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206 results on '"L. Guglielmi"'

2. Immediate use steam sterilization optimization and a methodology to forecast and justify instrumentation

Author

Elena Canacari, Ross W. Simon, Ryan Graue, Barbara L. DiTullio, and Charlotte L. Guglielmi

Subjects
Process (engineering), Computer science, Critical Care and Intensive Care Medicine, Sustainable process, Purchasing, Steam sterilization, Health administration, 03 medical and health sciences, Medical–Surgical Nursing, 0302 clinical medicine, Anesthesiology and Pain Medicine, Risk analysis (engineering), 030202 anesthesiology, Surgical site, Strategic decision making, Surgery, 030212 general & internal medicine, Instrumentation (computer programming)
Abstract

Background During the past two decades, the escalating rate of immediate use steam sterilization (IUSS) well beyond its intended use has become an area of intense focus as greater understanding of the link between IUSS and Surgical Site Infections (SSI) has emerged. Methods While in the process of completing an initial project, a team at Beth Israel Deaconess Medical Center developed a methodology that evolved into a framework used to determine instrument and kit requirements for various purposes. Results Most importantly, the tools and framework provide a reliable, sustainable process for providing exceptional patient care in the use, care, and cleaning of instrumentation for surgical procedures. Just as importantly, the framework has provided perioperative leadership at BIDMC with a way to evaluate the ongoing instrumentation needs and to assess, consider and justify budget expenses with a process that provides confidence and justification of expenditures to hospital administration. Conclusions With continued use, BIDMC has come to rely on the process and framework to provide insight, guide strategic decision making, and realize cost avoidance by making smart instrument purchasing decisions rather than buying more than needed when estimating usage.

Published
2021
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3. Effectively Processing Flexible Endoscopes

Author

Ellen K. Murphy, Linda K. Groah, Charlotte L. Guglielmi, Debra L. Fawcett, Cynthia Spry, Judith L. Goldberg, and Debra Martinez

Subjects
Endoscopes, 0301 basic medicine, Database, Computer science, 030106 microbiology, MEDLINE, Equipment Design, computer.software_genre, Disinfection, 03 medical and health sciences, Medical–Surgical Nursing, 0302 clinical medicine, Equipment Reuse, Equipment Contamination, Humans, 030212 general & internal medicine, computer
Published
2016
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4. Eliminating workplace hazards in the OR

Author

Barbara L. DiTullio, Ross W. Simon, Charlotte L. Guglielmi, Elena Canacari, and Lisa A. Foster

Subjects
Engineering, 030504 nursing, business.industry, Job safety analysis, Direct observation, Critical Care and Intensive Care Medicine, 03 medical and health sciences, Medical–Surgical Nursing, 0302 clinical medicine, Anesthesiology and Pain Medicine, Work (electrical), Industry sector, Cause and effect analysis, Hazardous waste, SAFER, Health care, Surgery, Operations management, 030212 general & internal medicine, 0305 other medical science, business
Abstract

Healthcare workplaces are among the most hazardous in the nation. In 2010, the Department of Labor reported 653,900 workplace injuries/illnesses occurred in healthcare, 152,000 more than the next most afflicted industry sector, manufacturing. A team from Beth Israel Deaconess Medical Center, Boston, MA adapted techniques used in industry to make the OR a safer place to work through formal observations of work performed and subsequent mitigation of recognized hazards. To help guide observations, the team identified critical safe behaviors and hazardous conditions in the OR using injury data, input from a staff survey, job safety analysis, direct observation and cause and effect analysis. An observation tool from industry was customized to address hazards unique to the healthcare environment such as sharps safety. Implementation of the process has been so successful in reducing or eliminating identified hazards, which led to a 68% reduction in days away from work due to injury in the east campus operating suite, that it is being spread to other areas of the hospital including Central Processing and Environmental Services.

Published
2016
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5. New Strategies to Assert the Value of the Perioperative Nurse

Author

Ellen K. Murphy, Jacque A. Crosson, Patricia C. Seifert, Angela J. Wright, Charlotte L. Guglielmi, Linda K. Groah, Pamela E. Windle, Gregory L. Lara, and William J. Duffy

Subjects
Medical–Surgical Nursing, medicine.medical_specialty, Perioperative nursing, business.industry, Perioperative Nursing, Societies, Nursing, Humans, Medicine, business, Intensive care medicine, Value (mathematics), United States
Published
2015
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7. Hand-held Communication Devices: Friend or Foe?

Author

Linda K. Groah, Susan K. Banschbach, Ross W. Simon, Jonathan Dort, Brian Ferla, and Charlotte L. Guglielmi

Subjects
Medical–Surgical Nursing, Microcomputers, Attitude of Health Personnel, Attitude to Computers, business.industry, Communication, Internet privacy, Hand held, Humans, business, United States
Published
2013
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8. Auger at the Telescope Array: Recent Progress Toward a Direct Cross-Calibration of Surface-Detector Stations

Author

R. Cady, P. Mantsch, R. Halliday, Toshiyuki Nonaka, L. Guglielmi, Corbin Covault, John Matthews, T. Trung, Fred Sarazin, Ryan Lorek, P. Lebrun, S. Colognes, B. Genolini, Hiroyuki Sagawa, E. Rauly, Ricardo Sato, B. Courty, John N. Matthews, Shoichi Ogio, M. Marton, O. Wolf, R. Takeishi, P.O. Mazur, Jeffrey A. Johnsen, S. Quinn, Toshihiro Fujii, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Pierre Auger, Telescope Array, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)

Subjects
air, data acquisition, Auger, law.invention, detector: fluorescence, Telescope, Data acquisition, Observatory, law, Calibration, hardware, (cross) calibration, Remote sensing, Pierre Auger Observatory, Physics, instrumentation, cosmic radiation: energy spectrum, hybrid, showers: atmosphere, detector: surface, Detector, sensitivity, calibration, laser, observatory, Central Laser Facility, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; Since 2007 the Telescope Array Project (TA) and the Pierre Auger Observatory (Auger) have collected extensive data sets spanning several orders of magnitude in energy of the cosmic-ray spectrum. In both experiments the bulk of data is generated from the surface-detector (SD) array, which is energetically calibrated with fluorescence detectors using a hybrid approach. However, each experiment has implemented a different SD station design, resulting in different sensitivities of extensive air-shower channels. Understanding these differences and any potential unforeseen systematic errors is essential for future joint analyses. In this paper we present an update on the progress of an in-situ cross-calibration program. We focus on recent hardware installations which enable the read out of co-located Auger and TA SD stations at the TA central laser facility (CLF). We also present a preliminary analysis of event signals observed at the CLF.

Published
2016
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10. The Difficulty With Implementing a Policy on Surgical Attire

Author

Linda K. Groah, Barbara L. DiTullio, Charlotte L. Guglielmi, Claire Everson, Richard A. Beers, Heather Hohenberger, Beverly Kirchner, and Amy L. Halverson

Subjects
business.industry, Health Personnel, 030501 epidemiology, medicine.disease, Organizational Policy, Management, 03 medical and health sciences, Medical–Surgical Nursing, 0302 clinical medicine, medicine, Humans, Surgical Attire, 030212 general & internal medicine, Medical emergency, 0305 other medical science, business
Published
2016

11. Intensity and polarization of the atmospheric emission at millimetric wavelengths at Dome Concordia

Author

F. Piacentini, Giampaolo Pisano, Maria Salatino, M. Maiello, A. Cruciani, R. Charlassier, E. Bréelle, Bruno Maffei, G. Amico, A. Baù, Y. Giraud-Héraud, M. Giard, L. Dumoulin, L. Bergé, A. Passerini, P. de Bernardis, Elia S. Battistelli, Alessandro Schillaci, M. Piat, Andrea Tartari, Roberto Sordini, Massimo Gervasi, C. Giordano, C. Dufour, Jean-Christophe Hamilton, L. Guglielmi, Lucio Piccirillo, Silvia Masi, C. Rosset, S. Spinelli, S. Marnieros, J. Landé, Sophie Collin, Mario Zannoni, and Gianluca Polenta

Subjects
Physics, Linear polarization, Astronomy and Astrophysics, Astrophysics, Polarization (waves), 01 natural sciences, 010309 optics, Atmosphere, Dome (geology), Wavelength, 13. Climate action, Space and Planetary Science, 0103 physical sciences, Radiative transfer, 010303 astronomy & astrophysics, Optical depth, Circular polarization
Abstract

Atmospheric emission is a dominant source of disturbance in ground-based astronomy at mm wavelengths. The Antarctic plateau is recognized to be an ideal site for mm and sub-mm observations, and the French/Italian base of Dome C is among the best sites on Earth for these observations. In this paper we present measurements, performed using the BRAIN-pathfinder experiment, at Dome C of the atmospheric emission in intensity and polarization at 150GHz, one of the best observational frequencies for CMB observations when considering cosmic signal intensity, atmospheric transmission, detectors sensitivity, and foreground removal. Careful characterization of the air-mass synchronous emission has been performed, acquiring more that 380 elevation scans (i.e. "skydip") during the third BRAIN-pathfinder summer campaign in December 2009/January 2010. The extremely high transparency of the Antarctic atmosphere over Dome Concordia is proven by the very low measured optical depth: =0.050 \pm 0.003 \pm 0.011 where the first error is statistical and the second is systematic error. Mid term stability, over the summer campaign, of the atmosphere emission has also been studied. Adapting the radiative transfer atmosphere emission model "am" to the particular conditions found at Dome C, we also infer the level of the PWV content of the atmosphere, notoriously the main source of disturbance in millimetric astronomy ( =0.77 +/- 0.06 + 0.15 - 0.12 mm). Upper limits on the air-mass correlated polarized signal are also placed for the first time. The degree of circular polarization of atmospheric emission is found to be lower than 0.2% (95%CL), while the degree of linear polarization is found to be lower than 0.1% (95%CL). These limits include signal-correlated instrumental spurious polarization.

Published
2012
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14. Design and Impact of an Intraoperative Pathway: A New Operating Room Model for Team-Based Practice

Author

Bernard T. Lee, Donald W. Moorman, Lynn M. Darrah, Charlotte L. Guglielmi, Elizabeth R. Wood, Adam M. Tobias, Eran Bar-Meir, Justine M. Carr, and Janet H. Yueh

Subjects
Microsurgery, Operating Rooms, medicine.medical_specialty, Time Factors, Mammaplasty, medicine.medical_treatment, MEDLINE, Professional practice, Efficiency, Organizational, Multidisciplinary team, Surgical Flaps, DIEP flap, medicine, Humans, Hospital Costs, Patient Care Team, business.industry, General surgery, Length of Stay, Middle Aged, Surgery, Staff satisfaction, Critical Pathways, Operative time, Female, Breast reconstruction, business
Abstract

The concept of a team-based model for delivery of care has been critical at our institution for improving efficiency and safety. Despite these measures, difficulties continue to occur during lengthy operating room procedures. Using a novel team-based practice model, a multidisciplinary team was organized to improve efficiency in microsurgical breast reconstruction. We describe development of an intraoperative pathway for deep inferior epigastric perforator (DIEP) flap breast reconstruction and its impact on various outcomes.We evaluated 150 patients who underwent DIEP flap breast reconstruction at Beth Israel Deaconess Medical Center from 2005 to 2008. Patient groups were subdivided into 50 unilateral and 50 bilateral procedures before the intraoperative pathway and 25 unilateral and 25 bilateral procedures after. Outcomes measured included operative time, complications, operating room and hospital costs, proper administration of prophylactic antibiotics and heparin, and staff satisfaction surveys.Mean operative times decreased after pathway implementation in both unilateral (8.2 hours to 6.9 hours; p0.001) and bilateral groups (12.8 hours to 10.6 hours; p0.001) and complication rates were unchanged. Mean operating room costs decreased in the unilateral group by 10.2% (p = 0.018). Prophylactic heparin administration showed substantial improvements, although antibiotic administration and redosing of antibiotics trended upward. Staff surveys showed improved interdisciplinary communication, transition guidelines, and enhanced efficiency through standardization.Implementation of an intraoperative pathway led to improvements in operative time, cost, quality measures, and staff satisfaction. Refinement of the pathway with team resolution of variances might continue to improve outcomes. Complex, multi-team procedures can derive benefits from standardization and intraoperative pathway development.

Published
2008
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15. Initial results of a direct comparison between the Surface Detectors of the Pierre Auger Observatory and of the Telescope Array

Author

Jeffrey A. Johnsen, R. Takeishi, B. Genolini, C. Covault, P. Mantsch, T. Trung, Fred Sarazin, R. Sato, S. Ogio, P. Mazur, R. Cady, E. Rauly, P. Lebrun, B. Courty, J.N. Matthews, O. Wolf, T. Nonaka, L. Smith, M. Marton, S. Collonges, Ryan Lorek, T. Fujii, J.A.J. Matthews, H. Sagawa, L. Guglielmi, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Telescope Array, Pierre Auger, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])

Subjects
Pierre Auger Observatory, Physics, Cherenkov detector, detector: surface, Telescope Array Experiment, Detector, Cosmic ray, Astrophysics, Coincidence, Auger, law.invention, Telescope, observatory, 13. Climate action, law, Observatory, muon, cosmic radiation: UHE, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

The Pierre Auger Observatory (Auger) in Mendoza, Argentina and the Telescope Array (TA) in Utah, USA aim at unraveling the origin and nature of Ultra-High Energy Cosmic Rays (UHECR). At present, there appear to be subtle differences between Auger and TA results and interpretations. Joint working groups have been established and have already reported preliminary findings. From an experimental standpoint, the Surface Detectors (SD) of both experiments makes use of different detection processes not equally sensitive to the components of the extensive air showers making it to the ground. In particular, the muonic component of the shower measured at ground level can be traced back to the primary composition, which is critical for understanding the origin of UHECRs. In order to make direct comparisons between the SD detection techniques used by Auger and TA, a two-phase approach is followed. First, one water Cherenkov detector (“Auger North” design) was deployed and operated locally at the TA Central Laser Facility. After a couple of months of operation before the summer, we expect to observe about 20 Auger SD events in coincidence with nearby TA stations. And a regular Auger station and a TA station will be added to the setup to allow for station-level comparisons. In a second phase, event-level comparisons of relatively low-energy showers with energies in the 1018 eV range will be possible as a result of co-locating six additional Auger North stations contiguous to TA surface detector stations. In this contribution, we present the status and prospects of this joint research project, including the first Auger SD data that were recorded in coincidence with the TA SD shower triggers.

Published
2015
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16. The Pierre Auger cosmic ray observatory

Author

A. Haungs, F. Diogo, R. M. de Almeida, J. L. Harton, Harm Schoorlemmer, F. Arneodo, Stijn Buitink, S. Westerhoff, Z. Szadkowski, F. Salamida, Carola Dobrigkeit, M. Plum, M. Chiosso, M. E. Bertaina, S. G. Blaes, Alan Watson, J. Alvarez Castillo, D. Nicotra, Paul Sommers, P. Gouffon, M. J. Cooper, Dragos Varnav, C. Aramo, Carlos Medina, M. De Domenico, M. Sutter, Maria Rita Coluccia, Bruno Daniel, Q. Dorosti Hasankiadeh, T. Yapici, Foteini Oikonomou, J. J. Masías Meza, D. Maurel, Luis Villaseñor, P. Abreu, D. Ravignani, Yingchun Zhu, B. Mitrica, Heino Falcke, J. Vicha, G. Cocciolo, B. Genolini, Luis A. Anchordoqui, M. Ambrosio, G. S. Varner, H. Gemmeke, M. Monasor, M. Iarlori, C. E. Santo, L. Martina, Yogendra N. Srivastava, Andreas Kopmann, E. J. Ahn, V. Tunnicliffe, A. F. Barbosa, Dusan Mandat, Martina Bohacova, Patrick Allison, E. Varela, N. Griffith, J. Sorokin, M. Boratav, B. Revenua, T. Porter, G. Torralba Elipe, A. Gorgi, Peter Schiffer, Benedikt Zimmermann, Rúben Conceição, R. Vasquez, Pascal Lautridou, D. V. Camin, Luis N. Epele, M. Blanco, V. Scherini, Alexandra Saftoiu, O. Kambeitz, H. Martinez, A. Di Matteo, N. Martínez, N. Palmieri, B. Wundheiler, D. Nitz, I. Lhenry-Yvon, Eva Santos, R. Krause, Vincent Marin, P. Walker, Gregory R Snow, Jan Pękala, A. Chiavassa, A. Menshikov, R. Habraken, M. S. A. B. Leão, J. D. Swain, Philipp Papenbreer, Petr Travnicek, John Kelley, S. Mueller, R. Bilhaut, Alan Coleman, M. Roberts, L. Ochilo, Federico Suarez, L. Valore, Amin Aminaei, A. E. Herve, K. B. Barber, L. R. Wiencke, K. Weidenhaupt, C. O. Escobar, A. Insolia, M. Kleifges, D. Zavrtanik, Trent D. Grubb, D. Huber, L. Nellen, Juan Manuel Figueira, A. Dorofeev, M. Melissas, Peter Mazur, Thomas Hebbeker, Joshua A. Gordon, R. A. Vázquez, A. Schmidt, Sergio Dasso, Denis Tcherniakhovski, Roberta Colalillo, John N. Matthews, R. M. Kieckhafer, A. G. Mariazzi, Igor Katkov, M. Muenchmeyer, V. Novotny, A. F. Grillo, G. P. Guedes, Rossella Caruso, Toshihiro Fujii, G. Sequeiros, J. Rautenberg, A. Lucero, J. R. Hoerandel, F. Sanchez, O. Wainberg, Stefano Argiro, S. Mathys, C. Morello, K. D. de Vries, Matthias Balzer, J. A.J. Matthews, F. Schreuder, F. Sarazin, W. Fulgione, W. C. Brown, Patricia María Hansen, Richard Dallier, A. Nelles, M. Erfani, L. Molina-Bueno, D. Melo, H. Verkooijen, T. Pierog, Marco Giammarchi, T. Ohnuki, David Walz, V. Pirronello, J. F. Valdés Galicia, I. De Mitri, A. Gascon Bravo, Iuri Muniz Pepe, Jaime Alvarez-Muñiz, Pedro Assis, A. Etchegoyen, Esteban Roulet, R. Randriatoamanana, C. Jarne, A. Stutz, P. L. Ghia, J. N. Albert, M. Horvat, Marco Cilmo, Arnulfo Zepeda, Alberto Daniel Supanitsky, Lu Lu, R. Sato, Octavian Sima, J. G. Gonzalez, A. Tepe, Dariusz Gora, Peter L. Biermann, R. Mussa, J. J. Beatty, Manuel Platino, J. Grygar, M. A. Leigui de Oliveira, F. Schroeder, Jeffrey A. Johnsen, F. Werner, J. Knapp, J. R. Vázquez, D. Garcia-Gamez, S. Quinn, D. PakkSelmi-Dei, G. Matthiae, T. Rossler, A. Bridgeman, Antonio Bueno, A. Segreto, Günter Sigl, Silvia Mollerach, J. Coppens, Markus Roth, H. Dembinski, H. Vorenholt, I. A. Minaya, B. Keilhauer, E. Petermann, S. J. Saffi, T. Wijnen, P. Sanchez-Lucas, G. Garilli, D. Maurizio, D. Garcia-Pinto, M. Risse, Paolo Privitera, H. Hucker, J. Allen, André Schulz, P. Kasper, S. J. Sciutto, Radomir Smida, Kai Daumiller, G. Mueller, D. Heck, R. Meyhandan, V. Purrello, M. Josebachuili, J. C. Diaz, Alberto Filevich, F. Guarino, Lorenzo Caccianiga, V. M. Theodoro, S. Colonges, B. D. Fox, Markus Lauscher, B. Zamorano, J. Pouryamout, A. Ferrero, Julien Aublin, A. Shadkam, F. Bracci, Florian Gaté, G. Parente, J. Phuntsok, Raul Sarmento, Carlos Hojvat, O. Kroemer, S. J. De Jong, Marcio Aparecido Muller, Peter Buchholz, M. M. Freire, Jeffrey Brack, Olaf Scholten, T. N. Trung, Humberto Ibarguen Salazar, V. de Souza, A. Curutiu, S. Sánchez Navas, T. Asch, H. J. Mathes, Jose Chinellato, Gualberto Avila, Ingomar Allekotte, A. van Vliet, M. Szuba, Eric Mayotte, I.M. Brancus, B. Tome, C. De Donato, Miguel Mostafa, B. Wilczynska, M. Candusso, Peter Gorham, N.R. Wild, Alina Mihaela Badescu, D. Rogozin, J. de Oliveira, A. Widom, M. Gómez Berisso, N. Kunka, R. C. Shellard, Alejandro Almela, W. Docters, M. Oliveira, L. Tomankova, G. Navarra, B. Vlcek, A. López Casado, C. A. Moura, T. Yamamoto, Brian Fick, Ugo Giaccari, Charles Timmermans, J. Lozano Bahilo, Segev BenZvi, A. Letessier-Selvon, M. Prouza, A. Smialkowski, I. Al Samarai, L. Voyvodic, Sasa Micanovic, Angela V. Olinto, C. Di Giulio, Samo Stanič, H. M. Spinka, F. Montanet, M. Patel, L. Collica, J. Rodriguez Rojo, Marco Aglietta, Corbin Covault, Y. Petrov, C. D'Olivo, Lorenzo Cazon, P. Dolron, E. Tusi, A. G. Chavez, Enrique Zas, Lino Miramonti, M. D. Rodríguez-Frías, Iván Sidelnik, E.M. Holt, Fernando Contreras, Johannes Schumacher, A. Saleh, S. Harmsma, L. Perrone, Jiri Chudoba, S. Robbins, Michael Unger, S. Jansen, M. Fernandes, J. R. T. de Mello Neto, A. G. K. Smith, Maria-Teresa Dova, M. R. Hampel, R. Alves Batista, G. C. Hill, D. Torres Machado, Miroslav Pech, Colin Baus, Thomas Harrison, Ralph Engel, J. Ridky, N. Barenthien, Pavel Horvath, P. Pieroni, H. Schieler, Sarka Wykes, Karl-Heinz Kampert, Antonella Castellina, Heiko Geenen, C. Pryke, Jing Zhou, F. Arqueros, P. Necesal, M. S. Sutherland, R. Meissner, B. Vargas Cárdenas, S. van Velzen, K. H. Becker, N. Guardone, L. Guglielmi, M. Videla, J. Pallotta, K. Louedec, David Wittkowski, M. Urban, A. C. Rovero, Paula Gina Isar, C. Bleve, E. J. Quel, Pedro Brogueira, F. Salesa Greus, T. Bergmann, G. Cataldi, A. Filipcic, Azadeh Keivani, Béatrice Fuchs, Niraj Dhital, Octavian Fratu, W. Gotink, I. Valiño, D. Lebrun, U. Froehlich, G. Salina, Danielle LaHurd, Olivier Deligny, Nicolás González, W. Rodrigues de Carvalho, Sofia Andringa, J. W. Cronin, R. Speelman, P. van Bodegom, P. Lebrun, K. Gibbs, M. Palatka, A. Aab, E. Colombo, L. Caramete, M. I. Micheletti, Vincenzo Rizi, D. Martello, M. Ziolkowski, V. B. B. Mello, O. Martínez Bravo, J. Neuser, D. D'Urso, Corinne Berat, M. Giller, G. Toma, van den Ad M Berg, Luca Latronico, Nataliia Borodai, N. Scharf, P. Heimann, W. Tkaczyk, A. C. Fauth, Lukas Middendorf, H. Bolz, E. Trovato, Diego Harari, Christine Peters, A. Horneffer, P. Petrinca, Jose A. Bellido, B. Gookin, E. Kemp, J. Stasielak, S. Coutu, Norberto Fazzini, Serguei Vorobiov, P. H. Nguyen, A. Tapia, E. M. Santos, Balázs Kégl, Jaime Rosado, Mariangela Settimo, Alexey Yushkov, Max Malacari, Bruce R. Dawson, Tim Huege, G. Rodriguez Fernandez, Piotr Homola, Hernán Asorey, S. Le Coz, R. Cester, P. Facal San Luis, C. Porowski, O. A. Taborda, F. Schuessler, A. Cordier, H. Bluemer, I. C. Mariş, Hernan Wahlberg, Denise Boncioli, German Ros, R. R. Prado, Libor Nozka, Marcus Niechciol, E. D. Fraenkel, A. Parra, R. J. Lauer, P. Ristori, V. M. Olmos-Gilbaja, B. Courty, B. García, R. Pelayo, S. Querchfeld, R. López, Karen S. Caballero-Mora, A. Castera, L. Niemietz, B. Caccianiga, N. Pacheco, A. Porcelli, Tim Niggemann, M. Mallamaci, M. Ludwig, S. Hartmann, Martin Erdmann, G. Yuan, M. L. Díaz Castro, G. Farrar, G. Vitali, Francesca Zuccarello, Roger W Clay, Maurice Stephan, Johannes Schulz, M. Ave, J. Pouthas, M. Pimenta, P. Clark, A. Tonachini, C. Bonifaz, J. Baeuml, Tobias Winchen, M. Zimbres Silva, P.F. Gómez Vitale, J. Stapleton, Giovanni Marsella, D. Nosek, A. Weindl, N. Hollon, V. Verzi, David Schmidt, Paulo J. S. Gonçalves, T. Suomijaervi, I. Jandt, Ralf Ulrich, Paul M. Mantsch, R. Piegaia, M. Zavrtanik, A. Kaeaepae, N. Giudice, K. Arisaka, H. Glass, V. M. Aranda, Petr Schovanek, J. Kleinfeller, M. Barkhausen, Daniel Kuempel, S. Maldera, Ivone F. M. Albuquerque, Ke Fang, Darko Veberič, R. Bonino, Marc Weber, M. Buscemi, M. Hrabovsky, Jan Ebr, Sergio Petrera, H.O. Klages, S. Messina, A. P. Ferguson, G. Woerner, C. J. Todero Peixoto, C. H. Wiebusch, J. Maller, N. Krohm, B. Sarkar, Christian Glaser, J. Espadanal, H. Wilczyński, P. Billoir, L. del Peral, M. Avenier, N. Awal, D. Martraire, S. Grebe, R. Squartini, T. Paul, Olivier Ravel, E. Menichetti, G. Medina-Tanco, G. van Aar, K. Link, Research unit Astroparticle Physics, Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina, the Australian Research Council, Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ), São Paulo Research Foundation (FAPESP) Grants # 2010/07359-6 and # 1999/05404-3, Ministério de Ciência e Tecnologia (MCT), Brazil, MSMT-CRLG13007, 7AMB14AR005, CZ.1.05/2.1.00/03.0058 and the Czech Science Foundation Grant 14-17501S, Czech Republic, Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS), Département Sciences de l׳Univers (SDU-INSU/CNRS),Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Württemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden-Württemberg, Germany, Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell׳Istruzione, dell׳Università e della Ricerca (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), CETEMPS Center of Excellence, Italy, Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico, Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands, National Centre for Research and Development, Grant nos. ERA-NET-ASPERA/01/11 and ERA-NET-ASPERA/02/11, National Science Centre, Grant nos. 2013/08/M/ST9/00322, and 2013/08/M/ST9/00728 and HARMONIA 5 – 2013/10/M/ST9/00062, Poland, Portuguese national funds and FEDER funds within COMPETE – Programa Operacional Factores de Competitividade through Fundação para a Ciencia e a Tecnologia, Portugal, Romanian Authority for Scientific Research ANCS, CNDI-UEFISCDI partnership projects nos. 20/2012 and nr.194/2012, project nos. 1/ASPERA2/2012 ERA-NET, PN-II-RU-PD-2011-3-0145-17, and PN-II-RU-PD-2011-3-0062, the Minister of National Education, Programme for research – Space Technology and Advanced Research – STAR, project number 83/2013, Romania, Slovenian Research Agency, Slovenia, Comunidad de Madrid, FEDER funds, Ministerio de Educación y Ciencia, Xunta de Galicia, Spain, Science and Technology Facilities Council, United Kingdom, Department of Energy, Contract no. DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107 and DE-SC0011689, National Science Foundation, Grant no. 0450696, The Grainger Foundation, USA, NAFOSTED, Vietnam, Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union 7th Framework Program, Grant no. PIRSES-2009-GA-246806, and UNESCO., Pierre AUGER, ANR-11-IDEX-0004,SUPER,Sorbonne Universités à Paris pour l'Enseignement et la Recherche(2011), European Project: 328826,EC:FP7:PEOPLE,FP7-PEOPLE-2012-IEF,AUGER2FUTURE(2013), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Irish Agriculture and Food Development Authority, Fiocruz Minas - René Rachou Research Center / Instituto René Rachou [Belo Horizonte, Brésil], Fundação Oswaldo Cruz (FIOCRUZ), Réseau International des Instituts Pasteur (RIIP)-Réseau International des Instituts Pasteur (RIIP), STMicroelectronics [Crolles] (ST-CROLLES), Dipartimento de Ingenieria Quimica y Quimica Inorganica, Universidad de Cantabria [Santander], Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Istituto Nazionale di Fisica Nucleare, Sezione di Catania (INFN), Università degli studi di Catania [Catania], Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire d'aérologie (LAERO), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Aab, A., Abreu, P., Aglietta, M., Ahn, E. J., Al Samarai, I., Albert, J. N., Albuquerque, I. F. M., Allekotte, I., Allen, J., Allison, P., Almela, A., Alvarez Castillo, J., Alvarez Muñiz, J., Alves Batista, R., Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Aramo, C., Aranda, V. M., Argirò, S., Arisaka, K., Arneodo, F., Arqueros, F., Asch, T., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Awal, N., Badescu, A. M., Balzer, M., Barber, K. B., Barbosa, A., Barenthien, N., Bäuml, J., Baus, C., Beatty, J. J., Becker, K. H., Bellido, J. A., Benzvi, S., Berat, C., Bergmann, T., Bertaina, M. E., Biermann, P. L., Bilhaut, R., Billoir, P., Blaess, S. G., Blanco, M., Bleve, C., Blümer, H., Boháčová, M., Bolz, H., Boncioli, D., Bonifazi, C., Bonino, R., Boratav, M., Borodai, N., Bracci, F., Brack, J., Brancus, I., Bridgeman, A., Brogueira, P., Brown, W. C., Buchholz, P., Bueno, A., Buitink, S., Buscemi, Mario, Caballero Mora, K. S., Caccianiga, B., Caccianiga, L., Camin, D., Candusso, M., Caramete, L., Caruso, R., Castellina, A., Castera, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. G., Chiavassa, A., Chinellato, J. A., Chiosso, M., Chudoba, J., Cilmo, M., Clark, P. D. J., Clay, R. W., Cocciolo, G., Colalillo, Roberta, Coleman, A., Collica, L., Colombo, E., Colonges, S., Coluccia, M. R., Conceiçáo, R., Contreras, F., Cooper, M. J., Coppens, J., Cordier, A., Courty, B., Coutu, S., Covault, C. E., Cronin, J., Curutiu, A., Dallier, R., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., De Almeida, R. M., De Domenico, M., De Donato, C., De Jong, S. J., De Mello Neto, J. R. T., De Mitri, I., De Oliveira, J., De Souza, V., De Vries, K. D., Del Peral, L., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Di Matteo, A., Diaz, J. C., Díaz Castro, M. L., Diogo, F., Dobrigkeit, C., Docters, W., D'Olivo, J. C., Dolron, P., Dorofeev, A., Dorosti Hasankiadeh, Q., Dova, M. T., D'Urso, D., Ebr, J., Engel, R., Epele, L. N., Erdmann, M., Erfani, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Facal San Luis, P., Falcke, H., Fang, K., Farrar, G., Fauth, A. C., Fazzini, N., Ferguson, A. P., Fernandes, M., Ferrero, A., Fick, B., Figueira, J. M., Filevich, A., Filipčič, A., Fox, B. D., Fraenkel, E. D., Fratu, O., Freire, M. M., Fröhlich, U., Fuchs, B., Fulgione, W., Fujii, T., García, B., Garcia Gamez, D., Garcia Pinto, D., Garilli, G., Gascon Bravo, A., Gate, F., Geenen, H., Gemmeke, H., Genolini, B., Ghia, P. L., Giaccari, U., Giammarchi, M., Gibbs, K., Giller, M., Giudice, N., Glass, H., Gómez Berisso, M., Gómez Vitale, P. F., Gonçalves, P., Gonzalez, J. G., González, N., Gookin, B., Góra, D., Gordon, J., Gorgi, A., Gorham, P., Gotink, W., Gouffon, P., Grebe, S., Griffith, N., Grillo, A. F., Grubb, T. D., Grygar, J., Guardone, N., Guarino, Fausto, Guedes, G. P., Guglielmi, L., Habraken, R., Hampel, M. R., Hansen, P., Harari, D., Harmsma, S., Harrison, T. A., Hartmann, S., Harton, J. L., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. E., Hill, G. C., Hojvat, C., Hollon, N., Holt, E., Homola, P., Hörandel, J. R., Horneffer, A., Horvat, M., Horvath, P., Hrabovský, M., Huber, D., Hucker, H., Huege, T., Iarlori, M., Insolia, A., Isar, P. G., Jandt, I., Jansen, S., Jarne, C., Johnsen, J. A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. H., Kasper, P., Katkov, I., Kégl, B., Keilhauer, B., Keivani, A., Kelley, J., Kemp, E., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Knapp, J., Kopmann, A., Krause, R., Krohm, N., Kröpmer, O., Kuempel, D., Kunka, N., La Hurd, D., Latronico, L., Lauer, R., Lauscher, M., Lautridou, P., Le Coz, S., Leão, M. S. A. B., Lebrun, D., Lebrun, P., Leiguide Oliveira, M. A., Letessier Selvon, A., Lhenry Yvon, I., Link, K., López, R., López Casado, A., Louedec, K., Lozano Bahilo, J., Lu, L., Lucero, A., Ludwig, M., Malacari, M., Maldera, S., Mallamaci, M., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. G., Marin, V., Mariş, I. C., Marsella, G., Martello, D., Martin, L., Martinez, H., Martinez, N., Martínez Bravo, O., Martraire, D., Masías Meza, J. J., Mathes, H. J., Mathys, S., Matthews, J., Matthews, J. A. J., Matthiae, G., Maurel, D., Maurizio, D., Mayotte, E., Mazur, P. O., Medina, C., Medina Tanco, G., Meissner, R., Melissas, M., Mello, V. B. B., Melo, D., Menichetti, E., Menshikov, A., Messina, S., Meyhandan, R., Mićanović, S., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Molina Bueno, L., Mollerach, S., Monasor, M., Montanet, F., Morello, C., Mostafá, M., Moura, C. A., Muller, M. A., Muller, G., Muller, S., Mussa, R., Navarra, G., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neuser, J., Nguyen, P. H., Nicotra, D., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Ochilo, L., Ohnuki, T., Oikonomou, F., Olinto, A., Oliveira, M., Olmos Gilbaja, V. M., Pacheco, N., Pakk Selmi Dei, D., Palatka, M., Pallotta, J., Palmieri, N., Papenbreer, P., Parente, G., Parra, A., Patel, M., Paul, T., Pech, M., Pȩkala, J., Pelayo, R., Pepe, I. M., Perrone, L., Petermann, E., Peters, C., Petrera, S., Petrinca, P., Petrov, Y., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porcelli, A., Porowski, C., Porter, T., Pouryamout, J., Pouthas, J., Prado, R. R., Privitera, P., Prouza, M., Pryke, C. L., Purrello, V., Quel, E. J., Querchfeld, S., Quinn, S., Randriatoamanana, R., Rautenberg, J., Ravel, O., Ravignani, D., Revenu, B., Ridky, J., Risse, M., Ristori, P., Rizi, V., Robbins, S., Roberts, M., Rodrigues De Carvalho, W., Rodriguez Fernandez, G., Rodriguez Rojo, J., Rodríguez Frías, M. D., Rogozin, D., Ros, G., Rosado, J., Rossler, T., Roth, M., Roulet, E., Rovero, A. C., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sánchez, F., Sanchez Lucas, P., Santo, C. E., Santos, E., Santos, E. M., Sarazin, F., Sarkar, B., Sarmento, R., Sato, R., Scharf, N., Scherini, V., Schieler, H., Schiffer, P., Schmidt, A., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovánek, P., Schreuder, F., Schröder, F. G., Schulz, A., Schulz, J., Schüssler, F., Schumacher, J., Sciutto, S. J., Segreto, A., Sequeiros, G., Settimo, M., Shadkam, A., Shellard, R. C., Sidelnik, I., Sigl, G., Sima, O., ͆miałkowski, A., Šmída, R., Smith, A. G. K., Snow, G. R., Sommers, P., Sorokin, J., Speelman, R., Spinka, H., Squartini, R., Srivastava, Y. N., Stanič, S., Stapleton, J., Stasielak, J., Stephan, M., Stutz, A., Suarez, F., Suomijärvi, T., Supanitsky, A. D., Sutherland, M. S., Sutter, M., Swain, J., Szadkowski, Z., Szuba, M., Taborda, O. A., Tapia, A., Tcherniakhovski, D., Tepe, A., Theodoro, V. M., Timmermans, C., Tkaczyk, W., Todero Peixoto, C. J., Toma, G., Tomankova, L., Tomé, B., Tonachini, A., Torralba Elipe, G., Torres Machado, D., Travnicek, P., Trovato, E., Trung, T. N., Tunnicliffe, V., Tusi, E., Ulrich, R., Unger, M., Urban, M., Valdés Galicia, J. F., Valiño, I., Valore, Laura, Van Aar, G., Van Bodegom, P., Van Den Berg, A. M., Van Velzen, S., Van Vliet, A., Varela, E., Vargas Cárdenas, B., Varnav, D. M., Varner, G., Vasquez, R., Vázquez, J. R., Vázquez, R. A., Veberič, D., Verkooijen, H., Verzi, V., Vicha, J., Videla, M., Villaseñor, L., Vitali, G., Vlcek, B., Vorenholt, H., Vorobiov, S., Voyvodic, L., Wahlberg, H., Wainberg, O., Walker, P., Walz, D., Watson, A. A., Weber, M., Weidenhaupt, K., Weindl, A., Werner, F., Westerhoff, S., Widom, A., Wiebusch, C., Wiencke, L., Wijnen, T., Wilczyńska, B., Wilczyński, H., Wild, N., Winchen, T., Wörner, G., Wundheiler, B., Wykes, S., Yamamoto, T., Yapici, T., Yuan, G., Yushkov, A., Zamorano, B., Zas, E., Zavrtanik, M., Zepeda, A., Zhou, J., Zhu, Y., Zimbres Silva, M., Zimmermann, B., Ziolkowski, M., Zuccarello, F., Ahn, E. . J., Albuquerque, I. . F. . M., Aranda, V. . M., Arsene, N., Badescu, A. . M., Barber, K. . B., Beatty, J. . J., Becker, K. . H., Bellido, J. . A., Bertaina, M. . E., Bertou, X., Biermann, P. . L., Blaess, S. . G., Blanco, A., Bleve, Carla, Brown, W. . C., Buscemi, M., Caballero Mora, K. . S., Chavez, A. . G., Chinellato, J. . A., Clay, R. . W., Colalillo, R., Coluccia, MARIA RITA, Conceição, R., Cooper, M. . J., Covault, C. . E., Dawson, B. . R., de Almeida, R. . M., de Jong, S. . J., De Mauro, G., de Mello Neto, J. . R. . T., DE MITRI, Ivan, de Oliveira, J., de Souza, V., del Peral, L., Diaz, J. . C., Díaz Castro, M. . L., D’Olivo, J. . C., Dova, M. . T., Escobar, C. . O., Fauth, A. . C., Ferguson, A. . P., Figueira, J. . M., Fox, B. . D., Freire, M. . M., Gherghel Lascu, A., Ghia, P. . L., Głas, D., Glaser, C., Golup, G., Gómez Vitale, P. . F., Grillo, A. . F., Grubb, T. . D., Guardincerri, Y., Guarino, F., Guedes, G. . P., Hampel, M. . R., Harrison, T. . A., Harton, J. . L., Herve, A. . E., Hill, G. . C., Hörandel, J. . R., Isar, P. . G., Johnsen, J. . A., Kampert, K. . H., Kieckhafer, R. . M., Klages, H. . O., Krömer, O., Lahurd, D., Leigui de Oliveira, M. . A., Lopes, L., Mariazzi, A. . G., Mariş, I. . C., Marsella, Giovanni, Martello, Daniele, Masías Meza, J. . J., Mathes, H. . J., Matthews, J. . A. . J., Mazur, P. . O., Mello, V. . B. . B., Micheletti, M. . I., Minaya, I. . A., Moura, C. . A., Muller, M. . A., Müller, G., Müller, S., Navarro, J. . L., Nguyen, P. . H., Niculescu Oglinzanu, M., Pepe, I. . M., Perrone, Lorenzo, Prado, R. . R., Quel, E. . J., Riggi, S., Rodrigues de Carvalho, W., Rodríguez Frías, M. . D., Rovero, A. . C., Saffi, S. . J., Santos, E. . M., Scarso, C., Schauer, M., Scherini, Viviana, Schröder, F. . G., Sciutto, S. . J., Shellard, R. . C., Śmiałkowski, A., Snow, G. . R., Srivastava, Y. . N., Stanca, D., Supanitsky, A. . D., Sutherland, M. . S., Taborda, O. . A., Theodoro, V. . M., Tiffenberg, J., Todero Peixoto, C. . J., Valdés Galicia, J. . F., Valore, L., van Aar, G., van Bodegom, P., van den Berg, A. . M., van Velzen, S., van Vliet, A., Vázquez, J. . R., Vázquez, R. . A., Watson, A. . A., Wittkowski, D., Yang, L., Zavrtanik, D., Physics, Elementary Particle Physics, Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Fundação Oswaldo Cruz / Oswaldo Cruz Foundation (FIOCRUZ), Università degli studi di Catania = University of Catania (Unict), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), and Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)

Subjects
detector [cosmic radiation], interaction [cosmic radiation], FLUORESCENCE YIELD, Physics - Instrumentation and Detectors, Air fluorescence detectors, hybrid observatory, Astronomy, Air fluorescence detector, Astrophysics, Auger, High energy cosmic ray, design [detector], Observatory, SURFACE DETECTOR ARRAY, High energy cosmic rays, Astrophysics::Solar and Stellar Astrophysics, fluorescence [air], Ultra-high-energy cosmic ray, ATMOSPHERIC MULTIPLE-SCATTERING, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Instrumentation, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, performance [detector], Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Pierre Auger Observatory, Instrumentation and Detectors (physics.ins-det), water Cherenkov detectors, LIGHT, Water Cherenkov detector, network [detector], LOWER IONOSPHERE, ddc:620, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Hybrid observatory, Water Cherenkov detectors, Nuclear and High Energy Physics, physics, air fluorescence detectors, Air fluorescence detectors, High energy cosmic rays, Hybrid observatory, Pierre Auger Observatory, Water Cherenkov detectors, Nuclear and High Energy Physics, Instrumentation, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, EXTENSIVE AIR-SHOWERS, Particle detector, VHE [cosmic radiation], ddc:530, RECONSTRUCTION, Cosmic-ray observatory, Instrumentation and Methods for Astrophysics (astro-ph.IM), Engineering & allied operations, Astrophysique, Ciencias Exactas, Nuclear and High Energy Physic, fluorescence [detector], high energy cosmic rays, Física, ASTROFÍSICA, ULTRA-HIGH ENERGY, Pierre Auger Observatory, High energy cosmic rays, Hybrid observatory, Water Cherenkov detectors, Air fluorescence detectors, Experimental High Energy Physics, RADIATION, EMISSION
Abstract

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ), São Paulo Research Foundation (FAPESP) Grants # 2010/07359-6 and # 1999/05404-3, Ministério de Ciência e Tecnologia (MCT), Brazil; MSMT-CR LG13007, 7AMB14AR005, CZ.1.05/2.1.00/03.0058 and the Czech Science Foundation Grant 14-17501S, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS), Département Sciences de l'Univers (SDU-INSU/CNRS), Institut Lagrange de Paris, ILP LABEX ANR-10-LABX-63, within the Investissements d'Avenir ProgrammeANR-11-IDEX-0004-02, France; Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Württemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden-Württemberg, Germany; Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Università e della Ricerca (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), CETEMPS Center of Excellence, Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; National Centre for Research and Development, Grant nos. ERA-NETASPERA/01/11 and ERA-NET-ASPERA/02/11, National Science Centre, Grant nos. 2013/08/M/ST9/00322, and 2013/08/M/ST9/00728 and HARMONIA 5 – 2013/10/M/ST9/00062, Poland; Portuguese national funds and FEDER funds within COMPETE – Programa Operacional Factores de Competitividade through Fundação para a Ciencia e a Tecnologia, Portugal; Romanian Authority for Scientific Research ANCS, CNDI-UEFISCDI partnership projects nos. 20/2012 and nr.194/2012, project nos. 1/ASPERA2/2012 ERA-NET, PN-II-RU-PD-2011-3-0145-17, and PN-II-RU-PD-2011- 3-0062, the Minister of National Education, Programme for research – Space Technology and Advanced Research – STAR, project number 83/2013, Romania; Slovenian Research Agency, Slovenia; Comunidad de Madrid, FEDER funds, Ministerio de Educación y Ciencia, Xunta de Galicia, European Community 7th Framework Program, Grant no. FP7-PEOPLE-2012-IEF-328826, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract no. DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107 and DE-SC0011689, National Science Foundation, Grant no. 0450696, The Grainger Foundation, USA; NAFOSTED, Vietnam; Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union 7th Framework Program, Grant no. PIRSES-2009- GA-246806; and UNESCO., The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world׳s largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2, 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory., Comision Nacional de Energia Atomica, Fundacion Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas, Australian Research Council, National Council for Scientific and Technological Development (CNPq), Ciencia Tecnologia e Inovacao (FINEP), Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2010/07359-6 1999/05404-3, Ministerio de Ciencia e Tecnologia (MCT), Brazil, Ministry of Education, Youth & Sports - Czech Republic LG13007 7AMB14AR005 CZ.1.05/2.1.00/03.0058, Grant Agency of the Czech Republic Czech Republic Government 14-17501S, Centre National de la Recherche Scientifique (CNRS), Region Ile-de-France, Departement Physique Nucleaire et Corpusculaire PNC-IN2P3/CNRS, Departement Sciences de l'Univers (SDU-INSU/CNRS), Institut Lagrange de Paris, French National Research Agency (ANR) ANR-11-IDEX-0004-02 ANR-10-LABX-63, Federal Ministry of Education & Research (BMBF), German Research Foundation (DFG), Finanzministerium Baden-Wurttemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz Association, Ministerium fur Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany, Istituto Nazionale Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare (INFN), Ministry of Education, Universities and Research (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), CETEMPS Center of Excellence, Italy, Consejo Nacional de Ciencia y Tecnologia (CONACyT), Ministerie van Onderwijs, Cultuur en Wetenschap, Netherlands Organization for Scientific Research (NWO), FOM (The Netherlands) Netherlands Government, National Centre for Research and Development ERA-NET-ASPERA/01/11 ERA-NET-ASPERA/02/11, National Science Centre, Poland 2013/08/M/ST9/00322 2013/08/M/ST9/00728 HARMONIA 5 - 2013/10/M/ST9/00062, Portuguese national funds, FEDER funds within COMPETE - Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia, Portugal, Romanian Authority for Scientific Research ANCS, CNDI-UEFISCDI 20/2012 194/2012 1/ASPERA2/2012 ERA-NET PN-II-RU-PD-2011-3-0145-17 PN-II-RU-PD-2011-3-0062, Programme for research - Space Technology and Advanced Research - STAR, Romania 83/2013, Slovenian Research Agency - Slovenia, Comunidad de Madrid Instituto de Salud Carlos III, European Union (EU), Spanish Government, Xunta de Galicia, European Community, Spain FP7-PEOPLE-2012-IEF-328826, Science & Technology Facilities Council (STFC), United States Department of Energy (DOE) DE-AC02-07CH11359 DE-FR02-04ER41300 DE-FG02-99ER41107 DE-SC0011689, National Science Foundation (NSF) 0450696, Grainger Foundation, USA, National Foundation for Science & Technology Development (NAFOSTED), Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union (EU) PIRSES-2009-GA-246806, UNESCO

Published
2015
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17. Polymorphismes génétiques et allergies médicamenteuses

Author

L. Guglielmi and Pascal Demoly

Subjects
Gynecology, medicine.medical_specialty, Anesthesiology and Pain Medicine, business.industry, β lactams, Immunology and Allergy, Medicine, business
Abstract

Resume Dix a 20 % des patients hospitalises presentent des effets secondaires aux medicaments et le tiers de ces reactions pourrait etre du a des allergies. Les mecanismes immunologiques de l'allergie medicamenteuse qui sont multiples. Les antibiotiques (s-lactamines surtout) sont la principale classe therapeutique concernee et entrainent le plus frequemment une allergie immediate mediee par les IgE. L'analyse des facteurs de risque des allergies medicamenteuses reste modeste et peu d'etudes de polymorphismes genetiques ont ete conduites, hormis celles concernant certaines enzymes du metabolisme des medicaments ou certains haplotypes HLA. Les donnees issues d'une approche immunogenetique doivent permettre de mettre a disposition de nouveaux outils de diagnostic et certainement de prediction. Cependant, les resultats de ce type d'etude peuvent varier suivant la population concernee. L'identification de marqueurs genetiques suffisamment predictifs pour etre utiles en clinique va necessiter le criblage de plus d'une centaine de SNP dans le genome et ainsi d'identifier les sous-populations de patients a risque pour chaque classe de medicaments.

Published
2005
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18. Development of Consensus Statement on Definitions for Consistent Emergency Department Metrics

Author

Jesse M. Pines, Sonia Astle, Suzette Thorby, Nicholas Tsarouhas, Susan K. Banschbach, William T. Durkin, Nancy L. Hughes, Michael G. Millin, Heather E. Russell, Diane Gurney, Suzanne Stone-Griffith, Linda K. Groah, Sandra M. Schneider, William T. Briggs, Charlotte L. Guglielmi, Randy Pilgrim, and Nicholas J. Jouriles

Subjects
medicine.medical_specialty, Time Factors, Statement (logic), business.industry, Emergency department, Emergency Nursing, medicine.disease, Crowding, United States, Societies, Nursing, Family medicine, Humans, Medicine, Medical emergency, Emergency Service, Hospital, business, Quality Indicators, Health Care
Published
2012
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19. Building a new organizational framework

Author

Linda K. Groah, Donna S. Watson, and Charlotte L. Guglielmi

Subjects
Medical–Surgical Nursing, Organizational framework, Knowledge management, business.industry, Organization development, Organizational engineering, Organizational learning, Business, Organizational network analysis
Published
2002
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20. Reflecting on the Freedom to Be

Author

Charlotte L. Guglielmi

Subjects
Freedom, Medical–Surgical Nursing, Perioperative nursing, Nursing, Perioperative Nursing, Societies, Nursing, Psychology
Published
2011
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22. Empowering providers to eliminate surgical fires

Author

Jayne MacPherson, Dennis R. Parker, Charlotte L. Guglielmi, Tom McKibban, Jane Flowers, Linda K. Groah, Ewa Greenier, Kathleen Shostek, Roy H. Constantine, and T Forcht Dagi

Subjects
Medical–Surgical Nursing, Operating Rooms, business.industry, Internet privacy, Humans, Business, Power, Psychological, Fires
Published
2014

23. 10 years in, why time out still matters

Author

Linda K. Groah, Elena Canacari, Katherine B. Lee, Donna S. Watson, Sharon Bachman, Alexander A. Hannenberg, Charlotte L. Guglielmi, Erin S. DuPree, and Sherri Alexander

Subjects
Medical–Surgical Nursing, Operating Rooms, Text mining, Medical Errors, business.industry, Medicine, Humans, Patient Safety, business, Operating Room Nursing, Data science, Checklist
Published
2014

24. The growing role of patient engagement: relationship-based care in a changing health care system

Author

Charlotte L. Guglielmi, David Shapiro, William J. Duffy, Gerald B. Healy, Barbara L. Dean, Linda K. Groah, and Martha Stratton

Subjects
medicine.medical_specialty, business.industry, Patient engagement, Medical–Surgical Nursing, Health Planning, Nursing, Patient Satisfaction, Family medicine, Perioperative Nursing, Health care, Self care, medicine, Humans, business, Nurse-Patient Relations, Delivery of Health Care
Published
2014

25. The Freedom to Seize a Teachable Moment

Author

Charlotte L. Guglielmi

Subjects
Medical–Surgical Nursing, Teachable moment, Interprofessional Relations, Teaching, Humans, Nurse-Patient Relations, Operating Room Nursing, Psychology, Health Education, Nurse's Role, Epistemology
Published
2010
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30. Miscount incidents: a novel approach to exploring risk factors for unintentionally retained surgical items

Author

Elena Canacari, Michael D. Howell, Timothy J. Judson, Kenneth Sands, and Charlotte L. Guglielmi

Subjects
Academic Medical Centers, Time Factors, Leadership and Management, business.industry, MEDLINE, Age Factors, Perioperative, medicine.disease, Foreign Bodies, Confidence interval, Checklist, United States, Cohort Studies, Personnel, Hospital, Increased risk, Multidisciplinary approach, Risk Factors, Surgical Procedures, Operative, Medicine, Humans, Medical emergency, Retained Surgical Items, business, Cohort study, Quality of Health Care
Abstract

An estimated 1,500 operations result in retained surgical items (RSIs) each year in the United States, resulting in substantial morbidity. The rarity of these events makes studying them difficult, but miscount incidents may provide a window into understanding risk factors for RSIs.A cohort study of all consecutive operative cases during a 12-month period was conducted at a large academic medical center to identify risk factors for surgical miscounts. A multidisciplinary electronic miscount reconciliation checklist (necessitating both surgeon and nurse input) was introduced into the internally developed electronic Perioperative Information Management System to build a predictive model for RSI cases.Among 23,955 operations, 84 resulted in miscount incidents (0.35% [95% confidence interval: 0.28% to 0.43%]). Increased case duration was strongly associated with increased risk of a miscount in unadjusted analyses (p.0001). In the nested case-control analysis, both the case duration and the number of providers present were independently associated with a more than doubling of the odds of a miscount, even after adjustment for one another, the elective/urgent/emergent status of a case, and personnel changes occurring during the case.The finding that both the length of the case and the number of providers involved in the case were independent risk factors for miscount incidents may offer insight into risk-targeted strategies to prevent RSIs, such as postoperative imaging, bar-coded surgical items, and radiofrequency technology. Miscounts trigger use of the Incorrect Count Safety Checklist, which can be used to determine whether a count completed at the procedure's conclusion is consistent across disciplines (circulating nurses, scrub persons, surgeons).

Published
2013

31. Experimental assessment of RSF, UF, RSF-O3 and RSF-H2O2/UV for unrestricted agricultural wastewater reuse in Italy

Author

L. Guglielmi, Francesca Gialdini, L. Canovi, C. Parabita, L. Furatian, Sabrina Sorlini, and D. Santoro

Subjects
chemistry.chemical_classification, Ultrafiltration, ultraviolet light, wastewater reuse, law.invention, combined processes, ozone, Hydrocarbon, Wastewater, chemistry, law, Environmental chemistry, ultrafiltration, medicine, rapid sand filtration, Sewage treatment, Mineral oil, Effluent, Filtration, Water Science and Technology, Total suspended solids, medicine.drug
Abstract

In this paper, tertiary treatment processes aimed at achieving a wastewater quality suitable for reuse in agriculture in Italy have been investigated, with experimental results generated by means of pilot and bench scale tests. Studies were conducted to assess the removal of mineral oil, total surfactants, total coliforms, Escherichia coli and Salmonella using the following treatment options: rapid sand filtration (RSF), hollow fiber ultrafiltration (UF), RSF followed by ozonation (RSF-O3) and RSF followed by hydrogen peroxide combined with UV radiation (RSF-H2O2/UV). Mineral oil concentration, evaluated by means of the hydrocarbon oil index measurement, indicated an effluent concentration consistently below 0.05 mg/L for all processes studied. While total surfactants in the secondary effluent never exceeded the applicable limit of 0.5 mg/L during the studies, the degree of removal measured in studied treatments ranged from moderate to low, with the greatest removal observed using RSF-O3 (24%) and RSF-H2O2/UV (30%) under applied conditions. Overall, the optimal treatment performances were achieved by the RSF-H2O2/UV combined process using ≥1.5 mg/L H2O2 and UV dose ≥45 mJ/cm2, which provided adequate mineral oil and total surfactants removal, complete removal of measurable total suspended solids (TSS) and Salmonella, and greater than 4-log reduction in total coliforms and Escherichia coli.

Published
2013

32. QUBIC: the Q&U Bolometric Interferometer for Cosmology

Author

Massimo Gervasi, C. Giordano, A. Passerini, Andrei Korotkov, E. Bréelle, Jean Christophe Hamilton, A. Ghribi, L. Vibert, Gregory S. Tucker, Emory F. Bunn, Angelo Cruciani, B. Maffei, P. de Bernardis, Michel Piat, J. Martino, G. Curran, A. Bounab, L. Guglielmi, F. Voisin, Elia S. Battistelli, Alessandro Schillaci, Roberto Sordini, R. Charlassier, F. Piacentini, Andrea Tartari, A. Baù, Lucio Piccirillo, G. Bordier, Y. Giraud-Heraud, Maria Salatino, M. Maiello, Martino Calvo, D. Bennett, S. Peterzen, L. Dumoulin, Peter Timbie, Silvia Masi, J. Kaplan, D. Prêle, S. Malu, Victor Haynes, Giampaolo Pisano, Martin Giard, M.-A. Bigot-Sazy, David Romano, J. Lande, Sophie Collin, Mario Zannoni, Federico Nati, Créidhe O'Sullivan, Laurent Bergé, Robert A. Watson, Marcin Gradziel, Gianluca Polenta, François Pajot, L. A. Montier, C. Parisel, A. Gault, S. Spinelli, C. Rosset, Anna Murphy, S. Marnieros, J.-P. Bernard, G. Sironi, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), QUBIC, Piat, M, Battistelli, E, Bau', A, Bennett, D, Berge, L, Bernard, J, de Bernardis, P, Bigot Sazy, M, Bordier, G, Bounab, A, Breelle, E, Bunn, E, Calvo, M, Charlassier, R, Collin, S, Cruciani, A, Curran, G, Dumoulin, L, Gault, A, Gervasi, M, Ghribi, A, Giard, M, Giordano, C, Giraud Heraud, Y, Gradziel, M, Guglielmi, L, Hamilton, J, Haynes, V, Kaplan, J, Korotkov, A, Lande, J, Maffei, B, Maiello, M, Malu, S, Marnieros, S, Martino, J, Masi, S, Montier, L, Murphy, A, Nati, F, O'Sullivan, C, Pajot, F, Parisel, C, Passerini, A, Peterzen, S, Piacentini, F, Piccirillo, L, Pisano, G, Polenta, G, Prele, D, Romano, D, Rosset, C, Salatino, M, Schillaci, A, Sironi, G, Sordini, R, Spinelli, S, Tartari, A, Timbie, P, Tucker, G, Vibert, L, Voisin, F, Watson, R, Zannoni, M, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), CSNSM INSTR, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'étude spatiale des rayonnements (CESR), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), CSNSM PS1, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), APC - Cosmologie, Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Dipartimento di Fisica, Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Dipartimento di Fisica 'Giuseppe Occhialini' = Department of Physics 'Giuseppe Occhialini' [Milano-Bicocca], Università degli Studi di Milano-Bicocca [Milano] (UNIMIB), Department of Experimental Physics, National University of Ireland Maynooth (Maynooth University), Université Paris-Sud - Paris 11 (UP11), CNRS/Université de Toulouse, Physics Department, University of Richmond, Richmond, Department of Physics [Madison], University of Wisconsin-Madison, University of Manchester [Manchester], Brown University, Università degli Studi di Siena = University of Siena (UNISI), Raman Research Institute, ASI Science Data Center, Bergé, L, A., B, Bréelle, E, Coppolecchia, A, Giraud Héraud, Y, Landé, J, O’Sullivan, C, de Petris, M, and Prêle, D

Subjects
Bolometric interferometry, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Cosmic microwave background, Astrophysics, 01 natural sciences, Cosmology, law.invention, Gravitational wave background, law, bolometer, cosmic microwave background, polarisation, interferometer, Cosmic Microwave Background, General Materials Science, Interferometer, 010303 astronomy & astrophysics, Instrumentation, Polarisation, media_common, Physics, instrumentation, Astrophysics::Instrumentation and Methods for Astrophysics, bolometric interferometry, Condensed Matter Physics, Atomic and Molecular Physics, and Optics, Interferometry, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], media_common.quotation_subject, Bolometer, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Cosmology, Cosmic Microwave Background, Inflation, Instrumentation, Bolometric interferometry, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], FIS/05 - ASTRONOMIA E ASTROFISICA, Materials Science(all), 0103 physical sciences, inflation, 010306 general physics, cosmology, Instrumentation and Methods for Astrophysics (astro-ph.IM), Inflation (cosmology), 010308 nuclear & particles physics, Gravitational wave, Astronomy, Astronomy and Astrophysics, Inflation, Universe, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract

One of the major challenges of modern cosmology is the detection of B-mode polarization anisotropies in the CMB. These originate from tensor fluctuations of the metric produced during the inflationary phase. Their detection would therefore constitute a major step towards understanding the primordial Universe. The expected level of these anisotropies is however so small that it requires a new generation of instruments with high sensitivity and extremely good control of systematic effects. We propose the QUBIC instrument based on the novel concept of bolometric interferometry, bringing together the sensitivity advantages of bolometric detectors with the systematics effects advantages of interferometry. Methods: The instrument will directly observe the sky through an array of entry horns whose signals will be combined together using an optical combiner. The whole set-up is located inside a cryostat. Polarization modulation will be achieved using a rotating half-wave plate and interference fringes will be imaged on two focal planes (separated by a polarizing grid) tiled with bolometers. We show that QUBIC can be considered as a synthetic imager, exactly similar to a usual imager but with a synthesized beam formed by the array of entry horns. Scanning the sky provides an additional modulation of the signal and improve the sky coverage shape. The usual techniques of map-making and power spectrum estimation can then be applied. We show that the sensitivity of such an instrument is comparable with that of an imager with the same number of horns. We anticipate a low level of beam-related systematics thanks to the fact that the synthesized beam is determined by the location of the primary horns. Other systematics should be under good control thanks to an autocalibration technique, specific to our concept, that will permit the accurate determination of most of the systematics parameters., Comment: 12 pages, 10 figures, submitted to Astronomy and Astrophysics

Published
2012
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33. The Pierre Auger Research and Development Array (RDA) in southeastern Colorado - R&D for a giant ground array

Author

A. Rokos, L. Guglielmi, E. Rauly, K. Kuhn, M. Maskevics, B. Courty, K. Nelson, M.A. Hevinga, M. Daubenspeck, A. Gaume, Fred Sarazin, C.F. Speelman, N. Solomey, J. Yadon, M. Marton, H. Meyer, J. Hodgson, O. Wolf, T. Nguyen Trung, B. Genolini, J. Thompson, M. Malinowski, S. Collonges, S. Robinson, J. Hollenbeck, AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), PIERRE AUGER, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)

Subjects
Pierre Auger Observatory, Physics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], 010308 nuclear & particles physics, Dynamic range, business.industry, QC1-999, Detector, Electrical engineering, Communications system, 01 natural sciences, 7. Clean energy, Auger, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Observatory, Hybrid array, 0103 physical sciences, Electronics, 010306 general physics, business, ComputingMilieux_MISCELLANEOUS, Remote sensing
Abstract

The Pierre Auger Research and Development Array (RDA) was originally designed to be the precursor of the northern Auger observatory, a hybrid array of 4400 surface detector stations and 39 fluorescence telescopes deployed over 20,000 square kilometers. It is conceived as a test bed aiming at validating an improved and more cost-effective 1-PMT surface detector design and a new peer-to-peer communication system. The array of ten surface detector stations and ten communication-only stations is currently being deployed in southeastern Colorado and will be operated at least until late 2013. It is configured in such a way that it allows testing of a new peer-to-peer communication protocol, as well as a new surface detector electronics design with a larger dynamic range aiming at reducing the distance from the shower core where saturation is observed. All these developments are expected in the short term to improve the performance of the Pierre Auger Observatory and enable future enhancements. In the longer term, it is hoped that some of these new developments may contribute to the design of a next-generation giant ground array.

Published
2012
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34. How to Report Adverse Events Related to the Use of Energy Devices in the Operating Room

Author

Charlotte L. Guglielmi

Subjects
Surgical team, Medical device, Computer science, Event (computing), Energy (esotericism), SAFER, medicine, Medical emergency, medicine.disease, Root cause analysis, Adverse effect
Abstract

A timely and directed response by all members of the surgical team is essential whenever a medical device fails. Beyond meeting the regulatory requirements of reporting, the learning that occurs as a result of the event once disseminated will assist in improving patient outcomes and creating systems that are safer.

Published
2012
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35. Intensity and polarization of the atmospheric emission at millimetric wavelengths at Dome Concordia

Author

E. S. Battistelli, G. Amico, A. Baù, L. Bergé, É. Bréelle, R. Charlassier, S. Collin, A. Cruciani, P. de Bernardis, C. Dufour, L. Dumoulin, M. Gervasi, M. Giard, C. Giordano, Y. Giraud-Héraud, L. Guglielmi, J.-C. Hamilton, J. Landé, B. Maffei, M. Maiello, S. Marnieros, S. Masi, A. Passerini, F. Piacentini, M. Piat, L. Piccirillo, G. Pisano, G. Polenta, C. Rosset, M. Salatino, A. Schillaci, R. Sordini, S. Spinelli, A. Tartari, M. Zannoni

Published
2012
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36. Defining competency in high-performance teams

Author

Charlotte L. Guglielmi, Alan P. Marco, Paula R. Graling, Linda K. Groah, Michelle Hoppes, David L. Feldman, and Larry L. Asplin

Subjects
Patient Care Team, Medical–Surgical Nursing, Risk Management, Process management, Societies, Nursing, Nurses, Clinical Competence, Credentialing, Psychology, Management, Boston
Published
2011

37. X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope

Author

L. Guglielmi, P. Francois, P. W. Albers, Jan Kragt, Christophe Martayan, S. D'Odorico, M. Vidali, E. Sweers, R. Manuputy, Gert Finger, P. Nørregaard, Filippo Maria Zerbi, Paul Bristow, J. Vinther, Joel Vernet, Celine Peroux, Eddy Elswijk, Per Kjaergaard, Isabelle Guinouard, Johan Pragt, J. P. Amans, A. de Ugarte Postigo, T. Adolfse, Gerben Wulterkens, Jens Hjorth, Pascal Vola, P. Goldoni, Lise Christensen, Andrea Modigliani, Florian Kerber, N. Michaelsen, Ralf Conzelmann, F. Riga, J. Klougart, Niels Christian Jessen, Hector Flores, P. van Dael, F. Royer, Sabine Moehler, H. van der Vliet, G. Fischer, Andrea Zacchei, H. H. Larsen, Hans Dekker, P. M. Groot, Niels Tromp, Francois Hammer, P. Kleszcz, Elena Mason, Mario Kiekebusch, Michael I. Andersen, Paolo Santin, Paolo Conconi, Lars Venema, C. Lucuix, D. Wistisen, R. Castillo, I. Hendriks, Marco Riva, P. Di Marcantonio, Matthew Horrobin, Ramón Navarro, Fanny Chemla, H. Hanenburg, T. Schoenmaker, Johannes Andersen, R. ter Horst, Vincenzo Mainieri, Ronald Roelfsema, Palle Møller, J. Dam, P. Binetruy, P. Spano, David Horville, R. Haigron, M. Tintori, G. G. Sacco, Mark Downing, C. Reinero, V. De Caprio, Bernard Delabre, Ferdinando Patat, Lex Kaper, L. Kern, R. Winters, Sofia Randich, A. Norup Sørensen, E. Pena, J.-L. Lizon, R. Mazzoleni, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), APC - THEORIE, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), High Energy Astrophys. & Astropart. Phys (API, FNWI), Low Energy Astrophysics (API, FNWI), PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)

Subjects
[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], 010504 meteorology & atmospheric sciences, Astronomy, FOS: Physical sciences, Dichroic glass, 01 natural sciences, Spectral line, Optics, Spectrographs, 0103 physical sciences, Spectral resolution, 010303 astronomy & astrophysics, Spectrograph, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), 0105 earth and related environmental sciences, Physics, instrumentation, Very Large Telescope, business.industry, Cassegrain reflector, Astronomy and Astrophysics, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Space and Planetary Science, spectrograph, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Prism, business, Astrophysics - Instrumentation and Methods for Astrophysics, Data reduction
Abstract

X-shooter is the first 2nd generation instrument of the ESO Very Large Telescope(VLT). It is a very efficient, single-target, intermediate-resolution spectrograph that was installed at the Cassegrain focus of UT2 in 2009. The instrument covers, in a single exposure, the spectral range from 300 to 2500 nm. It is designed to maximize the sensitivity in this spectral range through dichroic splitting in three arms with optimized optics, coatings, dispersive elements and detectors. It operates at intermediate spectral resolution (R~4,000 - 17,000, depending on wavelength and slit width) with fixed echelle spectral format (prism cross-dispersers) in the three arms. It includes a 1.8"x4" Integral Field Unit as an alternative to the 11" long slits. A dedicated data reduction package delivers fully calibrated two-dimensional and extracted spectra over the full wavelength range. We describe the main characteristics of the instrument and present its performance as measured during commissioning, science verification and the first months of science operations., accepted for publication in A&A

Published
2011
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38. Creating a culture of civility takes a team

Author

Callie Craig, William J. Duffy, Richard G. Cuming, Mark J. Lema, Amy E. Vinson, Linda K. Groah, Gerald B. Healy, and Charlotte L. Guglielmi

Subjects
Patient Care Team, Operating Rooms, Attitude of Health Personnel, Verbal Behavior, Communication, Interprofessional Relations, MEDLINE, Organizational culture, Professional competence, Operating Room Nursing, Dissent and Disputes, Organizational Culture, Management, Medical–Surgical Nursing, Professional Competence, Civility, Humans, Engineering ethics, Cooperative behavior, Cooperative Behavior, Psychology, Social Behavior
Published
2010

39. Planck pre-launch status: The HFI instrument, from specification to actual performance

Author

Peter A. R. Ade, V. Yurchenko, F. Piacentini, R. Pons, M. Nexon, G. Recouvreur, Christopher G. Paine, C. Dumesnil, Philippe Camus, J. Pahn, O. Perdereau, M. Tristram, Sarah E. Church, M.-A. Miville-Deschênes, A. Coulais, J. J. Bock, F.-X. Désert, J. Lande, G. Serra, J. F. Macías-Pérez, F. Pajot, J.-L. Beney, F. Bouchet, Simon Prunet, J.-P. Torre, C. Leroy, N. Ponthieu, Bruno Maffei, E. Bréelle, M. Giard, B. P. Crill, J.-L. Puget, L. Vibert, W. A. Holmes, T. C. Koch, E. Hivon, J. Haissinski, R. V. Sudiwala, B. Mansoux, L. Montier, K. Dassas, C. Renault, C. Evesque, R. S. Bhatia, Alain Benoit, J. Charra, Sophie Henrot-Versille, W. C. Jones, Y. Blanc, P. de Bernardis, A. Arondel, F. Couchot, C. Rosset, Martin Crook, C. Marty, Stéphane Plaszczynski, B. Leriche, Etienne Pointecouteau, D. Rambaud, D. Santos, J.-F. Sygnet, M. Charra, Tom Bradshaw, J.-M. Delouis, I. Ristorcelli, P. Eng, Jan Tauber, Thierry Maciaszek, Karim Benabed, H. Lagardère, D. Yvon, A. Moneti, J. Narbonne, Giorgio Savini, Andrew E. Lange, X. Dupac, Y. Longval, A. Catalano, R. Gispert, P. de Marcillac, P. Lami, George Efstathiou, C. Mercier, Silvia Masi, Jacques Delabrouille, J. A. Murphy, Ken Ganga, J.-Ph. Bernard, M. Piat, Adam Woodcraft, J.-M. Lamarre, G. Guyot, L. Guglielmi, P. Stassi, J.-J. Fourmond, Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Institut Néel (NEEL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), Centre d'étude spatiale des rayonnements (CESR), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Cryogénie (NEEL - Cryo), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), APC - Cosmologie, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, PLANCK, École normale supérieure - Paris (ENS Paris), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Hélium : du fondamental aux applications (HELFA), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Cryogénie (Cryo), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPP), École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), HELFA - Hélium : du fondamental aux applications, Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Cryo - Cryogénie, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)

Subjects
cosmic microwave background, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Point source, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Cosmic microwave background, Cosmic background radiation, Context (language use), Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 7. Clean energy, 01 natural sciences, Radio spectrum, law.invention, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, techniques: photometric, Optics, law, space vehicles: instruments, submillimeter: general, techniques: polarimetric, 0103 physical sciences, Calibration, Planck, 010303 astronomy & astrophysics, QB, Physics, 010308 nuclear & particles physics, business.industry, Bolometer, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Space and Planetary Science, symbols, business
Abstract

Context. The High Frequency Instrument (HFI) is one of the two focal instruments of the Planck mission. It will observe the whole sky in six bands in the 100 GHz–1 THz range.\ud \ud Aims. The HFI instrument is designed to measure the cosmic microwave background (CMB) with a sensitivity limited only by fundamental sources: the photon noise of the CMB itself and the residuals left after the removal of foregrounds. The two high frequency bands will provide full maps of the submillimetre sky, featuring mainly extended and point source foregrounds. Systematic effects must be kept at negligible levels or accurately monitored so that the signal can be corrected. This paper describes the HFI design and its characteristics deduced from ground tests and calibration.\ud \ud Methods. The HFI instrumental concept and architecture are feasible only by pushing new techniques to their extreme capabilities, mainly: (i) bolometers working at 100 mK and absorbing the radiation in grids; (ii) a dilution cooler providing 100 mK in microgravity conditions; (iii) a new type of AC biased readout electronics and (iv) optical channels using devices inspired from radio and infrared techniques.\ud \ud Results. The Planck-HFI instrument performance exceeds requirements for sensitivity and control of systematic effects. During ground-based calibration and tests, it was measured at instrument and system levels to be close to or better than the goal specification.

Published
2010
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40. Planck pre-launch status: HFI ground calibration

Author

L. Montier, Y. Giraud-Héraud, C. Mercier, C. Rosset, D. Yvon, Michel Lefebvre, J. P. Torre, Etienne Pointecouteau, Andrew E. Lange, J.-J. Fourmond, V. Hervier, P. Eng, D. Broszkiewicz, M. Charra, C. Nicolas, L. Guglielmi, G. Guyot, J.-L. Beney, O. Perdereau, K. Dassas, F. Piacentini, M. Piat, A. Chardin, C. Evesque, B. Leriche, Bruno Maffei, M. Veneziani, Peter A. R. Ade, F. Couchot, F. Pajot, R. V. Sudiwala, P. Duret, S. François, C. Marty, Sophie Henrot-Versille, J. Charra, Thierry Maciaszek, R. Pons, J. Haissinski, I. Ristorcelli, J.-M. Lamarre, A. Mahendran, W. C. Jones, Jean-Loup Puget, C. Rioux, W. A. Holmes, D. Vallée, Giorgio Savini, A. Catalano, Matthieu Tristram, Stéphane Plaszczynski, P. de Marcillac, C. Carabétian, Philippe Camus, B. Mansoux, N. Ponthieu, F. Noviello, M. Giard, B. P. Crill, P. Lami, J. C. Renault, Marc-Antoine Miville-Deschenes, Claude Leroy, J. F. Macías-Pérez, A. Coulais, Silvia Masi, E. Bréelle, F.-X. Désert, P. de Bernardis, J. Daubin, D. Rambaud, J.-M. Delouis, C. Renault, R. Cizeron, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Cryogénie (NEEL - Cryo), Institut Néel (NEEL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre d'étude spatiale des rayonnements (CESR), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), APC - Cosmologie, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, PLANCK, Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Cryogénie (Cryo), École normale supérieure - Paris (ENS Paris), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Cryo - Cryogénie, Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)

Subjects
cosmic microwave background, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Cosmic microwave background, Astrophysics, 01 natural sciences, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, 0103 physical sciences, Calibration, space vehicles: instruments, Planck, 010303 astronomy & astrophysics, space vehicles : instruments, QB, Physics, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, submillimeter: general, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], On board, Cardinal point, Space and Planetary Science, symbols, Vacuum chamber
Abstract

Context. The Planck satellite was successfully launched on May 14th 2009. We have completed the pre-launch calibration measurements of the High Frequency Instrument (HFI) on board Planck and their processing.\ud \ud Aims. We present the results ot the pre-launch calibration of HFI in which we have multiple objectives. First, we determine instrumental parameters that cannot be measured in-flight and predict parameters that can. Second, we take the opportunity to operate and understand the instrument under a wide range of anticipated operating conditions. Finally, we estimate the performance of the instrument built.\ud \ud Methods. We obtained our pre-launch calibration results by characterising the component and subsystems, then by calibrating the focal plane at IAS (Orsay) in the Saturne simulator, and later from the tests at the satellite level carried out in the CSL (Liège) cryogenic vacuum chamber. We developed models to estimate the instrument pre-launch parameters when no measurement could be performed.\ud \ud Results. We reliably measure the Planck-HFI instrument characteristics and behaviour, and determine the flight nominal setting of all parameters. The expected in-flight performance exceeds the requirements and is close or superior to the goal specifications.

Published
2010
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42. Celebrating the freedom to leverage the power of nursing

Author

Charlotte L. Guglielmi

Subjects
Knowledge management, business.industry, MEDLINE, Operating Room Nursing, Nurse's Role, United States, Management, Power (social and political), Medical–Surgical Nursing, Leadership, Leverage (negotiation), Health Care Reform, Patient-Centered Care, Societies, Nursing, Humans, Power, Psychological, business, Forecasting, Quality of Health Care
Published
2010

43. Study of the leptonic decays of the Z0 boson

Author

A. Klovning, U. Mjoernmark, Sandor Czellar, G. Polok, M. Bozzo, V.A. Uvarov, A. Ruiz, Ugo Gasparini, Paolo Pasini, P. Queru, W. K. Van Doninck, F. Richard, C. Matteuzzi, M. Hahn, B. Bouqquet, A. G. Frodesen, Andrey Korytov, Jan Krolikowski, N. N. Khovanski, W. Bartl, B. V. Batyunia, R. Pain, B. Koene, E. Lieb, A. Sebastia, I. Lippi, E.N. Tsyganov, J. H. Wickens, Jose Luis Contreras, C. Vander Velde, C. Lambropoulos, Ugo Amaldi, E. Zevgolatakos, R. Rongved, S. Almehed, C. Pinori, J. P. Laugier, J.A.M.A. Buytaert, A.N. Diddens, U. Kruener-Marquis, M. Gorbics, J.A. Lidbury, D. Radojicic, J.P. Grillet, M. Pimenta, N. De Groot, M. De Beer, G. Wormser, Ariella Cattai, Jacques Lemonne, A. Stocchi, Guido Barbiellini, M. Pernicka, G. Lenzen, J. E. Campagne, M. Koratzinos, L. Guglielmi, M. Bonapart, Wolfgang Adam, D. Bertrand, Francesco Navarria, Paolo Morettini, J. G. Loken, J.F. Genat, B. Kisielewski, Paolo Ronchese, T. Kreuzberger, J.C. Raoul, G. Goujon, G. Crosetti, Evgueni Vlasov, M. Nigro, Jan Ridky, A. S. Vodopianov, Tuure Tuuva, Clara Troncon, Itzhak Roditi, Gueorgui Chelkov, J. Guy, B. Dalmagne, M. Kopf, J. N. Jackson, P. Kokkinias, M. Passeneau, S. Ferroni, Z. Hajduk, F. Udo, G. Petrucci, M. Nordberg, R. Lauhakangas, H. Herr, Winfried Mitaroff, P. Beltran, Louis Lyons, C.W. Salgado, J. Mas, P. Lutz, G. Tristram, P. Laurikainen, S. Du, Paula Eerola, O. Ullaland, F. Djama, C. Gaspar, S. Haider, D.N. Edwards, C. Caso, M. Sessa, V. Castillo Gimenez, P. Negri, Tim Adye, C. De La Vaissiere, Laurent Chevalier, U. Trevisan, N. Crosland, J.V. Allaby, M. Jonker, Y. Sacquin, Maciej Górski, A. B. Fenyuk, L. Mattsson, J.J. Jaeger, Tiziano Rovelli, M. Cresti, J.H. Bibby, G.P. Barreira, B. Lund-Jensen, G. E. Kalmus, G. D. Alekseev, J. M. Yelton, A. Passeri, S. Gawne, Klaus Hamacher, A. Firestone, G. Kantardjian, C. De Clerco, Milos Lokajicek, K. Woschnagg, M. Nonni, P. Branchini, J. Krstic, Göran Jarlskog, W. Bell, N. I. Zimin, Stavros Maltezos, Mikael Berggren, H. Hofmann, J. Cuevas Maestro, H. B. Crawley, V. Lepeltier, H. Forsbach, F. Fulda-Quenzer, T. Bolognese, E. C. Katsoufis, G. Gopal, A. Letessier-Selvon, S. Gumenyuk, Nikolai Smirnov, V. Ruhlmann, O. Barring, G. Zhang, Paolo Checchia, B. Franek, W. Kucewicz, G. Matthiae, C. Stanescu, L.J. Carroll, M. L. Turluer, M. Vollmer, D. Reid, Ph. Gavillet, P. Spentzouris, E. Graziani, B. Jean-Marie, A. Hakansson, E. J. Sanchez, W. D. Apel, S. J. Alvsvaag, Roland Horisberger, L. Bugge, G. Hamel de Monchenault, E. G. Anassontzis, J. P. Engel, I. Kontaxis, P. Lorenz, P. Roudeau, M. J. Bates, Edoardo Castelli, D. Z. Toet, J. Joensuu, J. M. Brunet, H. Lebbolo, Josef Strauss, R. Llosa, N. Bingefors, P. Van Dam, M. Fernandez Alonso, P. Privitera, M.V. Reis, P. Weilhammer, Luc Pape, D. Imbault, R. Zitoun, D. Langerveld, P. Abreu, P. Borgeaud, Borge Svane Nielsen, M. H. Gros, F. J. Harris, H. Foeth, P. Allen, Gianni Zumerle, F. Astesan, Toralf Bernhard Skaali, Maria Roberta Monge, S. Barlag, A. Zalewska, Valery Pozdnyakov, G. Cabras, Krzysztof Doroba, Chiara Meroni, A.K. Topphol, C. Brand, M. Mc Cubbin, G. Ekspong, K. Hultqvist, Renato Turchetta, B. Grossetete, Allan Hallgren, B. Korzen, P. Poropat, G. Damgaard, C. Poiret, L. Tortora, Giovanni Valenti, I. Belokopytov, M. Boratav, D. Gamba, G. Voulgaris, Sverker Johansson, W. T. Meyer, Pierre Billoir, Mogens Dam, K. Rybicki, W. Venus, B. Muryn, V. Obraztsov, P. Aarnio, V. Gracco, M. Schaeffer, Andre Augustinus, P. Herquet, H. Palka, G. Skjevling, R. Contri, Giovanni Darbo, S. Simonetti, M. Voutilainen, G. Grosdidier, R. Sekulin, R. Dzhelyadin, T. Pettersen, Jose M. Benlloch, A. Grant, R.B. Kadyrov, F. Barao, P. V. Chliapnikov, M. Crozon, Craig Buttar, A. De Angelis, D. Delikaris, N. van Eijndhoven, J. Werner, L. Viseu Melo, E. Sundell, M.I. Laakso, Daniel Bloch, Hans Dijkstra, I. Herbst, Katri Huitu, T.K. Truong, B. Goret, M. Baubillier, R. Lucock, Alessandra Romero, Georgios Stavropoulos, J.M. Noppe, M. Turala, Barry King, Ahmimed Ouraou, Pavlos Ioannou, F. Simonetto, R. Gokieli, A. Tilquin, J. Perez, I.A. Gritsaenko, G. Leder, G. B. Chadwick, E. Higon, R. Seufert, V.M. Golovatyuk, W.S.C. Williams, Daniel Treille, J. J. Hernandez, R. Frühwirth, Manolis Dris, J. Pyythia, B. Åsman, P. Adrianos, C. J. Beeston, F. Scuri, Juan Fuster, N.K. Vishnevskij, A. M. Zaitsev, E. K. Johansson, J. E. Hooper, J.C. Le Grand, J. Timmermans, J. Pagot, A. Pullia, J.-E. Augustin, A. M. Wetherell, E. Lillethun, T. Moa, G. Maehlum, K. Pakonski, F. Bianchi, J. Michałowski, Kjell Fransson, L. Lanceri, D. Husson, J. Barlow, E. Vela, Lucio Cerrito, T. Buran, J.B.M. Pattison, I. A. Tyapkin, M. A. Houlden, D. Crennell, F. Mandl, A. Pinsent, A.M. Romaya, M. Ellila, Guenakh Mitselmakher, A.J. Camacho Rozas, D. Vilanova, G. Smadja, D.Yu. Barbin, S. Squarcia, K. W. Glitza, A. Zinchenko, E. Menichetti, Olga Botner, Krzysztof Korcyl, H. Saarikko, T. Hofmokl, Marek Szczekowski, N. Dimitriou, Stefano Ragazzi, José Salt, F. Couchot, R. Sosnowski, B. W. Heck, E. Rosso, H. Klein, H. Schneider, V. G. Timofeev, S. Nounos, J.-P. Vanuxem, Panos Kostarakis, M.-H. Gros, A. Markou, F. Cao, V. Falaleev, E. Lillestol, V. Chorowicz, O.A. Maeland, R. Downs, J. Haissinski, S. Braibant, Tord Ekelof, H. Staeck, G. Galeazzi, R. Strub, B. Loerstad, K. Moenig, S. Cairanti, H. Burmeister, D. Sacco, M. Mazzucato, E. Fokitis, Robert S. Brown, J. Drees, P. Szymanski, Patrick Jarry, M. Winter, G. Rinaudo, Evangelos Gazis, G. Vegni, N. Brummer, W. H. Range, E. Spiriti, B.D. Hyams, E. I. Rosenberg, K. Kurvinen, M. Dracos, R. Ragazzon, P. Siegrist, J-C. Marin, M. Davenport, B. Grung, A. A. Rademakers, S. O. Holmgren, D. Benedic, D. Loukas, George Kalkanis, P. B. Renton, M. Flinn, L. O. Eek, R. C. Shellard, L. Di Ciaccio, Josef Hrubec, A. M. Segar, D. C. Fries, G. Kuhn, P. S. Iversen, F. Fontanelli, J. Skeens, C. Astor Ferreres, J. Velasco, Marta Calvi, L. Tkachev, Vincenzo Canale, Geoffrey Smith, G. W. Van Apeldoorn, G. Sette, L.S. Curwen, W. Dulinski, L. Ventura, Håkan T Johansson, B. Lavigne, S. Palma Lopes, S. Quinton, Hans Muller, T. Odegaard, P. N. Bogolubov, Christine Kourkoumelis, E. Dahl-Jensen, H. De Boeck, M. Tyndel, P. Vaz, D. Bollini, M. Pegoraro, J. Maillard, P. Jalocha, S. Biagi, H. P. Borner, V. Kadyshevskiy, V. Perevozchikov, Theodora Papadopoulou, Tiziano Camporesi, N. G. Redaelli, P. Frenkiel, R. Moeller, A. Baroncelli, A. Hrisoho, H. J. Hilke, C. Bosio, F. Waldner, K. D. Brand, Antonio Ferrer, Roberto Cirio, L. K. Resvanis, C. Walck, G. E. Theodosiou, M. Zito, O. Pingot, K. Spang, E. Sanchis, L. Mathis, Massimo Caccia, N. Yamdagni, Paul Baillon, Alexander Lincoln Read, Vladimir Nikolaenko, M. Szeptycka, P. Juillot, M. Mur, M.A. Lopez Aguera, Francesca Romana Cavallo, Mitchell Wayne, V. V. Lapin, P. O. Hulth, F. Rossel, P. Delpierre, E. Daubie, G. Myatt, J.M. Gago, Joao Varela, P. Kluit, P. R. S. Gomes, S. Ueberschaer, A. Maltezos, M. Gaillard, A. Campion, R. Zukanovich Funchal, H. Wahlen, Ariel Goobar, D. Fraissard, K. H. Becks, P. Antilogus, M. E. Veitch, J. Bjarne, W. Klempt, F. Hahn, F. Stichelbaut, R. Mc Kay, Cesare Chiccoli, F. Adami, M. Barranco-Luque, R. Keranen, Philippe Charpentier, Mario Sannino, R. Orava, S. Topp-Jorgensen, Maria Elena Pol, S. Katsanevas, T. A. Filippas, M. Regler, Yu. Sedykh, B. Van Eijk, H. Mueller, J. Dolbeau, P. Folegati, P.S.L. Booth, P. N. Ratoff, J. J. Gómez Cadenas, J. Marco, M. P. Clara, Piotr Zalewski, Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), DELPHI, Heyd, Yvette, Abreu, P., Adam, W., Canale, Vincenzo, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), and Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], 010308 nuclear & particles physics, Electron–positron annihilation, Hadron, Width ratio, 01 natural sciences, 7. Clean energy, Nuclear physics, 0103 physical sciences, Physique des particules élémentaires, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Neutrino, 010306 general physics, Particle Physics - Experiment, Lepton, Boson
Abstract

Measurements are presented of the cross section ratios Rℓ = σℓ(e+e-→ℓ+ℓ -)/σhh(e+e-→hadrons) for ℓ = e, μ and τ using data taken from a scan around the Z0. The results are Re = (5.09±0.32±0.18)%, Rμ = (4.96±0.35±0.17)% and Rτ,=(4.72±0.38± 0.29)% where, for the ratio Re, the t-channel contribution has been subtracted. These results are consistent with the hypothesis of lepton universality and test this hypothesis at the energy scale s ∼ 8300 GeV2. The absolute cross sections σℓ(e+e-→ℓ +ℓ-) have also been measured. From the cross sections the leptonic partial widths Γe = (83.2±3.0±2.4) MeV, (ΓeΓμ) 1/2=(84.6±3.0±2.4) MeV and (ΓeΓτ) 1/2=(82.6±3.3±3.2) MeV have been extracted. Assuming lepton universality the ratio Γℓ/Γh=(4.89±0.20± 0.12) × 10-2 was obtained, together with Γℓ=(83.6±1.8±2.2) MeV. The number of light neutrino species is determined to be Nv=3.12±0.24±0.25. Al the data are consistent with the predictions of the standard model., 0, SCOPUS: ar.j, info:eu-repo/semantics/published

Published
1990
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45. Recent Results From The DELPHI Barrel Ring Imaging Cherenkov Counter

Author

E.G. Anassontzis, P. Ioannou, G. Kalkanis, S. Katsanevas, I. Kontaxis, C. Koukoumelis, S. Nounos, P. Preve, L.K. Resvanis, J.M. Brunet, J. Dolbeau, L. Guglielmi, F. Ledroit, D. Poutot, G. Tristram, P. Baillon, M. Barranco-Luque, M. Davenport, S. Delorme, J. Dixon, M. Dracos, D. Fraissard, J.B. Franco, E. Gaumann, B. Goret, F. Hahn, S. Haider, W. Klempt, B. Koene, G. Lecoeur, G. Mourgue, J. Perez, P. Queru, J. Raynaud, E. Rosso, D. Soria-Buil, D. Treille, A. Tsirou, S. Tzamarias, M. Zanolini, E. Aria, J.D. Berst, D. Bloch, E. Christophel, W. Dulinski, D. Husson, P. Juillot, M. Schaeffer, K. Galuszka, J. Michalowski, M. Stodulski, D. Loukas, G. Theodosiou, B. Dalmagne, F. Fulda-Quenzer, N. Greguric, J.M. Noppe, M. Chevry, J. Kesteman, G. van Apeldoorn, N. Brummer, P. van Dam, A.N. Diddens, G. Evers, J. Homma, F. Hulman, H. Kok, N. de Koning, A. Korporaal, W. Kuilman, D. Langerveld, H. Leenbeek, R. Leguyt, E. Schyns, D.Z. Toet, T. Ypma, M. Dris, T.A. Filippas, E. Fokitis, E. Gazis, E. Katsoufis, S. Maltezos, T. Papadopoulou, T. Ekelof, J. Drees, I. Herbst, G. Lenzen, J. Thadome, and J. Werner

Subjects
Physics, Nuclear and High Energy Physics, Wire chamber, Time projection chamber, Muon, Physics::Instrumentation and Detectors, Particle accelerator, Particle identification, Photon counting, Particle detector, law.invention, Nuclear physics, Nuclear Energy and Engineering, law, High Energy Physics::Experiment, Detectors and Experimental Techniques, Electrical and Electronic Engineering, Cherenkov radiation
Abstract

The DELPHI detector installed in the LEP (Large Electron-Positron Collider) is equipped with RICH (ring imaging Cherenkov) counters. The barrel part incorporates a liquid (C/sub 6/F/sub 14/) and a gaseous (C/sub 5/F/sub 12/) radiator, providing particle identification up to 20 GeV/c. The Cherenkov photons of both radiators are detected by TPC (time projection chamber)-like photon detectors. The drift gas (75% CH/sub 4/+25% C/sub 2/H/sub 6/) is doped with TMAE (tetrakis-dimethylamine-ethylene) by which the ultraviolet Cherenkov photons are converted into single free photoelectrons. These are drifted towards multiwire proportional chambers at the end of the drift tubes, and the space coordinates of the conversion point are determined. One half of the barrel RICH is now equipped with drift tubes and has provided results from the liquid radiator since spring 1990. The gas radiator has been tested with C/sub 2/F/sub 6/ as a preliminary filling since August 1990. The data obtained demonstrate the good particle identification potential. For the liquid radiator, the number of detected photons per ring in hadron jets is N=8, whereas for muon pairs (single tracks) N=10 has been obtained. For the gas radiator, 2.1 photons per track were observed, which demonstrates good functioning of the focussing mirrors. >

Published
2005
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46. Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by Archeops

Author

N. Ponthieu, J. F. Macías-Pérez, M. Tristram, P. Ade, A. Amblard, R. Ansari, J. Aumont, É. Aubourg, A. Benoît, J.-Ph. Bernard, A. Blanchard, J. J. Bock, F. R. Bouchet, A. Bourrachot, P. Camus, J.-F. Cardoso, F. Couchot, P. de Bernardis, J. Delabrouille, F.-X. Désert, M. Douspis, L. Dumoulin, Ph. Filliatre, P. Fosalba, M. Giard, Y. Giraud-Héraud, R. Gispert, J. Grain, L. Guglielmi, J.-Ch. Hamilton, S. Hanany, S. Henrot-Versillé, J. Kaplan, G. Lagache, A. E. Lange, K. Madet, B. Maffei, S. Masi, F. Mayet, F. Nati, G. Patanchon, O. Perdereau, S. Plaszczynski, M. Piat, S. Prunet, J.-L. Puget, C. Renault, C. Rosset, D. Santos, D. Vibert, D. Yvon, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Centre de Recherches sur les Très Basses Températures (CRTBT), Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique de Grenoble (INPG)-Université Joseph Fourier - Grenoble 1 (UJF), Centre d'étude spatiale des rayonnements (CESR), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées (LATT), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), ARCHEOPS, Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Ponthieu, N, Mac??as-P??rez, J, Tristram, M, Ade, P, Amblard, A, Ansari, R, Aumont, J, Aubourg, ?, Beno??t, A, Bernard, J, Blanchard, A, Bock, J, Bouchet, F, Bourrachot, A, Camus, P, Cardoso, J, Couchot, F, de Bernardis, P, Delabrouille, J, D??sert, F, Douspis, M, Dumoulin, L, Filliatre, P, Fosalba, P, Giard, M, Giraud-H??raud, Y, Gispert, R, Grain, J, Guglielmi, L, Hamilton, J, Hanany, S, Henrot-Versill??, S, Kaplan, J, Lagache, G, Lange, A, Madet, K, Maffei, B, Masi, S, Mayet, F, Nati, F, Patanchon, G, Perdereau, O, Plaszczynski, S, Piat, M, Prunet, S, Puget, J, Renault, C, Rosset, C, Santos, D, Vibert, D, Yvon, D, Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), and Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)

Subjects
media_common.quotation_subject, Cosmic microwave background, Extrapolation, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Radiation, 01 natural sciences, Cosmology: observation, Spectral line, Submillimetre, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Polarization, 0103 physical sciences, Cosmic Microwave Background, 010303 astronomy & astrophysics, Observations, Astrophysics::Galaxy Astrophysics, QB, media_common, Physics, Archeops, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, Astrophysics (astro-ph), Spectral density, Astronomy and Astrophysics, Dust, Extinction, Polarization (waves), Cosmology, 13. Climate action, Space and Planetary Science, Sky, Foreground, Cosmology: cosmic microwave background, ISM: dust, extinction
Abstract

We present the first measurement of temperature and polarization angular power spectra of the diffuse emission of Galactic dust at 353 GHz as seen by Archeops on 20% of the sky. The temperature angular power spectrum is compatible with that provided by the extrapolation to 353 GHz of IRAS and DIRBE maps using \cite{fds} model number 8. For Galactic latitudes $|b| \geq 5$ deg we report a 4 sigma detection of large scale ($3\leq \ell \leq 8$) temperature-polarization cross-correlation $(\ell+1)C_\ell^{TE}/2\pi = 76\pm 21 \mu\rm{K_{RJ}}^2$ and set upper limits to the $E$ and $B$ modes at $11 \mu\rm{K_{RJ}}^2$. For Galactic latitudes $|b| \geq 10$ deg, on the same angular scales, we report a 2 sigma detection of temperature-polarization cross-correlation $(\ell+1)C_\ell^{TE}/2\pi = 24\pm 13 \mu\rm{K_{RJ}}^2$. These results are then extrapolated to 100 GHz to estimate the contamination in CMB measurements by polarized diffuse Galactic dust emission. The $TE$ signal is then $1.7\pm0.5$ and $0.5\pm0.3 \mu\rm{K^2_{CMB}}$ for $|b| \geq 5$ and 10 deg. respectively. The upper limit on $E$ and $B$ becomes $0.2 \mu\rm{K^2_{CMB}} (2\sigma)$. If polarized dust emission at higher Galactic latitude cuts is similar to the one we report here, then dust polarized radiation will be a major foreground for determining the polarization power spectra of the CMB at high frequencies above 100 GHz., Comment: 11 pages, 8 figures, submitted to AA

Published
2005
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47. The CMB temperature power spectrum from an improved analysis of the Archeops data

Author

P. Camus, Alain Benoit, James J. Bock, Alain Blanchard, R. Gispert, J.-F. Cardoso, Federico Nati, Ph. Filliatre, J. F. Macías-Pérez, Stéphane Plaszczynski, D. Vibert, Éric Aubourg, L. Dumoulin, Bruno Maffei, Ch. Magneville, François R. Bouchet, F. Mayet, K. Madet, C. Renault, M. Tristram, Marian Douspis, L. Guglielmi, J.-Ch. Hamilton, Shaul Hanany, Y. Giraud-Heraud, Guilaine Lagache, M. Giard, G. Patanchon, O. Perdereau, Peter A. R. Ade, Silvia Masi, Pablo Fosalba, Andrew E. Lange, R. Ansari, C. Rosset, D. Yvon, Jean Kaplan, A. Bourrachot, J.-M. Lamarre, P. de Bernardis, Francois-Xavier Désert, M. Piat, Nicolas Ponthieu, F. Couchot, Simon Prunet, D. Santos, Alexandre Amblard, J. Delabrouille, Sophie Henrot-Versille, J.-Ph. Bernard, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Centre de Recherches sur les Très Basses Températures (CRTBT), Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique de Grenoble (INPG)-Université Joseph Fourier - Grenoble 1 (UJF), Centre d'étude spatiale des rayonnements (CESR), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées (LATT), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), ARCHEOPS, Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS-PSL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), Tristram, M, Patanchon, G, Macias-Perez, J, Ade, P, Amblard, A, Ansari, R, Aubourg, E, Benoit, A, Ph Bernard, J, Blanchard, A, Bock, J, Bouchet, F, Bourrachot, A, Camus, P, Cardoso, J, Couchot, F, De Bernardis, P, Delabrouille, J, Desert, F, Douspis, M, Dumoulin, L, Filliatre, P, Fosalba, P, Giard, M, Giraud-Heraud, Y, Gispert, R, Guglielmi, L, Ch Hamilton, J, Hanany, S, Henrot-Versille, S, Kaplan, J, Lagache, G, Lamarre, J, Lange, A, Madet, K, Maffei, B, Magneville, C, Masi, S, Mayet, F, Nati, F, Perdereau, O, Plaszczynski, S, Piat, M, Ponthieu, N, Prunet, S, Renault, C, Rosset, C, Santos, D, Vibert, D, and Yvon, D

Subjects
[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], media_common.quotation_subject, Cosmic microwave background, Data analysis, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Cosmology: observation, 01 natural sciences, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], cosmology : cosmic microwave background, cosmology : observations, cosmology: cosmic microwave background, cosmology: observations, data analysis, methodes, methodes : data analysis, Consistency (statistics), 0103 physical sciences, Cosmic Microwave Background, Range (statistics), 010303 astronomy & astrophysics, Observations, media_common, QB, Physics, Archeops, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, Methode, Astrophysics (astro-ph), Astrophysics::Instrumentation and Methods for Astrophysics, Spectral density, Astronomy and Astrophysics, CMB cold spot, Cosmology, Space and Planetary Science, Sky, Cosmology: cosmic microwave background, Multipole expansion, data analysi
Abstract

We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops flight. This refined analysis is obtained by using the 6 most sensitive photometric pixels in the CMB bands centered at 143 and 217 GHz and 20% of the sky, mostly clear of foregrounds. Using two different cross-correlation methods, we obtain very similar results for the angular power spectrum. Consistency checks are performed to test the robustness of these results paying particular attention to the foreground contamination level which remains well below the statistical uncertainties. The multipole range from l=10 to l=700 is covered with 25 bins, confirming strong evidence for a plateau at large angular scales (the Sachs-Wolfe plateau) followed by two acoustic peaks centered around l=220 and l=550 respectively. These data provide an independent confirmation, obtained at different frequencies, of the WMAP first year results., 14 pages, 16 figures, A&A

Published
2005
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48. Expression of the MN1-TEL fusion protein in the human UCSD/AML1 leukemic cell line

Author

L Guglielmi, Maryvonne Busson, Roland Berger, Olivier Bernard, E C Zwarthoff, and V Della Valle

Subjects
Cancer Research, Oncogene Proteins, Fusion, business.industry, MN1/TEL Fusion Protein, Hematology, Biology, Leukemia, Myelomonocytic, Acute, Cell biology, Gene Expression Regulation, Neoplastic, Text mining, Oncology, Cell culture, Tumor Cells, Cultured, Chromosomes, Human, Humans, business, In Situ Hybridization, Fluorescence, Transcription Factors
Published
2004

49. Mouse embryonic stem cell sorting for the generation of transgenic mice by sedimentation field-flow fractionation

Author

M. Le Bert, Yves Denizot, Philippe J.P. Cardot, Serge Battu, J. L. Faucher, L. Guglielmi, Physiologie Moléculaire de la Réponse Immune et des Lymphoproliférations (PMRIL), and Université de Limoges (UNILIM)-Génomique, Environnement, Immunité, Santé, Thérapeutique (GEIST FR CNRS 3503)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Genetically modified mouse, NLM, Ratón, MESH: Mice, Transgenic, Mice, Transgenic, MESH: Stem Cells, Cell Separation, 01 natural sciences, MESH: Cell Separation, Analytical Chemistry, 03 medical and health sciences, Chimera (genetics), Mice, In vivo, Animals, MESH: Animals, MESH: Mice, MESH: Chimera, 030304 developmental biology, 0303 health sciences, Chemistry, Chimera, Stem Cells, 010401 analytical chemistry, MESH: DNA, MESH: Embryo, Mammalian, MESH: Embryo Transfer, DNA, Cell Fraction, MESH: Fractionation, Field Flow, Embryo Transfer, Embryo, Mammalian, Molecular biology, Embryonic stem cell, Fractionation, Field Flow, 0104 chemical sciences, Genetically modified organism, [SDV.IMM]Life Sciences [q-bio]/Immunology, Stem cell
Abstract

Mouse embryonic stem (ES) cells are an important tool for generation of transgenic mice and genetically modified mice. A rapid and efficient separation of ES cells that respects cell integrity, viability, and their developmental potential while also allowing purified ES fraction collection under sterile conditions might be of great interest to facilitate the generation of chimeric animals. In this study, we demonstrated for the first time the effectiveness of a sedimentation field-flow fractionation (SdFFF) cell sorter to provide, with a characteristic DNA content, a purified ES cell fraction and with a high in vivo developmental potential to prepare transgenic mice by generation of chimeras having a high percentage of chimerism.

Published
2004
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50. First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops

Author

Anthony Murphy, R. Ansari, Pablo Fosalba, Guy Perrin, Simon Prunet, F. Mayet, Shaul Hanany, Y. Giraud-Héraud, D. Vibert, X. Dupac, M. Piat, Alain Blanchard, A. Bourrachot, Romain Teyssier, Daniel P. Marrone, R. S. Bhatia, Jacques Delabrouille, Alexei A. Starobinsky, F. Naraghi, D. Yvon, Alexandre Amblard, James G. Bartlett, G. Patanchon, F. Couchot, A. Boscaleri, Rashmikant V. Sudiwala, S. Bargot, Peter A. R. Ade, M. Giard, L. Dumoulin, R. Gispert, Ken Ganga, Bruno Maffei, Fred Gannaway, Sophie Henrot-Versille, C. Rosset, Jean Kaplan, Olivier Doré, J.-Ch. Hamilton, Alain Benoit, J.-Ph. Bernard, Carole Tucker, Éric Aubourg, K. Madet, James J. Bock, Jean-Loup Puget, Nicolas Ponthieu, Ch. Magneville, M. Tristram, Francois-Xavier Désert, François R. Bouchet, P. Filliatre, Guilaine Lagache, Philippe Camus, J.-M. Lamarre, B. Gautier, I. Strukov, Andrew E. Lange, J. F. Macías-Pérez, Marian Douspis, L. Guglielmi, Silvia Masi, Jean-Charles Vanel, P. de Bernardis, Federico Nati, Daniel Santos, E. Wakui, C. Renault, Centre de Recherches sur les Très Basses Températures (CRTBT), Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique de Grenoble (INPG)-Université Joseph Fourier - Grenoble 1 (UJF), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'étude spatiale des rayonnements (CESR), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Services communs OMP (UMS 831), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), ARCHEOPS, Université Joseph Fourier - Grenoble 1 (UJF)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS-PSL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Benoit, A, Ade, P, Amblard, A, Ansari, R, Aubourg, E, Bargot, S, Bartlett, J, Ph Bernard, J, Bhatia, R, Blanchard, A, Bock, J, Boscaleri, A, Bouchet, F, Bourrachot, A, Camus, P, Couchot, F, De Bernardis, P, Delabrouille, J, Desert, F, Dore, O, Douspis, M, Dumoulin, L, Dupac, X, Filliatre, P, Fosalba, P, Ganga, K, Gannaway, F, Gautier, B, Giard, M, Giraud-Heraud, Y, Gispert, R, Guglielmi, L, Ch Hamilton, J, Hanany, S, Henrot-Versille, S, Kaplan, J, Lagache, G, Lamarre, J, Lange, A, Macias-Perez, J, Madet, K, Maffei, B, Magneville, C, Marrone, D, Masi, S, Mayet, F, Murphy, A, Naraghi, F, Nati, F, Patanchon, G, Perrin, G, Piat, M, Ponthieu, N, Prunet, S, Puget, J, Renault, C, Rosset, C, Santos, D, Starobinsky, A, Strukov, I, Sudiwala, R, Teyssier, R, Tristram, M, Tucker, C, Vanel, J, Vibert, D, Wakui, E, and Yvon, D

Subjects
[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::High Energy Astrophysical Phenomena, Cosmic microwave background, FOS: Physical sciences, cosmology: cosmic microwave background, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, cosmology : cosmic microwave background, 01 natural sciences, Cosmology: observation, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, 0103 physical sciences, Stokes parameters, submillimeter, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Cosmic dust, QB, Physics, polarization, Archeops, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, extinction, Astrophysics (astro-ph), Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Galactic plane, Polarization (waves), ism: dust, cosmology : observations, cosmology: observations, ism : dust, Interstellar medium, Space and Planetary Science, symbols, Degree of polarization, ISM: dust, extinction
Abstract

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was launched by CNES from the Swedish Esrange base near Kiruna. In addition to the 143 GHz and 217 GHz frequency bands dedicated to CMB studies, Archeops had one 545 GHz and six 353 GHz bolometers mounted in three polarization sensitive pairs that were used for Galactic foreground studies. We present maps of the I, Q, U Stokes parameters over 17% of the sky and with a 13 arcmin resolution at 353 GHz (850 microns). They show a significant Galactic large scale polarized emission coherent on the longitude ranges [100, 120] and [180, 200] deg. with a degree of polarization at the level of 4-5%, in agreement with expectations from starlight polarization measurements. Some regions in the Galactic plane (Gem OB1, Cassiopeia) show an even stronger degree of polarization in the range 10-20%. Those findings provide strong evidence for a powerful grain alignment mechanism throughout the interstellar medium and a coherent magnetic field coplanar to the Galactic plane. This magnetic field pervades even some dense clouds. Extrapolated to high Galactic latitude, these results indicate that interstellar dust polarized emission is the major foreground for PLANCK-HFI CMB polarization measurement., Comment: Submitted to Astron. & Astrophys., 14 pages, 12 Fig., 2 Tables

Published
2004
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