet Alpaslan, Anne E. Sansom, Jochen Liske, Christopher J. Conselice, Cristina Popescu, Richard J. Tuffs, Andrew M. Hopkins, Simon P. Driver, Matthew Colless, Joss Bland-Hawthorn, Matthew Prescott, Peder Norberg, Steven Phillipps, Jonathan Loveday, Lee S. Kelvin, Angel R. Lopez-Sanchez, Science & Technology Facilities Council, and University of St Andrews. School of Physics and Astronomy
Subjects: Infrarot-Astrophysik - Abteilung Hofmann, Astrophysics, fundamental parameters [cD galaxies], Structural decomposition, 01 natural sciences, Elliptic galaxies, elliptical and lenticular [Galaxies], QB Astronomy, Astrophysics::Solar and Stellar Astrophysics, Metallicity relation, 10. No inequality, 010303 astronomy & astrophysics, QC, media_common, QB, Physics, education.field_of_study, luminosity function [Galaxies], Star-forming galaxies, Morphological class, Mass function, Stellar mass loss, Kinematic properties, Astrophysics::Earth and Planetary Astrophysics, Stellar mass, media_common.quotation_subject, Luminosity functions, Population, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Type (model theory), 0103 physical sciences, education, Digital sky survey, Astrophysics::Galaxy Astrophysics, spiral [Galaxies], 010308 nuclear & particles physics, Morphological type, Stellar collision, Astronomy, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Galaxy, Universe, Dark-matter Haloes, QC Physics, Space and Planetary Science, Atlas(3D) project, Astrophysics of Galaxies (astro-ph.GA)
Abstract: We present an estimate of the galaxy stellar mass function and its division by morphological type in the local (0.025 < z < 0.06) Universe. Adopting robust morphological classifications as previously presented (Kelvin et al.) for a sample of 3,727 galaxies taken from the Galaxy And Mass Assembly survey, we define a local volume and stellar mass limited sub-sample of 2,711 galaxies to a lower stellar mass limit of M = 10^9.0 M_sun. We confirm that the galaxy stellar mass function is well described by a double Schechter function given by M* = 10^10.64 M_sun, {\alpha}1 = -0.43, {\phi}*1 = 4.18 dex^-1 Mpc^-3, {\alpha}2 = -1.50 and {\phi}*2 = 0.74 dex^-1 Mpc^-3. The constituent morphological-type stellar mass functions are well sampled above our lower stellar mass limit, excepting the faint little blue spheroid population of galaxies. We find approximately 71+3-4% of the stellar mass in the local Universe is found within spheroid dominated galaxies; ellipticals and S0-Sas. The remaining 29+4-3% falls predominantly within late type disk dominated systems, Sab-Scds and Sd-Irrs. Adopting reasonable bulge-to-total ratios implies that approximately half the stellar mass today resides in spheroidal structures, and half in disk structures. Within this local sample, we find approximate stellar mass proportions for E : S0-Sa : Sab-Scd : Sd-Irr of 34 : 37 : 24 : 5., Comment: 16 pages, 6 figures, accepted for publication in MNRAS (see MNRAS version for high-quality figures)
Published: 2014

25. Measurement of the production cross sections for a Z boson and one or more b jets in pp collisions at sqrt{s}= 7 TeV

Author: Chatrchyan, S., Friedl, M., Basegmez, S., Shmatov, S., Shulha, S., Skatchkov, N., Smirnov, V., Tikhonenko, E., Zarubin, A., Evstyukhin, S., Golovtsov, V., Ivanov, Y., Kim, V., Beluffi, C., Levchenko, P., Murzin, V., Oreshkin, V., Smirnov, I., Sulimov, V., Uvarov, L., Vavilov, S., Vorobyev, A., Vorobyev, An., Andreev, Yu., Bruno, G., Dermenev, A., Gninenko, S., Golubev, N., Kirsanov, M., Krasnikov, N., Pashenkov, A., Tlisov, D., Toropin, A., Epshteyn, V., Erofeeva, M., Castello, R., Gavrilov, V., Lychkovskaya, N., Popov, V., Safronov, G., Semenov, S., Spiridonov, A., Stolin, V., Vlasov, E., Zhokin, A., Andreev, V., Caudron, A., Azarkin, M., Dremin, I., Kirakosyan, M., Leonidov, A., Mesyats, G., Rusakov, S. V., Vinogradov, A., Belyaev, A., Boos, E., Bunichev, V., Ceard, L., Dubinin, M., Dudko, L., Ershov, A., Klyukhin, V., Kodolova, O., Lokhtin, I., Markina, A., Obraztsov, S., Petrushanko, S., Savrin, V., Da Silveira, G. G., Snigirev, A., Azhgirey, I., Bayshev, I., Bitioukov, S., Kachanov, V., Kalinin, A., Konstantinov, D., Krychkine, V., Petrov, V., Ryutin, R., Delaere, C., Sobol, A., Tourtchanovitch, L., Troshin, S., Tyurin, N., Uzunian, A., Volkov, A., Adzic, P., Djordjevic, M., Ekmedzic, M., Krpic, D., du Pree, T., Milosevic, J., Aguilar-Benitez, M., Alcaraz Maestre, J., Battilana, C., Calvo, E., Cerrada, M., Chamizo Llatas, M., Colino, N., De La Cruz, B., Delgado Peris, A., Favart, D., Domínguez Vázquez, D., Fernandez Bedoya, C., Fernández Ramos, J. P., Ferrando, A., Flix, J., Fouz, M. C., Garcia-Abia, P., Gonzalez Lopez, O., Goy Lopez, S., Hernandez, J. M., Frühwirth, R., Forthomme, L., Josa, M. I., Merino, G., Navarro De Martino, E., Puerta Pelayo, J., Quintario Olmeda, A., Redondo, I., Romero, L., Santaolalla, J., Soares, M. S., Willmott, C., Giammanco, A., Albajar, C., de Trocóniz, J. F., Brun, H., Cuevas, J., Fernandez Menendez, J., Folgueras, S., Gonzalez Caballero, I., Lloret Iglesias, L., Piedra Gomez, J., Brochero Cifuentes, J. A., Hollar, J., Cabrillo, I. J., Calderon, A., Chuang, S. H., Duarte Campderros, J., Fernandez, M., Gomez, G., Gonzalez Sanchez, J., Graziano, A., Jorda, C., Lopez Virto, A., Jez, P., Marco, J., Marco, R., Martinez Rivero, C., Matorras, F., Munoz Sanchez, F. J., Rodrigo, T., Rodríguez-Marrero, A. Y., Ruiz-Jimeno, A., Scodellaro, L., Vila, I., Lemaitre, V., Vilar Cortabitarte, R., Abbaneo, D., Auffray, E., Auzinger, G., Bachtis, M., Baillon, P., Ball, A. H., Barney, D., Bendavid, J., Benitez, J. F., Liao, J., Bernet, C., Bianchi, G., Bloch, P., Bocci, A., Bonato, A., Bondu, O., Botta, C., Breuker, H., Camporesi, T., Cerminara, G., Militaru, O., Christiansen, T., Coarasa Perez, J. A., Colafranceschi, S., D’Alfonso, M., D’Enterria, D., Dabrowski, A., David, A., De Guio, F., De Roeck, A., De Visscher, S., Nuttens, C., Di Guida, S., Dobson, M., Dupont-Sagorin, N., Elliott-Peisert, A., Eugster, J., Funk, W., Georgiou, G., Giffels, M., Gigi, D., Gill, K., Pagano, D., Giordano, D., Girone, M., Giunta, M., Glege, F., Gomez-Reino Garrido, R., Gowdy, S., Guida, R., Hammer, J., Hansen, M., Harris, P., Pin, A., Hartl, C., Hinzmann, A., Innocente, V., Janot, P., Karavakis, E., Kousouris, K., Krajczar, K., Lecoq, P., Lee, Y.-J., Lourenço, C., Ghete, V. M., Piotrzkowski, K., Magini, N., Malgeri, L., Mannelli, M., Masetti, L., Meijers, F., Mersi, S., Meschi, E., Moser, R., Mulders, M., Musella, P., Popov, A., Nesvold, E., Orsini, L., Palencia Cortezon, E., Perez, E., Perrozzi, L., Petrilli, A., Pfeiffer, A., Pierini, M., Pimiä, M., Piparo, D., Selvaggi, M., Plagge, M., Quertenmont, L., Racz, A., Reece, W., Rolandi, G., Rovere, M., Sakulin, H., Santanastasio, F., Schäfer, C., Schwick, C., Vizan Garcia, J. M., Segoni, I., Sekmen, S., Sharma, A., Siegrist, P., Silva, P., Simon, M., Sphicas, P., Spiga, D., Stoye, M., Tsirou, A., Beliy, N., Veres, G. I., Vlimant, J. R., Wöhri, H. K., Worm, S. D., Zeuner, W. D., Bertl, W., Deiters, K., Erdmann, W., Gabathuler, K., Horisberger, R., Caebergs, T., Ingram, Q., Kaestli, H. C., König, S., Kotlinski, D., Langenegger, U., Renker, D., Rohe, T., Bachmair, F., Bäni, L., Bianchini, L., Daubie, E., Bortignon, P., Buchmann, M. A., Casal, B., Chanon, N., Deisher, A., Dissertori, G., Dittmar, M., Donegà, M., Dünser, M., Eller, P., Hammad, G. H., Freudenreich, K., Grab, C., Hits, D., Lecomte, P., Lustermann, W., Mangano, B., Marini, A. C., Martinez Ruiz del Arbol, P., Meister, D., Mohr, N., Alves, G. A., Moortgat, F., Nägeli, C., Nef, P., Nessi-Tedaldi, F., Pandolfi, F., Pape, L., Pauss, F., Peruzzi, M., Ronga, F. J., Rossini, M., Correa Martins, M., Sala, L., Sanchez, A. K., Starodumov, A., Stieger, B., Takahashi, M., Tauscher, L., Thea, A., Theofilatos, K., Treille, D., Urscheler, C., Hörmann, N., Martins, T., Wallny, R., Weber, H. A., Amsler, C., Chiochia, V., Favaro, C., Ivova Rikova, M., Kilminster, B., Millan Mejias, B., Robmann, P., Snoek, H., Pol, M. E., Taroni, S., Verzetti, M., Yang, Y., Cardaci, M., Chen, K. H., Ferro, C., Kuo, C. M., Li, S. W., Lin, W., Lu, Y. J., Souza, M. H. G., Volpe, R., Yu, S. S., Bartalini, P., Chang, P., Chang, Y. H., Chang, Y. W., Chao, Y., Chen, K. F., Dietz, C., Grundler, U., Aldá, W. L., Hou, W.-S., Hsiung, Y., Kao, K. Y., Lei, Y. J., Lu, R.-S., Majumder, D., Petrakou, E., Shi, X., Shiu, J. G., Tzeng, Y. M., Carvalho, W., Wang, M., Asavapibhop, B., Suwonjandee, N., Adiguzel, A., Bakirci, M. N., Cerci, S., Dozen, C., Dumanoglu, I., Eskut, E., Girgis, S., Chinellato, J., Gokbulut, G., Gurpinar, E., Hos, I., Kangal, E. E., Kayis Topaksu, A., Onengut, G., Ozdemir, K., Ozturk, S., Polatoz, A., Sogut, K., Custódio, A., Sunar Cerci, D., Tali, B., Topakli, H., Vergili, M., Akin, I. V., Aliev, T., Bilin, B., Bilmis, S., Deniz, M., Gamsizkan, H., Da Costa, E. M., Guler, A. M., Karapinar, G., Ocalan, K., Ozpineci, A., Serin, M., Sever, R., Surat, U. E., Yalvac, M., Zeyrek, M., Gülmez, E., De Jesus Damiao, D., Isildak, B., Kaya, M., Kaya, O., Ozkorucuklu, S., Sonmez, N., Bahtiyar, H., Barlas, E., Cankocak, K., Günaydin, Y. O., Vardarlı, F. I., De Oliveira Martins, C., Yücel, M., Levchuk, L., Sorokin, P., Brooke, J. J., Clement, E., Cussans, D., Flacher, H., Frazier, R., Goldstein, J., Grimes, M., Hrubec, J., Fonseca De Souza, S., Heath, G. P., Heath, H. F., Kreczko, L., Lucas, C., Meng, Z., Metson, S., Newbold, D. M., Nirunpong, K., Paramesvaran, S., Poll, A., Malbouisson, H., Senkin, S., Smith, V. J., Williams, T., Bell, K. W., Brew, C., Brown, R. M., Cockerill, D. J. A., Coughlan, J. A., Harder, K., Malek, M., Harper, S., Olaiya, E., Petyt, D., Radburn-Smith, B. C., Shepherdthemistocleous, C. H., Tomalin, I. R., Womersley, W. J., Bainbridge, R., Buchmuller, O., Burton, D., Matos Figueiredo, D., Colling, D., Cripps, N., Cutajar, M., Dauncey, P., Davies, G., Della Negra, M., Ferguson, W., Fulcher, J., Futyan, D., Gilbert, A., Mundim, L., Guneratne Bryer, A., Hall, G., Hatherell, Z., Hays, J., Iles, G., Jarvis, M., Karapostoli, G., Kenzie, M., Lane, R., Lucas, R., Nogima, H., Lyons, L., Magnan, A.-M., Marrouche, J., Mathias, B., Nandi, R., Nash, J., Nikitenko, A., Pela, J., Pesaresi, M., Petridis, K., Prado Da Silva, W. L., Pioppi, M., Raymond, D. M., Rogerson, S., Rose, A., Seez, C., Sharp, P., Sparrow, A., Tapper, A., Vazquez Acosta, M., Virdee, T., Santoro, A., Wakefield, S., Wardle, N., Chadwick, M., Cole, J. E., Hobson, P. R., Khan, A., Kyberd, P., Leggat, D., Leslie, D., Martin, W., Sznajder, A., Reid, I. D., Symonds, P., Teodorescu, L., Turner, M., Dittmann, J., Hatakeyama, K., Kasmi, A., Liu, H., Scarborough, T., Charaf, O., Tonelli Manganote, E. J., Cooper, S. I., Henderson, C., Rumerio, P., Avetisyan, A., Bose, T., Fantasia, C., Heister, A., Lawson, P., Lazic, D., Rohlf, J., Jeitler, M., Vilela Pereira, A., Sperka, D., St John, J. St. John, Sulak, L., Alimena, J., Bhattacharya, S., Christopher, G., Cutts, D., Demiragli, Z., Ferapontov, A., Garabedian, A., Bernardes, C. A., Heintz, U., Jabeen, S., Kukartsev, G., Laird, E., Landsberg, G., Luk, M., Narain, M., Segala, M., Sinthuprasith, T., Speer, T., Dias, F. A., Breedon, R., Breto, G., Calderon De La Barca Sanchez, M., Chauhan, S., Chertok, M., Conway, J., Conway, R., Cox, P. T., Erbacher, R., Gardner, M., Fernandez Perez Tomei, T. R., Houtz, R., Ko, W., Kopecky, A., Lander, R., Miceli, T., Pellett, D., Pilot, J., Ricci-Tam, F., Rutherford, B., Searle, M., Gregores, E. M., Shalhout, S., Smith, J., Squires, M., Tripathi, M., Wilbur, S., Yohay, R., Cline, D., Cousins, R., Erhan, S., Lagana, C., Everaerts, P., Farrell, C., Felcini, M., Hauser, J., Ignatenko, M., Jarvis, C., Rakness, G., Schlein, P., Takasugi, E., Traczyk, P., Mercadante, P. G., Valuev, V., Weber, M., Babb, J., Clare, R., Ellison, J., Gary, J. W., Hanson, G., Heilman, J., Jandir, P., Novaes, S. F., Long, O. R., Luthra, A., Malberti, M., Nguyen, H., Shrinivas, A., Sturdy, J., Sumowidagdo, S., Wilken, R., Wimpenny, S., Andrews, W., Sandra, S. Padula, Branson, J. G., Cerati, G. B., Cittolin, S., Evans, D., Holzner, A., Kelley, R., Lebourgeois, M., Letts, J., Macneill, I., Padhi, S., Genchev, V., Palmer, C., Petrucciani, G., Pieri, M., Sani, M., Sharma, V., Simon, S., Sudano, E., Tadel, M., Tu, Y., Vartak, A., Kiesenhofer, W., Iaydjiev, P., Wasserbaech, S., Würthwein, F., Yagil, A., Yoo, J., Barge, D., Campagnari, C., Danielson, T., Flowers, K., Geffert, P., George, C., Piperov, S., Golf, F., Incandela, J., Justus, C., Kovalskyi, D., Krutelyov, V., Lowette, S., Magaña Villalba, R., Mccoll, N., Pavlunin, V., Richman, J., Rodozov, M., Rossin, R., Stuart, D., To, W., West, C., Apresyan, A., Bornheim, A., Bunn, J., Chen, Y., Di Marco, E., Duarte, J., Sultanov, G., Kcira, D., Ma, Y., Mott, A., Newman, H. B., Pena, C., Rogan, C., Spiropulu, M., Timciuc, V., Veverka, J., Wilkinson, R., Vutova, M., Xie, S., Zhu, R. Y., Azzolini, V., Calamba, A., Carroll, R., Ferguson, T., Iiyama, Y., Jang, D. W., Liu, Y. F., Paulini, M., Dimitrov, A., Russ, J., Vogel, H., Vorobiev, I., Cumalat, J. P., Drell, B. R., Ford, W. T., Gaz, A., Luiggi Lopez, E., Nauenberg, U., Smith, J. G., Hadjiiska, R., Stenson, K., Ulmer, K. A., Wagner, S. R., Alexander, J., Chatterjee, A., Eggert, N., Gibbons, L. K., Hopkins, W., Khukhunaishvili, A., Kreis, B., Kozhuharov, V., Mirman, N., Nicolas Kaufman, G., Patterson, J. R., Ryd, A., Salvati, E., Sun, W., Teo, W. D., Thom, J., Thompson, J., Tucker, J., Litov, L., Weng, Y., Winstrom, L., Wittich, P., Winn, D., Abdullin, S., Albrow, M., Anderson, J., Apollinari, G., Bauerdick, L. A. T., Beretvas, A., Pavlov, B., Berryhill, J., Bhat, P. C., Burkett, K., Butler, J. N., Chetluru, V., Cheung, H. W. K., Chlebana, F., Cihangir, S., Elvira, V. D., Fisk, I., Knünz, V., Petkov, P., Freeman, J., Gao, Y., Gottschalk, E., Gray, L., Green, D., Gutsche, O., Hare, D., Harris, R. M., Hirschauer, J., Hooberman, B., Bian, J. G., Jindariani, S., Johnson, M., Joshi, U., Kaadze, K., Klima, B., Kunori, S., Kwan, S., Linacre, J., Lincoln, D., Lipton, R., Chen, G. M., Lykken, J., Maeshima, K., Marraffino, J. M., Martinez Outschoorn, V. I., Maruyama, S., Mason, D., Mcbride, P., Mishra, K., Mrenna, S., Musienko, Y., Chen, H. S., Newman-Holmes, C., O’Dell, V., Prokofyev, O., Ratnikova, N., Sexton-Kennedy, E., Sharma, S., Spalding, W. J., Spiegel, L., Taylor, L., Tkaczyk, S., Jiang, C. H., Tran, N. V., Uplegger, L., Vaandering, E. W., Vidal, R., Whitmore, J., Wu, W., Yang, F., Yun, J. C., Acosta, D., Avery, P., Liang, D., Bourilkov, D., Chen, M., Cheng, T., Das, S., De Gruttola, M., Di Giovanni, G. P., Dobur, D., Drozdetskiy, A., Field, R. D., Fisher, M., Liang, S., Fu, Y., Furic, I. K., Hugon, J., Kim, B., Konigsberg, J., Korytov, A., Kropivnitskaya, A., Kypreos, T., Low, J. F., Matchev, K., Meng, X., Milenovic, P., Mitselmakher, G., Muniz, L., Remington, R., Rinkevicius, A., Skhirtladze, N., Snowball, M., Yelton, J., Zakaria, M., Gaultney, V., Tao, J., Hewamanage, S., Linn, S., Markowitz, P., Martinez, G., Rodriguez, J. L., Adams, T., Askew, A., Bochenek, J., Chen, J., Diamond, B., Wang, X., Gleyzer, S. V., Haas, J., Hagopian, S., Hagopian, V., Johnson, K. F., Prosper, H., Veeraraghavan, V., Weinberg, M., Baarmand, M. M., Dorney, B., Krammer, M., Wang, Z., Hohlmann, M., Kalakhety, H., Yumiceva, F., Adams, M. R., Apanasevich, L., Bazterra, V. E., Betts, R. R., Bucinskaite, I., Callner, J., Cavanaugh, R., Xiao, H., Evdokimov, O., Gauthier, L., Gerber, C. E., Hofman, D. J., Khalatyan, S., Kurt, P., Lacroix, F., Moon, D. H., O’Brien, C., Silkworth, C., Asawatangtrakuldee, C., Strom, D., Turner, P., Varelas, N., Akgun, U., Albayrak, E. A., Bilki, B., Clarida, W., Dilsiz, K., Duru, F., Griffiths, S., Ban, Y., Merlo, J.-P., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Newsom, C. R., Ogul, H., Onel, Y., Ozok, F., Sen, S., Guo, Y., Tan, P., Tiras, E., Wetzel, J., Yetkin, T., Yi, K., Barnett, B. A., Blumenfeld, B., Bolognesi, S., Giurgiu, G., Gritsan, A. V., Li, Q., Hu, G., Maksimovic, P., Martin, C., Swartz, M., Whitbeck, A., Baringer, P., Bean, A., Benelli, G., Kenny, R. P., Murray, M., Li, W., Noonan, D., Sanders, S., Stringer, R., Wood, J. S., Barfuss, A. F., Chakaberia, I., Ivanov, A., Khalil, S., Makouski, M., Maravin, Y., Liu, S., Saini, L. K., Shrestha, S., Svintradze, I., Gronberg, J., Lange, D., Rebassoo, F., Wright, D., Baden, A., Calvert, B., Eno, S. C., Mao, Y., Gomez, J. A., Hadley, N. J., Kellogg, R. G., Kolberg, T., Lu, Y., Marionneau, M., Mignerey, A. C., Pedro, K., Peterman, A., Skuja, A., Qian, S. J., Temple, J., Tonjes, M. B., Tonwar, S. C., Apyan, A., Bauer, G., Busza, W., Cali, I. A., Chan, M., Di Matteo, L., Dutta, V., Krätschmer, I., Wang, D., Gomez Ceballos, G., Goncharov, M., Gulhan, D., Kim, Y., Klute, M., Lai, Y. S., Levin, A., Luckey, P. D., Ma, T., Nahn, S., Zhang, L., Paus, C., Ralph, D., Roland, C., Roland, G., Stephans, G. S. F., Stöckli, F., Sumorok, K., Velicanu, D., Wolf, R., Wyslouch, B., Zou, W., Yang, M., Yilmaz, Y., Yoon, A. S., Zanetti, M., Zhukova, V., Dahmes, B., De Benedetti, A., Franzoni, G., Gude, A., Haupt, J., Avila, C., Kao, S. C., Klapoetke, K., Kubota, Y., Mans, J., Pastika, N., Rusack, R., Sasseville, M., Singovsky, A., Tambe, N., Turkewitz, J., Carrillo Montoya, C. A., Acosta, J. G., Cremaldi, L. M., Kroeger, R., Oliveros, S., Perera, L., Rahmat, R., Sanders, D. A., Summers, D., Avdeeva, E., Bloom, K., Chaparro Sierra, L. F., Bose, S., Claes, D. R., Dominguez, A., Eads, M., Gonzalez Suarez, R., Keller, J., Kravchenko, I., Lazo-Flores, J., Malik, S., Meier, F., Gomez, J. P., Snow, G. R., Dolen, J., Godshalk, A., Iashvili, I., Jain, S., Kharchilava, A., Kumar, A., Rappoccio, S., Wan, Z., Alverson, G., Gomez Moreno, B., Barberis, E., Baumgartel, D., Chasco, M., Haley, J., Massironi, A., Nash, D., Orimoto, T., Trocino, D., Wood, D., Zhang, J., Sanabria, J. C., Anastassov, A., Hahn, K. A., Kubik, A., Lusito, L., Mucia, N., Odell, N., Pollack, B., Pozdnyakov, A., Schmitt, M., Stoynev, S., Godinovic, N., Sung, K., Velasco, M., Won, S., Berry, D., Brinkerhoff, A., Chan, K. M., Hildreth, M., Jessop, C., Karmgard, D. J., Kolb, J., Khachatryan, V., Liko, D., Lelas, D., Lannon, K., Luo, W., Lynch, S., Marinelli, N., Morse, D. M., Pearson, T., Planer, M., Ruchti, R., Slaunwhite, J., Valls, N., Plestina, R., Wayne, M., Wolf, M., Antonelli, L., Bylsma, B., Durkin, L. S., Hill, C., Hughes, R., Kotov, K., Ling, T. Y., Puigh, D., Polic, D., Rodenburg, M., Smith, G., Vuosalo, C., Winer, B. L., Wolfe, H., Berry, E., Elmer, P., Halyo, V., Hebda, P., Hegeman, J., Puljak, I., Hunt, A., Jindal, P., Koay, S. A., Lujan, P., Marlow, D., Medvedeva, T., Mooney, M., Olsen, J., Piroué, P., Quan, X., Antunovic, Z., Raval, A., Saka, H., Stickland, D., Tully, C., Werner, J. S., Zenz, S. C., Zuranski, A., Brownson, E., Lopez, A., Mendez, H., Kovac, M., Ramirez Vargas, J. E., Alagoz, E., Benedetti, D., Bolla, G., Bortoletto, D., De Mattia, M., Everett, A., Hu, Z., Jones, M., Jung, K., Brigljevic, V., Koybasi, O., Kress, M., Leonardo, N., Lopes Pegna, D., Maroussov, V., Merkel, P., Miller, D. H., Neumeister, N., Shipsey, I., Silvers, D., Kadija, K., Svyatkovskiy, A., Vidal Marono, M., Wang, F., Xie, W., Xu, L., Yoo, H. D., Zablocki, J., Zheng, Y., Parashar, N., Adair, A., Luetic, J., Akgun, B., Ecklund, K. M., Geurts, F. J. M., Michlin, B., Padley, B. P., Redjimi, R., Roberts, J., Zabel, J., Betchart, B., Mekterovic, D., Bodek, A., Covarelli, R., de Barbaro, P., Demina, R., Eshaq, Y., Ferbel, T., Garcia-Bellido, A., Goldenzweig, P., Han, J., Harel, A., Mikulec, I., Morovic, S., Miner, D. C., Petrillo, G., Vishnevskiy, D., Zielinski, M., Bhatti, A., Ciesielski, R., Demortier, L., Goulianos, K., Lungu, G., Tikvica, L., Mesropian, C., Arora, S., Barker, A., Chou, J. P., Contreras-Campana, C., Contreras-Campana, E., Duggan, D., Ferencek, D., Gershtein, Y., Gray, R., Attikis, A., Halkiadakis, E., Hidas, D., Lath, A., Panwalkar, S., Park, M., Patel, R., Rekovic, V., Robles, J., Salur, S., Schnetzer, S., Mavromanolakis, G., Seitz, C., Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Cerizza, G., Hollingsworth, M., Rose, K., Spanier, S., Mousa, J., Yang, Z. C., York, A., Bouhali, O., Eusebi, R., Flanagan, W., Gilmore, J., Kamon, T., Khotilovich, V., Montalvo, R., Osipenkov, I., Nicolaou, C., Pakhotin, Y., Perloff, A., Roe, J., Safonov, A., Sakuma, T., Suarez, I., Tatarinov, A., Toback, D., Akchurin, N., Cowden, C., Ptochos, F., Damgov, J., Dragoiu, C., Dudero, P. R., Kovitanggoon, K., Lee, S. W., Libeiro, T., Volobouev, I., Appelt, E., Delannoy, A. G., Greene, S., Razis, P. A., Gurrola, A., Johns, W., Maguire, C., Melo, A., Sharma, M., Sheldon, P., Snook, B., Tuo, S., Velkovska, J., Finger, M., Arenton, M. W., Boutle, S., Cox, B., Francis, B., Goodell, J., Hirosky, R., Ledovskoy, A., Lin, C., Neu, C., Wood, J., Gollapinni, S., Harr, R., Karchin, P. E., Kottachchi Kankanamge Don, C., Lamichhane, P., Sakharov, A., Belknap, D. A., Borrello, L., Carlsmith, D., Cepeda, M., Rabady, D., Abdelalim, A. 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S., Clerbaux, B., Colaleo, A., Creanza, D., De Filippis, N., De Palma, M., Fiore, L., Iaselli, G., Maggi, G., Maggi, M., Marangelli, B., My, S., De Lentdecker, G., Nuzzo, S., Pacifico, N., Pompili, A., Pugliese, G., Selvaggi, G., Silvestris, L., Singh, G., Venditti, R., Verwilligen, P., Zito, G., Favart, L., Abbiendi, G., Benvenuti, A. C., Bonacorsi, D., Braibant-Giacomelli, S., Brigliadori, L., Campanini, R., Capiluppi, P., Castro, A., Cavallo, F. R., Codispoti, G., Gay, A. P. R., Cuffiani, M., Dallavalle, G. M., Fabbri, F., Fanfani, A., Fasanella, D., Giacomelli, P., Grandi, C., Guiducci, L., Marcellini, S., Masetti, G., Hreus, T., Meneghelli, M., Montanari, A., Navarria, F. L., Odorici, F., Perrotta, A., Primavera, F., Rossi, A. M., Rovelli, T., Siroli, G. P., Tosi, N., Dragicevic, M., Léonard, A., Travaglini, R., Albergo, S., Chiorboli, M., Costa, S., Giordano, F., Potenza, R., Tricomi, A., Tuve, C., Barbagli, G., Ciulli, V., Marage, P. E., Civinini, C., D’Alessandro, R., Focardi, E., Frosali, S., Gallo, E., Gonzi, S., Gori, V., Lenzi, P., Meschini, M., Paoletti, S., Mohammadi, A., Sguazzoni, G., Tropiano, A., Benussi, L., Bianco, S., Piccolo, D., Fabbricatore, P., Ferretti, R., Ferro, F., Lo Vetere, M., Perniè, L., Musenich, R., Robutti, E., Tosi, S., Benaglia, A., Dinardo, M. E., Fiorendi, S., Gennai, S., Ghezzi, A., Govoni, P., Lucchini, M. T., Reis, T., Malvezzi, S., Manzoni, R. A., Martelli, A., Menasce, D., Moroni, L., Paganoni, M., Pedrini, D., Ragazzi, S., Redaelli, N., Tabarelli de Fatis, T., Seva, T., Buontempo, S., Cavallo, N., De Cosa, A., Fabozzi, F., Iorio, A. O. M., Lista, L., Meola, S., Merola, M., Paolucci, P., Azzi, P., Thomas, L., Bacchetta, N., Biasotto, M., Bisello, D., Branca, A., Carlin, R., Checchia, P., Dorigo, T., Fanzago, F., Galanti, M., Gasparini, F., Vander Velde, C., Gasparini, U., Giubilato, P., Gonella, F., Gozzelino, A., Kanishchev, K., Lacaprara, S., Lazzizzera, I., Margoni, M., Meneguzzo, A. T., Montecassiano, F., Vanlaer, P., Pazzini, J., Pozzobon, N., Ronchese, P., Simonetto, F., Torassa, E., Tosi, M., Vanini, S., Zotto, P., Zucchetta, A., Zumerle, G., Wang, J., Gabusi, M., Ratti, S. P., Riccardi, C., Vitulo, P., Biasini, M., Bilei, G. M., Fanò, L., Lariccia, P., Mantovani, G., Menichelli, M., Erö, J., Adler, V., Nappi, A., Romeo, F., Saha, A., Santocchia, A., Spiezia, A., Androsov, K., Azzurri, P., Bagliesi, G., Bernardini, J., Boccali, T., Beernaert, K., Broccolo, G., Castaldi, R., Ciocci, M. A., D’Agnolo, R. T., Dell’Orso, R., Fiori, F., Foà, L., Giassi, A., Grippo, M. T., Kraan, A., Benucci, L., Ligabue, F., Lomtadze, T., Martini, L., Messineo, A., Moon, C. S., Palla, F., Rizzi, A., Savoy-Navarro, A., Serban, A. T., Spagnolo, P., Cimmino, A., Squillacioti, P., Tenchini, R., Tonelli, G., Venturi, A., Verdini, P. G., Vernieri, C., Barone, L., Cavallari, F., Del Re, D., Diemoz, M., Costantini, S., Grassi, M., Longo, E., Margaroli, F., Meridiani, P., Micheli, F., Nourbakhsh, S., Organtini, G., Paramatti, R., Rahatlou, S., Rovelli, C., Dildick, S., Soffi, L., Amapane, N., Arcidiacono, R., Argiro, S., Arneodo, M., Bellan, R., Biino, C., Cartiglia, N., Casasso, S., Costa, M., Garcia, G., Degano, A., Demaria, N., Mariotti, C., Maselli, S., Migliore, E., Monaco, V., Musich, M., Obertino, M. M., Pastrone, N., Pelliccioni, M., Klein, B., Potenza, A., Romero, A., Ruspa, M., Sacchi, R., Solano, A., Staiano, A., Tamponi, U., Belforte, S., Candelise, V., Casarsa, M., Lellouch, J., Cossutti, F., Della Ricca, G., Gobbo, B., La Licata, C., Marone, M., Montanino, D., Penzo, A., Schizzi, A., Zanetti, A., Chang, S., Marinov, A., Kim, T. Y., Nam, S. K., Kim, D. H., Kim, G. N., Kim, J. E., Kong, D. J., Lee, S., Oh, Y. D., Park, H., Son, D. C., Fabjan, C., Mccartin, J., Kim, J. Y., Zero, J. Kim, Song, S., Choi, S., Gyun, D., Hong, B., Jo, M., Kim, H., Kim, T. J., Lee, K. S., Ocampo Rios, A. A., Park, S. K., Roh, Y., Choi, M., Kim, J. H., Park, C., Park, I. C., Park, S., Ryu, G., Choi, Y., Choi, Y. K., Ryckbosch, D., Goh, J., Kim, M. S., Kwon, E., Lee, B., Lee, J., Seo, H., Yu, I., Grigelionis, I., Juodagalvis, A., Sigamani, M., Castilla-Valdez, H., De La Cruz-Burelo, E., Heredia-de La Cruz, I., Lopez-Fernandez, R., Martínez-Ortega, J., Sanchez-Hernandez, A., Villasenor-Cendejas, L. M., Carrillo Moreno, S., Vazquez Valencia, F., Salazar Ibarguen, H. A., Strobbe, N., Casimiro Linares, E., Morelos Pineda, A., Reyes-Santos, M. A., Krofcheck, D., Butler, P. H., Doesburg, R., Reucroft, S., Silverwood, H., Ahmad, M., Asghar, M. I., Thyssen, F., Butt, J., Hoorani, H. R., Khan, W. A., Khurshid, T., Qazi, S., Shah, M. A., Shoaib, M., Bialkowska, H., Boimska, B., Frueboes, T., Tytgat, M., Górski, M., Kazana, M., Nawrocki, K., Romanowska-Rybinska, K., Szleper, M., Wrochna, G., Zalewski, P., Brona, G., Bunkowski, K., Cwiok, M., Walsh, S., Dominik, W., Doroba, K., Kalinowski, A., Konecki, M., Krolikowski, J., Misiura, M., Wolszczak, W., Almeida, N., Bargassa, P., Beirão Da Cruz E Silva, C., Yazgan, E., Faccioli, P., Ferreira Parracho, P. G., Gallinaro, M., Nguyen, F., Rodrigues Antunes, J., Seixas, J., Varela, J., Vischia, P., Golutvin, I., Gorbunov, I., Zaganidis, N., Karjavin, V., Konoplyanikov, V., Korenkov, V., Kozlov, G., Lanev, A., Malakhov, A., Matveev, V., Moisenz, P., Palichik, V., Perelygin, V., Karapınar, Güler, İYTE, Fen Fakültesi, Matematik Bölümü, SCOAP, and UCL - SST/IRMP - Institut de recherche en mathématique et physique
Subjects: showers [parton], measured [channel cross section], 5 [flavor], 114 Physical sciences, PARTICLE PHYSICS, LARGE HADRON COLLIDER, CMS, High Energy Physics - Experiment, hadroproduction [Z0], Jets, scattering [p p], ddc:530, associated production [jet], Monte Carlo, Bosons, Hadron-Hadron Scattering, Physics, leptonic decay [Z0], bottom [jet], MadGraph, CERN LHC Coll, Jet physics, 7000 GeV-cms, Quark, Kinematic properties, LHC, ratio [cross section], multiplicity [jet], Particle Physics - Experiment, experimental results
Abstract: We acknowledge the enduring support for the construction and operation of the LHC and the CMS detector provided by the following funding agencies: the Austrian Federal Ministry of Science and Research; the Belgian Fonds de la Recherche Scientifique, and Fonds voor Wetenschappelijk Onderzoek; the Brazilian Funding Agencies(CNPq, CAPES, FAPERJ, and FAPESP); the Bulgarian Ministry of Education and Science; CERN; the Chinese Academy of Sciences, Ministry of Science and Technology, and National Natural Science Foundation of China; the Colombian Funding Agency (COLCIENCIAS); the Croatian Ministry of Science, Education and Sport; the Research Promotion Foundation, Cyprus; the Ministry of Education and Research, Recurrent financing contract SF0690030s09 and European Regional Development Fund, Estonia; the Academy of Finland, Finnish Ministry of Education and Culture, and Helsinki Institute of Physics; the Institut National de Physique Nucléaire et de Physique des Particules/CNRS, and Commissariat à l’Énergie Atomique et aux Énergies Alternatives/CEA, France; the Bundesministerium für Bildung und Forschung, Deutsche Forschungsgemeinschaft, and Helmholtz-Gemeinschaft Deutscher Forschungszentren, Germany; the General Secretariat for Research and Technology, Greece; the National Scientific Research Foundation, and National Office for Research and Technology, Hungary; the Department of Atomic Energy and the Department of Science and Technology, India; the Institute for Studies in Theoretical Physics and Mathematics, Iran; the Science Foundation, Ireland; the Istituto Nazionale di Fisica Nucleare, Italy; the Korean Ministry of Education, Science and Technology and the World Class University program of NRF, Korea; the Lithuanian Academy of Sciences; the Mexican Funding Agencies (CINVESTAV, CONACYT, SEP, and UASLP-FAI); the Ministry of Science and Innovation, New Zealand; the Pakistan Atomic Energy Commission; the Ministry of Science and Higher Education and the National Science Centre, Poland; the Fundação para a Ciência e a Tecnologia, Portugal; JINR (Armenia, Belarus, Georgia, Ukraine, Uzbekistan); the Ministry of Education and Science of the Russian Federation, the Federal Agency of Atomic Energy of the Russian Federation, Russian Academy of Sciences, and the Russian Foundation for Basic Research; the Ministry of Science and Technological Development of Serbia; the Secretaría de Estado de Investigación, Desarrollo e Innovación and Programa Consolider-Ingenio 2010, Spain; the Swiss Funding Agencies (ETH Board, ETH Zurich, PSI, SNF, UniZH, Canton Zurich, and SER); the National Science Council, Taipei; the Scientific and Technical Research Council of Turkey, and Turkish Atomic Energy Authority; the Science and Technology Facilities Council, UK; the US Department of Energy, and the US National Science Foundation. 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 à la Recherche dans l’Industrie et dans l’Agriculture (FRIA-Belgium); the Agentschap voor Innovatie door Wetenschap en Technologie (IWTBelgium); the Council of Science and Industrial Research, India; the Compagnia di San Paolo (Torino); the HOMING PLUS programme of Foundation for Polish Science, cofinanced from European Union, Regional Development Fund; and the Thalis and Aristeia programmes cofinanced by EU-ESF and the Greek NSRF.
Published: 2014
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26. Evidence for associated production of a single top quark and W Boson in pp collisions at √s=7 TeV

Author: Chatrchyan, Serguei, Clerbaux, Barbara, De Lentdecker, Gilles, Dero, Vincent, Gay, Arnaud, Hreus, Tomas, Leonard, Alexandre, Marage, Pierre, Mohammadi, Abdollah, Reis, Thomas, Thomas, Laurent, Vander Marcken, G, Vander Velde, Catherine, Vanlaer, Pascal, and Wang, Jian
Subjects: Multi variate analysis, Integrated luminosity, Nonlinear Sciences::Exactly Solvable and Integrable Systems, High Energy Physics::Lattice, The standard model, Bosons, High Energy Physics::Phenomenology, Physics::Atomic and Molecular Clusters, Physique des particules élémentaires, Kinematic properties, Computer Science::Computers and Society, Tellurium compounds, High energy physics
Abstract: Evidence is presented for the associated production of a single top quark and W boson in pp collisions at âs, 0, info:eu-repo/semantics/published
Published: 2013

27. Monitoring and data quality assessment of the ATLAS liquid argon calorimeter

Author: Aad, G., Jovicevic, Jelena, Kuwertz, Emma S., Lund-Jensen, Bengt, Morley, Anthony K., Strandberg, Jonas, Zwalinski, L., et al., Aad, G., Jovicevic, Jelena, Kuwertz, Emma S., Lund-Jensen, Bengt, Morley, Anthony K., Strandberg, Jonas, Zwalinski, L., and et al.
Abstract: The liquid argon calorimeter is a key component of the ATLAS detector installed at the CERN Large Hadron Collider. The primary purpose of this calorimeter is the measurement of electron and photon kinematic properties. It also provides a crucial input for measuring jets and missing transverse momentum. An advanced data monitoring procedure was designed to quickly identify issues that would affect detector performance and ensure that only the best quality data are used for physics analysis. This article presents the validation procedure developed during the 2011 and 2012 LHC data-taking periods, in which more than 98% of the proton-proton luminosity recorded by ATLAS at a centre-of-mass energy of 7-8 TeV had calorimeter data quality suitable for physics analysis., QC 20141010
Published: 2014
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28. Student Session 27/28: Kaon Identification in the ALICE TPC using Kink Topology

Published: 2010

29. Galactic bulges from Hubble Space Telescope NICMOS observations: Global scaling relations

Author: Balcells, Marc, Graham, Alister W., Peletier, Reynier F., and Kapteyn Astronomical Institute
Subjects: VELOCITY DISPERSIONS, DWARF ELLIPTIC GALAXIES, Astrophysics::Cosmology and Extragalactic Astrophysics, BAND SURFACE PHOTOMETRY, KINEMATIC PROPERTIES, DISK-DOMINATED GALAXIES, STRUCTURAL PARAMETERS, COLD DARK-MATTER, FUNDAMENTAL PLANE, galaxies : structure, EARLY-TYPE GALAXIES, galaxies : spiral, Astrophysics::Earth and Planetary Astrophysics, SPIRAL GALAXIES, Astrophysics::Galaxy Astrophysics
Abstract: We investigate bulge and disk scaling relations using a volume-corrected sample of early-to intermediate-type disk galaxies in which, importantly, the biasing flux from additional nuclear components has been modeled and removed. Structural parameters are obtained from a seeing-convolved, bulge + disk + nuclear-component decomposition applied to near-infrared surface brightness profiles spanning similar to 10 pc to the outer disk. Bulge and disk parameters, and bulge-to-disk ratios, are analyzed as a function of bulge luminosity, disk luminosity, galaxy central velocity dispersion, and galaxy Hubble type. Mathematical expressions are given for the stronger relations, which can be used to test and constrain galaxy formation models. Photometric parameters of both bulges and disks are observed to correlate with bulge luminosity and with central velocity dispersion. In contrast, for the unbarred, early to intermediate types covered by the sample, Hubble type does not correlate with bulge and disk components, nor their various ratios. In this sense, the early-to-intermediate spiral Hubble sequence is scale free. However, galaxies themselves are not scale free, the critical scale being the luminosity of the bulge. Bulge luminosity is shown to affect the disk parameters, such that central surface brightness becomes fainter, and scale length bigger, with bulge luminosity. The lack of significant correlations between bulge parameters (size, luminosity, or density) on disk luminosity, remains a challenge for secular evolution models of bulge growth. The average near-infrared bulge-to-total flux ratio for our S0-S0a galaxies is 0.25 (+/- 0.09).
Published: 2007

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29 results on '"Kinematic properties"'

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29 results on '"Kinematic properties"'

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