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1. Reduced Length of Stay Following Patient Pathway Optimization for Primary Hip and Knee Arthroplasty at a Swiss Hospital

Author: Edelmann L, Hempel M, Podsiadlo N, Schweizer N, Tong C, Galvain T, Taylor H, and Schüler M
Subjects: enhanced recovery program, total hip replacement, total knee replacement, joint replacement, costs, Medicine (General), R5-920, Therapeutics. Pharmacology, RM1-950
Abstract: Lars Edelmann,1 Marike Hempel,2 Natalia Podsiadlo,1 Nora Schweizer,2 Cindy Tong,3 Thibaut Galvain,4 Hannah Taylor,5 Michael Schüler1 1Kantonsspital Münsterlingen, Münsterlingen, 8596, Switzerland; 2Johnson & Johnson AG, Zug, 6300, Switzerland; 3Johnson and Johnson Medical Devices, Somerville, NJ, USA; 4Johnson and Johnson Medical, Issy les Moulineaux, France; 5Johnson & Johnson Medical Limited, Berkshire, UKCorrespondence: Lars Edelmann, Klinik für Orthopädie und Traumatologie, Kantonsspital Münsterlingen, Spitalcampus 1, Münsterlingen, 8596, Switzerland, Tel +41-71-686-20 50, Fax +41-71-686-20 23, Email lars.edelmann@stgag.chPurpose: Total knee and hip arthroplasties (TKA and THA) are common surgical procedures in Switzerland and worldwide. Alongside increasing demand for these procedures, many providers have adopted enhanced recovery programs (ERPs) that aim to optimize recovery after these surgeries. We evaluated the impact of implementing a Patient Pathway Optimization (PPO) program designed around ERP principles for patients undergoing TKA or THA in a Swiss Cantonal hospital. The primary objective was to determine whether PPO implementation for patients undergoing TKA or THA reduced length of stay (LOS) during index hospitalization. Additional study outcomes were hospital inpatient costs, rate of complications and readmissions, and patient discharge destination.Methods: This was a retrospective, observational study comparing outcomes before and after PPO implementation for patients who underwent primary TKA or THA from 2014 to 2019. The PPO program modified the care pathway and implemented five ERP principles (preoperative patient education, pre-operative physiotherapy, local infiltration analgesia, early mobilization, and oral analgesia). Hospital electronic medical record and billing data were used for the analysis.Results: After implementation of PPO, LOS was shorter compared with the pre-PPO period (reduction of 2.5 and 2.4 days in TKA and THA cohorts, respectively, both p < 0.001). Mean inpatient costs per patient were also reduced following PPO (decrease of USD2016 [p = 0.015] and USD340 [p = 0.54] for TKA and THA cohorts, respectively). There were no observed increases in readmissions or complications after PPO implementation in either the TKA or THA cohort. More patients in the post-PPO groups were discharged to home vs an alternative health-care setting than in the pre-PPO groups (TKA, 83.8% vs 68.4% [p = 0.07]; THA, 80.4% vs 73.9%, [p = 0.31]).Conclusion: Patient pathway optimization and implementation of additional enhanced recovery principles for TKA and THA may benefit both health systems and patients, by reducing LOS and costs without increases in complications or readmissions.Keywords: enhanced recovery program, total hip replacement, total knee replacement, joint replacement, costs
Published: 2022

2. The VISTA Variables in the V\'ia L\'actea eXtended (VVVX) ESO public survey: Completion of the observations and legacy

Author: Saito, R. K., Hempel, M., Alonso-García, J., Lucas, P. W., Minniti, D., Alonso, S., Baravalle, L., Borissova, J., Caceres, C., Chené, A. N., Cross, N. J. G., Duplancic, F., Garro, E. R., Gómez, M., Ivanov, V. D., Kurtev, R., Luna, A., Majaess, D., Navarro, M. G., Pullen, J. B., Rejkuba, M., Sanders, J. L., Smith, L. C., Albino, P. H. C., Alonso, M. V., Amôres, E. B., Angeloni, R., Arias, J. I., Arnaboldi, M., Barbuy, B., Bayo, A., Beamin, J. C., Bedin, L. R., Bellini, A., Benjamin, R. A., Bica, E., Bonatto, C. J., Botan, E., Braga, V. F., Brown, D. A., Cabral, J. B., Camargo, D., Garatti, A. Caratti o, Carballo-Bello, J. A., Catelan, M., Chavero, C., Chijani, M. A., Clariá, J. J., Coldwell, G. V., Peña, C. Contreras, Ramos, R. Contreras, Corral-Santana, J. M., Cortés, C. C., Cortés-Contreras, M., Cruz, P., Daza-Perilla, I. V., Debattista, V. P., Dias, B., Donoso, L., D'Souza, R., Emerson, J. P., Federle, S., Fermiano, V., Fernandez, J., Fernández-Trincado, J. G., Ferreira, T., Lopes, C. E. Ferreira, Firpo, V., Flores-Quintana, C., Fraga, L., Froebrich, D., Galdeano, D., Gavignaud, I., Geisler, D., Gerhard, O. E., Gieren, W., Gonzalez, O. A., Gramajo, L. V., Gran, F., Granitto, P. M., Griggio, M., Guo, Z., Gurovich, S., Hilker, M., Jones, H. R. A., Kammers, R., Kuhn, M. A., Kumar, M. S . N., Kundu, R., Lares, M., Libralato, M., Lima, E., Maccarone, T. J., Cortés, P. Marchant, Martin, E. L., Masetti, N., Matsunaga, N., Mauro, F., McDonald, I., Mejías, A., Mesa, V., Milla-Castro, F. P., Minniti, J. H., Bidin, C. Moni, Montenegro, K., Morris, C., Motta, V., Navarete, F., Molina, C. Navarro, Nikzat, F., Castellón, J. L. Nilo, Obasi, C., Ortigoza-Urdaneta, M., Palma, T., Parisi, C., Ramírez, K. Pena, Pereyra, L., Perez, N., Petralia, I., Pichel, A., Pignata, G., Alegría, S. Ramírez, Rojas, A. F., Rojas, D., Roman-Lopes, A., Rovero, A. C., Saroon, S., Schmidt, E. O., Schröder, A. C., Schultheis, M., Sgró, M. A., Solano, E., Soto, M., Stecklum, B., Steeghs, D., Tamura, M., Tissera, P., Valcarce, A. A. R., Valotto, C. A., Vasquez, S., Villalon, C., Villanova, S., Cádiz, F. Vivanco, Bacigalupo, R. Zelada, Zijlstra, A., and Zoccali, M.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: The ESO public survey VISTA Variables in the V\'ia L\'actea (VVV) surveyed the inner Galactic bulge and the adjacent southern Galactic disk from $2009-2015$. Upon its conclusion, the complementary VVV eXtended (VVVX) survey has expanded both the temporal as well as spatial coverage of the original VVV area, widening it from $562$ to $1700$ sq. deg., as well as providing additional epochs in $JHK_{\rm s}$ filters from $2016-2023$. With the completion of VVVX observations during the first semester of 2023, we present here the observing strategy, a description of data quality and access, and the legacy of VVVX. VVVX took $\sim 2000$ hours, covering about 4% of the sky in the bulge and southern disk. VVVX covered most of the gaps left between the VVV and the VISTA Hemisphere Survey (VHS) areas and extended the VVV time baseline in the obscured regions affected by high extinction and hence hidden from optical observations. VVVX provides a deep $JHK_{\rm s}$ catalogue of $\gtrsim 1.5\times10^9$ point sources, as well as a $K_{\rm s}$ band catalogue of $\sim 10^7$ variable sources. Within the existing VVV area, we produced a $5D$ map of the surveyed region by combining positions, distances, and proper motions of well-understood distance indicators such as red clump stars, RR Lyrae, and Cepheid variables. In March 2023 we successfully finished the VVVX survey observations that started in 2016, an accomplishment for ESO Paranal Observatory upon 4200 hours of observations for VVV+VVVX. The VVV+VVVX catalogues complement those from the Gaia mission at low Galactic latitudes and provide spectroscopic targets for the forthcoming ESO high-multiplex spectrographs MOONS and 4MOST., Comment: 17 pages, 11 figures (+ appendix). Accepted for publication in Astronomy and Astrophysics in section 14: Catalogs and data
Published: 2024

3. The VVV near-IR galaxy catalogue in a Northern part of the Galactic disc

Author: Daza-Perilla, I. V., Sgró, M. A., Baravalle, L. D., Alonso, M. V., Villalon, C., Lares, M., Soto, M., Castellón, J. L. Nilo, Valotto, C., Cortés, P. Marchant, Minniti, D., and Hempel, M.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The automated identification of extragalactic objects in large surveys provides reliable and reproducible samples of galaxies in less time than procedures involving human interaction. However, regions near the Galactic disc are more challenging due to the dust extinction. We present the methodology for the automatic classification of galaxies and non-galaxies at low Galactic latitude regions using both images and, photometric and morphological near-IR data from the VVVX survey. Using the VVV-NIRGC, we analyse by statistical methods the most relevant features for galaxy identification. This catalogue was used to train a CNN with image data and an XGBoost model with both photometric and morphological data and then to generate a dataset of extragalactic candidates. This allows us to derive probability catalogues used to analyse the completeness and purity as a function of the configuration parameters and to explore the best combinations of the models. As a test case, we apply this methodology to the Northern disc region of the VVVX survey, obtaining 172,396 extragalatic candidates with probabilities of being galaxies. We analyse the performance of our methodology in the VVV disc, reaching an F1-score of 0.67, a 65 per cent purity and a 69 per cent completeness. We present the VVV-NIR Galaxy Catalogue: Northern part of the Galactic disc comprising 1,003 new galaxies, with probabilities greater than 0.6 for either model, with visual inspection and with only 2 previously identified galaxies. In the future, we intend to apply this methodology to other areas of the VVVX survey., Comment: 12 pages, 14 figures, accepted in MNRAS
Published: 2023
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4. The globular cluster system of the nearest Seyfert II galaxy Circinus

Author: Obasi, C., Gómez, M., Minniti, D., Alonso-García, J., Hempel, M., Pullen, J. B., Gregg, M. D., Baravalle, L. D., Alonso, M. V., and Okere, B. I.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Context. The globular cluster (GC) system of Circinus galaxy has not been probed previously partly because of the location of the galaxy at - 3.8$^\circ$ Galactic latitude which suffers severely from interstellar extinction, stellar crowding, and Galactic foreground contamination. However, the deep near-infrared (NIR) photometry by the VISTA Variables in the Via L\'actea Extended Survey (VVVX) in combination with the precise astrometry of Gaia EDR3 allow us to map GCs in this region. Aims. Our long-term goal is to study and characterise the distributions of GCs and Ultra-compact dwarfs of Circinus galaxy which is the nearest Seyfert II galaxy. Here we conduct the first pilot search for GCs in this galaxy. Methods. We use NIR VVVX photometry in combination with Gaia EDR3 astrometric features such as astrometric excess noise and BP/RP excess factor to build the first homogeneous catalogue of GCs in Circinus galaxy. A robust combination of selection criteria allows us to effectively clean interlopers from our sample. Results. We report the detection of$\sim$ 70 GC candidates in this galaxy at a 3 $\sigma$ confidence level. They show a bimodal colour distribution with the blue peak at (G-Ks)$_0$ = 0.985$\pm$0.127 mag with a dispersion of 0.211$\pm$0.091 mag and the red peak at (G-Ks)$_0$ = 1.625$\pm$0.177 mag with a dispersion of 0.482$\pm$0.114 mag. A GC specific frequency (S$_N$) of 1.3$\pm$0.2 was derived for the galaxy, and we estimated a total population of 120$\pm$40 GCs. Based on the projected radial distribution it appears that Circinus has a different distribution of GC candidates than MW and M31. Conclusions. We demonstrate that Circinus galaxy hosts a sizeable number of cluster candidates. This result is the first leap towards understanding the evolution of old stellar clusters in this galaxy., Comment: 15 pages, 12 figures
Published: 2022
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5. RVSPY -- Radial Velocity Survey for Planets around Young Stars. Target characterization and high-cadence survey

Author: Zakhozhay, O., Launhardt, R., Mueller, A., Brems, S., Eigenthaler, P., Gennaro, M., Hempel, A., Hempel, M., Henning, Th., Kennedy, G., Kim, S., Kuerster, M., Lachaume, R., Manerikar, Y., Patel, J., Pavlov, A., Reffert, S., and Trifonov, T.
Subjects: Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract: We introduce our Radial Velocity Survey for Planets around Young stars (RVSPY), characterise our target stars, and search for substellar companions at orbital separations smaller than a few au from the host star. We use the FEROS spectrograph to obtain high signal-to-noise spectra and time series of precise radial velocities (RVs) of 111 stars most of which are surrounded by debris discs. Our target stars have spectral types between early F and late K, a median age of 400 Myr, and a median distance of 45 pc. We determine for all target stars their basic stellar parameters and present the results of the high-cadence RV survey and activity characterization. We achieve a median single-measurement RV precision of 6 m/s and derive the short-term intrinsic RV scatter of our targets (median 22 m/s), which is mostly caused by stellar activity and decays with age from >100 m/s at <20 Myr to <20 m/s at >500 Myr. We discover six previously unknown close companions with orbital periods between 10 and 100 days, three of which are low-mass stars, and three are in the brown dwarf mass regime. We detect no hot companion with an orbital period <10 days down to a median mass limit of ~1 M_Jup for stars younger than 500 Myr, which is still compatible with the established occurrence rate of such companions around main-sequence stars. We find significant RV periodicities between 1.3 and 4.5 days for 14 stars, which are, however, all caused by rotational modulation due to starspots. We also analyse the TESS photometric time series data and find significant periodicities for most of the stars. For 11 stars, the photometric periods are also clearly detected in the RV data. We also derive stellar rotation periods ranging from 1 to 10 days for 91 stars, mostly from TESS data. From the intrinsic activity-related short-term RV jitter, we derive the expected mass-detection thresholds for longer-period companions., Comment: 24 pages, 14 figures, 4 tables; Accepted for publication in A&A
Published: 2022
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6. A new low-luminosity globular cluster discovered in the Milky Way with the VVVX survey

Author: Garro, E. R., Minniti, D., Gómez, M., Fernández-Trincado, J. G., Alonso-García, J., Hempel, M., and Bacigalupo, R. Zelada
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The VISTA Variables in the Via L\'actea Extended Survey (VVVX) allows probing previously unexplored regions of the inner Milky Way (MW). We are looking for new candidate globular clusters (GCs), with the aim of completing the census of the MW GC system. We searched and characterised new GCs, using a combination of the near-IR VVVX survey and 2MASS datasets, and the optical Gaia EDR3 photometry and its precise proper motions (PMs). We report the discovery of a new Galactic GC, named Garro 02, situated at RA=18:05:51.1, Dec=-17:42:02 and l=12.042 deg, b=+1.656 deg. Performing a PM-decontamination procedure, we built a final catalogue with all cluster members, on which we performed a photometric analysis. We calculated a reddening of $E(J-K_s)=1.07\pm 0.06$ mag and extinction of $A_{Ks}=0.79\pm 0.04$ mag in the near-IR; while $E(BP-RP)=2.40\pm 0.01$ mag and $A_{G}=4.80\pm 0.02$ mag in optical passbands. Its heliocentric distance is $D=5.6\pm 0.8$ kpc, which places Garro 02 at a Galactocentric distance of $R_G=2.9$ kpc and Z=0.006 kpc above the Galactic plane. We estimated the metallicity and age by comparison with known GCs and by fitting PARSEC isochrones, finding [Fe/H]$=-1.30\pm 0.2$ dex and age=$12\pm 2$ Gyr. We derived the mean cluster PM of $(\mu_{\alpha}^{\ast}, \mu_{\delta}) = (-6.07\pm 0.62, -6.15\pm 0.75)$ mas yr$^{-1}$. We calculated the cluster luminosity in the near-IR of $M_{Ks}=-7.52\pm 1.23$ mag, which is equivalent to $M_{V}=-5.44$ mag. The core and tidal radii from the radial density profile are $r_c =1.25\pm 0.27$ arcmin (2.07 pc) and $r_t = 7.13\pm 3.83$ arcmin (11.82 pc), respectively. We confirm Garro 02 as a new genuine Galactic GC, located in the MW bulge. It is a low-luminosity, metal-poor, and old GC, and it is a lucky survivor of the strong dynamical processes that occurred during the MW's entire life., Comment: 10 pages, 10 figures, Accepted for publication in A&A
Published: 2022
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7. Unveiling the nature of 12 new low-luminosity Galactic Globular Cluster Candidates

Author: Garro, E. R., Minniti, D., Alessi, B., Patchick, D., Kronberger, M., Alonso-García, J., Fernández-Trincado, J. G., Gómez, M., Hempel, M., Pullen, J. B., Saito, R. K., Ripepi, V., and Bacigalupo, R. Zelada
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The Galactic globular cluster system is incomplete, especially in the low latitude regions of the Galactic bulge and disk. We report the physical characterization of twelve star clusters in the Milky Way, most of which are explored here for the first time. Our aim is determining their main physical parameters, such as reddening and extinction, metallicity, age, total luminosity, mean cluster proper motions (PMs), distances, in order to unveil their physical nature. We study the clusters using optical and near-infrared (NIR) datasets. We use the Gaia Early Data Release 3 (EDR3) PMs in order to perform a PM-decontamination procedure and build final catalogues. We match the Gaia EDR3 with the VISTA Variables in the V\'ia L\'actea extended (VVVX) survey and Two Micron All Sky survey (2MASS) in the NIR, in order to construct complete colour-magnitude diagrams (CMDs) and investigate the clusters properties. The extinctions are evaluated using existing reddening maps, spanning $0.09\lesssim A_{Ks}\lesssim 0.86$ mag and $0.89 \lesssim A_{G}\lesssim 4.72$ mag in the NIR and optical, respectively. We obtain their heliocentric distances, that range from about 4 to 20 kpc, placing these clusters at $3\lesssim R_{G}\lesssim 14$ kpc from the Galactic centre. The best PARSEC isochrone fit yields a metallicity range of $-1.8<$[Fe/H]$<+0.3$ and an approximative age range of $2<$Age$<14$ Gyr. We find that all clusters have low-luminosities, with $-6.9
Published: 2021
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8. Expected impact from weak reactions with light nuclei in corecollapse supernova simulations

Author: Fischer T., Martínez-Pinedo G., Hempel M., Huther L., Röpke G., Typel S., and Lohs A.
Subjects: Physics, QC1-999
Abstract: We study the role of light nuclear clusters in simulations of core-collapse supernovae. Expressions for the reaction rates are developed for a large selection of charged current absorption and scattering processes with light clusters. Medium modifications are taken into account at the mean-field level. We explore the possible impact on the supernova dynamics and the neutrino signal during the mass accretion phase prior to the possible explosion onset as well as during the subsequent protoneutron star deleptnoization after the explosion onset has been launched.
Published: 2016
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9. From femtonova to supernova: Heavy-ion collisions and the supernova equation of state

Author: Hagel K., Hempel M., Natowitz J. B., Röpke G., Typel S., Wuenschel S., Wada R., Barbui M., and Schmidt K.
Subjects: Physics, QC1-999
Abstract: Calculations using astrophysical equations of state at low densities comparable to that of the neutrino emission surface in supernovae and accretion disks are confronted with experimental results from heavy ion collisions. An extension of previous work shows that it is important to include all of the measured experimental data to draw conclusions about the astrophysical equation of state. Armed with this information, the calculations of the astrophysical equation of state are significantly constrained. Predictions of temperatures and densities sampled in black hole accretion disks are compared to those sampled in the experimental data.
Published: 2016
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10. Discovery of new globular clusters in the Sagittarius dwarf galaxy

Author: Minniti, D., Ripepi, V., Fernández-Trincado, J. G., Alonso-García, J., Smith, L. C., Lucas, P. W., Gómez, M., Pullen, J. B., Garro, E. R., Cádiz, F. Vivanco, Hempel, M., Rejkuba, M., Saito, R. K., Palma, T., Clariá, J. J., Gregg, M., and Majaess, D.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Context. Globular clusters (GCs) are witnesses of the past accretion events onto the Milky Way (MW). In particular, the GCs of the Sagittarius (Sgr) dwarf galaxy are important probes of an on-going merger. Aims. Our main goal is to search for new GC members of this dwarf galaxy using the VISTA Variables in the Via Lactea Extended Survey (VVVX) near-infrared database combined with the Gaia Early Data Release 3 (EDR3) optical database. Methods. We investigated all VVVX-enabled discoveries of GC candidates in a region covering about 180 sq. deg. toward the bulge and the Sgr dwarf galaxy. We used multiband point-spread function photometry to obtain deep color-magnitude diagrams (CMDs) and luminosity functions (LFs) for all GC candidates, complemented by accurate Gaia-EDR3 proper motions (PMs) to select Sgr members and variability information to select RR Lyrae which are potential GC members. Results. After applying a strict PM cut to discard foreground bulge and disk stars, the CMDs and LFs for some of the GC candidates exhibit well defined red giant branches and red clump giant star peaks. We selected the best Sgr GCs, estimating their distances, reddenings, and associated RR Lyrae. Conclusions. We discover 12 new Sgr GC members, more than doubling the number of GCs known in this dwarf galaxy. In addition, there are 11 other GC candidates identified that are uncertain, awaiting better data for confirmation., Comment: 12 pages, 6 Figures
Published: 2021
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11. VVVX-Gaia Discovery of a Low Luminosity Globular Cluster in the Milky Way Disk

Author: Garro, E. R., Minniti, D., Gómez, M., Alonso-García, J., Barbá, R. H., Barbuy, B., Clariá, J. J., Chené, A. N., Dias, B., Hempel, M., Ivanov, V. D., Lucas, P. W., Majaess, D., Mauro, F., Bidin, C. Moni, Palma, T., Pullen, J. B., Saito, R. K., Smith, L., Surot, F., Alegría, S. Ramírez, Rejkuba, M., and Ripepi, V.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: Milky Way globular clusters (MW GCs) are difficult to identify at low Galactic latitudes because of high differential extinction and heavy star crowding. The new deep near-IR images and photometry from the VISTA Variables in the Via L\'actea Extended Survey (VVVX) allow us to chart previously unexplored regions. Our long term aim is to complete the census of MW GCs. The immediate goals are to estimate the astrophysical parameters, measuring their reddenings, extinctions, distances, total luminosities, proper motions, sizes, metallicities and ages. We use the near-IR VVVX survey database, in combination with Gaia DR2 optical photometry, and with the Two Micron All Sky Survey (2MASS) photometry. We report the detection of a heretofore unknown Galactic Globular Cluster at $RA =$ 14:09:00.0; $DEC=-$65:37:12 (J2000). We calculate a reddening of $E(J-K_s)=(0.3\pm 0.03)$ mag and an extinction of $A_{K_s}=(0.15\pm 0.01)$ mag for this new GC. Its distance modulus and corresponding distance were measured as $(m-M)=(15.93\pm0.03)$ mag and $D=(15.5\pm1.0)$ kpc, respectively. We estimate the metallicity and age by comparison with known GCs and by fitting PARSEC and Dartmouth isochrones, finding $[Fe/H]=(-0.70\pm0.2)$ dex and $t=(11.0\pm1.0)$ Gyr. The mean GC PMs from Gaia are $\mu_{\alpha^\ast}=(-4.68 \pm 0.47 )$ mas $yr^{-1}$ and $\mu_{\delta}=(-1.34 \pm 0.45)$ mas $yr^{-1}$. The total luminosity of our cluster is estimated to be $M_{Ks}=(-7.76\pm 0.5)$ mag. We have found a new low-luminosity, old and metal-rich globular cluster, situated in the far side of the Galactic disk, at $R_{G}=11.2$ kpc from the Galactic centre, and at $z=1.0$ kpc below the plane. Interestingly, the location, metallicity and age of this globular cluster are coincident with the Monoceros Ring (MRi) structure.
Published: 2020
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12. The VVV Infrared Variability Catalog (VIVA-I)

Author: Lopes, C. E. Ferreira, Cross, N. J. G., Catelan, M., Minniti, D., Hempel, M., Lucas, P. W., Angeloni, R., Jablonsky, F., Braga, V. F., Leao, I. C., Herpich, F. R., Alonso-Garcia, J., Papageorgiou, A., Pichara, K., Saito, R. K., Bradley, A., Beamin, J. C., Cortes, C., De Medeiros, J. R., and Russell, Christopher. M. P.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: Thanks to the VISTA Variables in the Via Lactea (VVV) ESO Public Survey it is now possible to explore a large number of objects in those regions. This paper addresses the variability analysis of all VVV point sources having more than 10 observations in VVVDR4 using a novel approach. In total, the near-IR light curves of 288,378,769 sources were analysed using methods developed in the New Insight Into Time Series Analysis project. As a result, we present a complete sample having 44, 998, 752 variable star candidates (VVV-CVSC), which include accurate individual coordinates, near-IR magnitudes (ZYJHKs), extinctions A(Ks), variability indices, periods, amplitudes, among other parameters to assess the science. Unfortunately, a side effect of having a highly complete sample, is also having a high level of contamination by non-variable (contamination ratio of non-variables to variables is slightly over 10:1). To deal with this, we also provide some flags and parameters that can be used by the community to de-crease the number of variable candidates without heavily decreasing the completeness of the sample. In particular, we cross-identified 339,601 of our sources with Simbad and AAVSO databases, which provide us with information for these objects at other wavelegths. This sub-sample constitutes a unique resource to study the corresponding near-IR variability of known sources as well as to assess the IR variability related with X-ray and Gamma-Ray sources. On the other hand, the other 99.5% sources in our sample constitutes a number of potentially new objects with variability information for the heavily crowded and reddened regions of the Galactic Plane and Bulge. The present results also provide an important queryable resource to perform variability analysis and to characterize ongoing and future surveys like TESS and LSST., Comment: 27 pages, 14 figures
Published: 2020
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13. VVV-WIT-01: highly obscured classical nova or protostellar collision?

Author: Lucas, P. W., Minniti, D., Kamble, A., Kaplan, D. L., Cross, N., Dekany, I., Ivanov, V. D., Kurtev, R., Saito, R. K., Smith, L. C., Catelan, M., Masetti, N., Toledo, I., Hempel, M., Thompson, M. A., Peña, C. Contreras, Forbrich, J., Krause, M., Dale, J., Borissova, J., and Emerson, J.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: A search of the first Data Release of the VISTA Variables in the Via Lactea (VVV) Survey discovered the exceptionally red transient VVV-WIT-01 ($H-K_s=5.2$). It peaked before March 2010, then faded by $\sim$9.5 mag over the following two years. The 1.6--22 $\mu$m spectral energy distribution in March 2010 was well fit by a highly obscured black body with $T \sim 1000$ K and $A_{K_s} \sim 6.6$ mag. The source is projected against the Infrared Dark Cloud (IRDC) SDC G331.062$-$0.294. The chance projection probability is small for any single event ($p \approx 0.01$ to 0.02) which suggests a physical association, e.g. a collision between low mass protostars. However, black body emission at $T \sim 1000$ K is common in classical novae (especially CO novae) at the infrared peak in the light curve, due to condensation of dust $\sim$30--60 days after the explosion. Radio follow up with the Australia Telescope Compact Array (ATCA) detected a fading continuum source with properties consistent with a classical nova but probably inconsistent with colliding protostars. Considering all VVV transients that could have been projected against a catalogued IRDC raises the probability of a chance association to $p=0.13$ to 0.24. After weighing several options, it appears likely that VVV-WIT-01 was a classical nova event located behind an IRDC., Comment: 13 pages, 7 figures. Accepted by MNRAS
Published: 2020
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14. The Pixel Luminosity Telescope: a detector for luminosity measurement at CMS using silicon pixel sensors

Author: Ayala, E., CarreraJarrin, E., Ahmed, I., Campbell, A., Danilov, V., EstevezBanos, L. I., Giraldi, A., Guthoff, M., Hempel, M., Henschel, H., Knolle, J., Lange, W., Leonard, J., Lohmann, W., Meyer, A. B., Myronenko, V., Penno, M., Ribeiro Lopes, B., Rübenach, J., Saggio, A., Scheurer, V., Sosa Ricardo, R. E., Turkot, O., Walter, D., Kassel, F., Mallows, S., Bartók, M., Chudasama, R., Farkas, K., Fejes, M., Gadallah, M. M. A., Major, P., Mehta, A., Pásztor, G., Rádl, A. J., Veres, G. I., Bakhshiansohi, H., Gholami, A., Khazaie, E., Sedghi, M., Zeinali, M., Fabbri, F., Tosi, N., Bacchetta, N., Trapani, P. P., Daugalas, J., Benitez, J. F., Castaneda Hernandez, A., Encinas Acosta, H. A., Gallegos Maríñez, L. G., León Coello, M., Murillo Quijada, J. A., Sehrawat, A., Valencia Palomo, L., Oropeza Barrera, C., Bheesette, S., Butler, A. P. H., Butler, P. H., Lokhovitskiy, A., Lujan, P., Auzinger, G., Ball, A. H., Çekmecelioğlu, Y. C., Dabrowski, A., Damanakis, K., Donadon Servelle, A., Eble, F., Haranko, M., Hegeman, J., Kessaci, K., Kornmayer, A., Loos, R., Miraglia, M., Nicolini, J., Orfanelli, S., Orsini, L., Petrucci, A., Ryjov, V., Saariokari, S., Schwick, C., Schneider, B., Tsoukias, S., Tsrunchev, P., Wanczyk, J., Zagoździńska-Bochenek, A. A., Zeuner, W. D., Rohe, T., Krintiras, G., Palmer, C., Jain, Sh., Mans, J., Rusack, R., Bueghly, J., Chen, Z., Gunter, T., Odell, N., Pozdnyakov, A., Velasco, M., Harrop, B., Higginbotham, S., Kalogeropoulos, A., Luo, J., Marlow, D., Stickland, D., Xie, Z., Bartz, E., Hidas, D., Karacheban, O., Schnetzer, S., Stone, R., Acharya, H., Delannoy, A. G., Heideman, J., Karunarathna, N., Riley, G., Rose, K., Spanier, S., Thapa, K., Gurrola, A., Johns, W., Romeo, F., Soubasis, B., Farrow, M. C., Azhgirey, I., Ershov, A., Gribushin, A., Kaminskiy, A., Kurochkin, I., Okhotnikov, V., Popova, E., Riabchikova, A., Selivanova, D., and Shevelev, A.
Published: 2023
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15. A Color-Excess Extinction map of the Southern Galactic disk from the VVV and GLIMPSE Surveys

Author: Soto, M., Barbá, R., Minniti, D., Kunder, A., Majaess, D., Nilo-Castellón, J. L., Alonso-García, J., Leone, G., Morelli, L., Haikala, L., Firpo, V., Lucas, P., Emerson, J. P., Bidin, C. Moni, Geisler, D., Saito, R. K., Gurovich, S., Ramos, R. Contreras, Rejkuba, M., Barbieri, M., Roman-Lopes, A., Hempel, M., Alonso, M. V., Baravalle, L. D., Borissova, J., Kurtev, R., and Milla, F.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: An improved high-resolution and deep A$_{Ks}$ foreground dust extinction map is presented for the Galactic disk area within $295^{\circ} \lesssim l \lesssim 350^{\circ}$, $-1.0^{\circ} \lesssim b \lesssim +1.0^{\circ}$. At some longitudes the map reaches up to $|b|\sim2.25^{\circ}$, for a total of $\sim$148 deg$^2$. The map was constructed via the Rayleigh-Jeans Color Excess (RJCE) technique based on deep near-infrared (NIR) and mid-infrared (MIR) photometry. The new extinction map features a maximum bin size of 1', and relies on NIR observations from the Two Micron All-Sky Survey (2MASS) and new data from ESO's Vista Variables in the V\'ia L\'actea (VVV) survey, in concert with MIR observations from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE). The VVV photometry penetrates $\sim$4 magnitudes fainter than 2MASS, and provides enhanced sampling of the underlying stellar populations in this heavily obscured region. Consequently, the new results supersede existing RJCE maps tied solely to brighter photometry, revealing a systematic underestimation of extinction in prior work that was based on shallower data. The new high-resolution and large-scale extinction map presented here is readily available to the community through a web query interface., Comment: 11 pages, 9 figures, published in MNRAS
Published: 2019
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16. A Sequoia in the Garden: FSR 1758 - Dwarf Galaxy or Giant Globular Cluster?

Author: Barba, R. H., Minniti, D., Geisler, D., Alonso-Garcia, J., Hempel, M., Monachesi, A., Arias, J. I., and Gomez, F. A.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: We present the physical characterization of FSR 1758, a new large, massive object very recently discovered in the Galactic Bulge. The combination of optical data from the 2nd Gaia Data Release (GDR2) and the DECam Plane Survey (DECaPS), and near-IR data from the VISTA Variables in the V\'{\i}a L\'actea Extended Survey (VVVX) led to a clean sample of likely members. Based on this integrated dataset, position, distance, reddening, size, metallicity, absolute magnitude, and proper motion of this object are measured. We estimate the following parameters: $\alpha=17:31:12$, $\delta=-39:48:30$ (J2000), $D=11.5 \pm 1.0$ kpc, $E(J-Ks)=0.20 \pm 0.03$ mag, $R_c=10$ pc, $R_t=150$ pc, $[Fe/H]=-1.5 \pm 0.3$ dex, $M_i < -8.6 \pm 1.0$, $\mu_{\alpha} = -2.85$ mas yr$^{-1}$, and $\mu_{\delta} = 2.55$ mas yr$^{-1}$. The nature of this object is discussed. If FRS 1758 is a genuine globular cluster, it is one of the largest in the Milky Way, with a size comparable or even larger than that of $\omega$ Cen, being also an extreme outlier in the size vs. Galactocentric distance diagram. The presence of a concentration of long-period RR Lyrae variable stars and blue horizontal branch stars suggests that it is a typical metal-poor globular cluster of Oosterhoff type II. Further exploration of a larger surrounding field reveals common proper motion stars, suggesting either tidal debris or that FRS\,1758 is actually the central part of a larger extended structure such as a new dwarf galaxy, tentatively named as Scorpius. In either case, this object is remarkable, and its discovery graphically illustrates the possibility to find other large objects hidden in the Galactic Bulge using future surveys., Comment: Accepted Astrophysical Journal Letters
Published: 2018
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17. Orbital and physical parameters of eclipsing binaries from the All-Sky Automated Survey catalogue - X. Three high-contrast systems with secondaries detected with IR spectroscopy

Author: Hełminiak, K. G., Tokovinin, A., Niemczura, E., Pawłaszek, R., Yanagisawa, K., Brahm, R., Espinoza, N., Ukita, N., Ratajczak, E. Kambe. M., Hempel, M., Jordán, A., Konacki, M., Sybilski, P., Kozłowski, S. K., Litwickim, M., and Tamura, M.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: We present results of the combined photometric and spectroscopic analysis of three detached eclipsing binaries, which secondary components are not visible or very hard to identify in the optical spectra - ASAS J052743-0359.7, ASAS J065134-2211.5, and ASAS J073507-0905.7. The first one is a known visual binary ADS 4022, and we found that it is a quadruple system, composed of two spectroscopic binaries, one of which shows eclipses. None of the systems was previously recognized as a spectroscopic binary. We collected a number of high-resolution optical and IR spectra to calculate the radial velocities (RVs) and later combined them with MITSuME and ASAS photometry. The IR spectra were crucial for secure identification of the cooler components' lines. RV measurements were done with the TODCOR technique, and RV curves modelled with our own procedure V2FIT. Light curve modelling was performed with JKTEBOP and PHOEBE codes. Temperatures and metallicities of two systems were estimated from spectra. For the ADS 4022 system we also used the archival WDS data and new SOAR observations in order to derive the orbit of the visual pair for the first time. Ages were estimated by comparing our results with PARSEC isochrones. The eclipsing pair A052743 A ($P=5.27$ d) is composed of a 1.03(6) M$_\odot$, 1.03(2) R$_\odot$ primary and a 0.60(2) M$_\odot$, 0.59(2) R$_\odot$ secondary. The components of the $P=21.57$ d non-eclipsing pair B likely have masses in between the two eclipsing components, and both pairs are on a $\sim$188 yr orbit around their common centre of mass. The system A065134 ($P=8.22$ d) consists of a 0.956(12) M$_\odot$, 0.997(4) R$_\odot$ primary and a 0.674(5) M$_\odot$, 0.690(7) R$_\odot$ secondary. Finally, A073507 ($P=1.45$ d), which consists of a 1.452(34) M$_\odot$, 1.635(12) R$_\odot$ primary and a 0.808(13) M$_\odot$, 0.819(11) R$_\odot$ secondary, is likely a PMS system., Comment: 22 pages, 13 figures, 8 tables, accepted for publication in A&A, abstract modified for arXiv
Published: 2018
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18. New Galactic Star Clusters Discovered in the Disk Area of the VVVX Survey

Author: Borissova, J., Ivanov, V. D., Lucas, P. W., Kurtev, R., Alonso-Garcia, J., Alegria, S. Ramirez, Minniti, D., Hempel, M., Medina, N., Chene, A. N., and Kuhn, M. A.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: The "VISTA Variables in the Via Lactea eXtended (VVVX)" ESO Public Survey is a near-infrared photometric sky survey that covers nearly 1700 sq. deg towards the Galactic disk and bulge. It is well-suited to search for new open clusters, hidden behind dust and gas. The pipeline processed and calibrated Ks-band tile images of 40% of the disk area covered by VVVX was visually inspected for stellar over-densities. Then, we identified cluster candidates by examination of the composite JHKs color images. The color-magnitude diagrams of the cluster candidates are constructed. Whenever possible the Gaia DR2 parameters are used to calculate the mean proper motions, radial velocities, reddening and distances. We report the discovery of 120 new infrared clusters and stellar groups. Approximately, half of them (47%) are faint, compact, highly reddened, and they seem to be associated with other indicators of recent star formation, such as nearby Young Stellar Objects, Masers, H II regions or bubbles. The preliminary distance determinations allow us to trace the clusters up to 4.5 kpc, but most of the cluster candidates are centered at 2.2 kpc. The mean proper motions of the clusters, show that in general, they follow the disk motion of the Galaxy., Comment: 19 pages, 10 figures, published in the MNRAS
Published: 2018
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19. Erratum: Measurement of prompt and nonprompt charmonium suppression in PbPb collisions at 5.02 TeV

Author: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Erö, J., Valle, A. Escalante Del, Flechl, M., Friedl, M., Frühwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., König, A., Krammer, N., Krätschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rad, N., Rohringer, H., Schieck, J., Schöfbeck, R., Spanring, M., Spitzbart, D., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Croce, D. Di, Janssen, X., Lauwers, J., De Klundert, M. Van, Haevermaet, H. Van, Mechelen, P. Van, Remortel, N. Van, Zeid, S. Abu, Blekman, F., D’Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Marchesini, I., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Doninck, W. Van, Mulders, P. Van, Parijs, I. Van, Beghin, D., Bilin, B., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Dorney, B., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Kalsi, A. K., Lenzi, T., Luetic, J., Maerschalk, T., Marinov, A., Seva, T., Starling, E., Velde, C. Vander, Vanlaer, P., Vannerom, D., Yonamine, R., Zenoni, F., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Salva, S., Tytgat, M., Verbeke, W., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caputo, C., Caudron, A., David, P., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Komm, M., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Saggio, A., Marono, M. Vidal, Wertz, S., Zobec, J., Júnior, W. L. Aldá, Alves, F. L., Alves, G. A., Brito, L., Junior, M. Correa Martins, Hensel, C., Moraes, A., Pol, M. E., Teles, P. Rebello, Chagas, E. Belchior Batista Das, Carvalho, W., Chinellato, J., Coelho, E., Da Costa, E. M., Da Silveira, G. G., De Jesus Damiao, D., De Souza, S. Fonseca, Guativa, L. M. Huertas, Malbouisson, H., De Almeida, M. Melo, Herrera, C. Mora, Mundim, L., Nogima, H., Rosas, L. J. Sanchez, Santoro, A., Sznajder, A., Thiel, M., Manganote, E. J. Tonelli, Da Silva De Araujo, F. Torres, Pereira, A. Vilela, Ahuja, S., Bernardes, C. A., Tomei, T. R. Fernandez Perez, Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Abad, D. Romero, Vargas, J. C. Ruiz, Aleksandrov, A., Hadjiiska, R., Iaydjiev, P., Misheva, M., Rodozov, M., Shopova, M., Sultanov, G., Dimitrov, A., Litov, L., Pavlov, B., Petkov, P., Fang, W., Gao, X., Yuan, L., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhang, S., Zhao, J., Ban, Y., Chen, G., Li, J., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Zhang, F., Wang, Y., Avila, C., Cabrera, A., Montoya, C. A. Carrillo, Sierra, L. F. Chaparro, Florez, C., Hernández, C. F. González, Alvarez, J. D. Ruiz, Delgado, M. A. Segura, Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Cipriano, P. M. Ribeiro, Sculac, T., Antunovic, Z., Kovac, M., Brigljevic, V., Ferencek, D., Kadija, K., Mesic, B., Starodumov, A., Susa, T., Ather, M. W., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Rykaczewski, H., Finger, M., Finger, Jr., M., Jarrin, E. Carrera, Mahmoud, M. A., Mohammed, Y., Salama, E., Dewanjee, R. K., Kadastik, M., Perrini, L., Raidal, M., Tiko, A., Veelken, C., Eerola, P., Kirschenmann, H., Pekkanen, J., Voutilainen, M., Havukainen, J., Heikkilä, J. K., Järvinen, T., Karimäki, V., Kinnunen, R., Lampén, T., Lassila-Perini, K., Laurila, S., Lehti, S., Lindén, T., Luukka, P., Siikonen, H., Tuominen, E., Tuominiemi, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. L., Ferri, F., Ganjour, S., Ghosh, S., Gras, P., de Monchenault, G. Hamel, Jarry, P., Kucher, I., Leloup, C., Locci, E., Machet, M., Malcles, J., Negro, G., Rander, J., Rosowsky, A., Sahin, M.Ö., Titov, M., Abdulsalam, A., Amendola, C., Antropov, I., Baffioni, S., Beaudette, F., Busson, P., Cadamuro, L., Charlot, C., de Cassagnac, R. Granier, Jo, M., Lisniak, S., Lobanov, A., Blanco, J. Martin, Nguyen, M., Ochando, C., Ortona, G., Paganini, P., Pigard, P., Salerno, R., Sauvan, J. B., Sirois, Y., Leiton, A. G. Stahl, Strebler, T., Yilmaz, Y., Zabi, A., Zghiche, A., Agram, J.-L., Andrea, J., Bloch, D., Brom, J.-M., Buttignol, M., Chabert, E. C., Chanon, N., Collard, C., Conte, E., Coubez, X., Fontaine, J.-C., Gelé, D., Goerlach, U., Jansová, M., Bihan, A.-C. Le, Tonon, N., Hove, P. Van, Gadrat, S., Beauceron, S., Bernet, C., Boudoul, G., Chierici, R., Contardo, D., Depasse, P., Mamouni, H. El, Fay, J., Finco, L., Gascon, S., Gouzevitch, M., Grenier, G., Ille, B., Lagarde, F., Laktineh, I. B., Lethuillier, M., Mirabito, L., Pequegnot, A. L., Perries, S., Popov, A., Sordini, V., Donckt, M. Vander, Viret, S., Toriashvili, T., Tsamalaidze, Z., Autermann, C., Feld, L., Kiesel, M. K., Klein, K., Lipinski, M., Preuten, M., Schomakers, C., Schulz, J., Teroerde, M., Zhukov, V., Albert, A., Dietz-Laursonn, E., Duchardt, D., Endres, M., Erdmann, M., Erdweg, S., Esch, T., Fischer, R., Güth, A., Hamer, M., Hebbeker, T., Heidemann, C., Hoepfner, K., Knutzen, S., Merschmeyer, M., Meyer, A., Millet, P., Mukherjee, S., Pook, T., Radziej, M., Reithler, H., Rieger, M., Scheuch, F., Teyssier, D., Thüer, S., Flügge, G., Kargoll, B., Kress, T., Künsken, A., Müller, T., Nehrkorn, A., Nowack, A., Pistone, C., Pooth, O., Stahl, A., Martin, M. Aldaya, Arndt, T., Asawatangtrakuldee, C., Beernaert, K., Behnke, O., Behrens, U., Martínez, A. Bermúdez, Anuar, A. A. Bin, Borras, K., Botta, V., Campbell, A., Connor, P., Contreras-Campana, C., Costanza, F., Pardos, C. Diez, Eckerlin, G., Eckstein, D., Eichhorn, T., Eren, E., Gallo, E., Garcia, J. Garay, Geiser, A., Luyando, J. M. Grados, Grohsjean, A., Gunnellini, P., Guthoff, M., Harb, A., Hauk, J., Hempel, M., Jung, H., Kasemann, M., Keaveney, J., Kleinwort, C., Korol, I., Krücker, D., Lange, W., Lelek, A., Lenz, T., Leonard, J., Lipka, K., Lohmann, W., Mankel, R., Melzer-Pellmann, I.-A., Meyer, A. B., Mittag, G., Mnich, J., Mussgiller, A., Ntomari, E., Pitzl, D., Raspereza, A., Savitskyi, M., Saxena, P., Shevchenko, R., Stefaniuk, N., Onsem, G. P. Van, Walsh, R., Wen, Y., Wichmann, K., Wissing, C., Zenaiev, O., Aggleton, R., Bein, S., Blobel, V., Vignali, M. Centis, Dreyer, T., Garutti, E., Gonzalez, D., Haller, J., Hinzmann, A., Hoffmann, M., Karavdina, A., Klanner, R., Kogler, R., Kovalchuk, N., Kurz, S., Lapsien, T., Marconi, D., Meyer, M., Niedziela, M., Nowatschin, D., Pantaleo, F., Peiffer, T., Perieanu, A., Scharf, C., Schleper, P., Schmidt, A., Schumann, S., Schwandt, J., Sonneveld, J., Stadie, H., Steinbrück, G., Stober, F. M., Stöver, M., Tholen, H., Troendle, D., Usai, E., Vanhoefer, A., Vormwald, B., Akbiyik, M., Barth, C., Baselga, M., Baur, S., Butz, E., Caspart, R., Chwalek, T., Colombo, F., De Boer, W., Dierlamm, A., Faltermann, N., Freund, B., Friese, R., Giffels, M., Harrendorf, M. A., Hartmann, F., Heindl, S. M., Husemann, U., Kassel, F., Kudella, S., Mildner, H., Mozer, M. U., Müller, Th., Plagge, M., Quast, G., Rabbertz, K., Schröder, M., Shvetsov, I., Sieber, G., Simonis, H. J., Ulrich, R., Wayand, S., Weber, M., Weiler, T., Williamson, S., Wöhrmann, C., Wolf, R., Anagnostou, G., Daskalakis, G., Geralis, T., Kyriakis, A., Loukas, D., Topsis-Giotis, I., Karathanasis, G., Kesisoglou, S., Panagiotou, A., Saoulidou, N., Kousouris, K., Evangelou, I., Foudas, C., Gianneios, P., Katsoulis, P., Kokkas, P., Mallios, S., Manthos, N., Papadopoulos, I., Paradas, E., Strologas, J., Triantis, F. A., Tsitsonis, D., Csanad, M., Filipovic, N., Pasztor, G., Surányi, O., Veres, G. I., Bencze, G., Hajdu, C., Horvath, D., Hunyadi, Á., Sikler, F., Veszpremi, V., Beni, N., Czellar, S., Karancsi, J., Makovec, A., Molnar, J., Szillasi, Z., Bartók, M., Raics, P., Trocsanyi, Z. L., Ujvari, B., Choudhury, S., Komaragiri, J. R., Bahinipati, S., Bhowmik, S., Mal, P., Mandal, K., Nayak, A., Sahoo, D. K., Sahoo, N., Swain, S. K., Bansal, S., Beri, S. B., Bhatnagar, V., Chawla, R., Dhingra, N., Kaur, A., Kaur, M., Kaur, S., Kumar, R., Kumari, P., Mehta, A., Singh, J. B., Walia, G., Kumar, Ashok, Shah, Aashaq, Bhardwaj, A., Chauhan, S., Choudhary, B. C., Garg, R. B., Keshri, S., Kumar, A., Malhotra, S., Naimuddin, M., Ranjan, K., Sharma, R., Bhardwaj, R., Bhattacharya, R., Bhattacharya, S., Bhawandeep, U., Dey, S., Dutt, S., Dutta, S., Ghosh, S., Majumdar, N., Modak, A., Mondal, K., Mukhopadhyay, S., Nandan, S., Purohit, A., Roy, A., Chowdhury, S. Roy, Sarkar, S., Sharan, M., Thakur, S., Behera, P. K., Chudasama, R., Dutta, D., Jha, V., Kumar, V., Mohanty, A. K., Netrakanti, P. K., Pant, L. M., Shukla, P., Topkar, A., Aziz, T., Dugad, S., Mahakud, B., Mitra, S., Mohanty, G. B., Sur, N., Sutar, B., Banerjee, S., Bhattacharya, S., Chatterjee, S., Das, P., Guchait, M., Jain, Sa., Kumar, S., Maity, M., Majumder, G., Mazumdar, K., Sarkar, T., Wickramage, N., Chauhan, S., Dube, S., Hegde, V., Kapoor, A., Kothekar, K., Pandey, S., Rane, A., Sharma, S., Chenarani, S., Tadavani, E. Eskandari, Etesami, S. M., Khakzad, M., Najafabadi, M. Mohammadi, Naseri, M., Mehdiabadi, S. Paktinat, Hosseinabadi, F. Rezaei, Safarzadeh, B., Zeinali, M., Felcini, M., Grunewald, M., Abbrescia, M., Calabria, C., Colaleo, A., Creanza, D., Cristella, L., De Filippis, N., De Palma, M., Errico, F., Fiore, L., Iaselli, G., Lezki, S., Maggi, G., Maggi, M., Miniello, G., My, S., Nuzzo, S., Pompili, A., Pugliese, G., Radogna, R., Ranieri, A., Selvaggi, G., Sharma, A., Silvestris, L., Venditti, R., Verwilligen, P., Abbiendi, G., Battilana, C., Bonacorsi, D., Borgonovi, L., Braibant-Giacomelli, S., Campanini, R., Capiluppi, P., Castro, A., Cavallo, F. R., Chhibra, S. S., Codispoti, G., Cuffiani, M., Dallavalle, G. M., Fabbri, F., Fanfani, A., Fasanella, D., Giacomelli, P., Grandi, C., Guiducci, L., Marcellini, S., Masetti, G., Montanari, A., Navarria, F. L., Perrotta, A., Rossi, A. M., Rovelli, T., Siroli, G. P., Tosi, N., Albergo, S., Costa, S., Mattia, A. Di, Giordano, F., Potenza, R., Tricomi, A., Tuve, C., Barbagli, G., Chatterjee, K., Ciulli, V., Civinini, C., D’Alessandro, R., Focardi, E., Lenzi, P., Meschini, M., Paoletti, S., Russo, L., Sguazzoni, G., Strom, D., Viliani, L., Benussi, L., Bianco, S., Fabbri, F., Piccolo, D., Primavera, F., Calvelli, V., Ferro, F., Ravera, F., Robutti, E., Tosi, S., Benaglia, A., Beschi, A., Brianza, L., Brivio, F., Ciriolo, V., Dinardo, M. E., Fiorendi, S., Gennai, S., Ghezzi, A., Govoni, P., Malberti, M., Malvezzi, S., Manzoni, R. A., Menasce, D., Moroni, L., Paganoni, M., Pauwels, K., Pedrini, D., Pigazzini, S., Ragazzi, S., de Fatis, T. Tabarelli, Buontempo, S., Cavallo, N., Guida, S. Di, Fabozzi, F., Fienga, F., Iorio, A. O. M., Khan, W. A., Lista, L., Meola, S., Paolucci, P., Sciacca, C., Thyssen, F., Azzi, P., Bacchetta, N., Benato, L., Bisello, D., Boletti, A., Carlin, R., De Oliveira, A. Carvalho Antunes, Checchia, P., Dall’Osso, M., De Castro Manzano, P., Dorigo, T., Gasparini, F., Gasparini, U., Gozzelino, A., Lacaprara, S., Lujan, P., Margoni, M., Meneguzzo, A. T., Pozzobon, N., Ronchese, P., Rossin, R., Simonetto, F., Torassa, E., Ventura, S., Zanetti, M., Zotto, P., Braghieri, A., Magnani, A., Montagna, P., Ratti, S. P., Re, V., Ressegotti, M., Riccardi, C., Salvini, P., Vai, I., Vitulo, P., Solestizi, L. Alunni, Biasini, M., Bilei, G. M., Cecchi, C., Ciangottini, D., Fanò, L., Leonardi, R., Manoni, E., Mantovani, G., Mariani, V., Menichelli, M., Rossi, A., Santocchia, A., Spiga, D., Androsov, K., Azzurri, P., Bagliesi, G., Boccali, T., Borrello, L., Castaldi, R., Ciocci, M. A., Dell’Orso, R., Fedi, G., Giannini, L., Giassi, A., Grippo, M. T., Ligabue, F., Lomtadze, T., Manca, E., Mandorli, G., Messineo, A., Palla, F., Rizzi, A., Savoy-Navarro, A., Spagnolo, P., Tenchini, R., Tonelli, G., Venturi, A., Verdini, P. G., Barone, L., Cavallari, F., Cipriani, M., Daci, N., Re, D. Del, Marco, E. Di, Diemoz, M., Gelli, S., Longo, E., Margaroli, F., Marzocchi, B., Meridiani, P., Organtini, G., Paramatti, R., Preiato, F., Rahatlou, S., Rovelli, C., Santanastasio, F., Amapane, N., Arcidiacono, R., Argiro, S., Arneodo, M., Bartosik, N., Bellan, R., Biino, C., Cartiglia, N., Cenna, F., Costa, M., Covarelli, R., Degano, A., Demaria, N., Kiani, B., Mariotti, C., Maselli, S., Migliore, E., Monaco, V., Monteil, E., Monteno, M., Obertino, M. M., Pacher, L., Pastrone, N., Pelliccioni, M., Angioni, G. L. Pinna, Romero, A., Ruspa, M., Sacchi, R., Shchelina, K., Sola, V., Solano, A., Staiano, A., Traczyk, P., Belforte, S., Casarsa, M., Cossutti, F., Ricca, G. Della, Zanetti, A., Kim, D. H., Kim, G. N., Kim, M. S., Lee, J., Lee, S., Lee, S. W., Moon, C. S., Oh, Y. D., Sekmen, S., Son, D. C., Yang, Y. C., Lee, A., Kim, H., Moon, D. H., Oh, G., Cifuentes, J. A. Brochero, Goh, J., Kim, T. J., Cho, S., Choi, S., Go, Y., Gyun, D., Ha, S., Hong, B., Jo, Y., Kim, Y., Lee, K., Lee, K. S., Lee, S., Lim, J., Park, S. K., Roh, Y., Almond, J., Kim, J., Kim, J. S., Lee, H., Lee, K., Nam, K., Oh, S. B., Radburn-Smith, B. C., Seo, S. H., Yang, U. K., Yoo, H. D., Yu, G. B., Kim, H., Kim, J. H., Lee, J. S. H., Park, I. C., Choi, Y., Hwang, C., Lee, J., Yu, I., Dudenas, V., Juodagalvis, A., Vaitkus, J., Ahmed, I., Ibrahim, Z. A., Ali, M. A. B. Md, Idris, F. Mohamad, Abdullah, W. A. T. Wan, Yusli, M. N., Zolkapli, Z., Reyes-Almanza, R., Ramirez-Sanchez, G., Duran-Osuna, M. C., Castilla-Valdez, H., De La Cruz-Burelo, E., La Cruz, I. Heredia-De, Rabadan-Trejo, R. I., Lopez-Fernandez, R., Mejia Guisao, J., Sanchez-Hernandez, A., Moreno, S. Carrillo, Barrera, C. Oropeza, Valencia, F. Vazquez, Eysermans, J., Pedraza, I., Ibarguen, H. A. Salazar, Estrada, C. Uribe, Pineda, A. Morelos, Krofcheck, D., Butler, P. H., Ahmad, A., Ahmad, M., Hassan, Q., Hoorani, H. R., Saddique, A., Shah, M. A., Shoaib, M., Waqas, M., Bialkowska, H., Bluj, M., Boimska, B., Frueboes, T., Górski, M., Kazana, M., Nawrocki, K., Szleper, M., Zalewski, P., Bunkowski, K., Byszuk, A., Doroba, K., Kalinowski, A., Konecki, M., Krolikowski, J., Misiura, M., Olszewski, M., Pyskir, A., Walczak, M., Bargassa, P., Da Cruz E Silva, C. Beirão, Francesco, A. Di, Faccioli, P., Galinhas, B., Gallinaro, M., Hollar, J., Leonardo, N., Iglesias, L. Lloret, Nemallapudi, M. V., Seixas, J., Strong, G., Toldaiev, O., Vadruccio, D., Varela, J., Baginyan, A., Golunov, A., Golutvin, I., Karjavin, V., Korenkov, V., Kozlov, G., Lanev, A., Malakhov, A., Matveev, V., Mitsyn, V. V., Palichik, V., Perelygin, V., Shmatov, S., Skatchkov, N., Smirnov, V., Yuldashev, B. S., Zarubin, A., Zhiltsov, V., Ivanov, Y., Kim, V., Kuznetsova, E., Levchenko, P., Murzin, V., Oreshkin, V., Smirnov, I., Sosnov, D., Sulimov, V., Uvarov, L., Vavilov, S., Vorobyev, A., Andreev, Yu., Dermenev, A., Gninenko, S., Golubev, N., Karneyeu, A., Kirsanov, M., Krasnikov, N., Pashenkov, A., Tlisov, D., Toropin, A., Epshteyn, V., Gavrilov, V., Lychkovskaya, N., Popov, V., Pozdnyakov, I., Safronov, G., Spiridonov, A., Stepennov, A., Toms, M., Vlasov, E., Zhokin, A., Aushev, T., Bylinkin, A., Chadeeva, M., Parygin, P., Philippov, D., Polikarpov, S., Popova, E., Rusinov, V., Andreev, V., Azarkin, M., Dremin, I., Kirakosyan, M., Terkulov, A., Baskakov, A., Belyaev, A., Boos, E., Demiyanov, A., Ershov, A., Gribushin, A., Kodolova, O., Korotkikh, V., Lokhtin, I., Miagkov, I., Obraztsov, S., Petrushanko, S., Savrin, V., Snigirev, A., Vardanyan, I., Blinov, V., Shtol, D., Skovpen, Y., Azhgirey, I., Bayshev, I., Bitioukov, S., Elumakhov, D., Godizov, A., Kachanov, V., Kalinin, A., Konstantinov, D., Mandrik, P., Petrov, V., Ryutin, R., Sobol, A., Troshin, S., Tyurin, N., Uzunian, A., Volkov, A., Adzic, P., Cirkovic, P., Devetak, D., Dordevic, M., Milosevic, J., Rekovic, V., Maestre, J. Alcaraz, Fernández, A. Álvarez, Bachiller, I., Luna, M. Barrio, Cerrada, M., Colino, N., De La Cruz, B., Peris, A. Delgado, Bedoya, C. Fernandez, Ramos, J. P. Fernández, Flix, J., Fouz, M. C., Lopez, O. Gonzalez, Lopez, S. Goy, Hernandez, J. M., Josa, M. I., Moran, D., Yzquierdo, A. Pérez-Calero, Pelayo, J. Puerta, Olmeda, A. Quintario, Redondo, I., Romero, L., Soares, M. S., Albajar, C., de Trocóniz, J. F., Missiroli, M., Cuevas, J., Erice, C., Menendez, J. Fernandez, Caballero, I. Gonzalez, Fernández, J. R. González, Cortezon, E. Palencia, Cruz, S. Sanchez, Vischia, P., Garcia, J. M. Vizan, Cabrillo, I. J., Calderon, A., Quero, B. Chazin, Curras, E., Campderros, J. Duarte, Fernandez, M., Garcia-Ferrero, J., Gomez, G., Virto, A. Lopez, Marco, J., Rivero, C. Martinez, Arbol, P. Martinez Ruiz del, Matorras, F., Gomez, J. Piedra, Rodrigo, T., Ruiz-Jimeno, A., Scodellaro, L., Trevisani, N., Vila, I., Cortabitarte, R. Vilar, Abbaneo, D., Akgun, B., Auffray, E., Baillon, P., Ball, A. H., Barney, D., Bendavid, J., Bianco, M., Bloch, P., Bocci, A., Botta, C., Camporesi, T., Castello, R., Cepeda, M., Cerminara, G., Chapon, E., Chen, Y., d’Enterria, D., Dabrowski, A., Daponte, V., David, A., De Gruttola, M., De Roeck, A., Deelen, N., Dobson, M., Pree, T. du, Dünser, M., Dupont, N., Elliott-Peisert, A., Everaerts, P., Fallavollita, F., Franzoni, G., Fulcher, J., Funk, W., Gigi, D., Gilbert, A., Gill, K., Glege, F., Gulhan, D., Harris, P., Hegeman, J., Innocente, V., Jafari, A., Janot, P., Karacheban, O., Kieseler, J., Knünz, V., Kornmayer, A., Kortelainen, M. J., Krammer, M., Lange, C., Lecoq, P., Lourenço, C., Lucchini, M. T., Malgeri, L., Mannelli, M., Martelli, A., Meijers, F., Merlin, J. A., Mersi, S., Meschi, E., Milenovic, P., Moortgat, F., Mulders, M., Neugebauer, H., Ngadiuba, J., Orfanelli, S., Orsini, L., Pape, L., Perez, E., Peruzzi, M., Petrilli, A., Petrucciani, G., Pfeiffer, A., Pierini, M., Rabady, D., Racz, A., Reis, T., Rolandi, G., Rovere, M., Sakulin, H., Schäfer, C., Schwick, C., Seidel, M., Selvaggi, M., Sharma, A., Silva, P., Sphicas, P., Stakia, A., Steggemann, J., Stoye, M., Tosi, M., Treille, D., Triossi, A., Tsirou, A., Veckalns, V., Verweij, M., Zeuner, W. D., Bertl, W., Caminada, L., Deiters, K., Erdmann, W., Horisberger, R., Ingram, Q., Kaestli, H. C., Kotlinski, D., Langenegger, U., Rohe, T., Wiederkehr, S. A., Backhaus, M., Bäni, L., Berger, P., Bianchini, L., Casal, B., Dissertori, G., Dittmar, M., Donegà, M., Dorfer, C., Grab, C., Heidegger, C., Hits, D., Hoss, J., Kasieczka, G., Klijnsma, T., Lustermann, W., Mangano, B., Marionneau, M., Meinhard, M. T., Meister, D., Micheli, F., Musella, P., Nessi-Tedaldi, F., Pandolfi, F., Pata, J., Pauss, F., Perrin, G., Perrozzi, L., Quittnat, M., Reichmann, M., Becerra, D. A. Sanz, Schönenberger, M., Shchutska, L., Tavolaro, V. R., Theofilatos, K., Olsson, M. L. Vesterbacka, Wallny, R., Zhu, D. H., Aarrestad, T. K., Amsler, C., Canelli, M. F., De Cosa, A., Burgo, R. Del, Donato, S., Galloni, C., Hreus, T., Kilminster, B., Pinna, D., Rauco, G., Robmann, P., Salerno, D., Schweiger, K., Seitz, C., Takahashi, Y., Zucchetta, A., Candelise, V., Chang, Y. H., Cheng, K. y., Doan, T. H., Jain, Sh., Khurana, R., Kuo, C. M., Lin, W., Pozdnyakov, A., Yu, S. S., Kumar, Arun, Chang, P., Chao, Y., Chen, K. F., Chen, P. H., Fiori, F., Hou, W.-S., Hsiung, Y., Liu, Y. F., Lu, R.-S., Paganis, E., Psallidas, A., Steen, A., Tsai, J. F., Asavapibhop, B., Kovitanggoon, K., Singh, G., Srimanobhas, N., Bakirci, M. N., Bat, A., Boran, F., Damarseckin, S., Demiroglu, Z. S., Dozen, C., Eskut, E., Girgis, S., Gokbulut, G., Guler, Y., Hos, I., Kangal, E. E., Kara, O., Kiminsu, U., Oglakci, M., Onengut, G., Ozdemir, K., Ozturk, S., Cerci, D. Sunar, Tok, U. G., Topakli, H., Turkcapar, S., Zorbakir, I. S., Zorbilmez, C., Karapinar, G., Ocalan, K., Yalvac, M., Zeyrek, M., Gülmez, E., Kaya, M., Kaya, O., Tekten, S., Yetkin, E. A., Agaras, M. N., Atay, S., Cakir, A., Cankocak, K., Köseoglu, I., Grynyov, B., Levchuk, L., Ball, F., Beck, L., Brooke, J. J., Burns, D., Clement, E., Cussans, D., Davignon, O., Flacher, H., Goldstein, J., Heath, G. P., Heath, H. F., Kreczko, L., Newbold, D. M., Paramesvaran, S., Sakuma, T., Nasr-storey, S. Seif El, Smith, D., Smith, V. J., Belyaev, A., Brew, C., Brown, R. M., Calligaris, L., Cieri, D., Cockerill, D. J. A., Coughlan, J. A., Harder, K., Harper, S., Linacre, J., Olaiya, E., Petyt, D., Shepherd-Themistocleous, C. H., Thea, A., Tomalin, I. R., Williams, T., Auzinger, G., Bainbridge, R., Borg, J., Breeze, S., Buchmuller, O., Bundock, A., Casasso, S., Citron, M., Colling, D., Corpe, L., Dauncey, P., Davies, G., De Wit, A., Negra, M. Della, Maria, R. Di, Elwood, A., Haddad, Y., Hall, G., Iles, G., James, T., Lane, R., Laner, C., Lyons, L., Magnan, A.-M., Malik, S., Mastrolorenzo, L., Matsushita, T., Nash, J., Nikitenko, A., Palladino, V., Pesaresi, M., Raymond, D. M., Richards, A., Rose, A., Scott, E., Seez, C., Shtipliyski, A., Summers, S., Tapper, A., Uchida, K., Acosta, M. Vazquez, Virdee, T., Wardle, N., Winterbottom, D., Wright, J., Zenz, S. C., Cole, J. E., Hobson, P. R., Khan, A., Kyberd, P., Reid, I. D., Teodorescu, L., Zahid, S., Borzou, A., Call, K., Dittmann, J., Hatakeyama, K., Liu, H., Pastika, N., Smith, C., Bartek, R., Dominguez, A., Buccilli, A., Cooper, S. I., Henderson, C., Rumerio, P., West, C., Arcaro, D., Avetisyan, A., Bose, T., Gastler, D., Rankin, D., Richardson, C., Rohlf, J., Sulak, L., Zou, D., Benelli, G., Cutts, D., Garabedian, A., Hadley, M., Hakala, J., Heintz, U., Hogan, J. M., Kwok, K. H. M., Laird, E., Landsberg, G., Lee, J., Mao, Z., Narain, M., Pazzini, J., Piperov, S., Sagir, S., Syarif, R., Yu, D., Band, R., Brainerd, C., Breedon, R., Burns, D., De La Barca Sanchez, M. Calderon, Chertok, M., Conway, J., Conway, R., Cox, P. T., Erbacher, R., Flores, C., Funk, G., Ko, W., Lander, R., Mclean, C., Mulhearn, M., Pellett, D., Pilot, J., Shalhout, S., Shi, M., Smith, J., Stolp, D., Tos, K., Tripathi, M., Wang, Z., Bachtis, M., Bravo, C., Cousins, R., Dasgupta, A., Florent, A., Hauser, J., Ignatenko, M., Mccoll, N., Regnard, S., Saltzberg, D., Schnaible, C., Valuev, V., Bouvier, E., Burt, K., Clare, R., Ellison, J., Gary, J. W., Shirazi, S. M. A. Ghiasi, Hanson, G., Heilman, J., Karapostoli, G., Kennedy, E., Lacroix, F., Long, O. R., Negrete, M. Olmedo, Paneva, M. I., Si, W., Wang, L., Wei, H., Wimpenny, S., Yates, B. R., Branson, J. G., Cittolin, S., Derdzinski, M., Gerosa, R., Gilbert, D., Hashemi, B., Holzner, A., Klein, D., Kole, G., Krutelyov, V., Letts, J., Masciovecchio, M., Olivito, D., Padhi, S., Pieri, M., Sani, M., Sharma, V., Tadel, M., Vartak, A., Wasserbaech, S., Wood, J., Würthwein, F., Yagil, A., Porta, G. Zevi Della, Amin, N., Bhandari, R., Bradmiller-Feld, J., Campagnari, C., Dishaw, A., Dutta, V., Sevilla, M. Franco, Gouskos, L., Heller, R., Incandela, J., Ovcharova, A., Qu, H., Richman, J., Stuart, D., Suarez, I., Yoo, J., Anderson, D., Bornheim, A., Lawhorn, J. M., Newman, H. B., Nguyen, T., Pena, C., Spiropulu, M., Vlimant, J. R., Xie, S., Zhang, Z., Zhu, R. Y., Andrews, M. B., Ferguson, T., Mudholkar, T., Paulini, M., Russ, J., Sun, M., Vogel, H., Vorobiev, I., Weinberg, M., Cumalat, J. P., Ford, W. T., Jensen, F., Johnson, A., Krohn, M., Leontsinis, S., Mulholland, T., Stenson, K., Wagner, S. R., Alexander, J., Chaves, J., Chu, J., Dittmer, S., Mcdermott, K., Mirman, N., Patterson, J. R., Quach, D., Rinkevicius, A., Ryd, A., Skinnari, L., Soffi, L., Tan, S. M., Tao, Z., Thom, J., Tucker, J., Wittich, P., Zientek, M., Abdullin, S., Albrow, M., Alyari, M., Apollinari, G., Apresyan, A., Apyan, A., Banerjee, S., Bauerdick, L. A. T., Beretvas, A., Berryhill, J., Bhat, P. C., Bolla, G., Burkett, K., Butler, J. N., Canepa, A., Cerati, G. B., Cheung, H. W. K., Chlebana, F., Cremonesi, M., Duarte, J., Elvira, V. D., Freeman, J., Gecse, Z., Gottschalk, E., Gray, L., Green, D., Grünendahl, S., Gutsche, O., Harris, R. M., Hasegawa, S., Hirschauer, J., Hu, Z., Jayatilaka, B., Jindariani, S., Johnson, M., Joshi, U., Klima, B., Kreis, B., Lammel, S., Lincoln, D., Lipton, R., Liu, M., Liu, T., De Sá, R. Lopes, Lykken, J., Maeshima, K., Magini, N., Marraffino, J. M., Mason, D., McBride, P., Merkel, P., Mrenna, S., Nahn, S., O’Dell, V., Pedro, K., Prokofyev, O., Rakness, G., Ristori, L., Schneider, B., Sexton-Kennedy, E., Soha, A., Spalding, W. J., Spiegel, L., Stoynev, S., Strait, J., Strobbe, N., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vernieri, C., Verzocchi, M., Vidal, R., Wang, M., Weber, H. A., Whitbeck, A., Acosta, D., Avery, P., Bortignon, P., Bourilkov, D., Brinkerhoff, A., Carnes, A., Carver, M., Curry, D., Field, R. D., Furic, I. K., Gleyzer, S. V., Joshi, B. M., Konigsberg, J., Korytov, A., Kotov, K., Ma, P., Matchev, K., Mei, H., Mitselmakher, G., Shi, K., Sperka, D., Terentyev, N., Thomas, L., Wang, J., Wang, S., Yelton, J., Joshi, Y. R., Linn, S., Markowitz, P., Rodriguez, J. L., Ackert, A., Adams, T., Askew, A., Hagopian, S., Hagopian, V., Johnson, K. F., Kolberg, T., Martinez, G., Perry, T., Prosper, H., Saha, A., Santra, A., Sharma, V., Yohay, R., Baarmand, M. M., Bhopatkar, V., Colafranceschi, S., Hohlmann, M., Noonan, D., Roy, T., Yumiceva, F., Adams, M. R., Apanasevich, L., Berry, D., Betts, R. R., Cavanaugh, R., Chen, X., Evdokimov, O., Gerber, C. E., Hangal, D. A., Hofman, D. J., Jung, K., Kamin, J., Gonzalez, I. D. Sandoval, Tonjes, M. B., Trauger, H., Varelas, N., Wang, H., Wu, Z., Zhang, J., Bilki, B., Clarida, W., Dilsiz, K., Durgut, S., Gandrajula, R. P., Haytmyradov, M., Khristenko, V., Merlo, J.-P., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Ogul, H., Onel, Y., Ozok, F., Penzo, A., Snyder, C., Tiras, E., Wetzel, J., Yi, K., Blumenfeld, B., Cocoros, A., Eminizer, N., Fehling, D., Feng, L., Gritsan, A. V., Maksimovic, P., Roskes, J., Sarica, U., Swartz, M., Xiao, M., You, C., Al-bataineh, A., Baringer, P., Bean, A., Boren, S., Bowen, J., Castle, J., Khalil, S., Kropivnitskaya, A., Majumder, D., Mcbrayer, W., Murray, M., Royon, C., Sanders, S., Schmitz, E., Takaki, J. D. Tapia, Wang, Q., Ivanov, A., Kaadze, K., Maravin, Y., Mohammadi, A., Saini, L. K., Skhirtladze, N., Rebassoo, F., Wright, D., Anelli, C., Baden, A., Baron, O., Belloni, A., Eno, S. C., Feng, Y., Ferraioli, C., Hadley, N. J., Jabeen, S., Jeng, G. Y., Kellogg, R. G., Kunkle, J., Mignerey, A. C., Ricci-Tam, F., Shin, Y. H., Skuja, A., Tonwar, S. C., Abercrombie, D., Allen, B., Azzolini, V., Barbieri, R., Baty, A., Bi, R., Brandt, S., Busza, W., Cali, I. A., D’Alfonso, M., Demiragli, Z., Ceballos, G. Gomez, Goncharov, M., Hsu, D., Hu, M., Iiyama, Y., Innocenti, G. M., Klute, M., Kovalskyi, D., Lee, Y.-J., Levin, A., Luckey, P. D., Maier, B., Marini, A. C., Mcginn, C., Mironov, C., Narayanan, S., Niu, X., Paus, C., Roland, C., Roland, G., Salfeld-Nebgen, J., Stephans, G. S. F., Tatar, K., Velicanu, D., Wang, J., Wang, T. W., Wyslouch, B., Benvenuti, A. C., Chatterjee, R. M., Evans, A., Hansen, P., Hiltbrand, J., Kalafut, S., Kubota, Y., Lesko, Z., Mans, J., Nourbakhsh, S., Ruckstuhl, N., Rusack, R., Turkewitz, J., Wadud, M. A., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Golf, F., Suarez, R. Gonzalez, Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Dolen, J., Godshalk, A., Harrington, C., Iashvili, I., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Freer, C., Hortiangtham, A., Massironi, A., Morse, D. M., Orimoto, T., De Lima, R. Teixeira, Trocino, D., Wamorkar, T., Wang, B., Wisecarver, A., Wood, D., Bhattacharya, S., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Schmitt, M. H., Sung, K., Trovato, M., Velasco, M., Bucci, R., Dev, N., Hildreth, M., Anampa, K. Hurtado, Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Li, W., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Siddireddy, P., Smith, G., Taroni, S., Wayne, M., Wightman, A., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Liu, B., Luo, W., Winer, B. L., Wulsin, H. W., Cooperstein, S., Driga, O., Elmer, P., Hardenbrook, J., Hebda, P., Higginbotham, S., Kalogeropoulos, A., Lange, D., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Piroué, P., Stickland, D., Tully, C., Malik, S., Norberg, S., Barker, A., Barnes, V. E., Das, S., Folgueras, S., Gutay, L., Jha, M. K., Jones, M., Jung, A. W., Khatiwada, A., Miller, D. H., Neumeister, N., Peng, C. C., Qiu, H., Schulte, J. F., Sun, J., Wang, F., Xiao, R., Xie, W., Cheng, T., Parashar, N., Stupak, J., Chen, Z., Ecklund, K. M., Freed, S., Geurts, F. J. M., Guilbaud, M., Kilpatrick, M., Li, W., Michlin, B., Padley, B. P., Roberts, J., Rorie, J., Shi, W., Tu, Z., Zabel, J., Zhang, A., Bodek, A., de Barbaro, P., Demina, R., Duh, Y. t., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, P., Verzetti, M., Ciesielski, R., Goulianos, K., Mesropian, C., Agapitos, A., Chou, J. P., Gershtein, Y., Espinosa, T. A. Gómez, Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Delannoy, A. G., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Hernandez, A. Castaneda, Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Perniè, L., Rathjens, D., Safonov, A., Tatarinov, A., Ulmer, K. A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Faulkner, J., Gurpinar, E., Kunori, S., Lamichhane, K., Lee, S. W., Libeiro, T., Mengke, T., Muthumuni, S., Peltola, T., Undleeb, S., Volobouev, I., Wang, Z., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Padeken, K., Sheldon, P., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, P., Cox, B., Hirosky, R., Joyce, M., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Wang, Y., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Poudyal, N., Sturdy, J., Thapa, P., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Hervé, A., Hussain, U., Klabbers, P., Lanaro, A., Levine, A., Long, K., Loveless, R., Ruggles, T., Savin, A., Smith, N., Smith, W. H., Taylor, D., and Woods, N.
Published: 2023
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20. Nucleosynthesis in 2D Core-Collapse Supernovae of 11.2 and 17.0 M$_{\odot}$ Progenitors: Implications for Mo and Ru Production

Author: Eichler, M., Nakamura, K., Takiwaki, T., Kuroda, T., Kotake, K., Hempel, M., Cabezón, R., Liebendörfer, M., and Thielemann, F-K.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Core-collapse supernovae are the first polluters of heavy elements in the galactic history. As such, it is important to study the nuclear compositions of their ejecta, and understand their dependence on the progenitor structure (e.g., mass, compactness, metallicity). Here, we present a detailed nucleosynthesis study based on two long-term, two-dimensional core-collapse supernova simulations of a 11.2 M$_{\odot}$ and a 17.0 M$_{\odot}$ star. We find that in both models nuclei well beyond the iron group (up to $Z \approx 44$) can be produced, and discuss in detail also the nucleosynthesis of the p-nuclei $^{92,94}$Mo and $^{96,98}$Ru. While we observe the production of $^{92}$Mo and $^{94}$Mo in slightly neutron-rich conditions in both simulations, $^{96,98}$Ru can only be produced efficiently via the $\nu$p-process. Furthermore, the production of Ru in the $\nu$p-process heavily depends on the presence of very proton-rich material in the ejecta. This disentanglement of production mechanisms has interesting consequences when comparing to the abundance ratios between these isotopes in the solar system and in presolar grains., Comment: 48 pages, 19 figures, accepted for publication in: J. Phys. G: Nucl. Part. Phys
Published: 2017
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21. Measurement of shower development and its Moli\`ere radius with a four-plane LumiCal test set-up

Author: Abramowicz, H., Abusleme, A., Afanaciev, K., Benhammou, Y., Bortko, L., Borysov, O., Borysova, M., Bozovic-Jelisavcic, I., Chelkov, G., Daniluk, W., Dannheim, D., Elsener, K., Firlej, M., Firu, E., Fiutowski, T., Ghenescu, V., Gostkin, M., Hempel, M., Henschel, H., Idzik, M., Ignatenko, A., Ishikawa, A., Kananov, S., Karacheban, O., Klempt, W., Kotov, S., Kotula, J., Kozhevnikov, D., Kruchonok, V., Krupa, B., Kulis, Sz., Lange, W., Leonard, J., Lesiak, T., Levy, A., Levy, I., Lohmann, W., Lukic, S., Moron, J., Moszczynski, A., Neagu, A. T., Nuiry, F. -X., Pandurovic, M., Pawlik, B., Preda, T., Rosenblat, O., Sailer, A., Schumm, B., Schuwalow, S., Smiljanic, I., Smolyanskiy, P., Swientek, K., Terlecki, P., Uggerhoj, U. I., Wistisen, T. N., Wojton, T., Yamamoto, H., Zawiejski, L., Zgura, I. S., and Zhemchugov, A.
Subjects: Physics - Instrumentation and Detectors
Abstract: A prototype of a luminometer, designed for a future e+e- collider detector, and consisting at present of a four-plane module, was tested in the CERN PS accelerator T9 beam. The objective of this beam test was to demonstrate a multi-plane tungsten/silicon operation, to study the development of the electromagnetic shower and to compare it with MC simulations. The Moli\`ere radius has been determined to be 24.0 +/- 0.6 (stat.) +/- 1.5 (syst.) mm using a parametrization of the shower shape. Very good agreement was found between data and a detailed Geant4 simulation., Comment: Paper published in Eur. Phys. J., includes 25 figures and 3 Tables
Published: 2017
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22. Equations of state for supernovae and compact stars

Author: Oertel, M., Hempel, M., Klähn, T., and Typel, S.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics, Nuclear Theory
Abstract: We review various theoretical approaches for the equation of state (EoS) of dense matter, relevant for the description of core-collapse supernovae, compact stars and compact star mergers. The emphasis is put on models that are applicable to all of these scenarios. Such EoS models have to cover large ranges in baryon number density, temperature and isospin asymmetry. The characteristics of matter change dramatically within these ranges, from a mixture of nucleons, nuclei, and electrons to uniform, strongly interacting matter containing nucleons, and possibly other particles such as hyperons or quarks. As the development of an EoS requires joint efforts from many directions we consider different theoretical approaches and discuss relevant experimental and observational constraints which provide insights for future research. Finally, results from applications of the discussed EoS models are summarized., Comment: 74 pages, 19 figures
Published: 2016
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23. Orbital and physical parameters of eclipsing binaries from the ASAS catalogue -- IX. Spotted pairs with red giants

Author: Ratajczak, M., Hełminiak, K. G., Konacki, M., Smith, A. M. S., Kozłowski, S. K., Espinoza, N., Jordán, A., Brahm, R., Hempel, M., Anderson, D. R., and Hellier, C.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: We present spectroscopic and photometric solutions for three spotted systems with red giant components. Absolute physical and orbital parameters for these double-lined detached eclipsing binary stars are presented for the first time. These were derived from the V-, and I-band ASAS and WASP photometry, and new radial velocities calculated from high quality optical spectra we obtained with a wide range of spectrographs and using the two-dimensional cross-correlation technique (TODCOR). All of the investigated systems (ASAS J184949-1518.7, BQ Aqr, and V1207 Cen) show the differential evolutionary phase of their components consisting of a main sequence star or a subgiant and a red giant, and thus constitute very informative objects in terms of testing stellar evolution models. Additionally, the systems show significant chromospheric activity of both components. They can be also classified as classical RS CVn-type stars. Besides the standard analysis of radial velocities and photometry, we applied spectral disentangling to obtain separate spectra for both components of each analysed system which allowed for a more detailed spectroscopic study. We also compared the properties of red giant stars in binaries that show spots, with those that do not, and found that the activity phenomenon is substantially suppressed for stars with Rossby number higher than $\sim$1 and radii larger than $\sim$20 R$_\odot$., Comment: Published in MNRAS, 18 pages, 11 figures
Published: 2016
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24. Expected impact from weak reactions with light nuclei in core-collapse supernova simulations

Author: Fischer, T., Martínez-Pinedo, G., Hempel, M., Huther, L., Röpke, G., Typel, S., and Lohs, A.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Nuclear Theory
Abstract: We study the role of light nuclear clusters in simulations of core-collapse supernovae. Expressions for the reaction rates are developed for a large selection of charged current absorption and scattering processes with light clusters. Medium modifications are taken into account at the mean-field level. We explore the possible impact on the supernova dynamics and the neutrino signal during the mass accretion phase prior to the possible explosion onset as well as during the subsequent protoneutron star deleptnoization after the explosion onset has been launched., Comment: 7 pages, 3 figures, contribution to the OMEG 2015 conference proceedings, appears in EPJ WoC proceedings
Published: 2015
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25. Stellar density profile and mass of the Milky Way Bulge from VVV data

Author: Valenti, E., Zoccali, M., Gonzalez, O. A., Minniti, D., Alonso-Garcia, J., Marchetti, E., Hempel, M., Renzini, A., and Rejkuba, M.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present the first stellar density profile of the Milky Way bulge reaching latitude $b=0^\circ$. It is derived by counting red clump stars within the colour\--magnitude diagram constructed with the new PSF-fitting photometry from VISTA Variables in the V\'\i a L\'actea (VVV) survey data. The new stellar density map covers the area between $|l|\leq 10^\circ$ and $|b|\leq 4.5^\circ$ with unprecedented accuracy, allowing to establish a direct link between the stellar kinematics from the Giraffe Inner Bulge Spectroscopic Survey (GIBS) and the stellar mass density distribution. In particular, the location of the central velocity dispersion peak from GIBS matches a high overdensity in the VVV star count map. By scaling the total luminosity function (LF) obtained from all VVV fields to the LF from Zoccali et al.(2003), we obtain the first fully empirical estimate of the mass in stars and remnants of the Galactic bulge. The Milky Way bulge stellar mass within ($|b|<9.5^\circ$, $|l|<10^\circ$) is $2.0\pm0.3\times 10^{10}M_{\odot}$., Comment: 4 pages, 5 figures, accepted for publication on A&A
Published: 2015
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26. Erratum to: Measurement of exclusive ΥsNN=5.02TeV photoproduction from protons in pPb collisions at ΥsNN=5.02TeV

Author: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Erö, J., Valle, A. Escalante Del, Flechl, M., Friedl, M., Frühwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., König, A., Krammer, N., Krätschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rad, N., Rohringer, H., Schieck, J., Schöfbeck, R., Spanring, M., Spitzbart, D., Taurok, A., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Croce, D. Di, Janssen, X., Lauwers, J., Pieters, M., De Klundert, M. Van, Haevermaet, H. Van, Mechelen, P. Van, Remortel, N. Van, Zeid, S. Abu, Blekman, F., D’Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Marchesini, I., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Doninck, W. Van, Mulders, P. Van, Parijs, I. Van, Beghin, D., Bilin, B., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Dorney, B., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Kalsi, A. K., Lenzi, T., Luetic, J., Seva, T., Starling, E., Velde, C. Vander, Vanlaer, P., Vannerom, D., Yonamine, R., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Trocino, D., Tytgat, M., Verbeke, W., Vermassen, B., Vit, M., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caputo, C., Caudron, A., David, P., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Saggio, A., Marono, M. Vidal, Wertz, S., Zobec, J., Júnior, W. L. Aldá, Alves, F. L., Alves, G.A., Brito, L., Silva, G. Correia, Hensel, C., Moraes, A., Pol, M. E., Teles, P. Rebello, Chagas, E. Belchior Batista Das, Carvalho, W., Chinellato, J., Coelho, E., Da Costa, E. M., Da Silveira, G.G., De Jesus Damiao, D., De Souza, S. Fonseca, Malbouisson, H., Jaime, M. Medina, De Almeida, M. Melo, Herrera, C. Mora, Mundim, L., Nogima, H., Rosas, L. J. Sanchez, Santoro, A., Sznajder, A., Thiel, M., Manganote, E. J. Tonelli, Da Silva De Araujo, F. Torres, Pereira, A. Vilela, Ahuja, S., Bernardes, C. A., Calligaris, L., Tomei, T. R. Fernandez Perez, Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Abad, D. Romero, Vargas, J. C. Ruiz, Aleksandrov, A., Hadjiiska, R., Iaydjiev, P., Marinov, A., Misheva, M., Rodozov, M., Shopova, M., Sultanov, G., Dimitrov, A., Litov, L., Pavlov, B., Petkov, P., Fang, W., Gao, X., Yuan, L., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhao, J., Ban, Y., Chen, G., Li, J., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Wang, Y., Avila, C., Cabrera, A., Montoya, C. A. Carrillo, Sierra, L. F. Chaparro, Florez, C., Hernández, C. F. González, Delgado, M. A. Segura, Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Cipriano, P. M. Ribeiro, Sculac, T., Antunovic, Z., Kovac, M., Brigljevic, V., Ferencek, D., Kadija, K., Mesic, B., Starodumov, A., Susa, T., Ather, M. W., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Rykaczewski, H., Finger, M., Finger, Jr., M., Jarrin, E. Carrera, Khalil, S., Mahmoud, M. A., Mohammed, Y., Bhowmik, S., Dewanjee, R. K., Kadastik, M., Perrini, L., Raidal, M., Veelken, C., Eerola, P., Kirschenmann, H., Pekkanen, J., Voutilainen, M., Havukainen, J., Heikkilä, J. K., Järvinen, T., Karimäki, V., Kinnunen, R., Lampén, T., Lassila-Perini, K., Laurila, S., Lehti, S., Lindén, T., Luukka, P., Mäenpää, T., Siikonen, H., Tuominen, E., Tuominiemi, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. L., Ferri, F., Ganjour, S., Ghosh, S., Givernaud, A., Gras, P., de Monchenault, G. Hamel, Jarry, P., Leloup, C., Locci, E., Machet, M., Malcles, J., Negro, G., Rander, J., Rosowsky, A., Sahin, M. Ö., Titov, M., Abdulsalam, A., Amendola, C., Antropov, I., Baffioni, S., Beaudette, F., Busson, P., Cadamuro, L., Charlot, C., de Cassagnac, R. Granier, Jo, M., Kucher, I., Lisniak, S., Lobanov, A., Blanco, J. Martin, Nguyen, M., Ochando, C., Ortona, G., Paganini, P., Pigard, P., Salerno, R., Sauvan, J. B., Sirois, Y., Leiton, A. G. Stahl, Yilmaz, Y., Zabi, A., Zghiche, A., Agram, J.-L., Andrea, J., Bloch, D., Brom, J.-M., Chabert, E. C., Collard, C., Conte, E., Coubez, X., Drouhin, F., Fontaine, J.-C., Gelé, D., Goerlach, U., Jansová, M., Juillot, P., Bihan, A.-C. Le, Tonon, N., Hove, P. Van, Gadrat, S., Beauceron, S., Bernet, C., Boudoul, G., Chanon, N., Chierici, R., Contardo, D., Depasse, P., Mamouni, H. El, Fay, J., Finco, L., Gascon, S., Gouzevitch, M., Grenier, G., Ille, B., Lagarde, F., Laktineh, I. B., Lattaud, H., Lethuillier, M., Mirabito, L., Pequegnot, A. L., Perries, S., Popov, A., Sordini, V., Donckt, M. Vander, Viret, S., Zhang, S., Toriashvili, T., Tsamalaidze, Z., Autermann, C., Feld, L., Kiesel, M. K., Klein, K., Lipinski, M., Preuten, M., Rauch, M. P., Schomakers, C., Schulz, J., Teroerde, M., Wittmer, B., Zhukov, V., Albert, A., Duchardt, D., Endres, M., Erdmann, M., Erdweg, S., Esch, T., Fischer, R., Güth, A., Hebbeker, T., Heidemann, C., Hoepfner, K., Knutzen, S., Merschmeyer, M., Meyer, A., Millet, P., Mukherjee, S., Pook, T., Radziej, M., Reithler, H., Rieger, M., Scheuch, F., Teyssier, D., Thüer, S., Flügge, G., Kargoll, B., Kress, T., Künsken, A., Müller, T., Nehrkorn, A., Nowack, A., Pistone, C., Pooth, O., Stahl, A., Martin, M. Aldaya, Arndt, T., Asawatangtrakuldee, C., Beernaert, K., Behnke, O., Behrens, U., Martínez, A. Bermúdez, Anuar, A. A. Bin, Borras, K., Botta, V., Campbell, A., Connor, P., Contreras-Campana, C., Costanza, F., Danilov, V., De Wit, A., Pardos, C. Diez, Damiani, D. Domínguez, Eckerlin, G., Eckstein, D., Eichhorn, T., Elwood, A., Eren, E., Gallo, E., Garcia, J. Garay, Geiser, A., Luyando, J. M. Grados, Grohsjean, A., Gunnellini, P., Guthoff, M., Harb, A., Hauk, J., Hempel, M., Jung, H., Kasemann, M., Keaveney, J., Kleinwort, C., Knolle, J., Korol, I., Krücker, D., Lange, W., Lelek, A., Lenz, T., Lipka, K., Lohmann, W., Mankel, R., Melzer-Pellmann, I.-A., Meyer, A. B., Meyer, M., Missiroli, M., Mittag, G., Mnich, J., Mussgiller, A., Pitzl, D., Raspereza, A., Savitskyi, M., Saxena, P., Shevchenko, R., Stefaniuk, N., Tholen, H., Onsem, G. P. Van, Walsh, R., Wen, Y., Wichmann, K., Wissing, C., Zenaiev, O., Aggleton, R., Bein, S., Blobel, V., Vignali, M. Centis, Dreyer, T., Garutti, E., Gonzalez, D., Haller, J., Hinzmann, A., Hoffmann, M., Karavdina, A., Kasieczka, G., Klanner, R., Kogler, R., Kovalchuk, N., Kurz, S., Kutzner, V., Lange, J., Marconi, D., Multhaup, J., Niedziela, M., Nowatschin, D., Peiffer, T., Perieanu, A., Reimers, A., Scharf, C., Schleper, P., Schmidt, A., Schumann, S., Schwandt, J., Sonneveld, J., Stadie, H., Steinbrück, G., Stober, F. M., Stöver, M., Troendle, D., Usai, E., Vanhoefer, A., Vormwald, B., Akbiyik, M., Barth, C., Baselga, M., Baur, S., Butz, E., Caspart, R., Chwalek, T., Colombo, F., De Boer, W., Dierlamm, A., Faltermann, N., Freund, B., Friese, R., Giffels, M., Harrendorf, M. A., Hartmann, F., Heindl, S. M., Husemann, U., Kassel, F., Kudella, S., Mildner, H., Mozer, M. U., Müller, Th., Plagge, M., Quast, G., Rabbertz, K., Schröder, M., Shvetsov, I., Sieber, G., Simonis, H. J., Ulrich, R., Wayand, S., Weber, M., Weiler, T., Williamson, S., Wöhrmann, C., Wolf, R., Anagnostou, G., Daskalakis, G., Geralis, T., Kyriakis, A., Loukas, D., Topsis-Giotis, I., Karathanasis, G., Kesisoglou, S., Panagiotou, A., Saoulidou, N., Tziaferi, E., Kousouris, K., Papakrivopoulos, I., Evangelou, I., Foudas, C., Gianneios, P., Katsoulis, P., Kokkas, P., Mallios, S., Manthos, N., Papadopoulos, I., Paradas, E., Strologas, J., Triantis, F. A., Tsitsonis, D., Csanad, M., Filipovic, N., Pasztor, G., Surányi, O., Veres, G. I., Bencze, G., Hajdu, C., Horvath, D., Hunyadi, Á., Sikler, F., Vámi, T. Á., Veszpremi, V., Vesztergombi, G., Beni, N., Czellar, S., Karancsi, J., Makovec, A., Molnar, J., Szillasi, Z., Bartók, M., Raics, P., Trocsanyi, Z. L., Ujvari, B., Choudhury, S., Komaragiri, J. R., Bahinipati, S., Mal, P., Mandal, K., Nayak, A., Sahoo, D. K., Swain, S. K., Bansal, S., Beri, S. B., Bhatnagar, V., Chauhan, S., Chawla, R., Dhingra, N., Gupta, R., Kaur, A., Kaur, M., Kaur, S., Kumar, R., Kumari, P., Lohan, M., Mehta, A., Sharma, S., Singh, J. B., Walia, G., Bhardwaj, A., Choudhary, B.C., Garg, R. B., Keshri, S., Kumar, A., Kumar, Ashok, Malhotra, S., Naimuddin, M., Ranjan, K., Shah, Aashaq, Sharma, R., Bhardwaj, R., Bhattacharya, R., Bhattacharya, S., Bhawandeep, U., Bhowmik, D., Dey, S., Dutt, S., Dutta, S., Ghosh, S., Majumdar, N., Mondal, K., Mukhopadhyay, S., Nandan, S., Purohit, A., Rout, P. K., Roy, A., Chowdhury, S. Roy, Sarkar, S., Sharan, M., Singh, B., Thakur, S., Behera, P. K., Chudasama, R., Dutta, D., Jha, V., Kumar, V., Mohanty, A. K., Netrakanti, P. K., Pant, L. M., Shukla, P., Topkar, A., Aziz, T., Dugad, S., Mahakud, B., Mitra, S., Mohanty, G. B., Sur, N., Sutar, B., Banerjee, S., Bhattacharya, S., Chatterjee, S., Das, P., Guchait, M., Jain, Sa., Kumar, S., Maity, M., Majumder, G., Mazumdar, K., Sahoo, N., Sarkar, T., Wickramage, N., Chauhan, S., Dube, S., Hegde, V., Kapoor, A., Kothekar, K., Pandey, S., Rane, A., Sharma, S., Chenarani, S., Tadavani, E. Eskandari, Etesami, S. M., Khakzad, M., Najafabadi, M. Mohammadi, Naseri, M., Mehdiabadi, S. Paktinat, Hosseinabadi, F. Rezaei, Safarzadeh, B., Zeinali, M., Felcini, M., Grunewald, M., Abbrescia, M., Calabria, C., Colaleo, A., Creanza, D., Cristella, L., De Filippis, N., De Palma, M., Florio, A. Di, Errico, F., Fiore, L., Gelmi, A., Iaselli, G., Lezki, S., Maggi, G., Maggi, M., Marangelli, B., Miniello, G., My, S., Nuzzo, S., Pompili, A., Pugliese, G., Radogna, R., Ranieri, A., Selvaggi, G., Sharma, A., Silvestris, L., Venditti, R., Verwilligen, P., Zito, G., Abbiendi, G., Battilana, C., Bonacorsi, D., Borgonovi, L., Braibant-Giacomelli, S., Campanini, R., Capiluppi, P., Castro, A., Cavallo, F. R., Chhibra, S. S., Codispoti, G., Cuffiani, M., Dallavalle, G. M., Fabbri, F., Fanfani, A., Fasanella, D., Giacomelli, P., Grandi, C., Guiducci, L., Marcellini, S., Masetti, G., Montanari, A., Navarria, F. L., Odorici, F., Perrotta, A., Rossi, A. M., Rovelli, T., Siroli, G. P., Tosi, N., Albergo, S., Costa, S., Mattia, A. Di, Giordano, F., Potenza, R., Tricomi, A., Tuve, C., Barbagli, G., Chatterjee, K., Ciulli, V., Civinini, C., D’Alessandro, R., Focardi, E., Latino, G., Lenzi, P., Meschini, M., Paoletti, S., Russo, L., Sguazzoni, G., Strom, D., Viliani, L., Benussi, L., Bianco, S., Fabbri, F., Piccolo, D., Primavera, F., Calvelli, V., Ferro, F., Ravera, F., Robutti, E., Tosi, S., Benaglia, A., Beschi, A., Brianza, L., Brivio, F., Ciriolo, V., Dinardo, M.E., Fiorendi, S., Gennai, S., Ghezzi, A., Govoni, P., Malberti, M., Malvezzi, S., Manzoni, R. A., Menasce, D., Moroni, L., Paganoni, M., Pauwels, K., Pedrini, D., Pigazzini, S., Ragazzi, S., de Fatis, T. Tabarelli, Buontempo, S., Cavallo, N., Guida, S. Di, Fabozzi, F., Fienga, F., Galati, G., Iorio, A. O. M., Khan, W. A., Lista, L., Meola, S., Paolucci, P., Sciacca, C., Thyssen, F., Voevodina, E., Azzi, P., Bacchetta, N., Benato, L., Bisello, D., Boletti, A., Carlin, R., De Oliveira, A. Carvalho Antunes, Checchia, P., De Castro Manzano, P., Dorigo, T., Dosselli, U., Gasparini, F., Gasparini, U., Gozzelino, A., Lacaprara, S., Lujan, P., Margoni, M., Meneguzzo, A. T., Pozzobon, N., Ronchese, P., Rossin, R., Simonetto, F., Tiko, A., Zanetti, M., Zotto, P., Zumerle, G., Braghieri, A., Magnani, A., Montagna, P., Ratti, S. P., Re, V., Ressegotti, M., Riccardi, C., Salvini, P., Vai, I., Vitulo, P., Solestizi, L. Alunni, Biasini, M., Bilei, G.M., Cecchi, C., Ciangottini, D., Fanò, L., Lariccia, P., Leonardi, R., Manoni, E., Mantovani, G., Mariani, V., Menichelli, M., Rossi, A., Santocchia, A., Spiga, D., Androsov, K., Azzurri, P., Bagliesi, G., Bianchini, L., Boccali, T., Borrello, L., Castaldi, R., Ciocci, M. A., Dell’Orso, R., Fedi, G., Giannini, L., Giassi, A., Grippo, M. T., Ligabue, F., Lomtadze, T., Manca, E., Mandorli, G., Messineo, A., Palla, F., Rizzi, A., Spagnolo, P., Tenchini, R., Tonelli, G., Venturi, A., Verdini, P. G., Barone, L., Cavallari, F., Cipriani, M., Daci, N., Re, D. Del, Marco, E. Di, Diemoz, M., Gelli, S., Longo, E., Marzocchi, B., Meridiani, P., Organtini, G., Pandolfi, F., Paramatti, R., Preiato, F., Rahatlou, S., Rovelli, C., Santanastasio, F., Amapane, N., Arcidiacono, R., Argiro, S., Arneodo, M., Bartosik, N., Bellan, R., Biino, C., Cartiglia, N., Castello, R., Cenna, F., Costa, M., Covarelli, R., Degano, A., Demaria, N., Kiani, B., Mariotti, C., Maselli, S., Migliore, E., Monaco, V., Monteil, E., Monteno, M., Obertino, M. M., Pacher, L., Pastrone, N., Pelliccioni, M., Angioni, G. L. Pinna, Romero, A., Ruspa, M., Sacchi, R., Shchelina, K., Sola, V., Solano, A., Staiano, A., Belforte, S., Casarsa, M., Cossutti, F., Ricca, G. Della, Zanetti, A., Kim, D. H., Kim, G. N., Kim, M. S., Lee, J., Lee, S., Lee, S. W., Moon, C. S., Oh, Y. D., Sekmen, S., Son, D. C., Yang, Y. C., Kim, H., Moon, D. H., Oh, G., Cifuentes, J. A. Brochero, Goh, J., Kim, T. J., Cho, S., Choi, S., Go, Y., Gyun, D., Ha, S., Hong, B., Jo, Y., Kim, Y., Lee, K., Lee, K. S., Lee, S., Lim, J., Park, S. K., Roh, Y., Almond, J., Kim, J., Kim, J. S., Lee, H., Lee, K., Nam, K., Oh, S. B., Radburn-Smith, B. C., Seo, S. h., Yang, U. K., Yoo, H. D., Yu, G. B., Kim, H., Kim, J. H., Lee, J. S. H., Park, I. C., Choi, Y., Hwang, C., Lee, J., Yu, I., Dudenas, V., Juodagalvis, A., Vaitkus, J., Ahmed, I., Ibrahim, Z. A., Ali, M. A. B. Md, Idris, F. Mohamad, Abdullah, W. A. T. Wan, Yusli, M. N., Zolkapli, Z., Castilla-Valdez, H., De La Cruz-Burelo, E., Duran-Osuna, M. C., La Cruz, I. Heredia-De, Lopez-Fernandez, R., Guisao, J. Mejia, Rabadan-Trejo, R. I., Ramirez-Sanchez, G., Reyes-Almanza, R., Sanchez-Hernandez, A., Moreno, S. Carrillo, Barrera, C. Oropeza, Valencia, F. Vazquez, Eysermans, J., Pedraza, I., Ibarguen, H. A. Salazar, Estrada, C. Uribe, Pineda, A. Morelos, Krofcheck, D., Bheesette, S., Butler, P. H., Ahmad, A., Ahmad, M., Hassan, Q., Hoorani, H. R., Saddique, A., Shah, M. A., Shoaib, M., Waqas, M., Bialkowska, H., Bluj, M., Boimska, B., Frueboes, T., Górski, M., Kazana, M., Nawrocki, K., Szleper, M., Traczyk, P., Zalewski, P., Bunkowski, K., Byszuk, A., Doroba, K., Kalinowski, A., Konecki, M., Krolikowski, J., Misiura, M., Olszewski, M., Pyskir, A., Walczak, M., Bargassa, P., Da Cruz E Silva, C. Beirão, Francesco, A. Di, Faccioli, P., Galinhas, B., Gallinaro, M., Hollar, J., Leonardo, N., Iglesias, L. Lloret, Nemallapudi, M. V., Seixas, J., Strong, G., Toldaiev, O., Vadruccio, D., Varela, J., Afanasiev, S., Bunin, P., Gavrilenko, M., Golutvin, I., Gorbunov, I., Kamenev, A., Karjavin, V., Lanev, A., Malakhov, A., Matveev, V., Moisenz, P., Palichik, V., Perelygin, V., Shmatov, S., Shulha, S., Skatchkov, N., Smirnov, V., Voytishin, N., Zarubin, A., Ivanov, Y., Kim, V., Kuznetsova, E., Levchenko, P., Murzin, V., Oreshkin, V., Smirnov, I., Sosnov, D., Sulimov, V., Uvarov, L., Vavilov, S., Vorobyev, A., Andreev, Yu., Dermenev, A., Gninenko, S., Golubev, N., Karneyeu, A., Kirsanov, M., Krasnikov, N., Pashenkov, A., Tlisov, D., Toropin, A., Epshteyn, V., Gavrilov, V., Lychkovskaya, N., Popov, V., Pozdnyakov, I., Safronov, G., Spiridonov, A., Stepennov, A., Stolin, V., Toms, M., Vlasov, E., Zhokin, A., Aushev, T., Bylinkin, A., Andreev, V., Azarkin, M., Dremin, I., Kirakosyan, M., Rusakov, S. V., Terkulov, A., Baskakov, A., Belyaev, A., Boos, E., Ershov, A., Gribushin, A., Khein, L., Klyukhin, V., Kodolova, O., Lokhtin, I., Lukina, O., Miagkov, I., Obraztsov, S., Petrushanko, S., Savrin, V., Snigirev, A., Blinov, V., Shtol, D., Skovpen, Y., Azhgirey, I., Bayshev, I., Bitioukov, S., Elumakhov, D., Godizov, A., Kachanov, V., Kalinin, A., Konstantinov, D., Mandrik, P., Petrov, V., Ryutin, R., Sobol, A., Troshin, S., Tyurin, N., Uzunian, A., Volkov, A., Babaev, A., Adzic, P., Cirkovic, P., Devetak, D., Dordevic, M., Milosevic, J., Maestre, J. Alcaraz, Fernández, A. Álvarez, Bachiller, I., Luna, M. Barrio, Cerrada, M., Colino, N., De La Cruz, B., Peris, A. Delgado, Bedoya, C. Fernandez, Ramos, J.P. Fernández, Flix, J., Fouz, M. C., Lopez, O. Gonzalez, Lopez, S. Goy, Hernandez, J. M., Josa, M. I., Moran, D., Yzquierdo, A. Pérez-Calero, Pelayo, J. Puerta, Redondo, I., Romero, L., Soares, M. S., Triossi, A., Albajar, C., de Trocóniz, J. F., Cuevas, J., Erice, C., Menendez, J. Fernandez, Folgueras, S., Caballero, I. Gonzalez, Fernández, J. R. González, Cortezon, E. Palencia, Cruz, S. Sanchez, Vischia, P., Garcia, J.M. Vizan, Cabrillo, I. J., Calderon, A., Quero, B. Chazin, Campderros, J. Duarte, Fernandez, M., Manteca, P. J. Fernández, Alonso, A. García, Garcia-Ferrero, J., Gomez, G., Virto, A. Lopez, Marco, J., Rivero, C. Martinez, Arbol, P. Martinez Ruiz del, Matorras, F., Gomez, J. Piedra, Prieels, C., Rodrigo, T., Ruiz-Jimeno, A., Scodellaro, L., Trevisani, N., Vila, I., Cortabitarte, R. Vilar, Abbaneo, D., Akgun, B., Auffray, E., Baillon, P., Ball, A. H., Barney, D., Bendavid, J., Bianco, M., Bocci, A., Botta, C., Camporesi, T., Cepeda, M., Cerminara, G., Chapon, E., Chen, Y., d’Enterria, D., Dabrowski, A., Daponte, V., David, A., De Gruttola, M., De Roeck, A., Deelen, N., Dobson, M., Pree, T. du, Dünser, M., Dupont, N., Elliott-Peisert, A., Everaerts, P., Fallavollita, F., Franzoni, G., Fulcher, J., Funk, W., Gigi, D., Gilbert, A., Gill, K., Glege, F., Gulhan, D., Hegeman, J., Innocente, V., Jafari, A., Janot, P., Karacheban, O., Kieseler, J., Knünz, V., Kornmayer, A., Krammer, M., Lange, C., Lecoq, P., Lourenço, C., Lucchini, M.T., Malgeri, L., Mannelli, M., Martelli, A., Meijers, F., Merlin, J. A., Mersi, S., Meschi, E., Milenovic, P., Moortgat, F., Mulders, M., Neugebauer, H., Ngadiuba, J., Orfanelli, S., Orsini, L., Pantaleo, F., Pape, L., Perez, E., Peruzzi, M., Petrilli, A., Petrucciani, G., Pfeiffer, A., Pierini, M., Pitters, F. M., Rabady, D., Racz, A., Reis, T., Rolandi, G., Rovere, M., Sakulin, H., Schäfer, C., Schwick, C., Seidel, M., Selvaggi, M., Sharma, A., Silva, P., Sphicas, P., Stakia, A., Steggemann, J., Stoye, M., Tosi, M., Treille, D., Tsirou, A., Veckalns, V., Verweij, M., Zeuner, W. D., Bertl, W., Caminada, L., Deiters, K., Erdmann, W., Horisberger, R., Ingram, Q., Kaestli, H. C., Kotlinski, D., Langenegger, U., Rohe, T., Wiederkehr, S. A., Backhaus, M., Bäni, L., Berger, P., Casal, B., Chernyavskaya, N., Dissertori, G., Dittmar, M., Donegà, M., Dorfer, C., Grab, C., Heidegger, C., Hits, D., Hoss, J., Klijnsma, T., Lustermann, W., Marionneau, M., Meinhard, M. T., Meister, D., Micheli, F., Musella, P., Nessi-Tedaldi, F., Pata, J., Pauss, F., Perrin, G., Perrozzi, L., Quittnat, M., Reichmann, M., Ruini, D., Becerra, D. A. Sanz, Schönenberger, M., Shchutska, L., Tavolaro, V. R., Theofilatos, K., Olsson, M. L. Vesterbacka, Wallny, R., Zhu, D. H., Aarrestad, T. K., Amsler, C., Brzhechko, D., Canelli, M.F., De Cosa, A., Burgo, R. Del, Donato, S., Galloni, C., Hreus, T., Kilminster, B., Neutelings, I., Pinna, D., Rauco, G., Robmann, P., Salerno, D., Schweiger, K., Seitz, C., Takahashi, Y., Zucchetta, A., Candelise, V., Chang, Y. H., Cheng, K. y., Doan, T. H., Jain, Sh., Khurana, R., Kuo, C. M., Lin, W., Pozdnyakov, A., Yu, S. S., Chang, P., Chao, Y., Chen, K. F., Chen, P. H., Fiori, F., Hou, W.-S., Hsiung, Y., Kumar, Arun, Liu, Y. F., Lu, R.-S., Paganis, E., Psallidas, A., Steen, A., Tsai, J. f., Asavapibhop, B., Kovitanggoon, K., Singh, G., Srimanobhas, N., Bat, A., Boran, F., Cerci, S., Damarseckin, S., Demiroglu, Z.S., Dozen, C., Dumanoglu, I., Girgis, S., Gokbulut, G., Guler, Y., Hos, I., Kangal, E. E., Kara, O., Kiminsu, U., Oglakci, M., Onengut, G., Ozdemir, K., Cerci, D. Sunar, Tali, B., Tok, U. G., Topakli, H., Turkcapar, S., Zorbakir, I. S., Zorbilmez, C., Karapinar, G., Ocalan, K., Yalvac, M., Zeyrek, M., Atakisi, I. O., Gülmez, E., Kaya, M., Kaya, O., Tekten, S., Yetkin, E.A., Agaras, M. N., Atay, S., Cakir, A., Cankocak, K., Komurcu, Y., Grynyov, B., Levchuk, L., Ball, F., Beck, L., Brooke, J. J., Burns, D., Clement, E., Cussans, D., Davignon, O., Flacher, H., Goldstein, J., Heath, G. P., Heath, H.F., Kreczko, L., Newbold, D. M., Paramesvaran, S., Sakuma, T., Nasr-storey, S. Seif El, Smith, D., Smith, V. J., Bell, K. W., Belyaev, A., Brew, C., Brown, R. M., Cieri, D., Cockerill, D. J. A., Coughlan, J. A., Harder, K., Harper, S., Linacre, J., Olaiya, E., Petyt, D., Shepherd-Themistocleous, C. H., Thea, A., Tomalin, I. R., Williams, T., Womersley, W. J., Auzinger, G., Bainbridge, R., Bloch, P., Borg, J., Breeze, S., Buchmuller, O., Bundock, A., Casasso, S., Colling, D., Corpe, L., Dauncey, P., Davies, G., Negra, M. Della, Maria, R. Di, Haddad, Y., Hall, G., Iles, G., James, T., Komm, M., Lane, R., Laner, C., Lyons, L., Magnan, A.-M., Malik, S., Mastrolorenzo, L., Matsushita, T., Nash, J., Nikitenko, A., Palladino, V., Pesaresi, M., Richards, A., Rose, A., Scott, E., Seez, C., Shtipliyski, A., Strebler, T., Summers, S., Tapper, A., Uchida, K., Acosta, M. Vazquez, Virdee, T., Wardle, N., Winterbottom, D., Wright, J., Zenz, S.C., Cole, J. E., Hobson, P.R., Khan, A., Kyberd, P., Morton, A., Reid, I.D., Teodorescu, L., Zahid, S., Borzou, A., Call, K., Dittmann, J., Hatakeyama, K., Liu, H., Pastika, N., Smith, C., Bartek, R., Dominguez, A., Buccilli, A., Cooper, S. I., Henderson, C., Rumerio, P., West, C., Arcaro, D., Avetisyan, A., Bose, T., Gastler, D., Rankin, D., Richardson, C., Rohlf, J., Sulak, L., Zou, D., Benelli, G., Cutts, D., Hadley, M., Hakala, J., Heintz, U., Hogan, J.M., Kwok, K. H. M., Laird, E., Landsberg, G., Lee, J., Mao, Z., Narain, M., Pazzini, J., Piperov, S., Sagir, S., Syarif, R., Yu, D., Band, R., Brainerd, C., Breedon, R., Burns, D., De La Barca Sanchez, M. Calderon, Chertok, M., Conway, J., Conway, R., Cox, P. T., Erbacher, R., Flores, C., Funk, G., Ko, W., Lander, R., Mclean, C., Mulhearn, M., Pellett, D., Pilot, J., Shalhout, S., Shi, M., Smith, J., Stolp, D., Taylor, D., Tos, K., Tripathi, M., Wang, Z., Zhang, F., Bachtis, M., Bravo, C., Cousins, R., Dasgupta, A., Florent, A., Hauser, J., Ignatenko, M., Mccoll, N., Regnard, S., Saltzberg, D., Schnaible, C., Valuev, V., Bouvier, E., Burt, K., Clare, R., Ellison, J., Gary, J.W., Shirazi, S. M. A. Ghiasi, Hanson, G., Karapostoli, G., Kennedy, E., Lacroix, F., Long, O.R., Negrete, M. Olmedo, Paneva, M. I., Si, W., Wang, L., Wei, H., Wimpenny, S., Yates, B.R., Branson, J. G., Cittolin, S., Derdzinski, M., Gerosa, R., Gilbert, D., Hashemi, B., Holzner, A., Klein, D., Kole, G., Krutelyov, V., Letts, J., Masciovecchio, M., Olivito, D., Padhi, S., Pieri, M., Sani, M., Sharma, V., Simon, S., Tadel, M., Vartak, A., Wasserbaech, S., Wood, J., Würthwein, F., Yagil, A., Porta, G. Zevi Della, Amin, N., Bhandari, R., Bradmiller-Feld, J., Campagnari, C., Citron, M., Dishaw, A., Dutta, V., Sevilla, M. Franco, Gouskos, L., Heller, R., Incandela, J., Ovcharova, A., Qu, H., Richman, J., Stuart, D., Suarez, I., Yoo, J., Anderson, D., Bornheim, A., Bunn, J., Lawhorn, J.M., Newman, H.B., Nguyen, T. Q., Pena, C., Spiropulu, M., Vlimant, J. R., Wilkinson, R., Xie, S., Zhang, Z., Zhu, R.Y., Andrews, M. B., Ferguson, T., Mudholkar, T., Paulini, M., Russ, J., Sun, M., Vogel, H., Vorobiev, I., Weinberg, M., Cumalat, J. P., Ford, W.T., Jensen, F., Johnson, A., Krohn, M., Leontsinis, S., MacDonald, E., Mulholland, T., Stenson, K., Ulmer, K. A., Wagner, S. R., Alexander, J., Chaves, J., Cheng, Y., Chu, J., Datta, A., Mcdermott, K., Mirman, N., Patterson, J. R., Quach, D., Rinkevicius, A., Ryd, A., Skinnari, L., Soffi, L., Tan, S. M., Tao, Z., Thom, J., Tucker, J., Wittich, P., Zientek, M., Abdullin, S., Albrow, M., Alyari, M., Apollinari, G., Apresyan, A., Apyan, A., Banerjee, S., Bauerdick, L.A.T., Beretvas, A., Berryhill, J., Bhat, P. C., Bolla, G., Burkett, K., Butler, J. N., Canepa, A., Cerati, G. B., Cheung, H. W. K., Chlebana, F., Cremonesi, M., Duarte, J., Elvira, V.D., Freeman, J., Gecse, Z., Gottschalk, E., Gray, L., Green, D., Grünendahl, S., Gutsche, O., Hanlon, J., Harris, R.M., Hasegawa, S., Hirschauer, J., Hu, Z., Jayatilaka, B., Jindariani, S., Johnson, M., Joshi, U., Klima, B., Kortelainen, M. J., Kreis, B., Lammel, S., Lincoln, D., Lipton, R., Liu, M., Liu, T., De Sá, R. Lopes, Lykken, J., Maeshima, K., Magini, N., Marraffino, J. M., Mason, D., McBride, P., Merkel, P., Mrenna, S., Nahn, S., O’Dell, V., Pedro, K., Prokofyev, O., Rakness, G., Ristori, L., Savoy-Navarro, A., Schneider, B., Sexton-Kennedy, E., Soha, A., Spalding, W. J., Spiegel, L., Stoynev, S., Strait, J., Strobbe, N., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vernieri, C., Verzocchi, M., Vidal, R., Wang, M., Weber, H. A., Whitbeck, A., Wu, W., Acosta, D., Avery, P., Bortignon, P., Bourilkov, D., Brinkerhoff, A., Carnes, A., Carver, M., Curry, D., Field, R. D., Furic, I. K., Gleyzer, S. V., Joshi, B. M., Konigsberg, J., Korytov, A., Kotov, K., Ma, P., Matchev, K., Mei, H., Mitselmakher, G., Shi, K., Sperka, D., Terentyev, N., Thomas, L., Wang, J., Wang, S., Yelton, J., Joshi, Y. R., Linn, S., Markowitz, P., Rodriguez, J. L., Ackert, A., Adams, T., Askew, A., Hagopian, S., Hagopian, V., Johnson, K. F., Kolberg, T., Martinez, G., Perry, T., Prosper, H., Saha, A., Santra, A., Sharma, V., Yohay, R., Baarmand, M.M., Bhopatkar, V., Colafranceschi, S., Hohlmann, M., Noonan, D., Roy, T., Yumiceva, F., Adams, M. R., Apanasevich, L., Berry, D., Betts, R. R., Cavanaugh, R., Chen, X., Dittmer, S., Evdokimov, O., Gerber, C.E., Hangal, D. A., Hofman, D. J., Jung, K., Kamin, J., Gonzalez, I. D. Sandoval, Tonjes, M. B., Varelas, N., Wang, H., Wu, Z., Zhang, J., Bilki, B., Clarida, W., Dilsiz, K., Durgut, S., Gandrajula, R. P., Haytmyradov, M., Khristenko, V., Merlo, J.-P., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Ogul, H., Onel, Y., Ozok, F., Penzo, A., Snyder, C., Tiras, E., Wetzel, J., Yi, K., Blumenfeld, B., Cocoros, A., Eminizer, N., Fehling, D., Feng, L., Gritsan, A. V., Hung, W. T., Maksimovic, P., Roskes, J., Sarica, U., Swartz, M., Xiao, M., You, C., Al-bataineh, A., Baringer, P., Bean, A., Boren, S., Bowen, J., Castle, J., Khalil, S., Kropivnitskaya, A., Majumder, D., Mcbrayer, W., Murray, M., Rogan, C., Royon, C., Sanders, S., Schmitz, E., Takaki, J. D. Tapia, Wang, Q., Ivanov, A., Kaadze, K., Maravin, Y., Modak, A., Mohammadi, A., Saini, L. K., Skhirtladze, N., Rebassoo, F., Wright, D., Baden, A., Baron, O., Belloni, A., Eno, S.C., Feng, Y., Ferraioli, C., Hadley, N. J., Jabeen, S., Jeng, G.Y., Kellogg, R. G., Kunkle, J., Mignerey, A. C., Ricci-Tam, F., Shin, Y. H., Skuja, A., Tonwar, S. C., Abercrombie, D., Allen, B., Azzolini, V., Barbieri, R., Baty, A., Bauer, G., Bi, R., Brandt, S., Busza, W., Cali, I. A., D’Alfonso, M., Demiragli, Z., Ceballos, G. Gomez, Goncharov, M., Harris, P., Hsu, D., Hu, M., Iiyama, Y., Innocenti, G. M., Klute, M., Kovalskyi, D., Lee, Y.-J., Levin, A., Luckey, P. D., Maier, B., Marini, A.C., Mcginn, C., Mironov, C., Narayanan, S., Niu, X., Paus, C., Roland, C., Roland, G., Stephans, G. S. F., Sumorok, K., Tatar, K., Velicanu, D., Wang, J., Wang, T. W., Wyslouch, B., Zhaozhong, S., Benvenuti, A. C., Chatterjee, R. M., Evans, A., Hansen, P., Kalafut, S., Kubota, Y., Lesko, Z., Mans, J., Nourbakhsh, S., Ruckstuhl, N., Rusack, R., Turkewitz, J., Wadud, M. A., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Golf, F., Suarez, R. Gonzalez, Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Godshalk, A., Harrington, C., Iashvili, I., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Freer, C., Hortiangtham, A., Massironi, A., Morse, D.M., Orimoto, T., De Lima, R. Teixeira, Wamorkar, T., Wang, B., Wisecarver, A., Wood, D., Bhattacharya, S., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Schmitt, M.H., Sung, K., Trovato, M., Velasco, M., Bucci, R., Dev, N., Hildreth, M., Anampa, K. Hurtado, Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Li, W., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Siddireddy, P., Smith, G., Taroni, S., Wayne, M., Wightman, A., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Ling, T. Y., Luo, W., Winer, B. L., Wulsin, H. W., Cooperstein, S., Driga, O., Elmer, P., Hardenbrook, J., Hebda, P., Higginbotham, S., Kalogeropoulos, A., Lange, D., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Piroué, P., Salfeld-Nebgen, J., Stickland, D., Tully, C., Malik, S., Norberg, S., Barker, A., Barnes, V.E., Das, S., Gutay, L., Jones, M., Jung, A.W., Khatiwada, A., Miller, D. H., Neumeister, N., Peng, C. C., Qiu, H., Schulte, J. F., Sun, J., Wang, F., Xiao, R., Xie, W., Cheng, T., Dolen, J., Parashar, N., Chen, Z., Ecklund, K. M., Freed, S., Geurts, F.J.M., Guilbaud, M., Kilpatrick, M., Li, W., Michlin, B., Padley, B.P., Roberts, J., Rorie, J., Shi, W., Tu, Z., Zabel, J., Zhang, A., Bodek, A., de Barbaro, P., Demina, R., Duh, Y. t., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, P., Verzetti, M., Ciesielski, R., Goulianos, K., Mesropian, C., Agapitos, A., Chou, J. P., Gershtein, Y., Espinosa, T.A. Gómez, Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Delannoy, A. G., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Hernandez, A. Castaneda, Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Perniè, L., Rathjens, D., Safonov, A., Tatarinov, A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Faulkner, J., Gurpinar, E., Kunori, S., Lamichhane, K., Lee, S. W., Mengke, T., Muthumuni, S., Peltola, T., Undleeb, S., Volobouev, I., Wang, Z., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Padeken, K., Alvarez, J.D. Ruiz, Sheldon, P., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, P., Cox, B., Hirosky, R., Joyce, M., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Wang, Y., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Poudyal, N., Sturdy, J., Thapa, P., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Carlsmith, D., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Hervé, A., Hussain, U., Klabbers, P., Lanaro, A., Levine, A., Long, K., Loveless, R., Rekovic, V., Ruggles, T., Savin, A., Smith, N., Smith, W. H., and Woods, N.
Published: 2022
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27. Erratum to: Search for new physics in dijet angular distributions using proton-proton collisions at s=13TeV and constraints on dark matter and other models

Author: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Erö, J., Valle, A. Escalante Del, Flechl, M., Friedl, M., Frühwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., König, A., Krammer, N., Krätschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rad, N., Rohringer, H., Schieck, J., Schöfbeck, R., Spanring, M., Spitzbart, D., Taurok, A., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Croce, D. Di, Janssen, X., Lauwers, J., Pieters, M., De Klundert, M. Van, Haevermaet, H. Van, Mechelen, P. Van, Remortel, N. Van, Zeid, S. Abu, Blekman, F., D’Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Marchesini, I., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Doninck, W. Van, Mulders, P. Van, Parijs, I. Van, Beghin, D., Bilin, B., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Dorney, B., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Kalsi, A. K., Lenzi, T., Luetic, J., Seva, T., Starling, E., Velde, C. Vander, Vanlaer, P., Vannerom, D., Yonamine, R., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Trocino, D., Tytgat, M., Verbeke, W., Vermassen, B., Vit, M., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caputo, C., Caudron, A., David, P., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Saggio, A., Marono, M. Vidal, Wertz, S., Zobec, J., Júnior, W. L. Aldá, Alves, F. L., Alves, G. A., Brito, L., Silva, G. Correia, Hensel, C., Moraes, A., Pol, M. E., Teles, P. Rebello, Chagas, E. Belchior Batista Das, Carvalho, W., Chinellato, J., Coelho, E., Da Costa, E. M., Silveira, G. G. Da, De Jesus Damiao, D., De Souza, S. Fonseca, Malbouisson, H., Jaime, M. Medina, De Almeida, M. Melo, Herrera, C. Mora, Mundim, L., Nogima, H., Rosas, L. J. Sanchez, Santoro, A., Sznajder, A., Thiel, M., Manganote, E. J. Tonelli, Da Silva De Araujo, F. Torres, Pereira, A. Vilela, Ahuja, S., Bernardes, C. A., Calligaris, L., Tomei, T. R. Fernandez Perez, Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Abad, D. Romero, Vargas, J. C. Ruiz, Aleksandrov, A., Hadjiiska, R., Iaydjiev, P., Marinov, A., Misheva, M., Rodozov, M., Shopova, M., Sultanov, G., Dimitrov, A., Litov, L., Pavlov, B., Petkov, P., Fang, W., Gao, X., Yuan, L., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhao, J., Ban, Y., Chen, G., Li, J., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Wang, Y., Avila, C., Cabrera, A., Montoya, C. A. Carrillo, Sierra, L. F. Chaparro, Florez, C., Hernández, C. F. González, Delgado, M. A. Segura, Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Cipriano, P. M. Ribeiro, Sculac, T., Antunovic, Z., Kovac, M., Brigljevic, V., Ferencek, D., Kadija, K., Mesic, B., Starodumov, A., Susa, T., Ather, M. W., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Rykaczewski, H., Finger, M., Finger, Jr., M., Jarrin, E. Carrera, Assran, Y., Elgammal, S., Khalil, S., Bhowmik, S., Dewanjee, R. K., Kadastik, M., Perrini, L., Raidal, M., Veelken, C., Eerola, P., Kirschenmann, H., Pekkanen, J., Voutilainen, M., Havukainen, J., Heikkilä, J. K., Järvinen, T., Karimäki, V., Kinnunen, R., Lampén, T., Lassila-Perini, K., Laurila, S., Lehti, S., Lindén, T., Luukka, P., Mäenpää, T., Siikonen, H., Tuominen, E., Tuominiemi, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. L., Ferri, F., Ganjour, S., Ghosh, S., Givernaud, A., Gras, P., de Monchenault, G. Hamel, Jarry, P., Leloup, C., Locci, E., Machet, M., Malcles, J., Negro, G., Rander, J., Rosowsky, A., Sahin, M.Ö., Titov, M., Abdulsalam, A., Amendola, C., Antropov, I., Baffioni, S., Beaudette, F., Busson, P., Cadamuro, L., Charlot, C., de Cassagnac, R. Granier, Jo, M., Kucher, I., Lisniak, S., Lobanov, A., Blanco, J. Martin, Nguyen, M., Ochando, C., Ortona, G., Paganini, P., Pigard, P., Salerno, R., Sauvan, J. B., Sirois, Y., Leiton, A. G. Stahl, Yilmaz, Y., Zabi, A., Zghiche, A., Agram, J.-L., Andrea, J., Bloch, D., Brom, J.-M., Chabert, E. C., Collard, C., Conte, E., Coubez, X., Drouhin, F., Fontaine, J.-C., Gelé, D., Goerlach, U., Jansová, M., Juillot, P., Bihan, A.-C. Le, Tonon, N., Hove, P. Van, Gadrat, S., Beauceron, S., Bernet, C., Boudoul, G., Chanon, N., Chierici, R., Contardo, D., Depasse, P., Mamouni, H. El, Fay, J., Finco, L., Gascon, S., Gouzevitch, M., Grenier, G., Ille, B., Lagarde, F., Laktineh, I. B., Lattaud, H., Lethuillier, M., Mirabito, L., Pequegnot, A. L., Perries, S., Popov, A., Sordini, V., Donckt, M. Vander, Viret, S., Zhang, S., Toriashvili, T., Tsamalaidze, Z., Autermann, C., Feld, L., Kiesel, M. K., Klein, K., Lipinski, M., Preuten, M., Rauch, M. P., Schomakers, C., Schulz, J., Teroerde, M., Wittmer, B., Zhukov, V., Albert, A., Duchardt, D., Endres, M., Erdmann, M., Erdweg, S., Esch, T., Fischer, R., Güth, A., Hebbeker, T., Heidemann, C., Hoepfner, K., Knutzen, S., Merschmeyer, M., Meyer, A., Millet, P., Mukherjee, S., Pook, T., Radziej, M., Reithler, H., Rieger, M., Scheuch, F., Teyssier, D., Thüer, S., Flügge, G., Kargoll, B., Kress, T., Künsken, A., Müller, T., Nehrkorn, A., Nowack, A., Pistone, C., Pooth, O., Stahl, A., Martin, M. Aldaya, Arndt, T., Asawatangtrakuldee, C., Beernaert, K., Behnke, O., Behrens, U., Martínez, A. Bermúdez, Anuar, A. A. Bin, Borras, K., Botta, V., Campbell, A., Connor, P., Contreras-Campana, C., Costanza, F., Danilov, V., De Wit, A., Pardos, C. Diez, Damiani, D. Domínguez, Eckerlin, G., Eckstein, D., Eichhorn, T., Elwood, A., Eren, E., Gallo, E., Garcia, J. Garay, Geiser, A., Luyando, J. M. Grados, Grohsjean, A., Gunnellini, P., Guthoff, M., Harb, A., Hauk, J., Hempel, M., Jung, H., Kasemann, M., Keaveney, J., Kleinwort, C., Knolle, J., Korol, I., Krücker, D., Lange, W., Lelek, A., Lenz, T., Lipka, K., Lohmann, W., Mankel, R., Melzer-Pellmann, I.-A., Meyer, A. B., Meyer, M., Missiroli, M., Mittag, G., Mnich, J., Mussgiller, A., Pitzl, D., Raspereza, A., Savitskyi, M., Saxena, P., Shevchenko, R., Stefaniuk, N., Tholen, H., Onsem, G. P. Van, Walsh, R., Wen, Y., Wichmann, K., Wissing, C., Zenaiev, O., Aggleton, R., Bein, S., Blobel, V., Vignali, M. Centis, Dreyer, T., Garutti, E., Gonzalez, D., Haller, J., Hinzmann, A., Hoffmann, M., Karavdina, A., Kasieczka, G., Klanner, R., Kogler, R., Kovalchuk, N., Kurz, S., Kutzner, V., Lange, J., Marconi, D., Multhaup, J., Niedziela, M., Nowatschin, D., Peiffer, T., Perieanu, A., Reimers, A., Scharf, C., Schleper, P., Schmidt, A., Schumann, S., Schwandt, J., Sonneveld, J., Stadie, H., Steinbrück, G., Stober, F. M., Stöver, M., Troendle, D., Usai, E., Vanhoefer, A., Vormwald, B., Akbiyik, M., Barth, C., Baselga, M., Baur, S., Butz, E., Caspart, R., Chwalek, T., Colombo, F., De Boer, W., Dierlamm, A., Faltermann, N., Freund, B., Friese, R., Giffels, M., Harrendorf, M. A., Hartmann, F., Heindl, S. M., Husemann, U., Kassel, F., Kudella, S., Mildner, H., Mozer, M. U., Müller, Th., Plagge, M., Quast, G., Rabbertz, K., Schröder, M., Shvetsov, I., Sieber, G., Simonis, H. J., Ulrich, R., Wayand, S., Weber, M., Weiler, T., Williamson, S., Wöhrmann, C., Wolf, R., Anagnostou, G., Daskalakis, G., Geralis, T., Kyriakis, A., Loukas, D., Topsis-Giotis, I., Karathanasis, G., Kesisoglou, S., Panagiotou, A., Saoulidou, N., Tziaferi, E., Kousouris, K., Papakrivopoulos, I., Evangelou, I., Foudas, C., Gianneios, P., Katsoulis, P., Kokkas, P., Mallios, S., Manthos, N., Papadopoulos, I., Paradas, E., Strologas, J., Triantis, F. A., Tsitsonis, D., Csanad, M., Filipovic, N., Pasztor, G., Surányi, O., Veres, G. I., Bencze, G., Hajdu, C., Horvath, D., Hunyadi, Á., Sikler, F., Vámi, T.Á., Veszpremi, V., Vesztergombi, G., Beni, N., Czellar, S., Karancsi, J., Makovec, A., Molnar, J., Szillasi, Z., Bartók, M., Raics, P., Trocsanyi, Z. L., Ujvari, B., Choudhury, S., Komaragiri, J. R., Bahinipati, S., Mal, P., Mandal, K., Nayak, A., Sahoo, D. K., Swain, S. K., Bansal, S., Beri, S. B., Bhatnagar, V., Chauhan, S., Chawla, R., Dhingra, N., Gupta, R., Kaur, A., Kaur, M., Kaur, S., Kumar, R., Kumari, P., Lohan, M., Mehta, A., Sharma, S., Singh, J. B., Walia, G., Bhardwaj, A., Choudhary, B. C., Garg, R. B., Keshri, S., Kumar, A., Kumar, Ashok, Malhotra, S., Naimuddin, M., Ranjan, K., Shah, Aashaq, Sharma, R., Bhardwaj, R., Bhattacharya, R., Bhattacharya, S., Bhawandeep, U., Bhowmik, D., Dey, S., Dutt, S., Dutta, S., Ghosh, S., Majumdar, N., Mondal, K., Mukhopadhyay, S., Nandan, S., Purohit, A., Rout, P. K., Roy, A., Chowdhury, S. Roy, Sarkar, S., Sharan, M., Singh, B., Thakur, S., Behera, P. K., Chudasama, R., Dutta, D., Jha, V., Kumar, V., Mohanty, A. K., Netrakanti, P. K., Pant, L. M., Shukla, P., Topkar, A., Aziz, T., Dugad, S., Mahakud, B., Mitra, S., Mohanty, G. B., Sur, N., Sutar, B., Banerjee, S., Bhattacharya, S., Chatterjee, S., Das, P., Guchait, M., Jain, Sa., Kumar, S., Maity, M., Majumder, G., Mazumdar, K., Sahoo, N., Sarkar, T., Wickramage, N., Chauhan, S., Dube, S., Hegde, V., Kapoor, A., Kothekar, K., Pandey, S., Rane, A., Sharma, S., Chenarani, S., Tadavani, E. Eskandari, Etesami, S. M., Khakzad, M., Najafabadi, M. Mohammadi, Naseri, M., Mehdiabadi, S. Paktinat, Hosseinabadi, F. Rezaei, Safarzadeh, B., Zeinali, M., Felcini, M., Grunewald, M., Abbrescia, M., Calabria, C., Colaleo, A., Creanza, D., Cristella, L., De Filippis, N., De Palma, M., Florio, A. Di, Errico, F., Fiore, L., Gelmi, A., Iaselli, G., Lezki, S., Maggi, G., Maggi, M., Marangelli, B., Miniello, G., My, S., Nuzzo, S., Pompili, A., Pugliese, G., Radogna, R., Ranieri, A., Selvaggi, G., Sharma, A., Silvestris, L., Venditti, R., Verwilligen, P., Zito, G., Abbiendi, G., Battilana, C., Bonacorsi, D., Borgonovi, L., Braibant-Giacomelli, S., Brigliadori, L., Campanini, R., Capiluppi, P., Castro, A., Cavallo, F. R., Chhibra, S. S., Codispoti, G., Cuffiani, M., Dallavalle, G. M., Fabbri, F., Fanfani, A., Fasanella, D., Giacomelli, P., Grandi, C., Guiducci, L., Marcellini, S., Masetti, G., Montanari, A., Navarria, F. L., Perrotta, A., Rossi, A. M., Rovelli, T., Siroli, G. P., Tosi, N., Albergo, S., Costa, S., Mattia, A. Di, Giordano, F., Potenza, R., Tricomi, A., Tuve, C., Barbagli, G., Chatterjee, K., Ciulli, V., Civinini, C., D’Alessandro, R., Focardi, E., Latino, G., Lenzi, P., Meschini, M., Paoletti, S., Russo, L., Sguazzoni, G., Strom, D., Viliani, L., Benussi, L., Bianco, S., Fabbri, F., Piccolo, D., Primavera, F., Calvelli, V., Ferro, F., Ravera, F., Robutti, E., Tosi, S., Benaglia, A., Beschi, A., Brianza, L., Brivio, F., Ciriolo, V., Dinardo, M. E., Fiorendi, S., Gennai, S., Ghezzi, A., Govoni, P., Malberti, M., Malvezzi, S., Manzoni, R. A., Menasce, D., Moroni, L., Paganoni, M., Pauwels, K., Pedrini, D., Pigazzini, S., Ragazzi, S., de Fatis, T. Tabarelli, Buontempo, S., Cavallo, N., Guida, S. Di, Fabozzi, F., Fienga, F., Galati, G., Iorio, A. O. M., Khan, W. A., Lista, L., Meola, S., Paolucci, P., Sciacca, C., Thyssen, F., Voevodina, E., Azzi, P., Bacchetta, N., Benato, L., Bisello, D., Boletti, A., Carlin, R., De Oliveira, A. Carvalho Antunes, Checchia, P., De Castro Manzano, P., Dorigo, T., Dosselli, U., Gasparini, F., Gasparini, U., Gozzelino, A., Lacaprara, S., Margoni, M., Meneguzzo, A. T., Pozzobon, N., Ronchese, P., Rossin, R., Simonetto, F., Tiko, A., Torassa, E., Zanetti, M., Zotto, P., Zumerle, G., Braghieri, A., Magnani, A., Montagna, P., Ratti, S. P., Re, V., Ressegotti, M., Riccardi, C., Salvini, P., Vai, I., Vitulo, P., Solestizi, L. Alunni, Biasini, M., Bilei, G. M., Cecchi, C., Ciangottini, D., Fanò, L., Lariccia, P., Leonardi, R., Manoni, E., Mantovani, G., Mariani, V., Menichelli, M., Rossi, A., Santocchia, A., Spiga, D., Androsov, K., Azzurri, P., Bagliesi, G., Bianchini, L., Boccali, T., Borrello, L., Castaldi, R., Ciocci, M. A., Dell’Orso, R., Fedi, G., Giannini, L., Giassi, A., Grippo, M. T., Ligabue, F., Lomtadze, T., Manca, E., Mandorli, G., Messineo, A., Palla, F., Rizzi, A., Spagnolo, P., Tenchini, R., Tonelli, G., Venturi, A., Verdini, P. G., Barone, L., Cavallari, F., Cipriani, M., Daci, N., Re, D. Del, Marco, E. Di, Diemoz, M., Gelli, S., Longo, E., Marzocchi, B., Meridiani, P., Organtini, G., Pandolfi, F., Paramatti, R., Preiato, F., Rahatlou, S., Rovelli, C., Santanastasio, F., Amapane, N., Arcidiacono, R., Argiro, S., Arneodo, M., Bartosik, N., Bellan, R., Biino, C., Cartiglia, N., Castello, R., Cenna, F., Costa, M., Covarelli, R., Degano, A., Demaria, N., Kiani, B., Mariotti, C., Maselli, S., Migliore, E., Monaco, V., Monteil, E., Monteno, M., Obertino, M. M., Pacher, L., Pastrone, N., Pelliccioni, M., Angioni, G. L. Pinna, Romero, A., Ruspa, M., Sacchi, R., Shchelina, K., Sola, V., Solano, A., Staiano, A., Belforte, S., Casarsa, M., Cossutti, F., Ricca, G. Della, Zanetti, A., Kim, D. H., Kim, G. N., Kim, M. S., Lee, J., Lee, S., Lee, S. W., Moon, C. S., Oh, Y. D., Sekmen, S., Son, D. C., Yang, Y. C., Kim, H., Moon, D. H., Oh, G., Cifuentes, J. A. Brochero, Goh, J., Kim, T. J., Cho, S., Choi, S., Go, Y., Gyun, D., Ha, S., Hong, B., Jo, Y., Kim, Y., Lee, K., Lee, K. S., Lee, S., Lim, J., Park, S. K., Roh, Y., Almond, J., Kim, J., Kim, J. S., Lee, H., Lee, K., Nam, K., Oh, S. B., Radburn-Smith, B. C., Seo, S.h., Yang, U. K., Yoo, H. D., Yu, G. B., Kim, H., Kim, J. H., Lee, J. S. H., Park, I. C., Choi, Y., Hwang, C., Lee, J., Yu, I., Dudenas, V., Juodagalvis, A., Vaitkus, J., Ahmed, I., Ibrahim, Z. A., Ali, M. A. B. Md, Idris, F. Mohamad, Abdullah, W. A. T. Wan, Yusli, M. N., Zolkapli, Z., Duran-Osuna, M. C., Castilla-Valdez, H., De La Cruz-Burelo, E., Ramirez-Sanchez, G., Cruz, I. Heredia-De La, Rabadan-Trejo, R. I., Lopez-Fernandez, R., Guisao, J. Mejia, Reyes-Almanza, R, Sanchez-Hernandez, A., Moreno, S. Carrillo, Barrera, C. Oropeza, Valencia, F. Vazquez, Eysermans, J., Pedraza, I., Ibarguen, H. A. Salazar, Estrada, C. Uribe, Pineda, A. Morelos, Krofcheck, D., Bheesette, S., Butler, P. H., Ahmad, A., Ahmad, M., Hassan, Q., Hoorani, H. R., Saddique, A., Shah, M. A., Shoaib, M., Waqas, M., Bialkowska, H., Bluj, M., Boimska, B., Frueboes, T., Górski, M., Kazana, M., Nawrocki, K., Szleper, M., Traczyk, P., Zalewski, P., Bunkowski, K., Byszuk, A., Doroba, K., Kalinowski, A., Konecki, M., Krolikowski, J., Misiura, M., Olszewski, M., Pyskir, A., Walczak, M., Bargassa, P., Da Cruz E Silva, C. Beirão, Francesco, A. Di, Faccioli, P., Galinhas, B., Gallinaro, M., Hollar, J., Leonardo, N., Iglesias, L. Lloret, Nemallapudi, M. V., Seixas, J., Strong, G., Toldaiev, O., Vadruccio, D., Varela, J., Afanasiev, S., Bunin, P., Gavrilenko, M., Golutvin, I., Gorbunov, I., Kamenev, A., Karjavin, V., Lanev, A., Malakhov, A., Matveev, V., Moisenz, P., Palichik, V., Perelygin, V., Shmatov, S., Shulha, S., Skatchkov, N., Smirnov, V., Voytishin, N., Zarubin, A., Ivanov, Y., Kim, V., Kuznetsova, E., Levchenko, P., Murzin, V., Oreshkin, V., Smirnov, I., Sosnov, D., Sulimov, V., Uvarov, L., Vavilov, S., Vorobyev, A., Andreev, Yu., Dermenev, A., Gninenko, S., Golubev, N., Karneyeu, A., Kirsanov, M., Krasnikov, N., Pashenkov, A., Tlisov, D., Toropin, A., Epshteyn, V., Gavrilov, V., Lychkovskaya, N., Popov, V., Pozdnyakov, I., Safronov, G., Spiridonov, A., Stepennov, A., Stolin, V., Toms, M., Vlasov, E., Zhokin, A., Aushev, T., Bylinkin, A., Chistov, R., Danilov, M., Parygin, P., Philippov, D., Polikarpov, S., Tarkovskii, E., Andreev, V., Azarkin, M., Dremin, I., Kirakosyan, M., Rusakov, S. V., Terkulov, A., Baskakov, A., Belyaev, A., Boos, E., Dubinin, M., Dudko, L., Ershov, A., Gribushin, A., Klyukhin, V., Kodolova, O., Lokhtin, I., Miagkov, I., Obraztsov, S., Petrushanko, S., Savrin, V., Snigirev, A., Blinov, V., Shtol, D., Skovpen, Y., Azhgirey, I., Bayshev, I., Bitioukov, S., Elumakhov, D., Godizov, A., Kachanov, V., Kalinin, A., Konstantinov, D., Mandrik, P., Petrov, V., Ryutin, R., Sobol, A., Troshin, S., Tyurin, N., Uzunian, A., Volkov, A., Babaev, A., Adzic, P., Cirkovic, P., Devetak, D., Dordevic, M., Milosevic, J., Maestre, J. Alcaraz, Fernández, A. Álvarez, Bachiller, I., Luna, M. Barrio, Cerrada, M., Colino, N., De La Cruz, B., Peris, A. Delgado, Bedoya, C. Fernandez, Ramos, J. P. Fernández, Flix, J., Fouz, M. C., Lopez, O. Gonzalez, Lopez, S. Goy, Hernandez, J. M., Josa, M. I., Moran, D., Yzquierdo, A. Pérez-Calero, Pelayo, J. Puerta, Redondo, I., Romero, L., Soares, M. S., Triossi, A., Albajar, C., de Trocóniz, J. F., Cuevas, J., Erice, C., Menendez, J. Fernandez, Folgueras, S., Caballero, I. Gonzalez, Fernández, J. R. González, Cortezon, E. Palencia, Cruz, S. Sanchez, Vischia, P., Garcia, J. M. Vizan, Cabrillo, I. J., Calderon, A., Quero, B. Chazin, Campderros, J. Duarte, Fernandez, M., Manteca, P. J. Fernández, Alonso, A. García, Garcia-Ferrero, J., Gomez, G., Virto, A. Lopez, Marco, J., Rivero, C. Martinez, Arbol, P. Martinez Ruiz del, Matorras, F., Gomez, J. Piedra, Prieels, C., Rodrigo, T., Ruiz-Jimeno, A., Scodellaro, L., Trevisani, N., Vila, I., Cortabitarte, R. Vilar, Abbaneo, D., Akgun, B., Auffray, E., Baillon, P., Ball, A. H., Barney, D., Bendavid, J., Bianco, M., Bocci, A., Botta, C., Camporesi, T., Cepeda, M., Cerminara, G., Chapon, E., Chen, Y., d’Enterria, D., Dabrowski, A., Daponte, V., David, A., De Gruttola, M., De Roeck, A., Deelen, N., Dobson, M., Pree, T. du, Dünser, M., Dupont, N., Elliott-Peisert, A., Everaerts, P., Fallavollita, F., Franzoni, G., Fulcher, J., Funk, W., Gigi, D., Gilbert, A., Gill, K., Glege, F., Gulhan, D., Hegeman, J., Innocente, V., Jafari, A., Janot, P., Karacheban, O., Kieseler, J., Knünz, V., Kornmayer, A., Krammer, M., Lange, C., Lecoq, P., Lourenço, C., Lucchini, M. T., Malgeri, L., Mannelli, M., Martelli, A., Meijers, F., Merlin, J. A., Mersi, S., Meschi, E., Milenovic, P., Moortgat, F., Mulders, M., Neugebauer, H., Ngadiuba, J., Orfanelli, S., Orsini, L., Pantaleo, F., Pape, L., Perez, E., Peruzzi, M., Petrilli, A., Petrucciani, G., Pfeiffer, A., Pierini, M., Pitters, F. M., Rabady, D., Racz, A., Reis, T., Rolandi, G., Rovere, M., Sakulin, H., Schäfer, C., Schwick, C., Seidel, M., Selvaggi, M., Sharma, A., Silva, P., Sphicas, P., Stakia, A., Steggemann, J., Stoye, M., Tosi, M., Treille, D., Tsirou, A., Veckalns, V., Verweij, M., Zeuner, W. D., Bertl, W., Caminada, L., Deiters, K., Erdmann, W., Horisberger, R., Ingram, Q., Kaestli, H. C., Kotlinski, D., Langenegger, U., Rohe, T., Wiederkehr, S. A., Backhaus, M., Bäni, L., Berger, P., Casal, B., Chernyavskaya, N., Dissertori, G., Dittmar, M., Donegà, M., Dorfer, C., Grab, C., Heidegger, C., Hits, D., Hoss, J., Klijnsma, T., Lustermann, W., Marionneau, M., Meinhard, M. T., Meister, D., Micheli, F., Musella, P., Nessi-Tedaldi, F., Pata, J., Pauss, F., Perrin, G., Perrozzi, L., Quittnat, M., Reichmann, M., Ruini, D., Becerra, D. A. Sanz, Schönenberger, M., Shchutska, L., Tavolaro, V. R., Theofilatos, K., Olsson, M. L. Vesterbacka, Wallny, R., Zhu, D. H., Aarrestad, T. K., Amsler, C., Brzhechko, D., Canelli, M. F., De Cosa, A., Burgo, R. Del, Donato, S., Galloni, C., Hreus, T., Kilminster, B., Neutelings, I., Pinna, D., Rauco, G., Robmann, P., Salerno, D., Schweiger, K., Seitz, C., Takahashi, Y., Zucchetta, A., Candelise, V., Chang, Y. H., Cheng, K. y., Doan, T. H., Jain, Sh., Khurana, R., Kuo, C. M., Lin, W., Pozdnyakov, A., Yu, S. S., Chang, P., Chao, Y., Chen, K. F., Chen, P. H., Fiori, F., Hou, W.-S., Hsiung, Y., Kumar, Arun, Liu, Y. F., Lu, R.-S., Paganis, E., Psallidas, A., Steen, A., Tsai, J. f., Asavapibhop, B., Kovitanggoon, K., Singh, G., Srimanobhas, N., Bat, A., Boran, F., Cerci, S., Damarseckin, S., Demiroglu, Z. S., Dozen, C., Dumanoglu, I., Girgis, S., Gokbulut, G., Guler, Y., Hos, I., Kangal, E. E., Kara, O., Topaksu, A. Kayis, Kiminsu, U., Oglakci, M., Onengut, G., Ozdemir, K., Cerci, D. Sunar, Tok, U. G., Topakli, H., Turkcapar, S., Zorbakir, I. S., Zorbilmez, C., Karapinar, G., Ocalan, K., Yalvac, M., Zeyrek, M., Atakisi, I. O., Gülmez, E., Kaya, M., Kaya, O., Tekten, S., Yetkin, E. A., Agaras, M. N., Atay, S., Cakir, A., Cankocak, K., Komurcu, Y., Grynyov, B., Levchuk, L., Ball, F., Beck, L., Brooke, J. J., Burns, D., Clement, E., Cussans, D., Davignon, O., Flacher, H., Goldstein, J., Heath, G. P., Heath, H. F., Kreczko, L., Newbold, D. M., Paramesvaran, S., Sakuma, T., Nasr-storey, S. Seif El, Smith, D., Smith, V. J., Bell, K. W., Belyaev, A., Brew, C., Brown, R. M., Cieri, D., Cockerill, D. J. A., Coughlan, J. A., Harder, K., Harper, S., Linacre, J., Olaiya, E., Petyt, D., Shepherd-Themistocleous, C. H., Thea, A., Tomalin, I. R., Williams, T., Womersley, W. J., Auzinger, G., Bainbridge, R., Bloch, P., Borg, J., Breeze, S., Buchmuller, O., Bundock, A., Casasso, S., Colling, D., Corpe, L., Dauncey, P., Davies, G., Negra, M. Della, Maria, R. Di, Haddad, Y., Hall, G., Iles, G., James, T., Komm, M., Lane, R., Laner, C., Lyons, L., Magnan, A.-M., Malik, S., Mastrolorenzo, L., Matsushita, T., Nash, J., Nikitenko, A., Palladino, V., Pesaresi, M., Richards, A., Rose, A., Scott, E., Seez, C., Shtipliyski, A., Strebler, T., Summers, S., Tapper, A., Uchida, K., Acosta, M. Vazquez, Virdee, T., Wardle, N., Winterbottom, D., Wright, J., Zenz, S. C., Cole, J. E., Hobson, P. R., Khan, A., Kyberd, P., Morton, A., Reid, I. D., Teodorescu, L., Zahid, S., Borzou, A., Call, K., Dittmann, J., Hatakeyama, K., Liu, H., Pastika, N., Smith, C., Bartek, R., Dominguez, A., Buccilli, A., Cooper, S. I., Henderson, C., Rumerio, P., West, C., Arcaro, D., Avetisyan, A., Bose, T., Gastler, D., Rankin, D., Richardson, C., Rohlf, J., Sulak, L., Zou, D., Benelli, G., Cutts, D., Hadley, M., Hakala, J., Heintz, U., Hogan, J. M., Kwok, K. H. M., Laird, E., Landsberg, G., Lee, J., Mao, Z., Narain, M., Pazzini, J., Piperov, S., Sagir, S., Syarif, R., Yu, D., Band, R., Brainerd, C., Breedon, R., Burns, D., De La Barca Sanchez, M. Calderon, Chertok, M., Conway, J., Conway, R., Cox, P. T., Erbacher, R., Flores, C., Funk, G., Ko, W., Lander, R., Mclean, C., Mulhearn, M., Pellett, D., Pilot, J., Shalhout, S., Shi, M., Smith, J., Stolp, D., Taylor, D., Tos, K., Tripathi, M., Wang, Z., Zhang, F., Bachtis, M., Bravo, C., Cousins, R., Dasgupta, A., Florent, A., Hauser, J., Ignatenko, M., Mccoll, N., Regnard, S., Saltzberg, D., Schnaible, C., Valuev, V., Bouvier, E., Burt, K., Clare, R., Ellison, J., Gary, J. W., Shirazi, S. M. A. Ghiasi, Hanson, G., Karapostoli, G., Kennedy, E., Lacroix, F., Long, O. R., Negrete, M. Olmedo, Paneva, M. I., Si, W., Wang, L., Wei, H., Wimpenny, S., Yates, B. R., Branson, J. G., Cittolin, S., Derdzinski, M., Gerosa, R., Gilbert, D., Hashemi, B., Holzner, A., Klein, D., Kole, G., Krutelyov, V., Letts, J., Masciovecchio, M., Olivito, D., Padhi, S., Pieri, M., Sani, M., Sharma, V., Simon, S., Tadel, M., Vartak, A., Wasserbaech, S., Wood, J., Würthwein, F., Yagil, A., Porta, G. Zevi Della, Amin, N., Bhandari, R., Bradmiller-Feld, J., Campagnari, C., Citron, M., Dishaw, A., Dutta, V., Sevilla, M. Franco, Gouskos, L., Heller, R., Incandela, J., Ovcharova, A., Qu, H., Richman, J., Stuart, D., Suarez, I., Yoo, J., Anderson, D., Bornheim, A., Bunn, J., Lawhorn, J. M., Newman, H. B., Nguyen, T. Q., Pena, C., Spiropulu, M., Vlimant, J. R., Wilkinson, R., Xie, S., Zhang, Z., Zhu, R. Y., Andrews, M. B., Ferguson, T., Mudholkar, T., Paulini, M., Russ, J., Sun, M., Vogel, H., Vorobiev, I., Weinberg, M., Cumalat, J. P., Ford, W. T., Jensen, F., Johnson, A., Krohn, M., Leontsinis, S., MacDonald, E., Mulholland, T., Stenson, K., Ulmer, K. A., Wagner, S. R., Alexander, J., Chaves, J., Cheng, Y., Chu, J., Datta, A., Mcdermott, K., Mirman, N., Patterson, J. R., Quach, D., Rinkevicius, A., Ryd, A., Skinnari, L., Soffi, L., Tan, S. M., Tao, Z., Thom, J., Tucker, J., Wittich, P., Zientek, M., Abdullin, S., Albrow, M., Alyari, M., Apollinari, G., Apresyan, A., Apyan, A., Banerjee, S., Bauerdick, L. A. T., Beretvas, A., Berryhill, J., Bhat, P. C., Bolla, G., Burkett, K., Butler, J. N., Canepa, A., Cerati, G. B., Cheung, H. W. K., Chlebana, F., Cremonesi, M., Duarte, J., Elvira, V. D., Freeman, J., Gecse, Z., Gottschalk, E., Gray, L., Green, D., Grünendahl, S., Gutsche, O., Hanlon, J., Harris, R. M., Hasegawa, S., Hirschauer, J., Hu, Z., Jayatilaka, B., Jindariani, S., Johnson, M., Joshi, U., Klima, B., Kortelainen, M. J., Kreis, B., Lammel, S., Lincoln, D., Lipton, R., Liu, M., Liu, T., De Sá, R. Lopes, Lykken, J., Maeshima, K., Magini, N., Marraffino, J. M., Mason, D., McBride, P., Merkel, P., Mrenna, S., Nahn, S., O’Dell, V., Pedro, K., Prokofyev, O., Rakness, G., Ristori, L., Savoy-Navarro, A., Schneider, B., Sexton-Kennedy, E., Soha, A., Spalding, W. J., Spiegel, L., Stoynev, S., Strait, J., Strobbe, N., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vernieri, C., Verzocchi, M., Vidal, R., Wang, M., Weber, H. A., Whitbeck, A., Wu, W., Acosta, D., Avery, P., Bortignon, P., Bourilkov, D., Brinkerhoff, A., Carnes, A., Carver, M., Curry, D., Field, R. D., Furic, I. K., Gleyzer, S. V., Joshi, B. M., Konigsberg, J., Korytov, A., Kotov, K., Ma, P., Matchev, K., Mei, H., Mitselmakher, G., Shi, K., Sperka, D., Terentyev, N., Thomas, L., Wang, J., Wang, S., Yelton, J., Joshi, Y. R., Linn, S., Markowitz, P., Rodriguez, J. L., Ackert, A., Adams, T., Askew, A., Hagopian, S., Hagopian, V., Johnson, K. F., Kolberg, T., Martinez, G., Perry, T., Prosper, H., Saha, A., Santra, A., Sharma, V., Yohay, R., Baarmand, M. M., Bhopatkar, V., Colafranceschi, S., Hohlmann, M., Noonan, D., Roy, T., Yumiceva, F., Adams, M. R., Apanasevich, L., Berry, D., Betts, R. R., Cavanaugh, R., Chen, X., Dittmer, S., Evdokimov, O., Gerber, C. E., Hangal, D. A., Hofman, D. J., Jung, K., Kamin, J., Gonzalez, I. D. Sandoval, Tonjes, M. B., Varelas, N., Wang, H., Wu, Z., Zhang, J., Bilki, B., Clarida, W., Dilsiz, K., Durgut, S., Gandrajula, R. P., Haytmyradov, M., Khristenko, V., Merlo, J.-P., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Ogul, H., Onel, Y., Ozok, F., Penzo, A., Snyder, C., Tiras, E., Wetzel, J., Yi, K., Blumenfeld, B., Cocoros, A., Eminizer, N., Fehling, D., Feng, L., Gritsan, A. V., Hung, W. T., Maksimovic, P., Roskes, J., Sarica, U., Swartz, M., Xiao, M., You, C., Al-bataineh, A., Baringer, P., Bean, A., Boren, S., Bowen, J., Castle, J., Khalil, S., Kropivnitskaya, A., Majumder, D., Mcbrayer, W., Murray, M., Rogan, C., Royon, C., Sanders, S., Schmitz, E., Takaki, J. D. Tapia, Wang, Q., Ivanov, A., Kaadze, K., Maravin, Y., Modak, A., Mohammadi, A., Saini, L. K., Skhirtladze, N., Rebassoo, F., Wright, D., Baden, A., Baron, O., Belloni, A., Eno, S. C., Feng, Y., Ferraioli, C., Hadley, N. J., Jabeen, S., Jeng, G. Y., Kellogg, R. G., Kunkle, J., Mignerey, A. C., Ricci-Tam, F., Shin, Y. H., Skuja, A., Tonwar, S. C., Abercrombie, D., Allen, B., Azzolini, V., Barbieri, R., Baty, A., Bauer, G., Bi, R., Brandt, S., Busza, W., Cali, I. A., D’Alfonso, M., Demiragli, Z., Ceballos, G. Gomez, Goncharov, M., Harris, P., Hsu, D., Hu, M., Iiyama, Y., Innocenti, G. M., Klute, M., Kovalskyi, D., Lee, Y.-J., Levin, A., Luckey, P. D., Maier, B., Marini, A. C., Mcginn, C., Mironov, C., Narayanan, S., Niu, X., Paus, C., Roland, C., Roland, G., Stephans, G. S. F., Sumorok, K., Tatar, K., Velicanu, D., Wang, J., Wang, T. W., Wyslouch, B., Zhaozhong, S., Benvenuti, A. C., Chatterjee, R. M., Evans, A., Hansen, P., Kalafut, S., Kubota, Y., Lesko, Z., Mans, J., Nourbakhsh, S., Ruckstuhl, N., Rusack, R., Turkewitz, J., Wadud, M. A., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Golf, F., Suarez, R. Gonzalez, Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Godshalk, A., Harrington, C., Iashvili, I., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Freer, C., Hortiangtham, A., Massironi, A., Morse, D. M., Orimoto, T., De Lima, R. Teixeira, Wamorkar, T., Wang, B., Wisecarver, A., Wood, D., Bhattacharya, S., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Schmitt, M. H., Sung, K., Trovato, M., Velasco, M., Bucci, R., Dev, N., Hildreth, M., Anampa, K. Hurtado, Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Li, W., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Siddireddy, P., Smith, G., Taroni, S., Wayne, M., Wightman, A., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Ling, T. Y., Luo, W., Winer, B. L., Wulsin, H. W., Cooperstein, S., Driga, O., Elmer, P., Hardenbrook, J., Hebda, P., Higginbotham, S., Kalogeropoulos, A., Lange, D., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Piroué, P., Salfeld-Nebgen, J., Stickland, D., Tully, C., Malik, S., Norberg, S., Barker, A., Barnes, V. E., Das, S., Gutay, L., Jones, M., Jung, A. W., Khatiwada, A., Miller, D. H., Neumeister, N., Peng, C. C., Qiu, H., Schulte, J. F., Sun, J., Wang, F., Xiao, R., Xie, W., Cheng, T., Dolen, J., Parashar, N., Chen, Z., Ecklund, K. M., Freed, S., Geurts, F. J. M., Guilbaud, M., Kilpatrick, M., Li, W., Michlin, B., Padley, B. P., Roberts, J., Rorie, J., Shi, W., Tu, Z., Zabel, J., Zhang, A., Bodek, A., de Barbaro, P., Demina, R., Duh, Y. t., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, P., Verzetti, M., Ciesielski, R., Goulianos, K., Mesropian, C., Agapitos, A., Chou, J. P., Gershtein, Y., Espinosa, T. A. Gómez, Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Delannoy, A. G., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Hernandez, A. Castaneda, Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Perniè, L., Rathjens, D., Safonov, A., Tatarinov, A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Faulkner, J., Gurpinar, E., Kunori, S., Lamichhane, K., Lee, S. W., Mengke, T., Muthumuni, S., Peltola, T., Undleeb, S., Volobouev, I., Wang, Z., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Padeken, K., Alvarez, J. D. Ruiz, Sheldon, P., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, P., Cox, B., Hirosky, R., Joyce, M., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Wang, Y., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Poudyal, N., Sturdy, J., Thapa, P., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Carlsmith, D., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Hervé, A., Hussain, U., Klabbers, P., Lanaro, A., Levine, A., Long, K., Loveless, R., Rekovic, V., Ruggles, T., Savin, A., Smith, N., Smith, W. H., and Woods, N.
Published: 2022
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28. Some properties of convection in hybrid stars

Author: Yudin, A. V., Hempel, M., Nadyozhin, D. K., and Razinkova, T. L.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Nuclear Theory
Abstract: It is shown that the unusual thermodynamic properties of matter within the region of two-phase coexistence in hybrid stars result in a change of the standard condition for beginning of convection. In particular, the thermal flux transported by convection may be directed towards the stellar center. We discuss favorable circumstances leading to such an effect of "inverse convection" and its possible influence on the thermal evolution of hybrid stars., Comment: 13 pages, 3 figures. The discussion is extended according to referees suggestions. New references added. Accepted to MNRAS
Published: 2015
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29. Hundreds of new cluster candidates in the VISTA variables in the Via Lactea survey DR1

Author: Barba, R. H., Roman-Lopes, A., Castellon, J. L. Nilo, Firpo, V., Minniti, D., Lucas, P., Emerson, J. P., Hempel, M., Soto, M., and Saito, R. K.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: VISTA variables in the Via Lactea is an ESO Public survey dedicated to scan the bulge and an adjacent portion of the Galactic disk in the fourth quadrant using the VISTA telescope and the near-infrared camera VIRCAM. One of the leading goals of the VVV survey is to contribute to the knowledge of the star cluster population of the Milky Way. To improve the census of the Galactic star clusters, we performed a systematic scan of the JHKs images of the Galactic plane section of the VVV survey. Our detection procedure is based on a combination of superficial density maps and visual inspection of promising features in the NIR images. The material examined are color-composite images corresponding to the DR1 of VVV. We report the discovery of 493 new star cluster candidates. The analysis of the spatial distribution show that the clusters are very concentrated in he Galactic plane, presenting some local maxima around the position of large star-forming complexes, such as G305, RCW 95, and RCW 106. The vast majority of the cluster candidates are quite compact and generally surrounded by bright and/or dark nebulosities. IRAS point sources are associated with 59% of the sample, while 88% are associated with MSX point sources. GLIMPSE 8 mum images of the cluster candidates show a variety of morphologies, with 292 clusters dominated by knotty sources, while 361 clusters show some kind of nebulosity. Spatial cross-correlation with young stellar objects, masers, and extended green-object catalogs suggest that a large sample of the new cluster candidates are extremely young. In particular, 104 star clusters associated to methanol masers are excellent candidates for ongoing massive star formation. Also, there is a special set of sixteen cluster candidates that present clear signspot of star-forming activity having associated simultaneosly dark nebulae, young stellar objects, EGOs, and masers., Comment: 13 pages, 8 figures, 3 tables. Accepted in Astronomy and Astrophysics. The full catalog and charts available at http://astro.userena.cl/science/lsclusters.php
Published: 2015
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30. Investigation of a direction sensitive sapphire detector stack at the 5 GeV electron beam at DESY-II

Author: Karacheban, O., Afanaciev, K., Hempel, M., Henschel, H., Lange, W., Leonard, J. L., Levy, I., Lohmann, W., and Schuwalow, S.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: Extremely radiation hard sensors are needed in particle physics experiments to instrument the region near the beam pipe. Examples are beam halo and beam loss monitors at the Large Hadron Collider, FLASH or XFEL. Currently artificial diamond sensors are widely used. In this paper single crystal sapphire sensors are considered as a promising alternative. Industrially grown sapphire wafers are available in large sizes, are of low cost and, like diamond sensors, can be operated without cooling. Here we present results of an irradiation study done with sapphire sensors in a high intensity low energy electron beam. Then, a multichannel direction-sensitive sapphire detector stack is described. It comprises 8 sapphire plates of 1 cm^2 size and 525 micro m thickness, metallized on both sides, and apposed to form a stack. Each second metal layer is supplied with a bias voltage, and the layers in between are connected to charge-sensitive preamplifiers. The performance of the detector was studied in a 5 GeV electron beam. The charge collection efficiency measured as a function of the bias voltage rises with the voltage, reaching about 10 % at 950 V. The signal size obtained from electrons crossing the stack at this voltage is about 22000 e, where e is the unit charge. The signal size is measured as a function of the hit position, showing variations of up to 20 % in the direction perpendicular to the beam and to the electric field. The measurement of the signal size as a function of the coordinate parallel to the electric field confirms the prediction that mainly electrons contribute to the signal. Also evidence for the presence of a polarisation field was observed., Comment: 13 pages, 7 figures, 3 tables
Published: 2015
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31. Pushing 1D CCSNe to explosions: model and SN 1987A

Author: Perego, A., Hempel, M., Fröhlich, C., Ebinger, K., Eichler, M., Casanova, J., Liebendoerfer, M., and Thielemann, F. -K.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: We report on a method, PUSH, for triggering core-collapse supernova explosions of massive stars in spherical symmetry. We explore basic explosion properties and calibrate PUSH such that the observables of SN1987A are reproduced. Our simulations are based on the general relativistic hydrodynamics code AGILE combined with the detailed neutrino transport scheme IDSA for electron neutrinos and ALS for the muon and tau neutrinos. To trigger explosions in the otherwise non-exploding simulations, we rely on the neutrino-driven mechanism. The PUSH method locally increases the energy deposition in the gain region through energy deposition by the heavy neutrino flavors. Our setup allows us to model the explosion for several seconds after core bounce. We explore the progenitor range 18-21M$_{\odot}$. Our studies reveal a distinction between high compactness (HC) and low compactness (LC) progenitor models, where LC models tend to explore earlier, with a lower explosion energy, and with a lower remnant mass. HC models are needed to obtain explosion energies around 1 Bethe, as observed for SN1987A. However, all the models with sufficiently high explosion energy overproduce $^{56}$Ni. We conclude that fallback is needed to reproduce the observed nucleosynthesis yields. The nucleosynthesis yields of $^{57-58}$Ni depend sensitively on the electron fraction and on the location of the mass cut with respect to the initial shell structure of the progenitor star. We identify a progenitor and a suitable set of PUSH parameters that fit the explosion properties of SN1987A when assuming 0.1M$_{\odot}$ of fallback. We predict a neutron star with a gravitational mass of 1.50M$_{\odot}$. We find correlations between explosion properties and the compactness of the progenitor model in the explored progenitors. However, a more complete analysis will require the exploration of a larger set of progenitors with PUSH., Comment: revised version as accepted by ApJ (results unchanged, text modified for clarification, a few references added); 26 pages, 20 figures
Published: 2015
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32. An Updated Census of RR~Lyrae Stars in the Globular Cluster $\omega$~Centauri (NGC\,5139)

Author: Navarrete, C., Ramos, R. Contreras, Catelan, M., Clement, C. M., Gran, F., Alonso-García, J., Angeloni, R., Hempel, M., Dékány, I., and Minniti, D.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: [ABRIDGED] $\omega$ Centauri (NGC 5139) contains large numbers of variable stars of different types and, in particular, more than a hundred RR Lyrae stars. We have conducted a variability survey of $\omega$ Cen in the NIR, using ESO's 4.1m Visible and Infrared Survey Telescope for Astronomy (VISTA). This is the first paper of a series describing our results. $\omega$ Cen was observed using VIRCAM mounted on VISTA. A total of 42 and 100 epochs in $J$ and $K_{\rm S}$, respectively, were obtained, distributed over a total timespan of 352 days. PSF photometry was performed, and periods of the known variable stars were improved when necessary using an ANOVA analysis. An unprecedented homogeneous and complete NIR catalogue of RR Lyrae stars in the field of $\omega$ Cen was collected, allowing us to study, for the first time, all the RR Lyrae stars associated to the cluster, except 4 located far away from the cluster center. Membership status, subclassifications between RRab and RRc subtypes, periods, amplitudes, and mean magnitudes were derived for all the stars in our sample. Additionally, 4 new RR Lyrae stars were discovered, 2 of them with high probability of being cluster members. The distribution of $\omega$ Cen stars in the Bailey (period-amplitude) diagram is also discussed. Reference lines in this plane, for both Oosterhoff type I (OoI) and II (OoII) components, are provided. In the present paper, we clarify the status of many (candidate) RR Lyrae stars that had been unclear in previous studies. This includes stars with anomalous positions in the color-magnitude diagram, uncertain periods or/and variability types, and possible field interlopers. We conclude that $\omega$ Cen hosts a total of 88 RRab and 101 RRc stars, for a grand total of 189 likely members. We confirm that most RRab stars in the cluster belong to an OoII component, as previously found using visual data., Comment: A\&A, in press
Published: 2015
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33. Discovery of a Pair of Classical Cepheids in an Invisible Cluster Beyond the Galactic Bulge

Author: Dékány, I., Minniti, D., Hajdu, G., Alonso-García, J., Hempel, M., Palma, T., Catelan, M., Gieren, W., and Majaess, D.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: We report the discovery of a pair of extremely reddened classical Cepheid variable stars located in the Galactic plane behind the bulge, using near-infrared time-series photometry from the VVV Survey. This is the first time that such objects have ever been found in the opposite side of the Galactic plane. The Cepheids have almost identical periods, apparent brightnesses and colors. From the near-infrared Leavitt law, we determine their distances with ~1.5% precision and ~8% accuracy. We find that they have a same total extinction of A(V)~32 mag, and are located at the same heliocentric distance of =11.4+/-0.9 kpc, and less than 1 pc from the true Galactic plane. Their similar periods indicate that the Cepheids are also coeval, with an age of ~48+/-3 Myr, according to theoretical models. They are separated by an angular distance of only 18.3", corresponding to a projected separation of ~1 pc. Their position coincides with the expected location of the Far 3 kpc Arm behind the bulge. Such a tight pair of similar classical Cepheids indicates the presence of an underlying young open cluster, that is both hidden behind heavy extinction and disguised by the dense stellar field of the bulge. All our attempts to directly detect this "invisible cluster" have failed, and deeper observations are needed., Comment: Accepted for publication in ApJL. Photometric data are available online at the CDS and also at http://www.astro.puc.cl/~idekany/pub/twincep.dat
Published: 2014
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34. Observation of the rare $B^0_s\to\mu^+\mu^-$ decay from the combined analysis of CMS and LHCb data

Author: CMS, The, Collaborations, LHCb, Khachatryan, V., Sirunyan, A. M., Tumasyan, A., Adam, W., Bergauer, T., Dragicevic, M., Erö, J., Friedl, M., Frühwirth, R., Ghete, V. M., Hartl, C., Hörmann, N., Hrubec, J., Jeitler, M., Kiesenhofer, W., Knünz, V., Krammer, M., Krätschmer, I., Liko, D., Mikulec, I., Rabady, D., Rahbaran, B., Rohringer, H., Schöfbeck, R., Strauss, J., Treberer-Treberspurg, W., Waltenberger, W., Wulz, C. -E., Mossolov, V., Shumeiko, N., Gonzalez, J. Suarez, Alderweireldt, S., Bansal, S., Cornelis, T., De Wolf, E. A., Janssen, X., Knutsson, A., Lauwers, J., Luyckx, S., Ochesanu, S., Rougny, R., Van De Klundert, M., Van Haevermaet, H., Van Mechelen, P., Van Remortel, N., Van Spilbeeck, A., Blekman, F., Blyweert, S., D'Hondt, J., Daci, N., Heracleous, N., Keaveney, J., Lowette, S., Maes, M., Olbrechts, A., Python, Q., Strom, D., Tavernier, S., Van Doninck, W., Van Mulders, P., Van Onsem, G. P., Villella, I., Caillol, C., Clerbaux, B., De Lentdecker, G., Dobur, D., Favart, L., Gay, A. P. R., Grebenyuk, A., Léonard, A., Mohammadi, A., Perniè, L., Randle-conde, A., Reis, T., Seva, T., Thomas, L., Velde, C. Vander, Vanlaer, P., Wang, J., Zenoni, F., Adler, V., Beernaert, K., Benucci, L., Cimmino, A., Costantini, S., Crucy, S., Dildick, S., Fagot, A., Garcia, G., Mccartin, J., Rios, A. A. Ocampo, Ryckbosch, D., Diblen, S. Salva, Sigamani, M., Strobbe, N., Thyssen, F., Tytgat, M., Yazgan, E., Zaganidis, N., Basegmez, S., Beluffi, C., Bruno, G., Castello, R., Caudron, A., Ceard, L., Da Silveira, G. G., Delaere, C., Pree, T. du, Favart, D., Forthomme, L., Giammanco, A., Hollar, J., Jafari, A., Jez, P., Komm, M., Lemaitre, V., Nuttens, C., Pagano, D., Perrini, L., Pin, A., Piotrzkowski, K., Popov, A., Quertenmont, L., Selvaggi, M., Marono, M. Vidal, Garcia, J. M. Vizan, Beliy, N., Caebergs, T., Daubie, E., Hammad, G. H., Júnior, W. L. Aldá, Alves, G. A., Brito, L., Junior, M. Correa Martins, Martins, T. Dos Reis, Herrera, C. Mora, Pol, M. E., Teles, P. Rebello, Carvalho, W., Chinellato, J., Custódio, A., Da Costa, E. M., Damiao, D. De Jesus, Martins, C. De Oliveira, De Souza, S. Fonseca, Malbouisson, H., Figueiredo, D. Matos, Mundim, L., Nogima, H., Da Silva, W. L. Prado, Santaolalla, J., Santoro, A., Sznajder, A., Manganote, E. J. Tonelli, Pereira, A. Vilela, Bernardes, C. A., Dogra, S., Tomei, T. R. Fernandez Perez, Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Aleksandrov, A., Genchev, V., Hadjiiska, R., Iaydjiev, P., Marinov, A., Piperov, S., Rodozov, M., Sultanov, G., Vutova, M., Dimitrov, A., Glushkov, I., Litov, L., Pavlov, B., Petkov, P., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Cheng, T., Du, R., Jiang, C. H., Plestina, R., Romeo, F., Tao, J., Wang, Z., Asawatangtrakuldee, C., Ban, Y., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Zou, W., Avila, C., Cabrera, A., Sierra, L. F. Chaparro, Florez, C., Gomez, J. P., Moreno, B. Gomez, Sanabria, J. C., Godinovic, N., Lelas, D., Polic, D., Puljak, I., Antunovic, Z., Kovac, M., Brigljevic, V., Kadija, K., Luetic, J., Mekterovic, D., Sudic, L., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Bodlak, M., Finger, M., Finger Jr., M., Assran, Y., Kamel, A. Ellithi, Mahmoud, M. A., Radi, A., Kadastik, M., Murumaa, M., Raidal, M., Tiko, A., Eerola, P., Fedi, G., Voutilainen, M., Härkönen, J., Karimäki, V., Kinnunen, R., Kortelainen, M. J., Lampén, T., Lassila-Perini, K., Lehti, S., Lindén, T., Luukka, P., Mäenpää, T., Peltola, T., Tuominen, E., Tuominiemi, J., Tuovinen, E., Wendland, L., Talvitie, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Fabbro, B., Faure, J. L., Favaro, C., Ferri, F., Ganjour, S., Givernaud, A., Gras, P., de Monchenault, G. Hamel, Jarry, P., Locci, E., Malcles, J., Rander, J., Rosowsky, A., Titov, M., Baffioni, S., Beaudette, F., Busson, P., Charlot, C., Dahms, T., Dalchenko, M., Dobrzynski, L., Filipovic, N., Florent, A., de Cassagnac, R. Granier, Mastrolorenzo, L., Miné, P., Mironov, C., Naranjo, I. N., Nguyen, M., Ochando, C., Ortona, G., Paganini, P., Regnard, S., Salerno, R., Sauvan, J. B., Sirois, Y., Veelken, C., Yilmaz, Y., Zabi, A., Agram, J. -L., Andrea, J., Aubin, A., Bloch, D., Brom, J. -M., Chabert, E. C., Collard, C., Conte, E., Fontaine, J. -C., Gelé, D., Goerlach, U., Goetzmann, C., Bihan, A. -C. Le, Skovpen, K., Van Hove, P., Gadrat, S., Beauceron, S., Beaupere, N., Boudoul, G., Bouvier, E., Brochet, S., Montoya, C. A. Carrillo, Chasserat, J., Chierici, R., Contardo, D., Depasse, P., Mamouni, H. El, Fan, J., Fay, J., Gascon, S., Gouzevitch, M., Ille, B., Kurca, T., Lethuillier, M., Mirabito, L., Perries, S., Alvarez, J. D. Ruiz, Sabes, D., Sgandurra, L., Sordini, V., Donckt, M. Vander, Verdier, P., Viret, S., Xiao, H., Tsamalaidze, Z., Autermann, C., Beranek, S., Bontenackels, M., Edelhoff, M., Feld, L., Heister, A., Hindrichs, O., Klein, K., Ostapchuk, A., Raupach, F., Sammet, J., Schael, S., Schulte, J. F., Weber, H., Wittmer, B., Zhukov, V., Ata, M., Brodski, M., Dietz-Laursonn, E., Duchardt, D., Erdmann, M., Fischer, R., Güth, A., Hebbeker, T., Heidemann, C., Hoepfner, K., Klingebiel, D., Knutzen, S., Kreuzer, P., Merschmeyer, M., Meyer, A., Millet, P., Olschewski, M., Padeken, K., Papacz, P., Reithler, H., Schmitz, S. A., Sonnenschein, L., Teyssier, D., Thüer, S., Weber, M., Cherepanov, V., Erdogan, Y., Flügge, G., Geenen, H., Geisler, M., Ahmad, W. Haj, Hoehle, F., Kargoll, B., Kress, T., Kuessel, Y., Künsken, A., Lingemann, J., Nowack, A., Nugent, I. M., Pooth, O., Stahl, A., Martin, M. Aldaya, Asin, I., Bartosik, N., Behr, J., Behrens, U., Bell, A. J., Bethani, A., Borras, K., Burgmeier, A., Cakir, A., Calligaris, L., Campbell, A., Choudhury, S., Costanza, F., Pardos, C. Diez, Dolinska, G., Dooling, S., Dorland, T., Eckerlin, G., Eckstein, D., Eichhorn, T., Flucke, G., Garcia, J. Garay, Geiser, A., Gunnellini, P., Hauk, J., Hempel, M., Jung, H., Kalogeropoulos, A., Kasemann, M., Katsas, P., Kieseler, J., Kleinwort, C., Korol, I., Krücker, D., Lange, W., Leonard, J., Lipka, K., Lobanov, A., Lohmann, W., Lutz, B., Mankel, R., Marfin, I., Melzer-Pellmann, I. -A., Meyer, A. B., Mittag, G., Mnich, J., Mussgiller, A., Naumann-Emme, S., Nayak, A., Ntomari, E., Perrey, H., Pitzl, D., Placakyte, R., Raspereza, A., Cipriano, P. M. Ribeiro, Roland, B., Ron, E., Sahin, M. Ö., Salfeld-Nebgen, J., Saxena, P., Schoerner-Sadenius, T., Schröder, M., Seitz, C., Spannagel, S., Trevino, A. D. R. Vargas, Walsh, R., Wissing, C., Blobel, V., Vignali, M. Centis, Draeger, A. R., Erfle, J., Garutti, E., Goebel, K., Görner, M., Haller, J., Hoffmann, M., Höing, R. S., Junkes, A., Kirschenmann, H., Klanner, R., Kogler, R., Lange, J., Lapsien, T., Lenz, T., Marchesini, I., Ott, J., Peiffer, T., Perieanu, A., Pietsch, N., Poehlsen, J., Poehlsen, T., Rathjens, D., Sander, C., Schettler, H., Schleper, P., Schlieckau, E., Schmidt, A., Seidel, M., Sola, V., Stadie, H., Steinbrück, G., Troendle, D., Usai, E., Vanelderen, L., Vanhoefer, A., Barth, C., Baus, C., Berger, J., Böser, C., Butz, E., Chwalek, T., De Boer, W., Descroix, A., Dierlamm, A., Feindt, M., Frensch, F., Giffels, M., Gilbert, A., Hartmann, F., Hauth, T., Husemann, U., Katkov, I., Kornmayer, A., Kuznetsova, E., Pardo, P. Lobelle, Mozer, M. U., Müller, T., Müller, Th., Nürnberg, A., Quast, G., Rabbertz, K., Röcker, S., Simonis, H. J., Stober, F. M., Ulrich, R., Wagner-Kuhr, J., Wayand, S., Weiler, T., Wolf, R., Anagnostou, G., Daskalakis, G., Geralis, T., Giakoumopoulou, V. A., Kyriakis, A., Loukas, D., Markou, A., Markou, C., Psallidas, A., Topsis-Giotis, I., Agapitos, A., Kesisoglou, S., Panagiotou, A., Saoulidou, N., Stiliaris, E., Aslanoglou, X., Evangelou, I., Flouris, G., Foudas, C., Kokkas, P., Manthos, N., Papadopoulos, I., Paradas, E., Strologas, J., Bencze, G., Hajdu, C., Hidas, P., Horvath, D., Sikler, F., Veszpremi, V., Vesztergombi, G., Zsigmond, A. J., Beni, N., Czellar, S., Karancsi, J., Molnar, J., Palinkas, J., Szillasi, Z., Makovec, A., Raics, P., Trocsanyi, Z. L., Ujvari, B., Sahoo, N., Swain, S. K., Beri, S. B., Bhatnagar, V., Gupta, R., Bhawandeep, U., Kalsi, A. K., Kaur, M., Kumar, R., Mittal, M., Nishu, N., Singh, J. B., Kumar, Ashok, Kumar, Arun, Ahuja, S., Bhardwaj, A., Choudhary, B. C., Kumar, A., Malhotra, S., Naimuddin, M., Ranjan, K., Sharma, V., Banerjee, S., Bhattacharya, S., Chatterjee, K., Dutta, S., Gomber, B., Jain, Sa., Jain, Sh., Khurana, R., Modak, A., Mukherjee, S., Roy, D., Sarkar, S., Sharan, M., Abdulsalam, A., Dutta, D., Kailas, S., Kumar, V., Mohanty, A. K., Pant, L. M., Shukla, P., Topkar, A., Aziz, T., Bhowmik, S., Chatterjee, R. M., Dewanjee, R. K., Dugad, S., Ganguly, S., Ghosh, S., Guchait, M., Gurtu, A., Kole, G., Kumar, S., Maity, M., Majumder, G., Mazumdar, K., Mohanty, G. B., Parida, B., Sudhakar, K., Wickramage, N., Bakhshiansohi, H., Behnamian, H., Etesami, S. M., Fahim, A., Goldouzian, R., Khakzad, M., Najafabadi, M. Mohammadi, Naseri, M., Mehdiabadi, S. Paktinat, Hosseinabadi, F. Rezaei, Safarzadeh, B., Zeinali, M., Felcini, M., Grunewald, M., Abbrescia, M., Calabria, C., Chhibra, S. S., Colaleo, A., Creanza, D., De Filippis, N., De Palma, M., Fiore, L., Iaselli, G., Maggi, G., Maggi, M., My, S., Nuzzo, S., Pompili, A., Pugliese, G., Radogna, R., Selvaggi, G., Sharma, A., Silvestris, L., Venditti, R., Verwilligen, P., Abbiendi, G., Benvenuti, A. C., Bonacorsi, D., Braibant-Giacomelli, S., Brigliadori, L., Campanini, R., Capiluppi, P., Castro, A., Cavallo, F. R., Codispoti, G., Cuffiani, M., Dallavalle, G. M., Fabbri, F., Fanfani, A., Fasanella, D., Giacomelli, P., Grandi, C., Guiducci, L., Marcellini, S., Masetti, G., Montanari, A., Navarria, F. L., Perrotta, A., Primavera, F., Rossi, A. M., Rovelli, T., Siroli, G. P., Tosi, N., Travaglini, R., Albergo, S., Cappello, G., Chiorboli, M., Costa, S., Giordano, F., Potenza, R., Tricomi, A., Tuve, C., Barbagli, G., Ciulli, V., Civinini, C., D'Alessandro, R., Focardi, E., Gallo, E., Gonzi, S., Gori, V., Lenzi, P., Meschini, M., Paoletti, S., Sguazzoni, G., Tropiano, A., Benussi, L., Bianco, S., Piccolo, D., Ferretti, R., Ferro, F., Vetere, M. Lo, Robutti, E., Tosi, S., Dinardo, M. E., Fiorendi, S., Gennai, S., Gerosa, R., Ghezzi, A., Govoni, P., Lucchini, M. T., Malvezzi, S., Manzoni, R. A., Martelli, A., Marzocchi, B., Menasce, D., Moroni, L., Paganoni, M., Pedrini, D., Ragazzi, S., Redaelli, N., de Fatis, T. Tabarelli, Buontempo, S., Cavallo, N., Di Guida, S., Fabozzi, F., Iorio, A. O. M., Lista, L., Meola, S., Merola, M., Paolucci, P., Azzi, P., Bacchetta, N., Bisello, D., Branca, A., Carlin, R., Checchia, P., Dall'Osso, M., Dorigo, T., Dosselli, U., Galanti, M., Gasparini, F., Gasparini, U., Giubilato, P., Gozzelino, A., Kanishchev, K., Lacaprara, S., Margoni, M., Meneguzzo, A. T., Pazzini, J., Pozzobon, N., Ronchese, P., Simonetto, F., Torassa, E., Tosi, M., Zotto, P., Zucchetta, A., Zumerle, G., Gabusi, M., Ratti, S. P., Re, V., Riccardi, C., Salvini, P., Vitulo, P., Biasini, M., Bilei, G. M., Ciangottini, D., Fanò, L., Lariccia, P., Mantovani, G., Menichelli, M., Saha, A., Santocchia, A., Spiezia, A., Androsov, K., Azzurri, P., Bagliesi, G., Bernardini, J., Boccali, T., Broccolo, G., Castaldi, R., Ciocci, M. A., Dell'Orso, R., Donato, S., Fiori, F., Foà, L., Giassi, A., Grippo, M. T., Ligabue, F., Lomtadze, T., Martini, L., Messineo, A., Moon, C. S., Palla, F., Rizzi, A., Savoy-Navarro, A., Serban, A. T., Spagnolo, P., Squillacioti, P., Tenchini, R., Tonelli, G., Venturi, A., Verdini, P. G., Vernieri, C., Barone, L., Cavallari, F., D'imperio, G., Del Re, D., Diemoz, M., Jorda, C., Longo, E., Margaroli, F., Meridiani, P., Micheli, F., Nourbakhsh, S., Organtini, G., Paramatti, R., Rahatlou, S., Rovelli, C., Santanastasio, F., Soffi, L., Traczyk, P., Amapane, N., Arcidiacono, R., Argiro, S., Arneodo, M., Bellan, R., Biino, C., Cartiglia, N., Casasso, S., Costa, M., Degano, A., Demaria, N., Finco, L., Mariotti, C., Maselli, S., Migliore, E., Monaco, V., Musich, M., Obertino, M. M., Pacher, L., Pastrone, N., Pelliccioni, M., Angioni, G. L. Pinna, Potenza, A., Romero, A., Ruspa, M., Sacchi, R., Solano, A., Staiano, A., Tamponi, U., Belforte, S., Candelise, V., Casarsa, M., Cossutti, F., Della Ricca, G., Gobbo, B., La Licata, C., Marone, M., Schizzi, A., Umer, T., Zanetti, A., Chang, S., Kropivnitskaya, A., Nam, S. K., Kim, D. H., Kim, G. N., Kim, M. S., Kong, D. J., Lee, S., Oh, Y. D., Park, H., Sakharov, A., Son, D. C., Kim, T. J., Kim, J. Y., Song, S., Choi, S., Gyun, D., Hong, B., Jo, M., Kim, H., Kim, Y., Lee, B., Lee, K. S., Park, S. K., Roh, Y., Yoo, H. D., Choi, M., Kim, J. H., Park, I. C., Ryu, G., Ryu, M. S., Choi, Y., Choi, Y. K., Goh, J., Kim, D., Kwon, E., Lee, J., Yu, I., Juodagalvis, A., Komaragiri, J. R., Ali, M. A. B. Md, Linares, E. Casimiro, Castilla-Valdez, H., De La Cruz-Burelo, E., La Cruz, I. Heredia-de, Hernandez-Almada, A., Lopez-Fernandez, R., Sanchez-Hernandez, A., Moreno, S. Carrillo, Valencia, F. Vazquez, Pedraza, I., Ibarguen, H. A. Salazar, Pineda, A. Morelos, Krofcheck, D., Butler, P. H., Reucroft, S., Ahmad, A., Ahmad, M., Hassan, Q., Hoorani, H. R., Khan, W. A., Khurshid, T., Shoaib, M., Bialkowska, H., Bluj, M., Boimska, B., Frueboes, T., Górski, M., Kazana, M., Nawrocki, K., Romanowska-Rybinska, K., Szleper, M., Zalewski, P., Brona, G., Bunkowski, K., Cwiok, M., Dominik, W., Doroba, K., Kalinowski, A., Konecki, M., Krolikowski, J., Misiura, M., Olszewski, M., Wolszczak, W., Bargassa, P., Silva, C. Beirão Da Cruz E, Faccioli, P., Parracho, P. G. Ferreira, Gallinaro, M., Iglesias, L. Lloret, Nguyen, F., Antunes, J. Rodrigues, Seixas, J., Varela, J., Vischia, P., Afanasiev, S., Bunin, P., Gavrilenko, M., Golutvin, I., Gorbunov, I., Kamenev, A., Karjavin, V., Konoplyanikov, V., Lanev, A., Malakhov, A., Matveev, V., Moisenz, P., Palichik, V., Perelygin, V., Shmatov, S., Skatchkov, N., Smirnov, V., Zarubin, A., Golovtsov, V., Ivanov, Y., Kim, V., Levchenko, P., Murzin, V., Oreshkin, V., Smirnov, I., Sulimov, V., Uvarov, L., Vavilov, S., Vorobyev, A., Vorobyev, An., Andreev, Yu., Dermenev, A., Gninenko, S., Golubev, N., Kirsanov, M., Krasnikov, N., Pashenkov, A., Tlisov, D., Toropin, A., Epshteyn, V., Gavrilov, V., Lychkovskaya, N., Popov, V., Pozdnyakov, I., Safronov, G., Semenov, S., Spiridonov, A., Stolin, V., Vlasov, E., Zhokin, A., Andreev, V., Azarkin, M., Dremin, I., Kirakosyan, M., Leonidov, A., Mesyats, G., Rusakov, S. V., Vinogradov, A., Belyaev, A., Boos, E., Dubinin, M., Dudko, L., Ershov, A., Gribushin, A., Klyukhin, V., Kodolova, O., Lokhtin, I., Obraztsov, S., Petrushanko, S., Savrin, V., Snigirev, A., Azhgirey, I., Bayshev, I., Bitioukov, S., Kachanov, V., Kalinin, A., Konstantinov, D., Krychkine, V., Petrov, V., Ryutin, R., Sobol, A., Tourtchanovitch, L., Troshin, S., Tyurin, N., Uzunian, A., Volkov, A., Adzic, P., Ekmedzic, M., Milosevic, J., Rekovic, V., Maestre, J. Alcaraz, Battilana, C., Calvo, E., Cerrada, M., Llatas, M. Chamizo, Colino, N., De La Cruz, B., Peris, A. Delgado, Vázquez, D. Domínguez, Del Valle, A. Escalante, Bedoya, C. Fernandez, Ramos, J. P. Fernández, Flix, J., Fouz, M. C., Garcia-Abia, P., Lopez, O. Gonzalez, Lopez, S. Goy, Hernandez, J. M., Josa, M. I., De Martino, E. Navarro, Yzquierdo, A. Pérez-Calero, Pelayo, J. Puerta, Olmeda, A. Quintario, Redondo, I., Romero, L., Soares, M. S., Albajar, C., de Trocóniz, J. F., Missiroli, M., Moran, D., Brun, H., Cuevas, J., Menendez, J. Fernandez, Folgueras, S., Caballero, I. Gonzalez, Cifuentes, J. A. Brochero, Cabrillo, I. J., Calderon, A., Campderros, J. Duarte, Fernandez, M., Gomez, G., Graziano, A., Virto, A. Lopez, Marco, J., Marco, R., Rivero, C. Martinez, Matorras, F., Sanchez, F. J. Munoz, Gomez, J. Piedra, Rodrigo, T., Rodríguez-Marrero, A. Y., Ruiz-Jimeno, A., Scodellaro, L., Vila, I., Cortabitarte, R. Vilar, Abbaneo, D., Auffray, E., Auzinger, G., Bachtis, M., Baillon, P., Ball, A. H., Barney, D., Benaglia, A., Bendavid, J., Benhabib, L., Benitez, J. F., Bernet, C., Bloch, P., Bocci, A., Bonato, A., Bondu, O., Botta, C., Breuker, H., Camporesi, T., Cerminara, G., Colafranceschi, S., D'Alfonso, M., d'Enterria, D., Dabrowski, A., David, A., De Guio, F., De Roeck, A., De Visscher, S., Di Marco, E., Dobson, M., Dordevic, M., Dupont-Sagorin, N., Elliott-Peisert, A., Franzoni, G., Funk, W., Gigi, D., Gill, K., Giordano, D., Girone, M., Glege, F., Guida, R., Gundacker, S., Guthoff, M., Hammer, J., Hansen, M., Harris, P., Hegeman, J., Innocente, V., Janot, P., Kousouris, K., Krajczar, K., Lecoq, P., Lourenço, C., Magini, N., Malgeri, L., Mannelli, M., Marrouche, J., Masetti, L., Meijers, F., Mersi, S., Meschi, E., Moortgat, F., Morovic, S., Mulders, M., Orsini, L., Pape, L., Perez, E., Perrozzi, L., Petrilli, A., Petrucciani, G., Pfeiffer, A., Pimiä, M., Piparo, D., Plagge, M., Racz, A., Rolandi, G., Rovere, M., Sakulin, H., Schäfer, C., Schwick, C., Siegrist, P., Silva, P., Simon, M., Sphicas, P., Spiga, D., Steggemann, J., Stieger, B., Stoye, M., Takahashi, Y., Treille, D., Tsirou, A., Veres, G. I., Wardle, N., Wöhri, H. K., Wollny, H., Zeuner, W. D., Bertl, W., Deiters, K., Erdmann, W., Horisberger, R., Ingram, Q., Kaestli, H. C., Kotlinski, D., Renker, D., Rohe, T., Bachmair, F., Bäni, L., Bianchini, L., Buchmann, M. A., Casal, B., Chanon, N., Dissertori, G., Dittmar, M., Donegà, M., Dünser, M., Eller, P., Grab, C., Hits, D., Hoss, J., Lustermann, W., Mangano, B., Marini, A. C., Marionneau, M., del Arbol, P. Martinez Ruiz, Masciovecchio, M., Meister, D., Mohr, N., Musella, P., Nägeli, C., Nessi-Tedaldi, F., Pandolfi, F., Pauss, F., Peruzzi, M., Quittnat, M., Rebane, L., Rossini, M., Starodumov, A., Takahashi, M., Theofilatos, K., Wallny, R., Weber, H. A., Amsler, C., Canelli, M. F., Chiochia, V., De Cosa, A., Hinzmann, A., Hreus, T., Kilminster, B., Lange, C., Mejias, B. Millan, Ngadiuba, J., Pinna, D., Robmann, P., Ronga, F. J., Taroni, S., Verzetti, M., Yang, Y., Cardaci, M., Chen, K. H., Ferro, C., Kuo, C. M., Lin, W., Lu, Y. J., Volpe, R., Yu, S. S., Chang, P., Chang, Y. H., Chang, Y. W., Chao, Y., Chen, K. F., Chen, P. H., Dietz, C., Grundler, U., Hou, W. -S., Kao, K. Y., Liu, Y. F., Lu, R. -S., Majumder, D., Petrakou, E., Tzeng, Y. M., Wilken, R., Asavapibhop, B., Singh, G., Srimanobhas, N., Suwonjandee, N., Adiguzel, A., Bakirci, M. N., Cerci, S., Dozen, C., Dumanoglu, I., Eskut, E., Girgis, S., Gokbulut, G., Gurpinar, E., Hos, I., Kangal, E. E., Topaksu, A. Kayis, Onengut, G., Ozdemir, K., Ozturk, S., Polatoz, A., Cerci, D. Sunar, Tali, B., Topakli, H., Vergili, M., Akin, I. V., Bilin, B., Bilmis, S., Gamsizkan, H., Isildak, B., Karapinar, G., Ocalan, K., Sekmen, S., Surat, U. E., Yalvac, M., Zeyrek, M., Albayrak, E. A., Gülmez, E., Kaya, M., Kaya, O., Yetkin, T., Cankocak, K., Vardarlı, F. I., Levchuk, L., Sorokin, P., Brooke, J. J., Clement, E., Cussans, D., Flacher, H., Goldstein, J., Grimes, M., Heath, G. P., Heath, H. F., Jacob, J., Kreczko, L., Lucas, C., Meng, Z., Newbold, D. M., Paramesvaran, S., Poll, A., Sakuma, T., Senkin, S., Smith, V. J., Bell, K. W., Brew, C., Brown, R. M., Cockerill, D. J. A., Coughlan, J. A., Harder, K., Harper, S., Olaiya, E., Petyt, D., Shepherd-Themistocleous, C. H., Thea, A., Tomalin, I. R., Williams, T., Womersley, W. J., Worm, S. D., Baber, M., Bainbridge, R., Buchmuller, O., Burton, D., Colling, D., Cripps, N., Dauncey, P., Davies, G., Della Negra, M., Dunne, P., Ferguson, W., Fulcher, J., Futyan, D., Hall, G., Iles, G., Jarvis, M., Karapostoli, G., Kenzie, M., Lane, R., Lucas, R., Lyons, L., Magnan, A. -M., Malik, S., Mathias, B., Nash, J., Nikitenko, A., Pela, J., Pesaresi, M., Petridis, K., Raymond, D. M., Rogerson, S., Rose, A., Seez, C., Sharp, P., Tapper, A., Acosta, M. Vazquez, Virdee, T., Zenz, S. C., Cole, J. E., Hobson, P. R., Khan, A., Kyberd, P., Leggat, D., Leslie, D., Reid, I. D., Symonds, P., Teodorescu, L., Turner, M., Dittmann, J., Hatakeyama, K., Kasmi, A., Liu, H., Scarborough, T., Charaf, O., Cooper, S. I., Henderson, C., Rumerio, P., Avetisyan, A., Bose, T., Fantasia, C., Lawson, P., Richardson, C., Rohlf, J., John, J. St., Sulak, L., Alimena, J., Berry, E., Christopher, G., Cutts, D., Demiragli, Z., Dhingra, N., Ferapontov, A., Garabedian, A., Heintz, U., Kukartsev, G., Laird, E., Landsberg, G., Luk, M., Narain, M., Segala, M., Sinthuprasith, T., Speer, T., Swanson, J., Breedon, R., Breto, G., Sanchez, M. Calderon De La Barca, Chauhan, S., Chertok, M., Conway, J., Conway, R., Cox, P. T., Erbacher, R., Gardner, M., Ko, W., Lander, R., Mulhearn, M., Pellett, D., Pilot, J., Ricci-Tam, F., Shalhout, S., Smith, J., Squires, M., Stolp, D., Tripathi, M., Wilbur, S., Yohay, R., Cousins, R., Everaerts, P., Farrell, C., Hauser, J., Ignatenko, M., Rakness, G., Takasugi, E., Valuev, V., Burt, K., Clare, R., Ellison, J., Gary, J. W., Hanson, G., Heilman, J., Rikova, M. Ivova, Jandir, P., Kennedy, E., Lacroix, F., Long, O. R., Luthra, A., Malberti, M., Negrete, M. Olmedo, Shrinivas, A., Sumowidagdo, S., Wimpenny, S., Branson, J. G., Cerati, G. B., Cittolin, S., D'Agnolo, R. T., Holzner, A., Kelley, R., Klein, D., Kovalskyi, D., Letts, J., Macneill, I., Olivito, D., Padhi, S., Palmer, C., Pieri, M., Sani, M., Simon, S., Tu, Y., Vartak, A., Welke, C., Würthwein, F., Yagil, A., Barge, D., Bradmiller-Feld, J., Campagnari, C., Danielson, T., Dishaw, A., Dutta, V., Flowers, K., Sevilla, M. Franco, Geffert, P., George, C., Golf, F., Gouskos, L., Incandela, J., Justus, C., Mccoll, N., Richman, J., Stuart, D., To, W., West, C., Yoo, J., Apresyan, A., Bornheim, A., Bunn, J., Chen, Y., Duarte, J., Mott, A., Newman, H. B., Pena, C., Pierini, M., Spiropulu, M., Vlimant, J. R., Wilkinson, R., Xie, S., Zhu, R. Y., Azzolini, V., Calamba, A., Carlson, B., Ferguson, T., Iiyama, Y., Paulini, M., Russ, J., Vogel, H., Vorobiev, I., Cumalat, J. P., Ford, W. T., Gaz, A., Krohn, M., Lopez, E. Luiggi, Nauenberg, U., Smith, J. G., Stenson, K., Wagner, S. R., Alexander, J., Chatterjee, A., Chaves, J., Chu, J., Dittmer, S., Eggert, N., Mirman, N., Kaufman, G. Nicolas, Patterson, J. R., Ryd, A., Salvati, E., Skinnari, L., Sun, W., Teo, W. D., Thom, J., Thompson, J., Tucker, J., Weng, Y., Winstrom, L., Wittich, P., Winn, D., Abdullin, S., Albrow, M., Anderson, J., Apollinari, G., Bauerdick, L. A. T., Beretvas, A., Berryhill, J., Bhat, P. C., Bolla, G., Burkett, K., Butler, J. N., Cheung, H. W. K., Chlebana, F., Cihangir, S., Elvira, V. D., Fisk, I., Freeman, J., Gao, Y., Gottschalk, E., Gray, L., Green, D., Grünendahl, S., Gutsche, O., Hanlon, J., Hare, D., Harris, R. M., Hirschauer, J., Hooberman, B., Jindariani, S., Johnson, M., Joshi, U., Kaadze, K., Klima, B., Kreis, B., Kwan, S., Linacre, J., Lincoln, D., Lipton, R., Liu, T., Lykken, J., Maeshima, K., Marraffino, J. M., Outschoorn, V. I. Martinez, Maruyama, S., Mason, D., McBride, P., Merkel, P., Mishra, K., Mrenna, S., Nahn, S., Newman-Holmes, C., O'Dell, V., Prokofyev, O., Sexton-Kennedy, E., Sharma, S., Soha, A., Spalding, W. J., Spiegel, L., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vidal, R., Whitbeck, A., Whitmore, J., Yang, F., Acosta, D., Avery, P., Bortignon, P., Bourilkov, D., Carver, M., Curry, D., Das, S., De Gruttola, M., Di Giovanni, G. P., Field, R. D., Fisher, M., Furic, I. K., Hugon, J., Konigsberg, J., Korytov, A., Kypreos, T., Low, J. F., Matchev, K., Mei, H., Milenovic, P., Mitselmakher, G., Muniz, L., Rinkevicius, A., Shchutska, L., Snowball, M., Sperka, D., Yelton, J., Zakaria, M., Hewamanage, S., Linn, S., Markowitz, P., Martinez, G., Rodriguez, J. L., Adams, T., Askew, A., Bochenek, J., Diamond, B., Haas, J., Hagopian, S., Hagopian, V., Johnson, K. F., Prosper, H., Veeraraghavan, V., Weinberg, M., Baarmand, M. M., Hohlmann, M., Kalakhety, H., Yumiceva, F., Adams, M. R., Apanasevich, L., Berry, D., Betts, R. R., Bucinskaite, I., Cavanaugh, R., Evdokimov, O., Gauthier, L., Gerber, C. E., Hofman, D. J., Kurt, P., Moon, D. H., O'Brien, C., Gonzalez, I. D. Sandoval, Silkworth, C., Turner, P., Varelas, N., Bilki, B., Clarida, W., Dilsiz, K., Haytmyradov, M., Merlo, J. -P., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Ogul, H., Onel, Y., Ozok, F., Penzo, A., Rahmat, R., Sen, S., Tan, P., Tiras, E., Wetzel, J., Yi, K., Barnett, B. A., Blumenfeld, B., Bolognesi, S., Fehling, D., Gritsan, A. V., Maksimovic, P., Martin, C., Swartz, M., Baringer, P., Bean, A., Benelli, G., Bruner, C., Kenny III, R. P., Malek, M., Murray, M., Noonan, D., Sanders, S., Sekaric, J., Stringer, R., Wang, Q., Wood, J. S., Chakaberia, I., Ivanov, A., Khalil, S., Makouski, M., Maravin, Y., Saini, L. K., Skhirtladze, N., Svintradze, I., Gronberg, J., Lange, D., Rebassoo, F., Wright, D., Baden, A., Belloni, A., Calvert, B., Eno, S. C., Gomez, J. A., Hadley, N. J., Kellogg, R. G., Kolberg, T., Lu, Y., Mignerey, A. C., Pedro, K., Skuja, A., Tonjes, M. B., Tonwar, S. C., Apyan, A., Barbieri, R., Bauer, G., Busza, W., Cali, I. A., Chan, M., Di Matteo, L., Ceballos, G. Gomez, Goncharov, M., Gulhan, D., Klute, M., Lai, Y. S., Lee, Y. -J., Levin, A., Luckey, P. D., Ma, T., Paus, C., Ralph, D., Roland, C., Roland, G., Stephans, G. S. F., Sumorok, K., Velicanu, D., Veverka, J., Wyslouch, B., Yang, M., Zanetti, M., Zhukova, V., Dahmes, B., Gude, A., Kao, S. C., Klapoetke, K., Kubota, Y., Mans, J., Pastika, N., Rusack, R., Singovsky, A., Tambe, N., Turkewitz, J., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Bose, S., Claes, D. R., Dominguez, A., Suarez, R. Gonzalez, Keller, J., Knowlton, D., Kravchenko, I., Lazo-Flores, J., Meier, F., Ratnikov, F., Snow, G. R., Zvada, M., Dolen, J., Godshalk, A., Iashvili, I., Kharchilava, A., Rappoccio, S., Alverson, G., Barberis, E., Baumgartel, D., Chasco, M., Massironi, A., Morse, D. M., Nash, D., Orimoto, T., Trocino, D., Wang, R. -J., Wood, D., Zhang, J., Hahn, K. A., Kubik, A., Mucia, N., Odell, N., Pollack, B., Pozdnyakov, A., Schmitt, M., Stoynev, S., Sung, K., Velasco, M., Won, S., Brinkerhoff, A., Chan, K. M., Drozdetskiy, A., Hildreth, M., Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Lynch, S., Marinelli, N., Musienko, Y., Pearson, T., Planer, M., Ruchti, R., Smith, G., Valls, N., Wayne, M., Wolf, M., Woodard, A., Antonelli, L., Brinson, J., Bylsma, B., Durkin, L. S., Flowers, S., Hart, A., Hill, C., Hughes, R., Kotov, K., Ling, T. Y., Luo, W., Puigh, D., Rodenburg, M., Winer, B. L., Wolfe, H., Wulsin, H. W., Driga, O., Elmer, P., Hardenbrook, J., Hebda, P., Hunt, A., Koay, S. A., Lujan, P., Marlow, D., Medvedeva, T., Mooney, M., Olsen, J., Piroué, P., Quan, X., Saka, H., Stickland, D., Tully, C., Werner, J. S., Zuranski, A., Brownson, E., Mendez, H., Vargas, J. E. Ramirez, Barnes, V. E., Benedetti, D., Bortoletto, D., De Mattia, M., Gutay, L., Hu, Z., Jha, M. K., Jones, M., Jung, K., Kress, M., Leonardo, N., Miller, D. H., Neumeister, N., Radburn-Smith, B. C., Shi, X., Shipsey, I., Silvers, D., Svyatkovskiy, A., Wang, F., Xie, W., Xu, L., Zablocki, J., Parashar, N., Stupak, J., Adair, A., Akgun, B., Ecklund, K. M., Geurts, F. J. M., Li, W., Michlin, B., Padley, B. P., Redjimi, R., Roberts, J., Zabel, J., Betchart, B., Bodek, A., Covarelli, R., de Barbaro, P., Demina, R., Eshaq, Y., Ferbel, T., Garcia-Bellido, A., Goldenzweig, P., Han, J., Harel, A., Khukhunaishvili, A., Korjenevski, S., Petrillo, G., Vishnevskiy, D., Ciesielski, R., Demortier, L., Goulianos, K., Mesropian, C., Arora, S., Barker, A., Chou, J. P., Contreras-Campana, C., Contreras-Campana, E., Duggan, D., Ferencek, D., Gershtein, Y., Gray, R., Halkiadakis, E., Hidas, D., Kaplan, S., Lath, A., Panwalkar, S., Park, M., Patel, R., Salur, S., Schnetzer, S., Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Rose, K., Spanier, S., York, A., Bouhali, O., Hernandez, A. Castaneda, Eusebi, R., Flanagan, W., Gilmore, J., Kamon, T., Khotilovich, V., Krutelyov, V., Montalvo, R., Osipenkov, I., Pakhotin, Y., Perloff, A., Roe, J., Safonov, A., Suarez, I., Tatarinov, A., Ulmer, K. A., Akchurin, N., Cowden, C., Damgov, J., Dragoiu, C., Dudero, P. R., Faulkner, J., Kovitanggoon, K., Kunori, S., Lee, S. W., Libeiro, T., Volobouev, I., Appelt, E., Delannoy, A. G., Greene, S., Gurrola, A., Johns, W., Maguire, C., Melo, A., Sharma, M., Sheldon, P., Snook, B., Tuo, S., Velkovska, J., Arenton, M. W., Boutle, S., Cox, B., Francis, B., Goodell, J., Hirosky, R., Ledovskoy, A., Li, H., Lin, C., Neu, C., Wood, J., Clarke, C., Harr, R., Karchin, P. E., Don, C. Kottachchi Kankanamge, Lamichhane, P., Sturdy, J., Belknap, D. A., Carlsmith, D., Cepeda, M., Dasu, S., Dodd, L., Duric, S., Friis, E., Hall-Wilton, R., Herndon, M., Hervé, A., Klabbers, P., Lanaro, A., Lazaridis, C., Levine, A., Loveless, R., Mohapatra, A., Ojalvo, I., Perry, T., Pierro, G. A., Polese, G., Ross, I., Sarangi, T., Savin, A., Smith, W. H., Taylor, D., Vuosalo, C., Woods, N., Bediaga, I., De Miranda, J. M., Rodrigues, F. Ferreira, Gomes, A., Massafferri, A., Reis, A. C. dos, Rodrigues, A. B., Amato, S., Akiba, K. Carvalho, De Paula, L., Francisco, O., Gandelman, M., Hicheur, A., Lopes, J. H., Tostes, D. Martins, Nasteva, I., Goicochea, J. M. Otalora, Polycarpo, E., Potterat, C., Rangel, M. S., Guimaraes, V. Salustino, De Paula, B. Souza, Vieira, D., An, L., Jing, F., Li, Y., Yang, Z., Yuan, X., Zhang, Y., Zhong, L., Beaucourt, L., Chefdeville, M., Decamp, D., Déléage, N., Ghez, Ph., Lees, J. -P., Marchand, J. F., Minard, M. -N., Pietrzyk, B., Qian, W., T'Jampens, S., Tisserand, V., Tournefier, E., Ajaltouni, Z., Baalouch, M., Cogneras, E., Deschamps, O., Rifai, I. El, Gándara, M. Grabalosa, Henrard, P., Hoballah, M., Lefèvre, R., Maratas, J., Monteil, S., Niess, V., Perret, P., Adrover, C., Akar, S., Aslanides, E., Cogan, J., Kanso, W., Gac, R. Le, Leroy, O., Mancinelli, G., Mordà, A., Perrin-Terrin, M., Serrano, J., Tsaregorodtsev, A., Amhis, Y., Barsuk, S., Borsato, M., Kochebina, O., Lefrançois, J., Machefert, F., Sánchez, A. Martín, Nicol, M., Robbe, P., Schune, M. -H., Teklishyn, M., Vallier, A., Viaud, B., Wormser, G., Ben-Haim, E., Charles, M., Coquereau, S., David, P., Del Buono, L., Henry, L., Polci, F., Albrecht, J., Brambach, T., Cauet, Ch., Deckenhoff, M., Eitschberger, U., Ekelhof, R., Gavardi, L., Kruse, F., Niet, R., Parkinson, C. J., Schlupp, M., Shires, A., Spaan, B., Swientek, S., Wishahi, J., Gutierrez, O. Aquines, Blouw, J., Britsch, M., Fontana, M., Popov, D., Schmelling, M., Volyanskyy, D., Zavertyaev, M., Bachmann, S., Bien, A., Comerma-Montells, A., De Cian, M., Dordei, F., Esen, S., Färber, C., Gersabeck, E., Grillo, L., Han, X., Hansmann-Menzemer, S., Jaeger, A., Kolpin, M., Kreplin, K., Krocker, G., Leverington, B., Marks, J., Meissner, M., Neuner, M., Nikodem, T., Seyfert, P., Stahl, M., Stahl, S., Uwer, U., Vesterinen, M., Wandernoth, S., Wiedner, D., Zhelezov, A., McNulty, R., Wallace, R., Zhang, W. C., Palano, A., Carbone, A., Falabella, A., Galli, D., Marconi, U., Moggi, N., Mussini, M., Perazzini, S., Vagnoni, V., Valenti, G., Zangoli, M., Bonivento, W., Cadeddu, S., Cardini, A., Cogoni, V., Contu, A., Lai, A., Liu, B., Manca, G., Oldeman, R., Saitta, B., Vacca, C., Andreotti, M., Baldini, W., Bozzi, C., Calabrese, R., Corvo, M., Fiore, M., Fiorini, M., Luppi, E., Pappalardo, L. L., Shapoval, I., Tellarini, G., Tomassetti, L., Vecchi, S., Anderlini, L., Bizzeti, A., Frosini, M., Graziani, G., Passaleva, G., Veltri, M., Bencivenni, G., Campana, P., De Simone, P., Lanfranchi, G., Palutan, M., Rama, M., Sarti, A., Sciascia, B., Gomez, R. Vazquez, Cardinale, R., Fontanelli, F., Gambetta, S., Patrignani, C., Petrolini, A., Pistone, A., Calvi, M., Cassina, L., Gotti, C., Khanji, B., Kucharczyk, M., Matteuzzi, C., Fu, J., Geraci, A., Neri, N., Palombo, F., Amerio, S., Collazuol, G., Gallorini, S., Gianelle, A., Lucchesi, D., Lupato, A., Morandin, M., Rotondo, M., Sestini, L., Simi, G., Stroili, R., Bedeschi, F., Cenci, R., Leo, S., Marino, P., Morello, M. J., Punzi, G., Stracka, S., Walsh, J., Carboni, G., Furfaro, E., Santovetti, E., Satta, A., Alves Jr, A. A., Auriemma, G., Bocci, V., Martellotti, G., Penso, G., Pinci, D., Santacesaria, R., Satriano, C., Sciubba, A., Dziurda, A., Kucewicz, W., Lesiak, T., Rachwal, B., Witek, M., Firlej, M., Fiutowski, T., Idzik, M., Morawski, P., Moron, J., Oblakowska-Mucha, A., Swientek, K., Szumlak, T., Batozskaya, V., Klimaszewski, K., Kurek, K., Szczekowski, M., Ukleja, A., Wislicki, W., Cojocariu, L., Giubega, L., Grecu, A., Maciuc, F., Orlandea, M., Popovici, B., Stoica, S., Straticiuc, M., Alkhazov, G., Bondar, N., Dzyuba, A., Maev, O., Sagidova, N., Shcheglov, Y., Belogurov, S., Belyaev, I., Egorychev, V., Golubkov, D., Kvaratskheliya, T., Machikhiliyan, I. V., Polyakov, I., Savrina, D., Semennikov, A., Zhokhov, A., Berezhnoy, A., Korolev, M., Leflat, A., Nikitin, N., Filippov, S., Gushchin, E., Kravchuk, L., Bondar, A., Eidelman, S., Krokovny, P., Kudryavtsev, V., Shekhtman, L., Vorobyev, V., Artamonov, A., Belous, K., Dzhelyadin, R., Guz, Yu., Novoselov, A., Obraztsov, V., Romanovsky, V., Shapkin, M., Stenyakin, O., Yushchenko, O., Badalov, A., Gomez, M. Calvo, Garrido, L., Gascon, D., Diaz, R. Graciani, Graugés, E., Benito, C. Marin, Olloqui, E. Picatoste, Molina, V. Rives, Ruiz, H., Vilasis-Cardona, X., Adeva, B., Cartelle, P. Alvarez, Suárez, A. Dosil, Albor, V. Fernandez, Torreira, A. Gallas, Pardiñas, J. García, Morata, J. A. Hernando, Casasus, M. Plo, Vidal, A. Romero, Silva, J. J. Saborido, Sedes, B. Sanmartin, Rios, C. Santamarina, Regueiro, P. Vazquez, Sierra, C. Vázquez, Diaz, M. Vieites, Alessio, F., Archilli, F., Barschel, C., Benson, S., Buytaert, J., Perez, D. Campora, Garcia, L. Castillo, Cattaneo, M., Charpentier, Ph., Vidal, X. Cid, Clemencic, M., Closier, J., Coco, V., Collins, P., Corti, G., Couturier, B., D'Ambrosio, C., Dettori, F., Di Canto, A., Dijkstra, H., Durante, P., Ferro-Luzzi, M., Forty, R., Frank, M., Frei, C., Gaspar, C., Gligorov, V. V., Cardoso, L. A. Granado, Gys, T., Haen, C., He, J., Head, T., van Herwijnen, E., Jacobsson, R., Johnson, D., Joram, C., Jost, B., Karacson, M., Karbach, T. M., Lacarrere, D., Langhans, B., Lindner, R., Linn, C., Lohn, S., Mapelli, A., Matev, R., Mathe, Z., Neubert, S., Neufeld, N., Otto, A., Panman, J., Altarelli, M. Pepe, Rauschmayr, N., Rihl, M., Roiser, S., Ruf, T., Schindler, H., Schmidt, B., Schopper, A., Schwemmer, R., Sridharan, S., Stagni, F., Subbiah, V. K., Teubert, F., Thomas, E., Tonelli, D., Trisovic, A., Garcia, M. Ubeda, Wicht, J., Wyllie, K., Battista, V., Bay, A., Blanc, F., Dorigo, M., Dupertuis, F., Fitzpatrick, C., Gianì, S., Haefeli, G., Jaton, P., Khurewathanakul, C., Komarov, I., La Thi, V. N., Lopez-March, N., Märki, R., Martinelli, M., Muster, B., Nakada, T., Nguyen, A. D., Nguyen, T. D., Nguyen-Mau, C., Prisciandaro, J., Navarro, A. Puig, Rakotomiaramanana, B., Rouvinet, J., Schneider, O., Soomro, F., Szczypka, P., Tobin, M., Tourneur, S., Tran, M. T., Veneziano, G., Bernet, R., Bowen, E., Bursche, A., Chiapolini, N., Chrzaszcz, M., Elsasser, Ch., Graverini, E., Lionetto, F., Lowdon, P., Müller, K., Serra, N., Steinkamp, O., Storaci, B., Straumann, U., Tresch, M., Vollhardt, A., Aaij, R., Ali, S., van Beuzekom, M., David, P. N. Y., De Bruyn, K., Farinelli, C., Heijne, V., Hulsbergen, W., Jans, E., Koppenburg, P., Kozlinskiy, A., van Leerdam, J., Merk, M., Oggero, S., Pellegrino, A., Snoek, H., van Tilburg, J., Tsopelas, P., Tuning, N., de Vries, J. A., Ketel, T., Koopman, R. F., Lambert, R. W., Santos, D. Martinez, Raven, G., Schiller, M., Syropoulos, V., Tolk, S., Dovbnya, A., Kandybei, S., Raniuk, I., Okhrimenko, O., Pugatch, V., Bifani, S., Farley, N., Griffith, P., Kenyon, I. R., Lazzeroni, C., Mazurov, A., McCarthy, J., Pescatore, L., Watson, N. K., Williams, M. P., Adinolfi, M., Benton, J., Brook, N. H., Cook, A., Coombes, M., Dalseno, J., Hampson, T., Harnew, S. T., Naik, P., Price, E., Prouve, C., Rademacker, J. H., Richards, S., Saunders, D. M., Skidmore, N., Souza, D., Velthuis, J. J., Voong, D., Barter, W., Bettler, M. -O., Cliff, H. V., Evans, H. -M., Tico, J. Garra, Gibson, V., Gregson, S., Haines, S. C., Jones, C. R., Sirendi, M., Ward, D. R., Wotton, S. A., Wright, S., Back, J. J., Blake, T., Craik, D. C., Crocombe, A. C., Dossett, D., Gershon, T., Kreps, M., Langenbruch, C., Latham, T., O'Hanlon, D. P., Pilař, T., Poluektov, A., Reid, M. M., Coutinho, R. Silva, Wallace, C., Whitehead, M., Easo, S., Nandakumar, R., Papanestis, A., Ricciardi, S., Wilson, F. F., Carson, L., Clarke, P. E. L., Cowan, G. A., Eisenhardt, S., Ferguson, D., Lambert, D., Luo, H., Morris, A. -B., Muheim, F., Needham, M., Playfer, S., Alexander, M., Beddow, J., Dean, C. -T., Eklund, L., Hynds, D., Karodia, S., Longstaff, I., Ogilvy, S., Pappagallo, M., Sail, P., Skillicorn, I., Soler, F. J. P., Spradlin, P., Affolder, A., Bowcock, T. J. V., Brown, H., Casse, G., Donleavy, S., Dreimanis, K., Farry, S., Fay, R., Hennessy, K., Hutchcroft, D., Liles, M., McSkelly, B., Patel, G. D., Price, J. D., Pritchard, A., Rinnert, K., Shears, T., Smith, N. A., Ciezarek, G., Cunliffe, S., Currie, R., Egede, U., Fol, P., Golutvin, A., Hall, S., McCann, M., Owen, P., Patel, M., Redi, F., Sepp, I., Smith, E., Sutcliffe, W., Websdale, D., Appleby, R. B., Barlow, R. J., Bird, T., Bjørnstad, P. M., Borghi, S., Brett, D., Brodzicka, J., Capriotti, L., Chen, S., De Capua, S., Dujany, G., Gersabeck, M., Harrison, J., Hombach, C., Klaver, S., Lafferty, G., McNab, A., Parkes, C., Pearce, A., Reichert, S., Rodrigues, E., Perez, P. Rodriguez, Smith, M., Cheung, S. -F., Derkach, D., Evans, T., Gauld, R., Greening, E., Harnew, N., Hill, D., Hunt, P., Hussain, N., Jalocha, J., John, M., Lupton, O., Malde, S., Stevenson, S., Thomas, C., Topp-Joergensen, S., Torr, N., Wilkinson, G., Counts, I., Ilten, P., Williams, M., Andreassen, R., Davis, A., De Silva, W., Meadows, B., Sokoloff, M. D., Sun, L., Todd, J., Andrews, J. E., Hamilton, B., Jawahery, A., Wimberley, J., Artuso, M., Blusk, S., Borgia, A., Britton, T., Ely, S., Gandini, P., Garofoli, J., Gui, B., Hadjivasiliou, C., Jurik, N., Kelsey, M., Mountain, R., Pal, B. K., Skwarnicki, T., Stone, S., Xing, Z., Zhang, L., Baesso, C., Torres, M. Cruz, Göbel, C., Rodriguez, J. Molina, Xie, Y., Milanes, D. A., Grünberg, O., Heß, M., Voß, C., Waldi, R., Likhomanenko, T., Malinin, A., Shevchenko, V., Ustyuzhanin, A., Vidal, F. Martinez, Oyanguren, A., Valls, P. Ruiz, Mayordomo, C. Sanchez, Onderwater, C. J. G., Wilschut, H. W., and Pesen, E.
Subjects: High Energy Physics - Experiment, High Energy Physics - Phenomenology
Abstract: A joint measurement is presented of the branching fractions $B^0_s\to\mu^+\mu^-$ and $B^0\to\mu^+\mu^-$ in proton-proton collisions at the LHC by the CMS and LHCb experiments. The data samples were collected in 2011 at a centre-of-mass energy of 7 TeV, and in 2012 at 8 TeV. The combined analysis produces the first observation of the $B^0_s\to\mu^+\mu^-$ decay, with a statistical significance exceeding six standard deviations, and the best measurement of its branching fraction so far. Furthermore, evidence for the $B^0\to\mu^+\mu^-$ decay is obtained with a statistical significance of three standard deviations. The branching fraction measurements are statistically compatible with SM predictions and impose stringent constraints on several theories beyond the SM., Comment: Correspondence should be addressed to cms-and-lhcb-publication-committees@cern.ch
Published: 2014
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35. Milky Way demographics with the VVV Survey III. Evidence for a Great Dark Lane in the 157 Million Star Bulge Color-Magnitude Diagram

Author: Minniti, D., Saito, R. K., Gonzalez, O. A., Zoccali, M., Rejkuba, M., Alonso-Garcia, J., Benjamin, R., Catelan, M., Dekany, I., Emerson, J. P., Hempel, M., Lucas, P. W., and Schultheis, M.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The new generation of IR surveys are revealing and quantifying Galactic features, providing an improved 3-D interpretation of our own Galaxy. We present an analysis of the global distribution of dust clouds in the bulge using the near-IR photometry of 157 million stars from the VVV Survey. We investigate the color magnitude diagram of the Milky Way bulge which shows a red giant clump of core He burning stars that is split in two color components, with a mean color difference of (Z-Ks)=0.55 magnitudes equivalent to A_V=2.0 magnitudes. We conclude that there is an optically thick dust lane at intermediate latitudes above and below the plane, that runs across several square degrees from l=-10 deg to l=+10 deg. We call this feature the "Great Dark Lane". Although its exact distance is uncertain, it is located in front of the bulge. The evidence for a large-scale great dark lane within the Galactic bulge is important in order to constrain models of the barred Milky Way bulge and to compare our galaxy with external barred galaxies, where these kinds of features are prominent. We discuss two other potential implications of the presence of the Great Dark Lane for microlensing and bulge stellar populations studies., Comment: 5 pages, 4 figures, accepted for publication in Astronomy and Astrophysics
Published: 2014
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36. New galactic star clusters discovered in the VVV survey. Candidates projected on the inner disk and bulge

Author: Borissova, J., Chené, A. -N., Alegría, S. Ramírez, Sharma, Saurabh, Clarke, J. R. A., Kurtev, R., Negueruela, I., Marco, A., Amigo, P., Minniti, D., Bica, E., Bonatto, C., Catelan, M., Fierro, C., Geisler, D., Gromadzki, M., Hempel, M., Hanson, M. M., Ivanov, V. D., Lucas, P., Majaess, D., Bidin, C. Moni, Popescu, B., and Saito, R. K.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: VISTA Variables in the V\'ia L\'actea (VVV) is one of six ESO Public Surveys using the 4 meter Visible and Infrared Survey Telescope for Astronomy (VISTA). The VVV survey covers the Milky Way bulge and an adjacent section of the disk, and one of the principal objectives is to search for new star clusters within previously unreachable obscured parts of the Galaxy. The primary motivation behind this work is to discover and analyze obscured star clusters in the direction of the inner Galactic disk and bulge. Regions of the inner disk and bulge covered by the VVV survey were visually inspected using composite JHKs color images to select new cluster candidates on the basis of apparent overdensities. DR1, DR2, CASU, and PSF photometry of 10x10 arcmin fields centered on each candidate cluster were used to construct color-magnitude and color-color diagrams. Follow-up spectroscopy of the brightest members of several cluster candidates was obtained in order to clarify their nature. We report the discovery of 58 new infrared cluster candidates. Fundamental parameters such as age, distance, and metallicity were determined for 20 of the most populous clusters., Comment: 23 pages, 20 figures and 3 tables
Published: 2014
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37. Stellar Variability in the VVV Survey: An Update

Author: Catelan, M., Dekany, I., Hempel, M., and Minniti, D.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: The Vista Variables in the Via Lactea (VVV) ESO Public Survey consists in a near-infrared time-series survey of the Galactic bulge and inner disk, covering 562 square degrees of the sky, over a total timespan of more than 5 years. In this paper, we provide an updated account of the current status of the survey, especially in the context of stellar variability studies. In this sense, we give a first description of our efforts towards the construction of the VVV Variable Star Catalog (VVV-VSC)., Comment: 10 pages, 6 figures. Invited review, to appear in BAAA (Boletin de la Asociacion Argentina de Astronomia)
Published: 2014

38. The VVV Templates Project. Towards an Automated Classification of VVV Light-Curves. I. Building a database of stellar variability in the near-infrared

Author: Angeloni, R., Ramos, R. Contreras, Catelan, M., Dékány, I., Gran, F., Alonso-García, J., Hempel, M., Navarrete, C., Andrews, H., Aparicio, A., Beamín, J. C., Berger, C., Borissova, J., Peña, C. Contreras, Cunial, A., de Grijs, R., Espinoza, N., Eyheramendy, S., Lopes, C. E. Ferreira, Fiaschi, M., Hajdu, G., Han, J., Hełminiak, K. G., Hempel, A., Hidalgo, S. L., Ita, Y., Jeon, Y. -B., Jordán, A., Kwon, J., Lee, J. T., Martín, E. L., Masetti, N., Matsunaga, N., Milone, A. P., Minniti, D., Morelli, L., Murgas, F., Nagayama, T., Navarro, C., Ochner, P., Pérez, P., Pichara, K., Rojas-Arriagada, A., Roquette, J., Saito, R. K., Siviero, A., Sohn, J., Sung, H. -I., Tamura, M., Tata, R., Tomasella, L., Townsend, B., and Whitelock, P.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: Context. The Vista Variables in the V\'ia L\'actea (VVV) ESO Public Survey is a variability survey of the Milky Way bulge and an adjacent section of the disk carried out from 2010 on ESO Visible and Infrared Survey Telescope for Astronomy (VISTA). VVV will eventually deliver a deep near-IR atlas with photometry and positions in five passbands (ZYJHK_S) and a catalogue of 1-10 million variable point sources - mostly unknown - which require classifications. Aims. The main goal of the VVV Templates Project, that we introduce in this work, is to develop and test the machine-learning algorithms for the automated classification of the VVV light-curves. As VVV is the first massive, multi-epoch survey of stellar variability in the near-infrared, the template light-curves that are required for training the classification algorithms are not available. In the first paper of the series we describe the construction of this comprehensive database of infrared stellar variability. Methods. First we performed a systematic search in the literature and public data archives, second, we coordinated a worldwide observational campaign, and third we exploited the VVV variability database itself on (optically) well-known stars to gather high-quality infrared light-curves of several hundreds of variable stars. Results. We have now collected a significant (and still increasing) number of infrared template light-curves. This database will be used as a training-set for the machine-learning algorithms that will automatically classify the light-curves produced by VVV. The results of such an automated classification will be covered in forthcoming papers of the series., Comment: 12 pages, 16 figures, 3 tables, accepted for publication in A&A. Most of the data are now accessible through http://www.vvvtemplates.org/
Published: 2014
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39. Specific heat of K071Na0.29Fe2As2 at very low temperatures

Author: Reifenberger, A., Hempel, M., Vogt, P., Aswartham, S., Abdel-Hafiez, M., Grinenko, V., Wurmehl, S., Drechsler, S. -L., Fleischmann, A., Enss, C., and Klingeler, R.
Subjects: Condensed Matter - Superconductivity
Abstract: A commercially available calorimeter has been used to investigate the specific heat of a high-quality \kn\ single crystal. The addenda heat capacity of the calorimeter is determined in the temperature range $0.02 \, \mathrm{K} \leq T \leq 0.54 \, \mathrm{K}$. The data of the \kn\ crystal imply the presence of a large $T^2$ contribution to the specific heat which gives evidence of $d$-wave order parameter symmetry in the superconducting state. To improve the measurements, a novel design for a calorimeter with a paramagnetic temperature sensor is presented. It promises a temperature resolution of $\Delta T \approx 0.1 \, \mathrm{\mu K}$ and an addenda heat capacity less than $200 \, \mathrm{pJ/K}$ at $ T < 100 \, \mathrm{mK}$., Comment: 8 pages, 5 figures
Published: 2014
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40. Massive open star clusters using the VVV survey III: A young massive cluster at the far edge of the Galactic bar

Author: Alegría, S. Ramírez, Borissova, J., Chené, A. N., O'Leary, E., Amigo, P., Minniti, D., Saito, R. K., Geisler, D., Kurtev, R., Hempel, M., Gromadzki, M., Clarke, J. R. A., Negueruela, I., Marco, A., Fierro, C., Bonatto, C., and Catelan, M.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Context: Young massive clusters are key to map the Milky Way's structure, and near-IR large area sky surveys have contributed strongly to the discovery of new obscured massive stellar clusters. Aims: We present the third article in a series of papers focused on young and massive clusters discovered in the VVV survey. This article is dedicated to the physical characterization of VVV CL086, using part of its OB-stellar population. Methods: We physically characterized the cluster using $JHK_S$ near-infrared photometry from ESO public survey VVV images, using the VVV-SkZ pipeline, and near-infrared $K$-band spectroscopy, following the methodology presented in the first article of the series. Results: Individual distances for two observed stars indicate that the cluster is located at the far edge of the Galactic bar. These stars, which are probable cluster members from the statistically field-star decontaminated CMD, have spectral types between O9 and B0V. According to our analysis, this young cluster ($1.0$ Myr $<$ age $< 5.0$ Myr) is located at a distance of $11^{+5}_{-6}$ kpc, and we estimate a lower limit for the cluster total mass of $(2.8^{+1.6}_{-1.4})\cdot10^3 {M}_{\odot}$. It is likely that the cluster contains even earlier and more massive stars., Comment: Accepted for publication as a Letter in A&A
Published: 2014
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41. Stellar Variability in the VVV survey

Author: Catelan, M., Minniti, D., Lucas, P. W., Dékány, I., Saito, R. K., Angeloni, R., Alonso-García, J., Hempel, M., Helminiak, K., Jordán, A., Ramos, R. Contreras, Navarrete, C., Beamín, J. C., Rojas, A. F., Gran, F., Lopes, C. E. Ferreira, Peña, C. Contreras, Kerins, E., Huckvale, L., Rejkuba, M., Cohen, R., Mauro, F., Borissova, J., Amigo, P., Eyheramendy, S., Pichara, K., Espinoza, N., Navarro, C., Hajdu, G., Espinoza, D. N. Calderón, Muro, G. A., Andrews, H., Motta, V., Kurtev, R., Emerson, J. P., Bidin, C. Moni, and Chené, A. -N.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: The Vista Variables in the V\'ia L\'actea (VVV) ESO Public Survey is an ongoing time-series, near-infrared (IR) survey of the Galactic bulge and an adjacent portion of the inner disk, covering 562 square degrees of the sky, using ESO's VISTA telescope. The survey has provided superb multi-color photometry in 5 broadband filters ($Z$, $Y$, $J$, $H$, and $K_s$), leading to the best map of the inner Milky Way ever obtained, particularly in the near-IR. The main variability part of the survey, which is focused on $K_s$-band observations, is currently underway, with bulge fields having been observed between 31 and 70 times, and disk fields between 17 and 36 times. When the survey is complete, bulge (disk) fields will have been observed up to a total of 100 (60) times, providing unprecedented depth and time coverage. Here we provide a first overview of stellar variability in the VVV data, including examples of the light curves that have been collected thus far, scientific applications, and our efforts towards the automated classification of VVV light curves., Comment: Presented at the "40 Years of Variable Stars: A Celebration of Contributions by Horace A. Smith" conference (arXiv:1310.0149). 49 pages, 28 figures
Published: 2013

42. VVV Survey Near-Infrared Photometry of Known Bulge RR Lyrae stars: the Distance to the Galactic Center and Absence of a Barred Distribution of the Metal-Poor Population

Author: Dékány, I., Minniti, D., Catelan, M., Zoccali, M., Saito, R. K., Hempel, M., and Gonzalez, O. A.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We have combined optical and near-infrared data of known RR Lyrae (RRL) stars in the bulge in order to study the spatial distribution of its metal-poor component by measuring precise reddening values and distances of 7663 fundamental-mode RRL stars with high-quality photometry. We obtain a distance to the Galactic center of R0 = 8.33 +/- 0.05 +/- 0.14 kpc. We find that the spatial distribution of the RRL stars differs from the structures traced by the predominantly metal-rich red clump (RC) stars. Unlike the RC stars, the RRL stars do not trace a strong bar, but have a more spheroidal, centrally concentrated distribution, showing only a slight elongation in its very center. We find a hint of bimodality in the density distribution at high southern latitudes (b < -5), which needs to be confirmed by extending the areal coverage of the current census. The different spatial distributions of the metal-rich and metal-poor stellar populations suggest that the Milky Way has a composite bulge., Comment: Accepted for publication in The Astrophysical Journal Letters, copyright AAS 2013
Published: 2013
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43. Milky Way Demographics with the VVV Survey II. Color Transformations and Near-Infrared Photometry for 136 Million Stars in the Southern Galactic Disk

Author: Soto, M., Barba, R., Gunthardt, G., Minniti, D., Lucas, P., Majaess, D., Irwin, M., Emerson, J. P., Gonzalez-Solares, E., Hempel, M., Saito, R. K., Gurovich, S., Roman-Lopes, A., Moni-Bidin, C., Santucho, M. V., Borissova, J., Kurtev, R., Toledo, I., Geisler, D., Dominguez, M., and Beamin, J. C.
Subjects: Astrophysics - Galaxy Astrophysics
Abstract: The new multi-epoch near-infrared VVV survey (VISTA Variables in the Via Lactea) is sampling 562 sq. deg of the Galactic bulge and adjacent regions of the disk. Accurate astrometry established for the region surveyed allows the VVV data to be merged with overlapping surveys (e.g., GLIMPSE, WISE, 2MASS, etc.), thereby enabling the construction of longer baseline spectral energy distributions for astronomical targets. However, in order to maximize use of the VVV data, a set of transformation equations are required to place the VVV JHKs photometry onto the 2MASS system. The impetus for this work is to develop those transformations via a comparison of 2MASS targets in 152 VVV fields sampling the Galactic disk. The transformation coefficients derived exhibit a reliance on variables such as extinction. The transformed data were subsequently employed to establish a mean reddening law of E_{J-H}/E_{H-Ks}=2.13 +/- 0.04, which is the most precise determination to date and merely emphasizes the pertinence of the VVV data for determining such important parameters., Comment: 24 pages, 12 figures, published in A&A
Published: 2013
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44. Evidence of d-wave Superconductivity in K_(1-x)Na_xFe_2As_2 (x = 0, 0.1) Single Crystals from Low-Temperature Specific Heat Measurements

Author: Abdel-Hafiez, M., Grinenko, V., Aswartham, S., Morozov, I., Roslova, M., Vakaliuk, O., Johnston, S., Efremov, D. V., Brink, J. van den, Rosner, H., Kumar, M., Hess, C., Wurmehl, S., Wolter, A. U. B., Buechner, B., Green, E. L., Wosnitza, J., Vogt, P., Reifenberger, A., Enss, C., Klingeler, R., Hempel, M., and Drechsler, S. -L.
Subjects: Condensed Matter - Superconductivity
Abstract: From the measurement and analysis of the specific heat of high-quality K_(1-x)Na_xFe_2As_2 single crystals we establish the presence of large T^2 contributions with coefficients alpha_sc ~ 30 mJ/mol K^3 at low-T for both x=0 and 0.1. Together with the observed square root field behavior of the specific heat in the superconducting state both findings evidence d-wave superconductivity on almost all Fermi surface sheets with an average gap amplitude of Delta_0 in the range of 0.4 - 0.8 meV. The derived Delta_0 and the observed T_c agree well with the values calculated within the Eliashberg theory, adopting a spin-fluctuation mediated pairing in the intermediate coupling regime., Comment: 8 pages, 5 figures, field dependence of the specific heat added, slightly changed title, changed sequence of authors, one author added, accepted by Phys. Rev. B Rapid Communications
Published: 2013
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45. A comparative study of statistical models for nuclear equation of state of stellar matter

Author: Buyukcizmeci, N., Botvina, A. S., Mishustin, I. N., Ogul, R., Hempel, M., Schaffner-Bielich, J., Thielemann, F. -K., Furusawa, S., Sumiyoshi, K., Yamada, S., and Suzuki, H.
Subjects: Nuclear Theory, Astrophysics - Solar and Stellar Astrophysics, Nuclear Experiment
Abstract: We compare three different statistical models for the equation of state (EOS) of stellar matter at subnuclear densities and temperatures (0.5-10 MeV) expected to occur during the collapse of massive stars and supernova explosions. The models introduce the distributions of various nuclear species in nuclear statistical equilibrium, but use somewhat different nuclear physics inputs. It is demonstrated that the basic thermodynamical quantities of stellar matter under these conditions are similar, except in the region of high densities and low temperatures. We demonstrate that mass and isotopic distributions have considerable differences related to the different assumptions of the models on properties of nuclei at these stellar conditions. Overall, the three models give similar trends, but the details reflect the uncertainties related to the modeling of medium effects, such as the temperature and density dependence of surface and bulk energies of heavy nuclei, and the nuclear shell structure effects. We discuss importance of new physics inputs for astrophysical calculations from experimental data obtained in intermediate energy heavy-ion collisions, in particular, the similarities of the conditions reached during supernova explosions and multifragmentation reactions., Comment: 52 pages including 24 figures, accepted to Nucl.Phys. A
Published: 2012
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46. Milky Way demographics with the VVV survey. I. The 84-million star colour-magnitude diagram of the Galactic bulge

Author: Saito, R. K., Minniti, D., Dias, B., Hempel, M., Rejkuba, M., Alonso-Garcia, J., Barbuy, B., Catelan, M., Emerson, J. P., Gonzalez, O. A., Lucas, P. W., and Zoccali, M.
Subjects: Astrophysics - Galaxy Astrophysics
Abstract: The Milky Way (MW) bulge is a fundamental Galactic component for understanding the formation and evolution of galaxies, in particular our own. The ESO Public Survey VISTA Variables in the Via Lactea is a deep near-IR survey mapping the Galactic bulge and southern plane. Data taken during 2010-11 covered 315 deg2 in the bulge area in the JHKs bands. We used VVV data for the whole bulge area as a single and homogeneous data set to build for the first time a single colour-magnitude diagram (CMD) for the entire Galactic bulge. Photometric data in the JHKs bands were combined to produce a single and huge data set containing 173.1M+ sources in the three bands. Selecting only the data points flagged as stellar, the total number of sources is 84.0M+. We built the largest CMDs published up to date, containing 173.1+ million sources for all data points, and more than 84.0 million sources accounting for the stellar sources only. The CMD has a complex shape, mostly owing to the complexity of the stellar population and the effects of extinction and reddening towards the Galactic centre. The red clump (RC) giants are seen double in magnitude at b ~ -8-10 deg, while in the inner part (b ~ 3deg) they appear to be spreading in colour, or even splitting into a secondary peak. The analysis of the outermost bulge area reveals a well-defined sequence of late K and M dwarfs, seen at (J-Ks) ~ 0.7-0.9 mag and Ks~14 mag. The interpretation of the CMD yields important information about the MW bulge, showing the fingerprint of its structure and content. We report a well-defined red dwarf sequence in the outermost bulge, which is important for the planetary transit searches of VVV. The double RC in magnitude seen in the outer bulge is the signature of the X-shaped MW bulge, while the spreading of the RC in colour are caused by reddening effects., Comment: 10 pages, 8 figures
Published: 2012
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47. Deconfinement to Quark Matter in Neutron Stars - The Influence of Strong Magnetic Fields

Author: Dexheimer, V., Negreiros, R., Schramm, S., and Hempel, M.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics, Nuclear Theory
Abstract: We use an extended version of the hadronic SU(3) non-linear realization of the sigma model that also includes quarks to study hybrid stars. Within this approach, the degrees of freedom change naturally as the temperature/density increases. Different prescriptions of charge neutrality, local and global, are tested and the influence of strong magnetic fields and the anomalous magnetic moment on the particle population is discussed., Comment: To appear in the proceedings of conference XII HADRON PHYSICS April, 22-27, 2012, Bento Goncalves, Wineyards Valley Region, Rio Grande do Sul, Brazil Revised version with corrections made to the text in page 4
Published: 2012
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48. Strange matter in core-collapse supernovae

Author: Sagert, I., Fischer, T., Hempel, M., Pagliara, G., Schaffner-Bielich, J., Thielemann, F. -K., and Liebendörfer, M.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We discuss the possible impact of strange quark matter on the evolution of core-collapse supernovae with emphasis on low critical densities for the quark-hadron phase transition. For such cases the hot proto-neutron star can collapse to a more compact hybrid star configuration hundreds of milliseconds after core-bounce. The collapse triggers the formation of a second shock wave. The latter leads to a successful supernova explosion and leaves an imprint on the neutrino signal. These dynamical features are discussed with respect to their compatibility with recent neutron star mass measurements which indicate a stiff high density nuclear matter equation of state., Comment: 8 pages, 3 figures, Invited talk at the "Strangeness in Quark Matter" conference, 18-24 September 2011, Polish Academy of Arts and Sciences, Cracow, Poland
Published: 2011
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49. Neutrino spectra evolution during proto-neutron star deleptonization

Author: Fischer, T., Martínez-Pinedo, G., Hempel, M., and Liebendörfer, M.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: The neutrino-driven wind, which occurs after the onset of a core-collapse supernova explosion, has long been considered as the possible site for the synthesis of heavy r-process elements in the Universe. Only recently, it has been possible to simulate supernova explosions up to ~10 seconds, based on three-flavor Boltzmann neutrino transport. These simulations show that the neutrino luminosities and spectra of all flavors are very similar and their difference even decreases during the deleptonization of the proto-neutron star. As a consequence, the ejecta are always proton rich which rules out the possible production of heavy r-process elements (Z>56). We perform a detailed analysis of the different weak processes that determine the neutrino spectra. Non-electron flavor (anti)neutrinos are produced and interact only via neutral-current processes, while electron (anti)neutrinos have additional contributions from charge-current processes. The latter are dominated by ve absorption on neutrons and anti-ve absorption on protons. At early times, charge-current processes are responsible for spectral differences between. However, as the region of neutrino decoupling moves to higher densities during deleptonization, charge-current reactions are suppressed by final state Pauli-blocking. anti-ve absorption on protons is suppressed due to the continuously increasing chemical potential of the neutrons. ve absorption on neutrons is blocked by the increasing degeneracy of the electrons. These effects result in negligible contributions from charge-current reactions on timescales on the order of tens of seconds, depending on the progenitor star. Hence, the neutrino spectra are mainly determined from neutral-current processes which do not distinguish between the different flavors and results in the convergence of the spectra. These findings are independent of the charge-current reaction rates used..., Comment: 18 pages, 10 figures, 1 table, submitted to PRD
Published: 2011
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50. VVV DR1: The First Data Release of the Milky Way Bulge and Southern Plane from the Near-Infrared ESO Public Survey VISTA Variables in the Via Lactea

Author: Saito, R. K., Hempel, M., Minniti, D., Lucas, P. W., Rejkuba, M., Toledo, I., Gonzalez, O. A., Alonso-Garcia, J., Irwin, M. J., Gonzalez-Solares, E., Hodgkin, S. T., Lewis, J. R., Cross, N., Ivanov, V. D., Kerins, E., Emerson, J. P., Soto, M., Amores, E. B., Gurovich, S., Dekany, I., Angeloni, R., Beamin, J. C., Catelan, M., Padilla, N., Zoccali, M., Pietrukowicz, P., Bidin, C. Moni, Mauro, F., Geisler, D., Folkes, S. L., Sale, S. E., Borissova, J., Kurtev, R., Ahumada, A. V., Alonso, M. V., Adamson, A., Arias, J. I., Bandyopadhyay, R. M., Barba, R. H., Barbuy, B., Baume, G. L., Bedin, L. R., Bellini, A., Benjamin, R., Bica, E., Bonatto, C., Bronfman, L., Carraro, G., Chene, A. N., Claria, J. J., Clarke, J. R. A., Contreras, C., Corvillon, A., de Grijs, R., Dias, B., Drew, J. E., Farina, C., Feinstein, C., Fernandez-Lajus, E., Gamen, R. C., Gieren, W., Goldman, B., Gonzalez-Fernandez, C., Grand, R. J. J., Gunthardt, G., Hambly, N. C., Hanson, M. M., Helminiak, K. G., Hoare, M. G., Huckvale, L., Jordan, A., Kinemuchi, K., Longmore, A., Lopez-Corredoira, M., Maccarone, T., Majaess, D., Martin, E. L., Masetti, N., Mennickent, R. E., Mirabel, I. F., Monaco, L., Morelli, L., Motta, V., Palma, T., Parisi, M. C., Parker, Q., Penaloza, F., Pietrzynski, G., Pignata, G., Popescu, B., Read, M. A., Rojas, A., Roman-Lopes, A., Ruiz, M. T., Saviane, I., Schreiber, M. R., Schroder, A. C., Sharma, S., Smith, M. D., Sodre Jr., L., Stead, J., Stephens, A. W., Tamura, M., Tappert, C., Thompson, M. A., Valenti, E., Vanzi, L., Walton, N. A., Weidmann, W., and Zijlstra, A.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The ESO Public Survey VISTA Variables in the Via Lactea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for ~5 years. In this paper we describe the progress of the survey observations in the first observing season, the observing strategy and quality of the data obtained. The observations are carried out on the 4-m VISTA telescope in the ZYJHKs filters. In addition to the multi-band imaging the variability monitoring campaign in the Ks filter has started. Data reduction is carried out using the pipeline at the Cambridge Astronomical Survey Unit. The photometric and astrometric calibration is performed via the numerous 2MASS sources observed in each pointing. The first data release contains the aperture photometry and astrometric catalogues for 348 individual pointings in the ZYJHKs filters taken in the 2010 observing season. The typical image quality is ~0.9-1.0". The stringent photometric and image quality requirements of the survey are satisfied in 100% of the JHKs images in the disk area and 90% of the JHKs images in the bulge area. The completeness in the Z and Y images is 84% in the disk, and 40% in the bulge. The first season catalogues contain 1.28x10^8 stellar sources in the bulge and 1.68x10^8 in the disk area detected in at least one of the photometric bands. The combined, multi-band catalogues contain more than 1.63x10^8 stellar sources. About 10% of these are double detections due to overlapping adjacent pointings. These overlapping multiple detections are used to characterise the quality of the data. The images in the JHKs bands extend typically ~4 mag deeper than 2MASS. The magnitude limit and photometric quality depend strongly on crowding in the inner Galactic regions. The astrometry for Ks=15-18 mag has rms ~35-175 mas., Comment: Accepted for publication in Astronomy and Astrophysics (Section 14: Catalogs and data)
Published: 2011
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